2007 Ocean Optics Catalog
Ocean Optics
bringing answers to light
07
catalog
Milestone Mania
Contact Information
Worldwide Headquarters
On April 9, 2007, we’ll mark the 15th anniversary of our first miniature
spectrometer sale – quite an accomplishment for a bunch of dreamers who
originally worked out of a shed (we couldn’t even afford a garage!). To
frame that accomplishment, consider this: sometime this year we’ll sell our
100,000th spectrometer. Here are some milestones from along the way:
1989
Ocean Optics is incorporated in Dunedin, Florida, a
lovely town on the Gulf of Mexico, thus beginning a
long history of people asking us why we named a
spectrometer company “Ocean” Optics.
1992
The “World’s First Miniature Spectrometer” is sold to
Los Alamos National Laboratories. The guy who sells
the system also builds it, packs it, and drops it off at
UPS. Fortunately, it’s not his turn to take out the trash
that day.
1993
The S1000 Spectrometer earns the company’s first
Photonics Circle of Excellence Award.
1995
Our booth space at the PITTCON show exceeds our
headquarters office space (750 square feet). Four
employees ask to move their desks to the booth.
1999
We establish a Thin Films Division, securing a supply
of optical components and expanding into new
markets with a patented technology for patterned
thin film filters.
2000
First overseas office, in Europe, is founded. In the
States, everyone immediately asks to have off the
month of August. (Just kidding!)
2001
Founder Mike Morris turns 50 during PITTCON. We
celebrate by building a pirate ship (really) for our
booth, donning foppish pirate shirts, and throwing a
parade in the streets of New Orleans complete with
motorcycle escort, jazz band and (of course) beads.
2003
Our Laser-induced Breakdown Spectrometer wins our
third Photonics Circle of Excellence Award.
2005
SeaChanger, a color-changer technology from our
Thin Films Division, is awarded the Entertainment
Services & Technology Association’s Dealers’ Choice
Product Award for Equipment. Six months later,
SeaChanger makes its Broadway debut in TARZAN®.
2006
Our company establishes its first Asia-based Sales,
Service & Support Office in China.
2007
The Jaz family of flexible sensing modules – a new
concept in optical sensing – has a dazzling debut at
Photonics West. The show is the most successful in
company history.
830 Douglas Avenue
Dunedin, FL 34698
USA
Expanded
Service Hours
8 a.m to 8 p.m. (EST)
Mondays - Thursdays
Tel 727.733.2447
Fax 727.733.3962
[email protected]
[email protected]
Worldwide Sales, Service
& Support Locations
See page 5 for contact
information for all of our Sales,
Service & Support locations
including Europe and Asia.
8 a.m. to 6 p.m. (EST)
Fridays
Real People,
Real Answers
Call Ocean Optics and
discuss your optical sensing
needs with one of our
knowledgeable
Applications Scientists.
727.733.2447
Ordering Information
Terms:
Net 30 days with credit approval. Contact us for further
information. All shipments are delivered EXWORKS, Dunedin,
Florida, USA. For all shipments into Florida, we are required to
charge sales tax unless a valid resale certificate is received prior to
shipment. Fax resale certificates to our Accounting Department at
727.734.0957. Specifications, descriptions, ordering information
and item codes described herein are subject to change without
notice. These commodities, technology or software are to be
exported from the United States in accordance with the Export
Administration Regulations. Diversion contrary to U.S. law prohibited.
Pricing:
Our Worldwide Pricing Policy ensures that a single, universal price
applies to every Ocean Optics product, regardless of where it’s
sold. While extra costs due to currency exchange, and customs,
shipping and other costs are borne by the customer, they should not
be confused with a product’s selling price. We adopted this policy
to provide clients with relief from excessive add-on costs that others
pass on to overseas customers. Here’s some additional tips about
pricing:
All prices are subject to change without notice.
For the most up-to-date pricing, contact us at 727.733.2447
or visit our website at OceanOptics.com.
We honor the pricing cited in a quotation for 30 days.
You can purchase Ocean Optics products from any of our
four locations around the world (for contact information, see
page 5), from an Ocean Optics distributor (visit
www.oceanoptics.com/corporate/distributors.asp for a
complete contact list) and from VWR (visit www.vwr.com).
Pricing for some light sources and accessories manufactured
in Europe are subject to exchange rates, and vary frequently.
Credit Cards:
Ocean Optics accepts American Express, MasterCard and VISA
credit cards.
Shipping:
Shipping charges are the responsibility of the customer. Orders are
shipped UPS Ground, unless otherwise requested. Customers may
reverse shipping charges to use the carrier of their choice.
What’s Inside
3 Our Value Proposition
4
5
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7
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9
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15 Years of Bringing Answers to Light
Worldwide Sales, Service & Support Locations
Worldwide Distribution
OEMs & Application Developers
Educational Spectroscopy Grants
Education Division
Customer Service
USB4000-series
Spectrometers
p. 14
11 Spectrometers
14
15
20
21
22
26
27
30
32
USB4000 Plug-and-Play Spectrometer
“USB”-series Optical Bench Options
HR2000+ High-speed, High-res Spectrometer
HR4000 High-resolution Spectrometer
“HR”-series Optical Bench Options
QE65000 Scientific-grade Spectrometer
“QE”-series Optical Bench Options
NIR-series Near-infrared Spectrometers
“NIR”-series Optical Bench Options
Red Tide USB-650
Spectrometer
p. 38
33 Spectrometer Systems & Setups
34
42
44
48
51
56
57
General-purpose Spectrometers
Liquid Absorbance Systems
Fluorescence Measurement Tools
Laser-induced Breakdown Spectroscopy
Raman Spectrometers
Spectroradiometric Systems
Metrology Systems
63 Optical Sensors
65
66
68
69
70
72
74
75
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Oxygen Sensor Operation
Oxygen Sensor Spectrometers
Oxygen Sensor Formulations
Oxygen Sensor Care & Compatibility
Oxygen Sensor Probes
Oxygen Sensor Accessories
Oxygen Sensor Temperature Compensation
Sensor Software
Pocket Carbon Monoxide Meter
Fiber Optic pH Sensors & Test Kit
LIBS2500 Laser-induced
Breakdown Spectrometer Systems
p. 48
Fiber Optic Chemical
Sensors
p. 67
What’s Inside
77 Software & Data Acquisition
80
82
83
84
SpectraSuite Spectroscopy Operating Software
OmniDriver Spectroscopy Developer Platform
SpecLine Software for Compound ID
Analog-to-Digital Converters
85 Sampling Accessories
SpectraSuite Spectroscopy
Operating Software &
OmniDriver Developer Platform
p. 80-82
FluoroVette
Micro-volume Cells
p. 103
88
90
94
100
104
105
109
113
118
Collimating Lenses & Accessories
Cuvette Holders & Accessories
Sampling Systems for Fluid Analysis
Fluorescence Sampling Tools
Light Collection Tools
Reflection Measurement Tools
Tools for Metrology
Filtering Light & Light Control Tools
Mapping Tables & Positioners
119 Light Sources
122
126
127
128
130
132
134
Deuterium Tungsten Halogen Sources
Deuterium Light Sources
Xenon Sources
Tungsten Halogen Light Sources
LED Sources
Radiometric Calibration Standards
Wavelength Calibration Standards
137 Fibers & Probes
Flow Cells for Flow
Injection Analysis
p. 94
139
142
143
144
146
147
153
154
Custom Fiber & Probe Assemblies
Premium-grade Assemblies
Unjacketed Bulk Optical Fiber
Laboratory-grade Assemblies
Xtreme Solarization-resistant Assemblies
Fiber Optic Probes
Vacuum Feedthroughs
Optical Fiber Kits
159 Thin Films & Optics
Premium-grade Xtreme
Solarization-resistant
Assemblies
p. 146
161
162
163
164
Thin Films & Optics Capabilities
Thin Films & Optics Applications
Metrology Tools
Absorbing Glass Filters
165 Resources
167
178
183
Sample Setups
Spectral Identity
Indices
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Our Value Proposition
15 Years of Bringing Answers
to Light
5
Worldwide Sales, Service & Support
6
Worldwide Distribution
7
OEMs & Application Developers
8
Educational Spectroscopy Grants
9
Education Division
10
Customer Service
Our Value Proposition
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15 Years of Bringing Answers to Light
What Really Matters
We value the opportunities to learn and to grow -- and to
expand the frontiers of optical sensing -- that come from
partnership. Recognizing and seizing these opportunities is
what Ocean Optics is all about -- and is reflected in an open,
collaborative approach that appeals to everyone from the
innovators and early adopters to the skeptics and the
traditionalists.
Ocean Optics in 2007: 100,000 Spectrometers!
Our Value Proposition
Founded in 1989, Ocean Optics manufactures miniature fiber
optic spectrometers and accessories, optical sensors, optical
fibers, and thin films and optics. Our palm-sized fiber optic
spectrometer -- “the world’s first miniature fiber optic
spectrometer” -- has spawned dozens of imitators and enabled
thousands of optical-sensing applications across a variety of
industries and disciplines. We’ve never been much for selfcongratulation, but Ocean Optics will mark two major
milestones in 2007: the 15th anniversary of our first sale, and
the 100,000th spectrometer sold since 1992. So we’ve paused
to reflect:
We started in 1989, when our founding fathers, a group
of university researchers, developed a fiber optic pH
sensor to study the role of the oceans in global warming.
Later, a Small Business Innovation Research grant from
the U.S. Department of Energy led to the development of
the world’s first miniature fiber optic spectrometer.
Our first commercial sale was in April 1992, to a
researcher at Los Alamos National Laboratories named
Ed Kaukell. Ed purchased an S1000 Spectrometer, which
he used in an application involving plutonium. Years
later we tracked down that first spectrometer -- no, it’s
not radioactive -- and now display it at company
headquarters.
In 1993, our S1000 Miniature Fiber Optic Spectrometer
earned the Photonics Circle of Excellence Award, which
recognizes innovation in photonics. We also won the
award in 2000 and 2003.
Our original miniature fiber optic spectrometer, the
S1000, retailed for $1,800 and required an additional
$500 A/D Converter. Its modern equivalent, the
USB4000 Spectrometer, retails for just $2,200 and
includes an onboard A/D Converter.
At the end of 1992, we had about 20 items in our
product line. Today, we offer nearly 1,200 spectrometers
and accessories.
NanoDrop Technologies purchased our 50,000th
spectrometer, a milestone we celebrated in January
2005. NanoDrop, a Delaware-based supplier of
UV-VIS spectrophotometers for extremely smallvolume sampling, is a prototypical Ocean Optics
customer: a small team of researchers with an
NanoDrop Technologies founder and engineering director, Charles Robertson,
celebrates our 50,000th spectrometer sold in 2005.
interesting application, the passion and know-how to
make it happen, and an appreciation for the advantages
of size, cost and flexibility that our spectrometers
provide.
If you took all 100,000 spectrometers and laid them
end-to-end, the line would stretch for nearly eight miles.
The optical benches of the 100,000 spectrometers
project spectra across approximately 200 million
detector pixels.
From its humble beginnings as a garage-shop operation with
just a handful of products, Ocean Optics has grown to two
manufacturing facilities and four Sales, Service & Support
locations worldwide selling nearly 1,200 unique products. Our
spectrometers have been used in thousands of applications,
from the volcanologist who duct-taped the spectrometer to a
bicycle helmet as he ventured inside an active site to monitor
sulphur dioxide, to the NASA researcher who strapped the
spectrometer to a reentry rocket to measure its exhaust plume.
Thanks to the thousands of Ocean Optics customers who have
helped us achieve such milestones!
Ocean Optics Vision Statement
To expand the frontiers of
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optical sensing and make it
the foundation on which innovative,
life-changing ideas are built.
For all your sensing needs, visit OceanOptics.com
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Worldwide Sales, Service & Support
From our humble beginning as a garage-shop operation with a handful of
dreamers and too many bills, we’ve grown to six sales and manufacturing
facilities worldwide supported by over 200 employees. Recent
developments include the expansion of our customer service and technical
support departments at headquarters and the addition of full-service sales
and support offices in Europe and Asia.
Worldwide Headquarters: Dunedin, Florida, USA
Worldwide headquarters in Dunedin, Florida (at right), are home to our
Sales & Marketing, Customer Service, Technical Support, Engineering and
R&D, and Accounting and Human Resources Departments. Our three-story,
27,000-square-foot facility on the Gulf of Mexico is a 35-minute drive west
of Tampa and is conveniently located near major airports.
Address:
830 Douglas Ave., Dunedin, FL 34698 USA
This 27,000-square-foot facility has been company headquarters
since 1998.
Telephone: 727.733.2447
Fax:
727.733.3962
Email:
[email protected] (general sales inquiries)
Hours:
8 a.m. to 8 p.m. EST Monday-Thursday
8 a.m. to 6 p.m. EST Friday
Ocean Optics is excited to announce that it has established a full-time
presence in Asia. Ocean Optics Asia opened its Sales, Service & Support
office in Shanghai, China to support rapidly growing markets in Asia. This
new office provides sales consultations and technical support; training
services; and enhanced support for OEM, distributor, academic and
research lab customers.
Address:
666 Gubei Rd, Kirin Tower, Suite 601B, Changning District,
Shanghai 200051, People’s Republic of China
Telephone: +86 21-6295-6600
Fax:
+86 21-6295-6708
Email:
[email protected]
Hours:
9 a.m. to 6 p.m. CST Monday-Friday
Sun Ling, Ph.D., Director of Asia Operations for Ocean Optics, and
her new staff of application scientists operate in the Changning
District in Shanghai.
European Operations: 7-Year Anniversary for OOBV
Established in 2000, Ocean Optics B.V. is a full-service subsidiary of
Ocean Optics dedicated to serving customers and prospects in Europe, the
Middle East and Africa. The office is located in Duiven, The Netherlands,
just outside of Arnhem. Ocean Optics B.V. provides sales and application
assistance and technical support for the entire line of Ocean Optics
products.
Address:
Geograaf 24, 6921 EW Duiven, The Netherlands
Telephone: +31 (0) 26 319 0500
Fax:
+31 (0) 26 319 0505
Email:
[email protected]
Hours:
8:30 a.m. to 5 p.m. CET Monday-Friday
European Operations: Old Friend Now a Part of the Family
In 2006, Mikropack GmbH, an innovative developer and manufacturer of
light sources, photonics accessories and metrology systems, became part
of the Ocean Optics family. Mikropack adds depth and experience to our
presence in Europe by providing support for our spectrometers and
accessories in Germany, Switzerland and Austria, and continues to sell and
support its thin film and plasma-emission metrology systems.
Address:
Maybachstrasse 11, D-73760 Ostfildern, Germany
Telephone: +49 (0) 711 34 16 96-0
Fax:
+49 (0) 711 34 16 96-85
Email:
[email protected]
Hours:
8 a.m. to 5 p.m. CET Monday-Friday
Tel: 727.733.2447 • Email: [email protected]
Our Value Proposition
Asian Operations: New Office Opens in China
Kees van de Steeg, Managing Director of Ocean Optics B.V., has
nearly 30 years of experience in the optoelectronics industry.
Co-presidents of
Mikropack, Gerald
Nitsch and Dieter
Steck, accept a BadenWuerttemberg award
for enterprise
companies. For over a
decade, Mikropack and
Ocean Optics have
collaborated successfully on engineering
and sales projects.
Now Mikropack is
Ocean Optics.
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Worldwide Distribution Network
Trusted Experience Around the World
We have an extensive network of domestic and international
distributors who provide comprehensive pre- and post-sales
service for our line of optical-sensing products. Our distributors
offer considerably more than simple order-taking: they provide
a local source for applications expertise and sales consultation,
as well as hands-on demonstrations of our spectrometers and
accessories. Many of them are former customers who liked our
products so well they jumped at the opportunity to join our sales
network. For an up-to-date list of Ocean Optics distributors,
click on the “Worldwide Distribution” link at OceanOptics.com.
Our Value Proposition
Ocean Optics Distributors & Worldwide Pricing
Our distributors abide by our “Worldwide Pricing” policy, which
ensures that a single, universal price applies to every Ocean
Optics product. Extra costs due to currency exchange, customs
duties and shipping charges should not be confused with a
product’s selling price. We originated this policy to provide
clients with relief from excessive add-on costs that other
manufacturers and distributors pass on to overseas customers.
Worldwide pricing is prominently displayed on our website and
in our print catalog. We adhere to fair business practices and
employ these principles in the Ocean Optics worldwide
distributors agreement.
Join Our Distributor Team
Our distributors come from a variety of backgrounds,
experiences and cultures, yet they all have one thing in
common: a passion for using Ocean Optics technologies to
help their customers solve an array of optical-sensing
applications challenges. We’re always looking for skilled and
enthusiastic people to help us sell the most innovative line of
photonics products in the market. If you are interested in
becoming part of our worldwide distributor network, contact us
at [email protected] -- we’d love to discuss
opportunities. If you qualify as a distributor, here are some of
the benefits you’ll enjoy:
Discounted Pricing
Qualifying distributors reap the benefits of discounted pricing on
spectrometers and accessories. Discount rates -- based on gross
margin of the product -- depend on sales volume, which is
reviewed annually and adjusted to reward top performers. Also,
top-tier distributors can take advantage of prospect-generation
and marketing support to promote Ocean Optics products.
OEM Client Development
Our spectrometers are used in thousands of OEM devices in
various industries worldwide. We offer special pricing for
distributors who prospect and manage OEM clients within their
territories. Under this unique margin-sharing program, OEM
client development offers a premium profit advantage for both
Ocean Optics and the distributor.
Technical Training
Because selling Ocean Optics products requires skilled
applications engineers who perform a significant consultative
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Distributors from around the globe met in Singapore for training in November
2006. Such events are scheduled throughout the year.
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role, we provide distributors with regular technical training. Nick
Sebastian, Worldwide Distributor Manager, and Gary Manche,
Training Manager, are available to provide provide sales and
technical support for new programs and products.
Sales & Marketing Support
Ocean Optics makes available to distributors various
promotional items, and encourages distributor participation at
major tradeshows. For top-tier distributors we offer cooperative
marketing support, in the form of expertise, cost-sharing and
other collaborative efforts on tradeshows and other promotional
items. Top-tier distributor support also includes sales prospect
lead-sharing and market-coordination programs designed for
greater territorial coverage and customer support.
Lead Sharing
Ocean Optics marketing efforts
generate thousands of prospects.
Top-tier distributors qualify for
lead sharing, an exchange of
leads between Ocean Optics and
the distributor. Lead sharing
ensures that our overseas
prospects receive rapid response
to their sales and technical needs.
Contact Information
Nick Sebastian, Worldwide
Distributor Manager.
To find a distributor, visit
www.oceanoptics.com/corporate/distributors.asp. For
information on distributing our products, contact Nick Sebastian
at [email protected]
For all your sensing needs, visit OceanOptics.com
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OEMs & Application Developers
Build your Success Using Ocean Optics Products!
Do you have a great idea for a commercial product that uses
optics? Maybe you’ve developed a new analytical technique,
or perhaps your company is already a world leader in
spectroscopy-based instrumentation. Whether you’re
developing a groundbreaking new analytical technique or
designing the next-generation system for a demanding and
sophisticated market, Ocean Optics has the skills, service,
and knowledge to help you succeed. We can we enable your
success with our innovative Original Equipment
Manufacturer (OEM) Partner Program. It is designed to guide
you through product development and launch by giving you
the two things you need most during this crucial period:
1) discounted pricing; and 2) customized advice on how to
get the most out of your Ocean Optics equipment.
Full-service Support
discounts for those with larger needs. With added volume comes
added benefits:
• Volume pricing to ensure you can provide the best value to
your customers -- with discounts of up to 50%!
• Flex-Order -- Our flexible product delivery program that
allows you to adjust delivery times and forecasts easily
• Quarterly Account Status meetings to ensure we continue to
meet your needs
• A subscription to Ocean Insider -- our OEM Newsletter that
keeps you informed on new products and services.
Our Value Proposition
As a member of the OEM Partner Program, you get free
consulting services from applications specialists with the
knowledge and connections to assist you from the beginning of
your product development cycle through launch and ramp-up.
The result is a high-performance, low-cost product designed for
manufacturability and quality field performance. In addition,
OEMs have at their disposal an array of a la carte R&D services,
from optical design and software engineering to prototype
development and testing and validation. In addition, members
receive these added-value benefits:
• Discounts without minimum orders or commitments
• Free access to all user interface and driver software
programs (a $1000+ value)
• Order status notification and expedited order fulfillment
• Development assistance from the technical experts
• Access to software development consultants with Ocean
Optics experience
• OEM Interface Guide, wiring diagrams, register maps and
spectrometer pin-out information
• Co-marketing opportunities through our website, tradeshows
and our distribution network
NanoDrop Technologies, an Ocean Optics
OEM, manufactures and sells unique
instruments that provide 1 µl photometric
analytical capability for labs throughout the
world. The company's patented retention system uses inherent surface
tension and fiber optic technology for highly accurate quantitation of nucleic
acids, proteins, and a wide variety of other chromophores and fluorophores,
without the need for cuvettes or capillaries. This novel technology is an
essential component in today's research environment as investigators
continue to perform molecular analysis on ever-smaller amounts of material.
For more on NanoDrop, visit www.nanodrop.com or call 302-479-7707.
Contact Information
Modular Components
Ocean Optics offers a comprehensive tool kit of optical
components and accessories that can be combined to serve
markets in medical diagnostics, analytical chemistry,
semiconductor process monitoring, and even intensity
measurements. By mixing and matching optical bench
components such as gratings and
slits, one optical bench alone can
be configured more than 500
different ways!
Discounts & Savings
Our goal is to make you
successful; we want our OEMs to
grow. The annual OEM
Developer’s Program membership
starts at $999 -- a great value
even for a small OEM. We also
have outstanding volume
Tel: 727.733.2447 • Email: [email protected]
For more information on OEM opportunities, call us at
727.733.2447 and ask for our OEM Sales Manager, or email us
at [email protected]
Number of Units
per Year
Discount
USB4000-UV-VIS
with OEM Discount*
1
Gross Margin
$2,649
5
10%
$2,384 per unit
10
15%
$2,251 per unit
20
20%
$2,119 per unit
35
25%
$1,986 per unit
50
30%
$1,854 per unit
75
35%
$1,721 per unit
100
40%
$1,589 per unit
150
45%
$1,456 per unit
200
50%
$1,324 per unit
250
53%
$1,245 per unit
500
55%
$1,192 per unit
* OEM Discount Price does not include the OEM Developer’s fee of $999 in
the first year and the $599 renewal fee each year thereafter.
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Educational Spectroscopy Grants
$1,500,000
Worth of Grant Winners
Our Value Proposition
Since 1999, we have awarded over $1.5 million
to learning institutions for funding spectroscopic
applications such as:
Analysis of surface water samples
Identification of organic dyes in textiles
Chlorophyll absorbance and its relationship to
photosynthesis
High school-level introduction to principles of
nanotechnology
Visible tissue reflectance as a diagnostic tool in
studies of the use of laser therapy for
dermatological lesions
Raman spectroscopy to analyze atmospheric
pollutants
Luminescence of mineral crystals to determine
the histories of components in sedimentary
rocks
Metabolic rate, oxygen tension and
hemoglobin concentration in fish
Detection and identification of atomic emission
lines from gas discharge tubes
Measurement of ionization constants in acids
and pH dyes
Study of seaweed photosynthesis and animal
respiration in aquatic chambers and under
various water velocities
Determination of DNA concentration using
absorbance spectroscopy
Fluorescence measurements of luminescent
semiconductor-nanocrystal quantum dots
Analysis of stellar and planetary absorption
spectra
Identification of organic dyes in Peruvian textiles
for archaeological and ethnographic origin
Measuring photosynthetic radiation through
leaf reflectance
Theoretical functioning and the effects of
different variables on the ability of glow
discharge plasmas to destroy pollutants
Color perception of bees
High temporal resolution measurements of
volcanic degassing
NIR analysis of the nutritional content of
(yikes!) feces of various grazing animals
Innovations in Educational Spectroscopy Grant Program
Today's students are the most tech-savvy generation in history. Tap their
enthusiasm by bringing the power of optical sensing to the modern teaching
lab. The Innovations in Educational Spectroscopy Grant Program provides
cost-sharing resources to educators and researchers to promote the use of
fiber optic spectroscopy in curricula and research. This is a great option for
educators on a limited budget, or for those outfitting an entire lab.
Cost Sharing on Proposals for Extramural Funding
We provide cost-sharing support for proposals to federal, state or private
institutions for the express purpose of purchasing our products to be used in
science or engineering teaching. Cost sharing varies according to the
product. There is no limit to the total cost-sharing amount.
Cost Sharing for Ocean Optics Equipment Used in Curricula
We provide cost sharing for purchasing products used to develop new
science and engineering curricula. Cost sharing varies according to the
product. Funding may come from any source, including an organization's
internal funds; however, awards are based on the strength of the applicant's
technical proposal and the novelty of the proposed curricula. The developed
materials must be made available for publication at OceanOptics.com, so
that other educators may have access to the information.
Trade-in Savings
Our trade-in programs provide discounts for all educational institutions on
the purchase of CHEM4-series Spectrophotometers for the purpose of
setting up a lab. Institutions qualify for discounts on our CHEM4-series
Spectrophotometers, provided the institution trades in an old spectrometer,
regardless of its condition.
Eligibility
Cost sharing is available to any qualified non-profit learning institution. For
more information, or to request an application:
Visit us online at OceanOptics.com/Corporate/Grantprogram.asp.
Call an Applications Scientist at 727.733.2447.
Email us at [email protected]
For details on the Grant Program outside of the U.S., contact your
regional Ocean Optics Sales, Service & Support office.
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For all your sensing needs, visit OceanOptics.com
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Education Division
Preparing Students for a Future in Science
The Spec20 -- for decades that workhorse spectrometer so
ubiquitous to university labs around the world -- is yesterday’s
technology. At least, that’s what you told us way back in 1995,
when we launched the first of our PC-based, full-spectrum
spectrometers for teaching labs. Today, we’ve built a full line of
education-friendly spectrometers, accessories and instructional
resources that take students and teachers beyond the limits of
old-fashioned technology and into the possibilities of the future.
Tools for the Modern Teaching Lab
Hardware is just part of the equation. Our SpectraSuite
Operating Software is a powerful yet student-friendly tool that
operates in Macintosh, Linux and Windows. Our educational
system hardware is also compatible with the software of our
educational vendor partners, including PASCO Scientific, Vernier
Software & Technology, and MeasureNet Technology, Inc.
You may have seen our new
promotions featuring “Dr. Q”
Monde Qhobosheane, who
received his Ph.D. from the
University of Florida and taught
chemistry at St. Petersburg
College before coming to Ocean
Optics to lead our Educational
Division. Email Dr. Q at
[email protected]
Curricula and Other Resources
When you invest in Ocean Optics for your teaching lab or
educational application, you’re tapping into the collective power
of 85,000+ spectrometers’ worth of applications know-how.
What’s more, we’ve begun to capture that knowledge in a
variety of easily accessible media:
Database of curricula from our Educational Spectroscopy
Grant Program awardees
The Basics of Spectroscopy Measurements video on
CD-ROM. See page 36 for more on the EDU-SPEC-CD.
An 84-page handbook, Introduction to Spectroscopy in the
Teaching Lab Using Ocean Optics Spectrometers, with
sample lab exercises, available in print or on CD (page 36).
”Spectroscopy 101” Educator Training
Our educator seminar is designed for teachers and department
heads interested in enhancing their science teaching curriculum.
(Contact [email protected] for details.) Here are
some of the topics to be covered:
New approaches to teaching Beer’s Law, kinetics, and
absorbance and transmission measurements
Reworking your old single-wavelength spectrometer
curricula to labs based on Ocean Optics spectrometers
Tel: 727.733.2447 • Email: [email protected]
Our Value Proposition
Ocean Optics offers small-footprint, multi-purpose PC-based
instrumentation -- and more -- to meet most any educational
application requirement:
Our fully integrated CHEM4-series Spectrophotometers come
with light sources and cuvette holders that attach directly to
the spectrometer or connect via fiber. See pages 36-37.
The $999 Red Tide is a general-purpose instrument for
budget-strapped teaching labs. It is a good choice for
simple visible absorbance setups. For more, see page 38.
For users who prefer to avoid PCs, consider our educational
partner Pasco and its Xplorer GLX, a datalogger and lab
analysis tool in one. The GLX turns our USB-based
spectrometers into PC-free systems. See page 39.
Our modular spectrometers work well with the industry’s
most extensive selection of spectroscopy accessories, from
cuvettes and standards to optical fibers and dip probes.
Getting the most out of your modular spectrometer -- how
one spectrometer design can be easily configured to explain
principles in chemistry, physics or other disciplines
Multiple Options, Maximum Convenience
Our low-cost, small-footprint educational spectrometer systems
are now available directly from Ocean Optics or through one of
our educational vendor partners:
PASCO Scientific (pasco.com)
Vernier Software & Technology (vernier.com)
MeasureNet Technology Ltd. (measurenet-tech.com)
MicroLab, Inc. (microlabinfo.com)
Nicholl Education (nicholl.co.uk)
SK Science Kit & Boreal Laboratories (sciencekit.com)
VWR Education (vwreducation.com) network of brands,
including Sargent-Welch and ScholAR Chemistry
WARD’S Natural Science (wardsci.com)
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Customer Service: Accessible & Flexible
Making Great Service Our Hallmark
We designed our products by first imagining how we would sell
them -- i.e., we actually pictured ourselves talking to our
prospects, discovering their needs and wants, and offering them
the best solutions possible. As researchers ourselves, we realized
the key to serving you well was flexibility -- flexibility in our
modular products, flexibility in our attitude, flexibility in the way
we handle your needs. We realize that great service is not a
slogan -- it’s an attitude, a philosophy.
Before the Sale: R&D and Applications Support
Our Value Proposition
Our Applications Scientists are consultants in the best sense of
the word, because they’re guided by one central question:
Why? If we don’t ask you what your sample is and why you
want to measure it, we haven’t given you our best effort.
Sentiment is all well and good, you say, but what specifically
can you do for me? Well, consider our pre-sale support:
R&D. Prospects interested in developing new applications
using our technology can draw on the resources of our OEM
and Applications Groups, which comprise sales, engineering
and technical support resources. We offer optical and electronic design services, software and firmware engineering,
testing and validation services, and rapid prototyping.
Applications. Our Applications Scientists take ownership of
your most challenging applications needs. When you ask if
our spectrometer can measure a certain sample, we
respond, “Well, we don’t know -- what is this sample and
why do you want to measure it?” In short order, we have
configured a system to measure the sample, we have put
your order in the queue, and we’ve perhaps even started to
work on a new accessory that we’ll need to fill the order.
Tradeshows and Seminars. What better opportunity to see
our products in action than to attend a tradeshow? Our
combined locations will exhibit at nearly 100 tradeshows
worldwide this year (for a schedule of shows in the U.S., see
www.oceanoptics.com/tradeshows.asp). In addition, we will
host various seminars throughout the year, including our
Customer Forum and Educator Training. Check
OceanOptics.com for details.
Sales & Service. With offices in Europe, Asia and the United
States, and a network of distributors around the world, our
service reach is truly global. In the States, we offer expanded
service hours (Mondays-Thursdays 8 a.m.-8 p.m. and
Fridays 8 a.m.-6 p.m. EST) and late-day shipping options.
Customer sales & service representatives are available to
take orders, provide order status, relay pricing and product
information, and handle any basic service request. We are
available via email and soon will add e-commerce and
other multimedia services to our website. For a list of our
locations see page 5 or visit oceanoptics.com/contactus.asp.
Help with the “Little” Things. Contact our Customer
Sales & Service Department (727.733.2447 or
[email protected]) for questions regarding order
status, delivery times, shipping charges and more. And
when you call, you’ll speak to an actual person.
Troubleshooting Challenges. If you run into an issue with
your order, our Applications Scientists and Technical Support
staff ([email protected]) can help. The former
are especially useful for help with your configuration or
experiment; the latter can assist with getting started,
hardware-software compatibility, firmware and software
programming issues and more.
Repairs and Returns. Occasionally, orders don’t work out
exactly as planned. If you need a Return Merchandise
Authorization (RMA) for a repair or an upgrade, contact us
at 727.733.2447 or [email protected] It’s rare
that spectrometer components or accessories fail; more
often than not, our RMAs cover changes in spectrometer
configuration, bench upgrades and the like.
Additional Resources
We provide readily accessible technical and support information
on our website and
in other media:
Our Software &
Technical
Resources CD
ships with every
order, and
contains
manuals,
operating
instructions and
software. These
materials are
also conveniently
available online at oceanoptics.com/technical.asp.
Engineering-level documents are also available online, at
oceanoptics.com/technical/engineeringdocs.asp. This is
where you’ll find information on topics such as CCD
detectors and linearity, lamp stability and USB adapter
interfaces.
Click the APPLICATIONS button at OceanOptics.com to view
an Applications Database of journal articles that reference
our products. And it’s always fun to do a search at
http://scholar.google.com. The last time we looked, there
were over 5,000 listings for Ocean Optics spectrometers.
Other resources include a UV-Vis Spectral Database CD,
short video clips on basic spectroscopy measurements, and
a handbook in both print and CD formats on the use of
spectroscopy in the teaching lab. For details, contact an
Applications Scientist.
After the Sale: Customer Service & Tech Support
Our relationship with the customer doesn’t end once the order
goes out the door. In fact, our assistance after the sale is often
where we provide the most value to our customers. Whether it’s
helping you to get started, or troubleshooting a challenge you’re
facing, we offer post-sale support in various guises:
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How Are We Doing?
We love hearing from our customers. Your feedback helps us
serve you better. Please direct your questions, concerns and
comments to [email protected] or write to us at Ocean
Optics, Inc., 830 Douglas Ave., Dunedin, FL 34698 USA.
For all your sensing needs, visit OceanOptics.com
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Spectrometers
wish to select components and options in their
spectrometer, from the wavelength range and grating
type to the size of the entrance aperture and type of
coatings on the detector.
14
USB4000 Plug-and-Play Spectrometer
15
“USB” Optical Bench Options
20
HR2000+ High-speed High-Resolution
Spectrometer
21
HR4000 High-resolution Spectrometer
22
“HR”-series Optical Bench Options
26
QE65000 Scientific-grade Spectrometer
27
“QE” Optical Bench Options
30
NIR-512 Near-infrared Spectrometer
30
NIR256 Extended-range NIR Spectrometers
32
“NIR”-series Optical Bench Options
Spectrometers
User-configured Spectrometers are for those who
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Overview: Spectrometers
We Have Your Spectrometer!
Since we introduced the world's first miniature spectrometer 15 years ago,
we've sold more than 85,000 spectrometers and enabled thousands of
applications. We pioneered the notion of flexible, modular spectroscopy,
making it possible for users in many industries to configure systems for
very different applications.
Spectrometers
For those who wish to select the components in their spectrometer, we
offer a complete range of options. You can make it your way:
The size of your entrance aperture helps determine how much light
enters your optical bench and is a factor in determining optical
resolution. We have six sizes of entrance apertures.
Our filters block second- and third-order effects or balance color.
You can opt to install standard collimating and focusing mirrors or
SAG+ mirrors, which increase reflectance and sensitivity.
We offer 14 different gratings. Your choice helps determine your
resolution and wavelength range.
An optional collection lens increases light-collection efficiency.
Our OFLV filters precisely block second- and third-order light from
reaching specific detector elements.
A UV upgrade enhances the spectrometer’s performance in the UV.
Our Applications Scientists have configured thousands of spectrometer
setups. Simply tell us what you want to measure and why and we’ll
configure the optimum system for your application.
Detector Type
Bench Type
Spectrometer Type
CCD Detectors
We use a 3648-pixel CCD-array detector from
Toshiba in both our “USB” and “HR” optical
benches that’s ideal for general-purpose
applications. The Sony ILX511 is a 2048-pixel
linear CCD-array detector that’s still used in a
couple of our specialized spectrometer
offerings.
General-purpose “USB” Bench
The “USB” optical bench (also called
the “S” bench) is ideal for absorbance,
reflectance, fluorescence and color
measurements. It’s a versatile bench
that is used in tens of thousands of
spectrometers around the world.
Spectrometers
You select the optical bench
options, such as the grating,
entrance aperture size, detector,
wavelength range and more to
create the optimum spectrometer
for your application.
High-resolution “HR” Bench
The “HR” optical bench is designed for
applications requiring sub-angstrom
optical resolution, such as laser
characterization and atomic emission
spectroscopy.
Spectrometer Systems & Setups
Systems are turnkey spectrophotometers where all the components
are included in one integrated
enclosure. Setups provide a list of
tools necessary for an application.
Both Systems and Setups include a
spectrometer, the necessary
sampling accessories, a light
source and software. Some
spectrometers are preset with a
grating, wavelength range and
other bench accessories for
specific measurement types such
as fluorescence. You still specify
other components, such as light
sources and sampling accessories.
Photodiode Detectors
Less-sensitive photodiode detectors provide a
high signal-to-noise ratio for applications with
high light levels. We use Hamamatsu’s S3903
and S3904 photodiode silicon linear arrays for
our Deep-well Spectrometers.
Back-thinned TE-cooled Detector
The Hamamatsu S7031-1006 detector in the
“QE” optical bench provides high quantum
efficiency, fast signal processing speed and a
high signal-to-noise ratio. This TE-cooled
detector generates virtually no dark noise.
InGaAs Detectors
We use three different Hamamatsu linear array
InGaAs detectors in our “NIR” optical bench for
general-purpose NIR applications.
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Scientific-grade “QE” Bench
The “QE” optical bench is designed for
demanding applications with low light
levels such as Raman and fluorescence.
Near-Infrared “NIR” Bench
The “NIR” optical bench is designed for
applications that require sensitivity in
the NIR region, such as moisture
analysis, tunable laser wavelength
characterization and general NIR
spectroscopy.
For all your sensing needs, visit OceanOptics.com
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Spectrometer Comparison Chart
This table outlines the specifications of our most popular user-configured spectrometers.
Please refer to specific product pages for more detailed information.
Specifications
PHYSICAL
Dimensions (in mm):
Weight:
DETECTOR
Detector:
USB4000
p. 14
HR2000+
p. 20
HR4000
p. 21
QE65000
p. 26
148.6 x 104.8 x 45.1
570 grams
148.6 x 104.8 x 45.1
570 grams
182 x 110 x 47
1050 grams
Toshiba TCD1304AP linear
CCD array
200-1100 nm
3648 pixels
8 µm x 200 µm
~100,000 electrons
Sony ILX511 linear silicon CCD
array
200-1100 nm
2048 pixels
14 µm x 200 µm
~62,500 electrons
Toshiba TCD1304AP linear
CCD array
200-1100 nm
3648 pixels
8 µm x 200 µm
~100,000 electrons
400 nm: 130 photons/count
600 nm: 60 photons/count
400 nm: 75 photons/count
600 nm: 41 photons/count
400 nm: 130 photons/count
600 nm: 60 photons/count
Hamamatsu S7031-1006 backthinned area CCD
200-1100 nm
1024 x 58 (1044 x 64 total)
24.6 µm square size
300,000 electrons/well
~1.5 million electrons/column
22 electrons/count for all
wavelengths
250 nm: 26 photons/count
f/4, Asymmetrical crossed
Czerny-Turner
42 mm
68 mm
5, 10, 25, 50, 100, or
200 µm wide slits or fiber
14 gratings, UV through
Shortwave NIR
No
f/4, Symmetrical crossed
Czerny-Turner
101.6 mm
101.6 mm
5, 10, 25, 50, 100 or
200 µm wide slits or fiber
14 gratings, UV through
Shortwave NIR
No
Yes, L4
OFLV-200-850
OFLV-350-1000
Longpass OF-1 filters
SMA 905 to 0.22 numerical
aperture single-strand fiber
Yes, L2
No
f/4, Symmetrical crossed
Czerny-Turner
101.6 mm
101.6 mm
5, 10, 25, 50, 100 or
200 µm wide slits or fiber
14 gratings, UV through
Shortwave NIR
Yes, HC-1 provides 2001050 nm range (best efficiency)
Yes, L4
OFLV-200-1100
f/4, Symmetrical crossed
Czerny-Turner
101.6 mm
101.6 mm
5, 10, 25, 50, 100 or
200 µm wide slits or fiber
14 gratings, UV through
Shortwave NIR
Yes, HC1-QE provides
200-950 nm range
No
OFLV-QE
Longpass OF-1 filters
SMA 905 to 0.22 numerical
aperture single-strand fiber
Longpass OF-1 filters
SMA 905 to 0.22 numerical
aperture single-strand fiber
Longpass OF-1 filters
SMA 905 to 0.22 numerical
aperture single-strand fiber
Grating dependent
~0.3-10.0 nm FWHM
300:1 (at full signal)
16 bit
50 RMS counts
2 x 108 (system); 1300:1 for a
single acquisition
3.8 ms to 10 seconds
<0.05% at 600 nm
<0.10% at 435 nm
>99.8%
Grating dependent
~0.035-6.8 nm FWHM
250:1 (at full signal)
14 bit
12 RMS counts
2 x 108 (system); 1300:1 for a
single acquisition
1 ms to 20 seconds
<0.05% at 600 nm
<0.10% at 435 nm
>99.8%
Grating dependent
~0.02-8.4 nm FWHM
300:1 (at full signal)
14 bit
12 RMS counts
2 x 108 (system); 1300:1 for a
single acquisition
3.8 ms to 10 seconds
<0.05% at 600 nm
<0.10% at 435 nm
>99.8%
Grating dependent
~0.14-7.7 nm FWHM
1000:1 (at full signal)
16 bit
2.5 RMS counts
7.5 x 109 (system); 25000:1 for
a single acquisition
8 ms to 15 minutes
<0.08% at 600 nm
<0.4% at 435 nm
>99.8%
250 mA @ 5 VDC
450 mA @ 5 VDC
450 mA @ 5 VDC
Data transfer speed:
Full spectrum to memory every
5 ms with USB 2.0 port,
18 ms with USB 1.1 port
Full spectrum to memory every
4 ms with USB 2.0 port,
18 ms with USB 1.1 port
Inputs/Outputs:
Yes, 8 onboard digital userprogrammable GPIOs
No
Yes, 10 onboard digital userprogrammable GPIOs
Yes, one 13-bit analog input
and one 9-bit analog output
4 modes
Yes
Yes
No
Yes, 10 onboard digital userprogrammable GPIOs
No
4 modes
Yes
Yes
Yes
Full spectrum to memory every
1 ms with USB 2.0 port,
15 ms with USB 1.1 port,
200 ms with serial port
Yes, 10 onboard digital userprogrammable GPIOs
Yes, one 13-bit analog input
and one 9-bit analog output
4 modes
Yes
Yes
Yes
500 mA @ 5 VDC no TE cool
3 A @ 5 VDC with TE cool
Full spectrum to memory every
8 ms with USB 2.0 port,
8 ms with USB 1.1 port
Windows 98/Me/2000/XP, Mac
OS X and Linux when using the
USB port;
Any 32-bit Windows OS when
using the serial port
USB 2.0 @ 480 Mbps
(USB 1.1 compatible);
RS-232 (2-wire) @ 115.2 K
baud
SPI (3-Wire);
I2C inter-integrated circuit\
Windows 98/Me/2000/XP, Mac
OS X and Linux when using the
USB port;
Any 32-bit Windows OS when
using the serial port
USB 2.0 @ 480 Mbps
(USB 1.1 compatible);
RS-232 (2-wire) @ 115.2 K
baud
SPI (3-Wire);
I2C inter-integrated circuit
Windows 98/Me/2000/XP, Mac
OS X and Linux when using the
USB port;
Any 32-bit Windows OS when
using the serial port
USB 2.0 @ 480 Mbps
(USB 1.1 compatible);
RS-232 (2-wire) @ 115.2 K
baud
SPI (3-Wire);
I2C inter-integrated circuit
Windows 98/Me/2000/XP, Mac
OS X and Linux when using the
USB port;
Any 32-bit Windows OS when
using the serial port
USB 2.0 @ 480 Mbps;
RS-232 (2-wire) @ 115.2 K
baud
Detector range:
Pixels:
Pixel size:
Pixel well depth:
Sensitivity:
OPTICAL BENCH
Design:
Focal length (input):
Focal length (output):
Entrance aperture:
Grating options:
HC-1 grating option:
Detector collection lens:
OFLV filters:
Order-sorting filters:
Fiber optic connector:
SPECTROSCOPIC
Wavelength range:
Optical resolution:
Signal-to-noise ratio:
A/D resolution:
Dark noise:
Dynamic range:
Integration time:
Stray light:
Corrected linearity:
ELECTRONICS
Power consumption:
Analog channels:
Trigger modes:
Auto nulling:
Strobe functions:
Gated delay feature:
COMPUTER
Operating systems:
Computer interfaces:
Peripheral interfaces:
Tel: 727.733.2447 • Email: [email protected]
Spectrometers
89.1 x 63.3 x 34.4
190 grams
4 modes
Yes
No
Yes
SPI (3-wire);
I2C inter-integrated circuit
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USB4000 Plug-and-Play Spectrometer
We’ve sold over 85,000 spectrometer channels
for thousands of applications, and we've used
that experience to make the most flexible, versatile and cost-effective spectrometer ever built.
World’s Most Popular Spectrometer Just Got Better
Spectrometers
In this setup, a USB4000 is
configured for fluorescence. A
PX-2 Pulsed Xenon Light
Source provides the
excitation via optical fiber
and a CUV-FL-DA Directattach Cuvette Holder holds
the sample and redirects light
energy directly into the
USB4000 Spectrometer. A filter,
such as one of our LVFs, are often
used to block excitation wavelengths.
Specifications
PHYSICAL
Dimensions (in mm):
Weight:
DETECTOR
Detector:
Detector range:
Pixels:
Pixel size:
Pixel well depth:
Sensitivity:
OPTICAL BENCH
Design:
Focal length:
Entrance aperture:
Grating options:
Fiber optic connector:
SPECTROSCOPIC
Wavelength range:
Optical resolution:
Signal-to-noise ratio:
A/D resolution:
Dark noise:
Dynamic range:
Integration time:
Stray light:
Corrected linearity:
ELECTRONICS
Power consumption:
Data transfer speed:
Inputs/Outputs:
Analog channels:
Trigger modes:
Strobe functions:
COMPUTER
Operating systems:
89.1 x 63.3 x 34.4
190 grams
Toshiba TCD1304AP linear CCD array (page 17)
200-1100 nm
3648 pixels
8 µm x 200 µm
~100,000 electrons
130 photons/count at 400 nm;
60 photons/count at 600 nm
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Electronic Advancements
The USB4000 Spectrometer is distinguished by its enhanced
electronics: 16-bit A/D resolution with auto nulling feature (an
enhanced electrical dark-signal correction); EEPROM storage
of calibration coefficients for simple spectrometer start-up;
8 programmable GPIO signals for controlling peripheral
devices; and an electronic shutter for spectrometer integration
times as fast as 3.8 milliseconds -- a handy feature to prevent
detector saturation. In addition, the USB4000 has signal-tonoise of 300:1 and optical resolution (FWHM) ranging from
0.03-8.4 nm (depending on your grating and entrance
aperture selection).
Here the versatile USB4000 is featured
in a liquid absorbance setup with optical
fiber, a DH2000 Deuterium Tungsten
Halogen Light Source and a CUV-UV-10
10-cm Pathlength Cuvette Holder.
f/4, Asymmetrical crossed Czerny-Turner
42 mm input; 68 mm output
5, 10, 25, 50, 100, or 200 µm wide slit or fiber (page 15)
14 gratings, UV through Shortwave NIR (page 16)
SMA 905 to 0.22 numerical aperture single-strand fiber
Grating dependent
~0.3-10.0 nm FWHM
300:1 (at full signal)
16 bit
50 RMS counts
2 x 108 (system); 1300:1 for a single acquisition
3.8 ms to 10 seconds
<0.05% at 600 nm; <0.10% at 435 nm
>99.8%
250 mA @ 5 VDC
Full spectrum to memory every 5 ms with USB 2.0 port,
18 ms with USB 1.1 port
Yes, 8 onboard digital user-programmable GPIOs
No
4 modes
Yes
Windows 98/Me/2000/XP, Mac OS X and Linux with
USB port; Any 32-bit Windows OS with serial port
Computer interfaces: USB 2.0 @ 480 Mbps; RS-232 (2-wire) @ 115.2 K baud
Peripheral interfaces: SPI (3-wire); I2C inter-integrated circuit
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We redesigned the USB4000 -- the most popular spectrometer
in the world -- to include an advanced detector and powerful
high-speed electronics. The USB4000 features a 16-bit A/D,
four triggering options, a dark-level correction during
temperature changes, and a 22-pin connector with eight userprogrammable GPIOs. What’s more, the USB4000 interfaces
to computers with Linux, Mac or Windows operating systems.
The modular USB4000 is responsive from 200-1100 nm and
can be configured with various Ocean Optics optical bench
accessories, light sources and sampling optics to create
application-specific systems for thousands of absorbance,
reflection and emission applications.
Streamlined Start-up Software & Hot Swapping
The USB4000 interfaces to a computer via USB 2.0. Data
unique to each spectrometer is programmed into a memory
chip on the USB4000; SpectraSuite Spectroscopy Operating
Software reads these values for easy setup and hot swapping
among computers, whether they run on Linux, Mac or
Windows operating systems. When connected to a computer
via USB, the USB4000 draws its power from the computer.
With its small-footprint design, plug-and-play convenience,
advanced electronics and powerful detector, the USB4000 has
succeed the USB2000 as the most frequently specified fiber
optic spectrometer in the world.
USB4000:
$2,199
SPECTRASUITE:
$199
For all your sensing needs, visit OceanOptics.com
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USB4000 Optical Bench Options
What makes the USB4000 Spectrometer so special are the options that allow you to configure the bench for
your application. Our Applications Scientists can help you choose the optimum components, or you can follow
this guide to choose an entrance aperture size, detector accessories, filters, a grating and more. The diagram
below shows how light moves through the asymmetrical crossed Czerny-Turner optical bench, which has no
moving parts that can wear or break; all components specified are fixed in place at the time of manufacture.
Components of the USB4000 Optical Bench
1 SMA 905 Connector
Light from a fiber enters the optical bench through the SMA 905 Connector. The
SMA 905 bulkhead provides a precise locus for the end of the optical fiber, fixed
slit, absorbance filter and fiber clad mode aperture.
4
2 Fixed Entrance Slit: specify slit size
8
Light passes through the installed slit, which acts as the entrance aperture. Slits
come in various widths from 5 µm to 200 µm. The slit is fixed in the SMA 905
bulkhead to sit against the end of a fiber.
6
7
3 Longpass Absorbing Filter: optional
9
10
If selected, an absorbance filter is installed between the slit and the clad mode
aperture in the SMA 905 bulkhead. The filter is used to block second- and thirdorder effects or to balance color.
5
3
2
4 Collimating Mirror: specify standard or SAG+
The collimating mirror is matched to the 0.22 numerical aperture of our optical
fiber. Light reflects from this mirror, as a collimated beam, toward the grating.
You can opt to install a standard mirror or a UV absorbing SAG+ mirror.
1
Spectrometers
8 Detector
5 Grating & Wavelength Range: specify grating & starting wavelength
We offer a 3648-element Toshiba TCD1304AP linear CCD
array detector. Each pixel responds to the wavelength of light
that strikes it. Electronics bring the complete spectrum to the
software.
We install the grating on a platform that we then rotate to select the starting
wavelength you’ve specified. Then we permanently fix the grating in place to
eliminate mechanical shifts or drift.
6 Focusing Mirror: specify standard or SAG+
This mirror focuses first-order spectra on the detector plane. Both the collimating
and focusing mirrors are made in-house to guarantee the highest reflectance and
the lowest stray light possible. You can opt to install a standard or SAG+ mirror.
9 OFLV Variable Longpass Order-sorting Filter: optional
Our proprietary filters precisely block second- and third-order
light from reaching specific detector elements.
10 UV4 Detector Upgrade: optional
7 L4 Detector Collection Lens: optional
When selected, the detector’s standard BK7 window is
replaced with a quartz window to enhance the performance
of the spectrometer for applications <340 nm.
This cylindrical lens, made in-house to ensure aberration-free performance, is
fixed to the detector to focus the light from the tall slit onto the shorter detector
elements. It increases light-collection efficiency.
1 SMA 905 Connector
A precision SMA 905 Connector aligns to the spectrometer’s entrance slit and ensures concentricity of the fiber.
For an upgrade fee that includes the cost of the custom connector and labor, we will replace the standard
SMA 905 Connector with a different connector of your choice. We also offer connector adapters, such as an
SMA-to-ST Adapter and an SMA-to-FC Adapter. Please call for details on connectors and adapters.
2 Fixed Entrance Slit
Another option available with a USB4000 user-configured spectrometer is the size of the entrance aperture.
Entrance slits are rectangular apertures, 1-mm tall and various widths from 5 µm to 200 µm, with the width
determining the amount of light entering the bench. A slit is permanent; it only can be changed by our
technicians. You can opt against having a slit, in which case the diameter of the fiber connected to the
spectrometer determines the size of the entrance aperture.
Slit
Description
Pixel Resolution
SLIT-5
5-µm wide x 1-mm high
~5.3 pixels
Price
$150
SLIT-10
10-µm wide x 1-mm high
~5.7 pixels
$150
SLIT-25
25-µm wide x 1-mm high
~7.5 pixels
$150
SLIT-50
50-µm wide x 1-mm high
~11.6 pixels
$150
SLIT-100
100-µm wide x 1-mm high
~21 pixels
$150
SLIT-200
200-µm wide x 1-mm high
~42 pixels
$150
Tel: 727.733.2447 • Email: [email protected]
A slit is
installed
on the inside
edge of the
bulkhead of an
SMA 905 Connector.
15
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USB4000 Optical Bench Options
3 Longpass Absorbing Filter
We offer longpass absorbing or blocking filters; each filter
has a transmission band and a blocking band to restrict
radiation to a certain wavelength region for eliminating
second- and third-order effects. These filters are installed
permanently between the slit and the clad mode aperture
in the bulkhead of the SMA 905 Connector.
Item
Description
OF1-WG305
Longpass filter; transmits light >305 nm
$50
OF1-GG375
Longpass filter; transmits light >375 nm
$50
OF1-GG475
Longpass filter; transmits light >475 nm
$50
OF1-OG515
Longpass filter; transmits light >515 nm
$50
OF1-OG550
Longpass filter; transmits light >550 nm
$50
OF1-OG590
Longpass filter; transmits light >590 nm
$50
4 Collimating & Focusing Mirrors
Spectrometers
6
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SAG+ Mirror Reflectivity
You can replace standard aluminum-coated reflective mirrors with our
proprietary, UV-absorbing SAG+ Mirrors, which increase reflectance in
the VIS-NIR and, in turn, increase the sensitivity of the spectrometer.
SAG+ Mirrors are often specified for fluorescence. These mirrors also
absorb nearly all UV light, which reduces the effects of excitation
scattering in fluorescence measurements. Unlike typical silver-coated
mirrors, the SAG+ mirrors won't oxidize. They have excellent reflectivity -more than 95% across the VIS-NIR.
SAG+UPG:
$250
100%
REFLECTIVITY
&
Price
80%
60%
40%
20%
0
200
400
600
800
1000
WAVELENGTH (nm)
5 Choosing a Grating & Wavelength Range
Wide Selection Allows Flexibility
Grating Selection Chart
The Groove Density (mm-1)
of a grating determines its
dispersion, while the angle of
the groove determines the most
efficient region of the spectrum.
The greater the groove density,
the better the optical resolution
Performance & Stability
possible, but the more truncated the
Instead of the gratings rotating as they do in instruments
spectral range.
such as scanning monochromators, our gratings are
permanently fixed in place at the time of manufacture to
The Spectral Range is the dispersion of the grating
ensure long-term performance and stability. (See page 18
across the linear array. The spectral range (bandwidth)
for Grating Efficiency Curves.) A grating must be specified
is a function of the groove density and does not
for each spectrometer. We offer ruled and holographic
change. When you choose a starting wavelength for a
diffraction gratings. Both are polymer replicas of master
spectrometer, you add its spectral range to the starting
gratings. There are trade-offs between these gratings:
wavelength to determine the wavelength range.
holographic gratings produce less stray light while ruled
For ruled gratings, the Blaze Wavelength is the peak
gratings are more reflective, resulting in higher sensitivity.
wavelength in an efficiency curve. For holographic
gratings, it is the most
Grating
Intended
Groove
Spectral
Blaze
Best Efficiency
efficient wavelength region.
Number
Use
Density
Range
Wavelength
(>30%)
The Best Efficiency region is
1
UV
600
650 nm
300 nm
200-575 nm
the range where efficiency is
2
UV-VIS
600
650 nm
400 nm
250-800 nm
>30%. In some cases,
3
VIS-Color
600
650 nm
500 nm
350-850 nm
4
NIR
600
625 nm
750 nm
530-1100 nm
gratings have a greater
5
UV-VIS
1200
300 nm
Holographic UV
200-400 nm
spectral range than is
6
NIR
1200
200-270 nm
750 nm
500-1100 nm
efficiently diffracted. For
7
UV-VIS
2400
100-140 nm
Holographic UV
200-500 nm
example, Grating #1 has a
8
UV
3600
50-75 nm
Holographic UV
290-340 nm
650 nm spectral range, but
9
VIS-NIR
1200
200-270 nm
Holographic VIS
400-800 nm
is most efficient from
10
UV-VIS
1800
100-190 nm
Holographic UV
200-635 nm
200-575 nm. In this case,
11
UV-VIS
1800
120-160 nm
Holographic VIS
320-720 nm
wavelengths >575 nm will
12
UV-VIS
2400
50-120 nm
Holographic VIS
250-575 nm
have lower intensity due to
13
UV-VIS-NIR
300
1700 nm
500 nm
300-1100 nm
the the grating’s reduced
14
NIR
600
625 nm
1000 nm
650-1100 nm
efficiency.
You choose from among 14 gratings for each spectrometer. With each grating, you consider its groove density (which
helps determine the resolution), its spectral range (which
helps determine the wavelength range) and its blaze wavelength (which helps determine the most efficient range).
16
For all your sensing needs, visit OceanOptics.com
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USB4000 Optical Bench Options
7 L4 Detector Collection Lens
This cylindrical lens, made in-house to ensure aberration-free performance, is fixed to the
detector’s window to focus the light from the tall slit onto the shorter detector elements. It
increases light-collection efficiency and reduces stray light. It also is useful in a
configuration with a large-diameter fiber for low light-level applications. At
right is a detector with the L4 lens.
L4 Detector Collection Lens: $150
Toshiba TCD1304AP Detector with L4 Detector
Collection Lens (above) and without (below).
8 Detector: 3648-element Linear CCD Array
In each USB4000, we install the Toshiba TCD1304AP
linear CCD array detector. In the USB2000, the
USB4000’s predecessor, we used the Sony ILX511
detector. Both are linear silicon CCD arrays, with an
effective range of 200-1100 nm, and with the same
dynamic range (1300:1).
9
10
Detector Sensitivity Comparison
4000
Sony 2048-element ILX511 Detector
INTENSITY (COUNTS)
Toshiba 3648-element TCD1304AP Detector
3000
2000
1000
0
200
300
Detector with OFLV Filter
Our OFLV Variable Longpass Order-sorting Filters are
applied to the detector’s window to eliminate secondand third-order effects. We use patented coating
technology to apply the filter onto the substrate. In fact,
we are the only miniature spectrometer manufacturer to
offer “clean” first-order spectra.
Detector with UV4 Detector Window Upgrade
When you specify a detector with the UV4 Detector
Window Upgrade, we replace the detector’s standard
BK7 window with a quartz window to enhance the
spectrometer‘s performance from 200-340 nm.
400
500
600
700
800
900
STARTING WAVELENGTH (nm)
Spectrometers
There are some differences between the Toshiba detector
and the Sony detector. For example, since the Toshiba’s
pixels are only 8 µm wide instead of 14 µm wide, the
sensitivity for a Toshiba pixel seems to be ~60%
(8 µm/14 µm) that of a Sony pixel (see graph at right).
However, on a per-unit area basis, the sensitivity is about
the same since the Toshiba has 3648 pixels compared with
the Sony’s 2048; the total signal is the same. Because the
Toshiba detector has an electronic shutter, you can almost
never have too much light; the shutter prevents the
detector from saturating.
Toshiba TCD1304AP Specifications
Detector:
Detector range:
Pixels:
Pixel size:
Pixel well depth:
Sensitivity:
Maximum pixel rate:
Toshiba TCD1304AP linear CCD array
200-1100 nm
3648 pixels
8 µm x 200 µm
~100,000 electrons
400 nm: 130 photons/count, 600 nm: 60 photons/count
Rate at which pixels are digitized is 1 MHz
Detector
Description
DET4-VIS
Toshiba TCD1304AP Detector installed into a USB4000 User-Configured Spectrometer; best for systems
Price
Free
with wavelength ranges above 400 nm
DET4-UV
Toshiba TCD1304AP Detector with UV4 Detector Window Upgrade installed into a USB4000 User-
$150
Configured Spectrometer; best for systems with wavelength ranges in the UV
DET4-350-1000
Toshiba TCD1304AP Detector with OFLV-350-1000 Variable Longpass Order-sorting Filter installed into a
$150
USB4000 User-Configured Spectrometer; best when using Grating #2, #3 or #4
DET4-200-850
Toshiba TCD1304AP Detector with UV4 Detector Window Upgrade and OFLV-200-850 Variable Longpass
$300
Order-sorting Filter installed into a USB4000 Spectrometer; best when using Grating #1 or #2
Tel: 727.733.2447 • Email: [email protected]
17
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USB4000 Optical Bench Options
Grating Efficiency Curves
Predicted Ranges & Resolution
Below are the Grating Efficiency Curves for gratings
with groove densities of 600, 1200, 1800 and
2400 mm-1. See curves for all of our gratings at
OceanOptics.com/Technical/GratingCharts.asp.
Here are a series of graphs to demonstrate the range and optical
resolution (FWHM) of your USB4000 Spectrometer with a 25 µm slit.
See our website for additional graphs of ranges and resolutions for
every slit size.
600 mm-1 Grating and 25-µm Slit
Gratings with Groove Density of 600
RELATIVE EFFICIENCY
70
#1
60
#2
50
#3
#4
40
#14
SPECTRAL RANGE (nm)
80
30
680
1.36
670
1.34
660
1.32
650
1.30
640
630
1.28
620
1.26
610
1.24
600
1.22
590
20
200
400
600
800
1000
580
200
1200
RESOLUTION (nm)
oo
300
400
500
600
700
800
1.20
900 1000
Example:
If the starting
wavelength is
250 nm, then
the range is
~667 nm,
providing a
250-917 nm
wavelength
range and
1.34 nm
resolution.
STARTING WAVELENGTH (nm)
WAVELENGTH (nm)
Efficiency Curves for Gratings 1, 2, 3, 4 and 14.
1200 mm-1 Grating and 25-µm Slit
Gratings with Groove Density of 1200
350
RELATIVE EFFICIENCY
60
#5
#6
50
#9
40
30
0.65
310
0.60
290
0.55
270
250
0.50
230
0.45
210
0.40
190
0.35
170
20
200
400
600
800
1000
150
200
1200
300
WAVELENGTH (nm)
400
500
600
700
800
900
0.30
1000
Example:
If the starting
wavelength is
350 nm, then
the range is
~310 nm,
providing a
350-660 nm
wavelength
range and
0.63 nm
resolution.
STARTING WAVELENGTH (nm)
Efficiency Curves for Gratings 5, 6 and 9.
1800 mm-1 Grating and 25-µm Slit
240
70
220
60
#10
#11
50
40
30
SPECTRAL RANGE (nm)
80
0.45
0.40
200
180
0.35
160
0.30
140
0.25
120
20
200
400
600
800
1000
100
200
1200
RESOLUTION (nm)
Gratings with Groove Density of 1800
RELATIVE EFFICIENCY
Spectrometers
70
SPECTRAL RANGE (nm)
330
RESOLUTION (nm)
80
WAVELENGTH (nm)
300
400
500
600
700
0.20
800
Example:
If the starting
wavelength is
400 nm, then
the range is
~190 nm,
providing a
400-590 nm
wavelength
range and
0.38 nm
resolution.
STARTING WAVELENGTH (nm)
Efficiency Curves for Gratings 10 and 11.
2400 mm-1 Grating and 25-µm Slit
Gratings with Groove Density of 2400
160
80
0.32
60
#7
#12
50
40
30
20
200
400
600
800
WAVELENGTH (nm)
1000
1200
0.30
140
0.28
130
0.26
120
0.24
110
0.22
100
0.20
90
0.18
80
200
300
400
500
0.16
600
RESOLUTION (nm)
RELATIVE EFFICIENCY
70
SPECTRAL RANGE (nm)
150
Example:
If the starting
wavelength is
300 nm, then
the range is
~140 nm,
providing a
300-440 nm
wavelength
range and
0.29 nm
resolution.
STARTING WAVELENGTH (nm)
Efficiency Curves for Gratings 7 and 12.
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18
For all your sensing needs, visit OceanOptics.com
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USB4000 Direct-attach Accessories
USB-DT Deuterium Tungsten Light Source
USB-DT
The USB-DT Deuterium Tungsten Light Source is our most versatile combination UV-VIS
lamp. Use the USB-DT as a stand-alone unit with any spectrometer, stack it with a
USB4000 Spectrometer, or combine it with a “breakout box” accessory and an “HR”series or QE65000 Spectrometer for software control of lamp functions. This compact
source is about the size of a deck of cards, provides stable, broadband output from
200-2000 nm, and requires a simple 5-volt wall transformer to operate. See page 124
for details.
USB-DT: $1,499
USB-ISS-UV-VIS
USB-ISS-UV-VIS Integrated Sampling System for Cuvettes
The USB-ISS-UV-VIS is a direct-attach sample holder and deuterium tungsten light source
(200-1100 nm) for measuring absorbance. This sampling system allows you to control
both the intensity of the tungsten bulb and the shutter via software. The USB-ISS-UV-VIS
requires an external power supply (included). See page 92 for more.
USB-ISS-UV-VIS: $1,499
USB-ISS-VIS
USB-ISS-VIS Integrated Sampling System for Cuvettes
Spectrometers
The USB-ISS-VIS is a direct-attach sample holder and violet LED-boosted tungsten light
source (390-900 nm) combination for measuring relative absorbance. The light source
boosts signal in the blue and provides over 10,000 hours of use. See page 92 for full
specifications.
USB-ISS-VIS: $499
USB-ISS-T
USB-ISS-T Integrated Sampling System for Test Tubes
The USB-ISS-T is a direct-attach sample holder and violet LED-boosted tungsten light
source (390-900 nm) combination for measuring absorbance in 12-mm outer diameter
test tubes. The sampling optics combine a diffuse source with a collimated input to the
spectrometer to eliminate optical artifacts in the test tubes. See page 92 for
specifications.
USB-ISS-T: $499
USB-LS-450
USB-LS-450 Pulsed Blue LED Module
The USB-LS-450 is an LED module designed for fluorescence measurements in the lab
or field, or as part of an Oxygen Sensor system. In addition, the USB-LS-450 has a port
for attaching a 100 ohm RTD temperature sensor and onboard memory for storing
temperature and oxygen calibration coefficients. See page 131 for details.
USB-LS-450: $549
USB-FHS
USB-FHS Filter Holder System
The USB-FHS is a filter holder and violet LED-boosted tungsten light source for
measuring filters and other samples up to 18-mm thick. The USB-FHS is optimized for
390-900 nm and attaches to the USB4000 via a mounting plate.
USB-FHS: $499
Tel: 727.733.2447 • Email: [email protected]
19
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HR2000+ High-speed Spectrometer
Monitoring LS-1 Start-up Condition
16000
AMPLITUDE (Counts)
14000
12000
10000
8000
The HR2000+ utilizes an onboard, 2-MHz A/D converter,
which allows you to capture and transfer one full spectrum
into memory every millisecond when the spectrometer is
interfaced to a PC via the USB port.
4000
2000
40
20
0
TIME (ms)
400
300
500
600
700
800
900
1000
WAVELENGTH (nm)
This power-up data for our LS-1 Tungsten Halogen Light Source was
taken by an HR2000+ at 2-millisecond intervals. The graph shows the
tremendous amount of data generated with the HR2000+’s acquisition
rate speed of 1000 spectra per second.
Spectrometers
In this setup,
a DH2000
Deuterium
Light Source
provides light
via optical
fiber to a
CUV-10 Cuvette
Holder for 10-cm
sample cells. A
second optical fiber
collects the light and
sends it to the HR2000+.
Specifications
PHYSICAL
Dimensions:
Weight:
DETECTOR
Detector:
Detector range:
Pixels:
Sensitivity:
OPTICAL BENCH
Design:
Focal length:
Entrance aperture:
Grating options:
Fiber optic connector:
SPECTROSCOPIC
Wavelength range:
Optical resolution:
Signal-to-noise ratio:
Dark noise:
Dynamic range:
Integration time:
ELECTRONICS
Power consumption:
Data transfer speed:
Inputs/Outputs:
Analog channels:
COMPUTER
Operating systems:
148.6 mm x 104.8 mm x 45.1 mm
570 g
Sony ILX511 linear silicon CCD array (page 24)
200-1100 nm
2048 pixels, pixel size of 14 µm x 200 µm
75 photons/count at 400 nm;
41 photons/count at 600 nm
f/4, Symmetrical crossed Czerny-Turner
101.6 mm input, 101.6 mm output
5, 10, 25, 50, 100 or 200 µm wide slits (page 22) or fiber
14 gratings, UV through Shortwave NIR (page 23)
SMA 905 to 0.22 numerical aperture single-strand fiber
Grating dependent
~0.035-6.8 nm FWHM
250:1 (at full signal)
12 RMS counts
2 x 108 (system); 1300:1 for a single acquisition
1 ms to 20 seconds
450 mA @ 5 VDC
Full spectrum to memory every 1 ms with USB 2.0 port,
15 ms with USB 1.1 port, 200 ms with serial port
Yes, 10 onboard digital user-programmable GPIOs*
One 13-bit analog input, one 9-bit analog output
Windows 98/Me/2000/XP, Mac OS X and Linux with
USB port; any 32-bit Windows OS with serial port
Computer interfaces: USB 2.0 @ 480 Mbps; RS-232 (2-wire) @ 115.2 K baud
Peripheral interfaces: SPI (3-Wire), I2C inter-integrated circuit
* Programming the GPIOs requires SpectraSuite, OmniDriver or one of our
other device drivers. See pages 80-82 for details.
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20
The HR2000+ Spectrometer integrates a powerful analog-todigital (A/D) converter, programmable electronics and a
high-resolution optical bench. This innovative combination
produces our fastest spectrometer yet and provides resolution
to 0.035 nm (FWHM).
1,000 Full Spectra/Second
6000
0
80
60
Dynamic Electronics Enhances Control
Programmable Microcontroller
The HR2000+ has an onboard programmable microcontroller
that provides flexibility in controlling the spectrometer and
accessories. Through a new 30-pin connector, you can
implement all operating parameters in the software, such as
controlling external light sources, creating processes and
routines and retrieving data from external devices. The
HR2000+ gives you access to 10 user-programmable digital
I/Os for interfacing to other equipment; one analog input and
one analog output; and a pulse generator for triggering other
devices. (Programming the I/Os requires SpectraSuite
Spectroscopy Operating Software.)
“HR” Optical Bench
The HR2000+ is responsive from 200-1100 nm,
but its specific range,
resolution and sensitivity
depend on your “HR”
Optical Bench options. You
select the grating,
wavelength range, mirror
coating, detector window
and entrance aperture size.
Choose from hundreds of
accessories to create
application-specific systems.
High-resolution Applications
The HR2000+ is ideal for applications where fast reactions
need to be monitored and high resolution is necessary, such
as protein dynamics. For solution chemistry or color measurements, the USB4000 is more likely to fill your requirements.
Plug-and-Play Operation
The HR2000+ interfaces to a PC, PLC or other embedded
controllers via USB 2.0 or serial port. When connected to a PC
via the USB port, the HR2000+ does not require an external
power supply -- the spectrometer draws its power from the PC.
When operating via the serial port, the HR2000+ requires a
power supply (not included). Data unique to each
spectrometer are programmed into a memory chip on the
HR2000+; software reads these values for easy setup and hot
swapping among PCs.
HR2000+: $3,499
For all your sensing needs, visit OceanOptics.com
HR4000 High-resolution Spectrometer
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0.02 nm Optical Resolution (FWHM) Possible
The HR4000 Spectrometer is our next-generation highresolution spectrometer. The HR4000 has a 3648-element
CCD-array detector from Toshiba that enables optical
resolution as precise as 0.02 nm (FWHM). The HR4000 is
responsive from 200-1100 nm, but the specific range and
resolution depend on your grating and entrance slit choices
(see pages 22-24 for options). This novel combination of
optics and electronics is ideal for applications such as
characterizing lasers, measuring gas absorbance, and
determining atomic emission lines.
Electronic Shutter Prevents Saturation
Sample Spectrum of Laser
1000
AMPLITUDE (Counts)
800
600
400
200
0
800
One popular application
for the HR4000 is laser
analysis. A typical setup
may look something
like this: a laser’s
beam is directed into
the FOIS-1 Integrating
Sphere. An optical fiber
collects the light and
sends it to the HR4000.
Onboard Microcontroller
The HR4000’s onboard microcontroller provides you with
considerable flexibility in controlling the spectrometer and
accessories. Through a 30-pin connector, you can implement
all operating parameters in the software: control light
sources, create processes, and retrieve information on
external objects. You have access to 10 user-programmable
digital inputs/outputs for interfacing to other equipment; one
analog input and one analog output; and a pulse generator
for triggering other devices. (Programming the GPIOs
requires SpectraSuite, OmniDriver or one of our other device
drivers. See pages 80-82 for details.)
Plug-and-Play USB Operation
The HR4000 interfaces to a PC, PLC or other embedded
controllers via USB 2.0 or RS-232 serial port. When using
the serial port, the HR4000 requires a single 5-volt power
supply (not included). Data unique to each spectrometer are
programmed into a memory chip on the HR4000; our
spectrometer operating software reads these values for easy
setup and hot swapping among PCs.
HR4000: $3,999
Tel: 727.733.2447 • Email: [email protected]
805
810
WAVELENGTH (nm)
815
Spectrometers
Integration Time is a setting in our software that is specified
by the user. It’s analogous to the shutter speed of a camera:
the value specified for the integration time is the amount of
time the detector “looks” at the incoming photons. Because
the Toshiba detector has an electronic shutter, you can
specify, via software, minimum integration times as short as
3.8 milliseconds, which allow you to measure transient
events like laser pulses. Also, the ability to integrate the
spectrometer for short durations eliminates saturation
problems that can occur in high light-level applications such
as laser analysis.
820
We acquired this spectrum of a 810-nm Multimode Diode Laser with
an HR4000, Grating H11 and a 5-µm slit.
Specifications
PHYSICAL
Dimensions:
Weight:
DETECTOR
Detector:
Detector range:
Pixels:
Pixel well depth:
Sensitivity:
OPTICAL BENCH
Design:
Focal length:
Entrance aperture:
Grating options:
Order-sorting filters:
Fiber optic connector:
SPECTROSCOPIC
Wavelength range:
Optical resolution:
Signal-to-noise ratio:
Dark noise:
Dynamic range:
Integration time:
ELECTRONICS
Power consumption:
Data transfer speed:
Inputs/Outputs:
Analog channels:
COMPUTER
Operating systems:
148.6 mm x 104.8 mm x 45.1 mm
570 g
Toshiba TCD1304AP linear CCD array (page 24)
200-1100 nm
3648 pixels, pixel size of 8 µm x 200 µm
~100,000 electrons
130 photons/count at 400 nm; 60 photons/count at 600 nm
f/4, Symmetrical crossed Czerny-Turner
101.6 mm input, 101.6 mm output
5, 10, 25, 50, 100 or 200 µm wide slits (page 22) or fiber
14 gratings, UV through Shortwave NIR (page 23)
longpass OF-1 filters and OFLV-200-1100 (page 24)
SMA 905 to 0.22 numerical aperture single-strand fiber
Grating dependent
~0.02-8.4 nm FWHM
300:1 (at full signal)
12 RMS counts
2 x 108 (system); 1300:1 for a single acquisition
3.8 ms to 10 seconds
450 mA @ 5 VDC
Full spectrum to memory every 4 ms with USB 2.0 port,
18 ms with USB 1.1 port
Yes, 10 onboard digital user-programmable GPIOs
One 13-bit analog input, One 9-bit analog output
Windows 98/Me/2000/XP, Mac OS X and Linux with
USB port; any 32-bit Windows OS using serial port*
Computer interfaces: USB 2.0 @ 480 Mbps; RS-232 (2-wire) @ 115.2 K baud
Peripheral interfaces: SPI (3-Wire), I2C inter-integrated circuit
* You cannot use SpectraSuite if you’re interfacing an HR4000 to a PC via
RS-232. A Command Set is included for writing your own software.
21
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Options for the “HR” Optical Bench
Below is a diagram of the “HR” Optical Bench used in HR2000+ and HR4000 High-resolution Spectrometers. It
shows how light moves through the symmetrical crossed Czerny-Turner design of the bench. All components in
the bench are fixed in place during manufacturing. Not only do you have detector choices with the “HR” bench,
you also have a whole host of other options when configuring your High-resolution Spectrometer. You can choose
various entrance aperture sizes, detector accessories, filters, gratings and more to optimize your spectrometer.
Components of the “HR” Optical Bench
4 Collimating Mirror: specify standard or SAG+
The collimating mirror is matched to the 0.22 numerical aperture of our optical
fiber. Light reflects from this mirror, as a collimated beam, toward the grating.
You can opt to install a standard mirror or a UV absorbing SAG+ mirror.
4
8
7
9
5 Grating & Wavelength Range: specify grating & starting wavelength
We install the grating on a platform that we then rotate to select the starting
wavelength you’ve specified. Then we permanently fix the grating in place to
eliminate mechanical shifts or drift.
10
6
6 Focusing Mirror: specify standard or SAG+
This mirror focuses first-order spectra on the detector plane. Both the
collimating and focusing mirrors are made in-house to guarantee the highest
reflectance and the lowest stray light possible. You can opt for a standard
mirror or SAG+ mirror.
5
3
7 L2 and L4 Detector Collection Lenses: optional
This cylindrical lens, made in-house to ensure aberration-free performance, is
fixed to the detector to focus the light from the tall slit onto the shorter detector
elements. It increases light-collection efficiency.
1
Spectrometers
2
1 SMA 905 Connector
Light from a fiber enters the optical bench through the SMA 905 Connector.
The SMA 905 bulkhead provides a precise locus for the end of the optical fiber,
fixed slit, absorbance filter and fiber clad mode aperture.
8 Detector: specify Sony or Toshiba detector
We offer two detectors for the “HR” Bench; both are linear CCD arrays. Each
pixel responds to the wavelength of light that strikes it. Electronics bring the
complete spectrum to the software.
2 Fixed Entrance Slit: specify slit size
Light passes through the installed slit, which acts as the entrance aperture.
Slits are available in widths from 5 µm to 200 µm. Each is permanently fixed
to the SMA 905 bulkhead. (Without a slit, a fiber acts as the entrance aperture.)
9 OFLV Variable Longpass Order-sorting Filter: optional
Our proprietary filters precisely block second- and third-order light from
reaching specific detector elements.
10 UV2 and UV4 Detector Upgrades: optional
3 Longpass Absorbance Filter: optional
If selected, an absorbance filter is installed between the slit and the clad mode
aperture in the SMA 905 bulkhead. The filter is used to block second- and thirdorder effects or to balance color.
When selected, the detector’s standard BK7 window is replaced with a
quartz window to enhance the performance of the spectrometer for
applications <340 nm.
1 SMA 905 Connector
A precision SMA 905 Connector aligns to the spectrometer’s entrance slit and ensures concentricity of the fiber.
For an upgrade fee that includes the cost of the custom connector and labor, we will replace the standard
SMA 905 Connector with a different connector of your choice. We also offer connector adapters, such as an
SMA-to-ST Adapter and an SMA-to-FC Adapter. Please call for details on connectors and adapters.
2 Fixed Entrance Slit
Another option available with “HR” User-configured Spectrometers is selecting the size of the
entrance aperture. Entrance slits are rectangular apertures, 1-mm tall and various widths from
5 µm to 200 µm, with the width determining the amount of light entering the bench. A slit is
fixed in place. Note that the smallest slit achieves the best optical resolution.
Slit
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22
Description
HR2000+
Pixel Resolution
HR4000
Pixel Resolution
A slit is installed
on the inside
edge of the
bulkhead of an
SMA 905
Connector.
Price
SLIT-5
5-µm wide x 1-mm high
1.5 pixels
2.0 pixels
$150
SLIT-10
10-µm wide x 1-mm high
2.0 pixels
3.7 pixels
$150
SLIT-25
25-µm wide x 1-mm high
2.5 pixels
4.4 pixels
$150
SLIT-50
50-µm wide x 1-mm high
4.2 pixels
7.4 pixels
$150
SLIT-100
100-µm wide x 1-mm high
8.0 pixels
14.0 pixels
$150
SLIT-200
200-µm wide x 1-mm high
15.3 pixels
26.8 pixels
$150
For all your sensing needs, visit OceanOptics.com
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Options for the “HR” Optical Bench
3 Longpass Absorbing Filters
We offer longpass absorbing or blocking filters; each filter
has a transmission band and a blocking band to restrict
radiation to a certain wavelength region for eliminating
second- and third-order effects. These filters are installed
permanently between the slit and the clad mode aperture in
the bulkhead of the SMA 905 Connector.
Item
Description
OF1-WG305
Longpass filter; transmits light >305 nm
Price
$50
OF1-GG375
Longpass filter; transmits light >375 nm
$50
OF1-GG475
Longpass filter; transmits light >475 nm
$50
OF1-OG515
Longpass filter; transmits light >515 nm
$50
OF1-OG550
Longpass filter; transmits light >550 nm
$50
OF1-OG590
Longpass filter; transmits light >590 nm
$50
4 Collimating & Focusing Mirrors
6
5 Choosing a Grating & Wavelength Range
Grating
Number
Intended
Use
Groove
Density
HC1*
UV-NIR
You choose from among 14 gratings
H1
UV
for each spectrometer. With each
H2
UV-VIS
grating, you consider its groove
H3
VIS-Color
density (which helps determine the
H4
NIR
resolution), its spectral range (which
H5
UV-VIS
helps determine the wavelength
H6
NIR
range) and its blaze wavelength
H7
UV-VIS
(which helps determine the most
H9
VIS-NIR
efficient range). Our gratings are
H10
UV-VIS
permanently fixed in place at the
H11
UV-VIS
time of manufacture to ensure longH12
UV-VIS
term performance and stability. We
H13
UV-VIS-NIR
offer ruled and holographic
H14
NIR
diffraction gratings. Both are
polymer replicas of master gratings. There are trade-offs
between these gratings: holographic gratings produce less
stray light while ruled gratings are more reflective, resulting
in higher sensitivity.
Grating Selection Chart
The Groove Density (mm-1) of a grating determines its
dispersion, while the angle of the groove determines the
most efficient region of the spectrum. The greater the
groove density, the better the optical resolution possible,
but the more truncated the spectral range.
The Spectral Range is the dispersion of the grating
across the linear array. The spectral range (bandwidth)
is a function of the groove density and does not
change. When you choose a starting wavelength for a
spectrometer, you add its spectral range to the starting
wavelength to determine the wavelength range.
For ruled gratings, the Blaze Wavelength is the peak
wavelength in an efficiency curve. For holographic
gratings, it is the most efficient wavelength region.
Tel: 727.733.2447 • Email: [email protected]
Spectral
Range
Blaze
Wavelength
Best Efficiency
(>30%)
300
200-1100 nm
variable
200-1100 nm
600
425-445 nm
300 nm
200-575 nm
600
415-445 nm
400 nm
250-800 nm
600
410-440 nm
500 nm
350-850 nm
530-1100 nm
600
410-430 nm
750 nm
1200
205-220 nm
holographic: UV
200-400 nm
1200
140-195 nm
750 nm
500-1100 nm
200-500 nm
2400
72-102 nm
holographic: UV
1200
165-205 nm
holographic: VIS
400-800 nm
1800
95-140 nm
holographic: UV
200-635 nm
1800
75-135 nm
holographic: VIS
320-800 nm
2400
60-100 nm
holographic: VIS
250-575 nm
300
900 nm
500 nm
300-1100 nm
600
410-420 nm
1000 nm
650-1100 nm
Spectrometers
Wide Selection Allows
Flexibility
The Best Efficiency region is the range where efficiency
is >30%. In some cases, gratings have a greater
spectral range than is efficiently diffracted. For example,
Grating #1 has a 650 nm spectral range, but is most
efficient from 200-575 nm. In this case, wavelengths
>575 nm will have lower intensity due to the the
grating’s reduced efficiency.
Grating Efficiency
HC-1Grating Efficiency Curve
Curves for the
60
“HR” bench are
50
the same as those
40
for the USB (see
30
page 18) except
20
for the HC-1
10
Grating; its curve
0
is shown here. All
200 300 400 500 600 700 800 900 1000 1100
WAVELENGTH (nm)
gratings are free
with the purchase
of a spectrometer, except for the HC-1, which is $600.
REFLECTION EFFICIENCY (%)
&
Another bench option is to replace the standard aluminum-coated reflective mirrors with our proprietary,
UV-absorbing SAG+ Mirrors, which increase reflectance in the VIS-NIR and, in turn, increase the sensitivity of
the spectrometer. SAG+ Mirrors are often specified for fluorescence. These mirrors also absorb nearly all UV
light, which reduces the effects of excitation scattering in fluorescence measurements. Unlike most silver-coated
mirrors, the SAG+ mirrors won't oxidize. See page 16 for a spectral graph illustrating SAG+ reflectivity.
SAG+UPG-HR: $250
23
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Options for the “HR” Optical Bench
7 L2 or L4 Detector Collection Lens
The cylindrical L2 and L4 Detector Collection Lenses -- made in-house to ensure
aberration-free performance -- are fixed to a detector’s window to focus the light from the
tall slit onto the shorter detector elements. They increase light-collection efficiency and
reduce stray light. They are also useful with a large-diameter fiber for low light-level
applications. Use the L2 with the Sony detector and the L4 with the Toshiba detector.
L2 or L4 Detector Collection Lens: $150
8 Detector: 2048-element or 3648-element Linear CCD Array
The HR2000+ utilizes the Sony ILX511 linear silicon CCD
array detector. Our next-generation HR4000 High-resolution
Spectrometer utilizes the Toshiba TCD1304AP linear CCD
array detector, which has some electronic advances over the
Sony, such as a user-programmable microcontroller. Both
are linear silicon CCD arrays, with an effective range of
200-1100 nm, and with the same dynamic range (1300:1).
4000
Sony 2048-element ILX511 Detector
INTENSITY (COUNTS)
Toshiba 3648-element TCD1304AP Detector
3000
2000
Spectrometers
1000
There are some differences between the detectors. For
example, the Toshiba detector achieves better optical
0
resolution (see the facing page for details). Also, since the
200
300
400
500
600
700
STARTING WAVELENGTH (nm)
Toshiba’s pixels are only 8 µm wide instead of 14 µm wide, the
sensitivity for a Toshiba pixel seems to be ~60% (8 µm/14 µm)
that of a Sony pixel (see graph at right). However, on a per-unit
area basis, the sensitivity is about the same since the Toshiba has 3648 pixels compared with the
Sony’s 2048; the total signal is the same. Because the Toshiba detector has an electronic shutter,
you can almost never have too much light; the shutter prevents the detector from saturating,
making possible analysis of transient events such as laser pulses.
800
900
Specifications
Detector range:
Pixels:
Pixel size:
Pixel well depth:
Maximum pixel rate:
9
10
Toshiba TCD1304AP linear CCD array
200-1100 nm
3648 pixels
8 µm x 200 µm
~100,000 electrons
Rate at which pixels are digitized is 1 MHz
Our OFLV Variable Longpass Order-sorting Filters are applied to the detector’s window to
eliminate second- and third-order effects. We use patented coating technology to apply the
filter onto the substrate. In fact, we are the only miniature spectrometer manufacturer to
offer “clean” first-order spectra.
2048-element
Sony Detector
3648-element
Toshiba Detector
with L4 Collection
Lens
Detector with UV2 or UV4 Detector Window Upgrade
When you specify a detector with a UV2 or UV4 Detector Window Upgrade, we replace
the detector’s standard BK7 window with a quartz window to enhance the spectrometer‘s
performance from 200-340 nm.
Item
Description
DET4-VIS
Toshiba TCD1304AP Detector installed into a HR4000 User-Configured Spectrometer;
best for systems with wavelength ranges above 400 nm
Toshiba TCD1304AP Detector with UV4 Detector Window Upgrade installed into a HR4000
User Configured Spectrometer; best for systems with wavelength ranges in the UV
Toshiba TCD1304AP Detector with OFLV-200-1100 Variable Longpass Order-sorting Filter
and UV4 Detector Window Upgrade installed into a HR4000 User-configured Spectrometer;
used with HC1 Grating ($600)
Sony ILX511 Detector installed into an HR2000+ User-Configured Spectrometer; best for
systems with wavelength ranges above 400 nm
Sony ILX511 Detector with UV2 Detector Window Upgrade installed into an HR2000+
User-Configured Spectrometer; best for systems with wavelength ranges in the UV
DET4-200-1100
DET2-VIS
DET2-UV
24
Sony ILX511 linear silicon CCD array
200-1100 nm
2048 pixels
14 µm x 200 µm
~62,500 electrons
Rate at which pixels are digitized is 2 MHz
Detector with OFLV Filter:
DET4-UV
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Detector Sensitivity Comparison
3648-element
Toshiba Detector
Spectrometer
Price
HR4000
Free
HR4000
$150
HR4000
$400
HR2000+
Free
HR2000+
$150
For all your sensing needs, visit OceanOptics.com
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Options for the “HR” Optical Bench
Predicted Ranges & Resolution
These graphs demonstrate the range and resolution of your “HR” Bench Spectrometer with a 5 µm slit. See our
website for additional graphs of ranges and resolutions for every slit size.
“HR” Bench with Sony Detector:
HR2000+
425
0.31
420
415
410
0.30
405
400
200
400
600
800
0.293
1000
440
430
0.235
425
420
0.230
415
405
400
200
180
0.13
170
0.12
160
0.11
150
0.10
1000
Example:
If the starting
wavelength is
600 nm, then
the range is
~188 nm,
providing a
600-788 nm
wavelength
range and
0.137 nm
resolution.
SPECTRAL RANGE (nm)
0.14
190
RESOLUTION (nm)
SPECTRAL RANGE (nm)
0.15
200
0.120
210
0.115
200
0.110
0.105
190
0.100
180
0.095
170
0.090
160
0.085
150
0.080
140
200
0.10
130
0.09
120
0.08
110
100
0.07
RESOLUTION (nm)
SPECTRAL RANGE (nm)
140
90
0.06
80
0.05
1000
Example:
If the starting
wavelength is
700 nm, then
the range is
~90 nm,
providing a
700-790 nm
wavelength
range and
0.065 nm
resolution.
0.080
130
0.070
120
0.060
110
100
0.050
90
80
70
200
0.05
0.04
50
0.03
400
600
800
0.02
1000
Example:
If the starting
wavelength is
600 nm, then
the range is
~56 nm,
providing a
600-656 nm
wavelength
range and
0.039 nm
resolution.
600
800
0.040
1000
STARTING WAVELENGTH (nm)
Tel: 727.733.2447 • Email: [email protected]
110
0.055
100
SPECTRAL RANGE (nm)
0.06
RESOLUTION (nm)
SPECTRAL RANGE (nm)
0.07
80
30
200
400
2400 mm-1 Grating and 5 µm Slit
90
40
0.075
1000
140
2400 mm-1 Grating and 5 µm Slit
60
800
STARTING WAVELENGTH (nm)
110
70
600
1800 mm-1 Grating and 5 µm Slit
STARTING WAVELENGTH (nm)
100
400
150
SPECTRAL RANGE (nm)
1800 mm-1 Grating and 5 µm Slit
800
0.220
1000
STARTING WAVELENGTH (nm)
150
600
800
220
STARTING WAVELENGTH (nm)
400
600
Spectrometers
210
70
200
400
1200 mm-1 Grating and 5 µm Slit
0.16
800
Example:
If the starting
wavelength is
600 nm, then
the range is
~56 nm,
providing a
600-656 nm
wavelength
range and
0.029 nm
resolution.
0.225
410
1200 mm-1 Grating and 5 µm Slit
600
Example:
If the starting
wavelength is
700 nm, then
the range is
~90 nm,
providing a
700-790 nm
wavelength
range and
0.05 nm
resolution.
0.240
435
STARTING WAVELENGTH (nm)
220
400
Example:
If the starting
wavelength is
300 nm, then
the range is
~215 nm,
providing a
300-515 nm
wavelength
range and
0.117 nm
resolution.
0.245
445
STARTING WAVELENGTH (nm)
140
200
RESOLUTION (nm)
430
Example:
If the starting
wavelength is
400 nm, then
the range is
~437 nm,
providing a
400-837 nm
wavelength
range and
0.239 nm
resolution.
RESOLUTION (nm)
0.32
435
600 mm-1 Grating and 5 µm Slit
450
RESOLUTION (nm)
440
RESOLUTION (nm)
SPECTRAL RANGE (nm)
445
Example:
If the starting
wavelength is
400 nm, then
the range is
~437 nm,
providing a
400-837 nm
wavelength
range and
0.32 nm
resolution.
RESOLUTION (nm)
0.33
SPECTRAL RANGE (nm)
600 mm-1 Grating and 5 µm Slit
450
“HR” Bench with Toshiba Detector:
HR4000
90
0.045
80
70
0.035
60
50
0.025
40
30
200
400
600
800
0.015
1000
STARTING WAVELENGTH (nm)
25
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QE65000 Scientific-grade Spectrometer
New Scientific-grade Spectrometer
The QE65000 Spectrometer is a unique combination of
detector and optical bench technologies that provides users
with high spectral response and high optical resolution in one
scientific-grade spectrometer package.
Quantum Efficiency to 90%
The Hamamatsu FFT-CCD detector used in the QE65000
provides 90% quantum efficiency (defined as how efficiently a
photon is converted to a photo-electron). Most of our other
detectors are linear CCDs but with this “2D” area detector,
we can bin a vertical row of pixels, which offers significant
improvement in the signal-to-noise ratio and signal
processing speed of the detector compared with a linear
CCD, where signals are digitally added by an external circuit.
Specifications
PHYSICAL
Dimensions (in mm):
Weight:
DETECTOR
Detector:
Detector range:
Pixels:
Pixel well depth:
Sensitivity:
OPTICAL BENCH
Design:
Focal length:
Entrance aperture:
Grating options:
Fiber optic connector:
SPECTROSCOPIC
Wavelength range:
Optical resolution:
Signal-to-noise ratio:
Dark noise:
Dynamic range:
Integration time:
Stray light:
ELECTRONICS
Power consumption:
182 x 110 x 47
1.18 kg (without power supply)
Hamamatsu S7031-1006 back-thinned FFT-CCD
200-1100 nm
1024 x 58 (1044 x 64 total); 24.6 µm square size
300,000 electrons/well ~1.5 mill. electrons/column
400 nm: 22 electrons/count, 250 nm: 26 photons/count
f/4, Symmetrical crossed Czerny-Turner
101.6 mm input, 101.6 mm output
5, 10, 25, 50, 100, or 200 µm wide slits (page 27)
14 gratings, UV through Shortwave NIR (page 28)
SMA 905 to 0.22 numerical aperture single-strand fiber
Grating dependent
~0.14-7.7 nm FWHM
1000:1 (at full signal)
2.5 RMS counts
25000:1 a single acquisition; 7.5 x 109 (system)
8 milliseconds to 15 minutes
<0.08% at 600 nm, <0.4% at 435 nm
500 mA @ 5 VDC no TE cool;
3 A @ 5 VDC with TE cool
Data transfer speed: Full spectrum to memory every 4 ms with USB 2.0
port, 8 ms with USB 1.1 port
Inputs/Outputs:
10 onboard digital user-programmable GPIOs
TEMPERATURE & THERMOELECTRIC (TE) COOLING
Temperature limits:
0 °C to 50 °C for spectrometer, no condensation
Temperature range:
13 °C maximum range between the high and low
Set point:
Software controlled
Lowest set point:
40 °C below ambient, to -15 °C
Stability:
±0.1 °C of set temperature in <2 minutes
COMPUTER
Operating systems:
Windows 98/Me/2000/XP, Mac OS X and Linux when
using the USB port; 32-bit Windows OS when using
the serial port
Computer interfaces: USB 2.0 @ 480 Mbps; RS-232 (2-wire) @ 115K baud
Peripheral interfaces: SPI (3-wire); I2C inter-integrated circuit
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Increased System Sensitivity
In our spectrometers with linear CCDs, the slit’s width, not its
height, regulates the amount of light entering the bench
because linear CCDs cannot efficiently collect the light from
the entire height of the slit. But in the QE65000, the 2D area
detector can better take advantage of the height of the slit
and the additional light, greatly improving system sensitivity.
Back-thinned: Great for the UV
Because the detector in the QE65000 is back-thinned (or
back-illuminated), it has great native response in the UV and
does not require the additional coatings that we typically
apply to other detectors for UV applications.
Demanding Low Light-level Applications
The QE65000 Spectrometer is a great option for low-light
level applications such as fluorescence, Raman spectroscopy,
DNA sequencing, astronomy and thin-film reflectivity. The TEcooled (down to -15 °C) detector features low noise and low
dark signal, which enables low-light-level detection and long
integration times from 8 milliseconds to 15 minutes.
Onboard Programming
The QE65000 also has an onboard programmable microcontroller for controlling the spectrometer and accessories.
You have access to 10 user-programmable digital inputs/
outputs and a pulse generator for triggering other devices.
QE65000: $9,999
Comparing Xylenes
40000
Mixed Xylene
35000
O-Xylene
30000
INTENSITY
Spectrometers
An example of a fluorescence setup
with a QE65000 uses the PX-2
Pulsed Xenon Lamp as an
excitation source and the
CUV-ALL Cuvette
Holder for samples. An
optical fiber delivers
excitation light to the
sample holder and
read light to the
spectrometer. A filter,
such as one of our LVFs,
would block excitation light from
entering the spectrometer
25000
20000
15000
10000
5000
0
0
500
1000
1500
2000
2500
3000
3500
4000
RAMAN SHIFT (cm-1)
To acquire Raman spectra for xylene, we used a QE65000 with a
10 µm slit and Grating H14, plus a 532 nm laser and probe.
For all your sensing needs, visit OceanOptics.com
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Options for the “QE” Optical Bench
Components of the “QE” Optical Bench
3 Longpass Absorbing Filter: optional
If selected, an OF-1 absorbance filter is installed between the slit and
the clad mode aperture in the SMA 905 bulkhead. The filter is used to
block second- and third-order effects.
4 Collimating Mirror: specify standard or SAG+
7
4
8
The collimating mirror is matched to the 0.22 numerical aperture of our
optical fiber. Light reflects from this mirror, as a collimated beam, toward
the grating. Opt to install a standard mirror or a SAG+UPG-HR mirror.
5 Grating: specify grating
We install the grating on a platform that we then rotate to select the
starting wavelength you’ve specified. Then we permanently fix the
grating in place to eliminate mechanical shifts or drift.
6
5
6 Focusing Mirror: specify standard or SAG+
3
1
This mirror focuses first-order spectra on the detector plane and sends
higher orders to light traps built into the optical bench. Both the
collimating and focusing mirrors are made in-house to guarantee the
highest reflectance and the lowest stray light possible. Opt for a
standard mirror or a UV-absorbing SAG+UPG-HR mirror.
2
7 Detector with TE cooling
1 SMA 905 Connector
Light from a fiber enters the optical bench through the SMA 905 Connector.
The SMA 905 bulkhead provides a precise locus for the end of the optical fiber,
fixed slit, absorbance filter and fiber clad mode aperture.
The TE-cooled, back-thinned, “2D” detector provides great signal
processing speed, improved signal-to-noise ratio and great native
response in the UV. It generates virtually no dark noise, allowing for
long integration times.
2 Fixed Entrance Slit: specify slit size
8 OFLV Filters: optional
Our proprietary filters precisely block second- and third-order light from
reaching specific detector elements.
1 SMA 905 Connector
A precision SMA 905 Connector aligns to the spectrometer’s entrance slit and ensures concentricity of
the fiber. For an upgrade fee that includes the cost of a another connector and labor, we will replace
the standard SMA 905 Connector with a different connector of your choice.
2
3
4
&
6
Fixed Entrance Slit
One option available with the user-configured
QE65000 Spectrometer is the size of the entrance
aperture, with the width determining the amount of
light entering the bench. A slit is fixed in place; it
only can be changed by our technicians.
Slit
Description
Pixel Resolution
SLIT-5
5-µm wide x 1-mm high
~2.0 pixels
$150
SLIT-10
10-µm wide x 1-mm high
~2.2 pixels
$150
SLIT-25
25-µm wide x 1-mm high
~2.6 pixels
$150
SLIT-50
50-µm wide x 1-mm high
~3.3 pixels
$150
SLIT-100
100-µm wide x 1-mm high
~4.7 pixels
$150
SLIT-200
200-µm wide x 1-mm high
~8.9 pixels
$150
Longpass Absorbing Filters
We offer longpass absorbing or blocking filters; each filter
has a transmission band and a blocking band to restrict
radiation to a certain wavelength region for eliminating
second- and third-order effects. These filters are installed
permanently between the slit and the clad mode aperture in
the bulkhead of the SMA 905 Connector.
Price
Item
Description
OF1-WG305
Longpass filter; transmits light >305 nm
$50
OF1-GG375
Longpass filter; transmits light >375 nm
$50
OF1-GG475
Longpass filter; transmits light >475 nm
$50
OF1-OG515
Longpass filter; transmits light >515 nm
$50
OF1-OG550
Longpass filter; transmits light >550 nm
$50
OF1-OG590
Longpass filter; transmits light >590 nm
$50
Spectrometers
Light passes through the installed slit, which acts as the entrance aperture.
Slits are available in widths from 5 µm to 200 µm. Each is permanently fixed
to the SMA 905 bulkhead. (Without a slit, a fiber acts as the entrance aperture.)
Price
Collimating & Focusing Mirrors
Another bench option is to replace the standard aluminum-coated reflective mirrors with our proprietary, UVabsorbing SAG+ Mirrors, which increase reflectance in the VIS-NIR and, in turn, increase the sensitivity of the
spectrometer. SAG+ Mirrors are often specified for fluorescence. These mirrors also absorb nearly all UV light,
which reduces the effects of excitation scattering in fluorescence measurements. Unlike most silver-coated
mirrors, the SAG+ mirrors won't oxidize. See page 16 for a spectral graph illustrating SAG+ reflectivity.
SAG+UPG-HR: $250
Tel: 727.733.2447 • Email: [email protected]
27
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Options for the “QE” Optical Bench
Spectrometers
5 Choosing a Grating & Wavelength Range
You choose from among 14 gratings for each spectrometer.
With each grating, you consider its groove density (which
helps determine the resolution), its spectral range (which
helps determine the wavelength range) and its blaze wavelength (which helps determine the most efficient range).
The Groove Density (mm-1) of a grating determines its
dispersion, while the angle of the groove determines the
most efficient region of the spectrum. The greater the
groove density, the better the optical resolution possible,
but the more truncated the spectral range.
The Spectral Range is the
Grating
Intended
dispersion of the grating across
Number
Use
the linear array. The spectral
HC1-QE
UV-NIR
range (bandwidth) is a function
H1
UV
H2
UV-VIS
of the groove density and does
H3
VIS-Color
not change. When you choose a
H4
NIR
starting wavelength for a
H5
UV-VIS
spectrometer, you add its
H6
NIR
spectral range to the starting
H7
UV-VIS
wavelength to determine the
H9
VIS-NIR
wavelength range.
H10
UV-VIS
For ruled gratings, the Blaze
H11
UV-VIS
Wavelength is the peak waveH12
UV-VIS
length in an efficiency curve. For
H13
UV-VIS-NIR
holographic gratings, it is the
H14
NIR
most efficient wavelength region.
The Best Efficiency region is the range where efficiency
is >30%. In some cases, gratings have a greater
spectral range than is efficiently diffracted. For example,
Grating #1 has a 650 nm spectral range, but is most
efficient from 200-575 nm so wavelengths >575 nm
will have lower intensity.
Grating Efficiency Curves are on the next page. (The HC-1
curve is on page 23.) All gratings are free with the purchase
of a spectrometer, except for the HC1-QE, which is $600.
Groove
Density
Spectral
Range
Blaze
Wavelength
Best Efficiency
(>30%)
300
200-950 nm
variable
200-950 nm
600
373-390 nm
300 nm
200-575 nm
600
365-390 nm
400 nm
250-800 nm
600
360-386 nm
500 nm
350-850 nm
530-1100 nm
600
360-377 nm
750 nm
1200
180-193 nm
holographic: UV
200-400 nm
1200
123-170 nm
750 nm
500-1100 nm
2400
63-90 nm
holographic: UV
200-500 nm
1200
145-180 nm
holographic: VIS
400-800 nm
1800
83-123 nm
holographic: UV
200-635 nm
1800
66-120 nm
holographic: VIS
320-800 nm
2400
52-88 nm
holographic: VIS
250-575 nm
300
790 nm
500 nm
300-1100 nm
600
360-370 nm
1000 nm
650-1100 nm
7 Back-thinned Area Detector
The QE65000’s Hamamatsu S7031-1006 FFT-CCD area detector provides 90%
quantum efficiency (defined as how efficiently a photon is converted to a
photoelectron). The TE-cooled detector features low noise and low dark signal,
which enables low-light-level detection and long integration times, thus achieving
a wide dynamic range.
Detector Quantum Efficiency
In our spectrometers with linear CCDs, the slit’s width, not its height,
regulates the amount of light entering the bench because linear
CCDs cannot efficiently collect the light from the entire height of the
slit. But in the QE65000, the 2D area detector can better take
advantage of the height of the entrance slit and the additional light,
greatly improving system sensitivity.
100
QUANTUM EFFICIENCY%
The S7031 is a 2D array, which allows us to bin pixels in a vertical
column to acquire light from the entire height of the spectrometer’s
slit image. This improves light collection and signal-to-noise significantly. Because the detector is back-thinned (or back-illuminated), it
has great native response in the UV and does not require the UV
detector upgrade that we apply to other detectors.
Hamamatsu
S7031-1006
Typical linear CCD
80
Typical linear CCD
with UV Coating
60
40
20
0
200
400
600
800
1000
1200
WAVELENGTH (nm)
Detector Specifications
8
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Detector with OFLV Filter
The OFLV-QE is one of our Variable Longpass Order-sorting Filters
used to eliminate second-order effects and is used with an HC-1
Grating in a 200-950 nm wavelength range system in a QE65000.
We use patented coating technology to apply the filter onto the
substrate of the detector’s window.
OFLV-QE: $250
Detector:
Detector range:
Pixels:
Pixel area:
Pixel well depth:
Sensitivity:
Dark current:
Hamamatsu S7031-1006 area CCD
200-1100 nm
1024 x 58 (1044 x 64 total); 24.6 µm square size
active area: 24.576 mm x 1.392 mm
300,000 electrons/well;
~1.5 million electrons/column sum well
400 nm: 22 electrons/count;
250 nm: 26 photons/count
4000 e-/pixel/sec @ 25 °C; 200 e-/pixel/sec @ 0 °C
For all your sensing needs, visit OceanOptics.com
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Options for the “QE” Optical Bench
Grating Efficiency Curves
Predicted Ranges & Resolution
Below are the Grating Efficiency Curves for gratings with
groove densities of 600, 1200, 1800 and 2400 mm-1.
See curves for all of our gratings at our website.
These graphs demonstrate the range and resolution of your
“QE” Bench Spectrometer with a 5 µm slit. See our website
for more graphs of ranges and resolutions for every slit size.
RESOLUTION (nm)
RESOLUTION (nm)
Example:
If the starting
wavelength is
600 nm, then
the range is
~152 nm,
providing a
600-752 nm
wavelength
range and
0.295 nm
resolution.
RESOLUTION (nm)
Example:
If the starting
wavelength is
300 nm, then
the range is
~112 nm,
providing a
300-412 nm
wavelength
range and
0.226 nm
resolution.
Example:
If the starting
wavelength is
450 nm, then
the range is
~62 nm,
providing a
450-512 nm
wavelength
range and
0.139 nm
resolution.
380
0.67
375
#1
60
#2
50
#3
#4
40
#14
30
20
200
400
600
800
1000
SPECTRAL RANGE (nm)
70
RELATIVE EFFICIENCY
Example:
If the starting
wavelength is
400 nm, then
the range is
~364 nm,
providing a
400-764 nm
wavelength
range and
0.645 nm
resolution.
RESOLUTION (nm)
600 mm-1 Grating and 5 µm Slit
Gratings with Groove Density of 600
80
0.66
370
0.65
365
0.64
360
0.63
355
350
0.62
345
0.61
340
0.60
335
200
1200
WAVELENGTH (nm)
400
600
800
0.59
1000
STARTING WAVELENGTH (nm)
Efficiency Curves for Gratings 1, 2, 3, 4 and 14.
Gratings with Groove Density of 1200
1200 mm-1 Grating and 5 µm Slit
80
180
70
#5
#6
50
#9
40
30
SPECTRAL RANGE (nm)
0.31
60
170
0.30
160
150
0.29
140
0.28
130
120
0.27
110
20
200
400
600
800
1000
100
200
1200
WAVELENGTH (nm)
400
600
800
0.26
1000
Spectrometers
RELATIVE EFFICIENCY
0.32
190
STARTING WAVELENGTH (nm)
Efficiency Curves for Gratings 5, 6 and 9.
1800 mm-1 Grating and 5 µm Slit
Gratings with Groove Density of 1800
80
120
110
60
#10
#11
50
40
30
SPECTRAL RANGE (nm)
RELATIVE EFFICIENCY
70
0.23
0.22
100
90
0.21
80
70
0.20
60
20
200
400
600
800
1000
50
200
1200
WAVELENGTH (nm)
400
600
800
0.19
1000
STARTING WAVELENGTH (nm)
Efficiency Curves for Gratings 10 and 11.
2400 mm-1 Grating and 5 µm Slit
Gratings with Groove Density of 2400
80
85
0.15
75
60
#7
#12
50
40
30
20
200
400
600
800
1000
1200
WAVELENGTH (nm)
SPECTRAL RANGE (nm)
RELATIVE EFFICIENCY
70
0.145
65
0.14
55
0.135
45
0.13
35
25
200
0.125
400
600
800
0.12
1000
STARTING WAVELENGTH (nm)
Efficiency Curves for Gratings 7 and 12.
Tel: 727.733.2447 • Email: [email protected]
29
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NIR-series Near-infrared Spectrometers
3 Wavelength-Range Options
Our NIR-series Near-infrared Spectrometers provide
full spectral analysis in real time and meet a wide
variety of measurement needs. Three different NIR
systems provide you with multiple wavelength ranges
for measuring sugar, alcohol, moisture, fats and
more. These small-footprint, plug-and-play systems
provide a full spectrum in one millisecond, and offer
optical resolution as low as 3.0 nm FWHM.
InGaAs Detector Cooled for Optimum
Signal-to-Noise and Sensitivity
The NIR-series Spectrometers each feature a
Hamamatsu InGaAs linear-array detector with
onboard thermoelectric cooling. A thermistor monitors
the array's temperature and a thermoelectric device
can cool each array to 30 °C below ambient, keeping
the array stable to within ±0.1 °C. You can set and
monitor the detector's temperature via software.
Specifications NIR-512
PHYSICAL
Dimensions (in mm):
Weight:
DETECTOR
Detector:
Detector range:
Pixels:
Pixel size:
Pixel well depth:
Defective pixels:
OPTICAL BENCH
Focal length:
Entrance aperture:
Grating options:
Fiber optic connector:
SPECTROSCOPIC
Wavelength range:
153.4 x 105.2 x 76.2
190 grams
153.4 x 105.2 x 76.2
190 grams
153.4 x 105.2 x 76.2
190 grams
Hamamatsu
G9204-512 InGaAs
linear array
850-1700 nm
512
25 µm x 500 µm
187,000,000 electrons
None
Hamamatsu
G9206-256 InGaAs
linear array
900-2100 nm
256
50 µm x 250 µm
187,000,000 electrons
2%
Hamamatsu
G9208-256 InGaAs
linear array
900-2550 nm
256
50 µm x 250 µm
187,000,000 electrons
5%
f/4, 40 mm
10, 25, 50, 100 or
200 µm wide slits
or fiber
Grating N1
SMA 905 to 0.22
numerical aperture
single strand fiber
f/4, 40 mm
10, 25, 50, 100 or
200 µm wide slits
or fiber
Grating N1 and N2
SMA 905 to 0.22
numerical aperture
single strand fiber
f/4, 40 mm
10, 25, 50, 100 or
200 µm wide slits
or fiber
Grating N2
SMA 905 to 0.22
numerical aperture
single strand fiber
900-1700 nm with
Grating N1
900-2100 nm with
Grating N2;
1200-2100 nm
with Grating N1
1.95 µm
With grating N1,
4.5-14.0 nm FWHM,
slit dependent;
with grating N2,
7.5-25.0 nm FWHM,
slit dependent
4000:1
16 bit
12 RMS counts
5 x 106 (system);
5000:1 for a
single acquisition
1 ms to 1 second*
>99.8%
120 pA @ -15 °C
900-2500 nm with
Grating N2
NIR512 Spectrometer: 900-1700 nm
Spectrometers
The NIR-512 Spectrometer features a 512-element
InGaAs linear-array detector. With the NIR-512, the
only diffractive grating available is Grating N1, and it
provides a 900-1700 nm wavelength range,
producing an optical resolution of <5.0 nm FWHM.
NIR256-2.1 Spectrometer: 1200-2100 nm
or 900-2100 nm
The NIR256-2.1 Spectrometer uses a 256-element
InGaAs linear-array detector. With the NIR256 you
have two grating options. With Grating N1, you have
a 1200-2100 nm wavelength range. Grating N2
provides a 900-2100 nm wavelength range.
NIR256-2.5 Spectrometer: 900-2500 nm
The NIR256-2.5 Spectrometer extends farther into the
NIR, acquiring real-time spectra up to 2.5 µm. With
the NIR256-2.5, you select Grating N2, which
provides a wavelength range of 900-2500 nm.
Responsivity peak:
Optical resolution:
Signal-to-noise ratio:
A/D resolution:
Dark noise:
Dynamic range:
Integration time:
Corrected linearity:
Max. dark current:
ELECTRONICS
Power consumption:
Data transfer speed:
Trigger modes:
Strobe functions:
COMPUTER
Operating systems:
Plug-and-Play USB Operation
All of the NIR-series Spectrometers interface to PCs
via USB 2.0. When operating the spectrometer via the
USB port, you have access to the spectrometer’s
EEPROM, where wavelength calibration coefficients
and other data unique to your spectrometer are
stored. SpectraSuite Spectroscopy Operating Software
reads these values for easy setup and swapping
among PCs. A 16-bit A/D converter is mounted with
the spectrometer in the same housing. A 5 VDC wall
transformer (included) is required. These systems also
have a serial port for interfacing to PCs, PLCs and
other devices that support the RS-232 protocol.
NIR-512:
$14,995
NIR256-2.1: $19,999
NIR256-2.5: $21,995
SpectraSuite:
$199
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Computer interfaces:
Peripheral interfaces:
NIR256-2.1 NIR256-2.5
1.6 µm
With grating N1,
4.2-14.0 nm FWHM,
slit dependent
4000:1
16 bit
12 RMS counts
5 x 106 (system);
5000:1 for a
single acquisition
1 ms to 3 seconds*
>99.8%
60 pA @ 20 °C
2.3 µm
With grating N2
7.5-25.0 nm FWHM,
slit dependent
4000:1
16 bit
12 RMS counts
5 x 106 (system);
4000:1 for a
single acquisition
1 to 30 milliseconds*
>99.8%
2000 pA @ 15 °C
2 A @ 5 VDC
3 A @ 5 VDC
2 A @ 5 VDC
Full spectrum to
Full spectrum to
Full spectrum to
memory every 10 ms memory every 10 ms memory every 10 ms
with USB port
with USB port
with USB port
3 modes
3 modes
3 modes
Yes
Yes
Yes
Windows 98/Me/
2000/XP, Mac OS X
& Linux with USB
port; Any 32-bit
Windows OS
with serial port
USB 2.0 @ 480
Mbps; RS-232
(2-wire) @
115.2 K baud
I2C inter-integrated
circuit; SPI (3-wire)
Windows 98/Me/
2000/XP, Mac OS X
& Linux with USB
port; Any 32-bit
Windows OS
with serial port
USB 2.0 @ 480
Mbps; RS-232
(2-wire) @
115.2 K baud
I2C inter-integrated
circuit; SPI (3-wire)
Windows 98/Me/
2000/XP, Mac OS X
& Linux with USB
port; Any 32-bit
Windows OS
with serial port
USB 2.0 @ 480
Mbps; RS-232
(2-wire) @
115.2 K baud
I2C inter-integrated
circuit; SPI (3-wire)
* Hardware allows integration times up to 32 seconds, but the detectors’ dark
characteristics do not support it.
For all your sensing needs, visit OceanOptics.com
NIR-series Near-infrared Spectrometers
NIR-512 Resolution & Intensity
vs. Slit Size
60
16
Resolution
Intensity
50
12
40
10
30
8
6
20
4
RELATIVE INTENSITY
RESOLUTION IN NM (FWHM)
14
10
2
0
200
0
0
50
100
150
SLIT SIZE (microns)
Use this
chart to help
determine
the best
entrance
aperture slit
size for your
application.
Note that
the smallersized slits
provide
excellent
resolution,
but lower
levels of
throughput
to the
detector.
NIR-series Applications
NIR-512: Silicon Wafer Reflectivity
102
100
Sugar analysis
Alcohol analysis in brewing
Moisture analysis
Nitrogen detection in soils
Pulpwood QC
Analysis of lubricants
Laser characterization
Fat, oil and lipid
determination
Spectrometers
NORMALIZED REFLECTIVITY
104
98
96
1000
1100
1200
1300
1400
1500
1600
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1700
WAVELENGTH (nm)
NIR256-2.1 Reflectance of Sugar
100%
REFLECTIVITY
80%
60%
Sugar
40%
Saccharin
20%
0
1250
1300
1450
1550
1650
1750
1850
1950
WAVELENGTH (nm)
NIR256-2.5 Heptane Absorbance
0.3
ABSORBANCE UNITS
0.25
0.2
0.15
0.1
0.05
0
900
1100
1300
1500
1700
1900
2100
2300
2500
WAVELENGTH (nm)
Tel: 727.733.2447 • Email: [email protected]
31
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Options for the “NIR” Optical Bench
Detectors
Spectral Response Curves
In the “NIR” Spectrometers, we offer three different InGaAs linear array
detectors, one 512-element array and two 256-element arrays. The
Hamamatsu detectors used in the “NIR” Optical Bench are InGaAs
photodiode linear arrays with each pixel connected to a charge
amplifier array consists of CMOS transistors. These detectors deliver
high sensitivity and stable operation in the near infrared.
NIR-512
1.4
NIR256-2.1
PHOTO SENSITIVITY (A/W)
NIR256-2.5
The detectors all include onboard thermoelectric cooling. A thermistor
monitors the array's temperature and a thermoelectric device can cool
the arrays to 30 °C below
ambient, keeping the array
stable to within ±0.1 °C. In
addition, you can set and
monitor the detector's
temperature via software.
1.2
1.0
0.8
0.6
0.4
0.2
0
500
1000
1500
2000
2500
3000
WAVELENGTH (nm)
This graph compares the spectral response of the three NIR
detectors at an operating temperature of 25 °C.
Fixed Entrance Slits
A slit is installed
on the inside
edge of the
bulkhead of an
SMA 905
Connector.
Spectrometers
An option available with user-configured “NIR” spectrometers is selecting the size of the entrance
aperture. Entrance slits are rectangular apertures, 1-mm tall and various widths from 10 µm to
200 µm, with the width determining the amount of light entering the optical bench. A slit is fixed
in place; it only can be changed by our technicians. You can opt against having a slit, in which case
the diameter of the fiber connected to the spectrometer determines the size of the entrance aperture.
Slit
Description
NIR-512
Pixel Resolution
NIR256-2.1
Pixel Resolution
NIR256-2.5
Pixel Resolution
Price
SLIT-10
10-µm wide x 1-mm high
~2.4 pixels
~1.2
~1.2
$150
SLIT-25
25-µm wide x 1-mm high
~2.4 pixels
~1.2
~1.2
$150
SLIT-50
50-µm wide x 1-mm high
~2.9 pixels
~1.5
~1.5
$150
SLIT-100
100-µm wide x 1-mm high
~4.4 pixels
~2.2
~2.2
$150
SLIT-200
200-µm wide x 1-mm high
~7.9 pixels
~4.0
~4.0
$150
Grating Selection Chart & Grating Efficiency Graphs
Here are the Grating Selection Chart and the Grating Efficiency Curves for the two gratings
available with the “NIR” optical bench.
Grating
Number
Intended
Use
Groove
Density
Spectral
Range
Blaze
Wavelength
Best Efficiency
N1
NIR-512 or NIR256-2.1
N2
NIR256-2.1 or NIR256-2.5
300
900 nm
1000 nm
700-2100 nm
150
1600 nm
1600 nm
700-2500 nm
100%
100%
80%
80%
60%
40%
20%
0
700
900
1100
1300
WAVELENGTH (nm)
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N2 Grating Efficiency
RELATIVE EFFICIENCY
RELATIVE EFFICIENCY
N1 Grating Efficiency
1500
1700
60%
40%
20%
0
700
900
1100
1300
1500
1700
1900
WAVELENGTH (nm)
For all your sensing needs, visit OceanOptics.com
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Spectrometer
Systems & Setups
Systems and Setups are either turnkey spectrometers
or complete setups necessary for a specific
measurement technique, such as fluorescence, or a
specific application, such as measuring LEDs.
Liquid Absorbance Systems
42
Deep-well Spectrometer for High S:N
43
Flow Injection Analysis System
Fluorescence Measurement Tools
44
PMT for Fluorescence Flow Analysis
45
QE65000 Configured for Fluorescence
46
Fluorescence Spectrometers
47
Gated Spectrometer for Fluorescence
Laser-induced Breakdown Spectroscopy
48
LIBS2500 Spectrometer & Accessories
50
LIBS-ELITE Laser Ablation Sampling System
Spectrometer Systems & Setups
General-purpose Spectrometers
34
UV-VIS & VIS-NIR Spectrometers
35
HR4000CG Spectrometer: UV-NIR
36
CHEM4 Systems for Education
38
Red Tide Spectrometer for Education
39
Xplorer GLX Handheld Datalogger
40
MEMS-based NIR Spectrometers
41
Process-2000 Process Control Systems
Raman Spectroscopy
51
Raman Selection Guide
52
Modular Raman Measurement Tools
54
Raman Systems for Lab & Field
55
Multimodal Multiplex Raman System
Spectroradiometric Systems
56
LED Measurement Tools
57
Spectroradiometric Tools
Metrology Systems
58
NanoCalc Thin-film Analysis System
59
SpecEl Ellipsometer System
59
PlasCalc Plasma Monitoring & Control
60
Transmission of Optics Tools
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UV-VIS & VIS-NIR Spectrometers
Great Versatility
We offer general-purpose UV-VIS and VIS-NIR
spectrometers that are preconfigured -- where all of
the optical bench options are already selected. By
switching out light sources and sampling accessories,
these spectrometers can measure absorbance in
solutions or reflectance of solids.
A typical USB4000-UV-VIS absorbance
setup might include components such
as UV-VIS Optical Fiber Assemblies, a
DH2000 Deuterium Tungsten Halogen
Light Source and a CUV-UV-10
Cuvette Holder.
200-850 nm UV-VIS Preconfigured
Spectrometer
Spectrometer Systems & Setups
The USB4000-UV-VIS utilizes the “USB” (also called
the “S”) Optical Bench. It has a 200-850 nm
wavelength range and comes with a detector
upgrade for working in the UV, a variable longpass
detector filter for second- and third-order rejection,
and a 25-µm slit as the entrance aperture. Optical
resolution is ~1.5 nm (FWHM).
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350-1000 nm VIS-NIR Preconfigured
Spectrometer
The USB4000-VIS-NIR spectrometer also utilizes
the “USB” (also called the “S”) Optical Bench. It
has a 350-1000 nm wavelength range and comes
with a 25-µm entrance slit and a variable
longpass detector filter for second- and third-order
rejection. With this optical bench configuration, the
USB4000-VIS-NIR achieves ~1.5 nm optical
resolution (FWHM).
Accessorize
A reflection
setup with the
USB4000-VIS-NIR
could include these
components: an
R200-VIS-NIR Reflection
Probe, an LS-1 Tungsten
Halogen Light Source and an
RPH-1 Reflection Probe Holder.
To complete your spectrometer system, select from
our comprehensive line of fiber optic accessories -light sources, sensors and probes, sample holders,
flow cells, optical fiber assemblies and more.
USB4000-UV-VIS: $2,649
USB4000-VIS-NIR: $2,499
Specifications
PHYSICAL
Dimensions (in mm):
Weight:
DETECTOR
Detector:
Pixels:
Sensitivity:
OPTICAL BENCH
Design:
Focal length:
Entrance aperture:
Grating:
Order-sorting filters:
Fiber optic connector:
SPECTROSCOPIC
Wavelength range:
Optical resolution:
Signal-to-noise ratio:
Dynamic range:
Integration time:
ELECTRONICS
Power consumption:
Data transfer speed:
Inputs/Outputs:
Operating systems:
34
USB4000-UV-VIS
USB4000-VIS-NIR
89.1 x 63.3 x 34.4
190 grams
89.1 x 63.3 x 34.4
190 grams
Toshiba TCD1304AP linear CCD array (page 17)
3648 pixels, size of each is 8 µm x 200 µm
130 photons/count at 400 nm; 60 photons/count at 600 nm
Toshiba TCD1304AP linear CCD array (page 17)
3648 pixels, size of each is 8 µm x 200 µm
130 photons/count at 400 nm; 60 photons/count at 600 nm
f/4, Asymmetrical crossed Czerny-Turner
42 mm input; 68 mm output
25 µm wide slit (page 15)
Grating #1, 600 lines per mm grating, blazed at 300 nm (page 17)
OFLV-200-850 (page 17)
SMA 905 to 0.22 numerical aperture single-strand fiber
f/4, Asymmetrical crossed Czerny-Turner
42 mm input; 68 mm output
25 µm wide slit (page 15)
Grating #3, 600 lines per mm grating, blazed at 500 nm (page 17)
OFLV-350-1000 (page 17)
SMA 905 to 0.22 numerical aperture single-strand fiber
200-850 nm
~1.5 nm FWHM
300:1 (at full signal)
2 x 108 (system); 1300:1 for a single spectrum
3.8 ms to 10 seconds
350-1000 nm
~1.5 nm FWHM
300:1 (at full signal)
2 x 108 (system); 1300:1 for a single spectrum
3.8 ms to 10 seconds
250 mA @ 5 VDC
Full spectrum to memory every 5 ms with USB 2.0 port
8 onboard digital user-programmable GPIOs
Windows 98/Me/2000/XP, Mac OS X and Linux with
USB port; Any 32-bit Windows OS with serial port
250 mA @ 5 VDC
Full spectrum to memory every 5 ms with USB 2.0 port
8 onboard digital user-programmable GPIOs
Windows 98/Me/2000/XP, Mac OS X and Linux with
USB port; Any 32-bit Windows OS with serial port
For all your sensing needs, visit OceanOptics.com
oo
HR4000CG Spectrometer: UV-NIR
200-1100 nm Range,
0.75 nm Resolution
1800
1600
POWER (µW/cm^2/nm)
The HR4000CG
Composite-grating
Spectrometer utilizes a
proprietary grating and
order-sorting filter to
provide a 200-1100 nm
wavelength range and 0.75 nm
optical resolution (FWHM). The
revolutionary HR4000CG is a
preconfigured HR4000
Spectrometer -- where all of the
optical bench options are
already selected for you.
Sample Spectrum
1400
1200
1000
600
400
200
0
200
300
400
500
600
700
800
900
1000
WAVELENGTH (nm)
Sample Spectrum
700
600
µW/cm^2/nm
500
400
300
200
100
0
200
300
400
500
600
700
800
900
1000
WAVELENGTH (nm)
A solar irradiance spectrum taken with the HR4000CG.
Specifications
Optical Bench
The HR4000CG Spectrometer uses the “HR” Optical Bench,
comes with a 5 µm entrance slit, and has a UV4 Detector
Upgrade to enhance the performance of the spectrometer in
the UV. The HR4000CG is an upgrade from the
HR2000CG. The HR4000CG comes with a 3648-element
linear-array CCD detector that provides better optical
resolution throughout the UV-NIR range.
USB 2.0 Compatibility and New Digital I/Os
The HR4000CG interfaces to a PC via a USB port. Software
reads programmed data unique to each spectrometer for
easy setup. The HR4000CG also offers 10 user-programmable
digital inputs/outputs, 1 analog input and 1 analog output.
HR4000CG-UV-NIR: $4,999
Tel: 727.733.2447 • Email: [email protected]
PHYSICAL
Dimensions:
Weight:
DETECTOR
Detector:
Pixels:
Pixel well depth:
Sensitivity:
OPTICAL BENCH
Design:
Focal length:
Entrance aperture:
Grating:
Order-sorting filters:
Fiber optic connector:
SPECTROSCOPIC
Wavelength range:
Optical resolution:
Signal-to-noise ratio:
Dark noise:
Dynamic range:
Integration time:
ELECTRONICS
Power consumption:
Data transfer speed:
Inputs/Outputs:
Analog channels:
Operating systems:
148.6 mm x 104.8 mm x 45.1 mm
570 g
Toshiba TCD1304AP linear CCD array (page 24)
3648 pixels, pixel size of 8 µm x 200 µm
~100,000 electrons
130 photons/count at 400 nm; 60 photons/count at 600 nm
Spectrometer Systems & Setups
Composite-grating &
Order-sorting Filter
The HR4000CG uses the HC-1 grating, which is a
revolutionary and proprietary variable blazed grating
designed to provide a 200-1100 nm wavelength range.
(Though the spectrometer is configured for 200-1100 nm,
its best efficiency is from 200-1050 nm. See the grating
efficiency curve for the HC-1 on page 23.) In addition to this
new composite grating, the HR4000CG has an
OFLV-200-1100 variable longpass order-sorting filter to
eliminate second- and third-order effects. Both are installed
at the time of manufacture and are fixed in place.
800
An irradiance
spectrum
of the
DH2000
Deuterium
Tungsten
Halogen
Light
Source
taken
with the
HR4000CG.
f/4, Symmetrical crossed Czerny-Turner
101.6 mm input, 101.6 mm output
5 µm wide slit (page 22)
HC-1, 300 lines per mm grating (page 23)
Installed OFLV-200-1100 (page 24)
SMA 905 to 0.22 numerical aperture single-strand fiber
200-1100 nm, best efficiency 200-1050 nm
0.75 nm FWHM
300:1 (at full signal)
12 RMS counts
2 x 108 (system); 1300:1 for a single acquisition
3.8 ms to 10 seconds
450 mA @ 5 VDC
Full spectrum to memory every 4 ms with USB 2.0 port,
18 ms with USB 1.1 port
10 onboard digital user-programmable GPIOs*
One 13-bit analog input, One 9-bit analog output
Windows 98/Me/2000/XP, Mac OS X and Linux with
USB port; any 32-bit Windows OS using serial port
* Programming the GPIOs requires SpectraSuite or OmniDriver. See
pages 80-82 for details.
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CHEM4 Systems for Education
Unique Teaching Tool = More Data, Faster
Our CHEM4-series Spectrophotometers for Education are
small-footprint, PC-based systems designed for
professors, teachers and others who use spectroscopy as
a teaching tool. These fully integrated systems -including spectrometer, light source and cuvette holder -are available at dramatic discounts with the trade-in of
an old lab instrument. Acquire and display real-time
complete spectral data (3648 wavelengths) in <1 second
with our convenient, PC-based systems.
Sampling Optics: Direct-attach or Fiber
Spectrometer Systems & Setups
Each CHEM4 system comes with a fully integrated light
source and cuvette holder that attaches to the
spectrometer, either directly or via fiber, for a smallfootprint system.
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Instructional Materials for Teaching Labs
We’ve begun to develop a rich library of spectroscopy
educational materials for both students and educators. Our
first effort, Introduction to Spectroscopy in the Teaching Lab
Using Ocean Optics Spectrometers, is a handy reference tool
for introducing Ocean Optics to the modern teaching lab.
Included are experiments and sample lab exercises for our
spectrometer and PASCO Scientific’s GLX Explorer dataloggers.
Here’s a sampling of featured exercises:
Absorbance of Light vs. Concentration (Beer’s Law)
Kinetics of Crystal Violet Bleaching
Spectrophotometric Determination of an Equilibrium
Constant
Spectrophotometric pH Determination Using Bromocresol
Green
With so many lab exercises built around use of the old Spec20,
these Ocean Optics spectrometer experiments -- all of which
come from recipients of our educational grants -- are great for
getting started in your new lab setup, or for use with any postdispersive spectrometer.
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Item
Description
Price
EDU-SPEC-BOOK
Print version of Educational Spectroscopy
Handbook
$100
EDU-SPEC-BOOK-S
Print version of Educational Spectroscopy
Handbook; when purchased with a
spectrometer
$75
EDU-SPEC-CD
CD version of Educational Spectroscopy
Handbook in PDF format; includes how-to
video for making basic measurements
$45
EDU-SPEC-CD-S
CD version of Educational Spectroscopy
Handbook in PDF format; includes how-to
video for making basic measurements;
when purchased with a spectrometer
$25
EDU-SPEC-D
Online version, educational spectroscopy
handbook
$20
EDU-SPEC-D-S
Online version, educational spectroscopy
handbook; when purchased with a
spectrometer
Free
Direct Attach: The CHEM4-UV-VIS has a state-of-the-art,
miniature RF-excited deuterium tungsten source. The
CHEM4-VIS-NIR has a direct-attach combination tungsten
and blue LED source. You can separate each
spectrometer from its integrated light source to couple the
spectrometer to any of our fiber optic accessories and
light sources.
Fiber: The CHEM4-UV-FIBER and CHEM4-VIS-FIBER
include a light source and cuvette assembly that attaches
to the spectrometer with an optical fiber. The advantage
of this design is that the light source can be easily
coupled to other fiber optic accessories such as reflection
probes or transmission dip probes. The CHEM4-UV-FIBER
uses a deuterium tungsten source and the
CHEM4-VIS-FIBER comes with a tungsten source.
USB Interface for Easy Startup
All of our CHEM4 systems interface to a PC via USB. All
you need is to install the software and connect the
included USB cable to your PC to be up and running.
Wavelength calibration data are loaded automatically
upon startup, and spectrometer power is supplied
through the USB.
Software for Linux, Macintosh & Windows
All CHEM4 systems come with student-friendly software,
which includes functions for absorbance, transmission,
relative irradiance and kinetics measurements. Our new
SpectraSuite Spectroscopy Operating Software (pages
80-81) works in Linux, Macintosh and Windows
operating systems.
Discount Pricing & Cost Sharing
Any learning institution qualifies for trade-in prices for
CHEM4 systems. Save $1,500 by trading in your old
monochromator or spectrometer. See the facing page for
retail and trade-in prices. Our Innovations in Education
Spectroscopy Grant Program rewards educators and
researchers for utilizing fiber optic spectroscopy in
curricula or in research. See page 8 for more.
For all your sensing needs, visit OceanOptics.com
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CHEM4 Systems for Education
Wavelength
Range*
USB4000-UV-VIS
210-880 nm
CHEM4-UV-VIS
Spectrometer &
A/D Converter
Light Source &
Sample Holder
Optical Fiber
Retail
Price
Trade-in
Price
USB-ISS-UV-VIS
None -- integrated
$3,999
$2,499
integrated
light source and
deuterium tungsten
sample holder
halogen light
directly attaches to
source and cuvette
spectrometer
(save
$1,500)
holder for 1-cm
square cuvettes
370-985 nm
CHEM4-VIS-NIR
USB4000-VIS-NIR
USB-ISS-VIS
None -- integrated
integrated tungsten
light source and
bulb with a violet
sample holder
LED and cuvette
directly attaches to
holder for 1-cm
spectrometer
$2,999
$1,499
(save
$1,500)
square cuvettes
CHEM4-UV-FIBER
200-885 nm
$3,999
ISS-UV-VIS
Lamp and sample
integrated
holder attach to
(save
deuterium tungsten
spectrometer via
$1,500)
halogen light
1-meter long
source and cuvette
P300-1-SR
holder for 1-cm
assembly with
square cuvettes
300 µm diameter
$2.499
solarizationresistant fiber
CHEM4-VIS-FIBER
USB4000-VIS-NIR
430-990 nm
$2,999
ISS-2 integrated
Lamp and sample
tungsten halogen
holder attach to
(save
light source and
spectrometer via
$1,500)
cuvette holder for
2-meter long
1-cm square
P400-2-UV-VIS
cuvettes
assembly with
$1,499
400 µm diameter
fiber
Specifications
CHEM4-UV-VIS
CHEM4-VIS-NIR
CHEM4-UV-FIBER
SYSTEM
Wavelength range*:
Optical resolution:
Integration time:
Dimensions (in mm):
210-880 nm
370-985 nm
200-885 nm
~1.0 nm FWHM
~1.0 nm FWHM
~1.0 nm FWHM
3.8 ms to 10 seconds
3.8 ms to 10 seconds
3.8 ms to 10 seconds
89.1 x 63.3 x 34.4 (USB4000)
89.1 x 63.3 x 34.4 (USB4000)
89.1 x 63.3 x 34.4 (USB4000)
198 x 105.1 x 40.6 (USB-ISS-UV) 40.7 x 88.8 x 34.1 (USB-ISS-VIS) 198 x 104.9 x 40.9 (ISS-UV-VIS)
DETECTOR & OPTICAL BENCH
Detector:
Toshiba CCD array (page 17)
Toshiba CCD array (page 17)
Toshiba CCD array (page 17)
Pixels:
3648 pixels
3648 pixels
3648 pixels
Optical bench design: f/4, crossed Czerny-Turner
f/4, crossed Czerny-Turner
f/4, crossed Czerny-Turner
Entrance aperture:
25 µm wide slit (page 15)
25 µm wide slit (page 15)
25 µm wide slit (page 15)
Grating:
Grating #1 (page 16)
Grating #2 (page 16)
Grating #1 (page 16)
Order-sorting filters:
OFLV-200-850 (page 17)
OFLV-350-1000 (page 17)
OFLV-200-850 (page 17)
LIGHT SOURCE/SAMPLE CHAMBER
Bulb(s):
Deuterium and tungsten halogen Tungsten halogen and violet LED Deuterium and tungsten halogen
Bulb lifetime:
800 hours
45,000 hours
800 hours
Cuvette pathlength:
1 cm
1 cm
1 cm
Optical fiber:
N/A
N/A
300 µm solarization-resistant, 1 m
ELECTRONICS & COMPUTER
Operating systems:
Windows 98/Me/2000/XP, Mac OS X and Linux when using the USB port
Computer interfaces:
USB 2.0 @ 480 Mbps (USB 1.1 compatible); RS-232 (2-wire) @ 115.2 K baud
Spectrometer Systems & Setups
USB4000-UV-VIS
CHEM4-VIS-FIBER
430-990 nm
~1.0 nm FWHM
3.8 ms to 10 seconds
89.1 x 63.3 x 34.4(USB4000)
155 x 50 x 53.3 (ISS-2)
Toshiba CCD array (page 17)
3648 pixels
f/4, crossed Czerny-Turner
25 µm wide slit (page 15)
Grating #2 (page 16)
OFLV-350-1000 (page 17)
Tungsten halogen
900 hours
1 cm
400 µm diameter fiber, 2 m
* The actual ranges may exceed these listed here. Ranges listed are where you will see changes as small
as 1.0 absorbance units.
Tel: 727.733.2447 • Email: [email protected]
37
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Red Tide Spectrometer for Education
World’s Most Amazing $999 Spectrometer
The Red Tide Spectrometer is a low-cost, smallfootprint lab spectrometer that's ideal as a generalpurpose instrument for budget-conscious teaching and
research labs. The Red Tide has a wavelength range of
350-1000 nm, and utilizes a detector with 650 active
pixels; that’s 650 data points in one full spectrum, or
one data point per nanometer. Configured with a 25 µm
entrance slit, the Red Tide offers ~2.0 nm optical
resolution (FWHM).
Flexible Platform, Convenient Interface
Spectrometer Systems & Setups
The Red Tide is a preconfigured, off-the-shelf
spectrometer where all of the optical bench options,
such as grating and entrance slit size, are already
selected. The Red Tide can be used with various Ocean
Optics accessories, light sources and sampling optics, to
create application-specific systems for various
absorbance, reflection and emission applications. With
its small footprint, convenient USB interface, and four
millisecond integration time, the Red Tide is a great tool
for basic lab measurements.
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Spectrometer Alone or with Sampling System
At just $999, the Red Tide is a great general-purpose spectrometer for budgetstrapped teaching labs. Combine the Red Tide with Ocean Optics light sources,
accessories and software to create a fully integrated, small-footprint system.
Specifications
PHYSICAL
Dimensions (in mm):
Weight:
DETECTOR
Type:
Pixels:
Pixel size:
Pixel well depth:
Sensitivity:
OPTICAL BENCH
Design:
Focal length:
Entrance aperture:
Fiber optic connector:
SPECTROSCOPIC
Wavelength range:
Optical resolution:
Signal-to-noise ratio:
A/D resolution:
Dark noise:
Dynamic range:
Integration time:
Stray light:
Corrected linearity:
COMPUTER
Operating systems:
Operating software:
38
89.1 x 63.3 x 34.4 (USB-650);
89.1 x 104 x 34.4 (USB-650-VIS-NIR)
190 g
Linear silicon CCD array
650 enabled pixels
14 µm x 200 µm
~62,500
75 photons/count @ 400 nm
f/4, asymmetrical crossed Czerny-Turner
42 mm input; 68 mm output
25 µm wide slit
SMA 905
350-1000 nm (USB-650); 370-980 nm (USB-650-VIS-NIR)
~2.0 nm FWHM
250:1 (at full signal)
12 bit
3.2 RMS counts
2 x 108; 1300:1 for a single acquisition
4 milliseconds to 10 seconds
<0.05% @ 600 nm; <0.10% @ 435 nm
>99.8%
Windows 98/Me/2000/XP, Mac OS X and Linux w/USB port
SpectraSuite Spectroscopy Operating Software
The USB-650 Red Tide comes without a light source or
sample system, allowing you the freedom to choose the
accessories that best fit your setup. The USB-650-VIS-NIR
(at right) comes with a direct-attach
light source and sample
holder. The light
source includes an
LED-boosted tungsten
source and a sample
holder for 1-cm cuvettes
that connects to the front of
the spectrometer. In this
configuration, the system has a
wavelength range of 370-980 nm.
Operable with PCs or Dataloggers
The Red Tide interfaces to PCs via its USB port, which
streamlines start-up and supports hot swapping of the
spectrometer. What's more, the Red Tide interfaces to
Pasco's Xplorer GLX, a unique combination of
datalogger and lab analysis tool that eliminates the
need for a PC. For details, see the facing page. The Red
Tide also works with Vernier’s Logger Pro Software. Visit
www.vernier.com/soft/lp.html for details.
Cross-platform Spectrometer Software
Red Tide operates via SpectraSuite Spectroscopy
Operating Software, the first spectroscopy software to
run in Macintosh, Linux and Windows. The Chemistry
module for SpectraSuite includes features specifically
designed for educational use, such as a Beer's Law
calculator for absorbance experiments.
USB-650:
$999
USB-650-VIS-NIR: $1,499
SpectraSuite:
$199
For all your sensing needs, visit OceanOptics.com
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Xplorer GLX Handheld Datalogger
The World's First Graphing Datalogger for Science
The new Xplorer GLX from PASCO captures, analyzes,
annotates and stores data quickly and seamlessly, without
being connected to a desktop computer. The Xplorer
GLX has been designed to function with our line of
Spectrometers for Education: the CHEM4
Spectrophotometers (pages 36-37) and
the USB-650 Red Tide
Spectrometer (page 38). The
Xplorer GLX is a science lab
wherever you need it, whether
you are in the lab or out in the
field. When combined with the
Xplorer GLX, our Spectrometers
for Education become powerful
measurement, display and analysis
tools for students. The Xplorer GLX can
display real-time intensity, absorbance,
transmission or relative irradiance spectra in less than
one second.
The PS-2636 Xplorer GLX (in blue)
easily connects via USB cable to the
USB-650 Red Tide Spectrometer for
capturing, displaying and analyzing
real-time spectroscopic data.
Stand-alone Computing Power
The Xplorer GLX is built for the demanding university teaching
environment. It incorporates an easy-to-use, icon-based operating
system as well as navigation buttons and a numeric/alphanumeric
keypad. With 10 MB of internal memory, the Xplorer can be used as
a stand-alone computer but also can interface to traditional desktop
computers. If more memory is needed, save Xplorer data to a flash
drive. For traditional navigation and annotation, you can plug in an
optional USB mouse and keyboard. The Xplorer’s rechargeable NiMH
battery enables field portability and its large backlit LCD screen is
visible in both sunlight and low-light conditions. In addition, a USB
port allows students to print graphs and tables directly from the
Xplorer GLX to select Hewlett-Packard printers.
Built for Science
The Xplorer GLX includes helpful student features such as a built-in
graphing calculator with an expression editor for analyzing trends.
The datalogger also includes statistical and mathematical tools to
easily review data and perform basic data analysis, such as linear
curve fits. Students can annotate data points with either text notes or
recorded voice messages (the GLX has a built-in speaker for sound
output). The Xplorer GLX has four universal sensor ports as well as
ports for two Temperature Sensors, a Sound Sensor, and a Voltage
Sensor (included).
Ordering Information
Order the PS-2555 License Key if you already own an Xplorer GLX
but want it to work with an Ocean Optics Spectrometer. The PS-2555
is a License Key only; it does not include a spectrometer or the
Xplorer GLX. The PS-2636 comes with the Xplorer GLX and the
License Key (an Ocean Optics spectrometer is sold separately). The
License Key also includes a feature set from our SpectraSuite
Spectroscopy Operating Software; however, if you wish to download
data from the Xplorer GLX and utilize it on a desktop PC, you may
want to purchase the full SpectraSuite Software.
PS-2636 Xplorer GLX & License Key: $425
PS-2555 License Key:
$129
Tel: 727.733.2447 • Email: [email protected]
Spectrometer Systems & Setups
For those who
already own an
Xplorer GLX, you
only need to purchase
the PS-2555 License
Key and an Ocean Optics
spectrometer; the key will
enable the Xplorer to work
with our line of education
spectrometers.
The Xplorer GLX comes with software, a power supply, a USB
cable, two temperature sensors, a sound sensor, a voltage
sensor and easy-to-use instructions.
Specifications
Dimensions (in mm):
Display screen:
89.1 x 63.3 x 34.4
320 x 240 backlit transflective
LCD grayscale display
Sampling rate:
50,000 Hz maximum
Internal memory:
10 MB
Battery:
Rechargeable NiMH battery
Xplorer with USB-650 Red Tide: Supports basic functions
Xplorer with CHEM4 units:
Supports triggering functions and
digital user-programmable GPIOs
39
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MEMS-based NIR Spectrometer
Compact, Low-Cost NIR Spectrometers
Digital Transform Spectroscopy (DTS) NIR Spectrometers by Polychromix are
compact, low-cost NIR systems powered by MEMS architecture. Available in
0.9-1.7 µm, 1.7-2.5 µm and 1.1-1.3 µm wavelength ranges, the spectrometers
have no moving parts, and feature a single-element InGaAs detector. The fully
programmable spectrometers can be configured to operate in various scanning
modes for a variety of general-purpose NIR applications that include quality control,
education, R&D and industrial process control. The DTS-series NIR Spectrometers
are compact and portable, interface to PCs via USB, and require no external power.
Digital Transform Spectroscopy (DTS)
Spectrometer Systems & Setups
Polychromix's DTS-series Spectrometers use a grating and an innovative MEMS
spatial light modulator to disperse light onto the the system's single-element InGaAs
detector. Each wavelength of light can be modulated on and off with differing time
sequences. The resulting time-varying signal is processed to create a spectrum.
We recommend
our VIS-NIR Optical
Fiber Assemblies in diameter sizes greater than
500 µm for use with the DTS Spectrometers.
Spectrometer Models and Accessories
Ocean Optics offers three Polychromix DTS NIR Spectrometer models that vary by
wavelength range. Each DTS Spectrometer includes a protective cover, DTS software,
a USB cable and documentation.
DTS-1700:
$7,199
DTS-2500: $10,999
DTS-NB:
$7,199
Specifications
Dimensions:
Weight:
Spectral range:
Detector:
Optical resolution:
Photometric stability:
Measurement time:
Operating systems:
Operating temp:
DTS-1700
105 mm x 85 mm x 145 mm
1.8 kg
~930-1690 nm
Single-element InGaAs
12.0 nm
<0.05% over 6 hours
<1 second per spectrum
Windows Me, 2000, XP
-5 °C to 40 °C
DTS-2500
105 mm x 85 mm x 145 mm
1.8 kg
~1710-2460 nm
Single-element InGaAs
22.0 nm
<0.05% over 6 hours
<1 sec. per spectrum
Windows Me, 2000, XP
-5 °C to 40 °C
DTS-NB
105 mm x 85 mm x 145 mm
1.8 kg
1100-1350 nm
Single-element InGaAs
4.0 nm
<0.05% over 6 hours
<1 sec. per spectrum
Windows Me, 2000, XP
-5 °C to 40 °C
Phazir MEMS-based NIR Material Analyzer
Point-and-shoot NIR Measurement Tool
The handheld Phazir NIR Material Analyzer enables real time
and instantaneous qualitative and quantitative material analysis
and provides both material ID and concentration levels via its
onboard color LCD screen. This non-destructive measurement
tool stores all data into memory, which allows the user to
transfer the data to a PC for logging or additional processing.
Applications
Specifications
Dimensions:
Weight:
Light source:
Wavelength range:
254 mm x 292 mm x 152 mm
1.7 kg
Tungsten light bulb
DTS-PHAZIR-1016: 1000-1600 nm;
DTS-PHAZIR-1624: 1600-2400 nm
Resolution (FWHM): DTS-PHAZIR-1016: 8.0 nm; DTS-PHAZIR-1624: 12.0 nm
Security:
Password protection, multiple security levels
Operating temp.:
5 °C to 45 °C (40 °F to 115 °F)
Batteries:
Rechargeable 5-8 hour lithium-ion battery pack
Included:
Waterproof carrying case, reference/calibration cap,
PC interface cable, 110/220 VAC battery charger/adapter,
documentation CD, spare bulb, bulb replacement tools
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Designed for the technician, the point-and-shoot Phazir
requires minimal training to operate. The Phazir is perfect for
use in materials identification, incoming material inspection,
quality control, quality assurance and portable field use.
Portability & Durability
The Phazir is a portable and handheld device weighing only
1.7 kg. Its rechargeable batteries allow 5-8 hours of continued
use. The instrument is housed in injection-molded plastic that
can withstand harsh environments.
DTS-PHAZIR-1016: $20,000
DTS-PHAZIR-1624: $24,000
For all your sensing needs, visit OceanOptics.com
Process-2000 Process Control Systems
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Multichannel Spectrometer Systems for Process Control
Process-2000 Multichannel Spectrometer Systems are designed
for the process control environment. The custom
experiment feature allows you to configure custom
experiment methods for your process. Once you save a
custom method, you need only select the method file to
execute your custom experiment. The systems allow you to
have full access, remotely if needed, to all software and
hardware functions via easy-to-use monitoring and
control software. Your spectral data (absorbance,
transmission, reflection or emission) can be acquired in
3.8 milliseconds, and mathematically calculated, subtracted and
monitored in situ and in real time.
Inputs/Outputs Provide Full Control
Multichannel Spectrometer Systems
Process-2000 systems provide the ultimate flexibility. Detector options for each
spectrometer channel include a 1024-, 2048- or 3648-element linear CCD
array. Choose all of your spectrometer options from the size of the bench’s
entrance aperture to the wavelength range of the channel for a true
application-specific system. Specify from two to six spectrometer channels.
Included Process-2000 Software
Process-2000 systems come with sophisticated software tools. The Recipe
Editor tool allows you to easily and rapidly configure, build and save
experiment methods even for the most difficult and complex processes. After
creating a “recipe,” you select it to execute the experiment. The Integrated
Formula Editor provides easy access to a full range of mathematical and
algorithmic functions. The Wavelength Editor allows you to optimize signal-tonoise. A dual-window interface shows the actual spectrum and all process
control information.
Additional Software: SpecLine Software for Compound ID
SpecLine Software is a powerful tool designed for identifying atomic emission
lines and molecular bands in spectral data. SpecLine’s advanced evaluation,
search, compare and identify functions enable you to quickly identify unknown
lines, peaks and bands. SpecLine was designed for scientists, engineers and
researchers using emission spectroscopy in fields such as astrophysics, the
plasma sciences, and plasma processing. For more on SpecLine, see page 83.
Process-2000 systems can make
absorbance, transmission,
reflection and emission
measurements. Applicationspecific measurements include:
Light emission
Peak detection
Particle densities
Electron densities
Electron temperature
Planarization
Contamination
Failure analysis
Pulsed magnetron sputtering
Quality control (pollutants,
discharges, etc.)
Endpoint detection
Film/layer monitoring
Thin film thickness
Etching and deposition
Plasma chamber health
control
Protection coatings
Item
Description
PROCESS-2000-2
2-channel spectrometer system with housing; select detector, wavelength range, entrance slit for each channel
$19,998
PROCESS-2000-3
3-channel spectrometer system with housing; select detector, wavelength range, entrance slit for each channel
$22,678
PROCESS-2000-4
4-channel spectrometer system with housing; select detector, wavelength range, entrance slit for each channel
$25,358
PROCESS-2000-5
5-channel spectrometer system with housing; select detector, wavelength range, entrance slit for each channel
$28,038
PROCESS-2000-6
6-channel spectrometer system with housing; select detector, wavelength range, entrance slit for each channel
$30,718
Tel: 727.733.2447 • Email: [email protected]
Spectrometer Systems & Setups
A Process-2000 system interfaces to a computer via a USB cord and can be
controlled remotely. These systems interface to other process equipment and
control hardware via digital and analog inputs/outputs. You have access to 16
digital inputs/outputs per spectrometer channel and eight analog outputs per
spectrometer channel. Some ways the inputs/outputs can be used:
A digital input could come from the process control setup
A digital output can display the upper and lower limits you have set for a
monitoring cycle, or could stop a process under special circumstances,
such as when an abnormal phenomena are detected
An analog output can read out measurement specifications or control a
pressure or liquid flow valve
Price
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Deep Well for High S:N
Sensitivity to 0.00001 Absorbance Units
The S1024DW Deep Well Detector Spectrometer has a 1024-element photodiode
array detector for applications requiring high signal-to-noise ratio measurements.
With the S1024DW, you can observe absorbance changes of less than 0.00001
absorbance units -- performance that makes the spectrometer ideal for high lightlevel applications.
“X” Option: Extra-deep Well Detector
The S1024DW is our standard deep well detector spectrometer. Its photodiodearray detector has a signal-to-noise ratio of 2500:1. Also available is the
S1024DWX, with a detector distinguished by both its deeper well depth and S:N of
8000:1.
Bench Ideal for High Light-level Applications
Spectrometer Systems & Setups
The S1024DW uses the “USB” (also called the “S”) Optical Bench, which allows
you to configure the bench for your application. You can choose an entrance
aperture size, detector accessories, filters, a grating and more (see pages 15-17).
The S1024DW bench operates much like the USB4000 bench seen on page 15.
The bench accepts light energy via an optical fiber and disperses it across a very
sensitive 1024-element photodiode array, instead of the 3648-element CCD array
that’s used in the USB4000.
Stackable System for Multipoint Sampling
You can add up to seven S1024DW Spectrometer channels to your master
S1024DW Spectrometer channel to measure multiple samples, expand your
wavelength range or monitor a reference. All channels operate from a single
ADC1000-USB A/D Converter, which has a channel rotator function that enables
simultaneous acquisition of data from up to eight spectrometer channels. The
ADC1000-USB interfaces the S1024DW to your PC via a USB port. You can
purchase the S1024DW and the ADC1000-USB separately, or buy them as one
item (S1024DW-USB) and save $99. See page 84 for more on the ADC1000-USB.
S1024DW-USB:
$3,099
S1024DW (master channel):
$2,599
S2-1024DW (additional channel): $1,399
S1024DW X (master channel):
$3,999
S2-1024DWX (additional channel): $2,899
ADC1000-USB:
$599
Detector Options for S1024DW-series
Detector Accessories for S1024DW-series
Features
S1024DW
S1024DWX
Item
Description
Price
Detector:
Hamamatsu S3903
Hamamatsu S3904
L2 Detector
Cylindrical lens placed on the
$150
linear photodiode array
linear photodiode array
Collection
detector for increased light-
Number of Elements:
1024 pixels
1024 pixels
Lens
collection efficiency
Pixel Size:
25 µm x 500 µm
25 µm x 2500 µm
OFLV-DW
Variable longpass filter removes
Well Depth:
31,000,000 electrons
156,000,000 electrons
S:N (at full signal):
2500:1
8000:1
A/D Resolution:
12 bit
16 bit
Dark Noise:
2 RMS counts
2 RMS counts
second- and third-order effects
Corrected Linearity:
>99%
>99%
for systems from 350-1000 nm
$150
second- and third-order effects
for systems from 200-850 nm
OFLV-350-DW
Variable longpass filter removes
$150
Specifications
Dimensions:
153.4 mm x 105.2 mm x 65.6 mm (when housed with the
ADC1000-USB A/D Converter)
Power consumption: 180 mA @ 5 VDC (master channels for S1024DW & DWX)
140 mA @ 5 VDC (additional channels for S1024DW & DWX)
Detector:
Linear photodiode array (see above)
Detector range:
200-1100 nm
Gratings:
14 gratings; UV through Shortwave NIR (page 16)
Entrance aperture: 5, 10, 25, 50, 100 or 200 µm wide slits (page 15)
or fiber (no slit)
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Order-sorting filters:
Focal length:
Optical resolution:
Installed bandpass and longpass filters (page 17)
42 mm (input); 68 mm (output)
~0.3-10.0 nm FWHM (depending on grating and size of
entrance aperture)
Stray light:
<0.05% at 600 nm; <0.10% at 435 nm
Relative sensitivity:
Compared to CCD detector in USB2000, S1024DW is ~30x
less sensitive in the UV and ~80x less sensitive in the VIS
Fiber optic connector: SMA 905 to 0.22 numerical aperture single-strand fiber
Integration time:
31 milliseconds to 65 seconds
For all your sensing needs, visit OceanOptics.com
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Flow Injection Analysis System
Automated System for Assays
The FIA-LAB-2500 is a flow injection analysis system
from FIAlab Instruments, a longtime Ocean Optics
partner. The FIA-LAB-2500 was designed for
automation of common environmental and agricultural
assays such as nitrate, phosphate and ammonia. A
complete, automated FIA-LAB-2500 system -including a USB4000 Spectrometer, light source, flow
cell, accessories and optional XYZ autosampler -can be configured for about $20,000. Affordability
and flexibility make the system ideal for teaching,
research and commercial labs, especially where routine
analyses demand a robust, easy-to-use system.
Commonly measured analytes include ammonia,
chloride, copper, iron, nitrate, nitrite and phosphate.
Built-in Flexibility, Affordability
Assay
Throughput
Working Range*
Nitrate
180 samples/hour
0.03 mg-200 mg/liter
Nitrite
220 samples/hour
0.005 mg-100 mg/liter
Ammonia
120 samples/hour
0.5 mg-200 mg/liter
Phosphate
120 samples/hour
0.1 mg-25 mg/liter
Chloride
120 samples/hour
1.0 mg-50 mg/liter
Iron
140 samples/hour
0.1 ppm-100 ppm
* Lower working ranges available with long pathlength flow cells, please contact
Ocean Optics for details.
Ease of Use Tops List of Benefits
Nitrate Run: Raw Data of Triple Injections
10 mg/L
1.6
1.4
ABSORBANCE (AU)
The FIA-LAB-2500 automates the handling of sample
and reagent solutions, so that messy, awkward and
inexact manual handling of solutions is unnecessary.
Ease of operation is one of several benefits:
There is no need to purchase separate expensive
manifolds for each type of analytical method.
Wavelength selections are made through software;
no additional filters or lamps are required.
Monitoring multiple wavelengths (up to four)
substantially extends the system's dynamic range.
Reference wavelengths are utilized for compensation
of colored matrices and index of refraction effects.
The system automatically corrects for response drift.
1.2
1.0
5 mg/L
0.8
Spectrometer Systems & Setups
The standard FIA-LAB-2500 consists of an automated
flow injection system with a four-channel peristaltic
pump, a six-port injector valve with fittings and tubing, a
flow cell, an LED light source and software. (Other light
sources are available at additional cost.) A spectrometer
does not come with the FIA-LAB-2500; we recommend
the USB4000-VIS-NIR (page 34). A range of accessories
is available, including the FIA-ASX260 Autosampler with
180-sample capacity, the flow-through FIA-HEATER for
elevated-temperature assays, and flow cells of varying
optical pathlengths. Longpath flow cells are available for
ultra-low concentration assays.
0.6
2 mg/L
0.4
0 mg/L
0.8 mg/L
0.2
0
0
25
50
75
100
125
150
175
200
225
250
275
TIME (seconds)
Example Applications
Nitrate/Nitrite Assay. This method performs FIA assays
for soil testing and analysis of potable water and
ground, surface, domestic and industrial wastewaters.
Phosphate Assay. A phosphate measurement method
based on U.S. EPA protocols, best suited for agricultural
and environmental testing.
Ammonia Assay. An FIA assay for low ammonia
concentrations using the salicylate method. Ideal for
agricultural and environmental testing.
FIA-LAB-2500:
$10,500
FIA-ASX260:
$5,800
FIA-HEATER:
$450
Tel: 727.733.2447 • Email: [email protected]
Specifications
Accuracy (typical):
Precision (typical):
Pump:
Dimensions:
Weight:
Recommended light source:
2%-3%
1%-2%
4-channel standard, 6-channel available
24 cm height x 24 cm depth x 16.5 cm width
6.75 kg
LS-1 Tungsten Halogen Light Source (360-2000 nm),
see page 128
Recommended spectrometer: USB4000-VIS-NIR (350-1000 nm), see page 34
Autosampler (optional):
180, 270 or 360 samples; 10 standards
Flow-through heater (optional): Ambient up to 50 °C (accuracy is +/- 0.5 °C)
43
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PMT for Fluorescence Flow Analysis
Parts-per-trillion Sensitivity
The FIA-PMT-FL Photomultiplier Flow-through Detection System
provides parts-per-trillion sensitivity for ultra-low fluorescence,
chemiluminescence and bioluminescence measurements. The
system can achieve sensitivity of 10 parts per trillion (measured
with fluorescein with a 200 millisecond integration time and
using an internal LED light source). Because of its heavy-duty,
chemically resistant housing, the system can withstand harsh
industrial environments.
Modular Design
Spectrometer Systems & Setups
The FIA-PMT-FL is built to order with either an internal excitation
lamp or with an optical fiber interfacing to an external lamp (as
seen at right). Excitation lamp source options include
tungsten, mercury vapor, ultraviolet and visible
LEDs, and laser diodes. Emission and
excitation filters are mounted in slots in the
enclosure, allowing for easy removal or
exchange. Though the system uses a 25 µL
flow-through cuvette, you can also use standard
1-cm pathlength cuvettes for manual measurements.
Easy PC Interface & Optimized Software
Included with the system is Windows-based software that allows
you to set the integration time and acquisition rates, and to
obtain time histories of the measurements, both plotted and
tabulated. The software can also automatically create calibration
curves, as well as controlling a host of additional devices such as
FIAlab's FIA/SIA systems, syringe and peristaltic pumps, injection
valves, selection valves, and autosamplers (please inquire for
details). For users who desire to control the PMT-FL from their
own software project, included is an ActiveX control for use with
Visual Basic, VC++, LabVIEW, or nearly any other ActiveXcompatible development environment.
Specifications
Dimensions:
Spectral range:
Detector:
PMT dynamic range:
Responsivity:
Detection limits:
Pulse-pair resolution:
Flow cell pathlength:
Flow cell volume:
Filters:
Example Assays Applications for the PMT-FL
Fluorometric ammonium analysis: ultra low level assays, parts
per billion sensitivity.
F4551: Fluorescein di(b-D-glucuronide) hydrolyzes to
fluorescent fluorescein. It has been used to detect ß
glucuronidase activity, an assay for lysosomal enzyme release
from neutrophils.
M8639: 2'-(4-Methylumbelliferyl)-a-D-N-acetylneuraminic
acid sodium salt hydrate, which is a fluorometric assay of
neuraminidase.
L9009: Luciferase Photinus pyralis. The bioluminescent
reaction of this enzyme with luciferin, ATP, and O2 results in
the emission of light. Luciferase can be used to detect trace
amounts of ATP.
GUS-A: b-Glucuronidase Fluorescent Activity Detection Kit.
The substrate used in this kit is MU-GlcA (4-methylumbelliferyl
b-D-glucuronide), a widely used fluorogenic substrate for
determining glucuronidase activity.
FIA-PMT-FL:
$6,495
Computer interface:
Operating systems:
Flow through heater:
Internal Excitation Source Options:
Laser Diodes (532 nm, 635 nm or 650 nm)
Quartz tungsten lamp (440-750 nm)
Mercury Vapor lamps (350-400 nm)
UV LED lamp (270-410 nm)
Various visible LED lamps
External Excitation Source Options:
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44
~13 cm x 18 cm x 25.4 cm
310-750 nm (filter/lamp selection dependent)
Photo-counting photomultiplier tube
2 x 106
5 x 1017 cps/watt (@ 400 nm)
10 parts per trillion measured with fluorescein
@ 200 msec integration time and internal LED
light source
10 ns
10 mm
25 µL with standard flow-through cuvette
Each FIA-PMT-FL includes your waveband
choice of 1 excitation filter and 1 emission filter
(call for options)
RS-232
Windows 98/Me/2000/XP operating systems
Heated flow cell (optional), ambient to 60 °C,
+/- 0.5 °C accuracy.
Laser Diodes (532 nm, 635 nm or 650 nm)
Quartz tungsten lamp (440-750 nm)
Mercury Vapor lamps (350-400 nm)
UV LED lamp (270-410 nm)
Various visible LED lamps
Deuterium lamp (200-400 nm)
For all your sensing needs, visit OceanOptics.com
QE65000 Configured for Fluorescence
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Scientific-grade Spectrometer
The QE65000 Spectrometer is a unique combination of
detector and optical bench technologies that provides users
with high spectral response and high optical resolution in
one scientific-grade spectrometer package.
QE65000 Scientificgrade Spectrometer
Demanding Low Light-level Applications
PX-2 Pulsed Xenon
Light Source
QE65000 Spectrometer
Fluorescence Standard
Specifications
PHYSICAL
Dimensions (in mm):
Weight:
DETECTOR
Detector:
Detector range:
Pixels:
Pixel size:
Signal-to-noise ratio:
Dark noise:
Sensitivity:
OPTICAL BENCH
Design:
Focal length:
Entrance aperture:
Gratings:
Filters:
SPECTROSCOPIC
Wavelength range:
Optical resolution:
Integration time:
Dynamic range:
Stray light:
Fiber optic connector:
ELECTRONICS
Power consumption:
182 x 110 x 47
1.05 kg
Hamamatsu S7031-1006 back-thinned CCD (page 28)
200-1100 nm
1024 x 58 (1044 x 64 total)
24.6 µm square size
1000:1 (at full signal)
2.5 RMS counts
400 nm: 22 electrons/count, 250 nm: 26 photons/count
f/4, Symmetrical crossed Czerny-Turner
101.6 mm input, 101.6 mm output
5, 10, 25, 50, 100, or 200 µm wide slits (page 27)
14 gratings, UV through Shortwave NIR (page 28)
OFLV-QE and OF-1 order sorting filters (page 27)
Grating dependent
~0.14-7.7 nm FWHM
8 milliseconds to 15 minutes
25000:1 a single acquisition; 7.5 x 109 (system)
<0.08% at 600 nm, <0.4% at 435 nm
SMA 905 to 0.22 numerical aperture single-strand fiber
500 mA @ 5 VDC no TE cool;
3 A @ 5 VDC with TE cool
Data transfer speed: Full spectrum to memory every 8 ms with USB 2.0 port,
8 ms with USB 1.1 port
Inputs/Outputs:
10 onboard digital user-programmable GPIOs
TEMPERATURE & THERMOELECTRIC (TE) COOLING
Temperature limits: 0 °C to 50 °C for spectrometer, no condensation
Temperature range: 13 °C maximum range between the high and low
Set point:
Software controlled
Lowest set point:
40 °C below ambient, to -15 °C
Stability:
±0.1 °C of set temperature in <2 minutes
COMPUTER
Operating systems: Windows 98/Me/2000/XP, Mac OS X and Linux when
using the USB port; 32-bit Windows OS when using
the serial port
Computer interfaces: USB 2.0 @ 480 Mbps; RS-232 (2-wire) @ 115K baud
Peripheral interfaces: SPI (3-wire); I2C inter-integrated circuit
Tel: 727.733.2447 • Email: [email protected]
CUV-ALL 4-Way
Cuvette Holder
Quantum Efficiency to 90%
The Hamamatsu FFT-CCD detector used in the QE65000
achieves up to 90% quantum efficiency (defined as how
efficiently a photon is converted to a photoelectron). Most of
our other detectors are linear CCDs, but with this “2D” area
detector we can bin a vertical row of 64 pixels that offers
significant improvement in the signal-to-noise ratio (1200:1)
and signal processing speed of the detector compared with
a linear CCD, where signals are digitally added by an
external circuit.
Spectrometer Systems & Setups
The QE65000 was designed for low-light level applications
such as fluorescence, Raman spectroscopy, DNA
sequencing, astronomy and thin-film reflectivity. For a
complete fluorescence system, combine the QE65000 with a
PX-2 Pulsed Xenon Light Source (page 127) to excite your
sample in a CUV-ALL 4-Way Cuvette Holder (page 90). In
addition, we offer LVF Linear Variable Filters (page 114) to
spectrally shape excitation energy from broadband sources
such as the PX-2. A solid secondary fluorescence standard,
the STAN-FL-RED, can be used for quick and easy
calibration, stability, and performance checks of your
fluorescence system.
Increased System Sensitivity
QE65000 system sensitivity is improved because the 2D
detector allows us to take advantage of the height of the
entrance slit. In our spectrometers, you regulate the light
entering the bench according to the slit’s width. Most of our
other spectrometers use linear detectors; in those
spectrometers, slit height doesn’t matter because linear
detectors cannot efficiently collect the light from the entire
height of the slit. But with the 2D detector in the QE65000,
we can better take advantage of this additional light,
extremely useful in low-light fluorescence applications.
QE65000:
$9,999
PX-2:
$769
CUV-ALL:
$809
STAN-FL-RED:
$179
45
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Fluorescence Spectrometers
Preconfigured Spectrometers for Use with Sensors
Our high-sensitivity, preconfigured fluorescence spectrometers -- the USB4000-FL,
USB4000-FL-450 and USB4000-FL-395 -- were conceived for use with fluorescence-based
sensors. Each unit is set to 360-1000 nm and comes with a 200-µm entrance aperture and
an L4 Detector Collection Lens for increased light throughput for fluorescence applications.
USB4000-FL: Excitation Source not Included
The USB4000-FL does not include an excitation source; this allows you the flexibility of
choosing from several compact, low-cost, modular excitation sources available, such as
one of our LEDs (pages 130-131). The excitation sources produce pulsed or continuous
output and couple easily to our spectrometers, optical fibers and accessories.
USB4000-FL
Spectrometer Systems & Setups
USB4000-FL-450 & USB4000-FL-395: Excitation Source Included
USB4000-FL-450
Specifications
PHYSICAL
Dimensions:
Weight:
DETECTOR
Detector:
OPTICAL BENCH
Design:
Focal length:
Entrance aperture:
Grating:
Fiber optic connector:
SPECTROSCOPIC
Wavelength range:
Optical resolution:
Signal-to-noise ratio:
A/D resolution:
Dark noise:
Stray light:
Corrected linearity:
ELECTRONICS
Power consumption:
Data transfer speed:
Inputs/Outputs:
COMPUTER
Operating systems:
Computer interfaces:
Peripheral interfaces:
LIGHT SOURCE
Stability:
Wavelength range:
Power consumption:
Power output:
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The USB4000-FL-450 and USB4000-FL-395 Spectrofluorometers are spectrometers configured the same as the USB4000-FL, but each comes with a direct-attach excitation source.
The USB4000-FL-450 comes with a 470 nm LED and the USB4000-FL-395 comes
with a 395 nm LED Excitation source. (When using these Spectrofluorometers with
one of our sensor probes, we recommend the USB4000-FL-450 with FOXY and
HIOXY sensing formulations and the USB4000-FL-450 with the FOSPOR sensing
formulation. See pages 65-68 for details.) The spectrometer provides power to the
LED and enables synchronization functions and I2C communications. In addition,
these sources connect to temperature sensors and contain onboard memory that can
be programmed to store temperature and oxygen calibration coefficients.
USB4000-FL:
$2,499
USB4000-FL-450: $3,049
USB4000-FL-395: $3,049
46
USB4000-FL
USB4000-FL450
USB4000-FL395
89.1 mm x 63.3 mm x 34.4 mm
190 grams
89.1 mm x 120.3 mm x 34.4 mm
310 grams
89.1 mm x 120.3 mm x 34.4 mm
310 grams
Toshiba TCD1304AP linear CCD array
(see page 17 for detector specifications)
Toshiba TCD1304AP linear CCD array
(see page 17 for detector specifications)
Toshiba TCD1304AP linear CCD array
(see page 17 for detector specifications)
f/4, Asymmetrical crossed Czerny-Turner
42 mm input; 68 mm output
200 µm wide slit
Grating #3, groove density of 600 lines
set to 360-1000 nm, blazed at 500 nm
SMA 905 to 0.22 numerical aperture fiber
f/4, Asymmetrical crossed Czerny-Turner
42 mm input; 68 mm output
200 µm wide slit
Grating #3, groove density of 600 lines
set to 360-1000 nm, blazed at 500 nm
SMA 905 to 0.22 numerical aperture fiber
f/4, Asymmetrical crossed Czerny-Turner
42 mm input; 68 mm output
200 µm wide slit
Grating #3, groove density of 600 lines
set to 360-1000 nm, blazed at 500 nm
SMA 905 to 0.22 numerical aperture fiber
360-1100 nm
~10.0 nm FWHM
300:1 (at full signal)
16 bit
50 RMS counts
<0.05% at 600 nm; <0.10% at 435 nm
>99.8%
360-1100 nm
~10.0 nm FWHM
300:1 (at full signal)
16 bit
50 RMS counts
<0.05% at 600 nm; <0.10% at 435 nm
>99.8%
360-1100 nm
~10.0 nm FWHM
300:1 (at full signal)
16 bit
50 RMS counts
<0.05% at 600 nm; <0.10% at 435 nm
>99.8%
250 mA @ 5 VDC
Full spectrum to memory every 5 ms with
USB 2.0 port, 18 ms with USB 1.1 port
Yes, 8 digital user-programmable GPIOs
250 mA @ 5 VDC and 60 mA @ 5 VDC
Full spectrum to memory every 5 ms with
USB 2.0 port, 18 ms with USB 1.1 port
Yes, 8 digital user-programmable GPIOs
250 mA @ 5 VDC and 60 mA @ 5 VDC
Full spectrum to memory every 5 ms with
USB 2.0 port, 18 ms with USB 1.1 port
Yes, 8 digital user-programmable GPIOs
Windows 98/Me/2000/XP, Mac OS X
and Linux with USB port; Any 32-bit
Windows OS with serial port
USB 2.0 @ 480 Mbps; RS-232
(2-wire) @ 115.2 K baud
I2C inter-integrated circuit; SPI (3-wire)
Windows 98/Me/2000/XP, Mac OS X
and Linux with USB port; Any 32-bit
Windows OS with serial port
USB 2.0 @ 480 Mbps; RS-232
(2-wire) @ 115.2 K baud
I2C inter-integrated circuit; SPI (3-wire)
Windows 98/Me/2000/XP, Mac OS X
and Linux with USB port; Any 32-bit
Windows OS with serial port
USB 2.0 @ 480 Mbps; RS-232
(2-wire) @ 115.2 K baud
I2C inter-integrated circuit; SPI (3-wire)
n/a
n/a
n/a
n/a
± 1.0% drift after 2-minute warm-up period
460-490 nm
60 mA @ 5 VDC
60 µW (minimum) into a 600 µm optical fiber
± 1.0% drift after 2-minute warm-up period
380-410 nm
60 mA @ 5 VDC
60 µW (minimum) into a 600 µm optical fiber
For all your sensing needs, visit OceanOptics.com
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Gated Spectrometer for Fluorescence
Ultimate Fluorescence Spectrometer
The USB2000-FLG Spectrofluorometer is a
preconfigured spectrometer for fluorescence
applications from 380-1050 nm. We utilize a
proprietary thin film technology and a timegated spectrometer to provide a spectrofluorometer that is 20 percent more sensitive
than the standard USB4000 Spectrometer.
Avoiding Scattered Light
Gated Fluorescence Mode
The USB2000-FLG is preloaded with variabledelay gating microcode, which allows you to
select a delay (from 5-500 microseconds) in
our software between the light turning on and
the start of the spectrometer's integration time,
when the detector “sees” the sample. In this
Gated Mode, the spectrometer only detects the
sample light when the source is off. In order to
use the Gated Mode, your fluorophore must
have a long fluorescence lifetime. Those
working with lanthanides and photoluminescent
materials will find this mode very useful. The
best excitation source to use with the Gated
Mode is our PX-2 Pulsed Xenon Source.
Terbium-dipicolinic acid (Tb-DPA) photoluminescence spectra acquired with the USB4000FLG while in the Gated Mode, with the data acquisition delay set at a range of values.
Analysis of samples with long emission lifetimes such as Tb-DPA improves when data
acquisition is delayed until the energy from the lamp pulse is no longer observed in the
spectrum, resulting in a cleaner, more resolved Tb-DPA spectrum -- achieved without using
optical filters. At delay times below 40 microseconds, lingering excitation energy and
background fluorescence overlap the Tb-DPA photoluminescence spectrum.
Specifications
Dimensions:
Weight:
Power consumption:
Wavelength range:
Detector:
Grating:
Entrance aperture:
Optical resolution:
Stray light:
Fiber optic connector:
Integration time:
Operating systems:
89.1 mm x 63.3 mm x 34.4 mm
190 g
90 mA @ 5 VDC
380-1050 nm
2048-element linear silicon CCD array
Grating #3 -- 600 lines per millimeter, blazed at 500 nm
200 µm wide slit
~10.0 nm FWHM
~0.05% at 600 nm, <0.10% at 435 nm
SMA 905 to 0.22 numerical aperture single-strand fiber
Gated mode - 5 milliseconds, normal mode - 3 milliseconds to 60 seconds
Windows 98/Me/2000/XP, Mac OS X and Linux operating systems when
using the USB port; any 32-bit Windows OS when using the serial port
Tel: 727.733.2447 • Email: [email protected]
Spectrometer Systems & Setups
In addition to the
USB2000-FLG, a
common fluorescence setup
may include products like those
shown above: the PX-2 Pulsed Xenon
Source, the CUV-ALL-UV Cuvette Holder, LVF Linear Variable Filters,
and optical fibers.
In addition to detecting fluorescence from a
sample, a spectrofluorometer will also detect
scattered excitation light from the light source
and the sampling compartment. (Scattering is
especially prevalent in turbid samples.) The
USB2000-FLG uses two features to avoid
detecting scattered light: special mirrors in the
optical bench to absorb ultraviolet light and
improve sensitivity and -- for fluorophores with
long fluorescence lifetimes -- a time-gated
mode that delays the start of spectral data
acquisition by 5-500 microseconds after the
excitation source is turned on (or pulses).
SAG+ High-reflectivity Mirrors
In the USB2000-FLG, we replaced our
standard mirrors with proprietary Ag-coated
mirrors to increase reflectance, which increases
the sensitivity of the spectrometer by more than
20 percent. They also absorb nearly all
ultraviolet light, virtually eliminating the
excitation source's spectra from interfering with
the sample spectra.
Application Flexibility
The USB2000-FLG can detect fluorophores in
solutions and powders, and from surfaces. The
USB2000-FLG has been used to measure
fluorescence in coral, fruit and other flora and
fauna.
USB2000-FLG: $2,999
47
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LIBS2500 Spectrometer & Accessories
Instant Elemental Analysis from 200-980 nm
We offer a full range of systems and components for laserinduced breakdown spectroscopy, a noninvasive technique for
real-time, qualitative and semi-quantitative spectral analysis
of elements in solids, solutions and gases. The
LIBS2500-7 is a broadband (200-980 nm), highresolution detection system with optical resolution of
~0.1 nm (FWHM). Sensitivity to parts-per-billion
and picogram levels is possible.
Spectrometer Systems & Setups
How the LIBS Systems Work
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Above is a LIBS2500-7 Spectrometer System with a
LIBS-BUN-7 Fiber Bundle. This seven channel
spectrometer system provides elemental analysis from
200-980 nm. A LIBS2500 system requires a laser to
ablate the sample (see page 49) and a sampling
system, such as our LIBS-SC Sample Chamber, to
collect the emitted light.
Specifications*
Dimensions:
Weight:
Power consumption:
Detector:
Wavelength range:
Optical resolution:
Frame rate:
Integration time:
Trigger delay:
Trigger jitter:
Trigger level:
33.4 cm X 15 cm x 14 cm maximum
(spectrometer system)
6.4 kg (spectrometer system only)
1 A @ 5 VDC (spectrometer system
only)
(7) 2048-element linear silicon CCD
arrays
Channel dependent
~0.1 nm (FWHM)
10 Hz capability (PC-controlled)
2.1 ms; variable in free-run mode
-121 µs to +135 µs in 500 ns steps
(PC-controlled)
± 250 nanoseconds
(± 20 nanoseconds optional)
TTL not to exceed 5.5 volts
* For seven-channel LIBS2500-7 system.
A high-intensity, pulsed laser beam is focused on the
sample area. A single 10 nanosecond-wide laser pulse
ablates the sample and generates plasma. As the plasma
decays or cools, excited atoms in the plasma emit light at
wavelengths distinct to each element. The emission is collected
by a probe and sent to the spectrometer system. The system
provides full spectral analysis in less than a second. OOILIBS Operating
Software includes a library of elemental emission lines and enables
automatic identification of all elements present in the sample.
High-resolution Spectrometers
Our LIBS2500-7 Spectrometer System uses seven linear CCD-array
detectors for broadband 200-980 nm analysis. All spectrometers are
triggered to acquire and read out data simultaneously. The detection
system can be portable and is interfaced to a PC via a USB port. As lowercost options, LIBS2500 Systems are available with fewer than seven
channels (see table below), with a narrower wavelength range for elementspecific analyses. Depending on the range of your analyses, you may
require a system with less than seven channels at a significantly lower cost.
LIBS2500 Uses in Diverse Applications
48
Environmental: soil, particulates, sediments
Materials Analysis: metals, slag, plastics, glass
Forensics & Biomedical: teeth, bones
Metrology: silicone wafers, semiconductor materials
Bioresearch: plants, grains
Safety & Military: explosives, chemical and biological warfare agents
Art Restoration & Conservation: pigments, paints
Gemology & Metallurgy: precious metals, gems
Item
LIBS System Description
Price of
LIBS System
LIBS2500-7
7 channel LIBS System, includes all channels (A-G) below
$29,999
LIBS-BUN-7
$985
LIBS2500-6
6 channel LIBS System, choose 6 channels from A through G
$25,740
LIBS-BUN-6
$885
LIBS2500-5
5 channel LIBS System, choose 5 channels from A through G
$21,450
LIBS-BUN-5
$785
LIBS2500-4
4 channel LIBS System, choose 4 channels from A through G
$17,160
LIBS-BUN-4
$685
LIBS2500-3
3 channel LIBS System, choose 3 channels from A through G
$12,870
LIBS-BUN-3
$485
LIBS2500-2
2 channel LIBS System, choose 2 channels from A through G
$8,580
BIF600-2-UV/VIS
$385
LIBS2500-1
1 channel LIBS System, choose 1 channel from A through G
$4,290
P600-2-UV/VIS
$205
OOILIBS
LIBS System Software (includes elemental emission lines library)
$500
Optical Fiber
Bundle Required
n/a
Price of
Fiber Bundle
n/a
LIBS2500 Spectrometer Channels
Ordering a LIBS2500 System is easy. Components are offered
LIBS-CH-A
Spectrometer channel with 200-305 nm wavelength range
to give you maximum flexibility so that you order only what
LIBS-CH-B
Spectrometer channel with 295-400 nm wavelength range
you need. Select the Spectrometer Channels (LIBS-CH-X) for
LIBS-CH-C
Spectrometer channel with 390-525 nm wavelength range
your LIBS2500 System depending on the wavelength ranges
LIBS-CH-D
Spectrometer channel with 520-635 nm wavelength range
needed for your application. Channels (A, B, C, etc.) do not
LIBS-CH-E
Spectrometer channel with 625-735 nm wavelength range
have to be consecutive. You will also need to specify the fiber
LIBS-CH-F
Spectrometer channel with 725-820 nm wavelength range
bundle that corresponds to the number of channels being
LIBS-CH-G
Spectrometer channel with 800-980 nm wavelength range
ordered. For additional accessories, see the following page.
For all your sensing needs, visit OceanOptics.com
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Additional LIBS Components
LIBS Sample Chamber
The LIBS-SC Sample Chamber is a key component of a LIBS system and is designed to
perform various functions safely and in clear view of the sample. The LIBS-SC has an
eyewear-safe enclosure. The chamber has a safety-interlock so the laser will not fire
when the door is open. It houses a manually controlled x-y-z stage and provides
illumination for the optional LIBS-IM-USB Imaging Module. The LIBS-SC has an inert gas
induction port and a suction nozzle to remove
Specifications
particulates. In addition, you have the ability to
Stages:
Manual x-y-z stage
focus the laser to a 40 µm spot size. The
Sample size:
6.5 cm x 6.5 cm x 4 cm max.
sample chamber is designed for use with the
Laser safety shield: OD 6 for 1.064 mm laser
The LIBS-SC includes an evacuation
Big Sky Lasers we resell (see below for laser
energy (call for other
system that removes material from the
wavelengths)
sample area. You also can feed gases such details). If you wish to use the LIBS-SC with a
Internal optics:
25 mm diameter focusing lens,
as argon into the chamber. Flooding the
different laser, please contact Ocean Optics.
75 mm focal length supplied
chamber with an inert gas provides greater
LIBS-SC: $9,800
Ablation spot size: approximately 40 µm
sensitivity for many elements.
This image is the "O" in the
text “Quarter Dollar” on a U.S.
coin.
The LIBS-IM-USB Imaging Module directly attaches to
the LIBS-SC Sample Chamber to enable users to
magnify a sample image and to establish a laser
ablation target on the sample. The camera is also
useful when you want to adjust the laser focus at the
surface of the sample, or above or below the sample
surface. When used with the LIBS-SC and laser, the
LIBS-IM-USB and laser are in the same focal plane
enabling precise, rapid and convenient laser focus.
The USB-enabled color camera captures pre- and
post-ablation images of the sample and provides up
to 1280 x 1024 pixel resolution.
LIBS-IM-USB:
$8,000
Specifications
Interface:
Power:
Frame size:
USB 2.0 (480 Mb/sec)
USB 5 VDC, max. 180 mA
1280 x 1024, 640 x 480, 320 x 240,
160 x 120
Data output:
RGB 24 bit
Requirements: -- Windows XP Professional SP1
-- Support of Direct X
-- Driver compatible Windows driver
model (WDM)
-- SDK iREZ WDM library
-- 3.2 GHz or higher processor
-- 1 GB recommended memory
-- 10 GB free hard disk space
-- Rocket-fast GeForce 4200Ti or
better video card recommended
LIBS Laser Options
We offer two LIBS25000 laser power options from industry leader Big Sky Laser Technologies. Laser ablation
and plasma formation are very specific to the sample matrix, and therefore the power requirements will vary by
sample type. For most applications we employ a Q-switched 1064 nm Nd:YAG laser, and for maximum
versatility, we recommend a 200 mJ laser with attenuator to adjust the laser power according to the sample
matrix. The choice of laser power and wavelength depend on the material being analyzed and the sample’s
tolerable damage threshold. The LIBS-LASER is a 50 mJ CFR Nd:YAG laser for metal and thin film samples.
The LIBS-LAS200MJ is a 200 mJ CFR Nd:YAG laser for most all other materials.
LIBS-LASER:
$14,500
LIBS-LAS200MJ: $22,500
Spectrometer Systems & Setups
LIBS Imaging Module for Pinpoint Analysis
LIBS Versus Other Technologies
Parameter
LIBS
SEM/EDS
XRF
LA-ICP-MS
EPMA
Sample depth:
~50-100 µm
~5 µm
~100 µm
~80 µm
<1 µm
Sensitivity:
10-50 ppm
1000 ppm
100 ppm
<1 ppm
100 ppm
Precision:
Fair-good
Poor
Fair-good
Excellent
Fair
Accuracy:
Semi-quantitative
Qualitative
Semi-quantitative
Quantitative
Semi-quantitative
Analysis time:
Fast
Slow
Very slow
Slow
Slow
Sample consump:
almost non-destructive
non-destructive
non-destructive
almost non-destructive
non-destructive
Complexity:
Easy to use
Easy to use
Easy to use
Complicated
Complicated
Discrimination:
Good
Poor
Good
Excellent
Fair
Cost:
$60,000
$120,000
$120,000
$250,000
$600,000
Tel: 727.733.2447 • Email: [email protected]
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LIBS-ELITE Laser Ablation System
Highly Refined Sampling System for LIBS
Laser-induced Breakdown Spectroscopy is a noninvasive
technique for real-time, qualitative and semi-quantitative
spectral analysis of elements in solids, solutions and gases. The
LIBS-ELITE, developed by New Wave Research and Ocean
Optics, is a high-quality LIBS sampling system with unparalleled
sample imaging and control. The LIBS-ELITE consists of a laser
head, sample chamber, software-controlled X-Y positioner and
a high-resolution imaging system in a single housing. New
Wave Research developed the LIBS-ELITE to work with the
LIBS2500 System (page 48).
200 mJ Nd:YAG Laser
Spectrometer Systems & Setups
The LIBS-ELITE-200 comes with New Wave Research's Tempest
200 mJ Nd:YAG laser. The Tempest delivers high-energy
densities to the sample to create plasma from even the most
challenging materials. The accuracy and precision of the
system results from the 98% pulse-to-pulse stability of the
Tempest. A laser power meter located adjacent to the sample
and a software-controlled attenuator are standard features that
help enable quantitative sample analysis. Another laser option
is available; the LIBS-ELITE-90 comes with a 90 mJ laser.
The LIBS-ELITE
works with the
Ocean Optics LIBS2500-7
Spectrometer System (see page 48) to provide full spectral analysis from
200-980 nm, with optical resolution of 0.1 nm and sensitivity to parts-perbillion. Below is a magnification of the sampling area where the ablation
plume is produced behind an orange Class 1 shield. The sample
compartment itself contains a quarter.
Sample Chamber: Unprecedented Control
The open architecture of the sample chamber allows the sample
and ablation plume to be viewed easily through its Class 1
shield. The sample chamber includes a quick-loading sample
drawer, and can accommodate samples up to two inches in
diameter. A gas port on the rear of the housing enables the
chamber to be purged with argon, which is useful for increasing
sampling sensitivity, or with nitrogen or helium, which is useful
when measuring emissions of elements such as oxygen that are
found in ambient environments. An integrated rotometer
regulates the gas flow in the chamber.
Exact Positioning & High-resolution Imaging
The ELITE's software-controlled X-Y stage allows you to precisely
control the target location, to create reproducible maps, and to
automate sample mapping, patterning and rastering for testing
sample homogeneity or for bulk analysis. The spot size
controller sets the ablation spot size from 20 µm to 1200 µm.
The LIBS-ELITE’s high-resolution sample magnification
capability (see software screen capture at right) allows you to
view an exact spot before and after the ablation event.
Software with Spectral Library
The LIBS-ELITE comes with intuitive operating software and a
library of elemental emission lines, which enables automatic
identification of all elements present in a sample. The software
includes controls for ablation mode, laser repetition rate, laser
power, sample spot size selection, X-Y positioning, sample
viewing, sample mapping, gas routing, spectrometer system
triggering and automating sampling processes.
Sold Exclusively by New Wave Research
For pricing on the LIBS-ELITE systems, contact New Wave
Research at [email protected] or 800-566-1743. Also,
visit www.new-wave.com for more product information.
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View an exact spot of the sample before, during and after the ablation
process. The LIBS-ELITE provides real-time, high-resolution qualitative
analysis of trace elements in diverse materials such as metals, biological
tissues, soils, optics, semiconductors, gems and other geological, biological
and environmental specimens.
For all your sensing needs, visit OceanOptics.com
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Raman Selection Guide
Raman System Selection Guide
Raman spectroscopy is quickly becoming one of the preferred
chemical identification techniques in many application areas.
Raman is advantageous because it is:
Non-invasive: Sample through glass and plastic
Non-destructive: Sample can be reused
Fast: Typical measurement times 5-30 seconds
Raman spectroscopy provides rapid and reliable non-destructive
chemical analysis of aqueous solutions, powders, tablets, gels
and surfaces. A basic setup consists of a monochromatic source,
typically a laser, which interacts with the sample. The scattered
radiation is then collected by a spectrometer. We offer several
options for using Raman as a measurement tool:
QE65000 Modular Raman System, pages 52-53
Turnkey Raman Systems, page 54
We offer several Raman turnkey sensing systems from our
partner, Raman Systems, Inc. Their high-performance systems
are designed specifically for quick material identification and
verification in almost any setting. The RSL-Plus is for field
deployment and fast incident response, while the R-3000 is a
self contained semi-portable system for lab or field use.
MMS-Raman, page 55
Centice Corporation offers their Multimodal Multiplex
Spectroscopy Raman System to provide high performance
chemical analysis for a fraction of the cost of research-grade
systems. Due to its high sensitivity and great resolution, the
MMS-Raman is an ideal system for substance verification and
accurate concentration analysis, as well as for analysis of very
low-concentration samples.
Raman System Selection Guide
Specification
QE65000
R-3000
R-3000-HR &
R-3000 QE
RSL-Plus
MMS-RAMAN
Optical resolution
6-18 cm-1; Grating
10 cm-1
6 cm-1; 8 cm-1
12 cm-1
4 cm-1
Excitation wavelength
785 nm or 532 nm
785 nm or 532 nm
785 nm or 532 nm
785 nm
785 nm
Spectral range
Several options
from 150 cm-1 to
7500 cm-1; Grating
& laser dependent
200-2700 cm-1 (785 nm);
200-4000 cm-1 (532 nm)
200-2700 cm-1 (785 nm);
200-4000 cm-1 (532 nm)
200-2700 cm-1 (785 nm)
220-2000 cm-1
Detector
Hamamatsu
Sony/Toshiba/
Sony/Toshiba/
Sony/Toshiba/
Hamamatsu
Hamamatsu
Hamamatsu
Hamamatsu
Linear CCD/
Linear CCD/
Linear CCD/
Back Thinned
Back Thinned
Back Thinned
2048 or 1024 x 58
2048 or 1024 x 58
2048 or 1024 x 58
and slit dependent
Detector type
Pixels
Back Thinned
1044 x 64
Back Thinned
512 x 122
Raman Application Areas
Spectrometer Systems & Setups
The QE65000 Scientific-grade Spectrometer was designed for
low-light level applications such as Raman spectroscopy. You
have several grating and entrance aperture sizes from which to
choose to optimize a system for your specific application. In
addition, we have lasers and Raman probes to complete your
own modular Raman setup.
Raman spectroscopy is useful for analyzing molecules without a permanent dipole moment, which
does not show up on an IR spectrum. Raman spectroscopy is used to determine bond lengths in
non-polar molecules. It is useful for determining the identity of organic and inorganic species in
solution, as the Raman transitions for these species are more characteristic than for IR, where the
transitions are much more affected by the other species present in the solution. Raman can be used
to analyze solid, liquid and gaseous sample components even through glass and plastic containers.
Art: Pigments, inks, substrates, resins
Biology: in vivo studies, surface studies, SERS
Catalysts: NO decomposition, kinetics of hydrogenation reactions
Corrosion: corrosion kinetic studies, bronze, aluminum
Forensics: drugs, explosives, pigments, powders, tablets, gels and surfaces, chemicals
Materials: diamond films, semiconductors, nanotubes, asbestos, materials ID
Pharmaceuticals: in situ crystal growth monitoring, kinetics, active ingredients, polymorphs
differentiation
Polymers: polymerization monitoring, plasticizer studies, density mapping of films
Process: online monitoring, quality control, research
Other: gemology, geology, chemical and petrochemical processes, water-quality analysis
Tel: 727.733.2447 • Email: [email protected]
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Modular Raman Measurement Tools
785 nm Excitation Laser for Raman
The LASER-785 is a 500-milliwatt, continuous-wave laser
specifically developed for Raman spectroscopy. The highpower excitation source has an integrated laser driver, a
thermoelectric cooler, a TEC controller and a TTL
modulation port for controlling the input up to 100 kHz.
The LASER-785 has a narrow spectral line width of only
0.2 nm (see spectrum below). Its compact and rugged
design and its hermetically sealed laser component make
it optimal for various industrial and medical applications.
LASER-785:
$6,499
HR4000 Spectrum of LASER-785
14000
12000
INTENSITY
Spectrometer Systems & Setups
10000
Specifications
Dimensions:
Weight:
Noise:
Output fiber:
Warm-up:
Temperature:
Stability:
Humidity:
110 mm x 89 mm x 53 mm
600 grams
<0.5% RMS
100 µm @ 0.22 NA
15 minutes
-10 °C to 40 °C
<3% peak-to-peak in
8 hours
5-95% non-condensing
Laser life:
Power consumption:
Power output (CW):
Peak wavelengths:
Spectral line width:
Rise time:
Control:
Connector:
10,000 hours
3.0 A @ 5 VDC
>500 mW
785 +/- 0.3 nm
0.2 nm (typical)
<500 msec
TTL modulation
-- 0 to 100 kHz
SMA 905
8000
6000
4000
2000
0
784.4
784.6
784.8
785.0
785.2
785.4
785.6
WAVELENGTH (nm)
Fiber Optic Probes for Raman Applications
We offer several fiber optic probes for Raman spectroscopy from our
corporate partner InPhotonics. Each probe provides complete optical
filtering of the Rayleigh line and high signal collection in a compact,
rugged probe design. Several probe models are available for
laboratory, industrial and environmental applications.
The probes listed below are available for several excitation
wavelengths. Please contact Ocean Optics for details.
RPB Laboratory Probe
Item
Description
Probe Size
(in mm)
Fiber
Length
Price
RIP-RPB
Laboratory probe for use with lasers up to 3 nm from specified operating
114 x 38 x 12.7
1.5 meter
$2,750
Stainless-steel focused probe for lab and field use; has 5-mm focal
12.7 OD x
5 meters
$4,950
length (7.5 mm or 10 mm also available)
101 length
Stainless-steel immersion probe is immersible up to 200 °C and has
15.87 OD x
5 meters
$6,745
adjustable working distance
203 length
Hastelloy C immersion probe with gold gasket for use in process control
15.87 OD x
5 meters
$9,200
applications up to 200 °C and 1500 psi; comes with sapphire window
330 length
5 meters
$8,200
5 meters
$10,200
wavelength; has 7.5-mm focal length
RIP-RPS
RIP-RP2
RIP-RPR-H
and has adjustable working distance
RIP-RPR-S
Stainless-steel immersion probe with elastomeric O-ring seal for use in
15.87 OD x
process control applications up to 200 °C and 1500 psi; comes with
330 length
sapphire window and has adjustable working distance
RIP-RPP
Stainless-steel probe with external optics for process control applications
9.52 OD x
up to 500 °C and 3000 psi; comes with sapphire lens and has short
300 length
working distance
RIP-PA-SH
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Sample holder, with inserts for round vials, square cuvettes, and cups
not applicable
not applicable
$850
For all your sensing needs, visit OceanOptics.com
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Modular Raman Measurement Tools
QE65000 Scientific-grade Spectrometer for Raman
New Scientific-grade Spectrometer
The QE65000 Spectrometer is a unique combination of detector and
optical bench technologies that provides users with high spectral
response and high optical resolution in one package.
Demanding Low Light-level Applications
The QE65000 was designed for low-light level applications
such as Raman spectroscopy. The detector is TE-cooled,
resulting in virtually no dark noise, which allows you to set the
integration time of the spectrometer (analogous to a camera’s
shutter speed) at up to 15 minutes with little spectral distortion.
Quantum Efficiency to 90%
Above, the QE65000
is configured for use with a
LASER-785 and an RIP-RPB
probe (see facing page for
details). At left is the
STAN-RAM785 for determining
the absolute spectral intensity
of your Raman system.
Increased System Sensitivity
NIST-traceable Raman Standards
The STAN-RAM785 and STAN-RAM532 are NIST-certified standards
for determining the absolute spectral intensity of your Raman system.
They consist of an optical glass that emits a broadband luminescence
spectrum when excited with a laser. (Select the STAN-RAM785 when
using a 785 nm laser as your excitation source; select the STANRAM532 when using a 532 nm laser.) The shape of this
luminescence spectrum is expressed by a polynomial equation that
relates the relative spectral intensity to the wavenumber from the
excitation wavelength. Determining the absolute spectral intensity of
your Raman system is essential for those performing peak-to-peak
height analysis and those collecting a spectral library.
QE65000:
$9,999
STAN-RAM532:
$1,015
STAN-RAM785:
$1,015
Examples of QE65000 Configurations for Raman
Sample
Config.
Spectral
Range
Excitation
Source
Grating
p. 28
Slit
p. 27
1
150-4000 cm-1
532 nm laser
H6
10 µm
~8 cm-1
2
150-4000 cm -1
532 nm laser
H6
25 µm
~10 cm -1
3
150-7500 cm -1
532 nm laser
H14
10 µm
~16 cm -1
4
150-7500 cm -1
532 nm laser
H14
25 µm
~19 cm -1
5
150-2100 cm -1
785 nm laser
H6
50 µm
~6 cm -1
6
150-2100 cm -1
785 nm laser
H6
100 µm
~8 cm -1
7
150-3950 cm -1
785 nm laser
H14
50 µm
~13 cm -1
8
150-3950 cm -1
785 nm laser
H14
100 µm
~18 cm -1
Tel: 727.733.2447 • Email: [email protected]
Resolution
(approx.)
Comparing Xylenes Using Raman
40000
35000
Mixed Xylene
30000
INTENSITY
QE65000 system sensitivity is improved because the 2D detector
allows us to take advantage of the height of the entrance slit. In our
spectrometers, you regulate the light entering the bench according to
the slit’s width. Most of our other spectrometers use linear detectors;
in those spectrometers, slit height doesn’t matter because linear
detectors cannot efficiently collect the light from the entire height of
the slit. But with the 2D detector in the QE65000, we can better take
advantage of this additional light.
O-Xylene
25000
20000
15000
10000
5000
0
0
500
1000
1500
2000
2500
3000
3500
4000
RAMAN SHIFT (cm-1)
We used the QE65000 Sample Configuration #3 (described
in the table at lower left), and an InPhotonics probe to
acquire Raman spectra of xylene samples.
Spectrometer Systems & Setups
With its scientific-grade detector, the QE65000 achieves up to 90%
quantum efficiency (defined as how efficiently a photon is converted
to a photoelectron). With this “2D” detector in the QE65000, we bin
a vertical row of 64 pixels, which increases the signal-to-noise ratio
to 1200:1. (See page 26 for detailed QE65000 specifications.)
Specifications
Dimensions:
Detector:
Pixels:
Signal-to-noise ratio:
Dark noise:
Optical bench design:
Focal length:
Entrance aperture:
Gratings:
Integration time:
Dynamic range:
Fiber optic connector:
Power consumption:
Data transfer speed
Inputs/Outputs
Operating systems:
Temperature limits:
Temperature range:
Set point:
Lowest set point:
Stability:
182 mm x 110 mm x 47 mm; 1.05 kg
Hamamatsu back-thinned CCD (page 28)
1024 x 58 (1044 x 64 total pixels)
1000:1 (at full signal)
2.5 RMS counts
f/4, Symmetrical crossed Czerny-Turner
101.6 mm input and 101.6 mm output
5, 10, 25, 50, 100, or 200 µm wide slits (page 27)
14 gratings UV through Shortwave NIR (page 28)
8 milliseconds to 15 minutes
7.5 x 109 (system); 25000:1 for one acquisition
SMA 905 to 0.22 numerical aperture fiber
3 A @ 5 VDC with TE cooling
Full spectrum to memory every 8 ms with USB 2.0
10 onboard digital user-programmable GPIOs
Windows 98/Me/2000/XP, Mac OS X and Linux
when using the USB port
0 °C to 50 °C
13 °C maximum range between high and low
Software controlled
40 °C below ambient, to -15 °C
±0.1 °C of set temperature in <2 minutes
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Raman Measurement Systems
Great Resolution & Stability in a Versatile Package
Raman Systems’ R-3000-series of Raman instruments are fully
integrated analyzers for real-time qualitative and quantitative analysis
of solutions, powders, tablets, gels and surface media from ~2002700 cm-1. The systems include high-performance lasers that provide
excellent resolution and achieve better than 1 cm-1 wavelength
stability and 4% output stability. The R-3000s are used in
pharmaceutical monitoring, petrochemical process control, drug and
explosives detection, and water-quality analysis.
Spectrometer Systems & Setups
Fully Integrated System with New Software
The R-3000’s
stainless steel
sampling tube is
12.7 mm in diameter
and 89 mm in length.
The tube can be any
length up to 254 mm. There
are two focusing caps: one for direct contact with a
sample; the other for use with a sample container.
The R-3000 systems come with a 785 nm or 532 nm solid-state
diode laser; a software-controlled laser shutter; a fiber optic
spectrometer with optional TE cooling; a multi-purpose fiber optic
probe for solutions, solids and powders; focusing and calibration
caps; a sample holder; operating software; and safety goggles. In
addition, the R-3000 systems have new software features that include
fingerprinting and quantification capabilities, and a multiple-spectrum
display function.
Specifications
Lasers:
Raman shift range:
Resolution:
Detector:
Stability:
Power output:
Sampling via:
Remote sampling:
PC interface:
Data storage:
Calibration:
Laser safety:
Tolerances:
Temperature limit:
Solid-state 785 nm or 532 nm diode
~200-2700 cm-1
~10 cm-1 to ~6 cm-1
Linear CCD array; option of cooled detector
1 cm-1 wavelength, 4% output stability
125 mW and 250 mW; software-controlled
Fiber optic probe for solutions, solids, gels
Up to 200 meters using optical fibers
USB
SPC or ASCII format
One-touch calibration
Class 3b laser requires use of safety eyewear
Up to 1500 psi and up to 200 ºC for tube and caps
Up to 80 ºC for probe head and fiber
Versatile Sampling Optics Add Value
The sample tubes and probe "caps" that come with the R-3000
systems provide easy transferability between samples in transparent
containers and in immersion applications. The probe head is coupled
to the spectrometer and laser via two 1-meter fibers (200 µm and
100 µm in diameter).
R-3000-785:
$14,950
R-3000-532:
$18,300
R-3000-HR-532: $19,950
R-3000-QE-532: $23,450
R-3000-QE-785: $21,950
RSL-Plus Handheld Raman System
Small Footprint
The RSL-Plus Handheld Raman Spectrometer is a 12" x 6" system for
performing low-resolution Raman spectroscopy for on-site materials
analysis. Although a high-resolution Raman spectrum provides
detailed information about the vibrational fine structure of sample
molecules, most routine applications need only ~15 cm-1 resolution
for quantitative or qualitative analysis. As a result, a system such as
the RSL-Plus can be assembled using less expensive optics and
lasers -- without sacrificing the power of Raman analysis.
Compact Spectral Matching System
Specifications
Dimensions:
Weight:
Raman shift range:
Resolution:
Laser:
Output power:
Detection via:
Sampling via:
Remote sampling:
Battery:
Computer:
Calibration:
Compliance:
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305 mm x 52 mm x 76 mm
1.72 kg
~200-2700 cm-1
~12 cm-1
Solid-state 785 nm diode
500 mW
Linear CCD-array detector spectrometer
Shuttered probe for solutions, solids, gels, etc.
Up to 200 meters using optical fibers
2-hour rechargeable battery
Embedded PC with spectral-matching software
Self-calibration and automated validation
Compliant with 21CFR Part 11
The RSL-Plus consists of an embedded computer with spectral
matching software for quality control, verification and validation
routines. The system includes a spectrometer, a 785 nm diode laser,
a fiber optic probe, and a 2-hour rechargeable battery.
FDA Compliance
The operating software of the RSL-Plus is compliant with the Food
and Drug Administration’s 21CFR Part 11, and includes features
such as audit logging, database creation, spectral matching, and
automatic detection of data tampering.
RSL-PLUS: $25,000
For all your sensing needs, visit OceanOptics.com
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MMS-Raman Spectrometer
Next-generation Raman Spectroscopy
We've teamed with Centice Corporation to offer next-generation
Raman spectroscopy that combines the simplicity of dispersive
instruments with the multiplex advantage of a transform
spectrometer. The MMS-Raman Spectrometer uses Centice's
patent-pending Multimodal Multiplex Spectroscopy to provide
high-performance Raman analysis for a fraction of the cost of
research-grade systems. The MMS-Raman Spectrometer offers a
unique combination of resolving power, spectral range and
flexibility, making it an ideal system for the routine analysis of
many types of liquids and solids.
How Multimodal Multiplex Spectroscopy Works
Spectrometer Systems & Setups
Dispersive, fixed-grating spectrometer designs typically use a slit
or a fiber as the input into the spectrometer. These apertures
restrict the amount of light that can reach the detector. In these
designs, there is an inherent tradeoff between resolution and light
throughput. While spectral resolution increases as slit width
decreases, a narrow input slit limits the light throughput and,
likewise, measurement sensitivity. In the MMS-Raman
Spectrometer, a wide-area coded aperture takes the place of a
traditional slit entrance that allows 10-1000x greater light
throughput -- and then applies precise algorithms to extract a
high resolution spectrum from the collected light. There is much
more light collected, without sacrificing resolution. Multimodal
Multiplex Spectroscopy instruments are ideal for measuring weak,
scattering and diffuse samples because the spectrometer can
collect and process far more light through its wide-area aperture,
without affecting spectral resolution.
Key Applications
Key applications include material inspection, identification of
unknown materials, and quantitative analysis of both intermediates and final products in the chemical and pharmaceutical
industries. Typical samples include powders, liquids and polymers.
All experimental and parameter set-up options are computercontrolled for increased ease of use, reliability and speed.
Integrated Sample Holder
The MMS-Raman Spectrometer has a sample holder with cover
for operation in full ambient light without affecting performance.
The spectrometer's removable sample compartment is integrated
into the optical path, avoiding inefficiencies associated with
remote compartments. Sample positioning is rapid and precise
using the external z-axis alignment control knob. The sample
compartment is especially useful for measuring measure weak,
scattering and diffuse sources with the highest possible sensitivity.
The sample holder supports up to 10-mm cuvettes and test tubes.
MMS-Raman Delivers Great Sensitivity & Resolution
The MMS-Raman spectrometer samples up to 1,000 optical
channels simultaneously through the large coded aperture. A
mathematical transformation algorithm precisely reconstructs the
spectrum with a 4x signal-to-noise improvement as compared
with a slit-based system equipped with identical source, grating
and detector components, and 70-80x greater than with a fiber
input of equivalent resolution.
MMS-RAMAN:
$19,995
Tel: 727.733.2447 • Email: [email protected]
Specifications
SYSTEM
Wavelength range:
Spectral resolution:
Grating:
Stray light:
Integration time:
A/D resolution:
APERTURE AND DETECTOR
MMS aperture size:
Detector array size:
Number of active pixels:
Pixel size:
Well depth:
Quantum efficiency:
Dark noise:
Readout noise:
Gain:
Detector temperature:
LASER
Excitation wavelength:
Laser power:
SAMPLE CHAMBER
Cuvettes:
Test tubes:
COMPUTER
Interface:
Operating systems:
RAM requirements:
220 cm-1 to 2000 cm-1
~4 cm-1
Transmissive
<0.1%
50 ms to 100 seconds
16-bit
0.58 mm x 2.3 mm
512 x 122 pixels
62,464
24 µm x 24 µm
~300,000 electrons
85% at 250 nm
300 e-/pixel/sec @ 0° C
2 RMS counts, 8 RMS electrons
4.7
To -20 °C below ambient
785 nm
70 mW at sample
Square, up to 10 mm
Up to 17 mm
USB 2.0
Windows XP (with SP2)
12 MB
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LED Measurement Tools
When coupled with the optimum sampling accessories, the
USB4000 Spectrometer is a highly accurate spectroradiometer
for measuring the color, relative power and absolute spectral
intensity of LEDs.
Miniature Fiber Optic Spectrometer
A USB4000 Spectrometer optimized for LED measurements is configured with a 350-1000 nm wavelength
range, a 25 µm entrance aperture and an L4 Collection
Lens to increase light efficiency. With this configuration,
optical resolution is ~1.33 nm (FWHM).
Before measuring the absolute irradiance of your LED,
you need to take a reference spectrum of a calibrated
blackbody energy source. The LS-1-CAL-INT Radiometric
Reference Source was designed for the FOIS-1
Integrating Sphere, our sample chamber for LEDs. The
LS-1-CAL-INT is inserted into the sample port of the
FOIS-1 (at right); optical fiber collects the light from the
FOIS-1 and funnels it to the spectrometer.
LED Power Supply: Secures, Powers & Drives LED
Spectrometer Systems & Setups
The LED-PS Power Supply provides three useful functions:
securing the LED in place, powering the LED, and
displaying the LED’s drive current. Use the adjustable
drive current feature to increase or decrease an LED’s
current up to 50 mA. We offer a standard LED-PS and a
NIST-traceable version.
After taking a reference and a dark
spectrum, insert an LED into the
LED-PS Power Supply, which holds
and powers the LED, displays the
LED drive current, and allows you
to adjust the current. The LED-PS
is placed over the FOIS-1, so that
the LED is inserted into the sample
port of the FOIS-1.
Integrating Sphere: 360° Energy Collection
The LED is powered by the LED-PS and is inserted into
the 9.5-mm diameter port of the FOIS-1 Fiber Optic
Integrating Sphere, which has a 360° field of view. The
P400-2-VIS-NIR Optical Fiber collects the light from the
FOIS-1 and funnels it to the USB4000 Spectrometer.
Light Source: Radiometric Reference Source
The LS-1-CAL-INT is a NIST-traceable light source
designed specifically to calibrate the spectral response of
a spectroradiometric system that uses the FOIS-1 as the
sampling device. It provides known absolute intensity
values at several wavelengths. The LS-1 is used as a
reference for relative power measurements.
Spectral & Color Measurement
Our software provides absolute spectral intensities for
LEDs, and calculates L*a*b*, XYZ, xyz, u'v'w', hue, RGB,
chroma, saturation and more. See page 81 for details.
Spectrometer Specifications
Toshiba TCD1304AP linear CCD array (page 17)
200-1100 nm
3648 pixels, size of 8 µm x 200 µm
130 photons/count at 400 nm;
60 photons/count at 600 nm
Bench design:
f/4, Asymmetrical crossed Czerny-Turner
Focal length:
42 mm input; 68 mm output
Entrance aperture:
5, 10, 25, 50, 100, or 200 µm wide slit or
fiber (page 15)
Grating options:
14 gratings, UV through Shortwave NIR (page 16)
Fiber optic connector: SMA 905 to 0.22 numerical aperture fiber
Wavelength range:
Grating dependent
Optical resolution:
~0.3-10.0 nm FWHM
Signal-to-noise ratio: 300:1 (at full signal)
Dynamic range:
2 x 108 (system); 1300:1 for a single acquisition
Integration time:
3.8 milliseconds to 10 seconds
Stray light:
<0.05% at 600 nm; <0.10% at 435 nm
Power consumption: 250 mA @ 5 VDC
Data transfer speed: Full spectrum to memory every 5 ms with USB 2.0
port, 18 ms with USB 1.1 port
Inputs/Outputs:
Yes, 8 onboard digital user-programmable GPIOs
Operating systems:
Windows 98/Me/2000/XP, Mac OSX and Linux with
USB port; Any 32-bit Windows OS with serial port
In this setup, the LED-PS is on top of the FOIS-1 Integrating Sphere.
A P400-2-VIS-NIR Optical Fiber collects the light energy from the
FOIS-1 and sends it to the spectrometer. Our software reports the
absolute spectral intensities for the LED as well as color values,
photopic data and more.
Detector:
Detector range:
Pixels:
Sensitivity:
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Item
Description
USB4000
Spectrometer ($2,199) with
Page
Price
14
$2,649
$749
25 µm slit ($150), L4 Lens
($150), and DET4-350-1000 with
OFLV-350-1000 filter ($150)
LS-1-CAL-INT
Radiometrically calibrated LS-1
133
FOIS-1
Fiber Optic Integrating Sphere
105
$499
LED-PS-NIST
NIST-traceable LED power supply
104
$749
SpectraSuite
Software for Color and Irradiance
P400-2-VIS-NIR
Optical fiber for connecting
81
$199
144
$120
144
$100
FOIS-1 to USB4000
P200-2-VIS-NIR
Optical fiber for connecting
LS-1-CAL-INT to USB4000
For all your sensing needs, visit OceanOptics.com
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Spectroradiometric Tools
Spectrometer for Light Analysis
Our spectrometers and accessories can be configured easily into spectroradiometric systems for
measuring the absolute or relative irradiance of radiant sources such as flat panel displays, CRTs,
incandescent lamps and the sun. The HR2000+ and HR4000 Spectrometers are designed for
laser analysis (pages 20-21), while the USB4000 (page 14) and the HR4000CG (page 35) are
good general-purpose choices. Working with our Applications Scientists to select and configure the
right spectrometer for your spectroradiometric system is the first step. Once the spectroradiometer
is configured, it’s time to select from several sampling options to complete your system.
Spectrometer Systems & Setups
The FOIS-1 Integrating Sphere collects light from 360° field of view.
The CC-3-UV (attached to a fiber) collects light from 180° field of view.
Fiber Optic Integrating Sphere
The FOIS-1 (at right) is used to collect light from a 360° field of view and funnel it to a
spectrometer via an optical fiber for measuring the spectral properties of emission
sources. Light enters the sphere via a 9.5-mm diameter port and an optical fiber -oriented at 90° to the sample port -- collects the light. For details, see page 105.
FOIS-1:
$499
Cosine Correctors
Our Cosine Correctors collect radiation with a 180° field of view. When used in a fiber
coupled to a spectrometer, they measure light intensity at the surface of the probe. See
page 104 for more.
CC-3-DA: $299
CC-3-UV: $129
The FOIS-1.
NIST-traceable Calibration Standards
Our NIST-traceable Calibration Standards provide you with known absolute intensity
values at the sources' fiber optic sample ports. These sources are strictly for calibrating
the absolute spectral response of your system before measuring the absolute irradiance
of radiant sources. For all your options, see pages 132-133.
LS-1-CAL:
$749
DH2000-CAL: $3,302
CC-3-DA (above left) directly attaches
to a spectrometer while the CC-3-UV
screws onto an optical fiber.
SpectraSuite Spectroscopy Operating Software
SpectraSuite Spectroscopy Operating Software is 32-bit acquisition and display software
for performing a number of functions in measuring the absolute spectral intensity of
emission sources. For more on the software, see pages 80-81.
SpectraSuite:
$199
Tel: 727.733.2447 • Email: [email protected]
The LS-1-CAL.
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NanoCalc Thin Film Analysis System
Analyze Layers from 10 nm in Thickness
The optical properties of thin films arise from reflection
and interference. The NanoCalc Thin Film Reflectometry
System allows you to analyze the thickness of optical
layers from 10 nm to ~250 µm. You can observe a
single thickness with a resolution of 0.1 nm. Depending
on your software choice, you can analyze single-layer or
multilayer films in less than one second and can measure
the thickness and removal rates of semiconductor process
films or anti-scratch coatings, hard coatings and antireflection coatings.
Theory of Operation
Spectrometer Systems & Setups
The two most common ways to measure thin film
characteristics are spectral reflectance/transmission and
ellipsometry. NanoCalc utilizes the reflectance method
and measures the amount of light reflected from a thin
film over a range of wavelengths, with the incident light
normal to the sample surface.
Search by n and k
NanoCalc Software displays a sample interference spectrum, predicted
spectra and up to four layers.
As many as four layers can be specified in a film stack.
The various films and substrate materials can be metallic,
dielectric, amorphous or crystalline semiconductors. The
NanoCalc Software includes a large library of n and k
values for the most common materials. You can edit and
add to this library. Also, you can define material types by
equation or dispersion formulas.
Applications
NanoCalc Thin Film Reflectometry Systems are ideal for
in situ, on-line thickness measurements and removal rate
applications, and can be used to measure the thickness
of oxides, SiNx, photoresist and other semiconductor
process films. NanoCalc Systems measure anti-reflection
coatings, anti-scratch coatings and rough layers on
substrates such as steel, aluminum, brass, copper,
ceramics and plastics.
Item
Wavelength Range
Thickness
Light Source Included
NC-UV-VIS-NIR
250-1100 nm
10 nm-70 µm
Deuterium and Tungsten Halogen
NC-UV-VIS
250-850 nm
10 nm-20 µm
Deuterium and Tungsten Halogen
NC-VIS-NIR
400-1100 nm
50 nm-100 µm (optional 1 µm-250 µm)
Tungsten Halogen
NC-VIS
400-850 nm
50 nm-20 µm
Tungsten Halogen
NC-NIR
650-1100 nm
70 nm-70 µm
Tungsten Halogen
NC-NIR-HR
700-978 nm
1 µm-250 µm
Tungsten Halogen
NC-512-NIR
900-1700 nm
50 nm-200 µm
High-power Tungsten Halogen
Specifications
Angle of incidence:
Number of layers:
Reference measurement needed:
Transparent materials:
Transmission mode:
Rough materials:
Measurement speed:
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90°
4 or fewer
Yes (bare substrate)
Yes
Yes
Yes
100 milliseconds to 1 second
On-line possibilities:
Mechanical tolerance (height):
Mechanical tolerance (angle):
Microspot option:
Vision option:
Mapping option:
Vacuum possibilities:
Yes
With new reference or collimation (74-UV)
Yes, with new reference
Yes, with microscope
Yes, with microscope
6" and 12" XYZ mapping tables
Yes
For all your sensing needs, visit OceanOptics.com
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SpecEl Ellipsometer System
Full Spectral Range in Easy-to-use System
Measure refractive index, absorbance and thickness of substrates
with the touch of a button! The SpecEl-2000-VIS Ellipsometer
from Mikropack measures polarized light reflected from the
surface of a substrate to determine the thickness and refractive
index of the material as a function of wavelength. The SpecEl is
controlled via a PC.
All-in-one Accurate System
The SpecEl houses an integrated light source, a spectrometer and
two polarizers fixed to 70°. It also includes a PC with a 32-bit
Windows operating system. The SpecEl can detect a single layer
as thin as 0.1 nm and up to 5 µm thick. In addition, it can
provide refractive indices to 0.005° over lambda.
SpecEl Software and “Recipe” Files
Specifications
Wavelength range:
Optical resolution:
Accuracy:
Angle of incidence:
Film thickness:
Spot size:
Sampling time:
Kinetic logging:
Mechanical tolerance:
Number of layers:
Reference:
450-900 nm
4.0 nm FWHM
0.1 nm thickness; 0.005% refractive index
70°
from 0.1 to 8000 nm for single transparent film
2 mm x 4 mm (standard) or 200 µm x 400 µm (optional)
5-15 seconds (minimum)
5 seconds
Height ± 1 mm, angle ± 1.0°
Up to 32 layers
Not applicable
This screen from the SpecEl Software demonstrates the Psi and Delta
values you can calculate for thickness, refractive index and absorbance.
PlasCalc Plasma Monitoring & Control
Real-time, Full-spectral Plasma Monitoring
PlasCalc-UV-NIR measures plasma emission from 200-1100 nm
in only three milliseconds. The PlasCalc benefits from advanced
process control systems and sophisticated algorithms for data
acquisition.
Spectrometer Systems & Setups
In SpecEl Software, you can configure and save experiment
method files for one-step analysis. After creating a “recipe,” you
can select the recipe to execute the experiment.
Recipe Editor
The Recipe Editor tool allows you to easily and rapidly configure,
build and save experiment methods. It is easy to build robust
recipes for the most difficult plasma processes such as measuring
film deposition, monitoring plasma etching, examining surface
cleaning, analyzing plasma chamber health control, and
monitoring abnormal pollution or discharge phenomena.
Multiple Tools for Easy Plasma Diagnosis
The Integrated Formula Editor provides easy access to a full range
of mathematical and algorithmic functions. An Emission
Wavelength Library provides species identification, while the
Wavelength Editor allows you to optimize signal-to-noise. A dualwindow interface shows the actual spectrum and all process
control information.
Tel: 727.733.2447 • Email: [email protected]
Specifications
Spectral range:
Optical resolution:
D/A-converter:
Digital inputs/outputs:
Analog output:
Interface:
Power consumption:
Power requirements:
Dimensions:
Weight:
200-1100 nm
1.0 nm FWHM
14 bit
8 x TTL digital inputs/outputs
4 x [0-10V]
USB 1.1
12 VDC @ 1.25 A
90-240 VAC 50/60 Hz
257 mm x 152 mm x 263 mm
5 kg
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Transmission of Optics Tools
We offer all of the components you need for measuring the
transmission of optics. Listed below is a sample order that
specifies an HR4000 High-resolution Spectrometer
configured with our novel HC-1 Composite Grating,
which provides a 200-1050 nm wavelength range.
In addition, we suggest a DT-MINI-2 Deuterium
Tungsten Halogen Source, plus fibers,
collimating lenses and a lens fixture for
sampling.
HR4000 with 200-1050 nm
Wavelength Range
Spectrometer Systems & Setups
The HR4000 configuration we
recommend for this application
includes a new 3648-element
CCD-array detector, the proprietary
HC-1 Composite Grating and an
order-sorting filter to provide a
200-1050 nm wavelength range
(best efficiency) and optical resolution
better than 1.0 nm (FWHM). We also suggest a
25 µm entrance slit and a UV2 Detector Upgrade to
enhance performance in the UV. The HR4000 interfaces to a PC via a
USB 2.0 port.
Spectrometer Specifications
Broad Spectral Range Light Source
The DT-MINI-2 Deuterium Tungsten Halogen Light Source combines
the continuous spectrum of a deuterium UV light source and a
tungsten halogen VIS-NIR light source in a single optical path. The
combined-spectrum source produces stable spectral output from
~200-2000 nm in a compact package.
Holder for a Variety of Samples
The 74-ACH Adjustable Collimating Lens Holder consists of adjustable
bars with several threaded holes for collimating lenses. The bars can
be set to accept samples up to ~100 mm thick, making the 74-ACH a
convenient option for transmission measurements of large samples.
Collimating Lenses
The 74-UV Collimating Lenses screw into the threaded holes of the
74-ACH to collimate light. The lenses have an inner barrel threaded
for attaching to optical fibers. When focused for collimation, beam
divergence is 2° or less. The inner barrel can slide relative to the lens
fixture to adjust the focus.
Optical Fiber
Our fiber assemblies can act as both illumination and read fibers. The
two 600 µm diameter optical fibers recommended are one meter in
length and connect easily from the collimating lenses installed in the
74-ACH to the HR4000 Spectrometer and the light source.
Quantity
Dimensions:
Weight:
Power consumption:
Detector:
148.6 mm x 104.8 mm x 45.1 mm
570 g
450 mA @ 5 VDC
3648-element linear CCD array
(page 24)
Wavelength range: 200-1100 nm, 200-1050 best efficiency
Optical resolution:
~1.0 nm FWHM
Grating:
HC-1, 300 lines per mm grating
(page 23)
Entrance aperture: 25 µm wide slit (page 22)
Order-sorting filters: Installed OFLV-200-1100 (page 24)
Focal length:
f/4, 101 mm
Dynamic range:
2 x 108 (system); 2000:1 for
a single acquisition
Stray light:
<0.05% at 600 nm;
<0.10% at 435 nm
Data transfer rate:
Full spectrum into memory every
4 ms with USB 2.0; 18 ms with
USB 1.1
Operating systems: Windows 98/Me/2000/XP,
Mac OS X and Linux when using
the USB port; any 32-bit Windows
operating system when using
the serial port
Inputs/Outputs:
10 digital user-programmable GPIOs*
Analog channels:
One 13-bit analog input and
one 9-bit analog output
* Programming the GPIOs requires SpectraSuite,
OmniDriver or another one of our device drivers. See
pages 80-82 for details.
Item
Description
1
HR4000
HR4000 ($3,999) with HC-1 Composite Grating ($600); 25 µm slit ($150); DET4-200-1100
Page
Price
21
$5,149
1
DT-MINI-2
Miniature Deuterium Tungsten Halogen Light Source
1
74-ACH
Adjustable Collimating Lens Holder
125
89
$1,499
2
74-UV
Collimating Lens
88
$318
2
P600-1-SR
600 µm diameter optical fiber in 1-meter length
144
$238
Detector with OFLV Order-sorting Filter and UV4 Detector Upgrade ($400)
TOTAL:
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$299
$7,503
For all your sensing needs, visit OceanOptics.com
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Spectrometer Accessories
Spectral Hyper Adapter for Picometer Resolution
Examples of Resolution Improvements
Slit
5 µm
Specifications
Grating
Starting
Wavelength
Wavelength
Range
Resolution
no SHA-1
Resolution
with SHA-1
H11
700 nm
700-791 nm
0.05 nm
0.004-0.006 nm
550 nm
550-615 nm
0.035 nm
0.003-0.004 nm
(1800 mm-1)
5 µm
H12
or 4.0-6.0 pm
(2400 mm-1)
or 3.0-4.0 pm
Breakout Box
For easier access to a variety of functions found in the HR4000,
specify the HR4-BREAKOUT, a passive module that separates the
signals from its 30-pin port to an array of standard connectors and
headers. The Breakout Box allows multiple interfaces to a
spectrometer, such as:
External triggering
General Purpose Inputs/Outputs (GPIO)
RS-232 interface
Light sources
Analog Inputs/Outputs
Dimensions:
Wavelength range:
Fiber size:
Integration time:
Optical resolution:
40.6 mm x 68.6 mm x 68.6 mm
550-900 nm
50 µm diameter optical fiber
2 seconds (minimum)
7x-10x improvement; see table
at left for examples
Optical throughput: 10-25%, specify throughput required
The Breakout Box includes a 30-pin
HR4000-CBL-BB Ribbon
Cable that connects the
Box to the spectrometer.
Spectrometer Systems & Setups
Get even higher spectral resolution from your
spectrometer with the SHA-1 Spectral Hyper Adapter
from Ocean Optics partner Spectral Applied
Research. The SHA-1 Spectral Hyper Adapter further
improves the optical resolution of the already highperformance HR4000. Increased resolution is
achieved by plugging the SHA-1 into a setup
between the sampling device and the HR4000. The
SHA-1 plugs directly into the HR4000’s 30-pin
connector and connects to the HR4000’s optical
bench via the included 50-µm optical fiber.
Commands are transmitted via the USB port and
data acquisition is synchronized with the HR4000. The table below
gives examples of the improvement in optical resolution the SHA-1
provides for certain HR4000 configurations.
SHA-1: $5,000
In addition to the accessory connector, the Breakout Box features a
circuit board based on a neutral breadboard pattern that allows
custom circuitry to be prototyped on the board itself. The Breakout
External
GPIO
Box receives its power from the spectrometer, which runs off of a PC Trigger
RS-232
via a USB port, or requires a separate 5-volt power supply when the
Light Source
spectrometer interfaces to a PC via the serial port. If you are wiring
Accessory
Analog I/O
custom circuitry on the Breakout Box, you likely will need the USBThis enlarged photo of the Breakout Box shows the connectors
CBL-PS power supply (purchased separately).
The Breakout Box can be used with the following spectrometers:
USB4000 Spectrometers Plug-and-Play Spectrometers (page 14)
HR4000 High-resolution Spectrometers (page 21).
HR2000+ High-speed, High-resolution Spectrometer (page 20)
QE65000 Scientific-grade Spectrometer (page 26)
HR4-BREAKOUT:
$199
USB-CBL-PS:
$25
Tel: 727.733.2447 • Email: [email protected]
available. Below is an example of a setup with the HR4000 and
Breakout Box.
61
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Cables, Adapters, Power Supplies & More
Enclosures & Cases for Spectrometers & Accessories
Item
Description
BOX-DESKTOP
Desktop Box Enclosure, 3U x 42HP, up to 7 slots
Price
$825
BOX-DUAL
Dual Box Enclosure, 153 x 105 x 66 mm
$350
BOX-DUAL-CE
Dual Box Enclosure, 153 x 105 x 66 mm, CE Approved
$450
BOX-RACK
Rack Mount Box Enclosure, 3U x 84HP, up to 14 slots
$900
BOX-SINGLE
Single Box Enclosure, 143 x 104 x 40 mm
$350
BOX-SINGLE-CE
Single Box Enclosure, 143 x 104 x 40 mm, CE Approved
$550
SPEC-CADDY
Rugged, water-tight case for spectrometers and accessories
$150
SPEC-CADDY
Adapters and Cables
Item
Description
USB-CBL-1
Cable connects from USB port on USB-enabled Spectrometers to USB port
Price
$25
on computer; included with purchase of USB-enabled Spectrometers
USB-ADP-PC
Cable and adapter block to connect from serial port on spectrometer to serial
$75
Spectrometer Systems & Setups
port on computer; comes with USB-CBL-PS power supply
USB-ADP-PC-E
European version of the USB-ADP-PC
USB-CBL-PS
5 VDC Power Supply for spectrometers in serial mode
$50
$25
USB-ADP-DT2
Adapter for directly attaching the USB-DT Light Source to the USB4000
$75
USB-ADP-PX2
Adapter block and cable to connect PX-2 Pulsed Xenon Lamp (page 127),
$50
DT-MINI (page 125) or LS-450 Blue LED (page 130) to the USB4000
HR4-CBL-DB15
HR4000 DB15 Accessory cable
$25
CBL-PX-2
Cable for connecting PX-2 to S2000 Spectrometer
$25
CBL-SER
Serial Cable, 9-pin
$25
Power Supplies*
USB-CBL-PS
Power Supply
USB-ADP-DT2
Item
Description
WT-12V
Regulated 12 VDC Power Supply (1.5A, 110/220 VAC)
Price
WT-12V-R-E
Regulated 12 VDC Power Supply (2.5 A, 220 V)
WT-12V-E
12 VDC Power Supply (800 mA, 220 V)
USB-BP
Lithium Ion Battery Pack has two lithium ion cells; provides 8 hours of power
USB-ADP-PX2
$25
$100
$20
$499
to a USB2000 or USB4000 Spectrometer; comes with charger; charges in
3 hours with the included charger; delivers 2 amp-hours at 5 volts
* Each Ocean Optics Sales, Service & Support location sells power supplies that best serves its region.
Device Control
USB-BP
Item
Description
Price
ACC-CON-US4
Accessory connector for external triggering for USB4000 Spectrometers
ACC-CON-US2
Accessory connector for external triggering for USB2000 Spectrometers
Free
HR4-BREAKOUT
A passive module that allows control of a variety of spectrometer functions such
$199
Free
as external triggering, GPIOs and light sources; includes USB4-CBL-BB Ribbon
Cable to interface to the spectrometer (see page 61 for details)
FIRMWARE-FLG
Gating Firmware Upgrade for USB2000s
PX-2-FIRMWARE
USB2000 or USB4000 programmed for use with PX-2
$250
Free
USB2000-O2CODE
Stand-alone Oxygen Firmware for USB2000
$499
USB-AOUT
4-20 mA Analog Output Module for USB2000 and USB4000 Spectrometers
$499
Extended Warranty and Annual Service Packages
ACC-CON-US2
Item
Description
ASP
Extends the standard warranty from 1 year to 2 years. Price is per spectrometer channel.
Price
$250
ASP-ES
A 1-year warranty package available to customers whose original warranty has expired.
$300
HR4-BREAKOUT
Price is per spectrometer channel.
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ASP-NIR
Extends the standard warranty on NIR Spectrometers from 1 year to 2 years.
ASP-QE
Extends the standard warranty on QE Spectrometers from 1 year to 2 years.
$750
ASP-R
1-year renewal option for holders of expiring ASPs; price is per channel.
$250
ASP-R-E
2-year renewal option for holders of expiring ASPs; price is per channel.
$350
62
$1,000
For all your sensing needs, visit OceanOptics.com
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Optical Sensors
Overview
65
Oxygen Sensor Operation
66
Oxygen Sensor Spectrometers
67
Oxygen Sensor Phase Fluorometer
68
Oxygen Sensor Formulations
69
Oxygen Sensor Care & Compatibility
70
Oxygen Sensor Probes
72
Oxygen Sensor Accessories
74
Oxygen Sensor Temperature
Compensation
75
Sensor Software
75
Pocket Carbon Monoxide Meter
76
Fiber Optic pH Sensors
76
Phenol Red pH Test Kit
Optical Sensors
64
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Overview: Optical Sensors
Optical Sensors
Sensors for Real-Time, In Situ Analyte Monitoring
Ocean Optics has
combined its expertise in
miniature fiber optic
spectroscopy with
advances in materials
science to develop an
innovative line of modular
fiber optic chemicalsensing systems.
Sensors are
constructed by placing a
transducer material at the
tip of an optical fiber.
These materials change
optical properties in
response to specific
analytes in their
immediate environment.
Our transducer
materials include both
fluorescence-based and
Optical sensors can be used for a variety of applications. Here,
absorbance-based
our “R” Optic Oxygen Sensor monitors oxygen in a liquid.
indicators. These
indicators are immobilized
or trapped in a variety of proprietary materials, including sol-gels, hydrophobic
and hydrophilic polymers, and cellulose acetate. Materials can be coated on flat
substrates such as optical fibers, optical flats, cuvettes and other containers.
We produce components that can be used to monitor oxygen or pH in
biological samples, headspace gases, slurries, cosmetics, foods, gases and
liquids in natural environments.
Optical O2 Sensors vs. Electrodes
Commercial Electrodes
Polarographic electrodes can be
affected by changes in pH, salinity and
ionic strength of the environment
Sensors are immune to environmental
changes in pH, salinity and ionic
strength
Electrochemical electrodes are subject
to interference from a number of
substances and sampling conditions
Sensors are immune to interference
from moisture, carbon dioxide, methane
and other substances
Electrodes can have a response time of
1.5 minutes, depending on temperature
Sensors response time is <1 second
for dissolved O2 and O2 gas
Electrodes have a typical lifetime of
3 months
Sensors have a long life – more than
1 year
Sensors do not consume oxygen,
allowing for continuous contact with
sample
Electrodes can consume oxygen of
~0.1 micrograms/hour
The temperature range for some
electrodes is 0-45 °C
Electrodes often introduce electrical
currents into a sampling setup
Calibration may be needed hourly
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Fiber Optic Oxygen Sensors
Most electrodes are designed for use in
gas or liquids, but not both media
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Sensors measure both oxygen gas and
dissolved oxygen in gases and liquids
Ocean Optics Offers Optical
Sensor Coating Services
Our optical-sensor coating services
provide OEMs and product developers
with multiple solutions in creating
proprietary products for chemical
sensing applications. You can take
advantage of these services to develop
and manufacture a variety of custom
optical oxygen and pH sensor
accessories including fiber optic probes,
cuvettes, Petri dishes, microscope slides
and more. The added services include
the licensing of Ocean Optics
proprietary oxygen and pH coating
technologies, custom sensor coating
development, and contract
manufacturing services.
We can supply our proprietary optical
sensor coating technologies to you
through a license agreement. We
manufacture the coatings and apply
them to any media specified.
You can supply a proprietary indicator
to be included in an Ocean Optics
coating. We then produce the coating
and apply it to the media specified.
You can supply a proprietary coating
and indicator to us and we will apply
the coating to the media specified. This
option requires a contract agreement.
We can research and develop a
proprietary coating for you. This option
is available through NRE and/or
research fees.
Services may also include costs
associated with the type of sensor
material; the surface area; and the time
required to apply the sensor material to
a substrate.
Frequent calibration is unnecessary
Sensor probe temperature range is
-60 °C to +80 °C
Sensors allows remote sampling without
introducing electrical fields to sample
For all your sensing needs, visit OceanOptics.com
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Oxygen Sensor Operation
Our Fiber Optic Oxygen Sensors are coated probes that use fluorescence quenching to measure the partial pressure
of dissolved or gaseous oxygen. You specify a sensor probe with one of our three sensing formulations -- along with
a sensing detector, excitation source and software -- to build a complete system that typically works like this:
1. An LED sends excitation light to one leg of a bifurcated
optical fiber assembly.
2. The fiber carries the light to the oxygen probe, which is
polished to a 45° angle. The distal end of the probe tip
consists of sensor formulation trapped in a sol-gel matrix,
immobilized and protected from the sample. FOXY and
HIOXY sensors use a ruthenium formulation, while FOSPOR
sensors use a Pt-porphyrin formulation.
3. The light from the LED excites the ruthenium or porphyrin
sensor formulation at the probe tip. The excited complexes
fluoresce, emitting energy at ~600 nm and 650 nm,
respectively.
Oxygen Sensor with MFPF100-1
MultiFrequency Phase Fluorometer
4. If the excited complex at the probe tip encounters an oxygen
molecule, the excess energy is transferred to the oxygen
molecule in a non-radiative transfer, decreasing or quenching
the fluorescence signal. The degree of quenching correlates
to the partial pressure of oxygen in the sol-gel, which is in
dynamic equilibrium with oxygen in the sample.
5. The fluorescence is collected by the probe and carried to the
USB4000-FL Spectrometer or MFPF Fluorometer via the
second leg of the bifurcated optical fiber assembly. The
fluorescence intensity (for USB4000-FL Spectrometer) or
phase (for MFPF Fluorometer) is measured and related to the
partial pressure of oxygen through the Stern-Volmer equation.
Oxygen Sensor with USB4000-FL
Spectrofluorometer
USB4000-FL connected
to a USB-LS-450
MFPF100-1
QBIF600-VIS-NIR
USB-LS-450-TP
21-02
Splice Bushing
FOXY-R
21-02
Splice Bushing
FOXY-R
Overview
Overview
Oxygen is sensed by measuring the phase shift of
fluorescence of a fluorophore bound to the tip of an optical
fiber. The sensor responds to the partial pressure of
oxygen. Below is a list of components typically specified in
an oxygen sensing application with a MultiFrequency Phase
Fluorometer (MFPF) as the sensor detector.
Oxygen is sensed by measuring the decrease in
fluorescence intensity of a fluorophore bound to the tip of
an optical fiber. The sensor responds to the partial
pressure of oxygen. It works equally well in gases, solutions
and even viscous samples. Below is a list of components
typically specified in an oxygen sensing application.
MultiFrequency Phase Fluorometer
Spectrometer
The MultiFrequency Phase Fluorometer (MFPF) is a flexible
platform for measurement of luminescence lifetime, phase
and intensity. The MFPF is especially useful for oxygen
sensing applications where sensitivity to drift is important
and where sample set-ups must be undisturbed for long
periods of time. Because it utilizes phase-shift technology, it
is invariant to fiber bending and stray light and has a wide
dynamic range of optical intensity as well as low optical
and electronic crosstalk, and low drift and phase noise.
We recommend the USB4000-FL Fluorescence
Spectrometer for general purpose oxygen measurements.
The USB4000-FL is preconfigured with a 200 µm Slit,
Grating #3 and a 360-1000 nm wavelength range.
Grating #3 is blazed at 500 nm to optimize the
fluorescence signal at 600 nm. Also included in the optical
bench is an L4 Detector Collection Lens to increase lightcollection efficiency.
Optical Sensors
QBIF600-VIS-NIR
USB-LS-450-TP
Sampling Optics
Sampling Optics
This compact, self-contained frequency-domain luminescence monitor uses included red and blue LED excitation
light that transmits to one leg of a QBIF600-VIS-NIR
Bifurcated Optical Fiber Assembly, which is connected to
one of our oxygen sensor probes, such as the FOXY-R, via
a 21-02 Splice Bushing.
Tel: 727.733.2447 • Email: [email protected]
The USB-LS-450 Pulsed Blue LED Excitation Source
transmits light (at ~475 nm) to one leg of a
QBIF600-VIS-NIR Bifurcated Optical Fiber Assembly, which
is connected to one of our oxygen sensor probes, such as
the FOXY-R, via a 21-02 Splice Bushing.
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Oxygen Sensor Spectrometers
Preconfigured Spectrometers for Use with Sensors
Our high-sensitivity, preconfigured fluorescence spectrometers -- the USB4000-FL,
USB4000-FL-450 and USB4000-FL-395 -- were conceived for use with fluorescencebased sensors. Each fluorescence unit is set to 360-1000 nm and comes with a 200-µm
entrance aperture and an L4 Detector Collection Lens for increased light throughput.
USB4000-FL: Excitation Source not Included
The USB4000-FL does not come with an excitation
source, which you will need to excite the sample. We
have a series of compact, low-cost excitation sources
that work with our fluorescence-based sensors such as
the LS-450 (at right) or the USB-LS-450 (see pages 130-131).
The excitation sources produce pulsed or continuous output and easily couple
to our line of spectrometers, optical fibers and other accessories.
USB4000-FL-450 & USB4000-FL-395: Excitation Source Included
Optical Sensors
The USB4000-FL-450 and USB4000-FL-395 Spectrofluorometers are spectrometers
configured the same way as the USB4000-FL, but each comes with a direct-attach
excitation source. The USB4000-FL-450 comes with a 470 nm LED Excitation source
and the USB4000-FL-395 comes with a 395 nm LED Excitation source. The 470 nm LED
is great for exciting the FOXY and HIOXY formulations, while the 395 nm LED is used
for exciting the FOSPOR formulation. In addition, these Excitation sources connect to
temperature sensors and contain onboard memory that can be programmed to store
temperature and oxygen calibration coefficients.
USB4000-FL:
$2,499
USB4000-FL-450: $3,049
USB4000-FL-395: $3,049
Specifications
PHYSICAL
Dimensions:
Weight:
DETECTOR
Detector:
OPTICAL BENCH
Design:
Focal length:
Entrance aperture:
Grating:
Fiber optic connector:
SPECTROSCOPIC
Wavelength range:
Optical resolution:
Signal-to-noise ratio:
A/D resolution:
Dark noise:
Stray light:
Corrected linearity:
ELECTRONICS
Power consumption:
Data transfer speed:
Inputs/Outputs:
COMPUTER
Operating systems:
Computer interfaces:
Peripheral interfaces:
LIGHT SOURCE
Stability:
Wavelength range:
Power consumption:
Power output:
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USB4000-FL
USB4000-FL-450
USB4000-FL-395
89.1 mm x 63.3 mm x 34.4 mm
190 grams
89.1 mm x 120.3 mm x 34.4 mm
310 grams
89.1 mm x 120.3 mm x 34.4 mm
310 grams
Toshiba TCD1304AP linear CCD array
(see page 17 for detector specifications)
Toshiba TCD1304AP linear CCD array
(see page 17 for detector specifications)
Toshiba TCD1304AP linear CCD array
(see page 17 for detector specifications)
f/4, Asymmetrical crossed Czerny-Turner
42 mm input; 68 mm output
200 µm wide slit
Grating #3, groove density of 600 lines
set to 360-1000 nm, blazed at 500 nm
SMA 905 to 0.22 numerical aperture fiber
f/4, Asymmetrical crossed Czerny-Turner
42 mm input; 68 mm output
200 µm wide slit
Grating #3, groove density of 600 lines
set to 360-1000 nm, blazed at 500 nm
SMA 905 to 0.22 numerical aperture fiber
f/4, Asymmetrical crossed Czerny-Turner
42 mm input; 68 mm output
200 µm wide slit
Grating #3, groove density of 600 lines
set to 360-1000 nm, blazed at 500 nm
SMA 905 to 0.22 numerical aperture fiber
360-1100 nm
~10.0 nm FWHM
300:1 (at full signal)
16 bit
50 RMS counts
<0.05% at 600 nm; <0.10% at 435 nm
>99.8%
360-1100 nm
~10.0 nm FWHM
300:1 (at full signal)
16 bit
50 RMS counts
<0.05% at 600 nm; <0.10% at 435 nm
>99.8%
360-1100 nm
~10.0 nm FWHM
300:1 (at full signal)
16 bit
50 RMS counts
<0.05% at 600 nm; <0.10% at 435 nm
>99.8%
250 mA @ 5 VDC
Full spectrum to memory every 4 ms with
USB 2.0 port, 18 ms with USB 1.1 port
Yes, 8 digital user-programmable GPIOs
250 mA @ 5 VDC and 60 mA @ 5 VDC
Full spectrum to memory every 4 ms with
USB 2.0 port, 18 ms with USB 1.1 port
Yes, 8 digital user-programmable GPIOs
250 mA @ 5 VDC and 60 mA @ 5 VDC
Full spectrum to memory every 4 ms with
USB 2.0 port, 18 ms with USB 1.1 port
Yes, 8 digital user-programmable GPIOs
Windows 98/Me/2000/XP, Mac OS X
and Linux with USB port; Any 32-bit
Windows OS with serial port
USB 2.0 @ 480 Mbps; RS-232
(2-wire) @ 115.2 K baud
I2C inter-integrated circuit; SPI (3-wire)
Windows 98/Me/2000/XP, Mac OS X
and Linux with USB port; Any 32-bit
Windows OS with serial port
USB 2.0 @ 480 Mbps; RS-232
(2-wire) @ 115.2 K baud
I2C inter-integrated circuit; SPI (3-wire)
Windows 98/Me/2000/XP, Mac OS X
and Linux with USB port; Any 32-bit
Windows OS with serial port
USB 2.0 @ 480 Mbps; RS-232
(2-wire) @ 115.2 K baud
I2C inter-integrated circuit; SPI (3-wire)
n/a
n/a
n/a
n/a
± 1.0% drift after 2-minute warm-up period
460-490 nm
60 mA @ 5 VDC
60 µW (minimum) into a 600 µm fiber
± 1.0% drift after 2-minute warm-up period
380-410 nm
60 mA @ 5 VDC
60 µW (minimum) into a 600 µm fiber
For all your sensing needs, visit OceanOptics.com
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Oxygen Sensor Phase Fluorometer
Flexibility in Luminescence Measurement
USB Cable connects
MFPF to a computer.
MFPF Power Supply
Used with Ocean Optics Fiber Optic Oxygen Sensors
and custom probes, the MultiFrequency Phase
Fluorometer (MFPF), manufactured by TauTheta, is a
flexible platform for measurement of luminescence
lifetime, phase and intensity. This compact, selfcontained frequency-domain luminescence monitor uses
LED excitation and avalanche photodiode detection with
filter-based wavelength selection for easy
experimental setup and control.
MFPF100-1
One-channel
MultiFrequency
Phase
Fluorometer
Perfect System for O2
Sensing
USB-LS-450-TP
Temperature Sensor
21-02 Splice Bushing
Optical Sensors
The MFPF is especially useful
for oxygen sensing
QBIF-600-VIS-NIR Bifurcated
applications where sensitivity
Optical Fiber Assembly
to drift is important and where
sample setups must be
undisturbed for long periods of
time. Because it utilizes phase-shift
technology, it is invariant to fiber
bending and stray light and has a wide dynamic range
of optical intensity as well as low optical and electronic
crosstalk, and low drift and phase noise. Auxiliary
pressure and temperature measurements make the
MultiFrequency Phase Fluorometer an ideal choice for
luminescence sensor design, testing and calibration.
FOXY-R Oxygen Sensor Probe
Application Flexibility
The MultiFrequency Phase Fluorometer can be use in
applications such as:
Luminescent materials characterization
Phase/Lifetime sensor development
Calibration of phase/lifetime sensors
Stability and photodegradation studies
Characterization of phase shift over frequency
Oxygen consumption measurement on cell and
islet cultures
Various Oxygen
Sensor Probes
Configuration Options
The MFPF can be configured with two-channel LED
excitation and detection and modulation frequencies to
500 kHz. This configuration will give you lifetime
measurements from 200 µsec down to 0.3 µsec. The
onboard pressure transducer measures atmospheric
pressure or external pressure with a 1/4” hose fitting.
The single-channel MFPF100-1 comes with one
thermistor, and the two-channel MFPF100-2 includes
two thermistors. The thermistor option allows
temperature logging, calibration and temperature
correction.
USB Connection for Easy Startup
The MultiFrequency Phase Fluorometer can connect to
your PC via an RS-232 or USB connection and saves
your data in an easy-to-use Excel format.
MFPF100-1 (one channel): $5,000
MFPF100-2 (two channels): $7,500
Tel: 727.733.2447 • Email: [email protected]
Specifications
LED modulation range: 2 kHz to 100 kHz (200 µsec to 0.3 µsec)
Parameters measured: Luminescence phase shift, AC luminescence intensity,
temperature (optional through external thermistors), pressure
(via onboard pressure transducer)
Control software:
Windows 2000/XP control software with data logging capability;
controls include: modulation frequency, data rate, LED duty
cycle, signal averaging, APD gain, analog gain, LED intensity
Measurement modes: Intermittent LED (to minimize photodegradation); Continuous
LED (for rapid measuring and accelerating photo-bleaching);
Frequency sweep for luminescence characterization
Thermistor probes:
Closed end stainless steel tube with thermistor sensor mounted
in tip; liquid immersible rugged design; 1/8” NPT fitting;
temperature range 0 to 75 °C, absolute maximum 100 °C
+/- 0.2 °C; Interchangeable thermistors
Pressure measurement: Onboard pressure transducer monitors atmospheric pressure,
optional configuration allows external connection for 0 to 15 psiA
Power input:
6v - 12v, 1.5 Amps
Communications:
USB or RS-232
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Oxygen Sensor Formulations
By combing miniature fiber optic spectrometers, excitation sources and optical probes coated with
chemically sensitive transducers, Ocean Optics has created an extensive line of fiber optic oxygen
sensors. Sensors are constructed by placing a transducer material -- typically, a dye embedded in a sol
gel -- at the tip of an optical fiber. These materials change optical properties in response to specific
analytes in their immediate environment. The sensor uses fluorescence quenching of the indicator dye
to measure the partial pressure of dissolved or gaseous oxygen.
Optical Sensors
FOXY
Sensor Formulation
HIOXY
Sensor Formulation
General-purpose Oxygen Sensors
High-sensitivity Coating
Hydrocarbon Environments
Our Oxygen Sensing Probes with the
FOXY Formulation are designed for
monitoring partial pressure of oxygen in
benign gases, liquids and gels. Standard
FOXY probe tips are covered with a layer
of hydrophobic sol-gel material with a
ruthenium compound trapped in the solgel matrix. When excited by an LED, the
ruthenium complex fluoresces. If the
excited ruthenium complex then
encounters an oxygen molecule, the
excess energy quenches the fluorescent
signal. The fluorescence intensity or phase
shift is measured by an Ocean Optics
spectrometer or MFPF system, and is
related to the partial pressure of oxygen.
Our FOSPOR sensor coating for
Oxygen Sensor Probes is a highly
sensitive sol-gel thin film immobilized
with Pt-porphyrin, a fluorescent dye
with high quantum efficiency and low
non-specific adsorption on different
surfaces. FOSPOR-coated sensors are
capable of monitoring low levels of
oxygen in gas (to ppm) and dissolved
oxygen in liquids (to ppb), making
them especially useful for measuring
trace amounts of oxygen in vacuum
systems and in food and
pharmaceutical packaging.
We’ve developed a high-performance
oxygen sensor compatible with
hydrocarbon environments. Our new
HIOXY formulation is a hydrophobic and
oleophobic coating material encapsulated
with oxygen-sensitive luminescence
molecules. The HIOXY sensor is designed
for monitoring oxygen in non-aqueous
vapors and solutions. The sensor coating
chemistry is ideal for use with oils,
alcohols and hydrocarbon-based vapors
and liquids. HIOXY has been tested
successfully in commercial and military
aviation fuels, gasoline, diesel, some
alcohols, glycol, military hydraulic fluids
and various wines.
Specifications
Specification
Principle:
Sensor mechanism:
Applications:
Time-constant (µsec) dynamic range:
Accuracy: (0-20% O2, 0-50 ºC):
Response time of probe with no overcoat:
Response time of dissolved oxygen in
liquid (with overcoat):
Response time of probe with overcoat of
Oxygen Gas (at 1 atmosphere):
Dynamic range of dissolved oxygen in
liquid:
Dynamic range of oxygen gas (at
1 atmosphere):
Stability dissolved oxygen in liquid:
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FOSPOR
Sensor Formulation
FOXY Probes
Photoluminescence-quenching using Ru
compound. Measures O2 partial pressure.
Phase shift due to change in partial
pressure of O2
Benign environment, aqueous liquids and
vapors
Air: 2.50, N2: 5.00; Low 1.00, High 7.00
HIOXY Probes
Photoluminescence-quenching using Ru
compound. Measures O2 partial pressure.
Phase shift due to change in partial
pressure of O2
Hydrocarbon-based liquids and vapors,
fuels, alcoholic beverages, vegetable oil
Air: 0.50, N2: 2.50; Low: 0.30, High: 6.00
5% of reading (using polynomial fit to
multipoint calibration)
~1 second, in liquid and gas
30-45 seconds
FOSPOR Probes
Photoluminescence-quenching using Pt
compound. Measures O2 partial pressure.
Phase shift due to change in partial
pressure of O2
Low O2 (0-5%), vacuum systems
packaging, benign environment
Air: 10.00; N2: 50.00; Low: 3.00,
High: 70.00
5% of reading (using polynomial fit to
multipoint calibration)
~1 second, in liquid and gas
30-45 seconds
15-20 seconds
15-20 seconds
Overcoat not required
0-40.7 ppm; 0-760 mm Hg partial
pressure
0-100% (mole percent); 0-760 mm Hg
partial pressure
Drift <0.01 ppm per hour
0-40.7 ppm; 0-760 mm Hg partial
pressure
0-100% (mole percent); 0-760 mm Hg
partial pressure
Drift <0.002 ppm per hour
5% of reading (using polynomial fit to
multipoint calibration)
~1 second, in liquid and gas
Overcoat not required
Stability oxygen gas (at 1 atmosphere):
Drift ~0.03% O2 per hour
Resolution of dissolved oxygen in liquid:
Resolution of oxygen gas (at
1 atmosphere):
Lowest detectable limit of dissolved
oxygen in liquid:
Lowest detectable limit of oxygen gas (at
1 atmosphere):
Overcoat available:
Temperature range:
Probe lifetime:
Recommended excitation source:
Recommended detector:
0.02 ppm at room temperature
0.05% (0.4 mm Hg) at room temperature
0-40.7 ppm; 0-760 mm Hg partial
pressure
0-100% (mole percent); 0-760 mm Hg
partial pressure
Drift <0.00008 ppm O2 per hour at low
dissolved oxygen; Drift ~ 0.006 ppm O2
per hour in air-saturated water
Drift ~0.0002% O2 drift per hour at low
O2; Drift ~0.015% O2 per hour air
0.002 ppm at room temperature
0.005% at room temperature
0.02 ppm
0.002 ppm at room temperature
0.02 ppm
0.05% (0.4 mm Hg)
0.005% (0.04 mm Hg)
0.05% (0.4 mm Hg)
Yes, FOXY-AF and FOXY-AF-MG
-50 ºC to +80 ºC
Recondition once per year
USB-LS-450 470-nm LED
MFPF-100-1, MFPF-100-2, USB4000-FL,
USB4000-FL-450
Yes, FOSPOR-AF and FOSPOR-AF-MG
0 ºC to +60 ºC
Recondition once per year
USB-LS-395 395-nm LED
USB4000-FL, USB4000-FL-395
No overcoat available
-50 ºC to +80 ºC
Recondition once per year
USB-LS-450 470-nm LED
MFPF-100-1, MFPF-100-2, USB4000-FL,
USB4000-FL-450
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Drift ~0.01% O2 per hour
0.02 ppm at room temperature
0.05% (0.4 mm Hg) at room temperature
For all your sensing needs, visit OceanOptics.com
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Oxygen Sensor Care & Compatibility
Care of Oxygen Sensor Formulation & Probe
Your Oxygen Sensor probe is very easy to maintain. It can be left in air indefinitely, but don't leave it
exposed to your excitation light source when it is not in use. Dropping the probe could cause the optical
fiber to break. Be sure not to over-tighten the SMA 905 Connectors. Clean your probes with 10%
hypochlorite detergent and sterilize them with gamma radiation or sodium hypochlorite (bleach). See below
for further details on cleaning and sterilization methods available for your Sensor Probes.
Method
FOXY
FOSPOR
HIOXY
Sodium hypochlorite (bleach)
Safe
Safe
Safe
Gamma radiation
Safe
Safe
Safe
Hydrogen peroxide plasma gas,
Degrades probe signal by
Degrades probe signal by
Degrades probe signal by
low temperature, Plazlyte
about 15% with each cycle
about 15% with each cycle
about 15% with each cycle
Autoclaving (steam sterilization)
Each cycle decreases signal by
Each cycle decreases signal by
Each cycle decreases signal by
>30 minutes at 121 °C
50%; probe lifetime is 6-8 cycles
50%; probe lifetime is 6-8 cycles
50%; probe lifetime is 6-8 cycles
Methanol and ethanol wash
Unsafe
Unsafe
Safe with brief exposure to ethanol
Hydrogen peroxide
Unsafe
Unsafe
Unknown
Ozone
Unsafe
Unsafe
Unsafe
Compatibility with Fiber Optic Oxygen Probes: Observational Results
Chemical
This table lists known
observational effects of
chemicals and gases on sensor
probes. If a chemical or gas
passes the "observational" test
(inserting the probe into the
environment for 24 hours and
observing no change in sensor
performance), it warrants
further comprehensive
determinate testing. Please note
that the table lists compatibility
on an observational level only.
(Comprehensive determinate
testing results are available
upon request.)
For chemical compatibility
testing of samples, we suggest
our SGS products (page 72),
coated substrates such as
microscope glass cover slips
that are ideal for evaluating
coating formulations exposed to
your sample environment.
For the most up-to-date
compatibility list, visit
www.oceanoptics.com/products/
sensorcarecompatibility.asp.
FOXY
FOSPOR
Acetone
No
No
HIOXY
No
Acetonitrile
No
No
Unknown
Acids
Yes
Yes
Unknown
Acrylonitrile
No
No
Unknown
Alcohols >50% concentration
No
No
Yes
Alcohols <50% concentration
Yes, overcoat required
Yes, overcoat required
Yes
Ammonia
Yes
Yes
Unknown
Benzene (long-term)
No
No
Yes
Benzene (short-term)
Yes
Yes
Yes
Diesel Fuel
No
No
Yes
Ethanol
No
No
Yes
Gasoline
No
No
Yes
Heptane
No
No
Unknown
Unknown
Hexane
No
No
Hydrofluoric Acid (HF)
No
No
No
Isopropyl Acetate >60% concen.
No
No
Unknown
Isopropyl Alcohol <60% concen.
Yes, overcoat required
Yes, overcoat required
Yes
No
No
Unknown
Hydrogen Peroxide
Ketones (such as acetone)
Methanol <50% concentration
No
No
No
Yes, overcoat required
Yes, overcoat required
Yes
Unknown
Methyl Methacrylate
No
No
Nitrogen Trifluoride (NF3)
Yes
Yes
Yes
Non-polar solvents
No
No
Unknown
N-Vinyl-2-Pyrrolidinone
No
No
Unknown
Organic solvents
No
No
Unknown
Perfluorodecalin & Perfluorohexane
Yes
Yes
Yes
Skydrol (Aviation Hydraulic Fluid)
No
No
Yes
Sodium Hypochlorite and Sulfide
Yes
Yes
Yes
Sodium Hydroxide (1 Molar) NaOH
Yes
Yes
Yes
Solutions with pH >10
No
No
No
Styrene
No
No
Unknown
Unknown
Sulfur Dioxide (SO2)
No
No
Sulfur Hexafluoride (SF6)
Yes
Yes
Yes
Tetrahydrofuran
No
No
Unknown
Toluene and Toluene/Ethyl Acetate
No
No
No
Trichloroethyelene
No
No
Unknown
Xylene
No
No
No
Tel: 727.733.2447 • Email: [email protected]
69
Optical Sensors
Though our oxygen sensing
probes work well in most
environments, some chemicals
interfere with performance by
deteriorating the fluorescence
irreversibly or by chemically
attacking the coating. In some
cases, overcoats may reduce
such interference.
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Oxygen Sensor Probes
Once you select the Sensor Formulation best suited for your application, you need to select the Sensor Probe
onto which the formulation or coating is applied. Ocean Optics offers several off-the-shelf Sensor Probes and
has the ability to create the custom probe assembly that best fits your needs. After selecting your Sensor
Formulation and Sensor Probe, you need to purchase a 21-02 Splice Bushing and Bifurcated Optical Fiber
Assembly (page 72) to attach the Sensor Probe to your Oxygen Sensing System.
18G Sensor Probe
Typical Usage:
Penetration of vial septa and rigid packaging
Probe Assembly:
300 µm optical fiber, 18-gauge needle tip
Dimensions:
1.27 mm diameter, 90 mm length tip
Pressure:
300 psi
Ordering Information
FOXY-18G
18G Sensor Probe with FOXY Formulation
FOSPOR-18G
18G Sensor Probe with FOSPOR Formulation
$599
$599
HIOXY-18G
18G Sensor Probe with HIOXY Formulation
$899
Optical Sensors
21G Sensor Probe
Typical Usage:
Penetration of vial septa and rigid packaging
Probe Assembly:
300 µm optical fiber, 21-gauge needle tip
Dimensions:
1.27 mm diameter, 90 mm length tip
Pressure:
300 psi
Ordering Information
FOXY-21G
21G Sensor Probe with FOXY Formulation
FOSPOR-21G
21G Sensor Probe with FOSPOR Formulation
$599
$599
HIOXY-21G
21G Sensor Probe with HIOXY Formulation
$899
OR125 Sensor Probe
Typical Usage:
Direct replacement for 1/8" OD O2 electrodes
Probe Assembly:
1000 µm optical fiber, stainless steel ferrule
Dimensions:
3.175 mm OD, 63.5 mm length
Pressure:
300 psi
Ordering Information
FOXY-OR125
OR125 Sensor Probe with FOXY Formulation
FOSPOR-OR125
OR125 Sensor Probe with FOSPOR Formulation
$599
$599
HIOXY-OR125
OR125 Sensor Probe with HIOXY Formulation
$899
OR125-G & OR125-GT Sensor Probes
Typical Usage:
Direct replacement for O-ring grooved electrodes
Probe Assembly:
1000 µm optical fiber, stainless steel ferrule or titanium ferrule
Dimensions:
3.175 mm OD, 63.5 mm length
Pressure:
300 psi
Ordering Information
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FOXY-OR125-G
OR125-G Sensor Probe with FOXY Formulation, SS ferrule
FOSPOR-OR125-G
OR125-G Sensor Probe with FOSPOR Formulation, SS ferrule
$599
$599
HIOXY-OR125-G
OR125-G Sensor Probe with HIOXY Formulation, SS ferrule
$899
FOXY-OR125-GT
OR125-GT Sensor Probe with FOXY Formulation, titanium ferrule
$649
FOSPOR-OR125-GT
OR125-GT Sensor Probe with FOSPOR Formulation, titanium ferrule
$649
HIOXY-OR125-GT
OR125-GT Sensor Probe with HIOXY Formulation, titanium ferrule
$979
For all your sensing needs, visit OceanOptics.com
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Oxygen Sensor Probes
R Sensor Probe
Typical Usage:
General Purpose
Probe Assembly:
1000 µm fiber in a stainless steel 1/16" OD ferrule
Dimensions:
1.587 mm OD, 152.4 mm length
Pressure:
300 psi
Ordering Information
FOXY-R
R Sensor Probe with FOXY Formulation
FOSPOR-R
R Sensor Probe with FOSPOR Formulation
$499
$499
HIOXY-R
R Sensor Probe with HIOXY Formulation
$749
AL-300 Sensor Probe
Typical Usage:
Fine spatial resolution applications
Probe Assembly:
300 µm aluminum-jacketed fiber assembly
Dimensions:
500 µm OD, 1 m length
Pressure:
300 psi
Ordering Information
FOXY-AL300
AL300 Sensor Probe with FOXY Formulation
FOSPOR-AL300
AL300 Sensor Probe with FOSPOR Formulation
$499
$499
HIOXY-AL300
AL300 Sensor Probe with HIOXY Formulation
$749
Optical Sensors
PI600 Sensor Probe
Typical Usage:
Environments where non-metallic probe is indicated
Probe Assembly:
600 µm optical fiber with silicone jacketing
Dimensions:
710 µm OD, 2 m length
Pressure:
300 psi
Ordering Information
FOXY-PI600
PI600 Sensor Probe with FOXY Formulation
$499
FOSPOR-PI600
PI600 Sensor Probe with FOSPOR Formulation
$499
T1000 Sensor Probe
Typical Usage:
Process environments, high-pressure applications
Probe Assembly:
1000 µm optical fiber, stainless steel ferrule
Dimensions:
6.35 mm OD, 177.8 mm length
Pressure:
3000 psi
Ordering Information
FOXY-T1000
T1000 Sensor Probe with FOXY Formulation
FOSPOR-T1000
T1000 Sensor Probe with FOSPOR Formulation
HIOXY-T1000
T1000 Sensor Probe with HIOXY Formulation
$999
$999
$1,499
T1000-RTD Sensor Probe
Typical Usage:
Process environments, has embedded RTD
Probe Assembly:
1000 µm optical fiber, stainless steel ferrule
Dimensions:
6.35 mm OD, 177.8 mm length
Pressure:
300 psi
Ordering Information
FOXY-T1000-RTD
T1000 Sensor Probe with FOXY Formulation
$1,499
FOSPOR-T1000-RTD T1000 Sensor Probe with FOSPOR Formulation
$1,499
HIOXY-T1000-RTD
$1,499
T1000 Sensor Probe with HIOXY Formulation
Tel: 727.733.2447 • Email: [email protected]
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Oxygen Sensor Accessories
Bifurcated Optical Fiber Assemblies and Splice Bushing
Our Y-shaped Bifurcated Optical Fiber Assemblies contain two fibers
side-by-side in the common end of the assembly, which connects to the
Sensor Probe. From the breakout of the assembly, the two fibers diverge into
two legs, one connects to a spectrometer, the other to the excitation source.
A 21-02 Splice Bushing is an adapter that connects an SMA 905-terminated
Sensor Probe to a SMA-terminated Bifurcated Optical Fiber Assembly.
Item
Description
21-02
Splice Bushing to connect Sensor Probe to Bifurcated
BIF-600-VIS-NIR Bifurcated Optical Fiber Assembly
Price
$13
Optical Fiber Assembly
BIF-600-VIS-NIR
Laboratory-grade Bifurcated Optical Fiber Assembly
QBIF-600-VIS-NIR
Premium-grade Bifurcated Optical Fiber Assembly
$329
$369
QBIF-600-VIS-BX
Premium-grade Bifurcated Optical Fiber Assembly with
$369
BX cable jacketing (not shown)
QBIF-600-VIS-NIR Bifurcated Optical Fiber Assembly
Sensor Probe
21-02 Splice Bushing
Bifurcated Optical Fiber Assembly
Optical Sensors
Respiration Monitor “RESP” Sensor Probe
The FOXY-RESP is a fiber optic oxygen sensor for in situ respiration monitoring of oxygen tension in respiratory
gases. The probe can be combined with a spectrometer and accessories to measure inspired and
expired oxygen in real time -- valuable data that complements existing respiratory parameters and
airway mechanic values. For remote monitoring, use the sensor with optical fiber of variable lengths.
You can also configure the stable probe with a monochromator for wavelength-specific analysis. The
sensor can be used in magnetic resonance imaging environments. The probe assembly contains
200 µm optical fiber in a plastic ferrule and is 6.35 mm OD and 107.9 mm in length. See the Planar
Oxygen Sensors table below on purchasing -RESP-FILM, the membranes needed for the FOXY-RESP Probe.
FOXY-RESP: $549
Planar Oxygen Sensors
Though our fiber optic sensor probes work well in most solutions, some
environments interfere with sensor performance by deteriorating the
fluorescence irreversibly or by chemically attacking the coating. We offer
a variety of coated substrates for testing or for applications where a
probe is undesirable.
-GF
-SGS-M
Item
Description
Typical Usage
-SGS
Custom coating service for coating various substrates (supplied by user or Ocean
Optics) with different transducer materials, specify Sensor Formulation
qualitative, quantitative
feasibility testing
Price
-SGS-M
One 1" x 3" sol-gel spin-coated microscope slide, specify Sensor Formulation
qualitative, quantitative testing
$300
-GF
Pack of 5 sol-gel coated fiberglass filters, specify Sensor Formulation
qualitative, quantitative testing
$50
-RESP-FILM
Pack of 25 sol-gel coated glass fiber membranes for Respiration Monitor (above)
qualitative, quantitative testing
$50
Custom
Pricing
Silicone Overcoats
We can apply silicone overcoats over FOXY and FOSPOR Oxygen Sensor Probes to improve chemical
resistance, exclude ambient light and eliminate refractive index effects of the sample. We recommend
an overcoat if you are using solutions or if you are switching between gases and solutions. Overcoats
are free. (The HIOXY Sensor Formulation does not benefit from overcoats.)
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Item
Description
Response in Gases
Response in Solutions
-AF
RTV silicone adhesive overcoat (overcoat increases response time),
specify FOXY or FOSPOR Sensor Formulation
10-30 seconds
15-45 seconds
-AF-MG
High-strength RTV silicone adhesive overcoat is a medical implant-grade
silicone -- a thicker and more robust coating than the -AF (overcoat
increases response time); specify FOXY or FOSPOR Sensor Formulation
15-45 seconds
45-60 seconds (depending
on viscosity)
For all your sensing needs, visit OceanOptics.com
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Oxygen Sensor Accessories
In-line Flow Cell
A FOXY-R,
FOSPOR-R
or HIOXY-R
probe would
be inserted
into the flow
cell here, for
O2 measurements.
The FOXY-FLOW-CELL is an in-line flow cell for 1.587 mm (1/16") OD
probes, such as the FOXY-R, FOSPOR-R and HIOXY-R. It was designed
for use in a low-pressure flowing stream of liquid with a peristaltic or
positive displacement pump. The flow cell also can be used as an online
sampling accessory for 1/16" OD reflectance probes.
The flow cell is made of PEEK polymer, a radiation-resistant material that
has excellent chemical resistance. Also included are four tubing barbs:
two for 1/16" ID tubing and two for 1/8" ID tubing. (Tubing and pump
are not included.) You can replace these fittings with other-sized fittings
from Upchurch Scientific as long as they have 1/4-28 threading.
FOXY-FLOW-CELL:
$100
Specifications
Tee:
Tubing barbs:
Ferrule:
Nut:
Threading size:
Pressure limits:
Two sets of
tubing barbs
are included
with the cell.
Upchurch Scientific PEEK tee
(2) 1/8" Tefzel tubing barbs, (2) 1/16" Tefzel tubings barbs
1/16" PTFE ferrule
1/16" PEEK nut
1/4-28
1000 PSI
Puncturing Needle
Optical Sensors
The Puncturing Needle is an Oxygen Sensor Probe accessory that allows
1.587 mm (1/16") outer diameter sensors -- such as the FOXY-R, FOSPOR-R
and HIOXY-R (page 71) -- to puncture a septum and seal without damaging
the sensor coating. The Puncturing Needle includes a 1/16" needle and a
1/16" Swagelok adapter to seal the sensor in place.
FOXY-R-PNA:
$150
O2 Acrylic Sampling Chambers, Respirometers
Our Acrylic Sampling Chambers are used by biologists and zoologists in dissolved oxygen sensing
applications such as respiration rate and metabolic rate monitoring of fish and crustaceans. You can
combine a sample chamber, probe, spectrometer and light source to configure a complete
respirometer. The sampling chambers provide users with a fixed-volume environment. Each chamber
cover is equipped with high-pressure (220 psi) polypropylene collars and a Swagelok fitting for an
Oxygen Sensor Probe. The acrylic chambers have a temperature range of -30 °C to 82 °C and are
FDA-approved for food applications. The polypropylene fittings are temperature rated from
0 °C to 100 °C. Each chamber has a watertight seal seated between the body and its cover.
Item
Acrylic Chamber Type
Dimensions (in mm)
Fittings
Price
RESP-CL2IN
Clear Round
44.4 ID x 139.7 length
1 bored 1/4" OD tubing fitting
$160
RESP-BL2IN
Black/Opaque Rectangle
139.7 x 50.8 x 50.8
1 bored 1/4" OD tubing fitting
$180
RESP-CL4IN
Clear Acrylic Round
95.2 ID x 139.7 length
2 bored 1/4" OD tubing fittings
$175
RESP-BL4IN
Black/Opaque Rectangle
140 x 101.6 x 101.6
2 bored 1/4" OD tubing fittings
$195
RESP-CL6IN
Clear Round
146 ID x 139.7 length
3 bored 1/4" OD tubing fittings
$190
RESP-BL6IN
Black/Opaque Rectangle
139.7 x 127 x 127
3 bored 1/4" OD tubing fittings
$210
Sensor Reconditioning/Recoating Service
Each Oxygen Sensor Probe contains a Sensor Formulation at its tip. Cleaning and protection from
harsh environments will extend the life of the sensor. Severe biofouling, physical abrasion, and chemical
etching of the glass may erode the sensing surface, requiring our probe recovery service. For -18G and
-21G Needle Probes, we re-polish the probe and add a new needle tip for $125. For all other probes,
we re-polish and re-coat the probe for $100. Specify FOXY, FOSPOR or HIOXY Sensor Formulation.
-RECOV:
$100
-RECOV-N:
$125
Tel: 727.733.2447 • Email: [email protected]
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Oxygen Sensor Temperature Compensation
Our Fiber Optic Sensors are affected by temperature. Temperature affects the fluorescence
decay time, fluorescence intensity, collisional frequency of the oxygen molecules with the
fluorophore, and the diffusion coefficient of oxygen. The net effect: a change in the calibration
slope. Because of this, the sample must be maintained at a constant temperature (± 3.0 °C) for
best results. If this is impractical, the sensor can be calibrated by measuring temperature and
oxygen concurrently using one of our temperature-compensation accessories and in-house
calibration services.
In-house Temperature Calibration Services
Optical Sensors
If your sample cannot be maintained at a constant temperature (± 3.0 °C),
you can perform a temperature calibration in OOISensors Software or we
can perform the calibration for you. The -CAL is an in-house factory-calibration service
for environments from 0-80 °C. The -CAL-EXT is a factory-calibration service for
extended temperature ranges below 0 °C or above 80 °C. You’ll need to determine the
temperature and O2 concentration range of your sample environment before ordering
an in-house calibration service. Be sure to specify the Oxygen Sensor Formulation (FOXY,
FOSPOR or HIOXY) being used in the calibration.
-CAL:
$199
-CAL-EXT:
$299
The USB-LS-450-TP
Platinum RTD -- for use with the
USB-LS-450 -- helps adjust for
temperature changes.
Thermistor & Thermocouples for Ocean Optics Spectrometers
Item
Description
Price
FOXY-TS1
Thermistor is 1/8" outer diameter stainless steel tubular electrode probe that monitors temperatures from
$105
0 °C to 100 °C; it most often is used for liquid immersion
FOXY-T-MOD-1
An RS-232 module interfaces up to four of the FOXY-TS1 Thermistors to your PC
$500
FOXY-TK1
Thermocouple is a 1/8" outer diameter K-type electrode that monitors temperatures from -150 °C to 220 °C
$105
FOXY-TK1-W
Wire-type thermocouple that monitors temperatures from -150 °C to 220 °C
$105
FOXY-T-MOD-K
An RS-232 module interfaces up to four of the FOXY-TK1 Thermocouples to your PC
$500
RTDs for Sensing Temperature Changes
We offer three RTDs to adjust for temperature
changes. The USB-LS-450-TP is a 1/8" outer diameter,
100 ohm platinum RTD that connects to the USB-LS450 Excitation Source (see page 131). The USB-LS450’s onboard memory can be programmed to store
temperature and oxygen calibration coefficients. The
USB-LS-450-TP16 is a 16-gauge needle RTD, also for
use with the USB-LS-450.
The -T1000-RTD (at right) is a -T1000 probe, but with
an embedded RTD in the 1/4" outer diameter casing.
When ordering the -T1000-RTD, be sure to specify the
FOXY, FOSPOR or HIOXY Sensor Formulation being
applied to the -T1000 Probe tip.
USB-LS-450-TP:
$99
USB-LS-450-TP16:
$249
FOXY-T1000-RTD:
$1,499
FOSPOR-T1000-RTD: $1,499
HIOXY-T1000-RTD: $1,499
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For all your sensing needs, visit OceanOptics.com
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Sensor Software
OOISensors:
Optical Sensors
OOISensors Software is a 32-bit,
advanced acquisition and display program
that provides a real-time interface to
display and processing functions for use
with our O2 and pH sensors as well as
with Ocean Optics spectrometers and the
MultiFrequency Phase Fluorometer.
OOISensors can acquire data, convert the
data into concentration values, and save
the data in spectral files and logs. The
software has the ability to perform timed
experiments and to display and correct for
temperature fluctuations and for
atmospheric pressure changes in the
sample. It can also display pH values
when used with our pH probe.
OOISensors features include:
Obtains oxygen partial pressure, pH
or concentration values from sensors
Contains easy-to-use functions for all
OOISensors Software gives you the opportunity to view spectral data from multiple spectrometer
system parameters
channels (top part of the graph) as well as collect and view oxygen, sensor or pH data over time
Performs time acquisition experiments (bottom part of the graph).
Collects data from up to eight
spectrometers simultaneously and displays the results in a single window
Allows each spectrometer channel to have its own data acquisition parameters
Monitors temperature (when using one of the temperature sensors on page 74), displays temperature
data and corrects the data for any fluctuations in temperature and pressure
Supports oxygen calibration procedures with first-order linear Stern-Volmer algorithm and with secondorder polynomial algorithm to provide more accurate data
Displays a time chart with the data from all active channels at a specific wavelength over time
Allows user to enable Data Logging function and add experiment notes to a log file
Works with all Windows 95/98/XP/2000/NT Operating Systems
$199
Pocket Carbon Monoxide Meter
Carbon monoxide (CO) is a colorless, odorless, poisonous gas. Appliances fueled with natural
gas, liquefied petroleum, oil, kerosene, coal, or wood may produce CO. Burning charcoal and
running cars produce CO. Every year, hundreds of people in the United States die from CO
produced by fuel-burning appliances and cars left running in attached garages.
The Pocket CO Carbon Monoxide Meter
from Transducer Technology, Inc., is a
technically advanced, long-life
electrochemical sensor (patents pending)
combined with a microprocessor for
convenient and reliable monitoring of
CO. The sensor’s features allow CO
monitoring, spot check measurements
and CO dosimetry.
Size as shown.
The tiny Pocket CO runs on a
watch battery.
The Pocket CO is warrantied for one
year. After one year, we recommend a
recalibration of the sensor and battery
change for best performance.
CHEMSEN-CO: $149
Tel: 727.733.2447 • Email: [email protected]
Specifications
Size:
Weight:
Material:
Range:
Accuracy:
Response time:
Warm-up time
Operating life
Operating temperature:
Temperature limits:
Pressure effect:
Humidity limits:
Alarms, visual, audio:
Interferences:
2.4" x 1.4" x 0.6"
Less than 1 ounce, 20 grams
Impact resistant plastic case
0-600 ppm CO
+/- 10% of reading at standard conditions
Less than 30 seconds to 90%
2 seconds (CO is measured every 2 seconds)
1 year minimum
32 °F to 105 °F, or 0 °C to 40 °C
10-120 °F; 3-50 °C
Reading decreases with decreasing
pressure, to 70% at 10,000 ft.
0-100% RH, non-condensing
CO level greater than 25 ppm
CO level greater than 125 ppm
Temperature greater than 105 °F or 40 °C
Temperature less than 32 °F or 0 °C
None significant, except hydrogen
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Fiber Optic pH Sensors
Sensor Holds Indicator Dyes
The Fiber Optic pH Sensor system consists of a fiber optic
probe designed to hold immobilized colorimetric indicator dye
materials, plus a light source, spectrometer and OOISensors
Software. You can supply your own indicator material, or
select from our line of transparent or reflective films.
Calibration involves recording spectra in high and low pH
samples, and in at least one pH standard such as a NISTtraceable buffer.
Transmissive & Reflective pH Films
Transmissive films are for clean, transparent samples. These
films consist of a cellulose mechanical matrix surrounded by a
hydrophilic polymer that entraps the indicator dye. Reflective
films are used for turbid or absorbing media. When immersed
in water, the film dyes may leach very slowly over time and
will have to be replaced. The film response rate is slow (on
the order of minutes), being limited by diffusion of ions into
the material. Increasing stirring speed, ionic strength and
temperature all tend to increase the response rate and do not
affect the pH measurement. Nearly any aqueous sample
environment is suitable, as are some solvents.
Use transmissive films
with the TP300-UV-VIS
Probe for transparent
samples. Use reflective
films with the RFP-200UV-VIS Probe for turbid,
dense samples.
Optical Sensors
TP300 Probe
The TP300-UV-VIS Probe (at right) is a chemically inert PEEK
transmission probe that can be equipped with a tip (RT-PH) for
mounting transmissive films in the optical path. Light is
directed via one fiber through the mounted film to a mirror.
Then light is redirected back through the film to a receive fiber
that returns the light to the spectrometer. The sample is free to
flow over the sides of the film. By using an RTP-2-10
(adjustable from 2-10 mm) or RTP-10-20 (adjustable from 1020 mm) transmission tip, the TP300-UV-VIS can be used for
routine transmission measurements. See page 151 for details.
TP300-UV-VIS: $750
RT-PH Tip:
$240
Transmissive Indicator Dye Films for pH Sensing
Item
Film Type
pH Range Color Change
F-PR
Phenol Red
6.5-8.5
yellow-purple
$50
F-CR
Cresol Red
8.0-10.0
orange-purple
$50
F-MCP
m-Cresol Purple
8.5-10.5
yellow-purple
$50
F-TB
Thymol Blue
9.0-12.0
yellow-purple
$50
F-BY
Brilliant Yellow
7.0-9.0
yellow/red-purple
$50
F-xxx
Transparent Film reference
not applicable
$50
FILM300 Sample pack of transmissive films
Price
$50
All pH films come in packages of 5 films.
Reflective Indicator Dye Films for pH Sensing
RFP200 Probe
Item
Film Type
pH Range Color Change
The RFP200-UV-VIS Reflective Film Probe consists of a 6around-1 fiber bundle in a chemically inert 6.35-mm outer
diameter Torlon body. The open tip of the probe screws onto
the body to hold 3.17-mm to 4.76-mm discs of reflective
indicator material. The 6-fiber leg attaches to the light source;
the central fiber leg connects to the spectrometer. The sample
has access to the sensing material from one side only.
RFP200-UV-VIS: $499
FR-PR
Phenol Red
6.5-8.5
yellow-purple
$50
FNY-PR
Phenol Red Nylon 6.5-8.5
yellow-purple
$50
FR-CR
Cresol Red
Price
8.0-10.0
orange-purple
$50
FR-MCP m-Cresol Purple
8.5-10.5
yellow-purple
$50
FR-TB
Thymol Blue
9.0-12.0
yellow-purple
$50
FR-BY
Brilliant Yellow
7.0-9.0
yellow/red-purple
$50
FILM
Sample pack of reflective films
$50
All pH films come in packages of 5 films.
Phenol Red pH Test Kit
The CHEMTEST-PH is a Phenol Red pH Test Kit that includes 100 tests in cuvettes with covers.
The CHEMTEST-PH can be used to determine the pH level in solution. Simply add 3 mL
solution to a cuvette, cap it, shake the cuvette to disperse the dye, and then measure the
absorbance value of the reactive color to determine the pH level. CHEMTEST-PH works with
any Ocean Optics system that is configured for absorbance, including the CHEM4-series
Spectrophotometers on pages 36-37. Software included.
CHEMTEST-PH:
$99
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For all your sensing needs, visit OceanOptics.com
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Software &
Data Acquisition
Overview
79
UV-VIS Spectral Database
80
SpectraSuite Spectroscopy
Operating Software
82
OmniDriver Development Platform
83
SpecLine Software for Compound ID
84
Analog-to-Digital Converters
Software & Data Acquisition
78
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Overview: Software & Data Acquisition
Real-time Interface to the PC of Your Choice
Ocean Optics data acquisition
options allow you to interface
your spectrometer to any
desktop or notebook PC,
whether it operates in Mac,
Linux or Windows operating
systems. Our plug-and-play
spectrometers connect directly
to the USB port of any desktop
or notebook PC. We also offer
external analog-to-digital
converters, including USB and
PCI-bus cards.
Software & Data Acquisition
Real-time data acquisition for
almost any type of application
is made possible by our new
operating, application and
software development
packages. We also offer custom
software-development services.
The Joys of Java
More About Java
SpectraSuite and OmniDriver: Multi-platform Marvels
One of the most important
decisions in developing
SpectraSuite and OmniDriver
was the selection of Java as
the programming language.
Java is an object-oriented
programming language,
developed in the mid-‘90s by
Sun Microsystems, Inc., that
was designed as a robust,
platform-independent
programming environment
that manages memory on its
own. (When it comes to
distributed applications,
nothing beats Java. For
additional information, visit
java.sun.com.) We’ve taken
Java a step further by
making it platform- and
spectrometer-independent -i.e., the same code works for
all of our USB-based
spectrometers.
You spoke, we listened. After nearly 15 years and
thousands of spectroscopy applications, we’ve
taken the best of your suggestions -- and added a
few clever wrinkles of our own -- to create the
industry’s first modular, operating systemindependent spectroscopy software platform and
driver. SpectraSuite, a Java-based spectroscopy
software that operates on Windows, Macintosh and
Linux operating systems, offers a host of robust
features for remarkable power and flexibility.
Like SpectraSuite, OmniDriver is cross-platform,
Java-based software. It combines the best of our
earlier device driver packages -- high-speed data
acquisition, customization of acquisition and
processing parameters, and so on -- with additional
features to make it the only spectroscopy driver
you’ll ever need.
There’s much more on SpectraSuite and
OmniDriver in the next few pages -- so prepare to
be dazzled.
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For all your sensing needs, visit OceanOptics.com
Overview: Software & Data Acquisition
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It’s long been a goal of ours to create one hardware device driver program that would control all of our
hardware as well as other manufacturers’ devices, from any type of computer operating system environment
and from which all software applications would run. The answer was to use Java as the programming
language. Java was designed to be platform-neutral, making it the perfect programming language for our
customers around the globe. Aside from the additional power and flexibility our software packages provide,
SpectraSuite and OmniDriver will affect customers in two significant ways. First, there is a $199 charge for
SpectraSuite, a price that’s comparable to what our competitors offer. Second, all existing Ocean Optics
software will no longer be upgraded -- supported, yes; upgraded, no. Here’s some additional important
information about the transition to SpectraSuite and OmniDriver:
Did SpectraSuite replace OOIBase32? Is there a charge for SpectraSuite?
Yes, SpectraSuite replaced OOIBase32, and yes, there is a charge for SpectraSuite -- $199.
OOIBase32 is no longer being upgraded and does not work with spectrometers developed after
August 2005. If you purchase a spectrometer today, you should include SpectraSuite in your order.
Q
A
Can I upgrade from OOIBase32 to SpectraSuite?
Absolutely. Upgrade to SpectraSuite for $199. Be sure to check with an Application Sales Engineer to
make sure your spectrometer will work with SpectraSuite.
Q
A
Which Ocean Optics software did SpectraSuite and OmniDriver replace?
OOIBase32 Spectrometer Operating Software, OOIBase32 Platinum Script-writing Software, OOIChem
Software for Education and OOIIrrad Irradiance Software; plus the OOIWinIP Windows Interface
Package, OOILVD LabVIEW Software Device Driver Package, OOIHSD High-speed Driver Library and
OOISPM Spectral Processing Module. Windows CE tools such as OOIPS2000-S Operating Software
and OOIHIP Handheld Interface Package have become obsolete.
Q
A
What about existing applications software?
SpectraSuite is the platform for all future Ocean Optics application software development. At press
time, OOISensors and OOILIBS Software are scheduled to migrate to the SpectraSuite platform
later in 2007.
Q
A
Will Ocean Optics continue to support earlier versions of its software?
Yes, we will continue to technically support old versions of all of our software products and, if
necessary, post software fixes on our website. In fact, we still occasionally get support questions about
SpectraScope -- our original spectrometer operating software, which is older than dirt in software
years. What we won’t do is upgrade any older software with new features, nor will we upgrade older
software to work with Ocean Optics hardware developed after August 2005.
Software & Data Acquisition
Q
A
UV-VIS Spectral Database
Ocean Optics has teamed with science-softCon to present the 4th edition of the science-softCon UV-Vis Spectral
Database. This is one of the most extensive UV-Vis databases now available, with nearly 3,000 entries (in ASCII
format) for some 400 substances. The database includes the following substance groups:
Alkali Compounds
Nitrogen Acids
Aromatic Compounds
Nitrogen/Nitrogen Oxides
Dyes
Organic Acids/Esters
Halogenated Alkanes, Alkenes
Organic Carbonyl Compounds
Halogenated Carbonyl Compounds
Organic Nitrogen Compounds
Halogenated Nitrogen Compounds
Other Oxygenated Organics
Halogens/Halogenoxides
Oxygen Hydrogen Compounds
Hydrocarbons
Pesticides
Hydrogenhalides/Hypohalides
Sulfur Compounds
This price of the database includes a CD with science-softCon's UV/Vis Spectral Database and a one year
unlimited online free subscription to the most up-to-date and comprehensive spectral data available.
CD-SPECTRA:
$195
Tel: 727.733.2447 • Email: [email protected]
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SpectraSuite Spectroscopy Software
The New Revolution
In 1992, we revolutionized the
optical sensing industry when we
introduced the first-ever
modular, miniature spectrometer.
Now, with more than 85,000
spectrometers sold and the
experience of thousands of
applications, we’re kick-starting
the market again with
SpectraSuite, the first modular,
OS-independent spectroscopy
software platform.
Spectroscopy on any
Operating System
Software & Data Acquisition
SpectraSuite is a completely
modular, Java-based
spectroscopy software platform
that operates on Windows,
Macintosh and Linux operating
systems. The software can
SpectraSuite is a platform-independent application that provides graphical and numeric representation of spectra
control any Ocean Optics USB
in one window.
spectrometer and device, as well
as any other manufacturer’s
USB instrumentation (using the appropriate drivers). The SpectraSuite
interface looks and feels the same on all operating systems yet retains
SpectraSuite
the familiar appearance of an application native to each OS. Ocean
Optics is the first to offer such a flexible, feature-packed application
with this level of cross-platform capability.
Can be used with these Ocean
Optics products when interfacing to
Our Platform for the Future
SpectraSuite is the platform for all future Ocean Optics application
software development. Software applications including OOIChem,
OOIColor and OOIIrrad-C have been migrated to the SpectraSuite
platform, with applications such as OOISensors and OOILIBS coming
in the near future.
Spectrometers
HR2000
HR2000+
Ultimate USB Spectrometer & Device Control
HR4000
SpectraSuite easily manages multiple USB spectrometers -- each with
different acquisition parameters -- in multiple windows or on the same
graph in a single window -- and provides graphical and numeric
representation of spectra from each spectrometer. Using SpectraSuite,
you can combine data from multiple sources for applications that
include upwelling/downwelling measurements, dual-beam referencing
and process monitoring.
Modular Framework Lets SpectraSuite Work The
Way You Work
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MMS-Raman
NIR256-2.1
NIR256-2.5
NIR512
QE65000
USB2000
USB2000+
USB2000-FLG
The SpectraSuite framework is modular, so that every function in it can
be altered or replaced. For instance, the data acquisition functions, the
scheduling functions, the data processing functions and the rendering
functions are all separate modules. You can add or delete modules to
create a proprietary user interface or functionality, create modules to
perform calculations, automate experiment routines and more. You or
your Ocean Optics application developer can easily customize
SpectraSuite through Java code.
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a computer via USB port:
USB4000
Other Devices
ADC1000-USB A/D Converter
SHA-1 Spectral Hyper Adapter
For all your sensing needs, visit OceanOptics.com
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SpectraSuite Spectroscopy Software
Original Equipment Manufacturers
OEMs in particular will find SpectraSuite’s modularity
most beneficial, as all visual aspects of the program’s
user interface can be altered to create a fully branded
application.
Advanced Data Capture Control
SpectraSuite provides the user with advanced control
of episodic data capture attributes. For instance, a
user can acquire data for a fixed number of spectra
or for a specific interval. Initiation of each spectrum
can be externally triggered or event-driven. Captured
data is quickly stored into system memory at speeds
as fast as one spectrum per millisecond, with speeds
limited by hardware performance.
SpectraSuite in the Future
SpectraSuite Pricing
Item
Description
SPECTRASUITE
One copy of SpectraSuite
SPECTRASUITE-U
Annual upgrade subscription
Price
$199
$99
fee
SPECTRASUITE-20
Site license for SpectraSuite
$1,499
allows up to 20 copies
SPECTRASUITE-E
Site license for SpectraSuite
$2,499
allows up to 40 copies for
educational institutions only
SPECTRASUITE-S
Site license for SpectraSuite
$4,999
allows unlimited copies
Tel: 727.733.2447 • Email: [email protected]
Check out our long list of new SpectraSuite features. Note
that most of the features from our other Application Software
Packages, such as OOIIrrad Software for Color & Irradiance
and OOIChem Software for the Teaching Lab, have migrated
to SpectraSuite.
General Features
Allows users to annotate graphs and to specify format
and precision of displayed values
Displays a color spectrum behind graphs
Corrects for non-unity for reflection measurements
Performs reference monitoring
Displays x-axis in GHz, microns, pixel number, Raman
shifts, wavenumbers or nanometers
Provides an Experiment Wizard that guides users on
configuring common experiments
Acquires data from one spectrometer using different
parameters to run multiple experiments
Stores data in other formats such as tab-delimited ASCII
(for Excel or other analysis packages) and GRAMS SPC
Features for Reflective & Emissive Color & Absolute
Irradiance
Provides dominant wavelength and wavelength purity
Provides radiometric and color analysis
Analyzes peak wavelength, full width at half max,
centroid and central wavelength
Measures absolute spectral intensity of light and other
emission sources
Calculates integrated intensity between user-specified
wavelengths
Obtains photopic or scotopic data calculated in lumen,
lux and candela based on CIE standards
Provides microjoules, microwatts, number of photons and
much more
Calculates reflective or emissive color
Provides chromaticity diagram of color-space values
Offers CIE standard illuminants for reflective color (A, B,
C, D50, D55, D65, D75, E, F1-F12, etc.)
Calculates L*a*b*, XYZ, xyz, u'v'w', hue, chroma, CCT
(correlated color temperature), saturation, and more
Software & Data Acquisition
SpectraSuite is constantly evolving. Be sure to check
for updates via SpectraSuite’s Update Center. With
the purchase of SpectraSuite, you are entitled to one
year of free, web-based automatic upgrades. Future
enhancements include:
SpectraSuite will soon be 21 CFR Part 11
compliant with an encoded binary file. This
binary data format will track the complete
history of all processing steps that are
performed on your data.
SpectraSuite will allow users “process doovers.” A user will be able to change the
values of various parameters in a process and
apply those changes to data without having to
recreate an entire process.
SpectraSuite will store and provide data in new
formats, such as JCAMP.
SpectraSuite will offer a database module
where arbitrary data can be stored in any userselectable format.
SpectraSuite will be fully “internationalized.” All
of the software’s menus, dialog boxes,
prompts, messages and files will be able to
reflect a native language by simply changing a
single file.
All-In-One SpectraSuite
Features for Chemistry Teaching Labs
Provides an easy-to-follow format ideal for
undergraduate-level students and beginning
spectroscopists
Contains five modes of operation: Scope, Absorbance,
Transmission, Relative Irradiance and Concentration
Includes a Beer's Law spreadsheet for performing
calibrations from standard solutions
Adds into the spectral window previously saved overlay
spectra
Performs kinetics experiments
Saves data as ASCII files and stores and retrieves
sample spectra
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OmniDriver Dev elopment Platform
More Than a Device Driver
OmniDriver is the culmination of our best
software driver packages. It allows you to
harness the power of high-speed data
acquisition, spectral processing, data analysis,
visual data representation and data flow in a
single cross-platform driver. Integrate
OmniDriver into your own software application
for complete control over USB spectrometers and
devices in virtually any environment.
Developed in Java
Software & Data Acquisition
It’s long been a goal of ours to create one
hardware device driver program that would
control all of our hardware as well as other
manufacturers’ devices, from any type of
computer operating system environment and
from which all software applications would run. The answer was to use Java as the
programming language. Java was designed to be platform-neutral, making it the
perfect programming language for our customers around the globe. OmniDriver was
created in the Java environment and includes native libraries for select Windows,
Macintosh and Linux operating systems. Using OmniDriver, you can develop robust
applications to control multiple Ocean Optics USB spectrometers and direct-attach
devices across these different operating systems. Ocean Optics is the first and only
provider in the optical sensing industry to offer this level of cross-platform compatibility.
Complete Platform & Device Independence
Applications written in Java are environment-independent; they can work across all
operating systems. This is an advantageous feature for product developers and OEMs
wanting to expand their product offering with systems that work on multiple operating
platforms. In developing OmniDriver, we took the Java philosophy a step further to
create a device driver that is not only platform-independent, but also spectrometerindependent; the same Java code works with all Ocean Optics USB spectrometers and
direct-attach devices. Plus, OmniDriver can control any manufacturer’s USB
spectrometer and supports any USB device.
OmniDriver
Can be used with these
Operating Systems
Windows Windows 2000 or
later
Macintosh OSX 10.2 or later
Linux* RedHat 9 or later
Fedora Core, any
version
Debian 3.1 (Sarge)
Suse, 9.0 or later
“I don’t know how to program in Java”
* OmniDriver will work with any Linux OS
Chances are you know how to program in C, C++, Pascal, Visual Basic, Delphi,
with a kernel 2.4.27 or later and libstdc ++
C++ Builder or one of many Microsoft Office Applications. You don’t need to know
version 5.
Java to use OmniDriver. Our wrapper libraries take care of the Java code; we
provide Framework (Mac), Dynamic Link Library (Windows), Shared Object (Linux), .NET object
(Windows) and LabVIEW 7.0.
OmniDriver Components
OmniDriver is a fully functional cross-platform USB device driver library. It allows software to
communicate with any USB device on any Windows, Macintosh or Linux operating system. What
does it take to make such a robust driver? OmniDriver offers these components:
HighResTiming: Time stamping that is accurate to sub-microsecond performance; great for
chemical kinetics and other applications that require complex time accountability.
SPAM: You’ll want this SPAM. Spectral Processing and Manipulation performs all spectral
processing math from subtracting dark to radiometric color analysis. SPAM provides you with
the ability to harness spectral processing commands for your own applications but does not
require you to use Ocean Optics spectrometers or hardware. SPAM is available as a standalone module or as part of the OmniDriver package (OMNI+SPAM).
OMNIDRIVER:
SPAM:
OMNI+SPAM:
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$399
$199
$499
For all your sensing needs, visit OceanOptics.com
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SpecLine Software for Compound ID
Identifies Elements & Compounds
SpecLine Software is a powerful new tool designed
for identifying atomic emission lines and molecular
bands in spectral data. SpecLine’s advanced evaluation, search, compare and identify functions -- and its
extensive library of over 100 elements and over 400
compounds -- enable you to quickly identify unknown
lines, peaks and bands. SpecLine was designed for
scientists, engineers and researchers using emission
spectroscopy in fields such as astrophysics, the
plasma sciences, and plasma processing.
Searching and Comparing Data
In the Identify Lines window, you can search atoms from a Periodic Table, molecules
from an extensive list, and elements in single or multiple ionization states.
Identification
SpecLine applies a variety of sophisticated filter
functions such as Wiener-Fourier and polynomial
noise removal to identify the elements and
compounds in your spectra. After SpecLine applies
comparative searches to its extensive atomic, ionic
and molecular database of over 100 elements in
several ionization states and over 400 elemental
compounds, it provides detailed data on each
identified peak and line, such as the name of the
element, the peak’s wavelength, the electron voltage
and its transition state and quantum number.
Opening Spectra & Saving Data
SpecLine can analyze spectral data from various
spectroscopy software applications; it also can open
all Ocean Optics software file formats as well as SPC
and ASCII file formats. In addition, you can save all
of SpecLine’s identification data in its native file
format or export it into various applications, such as
Excel.
In this window, a search on the peaks and lines in a spectrum has been completed
and identified successfully.
Software & Data Acquisition
In the Line Identification window, you can define all
the parameters for your search in a Periodic Table
screen (top right), and begin the process with just a
single click. SpecLine can analyze even the most
complex spectral data, including spectra with double
lines, line shoulders and complex band structures. Up
to 12 separate spectra, even if they are in different
file formats, can be combined for comparative
purposes.
Hardware Keys
SpecLine Software comes with a USB or parallel-port
(printer port) hardware key. The key is a security
device to protect against unlicensed copies. It
connects to an input/output port on your computer
and must be used to run the software. SpecLine-U
comes with a USB hardware key for use with
Windows 98/2000/ME/XP operating systems (but not
Windows 95 or NT). SpecLine-P comes with a feedthrough parallel port hardware key.
OOISPECLINE-P: $3,510
OOISPECLINE-U: $3,510
Tel: 727.733.2447 • Email: [email protected]
This window demonstrates SpecLine’s ability to provide detailed data on just one
emission line.
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Analog-to-Digital Converters
ADC2000-PCI+ for PCI-bus
This A/D card has 2 MHz sampling frequency for data acquisition
within 2 milliseconds
Channel rotator function acquires data from up to eight
spectrometer channels simultaneously
Has standard modes for free-running operation and external trigger
modes for synchronizing external events
Processes full spectrum into memory every 5 milliseconds
Half-length, 12-bit A/D card fits easily into a PCI-bus slot in a PC
and connects to the spectrometer via a 1-meter CBL-2 cable
(included)
Additional PC slot protector provides eight digital inputs/outputs
and eight analog outputs (analog outputs incur additional fees)
Provides advanced features such as pixel rotation with no loss of
resolution
Software & Data Acquisition
ADC2000-PCI+: $699
CBL-2 Cable:
$50 (included)
ADC1000-USB for External USB
Easily connects to PCs via USB port or serial port
1 MHz sampling frequency enables acquisition of
data in 3 ms
Plugs directly into back of your existing spectrometer (as in
the main picture at right), or can be stacked or rack-mounted
with the spectrometer in the same housing (see insets, one
with housing and one without)
Channel rotator function enables simultaneous acquisition of
data from up to eight spectrometer channels
Has standard modes for free-running operation and external
trigger modes for synchronization of external events
Provides D-Sub-15 pass-through for triggering the
spectrometer and other accessories
ADC1000-USB:
USB-CBL-1 USB Cable:
ADC-USB-SER Serial Cable:
$599
$25 (included)
$49 (not included)
Specifications
Dimensions:
Weight:
Power consumption:
Sampling frequency:
Integration time:
Data transfer rate:
Programmable flash delay:
Inputs/Outputs:
Shutdown S2000 power:
Spectrometer compatibility:
Board architecture/design:
Operating systems:
Interface cable:
Software compatibility:
Multiple-channel capability:
A/D resolution/channels:
Rotator capability:
Trigger modes:
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ADC2000-PCI+
168.8 mm x 127.9 mm x 18.3 mm
90 g
250 mA @ 5 VDC
2 MHz (maximum)
2 milliseconds to 60 seconds
Full spectrum into memory every 4 milliseconds;
software time acquisition ~25 ms
0-65 seconds
8 digital I/Os
Yes
Supports S2000 Spectrometers
32 bit/PCI bus
Any 32-bit Windows operating system
ADC1000-USB
105.83 mm x 104.9 mm x 40.9 mm
230 g
150 mA @ 5 VDC
1 MHz (maximum)
3 milliseconds to 60 seconds
Via USB port, full spectrum into memory every 14 milliseconds;
via RS-232, full spectrum into memory every 300 milliseconds
0-255 milliseconds
8 analog outputs, requires ADC-1000-DAC
No
Supports S2000 and S1024DW Spectrometers
USB and RS-232 interface external A/D board
Via USB port, Windows 98/Me/2000/XP, Mac OS X and Linux
Via RS-232, any 32-bit Windows operating system
Via USB port, comes with 1-meter cable (USB-CBL-1) to connect ADC1000-USB to PC
Via RS-232, requires serial cable (not included, order ADC-USB-SER)
All 32-bit Ocean Optics Software
Comes with a 25-pin, 1-meter cable for connecting
the ADC2000-PCI+ to the spectrometer
All 32-bit Ocean Optics software, except SpectraSuite
and OmniDriver
Up to eight spectrometer channels
12 bit/up to 8 spectrometer channels
yes
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For all your sensing needs, visit OceanOptics.com
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Sampling Accessories
Collimating Lenses & Accessories
88
74-series & 84-series Lens Fixtures
89
Collimating Lens Holders
Cuvette Holders & Accessories
90
Cuvette Holders
91
Temperature-regulated Cuvette Holder
92
Integrated Sampling Systems
93
Cuvettes & Sample Cells
Systems for Fluid Analysis
Flow Cells for Flow Injection Analysis
Sequential Injection System
Process Flow Cells
SpectroPipetter Microcell
Longpass Flow Cells
Cell for Capillary Electrophoresis
Positive Displacement Pump
Fluorescence Sampling Tools
100
Sample Holders for Fluorescence
101
Fluorescence Flow Analysis System
101
Fiber Optic Scanning Monochromator
102
Semiconductor Nanocrystals
103
FluoroVette Micro-volume Cells
Light Collection Tools
104
Cosine Correctors for Emission Collection
104
Power Supply & Controller for LEDs
105
Integrating Spheres for Irradiance/Emission
Sampling Accessories
Sampling
94
95
96
98
98
99
99
Reflection Measurement Tools
106
Integrating Spheres for Reflectance
107
Diffuse Reflection Sampling
108
Specular Reflection Sampling
Tools for
109
110
111
111
112
Metrology
Reflection & Transmission Sample Systems
Optical Flats
Shear-plate Collimation Testers
Thin Film Reference Wafer
Long Trace Profilometer
Tools for
113
114
116
Filtering & Controlling Light
Filter Holders
Linear Variable Filters
Tools for Controlling Light
Mapping Tables & Positioners
118
XYZ Mapping Tables & Linear Nanopositioners
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Overview: Sampling Accessories
Sampling Accessories for Every Application
Sampling Accessories
Ocean Optics provides modular components that can be configured easily for
absorbance, transmission, reflectance, fluorescence, emission or scattering
experiments. Often the sampling accessory is where light or excitation energy
is collected from the light source, interacts with the sample, and sends the
absorbed/transmitted, reflected or emitted light to the spectrometer. Sampling
accessories also include the fixtures, such as collimating lenses, that provide
specific sampling geometries. Accessories and fibers can be combined in an
almost endless variety of configurations.
What’s Your Field of View?
Four of our devices are used to control field of view (FOV) and aperture:
Optical Fiber (25° FOV, aperture = fiber diameter)
Collimating Lens (0°-45° FOV, aperture = 3 mm)
Cosine Corrector (180° FOV, aperture = 3.9 mm)
Integrating Sphere (360° FOV, aperture = 25 mm)
Optical Fiber: 25°
Adjustable Collimating Lens: ~0-45°
Cosine Corrector: ~180°
Integrating Sphere: 360°
Partner Spotlight:
FIAlab Instruments
In 1987, Alitea USA was a distributor
of Alitea AB peristaltic pumps.
However, after demand for complete
flow injection systems quickly grew,
Alitea USA began to manufacture
their own instruments. These early
instruments are still widely used,
evident by frequent mentions in
scientific papers and conferences. In
1989, Alitea USA changed its name
to FIAlab Instruments and have since
introduced seven new state-of-the-art
flow injection and sequential
injection analysis systems, as well as
a line of flow cells, sample changers
and syringe pumps.
Innovative technology, top quality
components, and the highest level of
experience make FIAlab’s FIA and
SIA instruments the most advanced,
precise, compact and economical
available. Automation of reagentbased assays is critical to laboratory
research in chemistry, biotechnology,
drug screening and environmental
studies, as well as in process control
in industry. FIAlab brings quality and
precision to this automation. The
technical staff of FIAlab Instruments
have a unique level of expertise in
flow injection and sequential
injection analyses with more than
20 years of direct research.
All of FIAlab’s instruments are constructed with the best components
available. Alitea peristaltic pumps
ensure precise dispensing of fluids.
Cavro microsyringe pumps offer a
wide range of speeds and volumes.
Valco "intelligent" valves are robust
and highly reliable, and Upchurch
fittings come in a large variety of
chemically resistant and
biocompatible materials.
For more information on FIAlab
Instruments’ products, see pages
43-44, 94-95, and 100-101. You
can contact them directly at
800-963-1101 or visit their web
site at www.flowinjection.com.
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For all your sensing needs, visit OceanOptics.com
Sampling Accessories by Measurement Type
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Our fiber optic sampling accessories create the optical interface part of our modular spectrometer
systems. With so many sampling accessories from which to choose, you can meet the demands of a
variety of experiments for absorbance, transmission, fluorescence, reflectance and emission.
Absorbance/Transmission
1-cm Cuvette Holder, p. 90
10-cm Cuvette Holder,
p. 90
Longpass Flow Cells,
p. 98
Cuvettes, p. 93
Integrated Sampling
Systems, p. 92
LED Power Supply,
p. 104
Integrating Spheres,
p. 105
Collimating Lenses,
p. 88
Direct-attach Integrating
Sphere, p. 105
Temperature-regulated
Cuvette Holder, p. 91
EviDots and EviTags,
p. 102
Linear Variable Filters,
p. 114
Flow Cells,
p. 94
Integrating Spheres,
p. 106
Long Trace Profilometer,
p. 112
Reflection Stage, p. 109
Reflection Sampling
System, p. 109
Filter Holders,
p. 113
Linear Variable Filters,
p. 114
Gershun Tube Kit,
p. 116
Multiplexer,
p. 117
Emission
Sampling Accessories
Cosine Correctors,
p. 104
Fluorescence
4-way Cuvette Holder,
p. 100
Reflectance
Diffuse Reflectance
Standard, p. 107
Modifying Light
Variable Attenuator,
p. 117
Tel: 727.733.2447 • Email: [email protected]
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Collimating Lenses
74-series Lens Fixtures
The 74-series Collimating Lenses are the common fiber optic-coupled lens fixture used
throughout our extensive line of sampling accessories. The 74-series Collimating Lenses
have an inner barrel threaded for SMA 905 Connectors. (FC barrels are available for
$29; see page 158 for more.) The inner barrel slides relative to the lens fixture for
adjusting the focus; a setscrew secures the barrel. Adjustment from a converging to
diverging field of view (~45°) is possible.
74-UV Collimating Lens (200-2000 nm)
The 74-UV has an f/2 fused silica lens for 200-2000 nm. When focused for
collimation, beam divergence is 2° or less, depending on fiber diameter. The 74-UV
can be adjusted for UV-VIS or VIS-NIR setups.
Sampling Accessories
74-VIS Collimating Lens (350-2000 nm)
The 74-VIS -- the basic lens fixture in an LS-1 Light Source -- has a BK7 lens
suitable for the VIS-NIR. These single-lens systems have the disadvantage of
chromatic aberration, due to dispersion or variation in refractive index with
wavelength.
74-ACR Collimating Lens (350-2000 nm)
The 74-ACR has two optical elements cemented together to form an achromatic
doublet, optimized to correct for the spherical and chromatic aberrations inherent to
single-lens systems.
74-DA Collimating Lens (200-2000 nm)
The 74-DA screw-in lens attaches directly to spectrometers for increased light
throughput.
84-series Lens Fixture
The 84-series Collimating Lens is designed for coupling
larger free-space beams to fibers. The fiber is coupled to the
assembly with an inner 17.85-mm threaded barrel. The
barrel positions the fiber ~100 mm from the lens surface and
is adjusted to achieve a fine focus. The lens of the 84-UV-25
is especially suitable for collimating light at long distances in
open air (it’s been tested to distances of up to 40 feet).
The 84-UV-25 has an 8-32 tapped hole for attaching
to an optical post mount and then installing the
mount in an optical breadboard or other fixture
(at left).
Item
Diameter
Focal
Length
Material
Wavelength
Operating
Temp.
Connector
Price
74-UV
5 mm
10 mm
f/2 fused silica Dynasil
200-2000 nm
120 °C
SMA 905, 6.35-mm ferrule,
$159
3/8-24 external thread
74-VIS
5 mm
10 mm
f/2 BK7 glass
350-2000 nm
70 °C
SMA 905, 6.35-mm ferrule,
$159
3/8-24 external thread
74-DA
5 mm
10 mm
f/2 fused silica Dynasil
200-2000 nm
70 °C
SMA 905, 1/4-36 internal
$159
thread, 3/8-24 external thread
74-ACR
5 mm
10 mm
BaF10 and FD10
350-2000 nm
70 °C
SMA 905, 6.35-mm ferrule,
$199
3/8-24 external thread
84-UV-25
25.4 mm
100 mm
f/2 fused silica Dynasil
200-2000 nm
70 °C
SMA 905, 6.35-mm ferrule,
$499
3/8-24 external thread
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Collimating Lens Accessories
Right-angle Collimating Lens Holder
The 74-90-UV is an assembly for mounting lenses at right angles, and is especially
useful for applications involving awkward optical fiber routing. It is temperature rated
to 120 °C and has a mirror located under its cap that reflects light from the collimating
lens to 90°. Two ports accommodate 74-series Collimating Lenses (not included) and
an included adapter allows you to mount the 74-90-UV in male or female ports.
74-90-UV: $139
Adjustable Collimating Lens Holders
The 74-ACH Adjustable Collimating Lens Holder consists of
adjustable bars with several threaded holes for collimating
lenses. The bars can be set far enough apart to accept samples
up to ~100 mm thick, making the 74-ACH a convenient
option for transmission measurements of large samples.
(Collimating lenses are not included.)
The 74-90-UV
comes with a
threaded
adapter. It
can be used
for routing light
around corners.
74-ACH
Adjustable
Collimating
Lens Holder
Sampling Accessories
The ACH-CUV-VAR Adjustable Collimating Lens and
Cuvette Holder is two products in one: a fixture for
positioning collimating lenses at various heights or for
holding extra-large or especially thick samples, and a
holder for accepting cuvettes for transmission
measurements. Its adjustable mount bars accept samples
up to ~150 mm thick and its threaded holes hold collimating
lenses. (Two 74-UV Collimating Lenses are included.)
74-ACH:
$299
ACH-CUV-VAR: $1,439
ACH-CUV-VAR Adjustable
Collimating Lens and Cuvette Holder
Optical Post-mount Assembly
Also available is the OPM-M, which is a post-mount assembly for optical
tables with metric M6 grids. The OPM-M has a lens holder (for a 74-UV
Collimating Lens), an M4 metric optical post and an M6 metric post holder.
OPM-M: $180
OPM-M Optical
Post Mount
Assembly
Optical Post Mount & Optical Posts
The OPM-SMA is a fixture for mounting 74-series Collimating Lenses and
SMA 905-terminated optical fibers. The OPM-SMA consists of a 1.5" OD disk
with 3/8-24 threads to accommodate the lenses. You can use the OPM-SMA
with SMA 905-terminated optical fibers. The OPM-SMA includes 8-32
(Imperial) and M6 (metric) threads for attaching to an optical post.
OPM-1, OPM-2 and
OPM-4 Optical Posts
We offer four optical posts (in 25.4-mm, 50.8-mm, 76.2-mm and 101.6-mm
heights) to attach to the OPM-SMA. These posts screw into optical breadboards via a 1/4-20 tapped hole in the bottom of each post.
OPM-SMA:
$149
OPM-1, -2, -3, -4: $15 each
OPM-SMA
Optical Post Mount
Specifications
Material:
74-90-UV
16.5 x 16.5 x 19.9
11.3 g
3/8-24 (ports)
9.525 x 25.4 mm (nipple)
Black anodized Al
Collimating lens included:
No
Dimensions (in mm):
Weight:
Threads:
74-ACH
152.4 x 76.2 x 152.4
890.2 g
3/8-24 (mounting bars)
10-32 (setscrews for base)
Blue anodized Al (base)
Black anodized Al (bars)
No
Tel: 727.733.2447 • Email: [email protected]
ACH-CUV-VAR
200 x 67 x 157
1,000 g
3/8-24 (mounting bars)
M6 (setscrews for base)
Black anodized Al (base)
Black anodized Al (bars)
(2) 74-UV Lenses
OPM-SMA
38.1 OD x 10.2 width
130 g (including post)
3/8-24 (lens holder)
8-32 (bore for mounting)
Black anodized Al (mount)
Stainless steel (post)
No
OPM-M
30 mm OD x 6.5 width
220 g (including post)
3/8-24 (lens holder)
M4 (bore for mounting)
Black anodized Al (mount)
Stainless steel (post)
No
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Cuvette Holders
CUV-UV Cuvette Holder
The CUV-UV (200-2000 nm) couples to lamps and spectrometers to create
absorbance or transmission measurement systems. Two 74-UV lenses are
mounted across a cell holder for square 1-cm cuvettes. The base includes
channels for connection to a water bath for temperature regulation. The unit
also accepts filters. An optional cover (CUV-COVER) excludes ambient light.
CUV-UV: $399
CUV-UV-10 Cuvette Holder
The CUV-UV-10 (200-2000 nm) accepts 10-cm cylindrical or flat-bottomed
cuvettes. The CUV-UV-10 has two 74-UV Collimating Lenses that couple to
light sources and spectrometers via optical fiber to make absolute absorbance
systems for solutions and gases. Included is a shutter, a clamp for filters, water
channels for temperature regulation, and a cover to exclude ambient light.
CUV-UV-10: $549
CUV-ALL-UV 4-way Cuvette Holder
Sampling Accessories
The CUV-ALL-UV provides ports for 1-cm cuvettes from four directions.
Position two collimators at 180° for absolute absorbance and transmission
measurements, position two collimators at 90° for fluorescence or scattering,
or use all four for simultaneous absorbance and fluorescence measurements.
For fluorescence applications, increase the signal by replacing
collimators with 74-MSP Mirror Plugs (see inset), which redirect
energy back to the sample or back into a collimating lens.
CUV-ALL-UV: $809
74-MSP:
$99
CUV-FL-DA Direct-attach Cuvette Holder
The CUV-FL-DA attaches to our light sources and couples via fibers to our
spectrometers, creating systems for fluorescence and relative absorbance. The
holder has a collimating lens and two mirrored screw plugs (74-MSP), which
can be positioned per your application. A 6.35-mm slot is included for filters.
CUV-FL-DA: $399
CUV-VAR Variable Pathlength Cuvette Holder
The CUV-VAR has three functions: use its cuvette holder insert to create a
1-10 cm pathlength cuvette holder, create a 2-mm pathlength filter holder, or
position its two 74-UV collimators to accept a flow cell. The included
collimators are screwed into fixtures that slide along the base and can be set
to create pathlengths up to 10 cm. Also available is a flow-cell adapter option
(CUV-VAR-OPTION) for the CUV-VAR.
CUV-VAR:
$1,291
CUV-VAR-OPTION: $399
Specifications
Dimensions:
Weight:
Pathlength:
Filter slot:
Water input fittings:
Collimating lenses:
Fiber termination:
“Z” dimension:
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CUV-UV
58 mm x 140 mm x 38 mm
230 g
1 cm
Up to 6 mm, screw clamp
3.175-mm (1/8") NPT
2 each 74-UV
SMA 905
15 mm
CUV-UV-10
97 mm x 248 mm x 50 mm
1,040 g
10 cm
Up to 6 mm, wheel clamp
3.175-mm (1/8") NPT
2 each 74-UV
SMA 905
15 mm
CUV-ALL-UV
147 mm x 147 mm x 40 mm
540 g
1 cm
Up to 6 mm, screw clamp
3.175-mm (1/8") NPT
4 each 74-UV
SMA 905
15 mm
CUV-FL-DA
57 mm x 61 mm x 29 mm
80 g
1 cm
Up to 6 mm, screw clamp
none
2 each 74-UV
SMA 905
15 mm
CUV-VAR
200 mm x 67 mm x 70 mm
726 g
1 cm up to 10 cm
none
none
2 each 74-UV
SMA 905
15 mm
For all your sensing needs, visit OceanOptics.com
Temperature-regulated Cuvette Holder
Precise Temperature Control
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The CUV-TLC-50F Temperature-regulated Cuvette Holder is
a high-quality, versatile sample chamber with a Peltier
temperature controller calibrated against a NIST-traceable
thermometer. The device controls the temperature of the
holder from -55 °C to +105 °C and maintains a constant
temperature to within ± 0.02 °C. The CUV-TLC-50F includes
the cuvette holder and the external temperature controller
box. To run the thermoelectric cooler efficiently, we offer a
simple water pump and a water container.
Absorbance or Fluorescence
The CUV-TLC-50F (200-2000 nm) provides ports for viewing
or illuminating 1-cm square cuvettes from four directions.
Lenses are purchased separately to allow you to choose the
best lenses for your application. For absorbance and
transmission measurements, position two CUV-TLC-CL
Collimating Lenses at 180°. For fluorescence applications,
position two CUV-TLC-IL Imaging Lenses at 90° and position
two CUV-TLC-MP Mirror Plugs in the remaining two
collimator positions for increasing light throughput.
A Collimating
Lens (far left)
and Mirror Plug.
3
7
4
Additional Features
A dry gas purge rids the chamber of condensation when
operating at low temperatures or excludes O2 (tubing
for water and gas connections are included)
Variable-speed magnetic stirring (a stir bar is included)
Several removable optical slits included for modifying
light entering and/or leaving the sample chamber
Slots for removable slits at each collimating lens port
PC Adapter Package
An optional CUV-TLC-ADP adapter package comes with
Windows-compatible software that allows you to remotely
start a test sequence, operate the controller box and monitor
experiments. Without the CUV-TLC-ADP, you can control the
holder’s temperature mechanically from the controller box.
2
Another option is
the CUV-TLC-FH
Filter Holder.
An absorbance setup might include the USB2000 or USB4000
Spectrometer, an LS-1 Light
Source and two optical fibers.
6
Sampling Accessories
The CUV-TLC-IJ
Insulation Jacket.
5
Specifications
Full (maximum) temperature range:
Normal temperature range:
Precision:
Reproducibility:
Maximum illuminated area:
“Z” dimension:
Item
-55 °C to +105 °C
0 °C to 85 °C
± 0.02 °C
± 0.05 °C
12 x 10 mm
8.5 mm
The CUV-TLC-50F includes the
controller box and the cuvette
holder. Optical fibers and the
CUV-TLC-BATH are separate.
Description
Price
1 CUV-TLC-50F
Fiber optic temperature-controlled cuvette holder and controller box with slits, magnetic stirrer and tubing
$3,820
2 CUV-TLC-FH
Filter holder for the CUV-TLC-50F
$470
3 CUV-TLC-CL
AR-coated fused-silica collimating lens with SMA 905 Connector (comes with steering plate)
$180
4 CUV-TLC-MP
Mirror plug for use with CUV-TLC-IL when conducting fluorescence measurements
$70
5 CUV-TLC-ADP
Optional PC adapter package for remotely operating the cuvette holder (serial cable included)
$95
6 CUV-TLC-BATH
Water pump and bucket for running the thermoelectric cooler efficiently
7 CUV-TLC-IJ
Insulating jacket for the CUV-TLC-50F
$175
CUV-TLC-IL
Imaging or focusing lens snaps onto CL collimating lens with SMA 905 Connector (comes with steering plate)
$290
CUV-TLC-SP
Steering plate that mounts a lens or mirror plug onto the cuvette holder
CUV-TLC-ABSKIT
A kit for absorbance/transmission; contains CUV-TLC-50F, CUV-TLC-ADP, two CUV-TLC-CL, CUV-TLC-BATH
$4,374
CUV-TLC-FLKIT
A kit for fluorescence; contains the CUV-TLC-50F, the CUV-TLC-ADP, two CUV-TLC-IL, two CUV-TLC-MP, two
$4,834
$99
$50
CUV-TLC-SP, CUV-TLC-BATH
CUV-TLC-MPKIT
A kit with all of the items necessary for absorbance/transmission and fluorescence
Tel: 727.733.2447 • Email: [email protected]
$4,964
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Integrated Sampling Systems
An Integrated Sampling System is a spectroscopy accessory where the light source and sample
compartments have been integrated into one package. These systems perform the same function as
our cuvette holders, but have an advantage in that one or both fibers are eliminated from the setup.
USB-ISS-UV-VIS Integrated Sampling System
The USB-ISS-UV-VIS Integrated Sampling System is a direct-attach sample
holder and deuterium tungsten halogen light source for 1-cm square
cuvettes. The USB-ISS-UV-VIS attaches directly to USB2000 and USB4000
Spectrometers. The sampling system allows you to adjust the intensity of
the bulb via software. The sampling system has an electronic shutter for
taking dark measurements and comes with a 5-volt power supply.
USB-ISS-UV-VIS: $1,499
USB-ISS-VIS Integrated Sampling Systems
Sampling Accessories
The USB-ISS-VIS and USB-ISS-T both have a violet LED-boosted tungsten
source and a sample holder that bolts to the front of a USB2000 or
USB4000 Spectrometer, which provides the power and control signals
for the light source. The USB-ISS-VIS holds 1-cm cuvettes while the
USB-ISS-T holds 12-mm OD test tubes. Both sampling systems cover the
390-900 nm range.
USB-ISS-VIS:
$499
USB-ISS-T:
$499
ISS-UV-VIS Integrated Sampling System
The ISS-UV-VIS combines a light source with a 1-cm cuvette holder for
absorbance measurements. The ultraviolet light is provided by a
deuterium bulb; visible light from a tungsten halogen bulb is focused
through the deuterium lamp onto a diffuser. Solarization-resistant fiber
(not included) is recommended. A 12 VDC wall transformer is included.
ISS-UV-VIS: $1,599
ISS-2 Integrated Sampling System
The ISS-2 Integrated Sampling System is a 1-cm cuvette holder and
tungsten halogen light source. The ISS-2 combines the light source
with a diffuser on the illumination side and a collimating lens on the
receiving side of the cuvette holder. A fiber (not included) connects
the ISS-2 to a spectrometer to create a small-footprint system for VIS-NIR
absorbance measurements. A 12 VDC wall transformer is included.
ISS-2: $799
Specifications
Dimensions (mm):
Weight:
Power consumption:
Wavelength range (source)*:
Pathlength:
Cuvette shape:
Light source:
Bulb life (hours):
Time to stabilized output:
Filter slot:
Recommended optical fibers:
Spectrometers:
“Z” dimension:
USB-ISS-UV-VIS
198 x 105.1 x 40.6
200 g
1.8 A @ 5 VDC
200-2000 nm
1 cm
Square
Deuterium tungsten
800 (deut.); 2,000 (tung.)
~30 minutes
None
None
USB2000 and USB4000
15 mm
USB-ISS-VIS
40.7 x 88.8 x 34.1
130 g
160 mA @ 5 VDC
390-2000 nm
1 cm
Square
Tungsten and violet LED
45,000
~5 minutes
None
None
USB2000 and USB4000
15 mm
USB-ISS-T
40.7 x 88.8 x 34.1
130 g
160 mA @ 5 VDC
390-2000 nm
12 mm OD
Round test tube
Tungsten and violet LED
45,000
~5 minutes
None
None
USB2000 and USB4000
15 mm
ISS-UV-VIS
198 x 104.9 x 40.9
400 g
420 mA @ 12 VDC
200-2000 nm
1 cm
Square
Deuterium tungsten
800 (deut.); 2,000 (tung.)
~30 minutes
None
QP400-025-SR
All
15 mm
ISS-2
155 x 50 x 53.3
240 g
600 mA @ 12 VDC
400-2000 nm
1 cm
Square
Tungsten
900
~30 minutes
6.35 mm
QP400-2-UV-VIS
All
15 mm
* The wavelength range of the source may exceed the wavelength range of your spectrometer.
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For all your sensing needs, visit OceanOptics.com
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Cuvettes & Sample Cells
Disposable UV & VIS Cuvettes
Cuvette Covers
Our CVD-series Disposable Cuvettes are a low-cost, no-maintenance alternative to quartz
cuvettes. All cuvettes have a 1-cm pathlength, 220-900 nm or 350-900 nm wavelength range
coverage, and various filling volumes.
CVD-UV1S
CVD-UV1U
CVD-VIS1S
CVD-VIS1M
Disposable cuvette covers
(top) come in packs of 100.
CVD-ROUND-RB:
$20
CVD-ROUND-RG:
$20
CVD-ROUND-RO:
$20
CVD-ROUND-RY:
$20
CVD-COVER (square): $20
Item
Range
Material
Volume
Window Clear
in mm
Sides*
Cover
Needed
CVD-UV1S (100 pk)
220-900 nm
Plastic
1.5-3.0 mL
4.5 x 23
4*
square
$63
220-900 nm
Plastic
70 µL-1.8 mL
2 x 3.5
2
round
$63
CVD-VIS1S (100 pk)
350-900 nm
Polystyrene
1.5-3.0 mL
5 x 23
4*
square
$13
CVD-VIS1M (100 pk)
350-900 nm
Polystyrene
2.5-4.0 mL
10 x 35
2
square
$14
CVD-UV1S-SAM (8 pk)
CVD-UV1U (100 pk)
Price
$10
CVD-UV1U-SAM (8 pk)
$10
one of our black anodized
covers.
CUV-COVER:
$25
CUV-COVER-TALL:
$30
Sampling Accessories
* Cuvettes with 4 clear sides are suitable for fluorescence measurements. Cuvettes with 2 clear sides are for
“straight-through” absorbance and transmission measurements.
To block ambient light, use
Quartz Cuvette Cells
We offer several popular Suprasil quartz cuvettes made by Starna, including macro, semi-micro, flow and
cylindrical cells. If you need a cell not listed here, you can order it through Ocean Optics using the Starna catalog
number (see Starna.com for details). The cells listed here are suitable for use from 200-2700 nm.
CV-Q-10
CVFL-Q-10
CVS-Q-10
CVF-Q-10
CV-Q-100
Item
Description
Windows
Path
Lid
Exterior (mm)
Volume
CV-Q-10
Standard
2 clear
10 mm
Teflon cover
12.5 x 12.5 x 45
3.5 mL
Price
$75
CVFL-Q-10
Fluorescence
4 clear
10 mm
Teflon stopper
12.5 x 12.5 x 45
3.5 mL
$149
$219
CVS-Q-10
Self-masking
2 clear
10 mm
Teflon stopper
12.5 x 12.5 x 48
1.4 mL
CVF-Q-10
Flow cell
2 clear
10 mm
M6 screws
12.5 x 12.5 x 35
0.42 mL
$369
CV-Q-100
Cylindrical
2 clear
100 mm
Teflon stoppers
22 OD x 102.5
28.2 mL
$165
Photometric Absorbance Standards
STAN-ABS Absorbance Standards are used to check the photometric accuracy of
spectrophotometer systems. Data charts and NIST-traceable certificates of analysis come
with each kit. Each kit consists of a background reference and low, medium and high
absorbance solutions, each 125 mL in volume. These polymer-based standards utilize
submicron, non-surface charged, solid spheres in ultrapure water. The STAN-ABS-UV is
certified for wavelengths from 200-450 nm, while the STAN-ABS-VIS covers wavelengths
from 400-900 nm.
STAN-ABS-UV:
$370
STAN-ABS-VIS: $370
Tel: 727.733.2447 • Email: [email protected]
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Flow Cells for Flow Injection Analysis
We offer several optical flow cells with a “Z” configuration, to
measure the optical absorbance of fluids. Couple them to our
spectrometers to monitor chemical or biological processes, and
immunoassays.
In the FIA-Z-SMA Flow Cells, standard optical fibers (available
separately) connect to SMA 905 fittings to transmit and receive
light through the central axis of the Z. The FIA-Z-SMA Cells use
silica windows as wetting surfaces at each fiber optic junction, and are
available in PEEK polymer, Plexiglas, stainless steel, Teflon and Ultem.
Common optical pathlengths are listed below. (Microvolume as well as ultrashort pathlength cells are also available. Contact Ocean Optics for details.)
In this setup, a FIA-Z-SMA-ULT
10-mm pathlength flow cell is
in-between a light source and
spectrometer. Tubing and
connectors are included.
The FIA-Z-CELL Flow Cells are different from the FIA-Z-SMAs; instead of windows
they use optical fibers in 1.58-mm ferrules, a design that allows you to slide the
ferrules in and out of the cell to adjust the optical pathlength from 0-10 mm.
Sampling Accessories
Item
Description
Pathlength
Cell Material
Fiber Type
Needed
Price
FIA-Z-SMA-PEEK
Z Flow Cell with SMA 905 Connectors
10 mm
PEEK
Standard
$529
FIA-Z-SMA-PLEX
Z Flow Cell with SMA 905 Connectors
10 mm
Plexiglas
Standard
$529
FIA-Z-SMA-SS
Z Flow Cell with SMA 905 Connectors
10 mm
Stainless steel
Standard
$529
FIA-Z-SMA-TEF
Z Flow Cell with SMA 905 Connectors
10 mm
Teflon
Standard
$529
FIA-Z-SMA-ULT
Z Flow Cell with SMA 905 Connectors
10 mm
Ultem
Standard
$529
FIA-Z-SMA-20-PE
Z Flow Cell with SMA 905 Connectors
20 mm
PEEK
Standard
$529
FIA-Z-SMA-20-PLE
Z Flow Cell with SMA 905 Connectors
20 mm
Plexiglas
Standard
$529
FIA-Z-SMA-20-SS
Z Flow Cell with SMA 905 Connectors
20 mm
Stainless steel
Standard
$529
FIA-Z-SMA-20-TEF
Z Flow Cell with SMA 905 Connectors
20 mm
Teflon
Standard
$529
FIA-Z-SMA-20-ULT
Z Flow Cell with SMA 905 Connectors
20 mm
Ultem
Standard
$529
FIA-Z-SMA-50-PE
Z Flow Cell with SMA 905 Connectors
50 mm
PEEK
Standard
$629
FIA-Z-SMA-50-PLE
Z Flow Cell with SMA 905 Connectors
50 mm
Plexiglas
Standard
$629
FIA-Z-SMA-50-SS
Z Flow Cell with SMA 905 Connectors
50 mm
Stainless steel
Standard
$629
FIA-Z-SMA-50-TEF
Z Flow Cell with SMA 905 Connectors
50 mm
Teflon
Standard
$629
FIA-Z-SMA-50-ULT
Z Flow Cell with SMA 905 Connectors
50 mm
Ultem
Standard
$629
FIA-Z-SMA-100-PE
Z Flow Cell with SMA 905 Connectors
100 mm
PEEK
Standard
$729
FIA-Z-SMA-100-PLE
Z Flow Cell with SMA 905 Connectors
100 mm
Plexiglas
Standard
$729
FIA-Z-SMA-100-SS
Z Flow Cell with SMA 905 Connectors
100 mm
Stainless steel
Standard
$729
FIA-Z-SMA-100-TEF
Z Flow Cell with SMA 905 Connectors
100 mm
Teflon
Standard
$729
FIA-Z-SMA-100-ULT
Z Flow Cell with SMA 905 Connectors
100 mm
Ultem
Standard
$729
FIA-Z-CELL-PEEK
Z Flow Cell with ferrules
10 mm
PEEK
Ferruled
$365
FIA-Z-CELL-PLEX
Z Flow Cell with ferrules
10 mm
Plexiglas
Ferruled
$365
FIA-Z-CELL-SS
Z Flow Cell with ferrules
10 mm
Stainless steel
Ferruled
$365
FIA-Z-CELL-TEF
Z Flow Cell with ferrules
10 mm
Teflon
Ferruled
$365
This FIA-Z-SMA-100-ULT is a
100 mm pathlength cell made
out of Ultem.
Specifications
Cell materials:
PEEK, Plexiglas, Teflon, stainless steel
or Ultem
Inner diameter:
1.5 mm
Window material:
UV-grade fused silica
Window thickness: 1 mm
Wavelength range:
FIA connectors:
Tubing:
Fiber connectors:
200-2000 nm
1/4-28 fittings (included)
1/16" Teflon, ~3 m
SMA 905 for FIA-Z-SMA cells; 1.58-mm
stainless steel ferrules for FIA-Z-CELL cells
Our standard fibers are designed
for the FIA-Z-SMA cells.
Fibers for Use with FIA Cells
An FIA-Z-SMA requires two 200 µm or 400 µm diameter fiber assemblies like the ones listed
below. (Your application may require optical fibers optimized for a specific wavelength range.
See pages 142-146 for more choices.) The FIA-ZCELL requires two fiber assemblies with
ferrule terminations. Each price below is for one assembly (two are required).
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Item
Description
For Use With
P400-2-UV-VIS
(1) 400 µm fiber assembly with SMA 905 Connectors
FIA-Z-SMA
P200-2-UV-VIS
(1) 200 µm fiber assembly with SMA 905 Connectors
FIA-Z-SMA
FIA-P400-SR
(1) 400 µm fiber assembly with ferrule terminations
FIA-Z-CELL
$215
FIA-P200-SR
(1) 200 µm fiber assembly with ferrule terminations
FIA-Z-CELL
$210
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Price
$119
$99
The FIA-P400-SR and FIA-P200-SR
fiber assemblies have ferrules for
use with the FIA-Z-CELL cells.
For all your sensing needs, visit OceanOptics.com
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Sequential Injection System
Lab-On-Valve Technology
The FIA-SIA-LOV Lab-On-Valve System is a compact sequential
injection analyzer for all-in-one chemical analyses. It combines a
computer-controlled six-position valve, precision syringe pump, and
spectrophotometric flow cell that can automate many wet-chemistry
lab procedures. All of the chemistry takes place within the valve
manifold -- eliminating the need for additional tubing and
connectors. All of the ports are interconnected by
microchannels, and a built-in flow cell interfaces to
optical fiber probes for spectral analyses in either
absorbance or fluorescence mode.
The system includes
a six-valve manifold unit,
syringe pump and valve,
and comes with tubing,
various connectors and other
fluidics parts. Spectrometer
and light source are
purchased separately.
Automate Wet Lab Procedures
The FIA-SIA-LOV includes software and interfaces to a PC, allowing
you to fully automate wet lab procedures with precise control of
assay parameters such as flowrates and volumes. Via the software,
you assign each of the Lab-On-Valve's ports a specific function.
Cost-effective Methodology
The FIA-SIA-LOV offers a cost-effective, microliter-volume
methodology -- it produces less waste, saves money and introduces
fewer chemicals into the environment than other wet chemistry
technologies. The unit weighs 3.6 kg, making it portable and easy to
install in small incubators for temperature and humidity control. Also,
the FIA-SIA-LOV can easily be positioned near ETAAS and MS
systems so that samples are not transported through long conduits,
which can cause sample degradation.
Bead trapping
Flow injection
Flow through
Holding coil
Mixing
Reagent aspiration
Sample dilution
Sample aspiration
Sequential injection
Waste elimination
Specifications
Dimensions:
Weight:
Spectral range:
Cell materials:
Inner diameter:
Window material:
Window thickness:
Pathlength:
Fiber connectors:
Tubing:
Tubing connectors:
Pump dimensions:
Pump weight:
Flow rate:
Pressure rating:
12.7 cm x 15.3 cm x 15.3 cm
3.6 kg
260-2000 nm
PEEK, Plexiglas, Teflon, stainless steel or Ultem
1.5 mm
UV-grade fused silica
1 mm
10 mm
SMA 905
1/16" Teflon, ~3 m
1/4-28
105 mm x 105 mm x 185 mm
2.1 kg
200 mL/minute/channel (depends on RPM an
tubing diameter)
25 psi
Modular Chemical Analyzer
The FIA-SIA-LOV unit was developed by flow injection system
specialist and Ocean Optics partner FIAlab Instruments. It is
compatible with our spectrometers and accessories for dynamic
spectral analyses of absorbance or fluorescence of fluids. The FIASIA-LOV consists of the FIA-SIA Micro Sequential Injection Analyzer
unit and the FIA-LOV Lab-on-a-Valve Manifold, each of which can be
purchased separately.
FIA-SIA-LOV: $13,450
FIA-SIA:
$10,950
FIA-LOV:
$1,275
Sampling Accessories
Control many assay parameters including:
Flow Cell Kit for Flow Injection Analysis
FIA-PUMP-C 2-channel
peristaltic pump.
The FIA-1000-Z Flow Cell Kit is a fluid sampling system that couples
to our spectrometers and light sources for rapid, quantitative analysis
of solutions. The kit consists of an FIA-Z-SMA flow cell (see page 94
for details), tubing and fittings, the FIA-PUMP-C (a computercontrolled 2-channel peristaltic pump), and software to control the
pump via a PC’s serial port. Two optical fibers (not included) are
required. You can also purchase the FIA-PUMP-C pump separately.
FIA-1000-Z: $1,470
FIA-PUMP-C:
$974
FIA-Z-SMA “Z”-type flow cell in Ultem.
Specifications
Spectral range:
Cell materials:
Inner diameter:
Window:
Pathlength:
260-2000 nm
PEEK, Plexiglas, Teflon, stainless steel or Ultem (shown)
1.5 mm
1 mm thick, UV-grade fused silica
10 mm
Tel: 727.733.2447 • Email: [email protected]
Pathlength:
Tubing:
Pump:
Flow rate:
Pressure rating:
10 mm
1/16" Teflon, ~3 m, with 1/4-28 connectors
105 mm x 105 mm x 185 mm; 2.1 kg
200 mL/minute/channel, depends on RPM and tubing diameter
25 psi
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Process Flow Cells
About Custom Sensors & Technology
Custom Sensors & Technology, Inc. is a full-service designer and manufacturer of photometric
transmitters, fiber optic probes and flow cells, oxygen transmitters, sampling handling systems and
other products for process applications. In addition, Custom Sensors & Technology offers applications
assistance, product validation and other services. Their process flow cells can easily be connected to
our spectrometers for spectral analysis of samples in online process applications.
Cross Process Flow Cells
The Adjustable-pathlength Cross Process Flow Cells are used in a variety of demanding
online flow analysis applications in industrial gas or liquid stream environments. The 1/2"
and 3/8" cells are available in various materials and have adjustable pathlengths.
Sampling Accessories
The 1/2" version has a pathlength that can easily be adjusted from 0.1-2.5 cm. This
version comes with two Optical Interface Couplers that collimate light and easily connect
optical fiber assemblies to the flow cell, spectrometer and light source. Also available is
a version that has a viewport; call for details.
The 3/8" version has a pathlength that can be adjusted from 0.1-1.5 cm. It does not
include Optical Interface Couplers but they can be purchased separately. The
PRO-CFC-3/8's titanium body (standard) allows the cell to be used in highly aggressive
process streams such as those often encountered in pulp and paper applications.
PRO-CFC-1/2:
$3,250
PRO-CFC-3/8:
$3,096
Micro Process Flow Cells
Process-ready Micro Flow Cells are useful for online measurements in gas or
liquid streams in demanding industrial environments The cells provide
extremely small pathlengths (to 0.02 mm) without restricting sample flow. Micro
Flow Cells are available in 1/8" and 3/8" sizes and have adjustable
pathlengths.
The PRO-MFC-OIC-VP
includes a viewport for
viewing the sample as it
flows through the cell. See a
close-up of the
viewport below.
The PRO-MFC is a 3/8" Micro Flow Cell. The PRO-MFC-OIC is a 1/8" Micro
Flow Cell that can be used in a variety of online flow analysis applications. The
PRO-MFC-OIC-VP includes a quartz port that allows the user to view the setting
and the sample as it flows through the cells. The PRO-MFC-S Sanitary Micro
Flow Cell is designed for online flow analysis applications to 200 AU/CM and
has high absorption characteristics from 200-2000 nm. Constructed of 316
stainless steel, the cell is available with outer diameters from 0.5" to 2.0".
PRO-MFC:
$2,675
PRO-MFC-OIC:
$5,400
PRO-MFC-OIC-VP: $6,000
PRO-MFC-S:
$5,250
Specifications
PRO-CFC-1/2
Adjustable 0.1-2.5 cm
316 stainless steel
(Hastelloy C, Titanium
and Monel available)
Sample inlet/outlet: 1/2" compression fittings
Window materials: Quartz (Sapphire
available)
Seals:
Viton (Chemraz and
Kalrez available)
PRO-CFC-3/8
Adjustable 0.1-2.5 cm
316 stainless steel
(Hastelloy C, Titanium
and Monel available)
3/8" compression fittings
Quartz (Sapphire
available)
Viton (Chemraz and
Kalrez available)
Temperature limit:
Pathlength:
Body & barrel:
204 °C (400 °F)
Pressure limit:
2000 psig
Fiber connections: SMA 905
Wavelength range: UV-NIR
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204 °C (400 °F)
PRO-MFC
Adjustable 0.02-2.0 mm
Titanium (316 stainless
steel, Hastelloy C and
Monel available)
3/8" compression fittings
Quartz (Sapphire
available)
Viton (Chemraz,
Kalrez, TFE,
Buna-N available)
121 °C (250 °F)
PRO-MFC-OIC
PRO-MFC-OIC-VP
Adjustable 0.02-2.0 mm Adjustable 0.02-2.0 mm
316 stainless steel
316 stainless steel
Viton (Chemraz,
Kalrez, TFE, Buna-N
available)
121 °C (250 °F)
Viton (Chemraz,
Kalrez, TFE, Buna-N
available)
121 °C (250 °F)
2000 psig
SMA 905
UV-NIR
1000 psig
SMA 905
UV-NIR
250 psig
SMA 905
UV-NIR
250 psig
SMA 905
UV-NIR
PRO-MFC-S
0.02-2.0 mm
316 stainless steel;
wetted body
1/8" compression fittings 1/8" compression fittings 1/8" compression fittings
Quartz
Quartz
Quartz
Sample end: B-type VCO
L-Ring Face Seal Fitting;
Process end: Tri-Clamp
149-232 °C (300-450 °F)
depending on gasket
2500 psig (137 Bar)
SMA 905
UV-NIR
For all your sensing needs, visit OceanOptics.com
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Process Flow Cells
Fluorescence Process Flow Cells
The PRO-FC-FL+TR Fluorescence Flow Cell is an adjustablepathlength fluorescence flow cell that can be used for fluorescence
and transmission measurements in a variety of industrial online flow
analysis applications. The PRO-FC-FL+TR can be configured with
Optical Interface Couplers (three OICs included) at 90° for
fluorescence applications. Add a third OIC at 180° to make
transmission and fluorescence measurements simultaneously.
The cell's pathlength can easily be adjusted from 0.5-15.0 mm.
PRO-FC-FL+TR:
$3,750
End-of-Column Process Flow Cells
Sampling Accessories
The Biotech End-of-Column Flow Cell is an adjustable-pathlength flow
cell for optical measurements in a variety of industrial online flow
analysis applications. The stainless steel PRO-FC-BIO is a Titanium
cell body that features an electropolished (RA 12 or better) interior
and two fiber-lensed Optical Interface Couplers (included). OICs and
sample inlet/outlet are secured in the cell body with standard
Upchurch fittings. The cell's pathlength can easily be adjusted from
0.02-10.0 mm.
PRO-FC-BIO:
$2,572
Long Pathlength Process Flow Cells
The PRO-FC-LP Long Pathlength Process Flow Cell can be used
in a variety of online flow analysis applications when longer
pathlengths are required. The PRO-FC-LP is available in
pathlengths from 50-500 mm. Contact an Applications Scientist
for detailed ordering information. Two Optical Interface
Couplers (included) collimate light and easily connect fiber
optic cables to the flow cell, spectrometer and light source.
PRO-FC-LP:
$3,145
Specifications
Pathlength:
Body & barrel material:
Sample inlet/outlet:
Window materials:
Seals:
Temperature limit:
Pressure limit:
Fiber connections:
Wavelength range:
PRO-FC-LP
50-500 mm
316 stainless steel (Hastelloy C, Titanium
and Monel available)
3/4" compression fittings
Quartz (Sapphire available)
Viton (Chemraz, Kalrez,
TFE, Buna-N available)
400 °F, 205 °C
2500 psig
SMA 905
UV-NIR
PRO-FC-FL+TR
0.5-15.0 mm
316 stainless steel (Hastelloy C, Titanium
and Monel available)
1/2" compression fittings
Quartz (Sapphire available)
Viton (Chemraz, Kalrez,
TFE, Buna-N available)
400 °F, 205 °C
2500 psig
SMA 905
UV-NIR
Tel: 727.733.2447 • Email: [email protected]
PRO-FC-BIO
0.02-10.0 mm
316 stainless steel (Hastelloy C, Titanium
and Monel available)
1/8" Upchurch compression fittings
Quartz (Sapphire available)
Viton (Chemraz, Kalrez,
TFE, Buna-N available)
200 °F, 93 °C
250 psig
SMA 905
UV-NIR
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SpectroPipetter Microcell
Easy to Use -- Just Pipette and Measure
The PIP-10-2 SpectroPipetter Microcell is a combination micropipetter
and 10-mm pathlength microcell for low-volume sampling.
Samples are loaded into a capillary tube with an optical fiber
plunger, which is activated by depressing the thumbpad and
releasing it to draw in the fluid. A mirror on the distal side of
the capillary completes the optical path.
Requires 2 µL of Sample
The pipetter is equipped with a bifurcated fiber, which couples
to our spectrometers and compact light sources to create lowvolume absorbance systems. The
SpectroPipetter requires only 2 µL of
sample for a spectral measurement.
Cleaning Kit
Sampling Accessories
Specifications
Wavelength range:
Sample volume:
Light pathlength of cell:
Temperature range:
Optical fiber length:
Core diameter of launch fibers:
Core diameter of return fiber:
230-850 nm
2 µL
10 mm
4 °C to 99 °C
1.3 m
Bundle of (3) 200 µm optical fibers
200 µm
To remove fluid or dye from the cell, use
the PIP-UCK Cleaning Kit. It contains an
ultrasonic cleaning bath (at right) and a
bottle of cleaning solution. Additional
PIP-UCK-CS Cleaning Solution
(below right) is also available.
PIP-10-2:
$1,995
PIP-UCK:
$165
PIP-UCK-CS:
$25
Longpass Flow Cells
100x Increase in Sensitivity
LPC Longpass Flow Cells couple to our spectrometers and light sources
for simple, efficient measurements of low-volume, low-concentration
aqueous samples. With the LPC-1, you have a 1-meter cell with an
internal volume of only 240 µL, giving you 100x the sensitivity over a
1-cm pathlength cuvette holder as your sampling device.
Easy to Use
LPC cells use a capillary tube as both the sample compartment and the
light waveguide. You inject the sample into the fluidic ports with a
syringe or pump; optical fibers connect to SMA 905 Connectors
to deliver and return light to the spectrometer. We
offer these cells in 1- and 5-meter pathlengths (call
for other pathlengths). A 5-meter cell (250 µL/meter) increases the
absorbance signal 500x more than a 1-cm cuvette. Also available is the
LPC-CLEANKIT (see inset), a waveguide cleaning kit for the LPCs.
LPC-1:
$1,695
LPC-5:
$3,350
LPC-CLEANKIT:
$59
Specifications
Dimensions:
Weight:
Wavelength range:
Tubing volume:
Fiber connectors:
Fiber core diameter:
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254 mm x 279 mm
140 g
230-800 nm for LPC-1, 325-700 nm for LPC-5
250 µL/meter
SMA 905
400 µm
Maximum sample temperature:
Tubing inner diameter:
Tubing:
Fluid fittings:
Maximum pressure:
Chemical resistance:
160 °C
550 µm
Fused silica inner tubing coated with Teflon AF
1/16", 1/32" compression fittings
2000 psi
Most organic and inorganic solvents
For all your sensing needs, visit OceanOptics.com
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Cell for Capillary Electrophoresis
Solutions Absorbance
The CUV-CCE Electrophoresis Sample Cell is an
optical fixture for measuring the absorbance of
solutions in chromatography or capillary electrophoresis systems. The cell’s design -- light projects through
the sides of the silica tubing -- eliminates pressure limits
commonly associated with tubing breakdown in electrophoresis systems.
Excellent Chemical Resistance
The CUV-CCE cell, fixtures and fittings are made of robust PEEK material.
The cell, which can be purchased separately as CUV-CCE-CROSS, has a
through-hole of 0.51 mm and comes with 10-32 coned female threads
and four fittings. Two fibers (included) face each other across
Specifications
the sample tubing. To complete the system, we recommend a
Dimensions:
spectrometer and a DH2000-BAL Light Source (see page 122).
Fibers & Tubing Sleeves Included
Positive Displacement Pump
Displaces Volumes from 1 µL
The PUMP-IT-1000 Positive Displacement Pump Kit is a pulsed pump that displaces from 1 µL to
250 µL of fluid with each pump or cycle. The amount of fluid displaced with each cycle is set via
software. The amount pumped is precise to 0.3% with repeatability of better than 0.5%. The pump
provides a ripple-free and bubble-free flow. For accurate mixing and/or dilution of fluids, the
pump has upper and lower limits that can be set mechanically and via the software (included),
which also allows you to select the displacement amount and the speed of the displacement.
Sampling Accessories
The CUV-CCE comes with two 300-µm solarization-resistant
fibers and tubing sleeves to connect tubing to the threaded
ports. You can also purchase the CUV-CCE-CROSS tubing
sleeves separately. Other sleeve sizes are available.
CUV-CCE:
$599
CUV-CCE-CROSS:
$65
CUV-CCE-TUBING:
$15
Weight:
Cell material:
Fixtures & fittings material:
Threads:
Through-hole:
Fittings:
Swept volume:
Tubing sleeve diameter:
Tubing sleeve length:
Tubing size accommodated:
Pressure rating (tubing):
28.6 mm x 28.6 mm (cross);
50.8 mm x 50.8 mm (cross with fittings)
9.4 g
PEEK polymer
PEEK polymer
10-32
0.51 mm
(4) F-300 double-winged nuts with F-142 ferrule
0.721 µL
0.41 mm inner diameter, 1.57 mm outer diameter
31.8 mm
350-390 µm outer diameter
6,000 psi (414 bar)
Applications
The PUMP-IT-1000 Kit is useful for those wanting to automate the delivery of reagents into accurate
flow setups. Typical applications include blood chemistry, blood analysis, particle sizing, in vitro
diagnostics and biopharmaceutical analysis. The PUMP-IT-1000 comes with everything needed for
a flow setup; you can also purchase the pump separately (PUMP-IT-PUMP).
PUMP-IT-1000: $999
PUMP-IT-PUMP: $565
Specifications
Volume:
250 µL full scale; 0.028 µL volume per full step
Throughput:
> 60% (based on 400 µm optical fiber)
Actuator:
5 VDC, 0.49 amp/phase, 10.2 ohm/phase, 9.6 mHz/phase
Accuracy:
< 0.5% repeatability; < 0.3% precision
Pump head:
Acrylic (custom options include polycarbonate and PEEK)
Pump piston:
PEEK (custom options include stainless steel, ceramic and glass)
Pump body:
Aluminum (custom options include stainless steel and acrylic)
Dimensions (in cm): Pump: 3.50 x 3.50 x 16.94; Controller: 11.93 x 11.93 x 6.35
Controller:
Unipolar/Bipolar dual stepper motor control PCB, 7.5 VAC, 1 A
Baud rate:
2400 or 9600 baud serial connection
AC adapter:
7.5 VAC, 1 A
Tubing:
10 feet of Tygon tubing
Nylon fittings:
10 female Luer fittings, 1/4 hex to 10-32 thread; 10 1/16" ID elbow fittings;
10 male Luer fittings, 1/4 hex to 10-32 thread; 10 Luer plugs and 10 caps;
10 1/16" ID barbed fittings with10-32 thread; and 10 1/16" ID barbed tee fittings
Tel: 727.733.2447 • Email: [email protected]
The PUMP-IT-1000 Kit comes with the Positive
Displacement Pump, a 250-µL sample bottle, 10 feet of
tubing, various nylon fittings, controller box and power
supply, RS-232 cable and software.
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Fluorescence Sampling Tools
CUV-ALL-UV 4-way Cuvette Holder
The CUV-ALL-UV provides ports for 1-cm cuvettes from four directions.
Position two collimators at 180° for absolute absorbance and transmission
measurements, position two collimators at 90° for fluorescence or scattering,
or use all four for simultaneous absorbance and fluorescence
measurements. For fluorescence applications, increase the signal by
replacing collimators with 74-MSP Mirror Plugs (see inset), which
redirect energy back to the sample or back into a collimating lens.
CUV-ALL-UV: $809
74-MSP:
$99
CUV-FL-DA Direct-attach Cuvette Holder
Sampling Accessories
The CUV-FL-DA attaches to our light sources and couples via fibers to our spectrometers,
creating systems for fluorescence and relative absorbance. The holder has a collimating
lens and two mirrored screw plugs (74-MSP), which can be positioned per your
application. A 6.35-mm slot is included for filters.
CUV-FL-DA: $399
Fluorescence Standard
For quickly and easily checking the calibration, stability, and performance of
your fluorescence system, use this Solid Secondary Fluorescence Standard.
STAN-FL-RED:
$179
Linear Variable Filters
We've combined our patented high-pass and low-pass Linear Variable Filters to create the
world's first bandpass filter with an adjustable center wavelength and adjustable bandpass. Each
filter features an excellent transmission band (~90%) and blocking band (99.8%). These filters
are especially useful for spectrally shaping the excitation energy from broadband sources used
for fluorescence. The filters are epoxied into slide carriers that allow you to move the
transmission or blocking band throughout the filter’s wavelength range. The LVF filters and
slide carriers can be inserted easily into spectrometer setups. For details, see page 114.
Fluorescence Flow Cell for Flow Injection
With the FIA-SMA-FL Fluorescence Flow Cell, a fiber sends excitation energy via
a window into a sample compartment. A second fiber, oriented at 90° and
connected to a spectrometer, collects the emitted energy. Each cell has two
optical windows and SMA 905 Connectors (which do not contact the fluids). Also
included are Teflon tubing and chemically-resistant tubing connectors and seals.
Two 600 µm fibers are required. See the bottom of page 94 for fiber details.
FIA-SMA-FL:
$435
Fluorescence Process Flow Cells
The PRO-FC-FL+TR Fluorescence Flow Cell is an adjustable-pathlength fluorescence
flow cell that can be used for fluorescence and transmission measurements in a
variety of industrial online flow analysis applications. The PRO-FC-FL+TR can be
configured with Optical Interface Couplers (three OICs included) at 90° for
fluorescence applications. Add a third OIC at 180°s to make transmission and
fluorescence measurements simultaneously. The cell's pathlength can easily be
adjusted from 0.5-15.0 mm.
PRO-FC-FL+TR:
$3,750
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Fluorescence Flow Analysis PMT
Parts-per-trillion Sensitivity
The FIA-PMT-FL Photomultiplier Flow-through Detection System
provides parts-per-trillion sensitivity for ultra-low fluorescence,
chemiluminescence and bioluminescence measurements.
Modular Design
The FIA-PMT-FL is built to order with either an internal excitation
lamp or with an optical fiber interfacing to an external lamp.
Excitation source options include tungsten, mercury vapor, LEDs
and laser diodes. Emission and excitation filters are mounted in
slots in the system, allowing for easy removal. Though the
system uses a 25 µL flow-through cuvette, you can also use
standard 1-cm pathlength cuvettes for manual measurements.
Easy PC Interface & Optimized Software
Specifications
Dimensions:
Spectral range:
Detector:
PMT dynamic range:
Responsivity:
Detection limits:
~13 cm x 18 cm x 25.4 cm
310-750 nm (filter/lamp selection dependent)
Photo-counting photomultiplier tube
2 x 106
5 x 1017 cps/watt (@ 400 nm)
10 parts per trillion measured with fluorescein
@ 200 msec integration time and internal LED
Pulse-pair resolution: 10 ns
Flow cell :
10 mm path, 25 µL volume with flow-through cuvette
Filters:
Your waveband choice of 1 excitation filter
and 1 emission filter (call for options)
Computer interface: RS-232 to Windows 98/Me/2000/XP OS
Fiber Optic Scanning Monochromator
Monochromator Allows 2 nm Bandwidth
The MonoScan2000 is a computer-controlled scanning monochromator with
a 300-700 nm wavelength range. It takes the MonoScan2000 only three
seconds to scan from 300-700 nm. To scan only one nanometer takes about
15-20 milliseconds. The MonoScan2000 is compatible with all Ocean Optics
spectrometers, light sources, accessories and optical fibers.
Sampling Accessories
Included with the system is Windows-based software that allows
you to set the integration time and voltage counts, and to obtain
time histories of the measurements, both plotted and tabulated.
The software can also automatically create calibration curves
and control additional devices such as certain syringe and
peristaltic pumps, injection valves, selection valves and
autosamplers. ActiveX control is included for controlling the FIAPMT-FL from your own software. The FIA-PMT-FL plugs into the
RS-232 serial port of a PC.
FIA-PMT-FL:
$6,495
Use as a Tunable Light Source or Excitation for Fluorescence
In this setup, a broadband light source provides light via optical fiber to the
MonoScan2000. You select a 2-to-3 nm bandpass in which the light passes
before exiting the MonoScan, interacting with a sample and passing to a
spectrometer. In this situation, the MonoScan takes the place of a filter. A
scanning monochromator is better able to provide excitation intensity than a
filter because of the monochromator’s ability to reject out-of-band
illumination. Filters can provide adequate excitation intensity but at reduced
optical transmittance because they typically have a wider bandpass. You often
sacrifice dynamic range with filters.
Use with Single-element Detector
A light source provides light via optical fiber to a sample, interacts with the
sample, and sends light to the MonoScan2000. The monochromator captures
the incoming light, transmits it via fiber to a single-element detector, such as
a photodiode, one wavelength at a time. The MonoScan2000 allows a high
optical throughput and provides an intense spectral signal. The MonoScan
has the ability to scan through a wavelength range you select via software.
Because the MonoScan has no slit, the diameter size of the optical fiber
determines the optical resolution of the system. When using 200 µm fibers,
for example, optical resolution is <3 nm (FWHM).
MonoScan2000:
$5,219
Tel: 727.733.2447 • Email: [email protected]
Specifications
Dimensions:
Weight:
Wavelength range:
Optical resolution:
112 mm x 132 mm x 145 mm
1.1 kg
300-700 nm
Fiber diameter dependent;
~4 nm (FWHM) using a 400 µm fiber
Holographic grating: 1250 l/mm, blazed at 350 nm
Accuracy:
<0.5 nm
Repeatability:
0.2 nm
Transition speed:
From wavelength to wavelength is
ca 3s 300-700 nm 1 nm step ~ 15 ms
Dispersion:
~10 nm per mm
Optical throughput: >50% with a 1000 µm fiber at 350 nm
>30% with a 1000 µm fiber at 500 nm
Grating scan angle: 14.8° (300-700 nm)
Computer interface: USB and RS-232
Power requirement: 12 VDC max. 1.2A (WT-12V-E)
Gearbox ratio:
1:261
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Semiconductor Nanocrystals
Evident Technologies, an Ocean Optics partner, develops extremely
high-quality, low-cost semiconductor nanocrystals. These quantum dots
are nanometer-scale materials that have properties between that of
molecules and bulk materials. This enables Evident to produce "designer
atoms" through atomic-level manipulation. When combined with our
spectrometers and excitation sources, these nanocrystals have been
used in biology applications as fluorescent tags to measure and
quantify biological phenomena, and in photonics as tunable colors for
light-emitting diodes. EviTags are an ideal tagging tool for highthroughput screening in micro-fluidic systems, as well as cell imaging
and pathogen detection. For most applications, we recommend our
USB2000-FLG Spectrometer and some combination of our light sources
and filters to excite EviDots and EviTags. Contact one of our
Applications Scientists for details.
Sampling Accessories
EviDot Core & Core-shell Nanocrystals
EviDot Core Nanocrystals are manufactured quantum dots ranging in size
from 2-10 nm with fewer than 1,000 atoms. Each Core type is made of
the same material but exhibits different emission properties based on size.
Cores produce high quantum yields with intense fluorescence at targeted
peak wavelengths. EviDot Core-shell Nanocrystals are Core Nanocrystals
with a zinc sulfide coating that stabilizes the Core, improves quantum yield
and reduces photodegradation.
Item Code
Description
Semiconductor
Nanocrystals
Vials
QD-CS-VIS
Core Shell EviDot Kit. Choose 6 vials from the following:
Cadmium selenide
6
• 490 nm • 520 nm • 540 nm • 560 nm
• 580 nm • 600 nm • 620 nm
nanocrystals with zinc
Core Shell EviDots. Specify 1 vial only from the following:
Cadmium selenide
• 490 nm • 520 nm • 540 nm • 560 nm
• 580 nm • 600 nm • 620 nm
nanocrystals with zinc
QD-CS-1V
Volume per Vial
Price
0.5 mg dots in 4 mL of
$699
toluene solvent
sulfide shell (CdSe/ZnS)
1
50 mg dots in 5 mL of
$449
toluene solvent
sulfide shell (CdSe/ZnS)
EviTag Core-shell Nanocrystals
EviTag Nanocrystals are Core-shell Nanocrystals with an additional
proprietary coating that makes the Core shells water-stable. These EviTags
are cadmium selenide nanocrystals with a zinc sulfide shell. Carboxyl
ligands are attached to the proprietary coating so that they can easily be
bound to nucleic acids, antibodies and proteins, making the EviTag
technology available to life science applications.
Item Code
Description
Volume per Vial
Price
QD-T2-MP-1V
Single vial of cadmium selenide nanocrystal compound with
6 nanomoles of EviTags per 0.5 milliliters
$399
a zinc sulfide shell (CdSe/ZnS) and a proprietary coating
of deionized water
containing carboxyl terminal groups; specify one of the following
QD-T2-MP-A-1V
• 490 nm
• 520 nm
• 540 nm
• 580 nm
• 600 nm
• 620 nm
• 560 nm
Single vial of cadmium selenide nanocrystal compound with
6 nanomoles of EviTags per 0.5 milliliters
a zinc sulfide shell (CdSe/ZnS) and a proprietary coating
of deionized water
$399
containing amine terminal groups; specify one of the following
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• 490 nm
• 520 nm
• 540 nm
• 580 nm
• 600 nm
• 620 nm
• 560 nm
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FluoroVette Micro-volume Cells
Fluorescence Cells for Nano-molar Detection
The FluoroVettes are ultra low-volume, disposable cells for
nano-molar range fluorescence detection. Only 50 µL of fluid
fills the microfluidic channel of a FluoroVette, which then
slides into a 1-cm cuvette adapter for use in a fluorescence
setup with a spectrometer and cuvette holder.
Advantages Versus Cuvettes
A pipetter is used
to inject fluid into the
CFV-PIP-SP FluoroVette.
For only $125, you receive 10 disposable FluoroVettes with a
Cuvette Adapter, making these cells a great alternative to
expensive quartz cuvettes. For the price of one micro-volume
quartz cuvette, you could use over 30 disposable FluoroVettes
with no risk of sample contamination.
A FluoroVette
slides into the top
of the Cuvette
Adapter, which
then inserts into a
cuvette holder.
Two Types of Disposable 50 µL FluoroVettes
A pump and tubing are
used to circulate the fluid through
the CFV-PUMP-SP FluoroVette.
Fluorescein Spectra in pH 8 Buffer
0.10
100 nM
50 nM
25 nM
RELATIVE INTENSITY
0.08
10 nM
5 nM
0.06
pH 8 Buffer
0.04
0.02
0
475
500
525
550
575
600
WAVELENGTH (nm)
Detection of fluorescein in the nanomolar range (nM) is typical with
FluoroVettes. These spectra were made with a CFV-PIP-SP,
USB2000-FLG Spectrometer, LS-450 Blue LED, CUV-ALL-UV
Cuvette Holder, 1000 µm illumination fiber and 600 µm read fiber.
The integration time was 1000 msec; a longer integration time
provides even lower detection limits.
Sampling Accessories
There are two types of FluoroVettes. The CFV-PIP-SP has an
inlet port for loading the sample into the FluoroVette with a
standard 20-200 µL pipetter and ordinary tips, making it a
snap to fill and perform measurements. The CFV-PUMP-SP
has tubing barbs at the inlet and outlet ports so the
FluoroVette can be used in continuous or flow injected
measurements using a syringe or peristaltic pump. Each type
of FluoroVette slips easily into the Cuvette Adapter for using
with a standard 1-cm cuvette holder, such as our
CUV-ALL-UV 4-way Cuvette Holder. The Cuvette Adapter’s
two ports are positioned at 90° for fluorescence
measurements. (See complete setup below.)
Specifications
In this setup, the CFV-PUMP-SP
FluoroVette and Cuvette Adapter sit in
a CUV-ALL 4-way Cuvette Holder. A pump
circulates the sample through the FluoroVette.
High-sensitivity Applications of Precious Samples
FluoroVettes are easy to fill and empty, making it possible to
perform a dilution series to optimize data from scarce
samples. The FluoroVettes are ideal for a variety of real-time
high-sensitivity fluorescence applications, such as
Assay development with quantum dots
GFP-based assays
Protein conformation analysis
DNA quantification via Pico-Green assay reagent
Cell marker identification
Enzyme inhibitors using FRET Assays
Tel: 727.733.2447 • Email: [email protected]
Size:
Volume:
Pathlength:
Detection limit:
50 mm tall, 9 mm wide, and 1 mm thick
50 µL
0.75 mm
5 nM detection limit of fluorescein with pH 8 buffer
and 1000 msec integration time
Dead volume:
1 µL for pipette interface; for tubing interface, dead volume
depends on tubing length
Wavelength range: 220-2500 nm
Accuracy:
FluoroVettes are linear over the concentration range,
typical error is less than 5%
Item
Description
CFV-PIP-SP
Pack of 10 FluoroVettes with pipetter
interface (for use with a pipetter) and
one FluoroVette Cuvette Adapter
Assembly for 1-cm standard cuvette
holders
Price
$125
CFV-PUMP-SP
Pack of 10 FluoroVette Flow Cells with
tubing interface (for use with pump
and tubing, neither included) and one
FluoroVette Cuvette Adapter Assembly
for 1-cm standard cuvette holders
$125
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Cosine Correctors: Emission Collection
Collect Radiation from 180°
Our Cosine Correctors couple to optical fibers and
spectrometers for relative and absolute spectral intensity
measurements, for emissive color applications, and for
evaluation of light sources such as LEDs and lasers.
Probe Option
When the CC-3 and CC-3-UV are
screwed onto the end of an optical
fiber, the cosine corrector and optical
fiber become an irradiance probe.
The probe couples to one of our
spectrometers to measure the intensity of
light normal to the probe surface.
The CC-3-DA (above left) attaches directly to an SMA 905 Connector
on a spectrometer, creating a spectroradiometer. The CC-3 and
CC-3-UV (above, right) attach to fibers, creating Irradiance Probes.
Direct-attach Option
The CC-3-DA screws directly onto the SMA 905 Connector of
an Ocean Optics Spectrometer, creating a complete
spectroradiometric system and eliminating the need for an
optical fiber.
CC-3-UV Angular Response
3500
Spectralon
Lambert’s Cosine Law
Diffusing Material: UV-VIS or VIS-NIR
The diffusing material used in the cosine corrector is a thin disk
of opaline glass (350-1100 nm) or Spectralon (200-1100 nm)
that sits at the end of a stainless steel barrel.
CC-3:
$99
CC-3-UV:
$129
CC-3-DA:
$299
2500
COUNTS
Sampling Accessories
3000
2000
1500
1000
500
Specifications
Diffusing material:
Wavelength range:
Dimensions:
Field of view:
CC-3
Opaline glass
350-1000 nm
6.35 mm OD
180°
0
CC-3-UV
Spectralon
200-1100 nm
6.35 mm OD
180°
CC-3-DA
Spectralon
200-1100 nm
12.7 mm OD
180°
0
10
20
30
40
50
60
70
80
90
100
ANGLE
The response of the Spectralon disc (red trace) used in the
CC-3-UV closely matches that of Lambert’s Cosine Law.
Power Supply & Controller for LEDs
Measuring LEDs
The LED-PS Power Supply works with our spectrometers and
the FOIS-1 Fiber Optic Integrating Sphere (see page 105) for
spectroradiometric and color measurements of LEDs. The
LED-PS unit has easy-to-reach electrical connectors for
mounting LEDs that are 9.52-mm diameter or smaller with
2.77-mm lead spacing.
Adjustable Drive Current
The LED-PS holds the LED in place, powers the LED, and
displays the LED’s drive current. The drive current is
adjustable, with a digital display to indicate the current level.
With the LED-PS-NIST, the current meter is calibrated against
a NIST-traceable standard. For more on LED measurements,
see page 56.
LED-PS:
$499
LED-PS-NIST:
$749
LED-PS-RECAL: $199
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Specifications
Dimensions:
Weight:
Power consumption:
LED drive current:
Drive current accuracy:
LED mount:
56.8 mm x 56.8 mm x 56 mm
170 g
Up to 100 mA @ 12 VDC; depends on setting
12-50 mA with 0.1 mA resolution
± 1.0%
2.77 mm lead spacing, PTFE base
For all your sensing needs, visit OceanOptics.com
Integrating Spheres: Irradiance/Emission
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ISP-I Integrating Spheres
Emission Collection
ISP-I Integrating Spheres are convenient sampling optics that couple
to our spectrometers via optical fibers to measure the spectral output
from 200-2500 nm of LEDs, lasers and other light sources. Each
integrating sphere consists of a proprietary PTFE-based, sintered
diffusing material -- in diameters of 30 mm, 50 mm or 80 mm -that provides a Lambertian surface for irradiance measurements.
LED Measurement & Direct-attach Option
An ISP-LED-ADP adapter holds in place 3 mm, 5 mm
or 8 mm LEDs and screws into the sample port of the
ISP-50-8-I Integrating Sphere for measuring LEDs. The
adapter ensures reproducibility. Other options are the
USB-ISP-50 or USB-ISP-80, which directly attach to a
USB2000 and USB4000 Spectrometer, eliminating the need for a
read fiber. If the sample ports are too small, we offer custom sample
port sizes for all ISPs. Custom machining for ports in diameters of 8,
10, 12, 14, 16 or 20 mm is available (see below).
Specifications
Weight:
Spectral range:
Sphere coating:
Reflectivity:
330 g (ISP-30); 730 g (ISP-50); 1,650 g (ISP-80)
200-2500 nm
Proprietary PTFE-based diffusing material
>98% (400-1500 nm); >95% (250-2000 nm)
Description
Sample Port
Max. Fiber
Price
ISP-30-6-I
Integrating sphere, 59 mm diameter, 58 mm high
6 mm
800 µm
$1,337
ISP-50-8-I
Integrating sphere, 80 mm diameter, 78 mm high
8 mm
600 µm
$1,741
ISP-80-8-I
Integrating sphere, 107 mm diameter, 117 mm high
8 mm
400 µm
$2,156
ISP-LED-ADP
Holds in place 3, 5 or 8 mm LED for reproducibility; for use with ISP-50-8-1
N/A
N/A
USB-ISP-50-I
ISP-50-8-I designed to directly attach to a USB2000 or USB4000 Spectrometer
8 mm
600 µm
$2,217
USB-ISP-80-I
ISP-80-8-I designed to directly attach to a USB2000 or USB4000 Spectrometer
8 mm
600 µm
$2,632
ISP-PORT-1
Custom sample port machining of 8, 10, or 12 mm diameter
8, 10 or 12 mm
400 µm
$172
ISP-PORT-2
Custom sample port machining of 14,16 or 20 mm diameter
14, 16 or 20 mm
400 µm
$335
HL-2000-CAL-ISP
NIST-traceable radiometric standard for use with ISP-50-8-I; see page 133
N/A
N/A
$883
$202
FOIS-1 Fiber Optic Integrating Sphere
Sampling Accessories
Item
360° Emission Collection
The FOIS-1 is a compact sampling optic that collects
light from emission sources such as LEDs and lasers,
or that measures light fields with a 360° field of view.
Principle of Operation
At the heart of the FOIS-1 is Spectralon, a white
diffusing material with a highly Lambertian surface.
Light enters the sphere via a 9.5-mm diameter port
while a fiber -- oriented at 90° to the sample port -collects the light. The size of the FOIS-1 and its three
mounting holes make it easy to connect the sphere to
other items, such as the 74-ACH Adjustable
Collimating Lens Holder (at left).
In the picture top right, the FOIS-1 is being used to measure
LEDs. In the picture bottom right, the FOIS-1 is attached to a 74-ACH, a setup often
used when making transmission measurements of curved optics. An optic is set
between the FOIS-1 and the right arm of the 74-ACH.
Specifications
Dimensions:
Top mounts:
Side mounts:
56.8 mm x 62.4 mm (housing)
38.1 mm diameter (sphere)
(2) 6-32; (2) 8-32; (1) 1/4-20
SMA 905 Connector; (1) 8-32
Weight:
Spectral range:
Sample port:
Sphere coating:
240 g
200-2500 nm
9.5 mm aperture
Spectralon
Tel: 727.733.2447 • Email: [email protected]
Use with Calibrated Light Source
Before measuring the absolute spectral intensity of
emission sources, use the LS-1-CAL-INT Calibrated
Light Source to calibrate the absolute spectral
response of your spectroradiometric system. For more
on the LS-1-CAL-INT, see page 133.
FOIS-1: $499
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Integrating Spheres for Reflectance
ISP-REF Illuminated Integrating Sphere
The ISP-REF Illuminated Integrating Sphere couples to our spectrometers to
measure the total integrated reflectance of surfaces placed against the sphere’s
sample port. The ISP-REF can measure variegated and opaque samples.
Sampling Accessories
The ISP-REF measures the reflectance from flat surfaces pressed against its
10.3-mm diameter sample port. Illumination is provided by an internal
tungsten halogen lamp powered with a 12 VDC wall transformer. The lamp is
baffled so that all light that strikes the sample has been reflected from the
sphere walls. The sphere’s highly Lambertian interior provides a uniform 180°
illumination field. The sample is viewed from 8° from normal by a lens system
that couples to the fiber optic sample port. The field of view is restricted to the
sample area, and has a divergence of ~2°. A simple switch allows you to open
or close a gloss trap opposite the lens for the inclusion or exclusion of specular
reflectance. A reference fiber port is provided to connect to a second
spectrometer channel to monitor the output of the light source during long
experiments, or for bringing external light into the sphere.
ISP-REF:
$1,599
ISP-REF-B Bulb:
$40
ISP-R Integrating Spheres
The ISP-Rs are distinguished by their compact size and sturdy design. Each has
SMA 905 fiber ports at 90° (to connect to a spectrometer) and 8° (to connect to
a light source for direct illumination).
Each sphere is made of a sintered PTFE, which is >98% reflective in the visible.
The spheres are available in diameters of 30 mm, 50 mm and 80 mm. Sample
port diameters are 6 mm for the 30-mm sphere and 8 mm for the 50-mm and
80-mm spheres. If the 6-mm or 8-mm diameter sample ports are too small,
custom sample port sizes for all ISP-Rs are available. For sample ports in
diameters of 8, 10, or 12 mm, select ISP-PORT-1. To custom machine a
14,16 or 20 mm sample port, order an ISP-PORT-2.
The gloss-trap version (see inset, far right) comes with two cylindrical pieces -one is made of black absorbing material and the other of white reflecting
material -- that fit into a hole at the top of the sphere. When using the white
gloss trap, you can make specular and diffuse measurements. When using the
black gloss trap, you can use the ISP-Rs for diffuse measurements.
ISP-30-6-R:
$1,739
ISP-50-8-R:
$2,009
ISP-80-8-R:
$2,424
ISP-50-8-R-GT:
$2,163
ISP-PORT-1:
$172
ISP-PORT-2:
$335
Specifications
Dimensions:
Weight:
Power consumption:
Spectral range:
Sphere diameter:
Sample port diameter:
Sphere coating:
Reflectance:
Reflectivity:
Bulb:
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106
ISP-REF
54 mm x 57 mm x 83 mm
864.7 g
600 mA @ 12 VDC (lamp)
360-2000 nm
38.1 mm
10.32 mm
Spectralon
Diffuse or specular and diffuse
>98% (400-1500 nm)
>95% (250-2000 nm)
900-hour bulb; 3100 K color temp.
ISP-30-6-R
59 mm dia., 58 mm high
330 g
None
200-2500 nm
30 mm
6 mm
PTFE material
Specular and diffuse
>98% (400-1500 nm)
>95% (250-2000 nm)
None
ISP-50-8-R
80 mm dia., 78 mm high
730 g
None
200-2500 nm
50 mm
8 mm
PTFE material
Specular and diffuse
>98% (400-1500 nm)
>95% (250-2000 nm)
None
ISP-80-8-R
107 mm dia., 117 mm high
1,650 g
None
200-2500 nm
80 mm
8 mm
PTFE material
Specular and diffuse
>98% (400-1500 nm)
>95% (250-2000 nm)
None
ISP-50-8-R-GT
80 mm dia., 78 mm high
743.3 g
None
200-2500 nm
50 mm
8 mm
PTFE material
Diffuse
>98% (400-1500 nm)
>95% (250-2000 nm)
None
For all your sensing needs, visit OceanOptics.com
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Diffuse Reflectance Standards
WS-1 Diffuse Reflectance Standard
The WS-1 Diffuse Reflectance Standard (at left) is made of PTFE, a diffuse white
plastic that provides a Lambertian reference surface for reflectance experiments.
The WS-1 comes in an anodized aluminum housing, and is hydrophobic,
chemically inert and very stable, even in deep-ultraviolet applications. It is >98%
reflective from 250-1500 nm and >95% reflective from 250-2200 nm.
WS-1: $299
WS-1
WS-1-SL White Reflectance Standard with Spectralon
The WS-1-SL is a diffuse reflectance standard from Labsphere and is made from
their patented diffuse reflectance material, Spectralon. Spectralon is hydrophobic
and is thermally stable to 350 °C. The durable material provides highly accurate,
reproducible data. Unlike all the other PTFE-based standards on this page, the
WS-1-SL often can be smoothed, flattened and cleaned if nicked or soiled.
WS-1-SL: $329
WS-1-SS Includes Stainless-steel Housing
WS-3-GEM White Reference Tile
Conceived for use in colorimetric applications involving diamonds and other
gems, the WS-3-GEM White Reference Tile consists of a diffuse PTFE material,
shaped to form a holder within its stainless steel receptacle. Because of its
concave shape, the WS-3-GEM becomes an integrating sphere when illuminated.
The WS-3-GEM has >98% reflectivity from 250-1500 nm and >95% reflectivity
from 250-2200 nm. Like the WS-1, the WS-3-GEM’s reflectance material is
hydrophobic, chemically inert and very stable, even in deep-UV applications.
WS-3-GEM: $530
WS-1-SS
Sampling Accessories
The WS-1-SS comes in a stainless steel housing and has the same properties as
the WS-1. In addition, the surface of the WS-1-SS is slightly recessed to allow the
RPH-1 Reflection Probe Holder to sit on the standard without coming in direct
contact with the standard’s surface.
WS-1-SS: $396
WS-1-SL
Reflectivity of the White Standards
PTFE (WS-1, WS-1-SS
and WS-3-GEM
100
REFLECTANCE (%)
Spectralon (WS-1-SL)
98
96
94
WS-3-GEM
92
200
600
1000
1400
1800
2200
2600
WAVELENGTH (nm)
Specifications
Dimensions:
Weight:
Spectral range:
Housing:
Reflectivity:
WS-1
38 mm diameter (housing)
32 mm OD, 10 mm thick (tile)
30 g
250-2000 nm
Aluminum
>98% (250-1500 nm)
>95% (250-2200 nm)
WS-1-SL
38 mm diameter (housing)
32 mm OD, 10 mm thick (tile)
30 g
250-2500 nm
Delrin holder, protective cover
99% (400-1500 nm)
>96% (250-2000 nm)
Tel: 727.733.2447 • Email: [email protected]
WS-1-SS
38 mm diameter (housing)
32 mm OD, 10 mm thick (tile)
30 g
250-2000 nm
Stainless steel
>98% (250-1500 nm)
>95% (250-2200 nm)
WS-3-GEM
38 mm diameter (housing)
31 mm OD, 10 mm thick (tile)
30 g
250-2000 nm
Stainless steel
>98% (250-1500 nm)
>95% (250-2200 nm)
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Specular Reflectance Standards
Versatile & Durable Standards
We offer three specular reflectance standards for use as
references when measuring the reflection of surfaces with high or
low specular reflectivity. Each standard consists of a 31.7-mm
outer diameter optical reflectance material in a protective
aluminum receptacle with screw-on top. The superior coatings on
the substrates are environmentally stable; they are able to
withstand high temperatures and mechanical stresses.
Software Referencing & Calibration
Reflectivity values for the standards are built into our
Spectroscopy Operating Software to provide a reference for
any specular measurement. You simply choose the standard from
a software menu and the software reads data from the electronic
file shipped with the standard.
With the STAN-SSH Highreflectivity Specular
Reflectance Standard (above),
you receive a certificate of
calibration in paper and
electronic formats.
The STAN-SSH High-reflectivity Specular Reflectance Standard is
a fused-silica substrate coated with aluminum and protected by a
thin layer of magnesium fluoride. This standard is typically used
for measuring high-reflectance surfaces of optical substrates and
coatings, machined metals and semiconductor materials. Values
for the STAN-SSH are calculated for any angle from 0-45°.
Reflectance of STAN-SSL at 6°
10%
For Calibrated High Reflectivity
9%
Also available is a calibrated version of the STAN-SSH. The
STAN-SSH-NIST is calibrated at a 6° angle traceable to NIST and
is accurate to ± 0.1% from 250-2500 nm. The STAN-SSH-NIST
comes with calibrated reflectivity values (from a 6° angle) in both
paper and electronic formats. We recommend a periodic
recalibration of the STAN-SSH-NIST, which costs $149. Should
the calibrated surface become corrupted, a recoat and
calibration service is available for $299.
8%
% REFLECTION
Sampling Accessories
For High Reflectivity
7%
6%
5%
4%
3%
2%
1%
0
300
500
700
900
1100
1300
1500
1700
1900
WAVELENGTH (nm)
For Low Reflectivity
The STAN-SSL Low-reflectivity Specular Reflectance Standard is a
black glass standard that can be used as a reference when
measuring the low-reflectance surfaces of samples
such as thin film coatings, anti-reflective
coatings, blocking filters and substrates.
Reflectance of STAN-SSH at 6°
98%
Holder Protects Standards
We also offer a holder for use with our
reflectance standards. The STAN-HOLDER
supports a standard during measurements, which
helps to preserve its coating.
STAN-SSH:
$499
STAN-SSH-NIST: $999
STAN-SSL:
$499
STAN-HOLDER:
$75
% REFLECTION
96%
94%
92%
90%
88%
86%
200
400
600
800
1000
1200
1400
WAVELENGTH (nm)
1600
1800
2000
Specifications
Substrate dimensions:
Housing dimensions:
Weight:
Reflectance material:
Reflectivity:
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108
STAN-SSH
31.75 mm outer diameter x 6.35 mm height
38 mm outer diameter x 19 mm height
40 g
Front-surface protected aluminum mirror
on fused silica substrate
~87-93% (200-1000 nm)
~93-98% (1000-2500 nm)
STAN-SSH-NIST
31.75 mm outer diameter x 6.35 mm height
38 mm outer diameter x 19 mm height
40 g
Front-surface protected aluminum mirror
on fused silica substrate
~87-93% (200-1000 nm)
~93-98% (1000-2500 nm)
STAN-SSL
31.75 mm outer diameter x 6.35 mm height
38 mm outer diameter x 19 mm height
40 g
Schott ND9 glass
~5% (200-950 nm)
~4% (950-2500 nm)
For all your sensing needs, visit OceanOptics.com
Variable-angle Reflection Sampling System
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Measure Optical Substrates at Different AOI
The RSS-VA Variable-angle Reflection Sampling System
is a cleverly designed opto-mechanical device for
measuring specular reflection of optical substrates at
varying angles of incidence (AOI). When coupled to our
spectrometers and light sources, the RSS-VA becomes a
compact alternative to unwieldy, high-priced systems
typically used to characterize optical substrates.
Optical sample is
placed on this port.
Light enters
the RSS-VA
via optical
fiber.
Opto-Mechanical Design
To spectrometer.
Specifications
114.3 mm x 41.3 mm x 101.6 mm
980 g
19.0 mm x 6.4 mm
(2) SMA 905 Connectors (for illumination fiber & read fiber)
3-point
~10° to ~50° (user-adjusted)
100 µm (illumination and read)
Black anodized aluminum
Reflection & Transmission Stages
The Single-Point Reflection Stage (at right) is a probe holder for reflection measurements of
optical layers and other substrates up to 150 mm in diameter. The probe holder accommodates
fiber optic probes up to 6.35 mm in diameter, and slides up and down a stainless steel post for
adjustment to heights as great as ~63.5 mm. The Stage has an anodized base plate scored in
concentric circles of varying diameters, to act as a guide when positioning round samples.
Sampling Accessories
Dimensions:
Weight:
Sample port:
Connectors:
Surface mount:
Angles of incidence:
Recommended fibers:
Material:
The RSS-VA has two ports for SMA 905-terminated
optical fibers: one to illuminate the optical substrate,
the other to collect the reflectance and send it to the
spectrometer (see drawing). This fiber-in/fiber-out
design takes advantage of a sophisticated optical train
that allows users to change the angle of incidence
(AOI) from 10° to 50° simply by manipulating the
carriage inside the black anodized stainless steel device
housing. Also included is a three-point surface mount
for holding the sample in a fixed position. To normalize
measurements taken with the RSS-VA, you will need a
reflectance standard such as the Specular Reflectance
Standards on page 108.
RSS-VA:
$1,400
RSS-VA-ADP:
$99
The Stage-RTL-T is a novel sampling system for analysis of substrate materials such as silicon,
metals, glass and plastics. The RTL-T couples to our spectrometers and light sources, and can
be used in a variety of setups for reflection and transmission measurements. The Stage-RTL-T
consists of a variable rail attached to a base plate, with three devices that attach to the rail with
a thumbscrew. These devices are a fiber holder with collimating lens, a sample holder for
reflection or transmission, and a light trap to mitigate the effects of back
reflection and ambient light. The STAGE-RTL-T is remarkably versatile:
perform reflection measurements with the probe positioned above or below
the sample (measuring from below maintains a constant distance between
probe and sample); make reflection measurements with the light trap in
place; or measure transmission of samples using two fibers.
STAGE:
$631
STAGE-RTL-T: $2,303
Specifications
Dimensions:
Dimensions:
Weight:
Height:
Materials:
STAGE
152.4 mm diameter (base)
101.6 mm diameter* (sample area)
620 g
Rail height adjustable to 63.5 mm
Anodized aluminum plate, stainless steel
post and post holder
STAGE-RTL-T
206.3 mm diameter (base)
152.4 mm diameter (sample area)
4.5 kg
Rail height adjustable to 400 mm
Anodized aluminum
* Represents the area of scored concentric circles. You could use the entire base plate area, which is
larger, for your sample.
Tel: 727.733.2447 • Email: [email protected]
109
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Optical Flats
Fused Silica Optical Flats
Sampling Accessories
Item
Aluminum
Coating
Flatness
Price
0.5"
No
1/10λ
$200
0.5"
Yes
1/10λ
$250
1.0"
0.5"
No
1/20λ
$225
FLS-12-SSM
1.0"
0.5"
Yes
1/20λ
$270
FLS-14-SS
1.0"
0.5"
No
1/4λ
$170
FLS-14-SSM
1.0"
0.5"
Yes
1/4λ
$210
FLS-20-SS
2.0"
0.5"
No
1/10λ
$290
FLS-20-SSM
2.0"
0.5"
Yes
1/10λ
$330
FLS-22-SS
2.0"
0.5"
No
1/20λ
$350
FLS-22-SSM
2.0"
0.5
Yes
1/20λ
$400
FLS-24-SS
2.0"
0.5"
No
1/4λ
$230
Visual Reference
FLS-24-SSM
2.0"
0.5"
Yes
1/4λ
$255
Each Optical Flat is a finely polished optical reference
surface that can be used to visually inspect the flatness of
optical components such as mirrors, filters, prisms and
windows. Flats can also be used as windows for
interferometry applications.
FLS-40-SS
4.0"
0.75"
No
1/10λ
$650
FLS-40-SSM
4.0"
0.75"
Yes
1/10λ
$765
FLS-42-SS
4.0"
0.75"
No
1/20λ
$765
FLS-42-SSM
4.0"
0.75"
Yes
1/20λ
$875
FLS-60-SS
6.0"
1.0"
No
1/10λ
$1,200
FLS-60-SSM
6.0"
1.0"
Yes
1/10λ
$1,325
What to Select
FLS-62-SS
6.0"
1.0"
No
1/20λ
$1,395
We offer single-sided flats made from either fused silica
or Zerodur, each of which can be enhanced with an
aluminum coating to increase contrast and improve the
visual reference. We manufacture flats ranging from
1" to 6" in diameter and with flatness accuracies as
precise as 1/20 wave.
FLS-62-SSM
6.0"
1.0"
Yes
1/20λ
$1,665
Aluminum
Coating
Flatness
Price
Fused Silica or Zerodur
Your selection of fused silica or Zerodur flats depends on
the application. Fused silica has a low thermal expansion
and is highly resistant to abrasion. Zerodur is a glass
ceramic that exhibits an even lower thermal expansion,
making it useful for applications with significant
temperature fluctuations.
How Flats Work
The choice of flatness accuracy depends on the
application. For example, if the test surface is flatter than
1/4 wave, a more precise 1/10 wave flat is required to
display the interference pattern change. When an
Optical Flat is placed in contact with a test surface and
illuminated with monochromatic light, an interference
pattern of light and dark bands forms. A curved
interference pattern like the one shown here indicates
that the flatness of the test
surface is less than that of
the reference. Evenly
spaced patterns
indicate that the
flatness of the test
surface is equal to or
higher than that of the
reference.
Diameter
Center
Thickness
FLS-10-SS
1.0"
FLS-10-SSM
1.0"
FLS-12-SS
Zerodur Optical Flats
Item
Diameter
FLZ-10-SS
1.0"
0.5"
No
1/10λ
$200
FLZ-10-SSM
1.0"
0.5"
Yes
1/10λ
$250
FLZ-12-SS
1.0"
0.5"
No
1/20λ
$225
FLZ-12-SSM
1.0"
0.5"
Yes
1/20λ
$270
FLZ-14-SS
1.0"
0.5"
No
1/4λ
$170
FLZ-14-SSM
1.0"
0.5"
Yes
1/4λ
$210
FLZ-20-SS
2.0"
0.5"
No
1/10λ
$290
FLZ-20-SSM
2.0"
0.5"
Yes
1/10λ
$330
FLZ-22-SS
2.0"
0.5"
No
1/20λ
$350
FLZ-22-SSM
2.0"
0.5"
Yes
1/20λ
$400
FLZ-24-SS
2.0"
0.5"
No
1/4λ
$230
FLZ-24-SSM
2.0"
0.5"
Yes
1/4λ
$255
FLZ-40-SS
4.0"
0.75"
No
1/10λ
$650
FLZ-40-SSM
4.0"
0.75"
Yes
1/10λ
$765
FLZ-42-SS
4.0"
0.75"
No
1/20λ
$765
FLZ-42-SSM
4.0"
0.75"
Yes
1/20λ
$875
FLZ-60-SS
6.0"
1.0"
No
1/10λ
$1,200
FLZ-60-SSM
6.0"
1.0"
Yes
1/10λ
$1,325
FLZ-62-SS
6.0"
1.0"
No
1/20λ
$1,395
FLZ-62-SSM
6.0"
1.0"
Yes
1/20λ
$1,665
Specifications
Surface quality:
Wedge:
Tolerance:
Refractive index:
Abbe #:
Thermal expansion:
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Center
Thickness
FLS (Fused Silica)
FLZ (Zerodur)
60-40
< 5 minutes
± 1 mm on CT
± 0.25 mm on diameter
1.458 nd
67.7 vd
0.55 x 10-6 ºC-1
60-40
< 5 minutes
± 1 mm on CT
± 0.25 mm on diameter
1.542 nd
56.2 vd
0.10 x 10-6 ºC-1
For all your sensing needs, visit OceanOptics.com
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Shear-plate Collimation Testers
Applications Versatility
Use Shear-plate Collimation Testers to examine and
adjust the collimation of laser light, or to measure the
wavefront curvature and divergence/convergence
magnitude of large-radius optical components.
Various Aperture Sizes
from 350-2500 nm
Each tester is useable from 350-2500 nm, and is
available in apertures ranging from 10-200 mm. Each
tester consists of a wedged, high-quality optical flat
housed in a heavy-duty anodized aluminum frame.
Basic Operation with
Interferometric Design
Sampling Accessories
The testers are remarkably easy to use: When a planar
wavefront is incident at an angle of 45°, two reflected
wavefronts result. The lateral separation of these
wavefronts is referred to as
shear. Fringes -- parallel
patterns of light and
dark areas -- will be
seen in the
overlapping region
of the two images.
Collimating the
laser beam is a
matter of adjusting
the collimating system
until the fringe pattern is
parallel to the shadow of the
collimation tester's reference wire.
Collimation Testers
Item Code
Aperture Size
Price
CT-10
10 mm
$600
CT-20
20 mm
$700
CT-50
50 mm
$800
CT-75
75 mm
$950
CT-100
100 mm
$1,200
CT-125
125 mm
$1,700
CT-150
150 mm
$2,800
CT-200
200 mm
$4,800
Thin Film Reference Wafer
5-step Wafer
When measuring the thickness of substrates such as silicon wafers
or optical layers, consider our Silicon-Silicon Dioxide (Si-SiO2)
Reference Wafer. This 9.8-cm (4”) diameter, 5-step wafer has a
calibrated thickness range of 0-500 nm, and is ideal for use as a
reference standard when measuring the thickness of thin,
transparent layers on various substrates.
Calibrated
The Reference Wafer consists of a thin wafer of silicon dioxide on
silicon, with each transparent step numbered and etched on the
wafer surface. A calibration data sheet -- the wafer is calibrated
using an ellipsometer -- includes information for each step such as
the X and Y positions, δ (Psi), ψ (Delta), period (in nm) and
thickness (in nm).
REFERENCE:
$669
Tel: 727.733.2447 • Email: [email protected]
Step Sizes
0-500 nm with 100 nm steps:
0 nm (uncoated)
100 nm (± 20 nm)
200 nm (± 20 nm)
300 nm (± 20 nm)
400 nm (± 20 nm)
500 nm (± 20 nm)
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Long Trace Profilometer
Unique Optical Profiling Tool
The LTP-V Long Trace Profilometer is an
interferometric optical profiling instrument for
absolute figure measurement of flats, spheres and
aspheres up to 1500 mm in diameter. The LTP-V
characterizes the figure and mid-frequency errors
on cylindrical aspheres over one meter in length,
and excels at measuring the shape of exotic
aspheric optics, adaptive optics and mirrorbending mechanisms. With the LTP-V, optical
surfaces can be measured quickly, easily and with
nanometer precision and accuracy -- without the
need for null corrector lenses or external
reference surfaces. It is the only instrument now
available for absolute figure measurement of
optics as large as 150 cm in diameter.
About the Instrument
Sampling Accessories
Conceived at Brookhaven National Laboratory
and commercialized by Continental Optical in the
early 1990s, the Long Trace Profilometer has
been completely redesigned since our acquisition
of Continental Optical in 2000. The LTP-V is a
slope-measuring interferometer that measures the
phase difference between two co-linear probe
beams as they move across the sample surface. It
is extremely insensitive to vibrations, which makes
it suitable for use in laboratory environments.
Absolute Accuracy
What sets the LTP-V apart from other profilemeasuring instruments is its ability to correct for
real-time probe beam angular errors during the
traverse of the linear beam, without the need for
a calibrated external reference standard.
Variations in the probe beam pointing direction
are measured and subtracted from the test
surface slope, resulting in the absolute slope
profile and measurement of the absolute radius
of curvature of the test surface.
Pricing
The LTP-V has a linear servomotor that’s so accurate it can
position itself within 0.5 mm. The streamlined optical head
design (shown above) is temperature-insensitive and has
only two optical controls -- beam amplitude and sampleversus-reference balance. A polarizing beamsplitter is
accurate to 1/20 wave. Included is a miniature CCD-array
system that interfaces to PCs via a USB cable.
Specifications
Scan length:
Scan velocity:
Position accuracy:
Slope accuracy:
Height accuracy:
Slope measurement range:
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1500 mm
3 mm/second (assuming 1-mm steps, 1 sample)
± 0.5 µm
<1 microradian
<50 nm; 10-nm variations have been measured
± 5.0 milliradian
A great deal of care and consultation is required
before the purchase of an LTP-V. The cost for the
LTP-V includes these consultations, shipping of the
instrument, installation of the instrument, and
training in its operation. The LTP-VMIR is an
additional attachment for taking vertical and
inverted mirror scans. The LTP-CALSTD is a
calibrated standard mirror for use as a reference
source.
LTP-V:
$120,000
LTP-VMIR:
$1,500
LTP-CALSTD: $1,000
For all your sensing needs, visit OceanOptics.com
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Filter Sample Holders
In-line Filter Holder
The FHS-UV In-line Filter Holder is a dual-purpose fixture for
projecting a collimated beam of light through a flat optical filter. The
FHS-UV can measure the transmission of filters, or provide a location
in an optical system for inserting filters. It has two 74-UV Collimating
Lenses mounted across a filter holder, which holds round filters up to
25 mm in diameter and samples up to six millimeters thick. (For
large filters and other samples, see the 74-ACH Adjustable
Collimating Lens Holder.) A bushing keeps the filter against the
reference surface. A shutter facilitates taking dark measurements.
FHS-UV:
$399
FHS-UV In-line
Filter Holder
Filter & Cuvette Holders
Sampling Accessories
What’s unique about the FHSA Filter/Cuvette Holders is you can
configure the holders to sample either cuvettes or filters. Use the
FHSAs to measure transmission of 1-cm square cuvettes or filters
up to seven millimeters thick. In addition, FHSAs interface via
RS-232 bus to PCs, allowing you to control some functions of the
FHSAs via software, which is included. With the FHSA-TTL, you
have manual control of attenuation (adjustable from 0-100%), and
manual or software control of a shutter. With the FHSA-RS232, you
have software control of both the attenuation and shutter functions.
Both versions include a 12 VDC power supply.
FHSA-TTL:
$1,332
FHSA-RS232: $2,349
FHSA-TTL as Filter Holder
Specifications
Dimensions:
Weight:
Power consumption:
Filter size (maximum):
FHSA-TTL
140 mm x 50 mm x 50 mm
490 g
100 mA @ 12 VDC
Any sample up to 7 mm thick
Light source:
Wavelength range:
Optical fibers required:
Cuvette dimensions:
Shutter frequency:
Shutter response time:
None
200-2000 nm
Yes
10 mm x 10 mm
5 Hz/60 dB (maximum)
7 µsec
FHS-UV
50.6 mm x 140 mm x 43.1 mm
240 g
None
25-mm diameter round;
any sample up to 6-mm thick
None
200-2000 nm
Yes
None
None
None
FHSA-TTL as Cuvette Holder
Filter Holders for Optical Fibers
The INLINE-FH In-line Filter Holder (top photos) holds INLINE-OF Filters or other
filters 8 mm in diameter and 2-5 mm thick. The Filter Holder includes two collimating
lenses and connects to two fibers for in-line filtering. The FH-SMA (bottom photos)
allows you to mount filters or diffusers at the end of SMA 905-terminated optical
fibers. The FH-SMA accepts 8-mm diameter filters in thicknesses of 1-7 mm. See
page 164 for information on available filters for the INLINE-FH or FH-SMA.
INLINE-FH:
$436
INLINE-OF:
$102
FH-SMA:
$142
Specifications
Dimensions:
Weight:
Filter size:
Material:
FH-SMA
16 mm diameter
10 g
8 mm diameter, 1-7 mm thick
Anodized aluminum
INLINE-FH
15 mm diameter
20 g
8 mm diameter, 2-5 mm thick
Stainless steel (collimating lenses have
anodized housings)
Tel: 727.733.2447 • Email: [email protected]
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Linear Variable Filters
Novel Filtering Technology
We've combined our patented high-pass and low-pass Linear
Variable Filters to create the world's first bandpass filter with an
adjustable center wavelength and adjustable bandpass. Each
filter features an excellent transmission band (~90%) and
blocking band (99.8%). These filters -- with interference
coatings applied to 57 mm x 10 mm quartz substrates -- are
especially useful for spectrally shaping the excitation energy
from broadband sources used for fluorescence.
Slide Carriers
These off-the-shelf filters are epoxied into slide carriers that allow you
to move the transmission or blocking band throughout the filter’s
wavelength range.
LVF-HL Variable Bandwidth Filter
Sampling Accessories
%TRANSMISSION
80
60
40
Single High-pass & Single Low-pass Filter
The LVF-H High-pass Filter is a single filter that blocks light at 98.8%
up to a transition wavelength that varies along its length. At that
point, the LVF-H passes light better than 90%. The LVF-L Low-pass
Filter is a single filter that passes light at 88% up to a transition
wavelength that varies along its length. At that point, the LVF-L blocks
light better than 98.8%.
20
0
250
Double High-pass & Double Low-pass Filters
350
450
550
WAVELENGTH (nm)
650
These spectra were taken with an LVF-HL to show
how a transmission bandwidth can be set throughout
the filter's range (300-750 nm).
LVF-H High-pass Filter
High-pass & Low-pass Variable Bandpass Filters
100
By fastening together a high-pass filter and a low-pass filter, we
created a variable bandpass filter that allows you to adjust the center
wavelength and the bandwidth. We preset the transmission
bandwidth at ~25 nm FWHM, but adjusting four screws allows you
to slide the filters against one another to create a transmission
bandwidth as wide as ~100 nm and as narrow as ~20 nm.
%TRANSMISSION
80
60
40
20
0
250
We take two identical LVF-H or LVF-L filters, align them so that the
transition wavelengths of both filters are matched, and then epoxy
them together in their slide carriers. The benefit of having double
filters versus a single filter is that the optical density of the blocking
band increases to 99.96%. However, the transmission band is
reduced to 80%.
350
450
550
WAVELENGTH (nm)
650
750
The transition wavelength from blocking to
transmission band varies according to the filter's
position in front of the collimating lens.
LVF Accessories
The LVF filters and slide carriers can be inserted easily into
spectrometer setups with our LVF accessories. See the next page
for details.
Item
Description
Price
LVF-H
A single high-pass filter for 300-750 nm
$249
LVF-L
A single low-pass filter for 300-750 nm
$249
LVF-HH
Two LVF-H high-pass filters epoxied together for 300-750 nm
$499
LVF-LL
Two LVF-L low-pass filters epoxied together for 300-750 nm
$499
LVF-HL
An LVF-H high-pass filter and LVF-L low-pass filter fastened together to create an adjustable bandpass
$499
linear variable filter
LVF-UV-H
A single high-pass filter for 230-500 nm
$249
LVF-UV-L
A single low-pass filter for 230-500 nm
$249
LVF-UV-HH
Two LVF-UV-H high-pass filters epoxied together for 230-500 nm
$499
LVF-UV-LL
Two LVF-UV-L low-pass filters epoxied together for 230-500 nm
$499
LVF-UV-HL
An LVF-UV-H high-pass filter and LVF-UV-L low-pass filter fastened together to create an adjustable
$499
bandpass linear variable filter
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For all your sensing needs, visit OceanOptics.com
Accessories for Linear Variable Filters
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LVF Accessories in Setups
We offer several LVF Linear Variable Filters as either
high-pass, low-pass or, when we use them as pairs
-- as we do for the LVF-HL -- variable bandwidth
filters. These filters are installed into slide carriers,
which can accommodate both the single-filter and
double-filter configurations. The slide carriers fit
into our slide carrier accessories, which make it
possible to integrate LVFs with our spectrometers
and accessories into fluorescence and
absorbance setups.
The LVF is epoxied into a
slide carrier, which fits into
such LVF accessories as
the FH-LVF Filter Holder.
The CVD-DIFFUSE
redirects excitation
energy into the
spectrometer and
helps set the filter
position.
In-Line Filtering with LVFs
Sampling Accessories
The FHS-LVF is an in-line filter
holder used in absorbance and
transmission applications.
This in-line LVF holder
features two collimating
lenses with SMA 905
Connectors. Its slot
accommodates the LVF slide carrier.
Screws hold the LVF in place.
Cuvette Holder Adapter
The LVF-CUV-ADP is an adapter that fits onto our
1-cm cuvette holders and holds the LVF slide
carrier. The cuvette adapter slides over the top of
the cuvette holder and includes screws to clamp the
LVF’s slide carrier into place. The LVF-CUV-ADP
comes with a cover to block out ambient light.
Diffuser for Redirecting Excitation Light
The CVD-DIFFUSE, a 1-cm cuvette-shaped piece of
PTFE material, has a 45° surface at the
measurement height and is used with an LVF in a
fluorescence cuvette holder to redirect excitation
energy 90° into the spectrometer. This facilitates
setting the filter position -- i.e., while the
CVD-DIFFUSE is inserted in the cuvette holder, you
position the LVF to select the wavelength region
passed by the filter.
When using an LVF with a
cuvette holder like our
CUV-ALL 4-way Cuvette
Holder, you will need the
LVF-CUV-ADP Cuvette
Holder Adapter. The LVF
(in a slide carrier) is
inserted in front of the
sample and held in place
by the LVF-CUV-ADP
(shown at right), with a
cover to block ambient
light.
Item
Description
LVF-CUV-ADP
An adapter for a 1-cm pathlength cuvette holder that holds the slide carriers in place
CVD-DIFFUSE
A 1-cm cuvette-shaped PTFE for redirecting excitation energy
FHS-LVF
In-line filter holder for LVFs
$399
LVF-KIT
Consists of the LVF-HL, LVF-CUV-ADP, FHS-LVF and CVD-DIFFUSE
$999
LVF-UV-KIT
Consists of the LVF-UV-HL, LVF-CUV-ADP, FHS-LVF and CVD-DIFFUSE
$999
Tel: 727.733.2447 • Email: [email protected]
Price
$99
$99
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Fiber Optic Dual Switch with TTL Line
The FOS-2X2-TTL Fiber Optic Dual Switch was designed to provide you with flexibility
in routing, splitting and controlling light. The FOS has two light channels. You can
opt to have one light channel open at a time or have both closed. The FOS is useful
for monitoring the drift of the light source or for measuring two samples with one
spectrometer channel and one light source. The diagram below is an example of
how the FOS can be utilized. In this setup, the FOS eliminates the need for a second
spectrometer channel.
FOS-2X2-TTL: $1,664
Sample 1
P400-025-SR
Spectrometer
Light
Source
BIF400-UV-VIS
Sample 2
P400-025-SR
BIF400-UV-VIS
FOS-2X2-TTL
Specifications
Sampling Accessories
In this setup, light enters a Bifurcated Optical Fiber Assembly and then splits into two arms, one for
each sample. Light interacts with each sample and travels through another fiber assembly, each
into its own port in the FOS. Another Bifurcated Assembly collects the light from the FOS and
sends it to the spectrometer. Here you would switch the shutter on the FOS from one light channel
to another in order to get clean data from each sample. Without the FOS, you would need another
spectrometer channel to monitor the two samples.
Dimensions:
Weight:
Material:
Switch frequency:
Power:
Operation:
100 mm x 70 mm x 70 mm
455 g
Anodized aluminum
Maximum of 5 Hz
12 VDC
Manual switch or TTL input signal
Electronic TTL Shutter
In spectrometer setups, the INLINE-TTL TTL-driven shutter allows you
to block the light path without disturbing the experiment -- for
example, by turning the light source on and off. The laser-cut shutter
is installed between two collimating lenses, which attach to two optical
fibers. The INLINE-TTL is driven by a small board with a TTL input.
Included is a cable for interfacing to a spectrometer.
INLINE-TTL-S:
$1,076
Specifications
Dimensions:
Weight:
Shutter-Input:
Power requirements:
Power consumption:
Maximum frequency:
140 mm x 50 mm x 50 mm
~600 g
TTL maximum 5 Hz
12 VDC (power supply included)
100 mA maximum
5 Hz
Field of View Control
The Gershun Tube Kit (GER-KIT) controls the field of view of our
SMA 905-terminated optical fiber. It also directly attaches to a spectrometer with an SMA 905 Connector. User-interchangeable apertures
provide many different fields of view from 1° to 28°. (When the
GER-KIT is used with our optical fiber, the field of view cannot exceed
the optical fiber's 25° field of view if you are measuring radiance.)
GER-KIT:
$499
Specifications
Material:
Interior:
Connection:
Apertures:
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Black anodized aluminum
Bead-blasted surface to reduce off-axis reflections
Directly attaches to one of our spectrometers or couples to an
SMA 905-terminated optical fiber with included adapter barrel
1°, 3°, 8°, 10° and 14° apertures included, providing
1°, 2°, 3°, 6°, 8°, 10°, 14°, 16°, 20° and 28° fields of view
For all your sensing needs, visit OceanOptics.com
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Optical Multiplexer
Flexibility for Multipoint Sampling
Our MPM-2000 Fiber Optic Multiplexers take light to
a spectrometer or from a light source connected to
one of the input ports and distribute it to either
8 or 16 outputs. The light is distributed through
the output ports in sequential order, with
switching times between channels of less than
150 milliseconds. Multiplexers often are found in
process industries, where multiple locations need to be
measured with one spectrometer channel and/or light source.
An MPM-2000-2x8 has two
input ports and 16 outputs.
Here, we used a USB2000
Spectrometer and an LS-1
Light Source as the
input ports.
High-precision Instrument
All versions of the MPM-2000 include a DC motor, which has
excellent speed control without sacrificing power. The motor is on
a rotator block and includes an encoder, which converts
movement into a digital pulsed output. Each channel in the
multiplexer has a collimating lens connecting to an internal
optical fiber system. The MPM-2000 provides accurate
measurements with an excellent repeatability of 99%.
Multiple Versions
Specifications
Dimensions:
230 mm x 200 mm x 150 mm
(fits into 19" system: 33TE, 3HE, etc.)
Wavelength range: 250-800 nm (UV/VIS) or 350-2000 nm (VIS/NIR)
Optical throughput: > 60% when using standard 400 µm fibers @ 650 nm
Motor:
Direct-current motor
Optical fibers:
400 µm diameter optical fibers
Repeatability:
> 99%
Switching time:
150 milliseconds between adjacent positions
Interface:
RS-232 (optional USB)
Power requirement: 24 VDC, 1.2 A (includes WT-24V-E power supply)
Connectors:
SMA 905
Software-controlled
The multiplexers interface to a PC via an RS-232 port and come
with software and a driver for complete PC control. The software
allows you full control of the switching order, switching delay time
and system calibration.
MPM-2000-1X16-UV: $8,401
MPM-2000-1X16-VIS: $8,401
MPM-2000-2X8-UV:
$8,736
MPM-2000-2X8-VIS:
$8,736
Sampling Accessories
The MPM-2000 comes with either two input channels -- with each
input channel corresponding to eight output channels -- or with
one input channel and 16 output channels. Choose either a
UV-VIS (250-800 nm) or VIS-NIR (350-2000 nm) multiplexer.
Fiber Optic Variable Attenuator
The FVA-UV Fiber Optic Variable Attenuator is an opto-mechanical
device that helps control the amount of light transmitted between two
fibers. Two fibers screw into either side of the FVA-UV via SMA 905
Connectors with collimating lenses, which project light across a metal
disc in which a slit has been cut. The width of the slit varies as a function
of radial position, which is adjusted manually. Rotating the disc varies the
attenuation from 0-100% uniformly across a 200-2000 nm wavelength
range. An FVA-ADP attaches the FVA-UV directly to a light source.
FVA-UV:
$499
FVA-ADP:
$99
Specifications
Dimensions:
Weight:
Assembly ports:
Wheel lock:
ADP adapter:
Connector:
38.1 mm x 59.4 mm x 40 mm
90 g
3/8-24 threads for collimating lenses
6-32 nylon thumbscrew
Directly attaches to a light source with a collimating lens
SMA 905
Tel: 727.733.2447 • Email: [email protected]
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XYZ Mapping Tables
Versatile Design
We offer four high-precision linear XYZ Mapping Tables. The mapping
table -- with a linear axis resolution of 1 µm and an accuracy of ± 5 µm
-- is ideal for spatial mapping of spectral features or for multisampling
in microwell plates. See the table below for table options and prices.
Additional Functions
The XYZ Table comes with an electric motor and encoder to drive each
axis, along with a CNC Controller and a portal for the vertical (Z-axis)
stage. The table makes it possible to measure every sample within an
X-Y range of 150 mm x 150 mm or 200 mm x 150 mm. With the
100-mm vertical (Z-axis) stage, you can attach holders for probes and
other sampling devices, which are purchased separately.
PC Control
Sampling Accessories
The system requires 110-240 VAC to operate (included) and interfaces
via RS-232 bus to PCs. Computer-controlled operation of the motors is
available. Contact an Applications Scientist for details.
Item
X-axis
Y-axis
Z-axis
XY(Z)-150 X150+
150 mm
150 mm
Optional
Price
$12,650
XY(Z)-200X150+
200 mm
150 mm
Optional
$13,119
XYZ-150 X150X100
150 mm
150 mm
100 mm
$15,397
XYZ-200X150X100
200 mm
150 mm
100 mm
$15,866
Z-AXIS-100+
None
None
100 mm
$2,896
Dimensions base:
Dimensions rail:
Weight:
Power input:
Travel range:
Controller:
Interface:
476 x 375 x 89 mm
508 x 38 x 165 mm
14.7 kg
110-240 VAC
150 mm x 150 mm (minimum)
CNC Controller (2-3 axes)
RS-232
NTS-series Linear Nanopositioners
The NTS-series Linear Nanopositioners are software-controlled
linear nanopositioning systems that combine superior 0.4 nm
high-resolution incremental movement and extended travel
range (10 mm, 25 mm and 100 mm). Competing technologies
are limited in that they provide either high resolution or
extended travel range, but not both. What’s more, the systems
offer long-term stability in open loop mode of less than 2 nm
drift per hour for high repeatability and accuracy. The NTSseries Nanopositioners can be used in applications including
metrology, semiconductor analysis, microscopy, cell
manipulation, microlithography and fiber optic alignment.
NTS-25 25 mm Linear
Nanopositioner
NTS-100 100 mm Linear
Nanopositioner
The nanopositioners feature piezoelectric motors that have high
torque (0.2 Newton meter), variable speeds and high angular
resolution. Additionally, the motor uses a shaft-mounted 4000
counts/revolution optical encoder. These features enable both
continuous or step operation modes to provide accurate angular
positioning. For details on the NTS Nanopositioners and
Controllers, visit www.oceanoptics.com/products/nts10.asp.
NTS-ND-3 Controller
Item
Description
NTS-10
Nanopositioner, 10 mm travel
$3,500
Price
NTS-25
Nanopositioner, 25 mm travel
$3,800
NTS-100
Nanopositioner, 100 mm travel
$4,950
NTS-ND-1
NTS Controller, 1 axis
$2,000
NTS-ND-2
NTS Controller, 2 axes
$2,500
NTS-ND-3
NTS Controller, 3 axes
$3,000
NTS-NJ
Joystick controller
$400
NTS-SOFTWARE
NTS Operating Software
Free
LabVIEW software available; contact an Applications Scientist for details.
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Specifications
118
Features include:
Resolution of 1 nm and wide velocity range (5 orders)
Acceleration time to maximum velocity less than 0.3 ms
Continuous or stepping modes
Self-locking technology, eliminated "stick-slip" effect
DSP Controllers for 1-, 2- or 3-channel configurations
enable wide dynamic range and high accuracy
Stages support loads up to 3 kg
For all your sensing needs, visit OceanOptics.com
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Light Sources
Overview
121
Ways to Modify Light
122
Balanced Deuterium Tungsten Source
123
Deuterium Tungsten Halogen Sources
124
Mini Deuterium Tungsten Halogen
Sources
126
Deuterium Light Sources
127
Xenon Sources
128
Tungsten Halogen Light Sources
130
LED Light Sources
132
Radiometric Calibration Standards
134
Wavelength Calibration Standards
136
Bulbs, Power Supplies & Accessories
Light Sources
120
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Overview: Light Sources
Sources for Illumination, Excitation, Calibration
The development of Ocean Optics miniature fiber optic spectrometers created
the need for comparably sized and priced accessories, including light sources.
Since no such sources existed, we developed our own -- compact, modular
sources complemented by the best bulbs for spectroscopy that our vendor
partners can provide.
Sources for illumination cover various wavelength ranges to enable
absorbance, reflectance and fluorescence measurements from the deep UV to the
NIR. Compact light-emitting diodes produce output for fluorescence
measurements. For fast, reliable spectrometer wavelength calibrations, we offer
Mercury and Argon sources. Design features such as built-in filter slots, combined with
optional accessories such as direct-attach cuvette holders, make sampling simple.
Ocean Optics Modular Light Source Options
Deuterium Light Sources: Used most often for UV
absorbance and reflectance measurements.
Light Sources
Combination Deuterium and Tungsten Light Sources:
Used as single illumination sources for measurements
across broad wavelength ranges.
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Pulsed Xenon Lamps: Used as long-life sources for
absorbance, reflectance and fluorescence measurements,
and for measuring optically or thermally labile samples.
Calibrated Light Sources: Used to calibrate the absolute
spectral intensity of a system in irradiance applications.
Tungsten Halogen Light Sources: Used most often as
standard VIS-NIR light sources for absorbance, reflectance
of solid objects, and color measurement.
Light-emitting Diodes: Used as excitation sources for
fluorescence. Feature minimal warm-up and high stability.
Power is lower and spectral width is wider than with
lasers.
Wavelength Calibration Sources: Used to calibrate
the wavelength of spectrophotometric systems.
The mercury argon source is for UV-NIR and the argon
source is for VIS-NIR.
Type
Product
Wavelength Range
Output
Measurement Type
Deuterium Tungsten
Halogen
DH2000-BAL
DH2000
~230-2000 nm
Continuous
Absorbance, Reflectance,
Fluorescence, Transmission
122
123
Miniature Deuterium
Tungsten Halogen
DT-MINI-2
DT-MINI
DT-MINI-2-GS
USB-DT
~200-2000 nm
Continuous
Absorbance, Transmission,
Reflectance
125
125
125
124
Deuterium
D2000
~215-400 nm
Continuous
Absorbance, Reflectance,
Fluorescence, Transmission
126
Xenon
PX-2
HPX-2000
220-750 nm
185-2000 nm
Pulsed
Continuous
Absorbance, Reflectance,
Fluorescence, Transmission
127
LEDs
LEDs (several
wavelengths)
380, 395, 470, 475, 518,
590, 640 and 450-630 nm
Pulsed or
Continuous
Fluorescence
Tungsten Halogen
LS-1
HL-2000
360-2000 nm
360-2000 nm
Continuous
Absorbance, Reflectance,
Transmission
128
129
Calibrated Deuterium
Tungsten Halogen
DH2000-CAL
~220-1050 nm
Continuous
Calibration (Radiometric)
132
Calibrated Tungsten
Halogen
LS-1-CAL
HL-2000-CAL
300-1050 nm
300-1050 nm
Continuous
Calibration (Radiometric)
133
Mercury Argon
HG-1
CAL-2000
253-1700 nm
253-1700 nm
Continuous
Calibration (Wavelength)
134
Argon
AR-1
700-1700 nm
Continuous
Calibration (Wavelength)
135
120
Page
130-131
For all your sensing needs, visit OceanOptics.com
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Overview: Light Sources
Ways to Modify Light
Our products provide you with many options for
modifying the light transmitted to the spectrometer’s
detector. The illustration here is a fabricated
configuration -- as few would have a setup exactly like
it -- to demonstrate several ways in which you can
modify light.
Notebook
Computer
USB4000 Spectrometer
7
For high-intensity light-level applications such as laser
characterization, more light will reach the
spectrometer than likely can be detected successfully
by the high-sensitivity CCD-array detector used in
most of our spectrometers. Also, some absorbance
experiments may require signal attenuation; too much
light can saturate the reference measurement.
3
LS-1 Light Source
with Filter Slot
Cuvette Holder
with Filter Slot
6
Fiber Optic
Variable Attenuator
5
3
4
Our loose filters fit into our light
sources, cuvette holders and in-line
filter holders. High-pass Filters
eliminate second- and third-order
effects, test for stray light, and block
excitation energy. Balancing Filters
absorb energy in some regions while
transmitting in others. Bandpass Filters
pass energy in one region and block
light above and below that region.
Installed Filters
2
6
4
7
5
Linear Variable Filters
Our high-pass, low-pass and adjustablebandpass filters have excellent blocking
characteristics and resistance to heat,
making these filters ideal for spectrally
shaping the light emitted from
broadband sources.
Tel: 727.733.2447 • Email: [email protected]
6
Fiber Optic Variable Attenuator
The FVA-UV Fiber Optic Variable
Attenuator is an opto-mechanical
device that helps control the amount of
light transmitted between two fibers.
The FVA-UV attenuates light uniformly
at all wavelengths from the ultraviolet
through the near-infrared.
3
Optical Fiber
Our optical fibers are available from
8 µm to 1000 µm in diameter. If you
need a great deal of light for your
application, you should select a largediameter fiber. Also, in the absence of a
slit, the fiber connected to the
spectrometer acts as the optical bench
entrance aperture.
Loose Filters
Light Sources
1
Entrance Aperture: Slit
In addition to the variable longpass
OFLV Filter -- an order-sorting filter
applied to the detector’s window -- we
offer optional bandpass and longpass
blocking filters to restrict radiation in
certain wavelength regions.
5
5
An installed slit acts as the entrance
aperture to the optical bench and
regulates the amount of light entering
the optical bench. The slit size is
specified by the user. Slits are optional,
and range in size from 5 µm to 200 µm.
2
2
1
In some instances, saturation is avoided by using a
different grating, changing the optical bench entrance
aperture or adding neutral-density filters to the optical
path. Another option is to adjust (via software) the
spectrometer integration time to limit the interval
during which the detector collects light.
1
2
Integration Time
Integration Time is a setting in our
software and is specified by the user.
The integration time of the
spectrometer is analogous to the
shutter speed of a camera. The higher
the value specified for the integration
time, the longer the detector “looks” at
the incoming photons. For more
information about integration time, see
any of our software manuals.
121
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Balanced Deuterium Tungsten Source
UV-NIR Spectral Range with Balanced Output
We’ve applied our expertise in patterned dichroic filters
to an innovation in light source technology to create the
only combined-spectrum illumination source available
that eliminates saturation and signal-to-noise problems
associated with the D-alpha line in the deuterium source.
The DH2000-BAL Deuterium Tungsten Halogen Light
Source combines deuterium and tungsten halogen light
sources in a single optical path, producing a powerful,
stable output from 230-2000 nm.
About the D-alpha Line
Light Sources
You can operate the
shutter via a switch
on the front of the
light source . . .
. . . or via a TTL
line from the
back of the lamp.
Here, you can
adjust the
power for the
tungsten bulb.
Proprietary Filtering Technology
Using the same high-precision patterned dichroic filter
technology that distinguishes our Linear Variable Filters
(page 114), the DH2000-BAL:
balances the intensity of the deuterium and
tungsten halogen sources
eliminates the D-alpha, D-beta and Fulcher lines
eliminates problems associated with saturation
produces a “smoother” spectrum across the entire
wavelength range.
DH2000-BAL Spectral Output
600
POWER (µW/cm2/nm)
500
400
300
Upgrading Existing DH2000s with Kits
200
100
0
200
300
400
500
600
700
800
900
1000
WAVELENGTH (nm)
Specifications
Dimensions:
Weight:
Wavelength range:
Power consumption:
150 mm x 135 mm x 319 mm
3.8 kg
230-400 nm (deuterium); 360-2000 nm (tungsten halogen)
25 W (deuterium); 20 W (tungsten halogen);
190 W maximum
Power requirements:
85-264 V 50/60 Hz
Voltage:
Ignition 350 V/20°; tungsten bulb voltage is
adjustable from 4.5 to 11.5 volts
Current:
Operating 85 V/0.3A
Stability:
<5 x 10-6 peak-to-peak (0.1-10.0 Hz)
Drift:
<0.01% per hour
Time to stable output:
20 minutes
Bulb life:
1,000 hours
Operating temperature: 5 °C - 35 °C
Humidity:
5-95% non-condensing at 40 °C
Electronic certifications: CE; VDI/VDE 0160; EN 61010
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122
All deuterium sources have a D-alpha line, revealed as a
sharp peak in the visible portion of the spectrum, that
produces “unbalanced” output in the deuterium and
tungsten halogen sources. Correcting for this peak -- a
sharp spectral feature near 655 nm -- is difficult. For
example, if you adjust spectrometer integration time to
reduce the intensity of this saturated peak, the efficiency
of the system at ultraviolet wavelengths drops
significantly, compromising the signal-to-noise of the
spectrum. Also, spectrometer efficiency is typically
greatest in the same general spectral range as the
655 nm line, exaggerating its effects.
If you own a DH2000 and would like to upgrade the
light source with the filtering technology used in the
DH2000-BAL, but don’t wish to
purchase a new light source, you
can order a DH-BAL-KIT (at left)
and install the upgrade yourself.
For those owning a
DH2000-S shuttered
version of the
lamp, specify the
DH-BAL-KIT-S.
Optical Fibers
We recommend using our solarization-resistant optical
fibers with the DH2000-BAL. See page 146 for details.
DH2000-BAL:
DH-BAL-KIT:
DH-BAL-KIT-S:
$3,588
$1,761
$1,761
For all your sensing needs, visit OceanOptics.com
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Deuterium Tungsten Halogen Sources
UV-NIR Spectral Range
The DH2000 Deuterium Tungsten Halogen Light Source
combines the continuous spectrum of deuterium and
tungsten halogen light sources in a single optical path. The
combined-spectrum light source produces a powerful, stable
output from 215-2000 nm. In addition, deep-UV versions of
the DH2000 are available, with a 190-2000 nm range.
Options & Accessories: Shutter &
Filter Holder
Integrated shutters are available and can
be driven either by a switch or by a TTL
signal. Another option is to include a filter
holder with the source (see inset), which
accepts filters up to four millimeters in
thickness and as large as 25-mm square or
25-mm round in diameter. All versions of the
DH2000 have an SMA 905 Connector for easy
coupling to our spectrometers and accessories via optical
fiber.
DH2000 Spectral Output
1600
1400
DH2000 at full power
1200
DH2000 at low power
1000
800
600
400
200
0
200
Optical Fibers
We recommend using our solarization-resistant optical fibers
with all versions of the DH2000. See page 146 for details.
DH2000: $2,421
400
600
800
1000
WAVELENGTH (nm)
The spectral output of the DH2000 at full power is in red and the
tungsten halogen bulb at low power is in pink.
Light Sources
All versions of the DH2000 have a potentiometer on the
back of the light source to adjust the intensity of the
tungsten halogen output. This potentiometer allows you to
adjust the optical power of the tungsten halogen light from
10-100%.
POWER (µW/cm2/nm)
Adjustable Power
Additional DH2000 Light Sources and Accessories
Item
Description
DH2000-DUV
Uses a deep-UV deuterium bulb, which provides a 190-2000 nm wavelength range
Price
$2,907
DH2000-S
Comes with a shutter controlled via a TTL signal or a manual switch up to 5 Hz
$3,049
DH2000-S-DUV
Uses a deep-UV deuterium bulb, which provides a 190-2000 nm wavelength range and comes
$3,330
DH2000-FHS
Comes with a filter holder for filters up to 25-mm square or 25-mm round and 4-mm thick
$3,328
DH2000-FHS-DUV
Uses a deep-UV deuterium bulb, which provides a 190-2000 nm wavelength range; comes with a filter
$3,752
DH2000-S-DUV-TT
Uses a deep-UV deuterium bulb, which provides a 190-2000 nm wavelength range and comes with a
with a shutter (controlled via a TTL signal or a manual switch up to 5 Hz)
holder for filters up to 25-mm square or 25-mm round and 4-mm thick; and has a shutter controlled via TTL
$3,755
shutter (controlled via an included external TTL line) for remote on/off of the deuterium and halogen bulbs
DH2000-BH
Replacement tungsten halogen bulb for all versions of the DH2000
$158
DH2000-BD
Replacement deuterium bulb for DH2000, DH2000-S, DH2000-FHS
$649
DH2000-DUV-B
Deep-UV replacement deuterium bulb for DH2000-DUV, DH2000-S-DUV, DH2000-FHS-DUV
$775
Specifications
Dimensions:
Weight:
Wavelength range:
150 mm x 135 mm x 319 mm
3.8 kg
190-2000 nm (deep-UV deuterium bulb & tungsten halogen
bulb) or 215-2000 nm (standard deuterium bulb & tungsten
halogen bulb)
Power consumption: 25 W (deuterium); 20 W (tungsten halogen); 190 W maximum
Power requirements: 85-264 V 50/60 Hz
Output:
100 W
Voltage:
Ignition 350 V/20°; tungsten bulb adjustable 4.5-11.5 volts
Current:
Operating 85 V/0.3A
Tel: 727.733.2447 • Email: [email protected]
Stability:
Drift:
Time to stable output:
Bulb type:
Bulb life:
Bulb aperture:
Operating temperature:
Humidity:
Electronic certifications:
Connector:
<5 x 10-6 peak-to-peak (0.1-10.0 Hz)
<0.01% per hour
20 minutes deuterium; 20 minutes tungsten halogen
Deuterium and tungsten halogen
1,000 hours
0.5 mm
5 °C - 35 °C
5-95% without condensation at 40 °C
CE; VDI/VDE 0160; EN 61010
SMA 905
123
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USB-DT Mini Deuterium Tungsten Source
Most Versatile Lamp We Offer
The USB-DT Deuterium Tungsten Light Source is our most versatile
combination UV-VIS light source. There are several ways to use the
USB-DT: as a stand-alone source, stacked atop the USB2000 or
USB4000 Spectrometer via the USB-ADP-DT2 adapter, or connected
to a spectrometer via a Breakout Box. Though the USB-DT can be
stacked on top of the USB2000 or USB4000, it is not the kind of
direct-attach source that eliminates fibers; the USB-DT requires
fibers. This compact source is about the size of a deck of cards,
provides stable, broadband output from 200-2000 nm, and requires
a 5-volt wall transformer for power.
Software Control
When the USB-DT is stacked with the USB2000 or USB4000 or used
with an HR2000+, HR4000 or QE65000 and the Breakout Box, you
can control the following lamp functions through software:
adjusting the intensity of the tungsten source
activating the internal shutter to block the light path
controlling on/off switch of each source independently
utilizing a low-power shutdown mode
saving settings in memory
The USB-DT has a
15-pin connector
for interfacing to
the spectrometer.
Light Sources
Novel Deuterium Tungsten Halogen Sources
Our deuterium tungsten halogen sources combine the continuous
spectrum of deuterium and tungsten halogen lamps in a single
optical path. These combined-spectrum sources produce stable,
continuous UV-VIS output that make them ideal for applications such
as absorbance spectroscopy.
USB-DT:
$1,499
USB-DT-B Bulb:
$399
USB-ADP-DT2:
$75
HR4-BREAKOUT:
$199
Spectrometer
Directly
With USB-DT
Stackable
USB2000
Software Control
of all USB-DT Functions
Yes, with
Yes, when stacked atop the USB2000
USB-ADP-DT2
USB4000
Yes, with
USB-ADP-DT2
The USB-DT can be
set up in a variety of
ways. It can be
stacked with the
USB4000 via the
USB-ADP-DT2
connector (above),
or used as a standalone component
with an Ocean
Optics spectrometer.
with a USB-ADP-DT2
Yes, when stacked atop the USB4000
with a USB-ADP-DT2
HR2000
No
HR2000+
No
Yes, when used with HR4-BREAKOUT
HR4000
No
Yes, when used with HR4-BREAKOUT
QE65000
No
Yes, when used with HR4-BREAKOUT
USB-ADP-DT2
Connector.
No
USB-DT Spectral Output
POWER (µW/cm2/nm)
160
120
Specifications
80
40
0
200
300
400
500
600
700
800
900
Dimensions:
Weight:
Wavelength range:
Power consumption:
Output:
Stability:
Time to stable output:
Bulb life:
WAVELENGTH (nm)
Connector:
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124
81 mm x 90 mm x 37 mm
260 g
200-2000 nm
1.5 A @ 5 VDC
see Spectral Output graph at left
0.5% peak-to-peak (after warm-up)
15 minutes
800 hours for deuterium;
2,000 hours for tungsten
SMA 905
For all your sensing needs, visit OceanOptics.com
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Mini Deuterium Tungsten Sources
~200-2000 nm Spectral Range
Our DT-MINI-series Deuterium Tungsten Halogen
Light Sources combine the continuous spectrum of a
high-powered, RF-excited deuterium light source and
a tungsten halogen light source in a single optical
path. The combined-spectrum sources produce
stable spectral output from ~200-2000, nm in a
compact package.
0.5 mm Aperture: More Powerful Output
The original DT-MINI was our first foray into a
compact and versatile UV-NIR light source, and is
still a great choice for a range of applications and
measurements. The advantage of the newer DTMINI-2 is that it uses a bulb with a 0.5 mm diameter
aperture, which results in more focused, uniform
beam coupling to our optical fibers. Also, the DTMINI-2 is only $100 more than the DT-MINI, which
we will continue to offer.
Shutter Version
Rack-mount Version
Spectral Output: DT-MINI-2 vs. DT-MINI
500
DT-MINI-2 and DT-MINI-2-GS
DT-MINI
POWER (µW/cm2/nm)
400
Rack-mount versions of DT-MINI-series lamps are
available. These sources can be hard-wired to a
spectrometer channel and racked into a Dual Box,
Rack Box or Desktop Box with other accessories. For
more on rack-mount systems and enclosures, see
page 62.
Light Sources
The DT-MINI-2-GS Deuterium Tungsten Halogen
Light Source (lower left) also utilizes the bulb with the
0.5-mm diameter aperture. Its added feature is a
shutter for blocking the light path, which can be
controlled via a manual switch or T TL. There is also
a switch for turning the deuterium source on and off,
and one for turning the tungsten halogen source on
and off (this can also be accomplished via TTL);
each switch can be used independently of the other.
300
DT-MINI-2:
DT-MINI-2-GS:
DT-MINI:
DT-MINI-2-B Bulb*:
DT-MINI-B Bulb*:
200
100
$1,499
$1,754
$1,399
$526
$487
0
200
300
400
500
600
700
800
900
1000
WAVELENGTH (nm)
* The DT-MINI-2-B Bulb can only be used in the DT-MINI-2 and
DT-MINI-2-GS sources. Likewise, the DT-MINI-B Bulb can only
be used in the DT-MINI and DT-MINI-GS.
Specifications
Dimensions:
Weight:
Wavelength range:
Power consumption:
Output:
Stability:
Time to stable output:
Bulb life:
Ignition delay:
Connector:
DT-MINI-2
153.4 mm x 104.9 mm x 40.9 mm
330 g
200-410 nm (deuterium); 360-2000 nm (tungsten halogen)
350 mA @ 12 VDC
3.8 watts (deuterium); 1.2 watts (tungsten halogen)
0.3% peak-to-peak (over 4 hours) after 30-minute warm-up
10 minutes (deuterium); 1 minute (tungsten halogen)
~800 hours (deuterium); 2,000 hours (tungsten halogen)
<2.0 seconds (delay for cold start-up may be longer)
SMA 905
Tel: 727.733.2447 • Email: [email protected]
DT-MINI-2-GS
140 mm x 50 mm x 125 mm
475 g
200-410 nm (deuterium); 360-2000 nm (tungsten halogen)
350 mA @ 12 VDC
3.8 watts (deuterium); 1.2 watts (tungsten halogen)
0.3% peak-to-peak (over 4 hours) after 30-minute warm-up
10 minutes (deuterium); 1 minute (tungsten halogen)
~800 hours (deuterium); 2,000 hours (tungsten halogen)
<2.0 seconds (delay for cold start-up may be longer)
SMA 905
125
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D2000 Deuterium Light Sources
UV Range + Great Performance
The D2000 Deuterium Light Source produces
a powerful, stable output from 215-400 nm.
A deep-UV version is available for wavelength
coverage of 190-400 nm. The D2000 is an
extremely stable source, with peak-to-peak
stability of <0.005% and drift of only ± 0.5%
per hour.
Options & Accessories
All versions of the D2000 have an SMA 905
Connector for easy coupling to our
spectrometers and fiber optic accessories, as
well as safety goggles and a cover for
blocking the light when the fiber is not
attached. The 1,000-hour deuterium bulb
used in the D2000 can be replaced easily.
The D2000 is available with an optional
integrated shutter. You can operate the shutter
via a manual switch on the front of the lamp.
In addition, you can control the shutter
electronically via software or a TTL signal from
an output port on the back of the lamp.
D2000 Spectral Output
300
Optical Fibers
We recommend using our solarizationresistant optical fibers with all versions of the
D2000. See page 146 for details.
D2000: $2,003
POWER (µW/cm2/nm)
Light Sources
Shutter Option
200
100
0
200
300
400
WAVELENGTH (nm)
500
Additional D2000 Light Sources and Accessories
Item
Description
D2000-DUV
Uses a deep-UV deuterium bulb, which provides a 190-400 nm wavelength range
Price
$2,475
D2000-S
Comes with a shutter (controlled via a TTL signal or switch)
$2,580
D2000-S-DUV
Uses a deep-UV deuterium bulb, which provides a 190-400 nm wavelength range, and
$2,873
DH2000-BD
Replacement deuterium bulb for the D2000 and the D2000-S
$649
DH2000-DUV-B
Replacement deuterium bulb for the D2000-DUV and the D2000-S-DUV
$775
comes with a shutter (controlled via a TTL signal or switch)
Specifications
Dimensions:
Weight:
Wavelength range:
Power consumption:
Power requirements:
Stability:
Drift:
Time to stable output:
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126
150 mm x 135 mm x 319 mm
3.8 kg
215-400 nm (standard bulb); 190-400 nm (deep-UV bulb)
830 mA @ 230 VDC or 1660 mA @ 115 VDC
85-264 V 50/60 Hz
<0.005% at 250 nm peak-to-peak
±0.5% per hour at 250 nm
20 minutes
Voltage:
Bulb life:
Bulb aperture:
Operating temperature:
Humidity:
Electronic certifications:
TTL-shutter input:
Shutter speed:
Ignition 350V/20°; operating 85 V/0.3A
1,000 hours for standard or deep-UV bulb
Aperture 0.5 mm, numerical aperture 26°
5 °C - 35 °C
5-95% without condensation at 40 °C
CE; VDI/VDE 0160; EN 61010
Up to 5 Hz maximum (shutter versions only)
10 millisecond minimum
For all your sensing needs, visit OceanOptics.com
oo
Xenon Pulsed & Continuous Sources
Pulsed & Continuous Xenon Light Source
The PX-2 Pulsed Xenon Lamp is a high flash rate, short-arc xenon lamp from
220-750 nm. The PX-2 is a great source for applications requiring absorbance,
reflectance or fluorescence measurements, and is especially useful for
measuring optically or thermally labile samples. The PX-2 is a low-power lamp
with excellent pulse-to-pulse stability. It provides two trigger modes for software
control of the flash rate. It comes with a regulated power supply and an
interface cable to connect to the spectrometer.
PX-2:
$769
PX-2-B Bulb:
$379
USB-ADP-PX2:
$50
High-powered Continuous-wave Xenon Source
The HPX-2000 Xenon Light Source (185-2000 nm) is especially useful for
fluorescence applications, and for other applications where a high-intensity
lamp is necessary. The HPX-2000 has an integrated shutter, which can be driven
either by a switch or by a TTL signal. It also comes equipped with a slot for
filters up to 25-mm diameter or square, and up to 9-mm thick. (If operating the
HPX-2000 for ultraviolet applications, use the solarization-resistant fiber
described on page 146.)
HPX-2000 Spectral Output
Light Sources
The bulb is housed in an easy-to-remove bulb module. If your bulb needs to be
replaced, you have two options. You can send the module back to us to replace
the bulb (HPX-2000-B), or you can order another bulb module (HPX-2000-BM).
HPX-2000:
$6,006
HPX-2000-B:
$1,158
HPX-2000-BM: $2,692
PX-2 Spectral Output
1.0
POWER (µW/cm2/nm)
RELATIVE INTENSITY UNITS
150
0.8
0.6
0.4
0.2
0
300
400
500
600
700
800
900
1000
100
50
0
200
300
400
500
600
700
800
WAVELENGTH (nm)
WAVELENGTH (nm)
Specifications
Dimensions:
Weight:
Wavelength range:
Power consumption:
Output*:
HPX-2000
145 mm x 165 mm x 260 mm
4.3 kg
185-2000 nm
50 W AC; 50/60 Hz; 110
35 watts
Bulb life:
Connector:
Trigger input:
Pulse duration:
1,000 hours minimum; 2,000 hours typical
SMA 905
External TTL positive pulse via 15-pin connector (shutter)
Not applicable
PX-2
153.4 mm x 104.9 mm x 40.9 mm
370 g
220-750 nm
1 A @ 12 VDC
45 microjoules per pulse maximum; 9.9 watts average power;
220 Hz pulse rate maximum
109 pulses (estimated 230 days continuous operation at 50 Hz pulse rate)
SMA 905
External TTL positive pulse via 15-pin connector
5 microseconds (at 1/3 height of pulse)
* Power output is measured with an integrating sphere. Power out of a fiber depends on fiber size.
Tel: 727.733.2447 • Email: [email protected]
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LS-1 Tungsten Halogen Sources
360-2000 nm Spectral Range
The LS-1 Tungsten Halogen Light Source is a versatile
white-light source useful for absorbance, reflectance and
color measurements for the VIS-NIR (360-2000 nm).
The lamp offers high color temperature and efficient
output.
Long Life
The LS-1 comes with a 900-hour bulb. Also available is
the LS-1-LL, which comes with a 10,000-hour bulb for
extra-long life bulb performance. LS-1 Light Sources
come with a 12 VDC power supply (WT-12V).
Color-correcting & Signal-attenuating
Accessories
The LS-1 is one of the most popular miniature
spectroscopy light sources ever. As a result of customer
feedback, we’ve enhanced our LS-1 offering to include
components -- at no extra charge -- that allow users to
modify the light source output:
a 12.7-mm diameter color-correcting filter that can
be installed into the light source to enhance the
signal in the blue and NIR regions
three PTFE discs of various thickness to create a
diffuse source -- by attenuating the light 50%, 75%
or 99% -- when spectrometer saturation is an issue
Light Sources
LS-1 and LS-1-LL Spectral Output
LS-1 (900-hour bulb)
2500
LS-1-LL (10,000-hour bulb)
Maximum Flexibility
POWER (µW/cm2/nm)
2000
The LS-1 has an SMA 905 Connector for easy coupling
to our spectrometers and accessories, including optical
fibers, cuvette holders and probes. A built-in slot accepts
optical filters up to three millimeters in thickness.
1500
1000
Rack-mountable
500
Install sources with spectrometers and other devices into
a Rack Box or Desktop Box. For details, see page 62.
0
340
440
540
640
740
840
940
LS-1:
LS-1-LL:
WAVELENGTH (nm)
$499
$549
Additional LS-1-series Light Sources and Accessories
Item
Description
Price
R-LS-1
Rack-mounted LS-1 with color-correcting filter and diffusers
$499
R-LS-1-LL
Rack-mounted LS-1-LL with color-correcting filter and diffusers
$549
LS-1-B
900-hour replacement bulb for LS-1
LS-1-LL-B
10,000-hour replacement bulb for LS-1-LL
OF2-LS
Additional filter set for use with LS-1 source includes: BG 34, GG 395 and OG 550 filters, as well as PTFE
$45
$55
$100
diffusing discs
Specifications
Dimensions:
Weight:
Wavelength range:
Power consumption:
Output:
Current:
Time to stable output:
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113.5 mm x 50.8 mm x 31.6 mm
140 g
360-2000 nm
600 mA @ 12 VDC
6.5 watts (without a fiber)
5 V, 1.3 A
~10 minutes
Bulb type:
Bulb life:
Bulb color temperature:
Connector:
Internal filter accessory:
External filter slot:
Spectral attenuation:
Tungsten halogen
900 hours (LS-1); 10,000 hours (LS-1-LL)
3100 K (900-hour bulb); 2800 K (10,000-hour bulb)
SMA 905
BG 34 balancing filter
Accepts filters up to 3-mm thickness
50%, 75% and 99% with PTFE disc accessories
For all your sensing needs, visit OceanOptics.com
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HL-2000 Tungsten Halogen Sources
Great Versatility
The HL-2000 Tungsten Halogen Light Sources are
versatile sources optimized from 360-2000 nm. The
lamps feature adjustable focusing of the SMA 905
Connector to maximize light coupling into a fiber. A fan
keeps the light sources cool and stable. The HL-2000
comes with a 1,500-hour bulb. A 10,000-hour long-life
version is also available.
HL-2000 with
fiber (fiber not included).
Filter Slot
A built-in filter slot on all standard HL-2000s accepts
optical filters up to 25.4-mm round or up to 50.8-mm
square and three millimeters thick. The HL-2000-LVF-HP
version also accepts our LVF Linear Variable Filters (for
more on the LVFs, see page 114.)
HL-2000 Spectral Output
14000
High-power Version
For applications requiring large-diameter optical fibers
or fiber and probe bundles, a special high-power
version of the HL-2000 is available. The bulb used in
the HL-2000-HP is a 20-watt bulb. We recommend
1000 µm diameter optical fiber for use with the highpower versions of the HL-2000.
POWER (µW/cm2/nm)
12000
10000
8000
6000
4000
2000
0
300
400
500
600
700
800
900
1000
WAVELENGTH (nm)
The HL-2000-FHSA version of the HL-2000 includes a
shutter and an attenuator that allows you to control the
intensity of the light source from 0-100%. A locking
screw allows you to manually fix the intensity position for
the long term. In addition, you can opt to control the
attenuator and the TTL shutter via RS-232 with the
HL-2000-HP-232.
HL-2000:
$635
Additional HL-2000 Light Sources & Bulbs
Item
Description
HL-2000-LL
Long-life version (10,000-hour)
Price
HL-2000-FHSA
Includes filter holder, attenuator and
$688
$1,342
shutter
HL-2000-FHSA-LL
Includes filter holder, attenuator,
$1,389
Light Sources
Attenuator & Shutter Option
shutter and long-life 10,000-hour bulb
HL-2000-HP
High-powered, 20 W version
$1,089
HL-2000-HP-FHSA
High-powered, 20 W version with
$1,655
filter holder, attenuator and shutter
HL-2000-HP-232
High-powered, 20 W version with
$2,350
RS-232 control in rack mount housing;
comes with script for software control
HL-2000-LVF-HP
High-powered, 20 W version with filter
$1,719
slot for Linear Variable Filters; comes
with shutter and attenuator
HL-2000-HP-232 is being
used to measure adaptive
optics in observatories.
HL-2000-B
Standard 1,500-hour spare bulb
HL-2000-B-LL
Long-life 10,000-hour spare bulb
HL-2000-HP-B
High-power 1,000-hour spare bulb
$83
$96
$132
Specifications
Dimensions:
Weight:
Wavelength range:
Power consumption:
Output:
Stability:
Drift:
Time to stable output:
Bulb life:
Bulb color temperature:
Operating temperature:
Humidity:
HL-2000
62 mm x 60 mm x 150 mm
500 g
360-2000 nm
1.2 A @ 12 VDC
7 watts
0.5%
<0.3% per hour
~5 minutes
1,500 hours
2,960 K
5 °C - 35 °C
5-95% at 40 °C
HL-2000-LL
62 mm x 60 mm x 150 mm
500 g
360-2000 nm
1.0 A @ 12 VDC
7 watts
0.5%
<0.3% per hour
~5 minutes
10,000 hours
2,800 K
5 °C - 35 °C
5-95% at 40 °C
Tel: 727.733.2447 • Email: [email protected]
HL-2000-HP
62 mm x 60 mm x 150 mm
500 g
360-2000 nm
1.2 A @ 24 VDC
20 watts
0.5%
<0.3% per hour
~5 minutes
1,000 hours
3,000 K
5 °C - 35 °C
5-95% at 40 °C
HL-2000-HP-232
70 mm x 100 mm x 160 mm
600 g
360-2000 nm
1.2 A @ 24 VDC
20 watts
0.5%
<0.3% per hour
~5 minutes
1,000 hours
3,000 K
5 °C - 35 °C
5-95% at 40 °C
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Light Emitting Diodes
Excellent Excitation Sources for Fluorescence
Our LED Light Sources produce either pulsed or continuous
output for high-sensitivity fluorescence measurements. They
were designed for use with our fluorescence spectrometers,
such as the USB4000-FLG and USB4000-FL (pages 46-47),
sensors and other accessories.
Software Operation & Synching with Detector
The LED Sources can be turned on/off through manual or
software operation via SpectraSuite Spectroscopy Operating
Software (page 80).
Stand-alone and Rack-mount Versions
Light Sources
Choose your LED in a stand-alone housing
(above) or mounted with a spectrometer and
other accessories. We also sell the LEDs
listed below individually in a 12.7-mm barrel
(right) for easy installation and alignment.
Each LED Source connects to a spectrometer via an interface
cable. First, decide if you want an LED in its own standalone housing (see top left) or if you want the LED racked
with a spectrometer. Then, choose the LED distinguished by
wavelength to install in the housing. For those with limited
space, we can install two LEDs on one rack-mount card. You
can also purchase just the LED; they come in easy-to-install
barrels.
LED with Housing:
$499
LED Rack-mounted: $499
LED Bulb alone:
$100
Additional LED Light Sources
You can order one of the LEDs listed below, either alone or installed in a housing/rack mount.
We offer seven LEDs that can be used in the same housing. All LEDs can be used in pulsed or
continuous mode through manual or software operation.
Item
Description
Color
Power*
Price of
LED Alone
Price of LED
with Housing
LED-380
LED-395
380 nm wavelength UV LED
UV
45 µW
$100
$499
395 nm wavelength VIS LED
Light Blue
25 µW
$100
$499
LED-470
470 nm wavelength VIS LED
Blue
35 µW
$100
$499
LED-518
518 nm wavelength VIS LED
Green
35 µW
$100
$499
LED-590
590 nm wavelength VIS LED
Yellow
40 µW
$100
$499
LED-640
640 nm wavelength VIS LED
Red
50 µW
$100
$499
LED-WHITE
450-630 nm wavelength VIS LED
White
50 µW
$100
$499
LED-KIT
Set of 6 LEDs: LED-380, LED-395, LED-518,
Mixed
Mixed
$499
$998
LED-590, LED-640, LED-WHITE
* Power into a 600 µm Patch Cord Optical Fiber Assembly
Spectral Output for LED Bulbs:
380 nm, 470 nm, 518 nm and 640 nm
Spectral Output for LED Bulbs:
395 nm, White, 590 nm
380
395
80
470
300
White
590
640
POWER (µW/cm2/nm)
POWER (µW/cm2/nm)
518
200
100
60
40
20
0
350
400
450
500
550
WAVELENGTH (nm)
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600
650
0
350
400
450
500
550
600
650
WAVELENGTH (nm)
For all your sensing needs, visit OceanOptics.com
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Pulsed Blue LED Light Source
LS-475 nm Spectral Output
POWER (µW/cm2/nm)
300
200
100
0
350
400
450
500
550
WAVELENGTH (nm)
Lamp Available for
All Spectrometers
The LS-475 Blue LED
Light Source produces
pulsed or continuous
spectral output
centered at 475 nm.
The LS-475 is
designed as an
excitation source for
fluorescence measurements. The
LS-475 often is paired with one of our
preconfigured fluorescence spectrometers (pages 46-47).
High-stability & Fan-cooled
Specifications
Dimensions:
Wavelength range:
Power consumption:
Output:
Stability:
Connector:
62 mm x 60 mm x 150 mm
460-490 nm
25 mA @ 12 VDC
50 µW with a 600 µm optical fiber
± 1.0% drift after 2-minute warm-up
SMA 905
The LS-475 has a very stable output and keeps cool with a built-in fan. The
lamp provides better than ± 1.0% drift after a 2-minute warm-up time. It has
an SMA 905 Connector for coupling to optical fiber assemblies and a filter
slot that accepts 25.4-mm round or 50.8-mm square filters up to 3-mm
thick. An 800 mA, 12 VDC power supply comes with the unit.
LS-475: $774
Light Sources
Direct-attach LED Light Source
Direct-attach Lamp for USB4000 Spectrometer
The USB-LS-450 and USB-LS-395 Pulsed LED Light Sources are designed
as a direct-attach excitation source for USB2000 and USB4000
Spectrometers. The USB-LS-450 is an LED that produces either pulsed
or continuous output centered at 470 nm -- the blue region. The USBLS-395 is an LED that produces either pulsed or continuous output
centered at 395 nm. Each LED connects to the spectrometer via a
10-pin connector. The USB2000 and USB4000 provide power to the
LEDs and also enable synchronization functions. These sources are
primarily used in fluorescence measurements and in our oxygen
sensing systems. The 470 nm LED is great for exciting the FOXY and
HIOXY oxygen sensing formulations, while the 395 nm LED is used for
exciting the FOSPOR oxygen sensing formulation (pages 65-71).
Benefit for O2 Sensor Users
The sources features a built-in, 24-bit A/D converter that is configured for
a 100 ohm platinum temperature probe (The USB-LS-450-TP is seen at
right with a direct-attach LED and a spectrometer.) These excitation sources
have onboard memory that can be programmed to store temperature
and oxygen calibration coefficients. If neither the 450 nor 395 LED fits
your needs, you can purchase the USB-LS-LED and then specify one of
the other LEDs we offer on page 130.
USB-LS-450:
$549
USB-LS-395:
$549
USB-LS-LED:
$549
USB-LS-450-TP: $99
Specifications
Dimensions:
Weight:
Stability:
89 mm x 57 mm x 34.5 mm
120 g
± 1.0% drift after 2-minute
warm-up period
Wavelength range:
Power consumption:
Output:
460-490 nm
60 mA @ 5 VDC
60 µW (minimum) into a
600 µm optical fiber
Tel: 727.733.2447 • Email: [email protected]
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Radiometric Calibration Standards: UV-NIR
Calibrated from 220-1050 nm
The DH2000-CAL Deuterium Tungsten Halogen
Calibration Standard is a UV-NIR light source used to
calibrate the absolute spectral response of a
radiometric system. With the DH2000-CAL and our
SpectraSuite Spectroscopy Operating Software, you can
determine known absolute intensity values at
wavelengths from 220-1050 nm.
Calibrated for Bare Fiber & Cosine Corrector
The DH2000-CAL is calibrated for use with optical
fibers or a cosine corrector; the calibration data
includes absolute intensities for wavelengths between
220-1050 nm at the fiber entrance port for both a bare
fiber and an included CC-3-UV Cosine Corrector
(page 104).
NIST-traceable Calibration Certificate
The DH2000-CAL is calibrated with a NIST-traceable
standard. The DH2000-CAL comes with a calibration
certificate and a diskette with a data file compatible
with our software. The calibration data -- absolute
spectral intensity values in µW/cm2/nm measured at the
fiber port -- is provided for use with our SpectraSuite
software (not included, see pages 80-81).
Light Sources
The DH2000-CAL is
calibrated for use with either a
CC-3-UV Cosine Corrector or with an optical
fiber. The lamp comes with a CC-3-UV.
Recalibration of Your DH2000-CAL
DH2000-CAL Spectral Output
0.6
The DH2000-CAL typically provides 50 hours of
operation before recalibration is necessary. We
recalibrate these lamps in-house. (For more information
on the DH2000-RECAL service, contact an Applications
Scientist.)
DH2000-CAL:
$3,275
DH2000-RECAL:
$399
Deuterium
Tungsten Halogen
POWER (µW/cm2/nm)
0.5
0.4
0.3
In-house Calibration Service
0.3
0.1
0
200
300
400
500
600
700
800
900
WAVELENGTH (nm)
These spectral output graphs were taken separately for the deuterium
(200-400 nm) and the tungsten halogen bulbs (400-1100 nm).
1000
Also, you don’t need a DH2000-CAL to take advantage
of our in-house SPEC-CAL-UV radiometric calibration
service for UV spectrometers. The calibration is good
for about one year, provided the optical fiber is not
removed from the setup, as the system is calibrated for
use with a specific fiber.
SPEC-CAL-UV:
$499
Radiometric Calibration Sources are not illumination sources for
spectroscopic measurements. Use the DH2000-BAL (page 122) for
illumination.
Specifications
Dimensions:
Weight:
Wavelength range:
Power consumption:
Power requirements:
Output:
Voltage:
Current:
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132
150 mm x 135 mm x 319 mm
3.8 kg
220-1050 nm calibrated
25 W (deuterium); 20 W (tungsten halogen);
190 W maximum
85-264 V 50/60 Hz
100 watts
350 V
Operating 85 V/0.3A
Stability:
Drift:
Time to stable output:
Operating temperature:
Humidity:
Electronic certifications:
Connector:
Calibration accuracy:
Calibration valid for:
<5 x 10-6 peak-to-peak (0.1-10.0 Hz)
<0.01% per hour
20 minutes
5 °C - 35 °C
5-95% without condensation at 40 °C
CE; VDI/VDE 0160; EN 61010
SMA 905
± 5%
50 hours
For all your sensing needs, visit OceanOptics.com
Radiometric Calibration Standards: VIS-NIR
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Calibrated with Fiber & Cosine Corrector
The LS-1-CAL is designed for calibrating the absolute
spectral response of a complete system consisting of a
spectrometer and an optical fiber and/or a CC-3-UV
Cosine Corrector (page 104). The HL-2000-CAL is also
designed for calibrating a system consisting of a
spectrometer and a cosine corrector. The calibration
data for both the LS-1-CAL and the HL-2000-CAL
includes absolute intensities for wavelengths between
300-1050 nm.
LS-1-CAL:
$749
HL-2000-CAL:
$871
The LS-1-CAL is
calibrated for use with a fiber
and/or a CC-3-UV Cosine
Corrector (not included).
Calibrated for Use with Integrating Sphere
The LS-1-CAL-INT is calibrated
specifically for use with the
FOIS-1 Integrating Sphere.
Notice the PTFE diffuser plug
that’s seated where an SMA 905
Connector is usually installed.
This plug fits snugly into the sample
port of the FOIS-1.
What’s Included
Each of these radiometric sources comes with a regulated
12 VDC power supply. Also included is a calibration
certificate and electronic files for use with our irradiance
functions in SpectraSuite Spectroscopy Operating
Software. Neither the LS-1-CAL nor the HL-2000-CAL
lamps comes with a CC-3-UV Cosine Corrector.
Light Sources
The LS-1-CAL-INT is designed for calibrating the absolute
spectral response of a system that uses the FOIS-1 Fiber
Optic Integrating Sphere (page 105) as the sampling
optic. The LS-1-CAL-INT comes with a diffuser plug that
fits into the sample port of the FOIS-1 to measure
absolute spectral intensities of LEDs and other emission
sources. The HL-2000-CAL-ISP is designed for calibrating
the absolute spectral response of your system when using
the ISP-50-8-I Integrating Sphere (page 105) as your
sampling optic.
LS-1-CAL-INT:
$749
HL-2000-CAL-ISP:
$882
Recalibrating Your Source
These calibrated sources provide 50 hours of operation
before an in-house recalibration (called the LS-1-RECAL
and the HL-2000-RECAL) is necessary.
LS-1-RECAL:
$199
HL-2000-RECAL:
$199
The HL-2000-CAL is used for
calibrating most radiometric systems,
while the HL-2000-CAL-ISP is used with
ISP Integrating Spheres.
In-house Calibration
Specifications
Power consumption:
Wavelength range:
Output:
Recalibration:
Time to stable output:
Bulb color temperature:
Connector:
600 mA @ 12 VDC
300-1050 nm (calibrated)
6.5 watts
Required after 50 hours of operation
~20 minutes
3100 K for LS-1-CALs, 2800 K for HL-2000-CALs
SMA 905 for fiber; 6.35-mm barrel for cosine corrector;
PTFE plug for integrating sphere
Tel: 727.733.2447 • Email: [email protected]
LS-1-CAL Spectral Output
90
80
70
POWER (µW/cm2/nm)
If you do not want to purchase one of these calibration
sources, we offer in-house radiometric calibration services
that calibrate the absolute spectral response of your
system. The SPEC-CAL service is for 300-1050 nm and
the SPEC-CAL-NIR service is for 900-2400 nm.
SPEC-CAL:
$499
SPEC-CAL-NIR:
$499
60
50
40
30
20
10
0
300
400
500
600
700
800
900
1000
WAVELENGTH (nm)
Above is the typical calibration output when using the LS-1-CAL or
HL-2000-CAL with a CC-3 Cosine Corrector.
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Wavelength Calibration Standards: UV-VIS
Wavelength Calibration Sources
The HG-1 and CAL-2000 Mercury Argon
Calibration Sources are spectral wavelength
calibration sources for spectrometer systems. The
HG-1 and the CAL-2000 produce low-pressure
mercury and argon atomic emission lines from
253-1700 nm for use in performing fast,
reliable spectrometer wavelength calibrations. A
list of mercury and argon spectral emission lines
is printed on each lamp's housing.
Drift Occurs in all Spectrometers
Our spectrometers are carefully calibrated as
part of our standard quality assurance process.
However, as is the case with all optical benches,
slight drifts in wavelength occur due to time and
environmental conditions. If wavelength
accuracy is an important part of your
application, consider including calibration
spectra with every experiment.
The HG-1.
Light Sources
Convenient Operation
Wavelength calibration with the HG-1 or the
CAL-2000 requires a power supply (included)
and an optical fiber to connect from the source
to your spectrometer. You will need a
spreadsheet program such as Microsoft Excel or
a calculator that performs third-order
polynomial regressions.
The CAL-2000.
Convenient Portability
Both calibration sources operate with a 12 VDC
power supply (included) or a 9V battery (not
included) for field use. Both sources feature an
SMA 905 Connector for interfacing to optical
fiber assemblies and have bulbs with a 3,500hour lifetime. You can replace the bulb in the
CAL-2000, but not in the HG-1.
HG-1:
$399
CAL-2000:
$475
CAL-2000-B Bulb:
$191
HG-1 & CAL-2000 Spectral Output
ARBITRARY INTENSITY
4000
3000
2000
1000
0
200
300
400
500
600
700
800
900
For as low as $250 per spectrometer channel, you can
purchase the ASP Annual Service Package, which entitles
you to a yearly spectrometer inspection, wavelength
calibration, optical alignment, linearity calibration, signal-tonoise analysis and much more.
1000
WAVELENGTH (nm)
Mercury emission lines are <600 nm. Argon emission lines are >600 nm, and
are shown on an exaggerated amplitude scale.
Specifications
Dimensions:
Weight:
Wavelength range*:
Power consumption:
Power requirements:
Voltage:
Bulb life:
Time to stable output:
Connector:
HG-1
125.7 mm x 70 mm x 25.8 mm
40 g
253-1700 nm
250 mA @ 12 VDC
12 VDC wall transformer (included) or 9 VDC battery (not included)
600 volts at 30 kHz
~3,500 hours (at 20 mA)
1 minute
SMA 905
CAL-2000
130 mm x 125 mm x 50 mm
410 g
253-1700 nm
250 mA @ 12 VDC
12 VDC wall transformer (included) or 9 VDC battery (not included)
600 volts at 30 kHz
~3,500 hours (at 20 mA)
1 minute
SMA 905
* For performing wavelength calibrations for spectrometers in the VIS-NIR, consider using the AR-1 Argon Calibration Source on page 135.
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Wavelength Calibration Standard: NIR
Calibration Source for NIR Spectrometers
The AR-1 Argon Calibration Source is a spectral
wavelength calibration source specifically designed for
NIR spectrometers like our NIR256 and NIR-512 (see
pages 30-31). The AR-1 produces low-pressure argon
atomic emission lines from 696-1704 nm for use in
performing fast, reliable spectrometer wavelength
calibrations. The spectral emission lines are printed on
the lamp's housing.
Convenient Operation
Our spectrometers are carefully calibrated as part of
our standard quality assurance process. However, as is
the case with all optical benches, slight drift in
wavelength occurs due to time and environmental
conditions. With the AR-1, you can recalibrate your
spectrometer using a spreadsheet program such as
Microsoft Excel or a calculator that performs third-order
polynomial regressions.
AR-1 Spectral Output
Conveniently Portable
4000
Dimensions:
Weight:
Wavelength range:
Power consumption:
Power requirements:
Voltage:
Bulb life:
Time to stable output:
Connector:
125.7 mm x 70 mm x 25.8 mm
40 g
696-1704 nm
250 mA @ 12 VDC
12 VDC wall transformer (included)
or 9 VDC battery (not included)
600 volts at 30 kHz
~3,500 hours (at 20 mA)
~1 minute
SMA 905
3000
ARBITRARY INTENSITY
Specifications
3500
Light Sources
The AR-1 operates with a 12 VDC power supply
(included) or a 9V battery (not included) for field use.
The AR-1 features an SMA 905 Connector for
interfacing to optical fiber assemblies.
AR-1:
$399
2500
2000
1500
1000
500
0
1000
1100
1200
1300
1400
1500
1600
1700
WAVELENGTH (nm)
Cuvette Wavelength Calibration Adapter
The PS-HG1-ADP Wavelength Calibration
Adapter is a 1-cm square fixture that fits into a
1-cm pathlength sample chamber and then
connects to the HG-1 Mercury Argon
Calibration Standard or the AR-1 Argon
Wavelength Calibration Standard via optical
fiber. (Neither Wavelength Calibration
Standard nor optical fiber is included.) The
adapter is designed for performing a
wavelength calibration for a USB2000 or
USB4000 Spectrometer and a direct-attach
sampling system. However, the adapter can be
used with any post-dispersive spectrometer and
1-cm cuvette holder, whether it’s designed by
Ocean Optics or another manufacturer.
PS-HG1-ADP:
$259
Tel: 727.733.2447 • Email: [email protected]
135
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Bulbs, Power Supplies & Accessories
Power Supplies*
Item
Description
Plug Style
Current
WT-12V
12-volt power supply, 110/220
Americas/Japan
800 milliamps
Regulated
Yes
Price
$25
WT-12V-R
12-volt power supply, 110/220
Americas/Japan
2.5 Amps
Yes
$100
WT-12V-E
12-volt power supply, 110/220
European
800 milliamps
Yes
$20
WT-12V-R-E
12-volt power supply, 110/220
European
2.5 Amps
Yes
$100
WT-24V
24-volt power supply, 110/220
Americas/Japan
2.5 Amps
Yes
$50
WT-12V-E European Power Supply.
* Each Ocean Optics Sales, Service & Support location sells power supplies that best serves its region.
Bulbs for Ocean Optics Light Sources
Item
Description
DH2000-BD
Spare or replacement deuterium bulb for D2000, DH2000 and
Price
$650
DH2000-BAL sources
DH2000-DUV-B
Spare or replacement deep-UV deuterium bulb for D2000-DUV and
The DH2000-BD deuterium
bulb used in all D2000s and
DH2000s.
$776
DH2000-DUV sources
DH2000-BH
Spare or replacement tungsten halogen bulb for DH2000 and
$158
DH2000-BAL sources
DT-MINI-B
Spare bulb for DT-MINI and DT-MINI-GS (white or blue bulb housing)
$487
DT-MINI-2-B
Spare bulb for DT-MINI-2 and DT-MINI-2-GS (yellow bulb housing)
$526
HL-2000-B
Spare or replacement tungsten halogen bulb for the HL-2000
$83
The CAL-2000-B.
(1,500-hour, 2,960 K)
Light Sources
HL-2000-B-LL
Spare or replacement long-life tungsten halogen bulb for the HL-2000-LL
$96
(10,000-hour, 2,800 K)
HL-2000-HP-B
Spare or replacement tungsten halogen bulb for all HL-2000-HPs
HPX-2000-BM
Spare or replacement xenon bulb module for the HPX-2000
$2,692
$132
HPX-2000-B
Spare or replacement xenon bulb for the HPX-2000
$1,158
LED-380
Interchangeable, 380-nm LED for LS-450
$100
LED-395
Interchangeable, 395-nm LED for LS-450
$100
LED-518
Interchangeable, 518-nm LED for LS-450
$100
LED-590
Interchangeable, 590-nm LED for LS-450
$100
LED-640
Interchangeable, 640-nm LED for LS-450
$100
LED-WHITE
Interchangeable, white LED for LS-450
$100
LED-KIT
LED kit with 380-nm, 395-nm, 518-nm, 590-nm, 640-nm and white LEDs,
$499
The DH2000-BH
tungsten halogen
bulb used in all
DH2000s.
Bulb for the HL-2000.
for LS-450
LS-1-B
Spare or replacement tungsten halogen bulb for LS-1 (900-hour, 3100 K bulb)
$45
LS-1-LL-B
Spare or replacement long-life tungsten halogen bulb for LS-1 or LS-1-LL
$55
(10,000-hour, 2800 K bulb)
PX-2-B
Spare or replacement xenon bulb for the PX-2
$379
USB-ISS-UV-B
Spare or replacement deuterium and tungsten bulb for USB-ISS-UV-VIS
$399
USB-ISS-VIS-B
Spare or replacement tungsten bulb for the USB-ISS-VIS source
$199
D-1000-B
Spare or replacement deuterium bulb for the D-1000
$525
D-1000-REM-B
Spare or replacement bulb for D-1000-REM systems
$425
DT-1000-B
Spare or replacement deuterium bulb for the DT-1000
$595
DT-1000-BT
Spare or replacement tungsten halogen bulb for the DT-1000
$135
DT-1000-REM-B
Spare or replacement bulb for DT-1000-REM systems
$485
DT-1000-BT-CE
CE-certified tungsten halogen bulb for the DT-1000
$135
The DT-MINI
bulb unit.
The LS-1-B
replacement bulb
for the LS-1.
Other Light Source Accessories
Item
Description
CBL-PX-2
Cable for connecting PX-2 to S2000 Spectrometer
Price
$25
FCBARREL
6.35-mm outer diameter stainless steel barrel threaded for FC connectors
$29
that inserts into our 74-series Collimating Lenses
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FOT-SMA
SMA wrench for easily attaching Laboratory-grade optical fibers to
WRENCH
SMA 905 Connectors on Ocean Optics products
$10
Bulb module
for the HPX-2000.
For all your sensing needs, visit OceanOptics.com
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Fibers & Probes
Overview
139
Custom Fiber & Probe Options
142
Premium-grade Assemblies
143
Unjacketed Bulk Optical Fiber
144
Laboratory-grade Assemblies
146
Xtreme Solarization-resistant
Assemblies
147
Flame Loop Fiber Optic Probe
147
Cosine-corrected Irradiance Probe
148
Reflection/Backscattering Probes
150
Transmission Dip Probes
152
Industrial Process Probe
153
Vacuum Feedthroughs
154
Optical Fiber Kits
157
Fiber & Probe Fixtures & Holders
158
Fiber & Probe Accessories
Fibers & Probes
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Overview: Fibers & Probes
The Most Flexible Line in the Industry
Ocean Optics is the most versatile supplier of optical fibers and accessories for spectroscopy in the industry.
We offer everything from one-off patch cords and custom assemblies, to OEM builds for all sorts of
applications. Our fiber accessories, fixtures and fiber assembly kits allow you to easily connect or
manipulate fibers, and integrate them into tricky experiment set-ups. Optical fiber technology has been
paramount to our success and makes possible our “take the instrument to the sample” maxim. Fiber is the
nucleus of our analytical instrumentation and accessory design philosophy. And it’s optical fiber technology
that helped us create the world’s most flexible line of sensing instruments.
Anatomy of an Assembly
Fibers & Probes
At the fiber’s core is pure silica; it’s the diameter of the core that you need to consider when purchasing an
optical fiber assembly. (The core diameter is often in the product’s item code. For example, the P600-UV-VIS
has a 600 µm diameter silica core.) Surrounding the core is a doped-fluorine silica cladding. A buffer
material is then applied. A buffer coats the core and cladding , strengthens the fiber and reduces stray light
even further. In most assemblies polyimide is used as the buffer; other assemblies use aluminum or acrylate.
Then a jacketing is applied over the core, cladding and buffer to protect the fiber and provide strain relief.
For off-the-shelf Premium-grade “Q” Optical Fiber Assemblies, the standard jacketing is stainless steel
silicone monocoil. For off-the-shelf the Laboratory-grade Optical Fiber Assemblies, the standard jacketing is
zip tube blue PVDF. (There are several other jacketing options when creating a custom assembly.) Precision
SMA 905 Connectors terminate the assembly and are precisely aligned to the spectrometer’s slit to ensure
concentricity of the fiber. Finally, captive end caps protect the fiber tips against scratches and contaminants.
Assembly Identifiers
Our optical fiber and probe assemblies are clearly and cleanly labeled in
three ways so that you always know the following about your assembly: its
name, its core diameter, and its most efficient wavelength region.
The BOOT COLLAR color
corresponds to the assembly’s
fiber type (and its most
efficient wavelength range).
A WHITE PRODUCT LABEL
on an assembly includes the
product name and item code.
The BAND COLOR
signals the diameter of
the assembly’s core.
BOOT COLLARS
BAND COLORS
A color band tells you the diameter
fiber with which you are working.
8 µm
50 µm
Purple
Blue
100 µm
Green
200 µm
Yellow
300 µm
Gray
400 µm
Red
500 µm
Orange
600 µm
Brown
1000 µm
Clear
The assembly’s boot color lets you know the fiber type and the most
efficient wavelength range in which your fiber will work.
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Boot
Color
Fiber Type
Most Efficient
Wavelength Range
Gray
UV-VIS XSR Solarization-resistant
180-900 nm
Gray
UV/SR-VIS High OH content
200-1100 nm
Blue
UV-VIS High OH content
300-1100 nm
Red
VIS-NIR Low OH content
400-2500 nm
Premuim-grade Optical Fiber
Assembly for each Fiber Type
For all your sensing needs, visit OceanOptics.com
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Custom Fiber & Probe Assemblies
Custom Fiber & Probe Quoting Website
Continuous innovation is a critical ingredient for our growth. Our
parent company, Halma p.l.c., believes that innovation is not just the
responsibility of our development departments but is integral to all
commercial activities within the business. Halma’s successful
Innovation Initiative allows all employees to deliver innovative ideas
to help their companies achieve growth objectives. In 2006, Halma
awarded Ocean Optics employees for our Custom Fiber Assembly
Quoting and CAD Design website, designed to rapidly create
quotations and CAD drawings of custom optical fiber assemblies.
The website allows our application sales scientists and customer
service and support personnel to custom-create an optical fiber or
probe assembly that automatically generates quotes and drawings for
customers to view, modify and approve. Customers have hundreds of
options available to them when creating a custom assembly. Our
team of engineers uses our award-winning site to help guide you
through choosing the best options for your unique application.
Custom Option: Fiber Type
UV/SR-VIS Fibers: 200-1100 nm
2.0
2.0
1.8
1.8
1.6
1.6
ATTENUATION (dB/m)
ATTENUATION (dB/m)
XSR Solarization-resistant: 180-900 nm
1.4
1.2
1.0
0.8
0.6
1.4
1.2
1.0
0.8
0.6
0.4
0.4
0.2
0.2
0
180
255
330
405
480
555
630
705
780
855
0
200
930
300
400
500
WAVELENGTH (nm)
1.8
1.6
1.6
ATTENUATION (dB/m)
ATTENUATION (dB/m)
2.0
1.8
1.4
1.2
1.0
0.8
0.6
800
1100
1200
0.8
0.6
0.2
700
1000
1.0
0.4
600
900
1.2
0.2
500
800
1.4
0.4
400
700
VIS-NIR Low OH Fibers: 400-2500 nm
2.0
300
600
WAVELENGTH (nm)
UV-VIS High OH Fibers: 300-1100 nm
0
200
Fibers & Probes
One important consideration in building a custom assembly is which fiber type you should
specify for your application. Typically, the wavelength range needed for your application
should match the wavelength range of the fiber type. Here are the attenuation spectra for
each fiber type we offer.
900
1000
1100
1200
WAVELENGTH (nm)
Tel: 727.733.2447 • Email: [email protected]
0
300
500
700
900
1100
1300
1500
1700
1900
2100
2300 2500
WAVELENGTH (nm)
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Custom Fiber & Probe Assemblies
Custom Option: Optical Fiber Diameter Sizes
After selecting the best Fiber Type, you should consider the diameter size of the
pure silica core needed inside of your assembly. We offer several diameter sizes,
and can recommend the appropriate assembly based on these criteria:
1. How much light do you need for your application? Reflection and fluorescence
applications generally need more light, and larger diameter fibers are often
better choices than smaller diameter fibers. For a laser application, however,
we may suggest a smaller diameter fiber.
2. What is the entrance aperture size of your spectrometer? Make sure that your
fiber diameter size and the entrance aperture to your spectrometer are
compatible and are configured properly for your application needs.
3. If you have too much light in your setup, are there ways you can attenuate the
light? We believe that it’s better to have too much light than not enough.
Optical Fiber Diameter
Sizes Available for
Custom Assemblies
8 µm
50 µm
115 µm
200 µm
230 µm
300 µm
320 µm
400 µm
455 µm
500 µm
550 µm
600 µm
800 µm
1000 µm
Fibers & Probes
Custom Option: Jacketing Options
The fiber assembly jacketing is designed to protect the fiber and provide strain relief. But we have jacketing options
that can do so much more. We offer over 15 different jacketing options; our most popular selections are listed below.
With options from PEEK polymer jacketing (No. 3) designed for environments with temperatures up to 260 °C to
stainless-steel BX cable with neoprene synthetic rubber (No. 8) designed for excellent mechanical tolerance, we are
sure to have the right jacketing for your application environment. Each jacketing has a set of specifications so that
you and one of our Applications Scientists can choose the best option for your setup.
1
2
3
Item
4
5
6
Description
1
PVC Monocoil
OEM applications only
2
Zip Tube Blue PVDF
Best for budget-conscious applications;
3
PEEK
4
Zip Tube Blue PVDF
7
8
Temp.
Limits
Chemical
Resistance
9
10
Steam
Sterilizable
11
Mechanical
Tolerance
Length
Limits
70 °C
Poor
No
Good
6m
100 °C
Poor
No
Good
50 m
Good for hydrogen peroxide applications
260 °C
Excellent
Yes
Good
10 m
Best for budget-conscious applications;
100 °C
Poor
No
Good
50 m
standard in Laboratory-grade Assemblies
larger diameter than #2
5
PVC over Brass BX Tube
Glossy PVC covered over brass BX tube
100 °C
Good
No
Good
20 m
6
Silicone Monocoil
High-end jacketing; standard in Premium-
250 °C
Good
Yes
Good
20 m
250 °C
Good
Yes
Poor
4m
250 °C
Good
Yes
Excellent
40 m
grade Assemblies
7
Stainless-steel BX
OEM applications only; optional polyolefin
heatshrink overcoat
8
Stainless-steel
Excellent stainless steel jacketing
fully interlocked BX
supports longer lengths of fiber; optional
Brake cable
OEM applications only
120 °C
Good
No
Good
20 m
Neoprene synthetic rubber over stainless
120 °C
Good
No
Excellent
10 m
250 °C
Good
Yes
Poor
4m
polyolefin heatshrink overcoat
9
10 Stainless-steel BX
with heat shrink
11 Large-diameter
stainless-steel BX
steel; resists heat
OEM applications only; optional polyolefin
heatshrink overcoat
* Custom printing available for OEMs.
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For all your sensing needs, visit OceanOptics.com
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Custom Fiber & Probe Assemblies
Custom Option: Connectors & Connector Adapters
Our fiber assemblies are available with several connector options. For an upgrade fee that
includes the cost of the custom connector and labor, we will replace the standard SMA 905 CONN-QSMA
Connector (included in the assembly price) with any custom connector from the list below
(priced separately). When ordering custom connectors, please specify the diameter size of
CONN-SMA
the optical fiber to which it will be attached. You also can order connectors separately.
Item
Description
Connector
Price
CONN-ST
Stainless-steel ST Connector
CONN-FC
Stainless-steel FC Connector
$20
$18
CONN-QSMA
Premium-grade SMA 905 Connector (standard in Premium-grade assemblies)
$16
CONN-SMA
Laboratory-grade SMA 905 Connector (standard in Laboratory-grade assemblies)
$13
CONN-PSMA
Process-grade SMA 905 Connector used with an assembly with Tefzel jacketing
$23
CONN-QSMA-O
Premium-grade SMA 905 Connector with O-ring
$26
CONN-SMA-O
Laboratory-grade SMA 905 Connector with O-ring
$23
CONN-PSMA-O
Process-grade SMA 905 Connector with O-ring
$33
CONN-LSMA
Laser SMA 905 Connector for use during laser or other high-intensity applications
$30
Custom Option: Connector Adapters
Item
Description
SMA-ST-ADP
SMA-to-ST Adapter for interfacing an item with an SMA 905 Connector to
SMA-FC-ADP
SMA-to-FC Adapter for interfacing an item with an SMA 905 Connector to
SMA-ST-ADP
Price
$50
an item that has an ST Connector
$50
an item that has an FC Connector
SMA-FC-ADP
Custom Option: Ferrules for Probe Assemblies
Fibers & Probes
Connector adapters allow you to mate an item with an SMA 905 Connector to an item
with either an ST or FC Connector.
1
2
3
4
5
6
Description
1
1/4" diameter stainless-steel ferrule often used in solution transmission measurements
2
1/4" diameter PEEK ferrule used in harsh environments for solution transmission measurements
3
1/4" diameter stainless-steel ferrule used in reflection measurements
4
1/4" diameter Torlon ferrule with cap
5
1/4" diameter PEEK ferrule used in harsh environments
6
1/8" diameter stainless-steel ferrule
1/16" diameter stainless-steel ferrule
1/4" diameter stainless-steel ferrule with the tip angled to 30°
Fiber-to-lens ferrule that comes with a collimating lens
Custom Option: Epoxy
Item
Description
EPO-TEK 353ND
Standard epoxy in all fiber assemblies
220 °C
350 °C
Good
EPO-TEK 354ND
Slightly lower curing stress on the fiber than 353ND
200 °C
300 °C
Good
EPO-TEK OM125
Lowest curing stress on the fiber of the three epoxies
150 °C
250 °C
Fair
EPOXY-TEST
Free sample slide of all epoxies for compatibility testing
NA
NA
NA
Tel: 727.733.2447 • Email: [email protected]
Operating Temp.
Continuous
Operating Temp.
Intermittent
Chemical
Compatibility
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Premium-grade Assemblies
Premium-grade Patch Cord Assemblies
Our Premium-grade Optical Fiber Assemblies are durable, high-quality
assemblies that consistently deliver uniform results with minimal signal variance.
These assemblies are available in a wide variety of off-the-shelf configurations.
With every order, you receive a Quality Control Report that includes both the serial
number and transmission curve of the assembly. Our 2-meter Premium-grade
Patch Cord Assemblies are terminated with precision SMA 905 Connectors. They
connect easily to spectrometers, light sources and sampling accessories and are
available in standard lengths or can be ordered in custom lengths.
Fibers & Probes
Item Code
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Wavelength
Range
Core Diameter
Buffer /
Coating
Assembly
Length
Premium-grade Assemblies have a siliconecoated steel monocoil jacketing with a Nomex
braid for superior strain relief and protection.
Jacketing
LTBR*
STBR**
Price
QP8-2-SMA
400-2500 nm
8 µm ± 0.5 µm
acrylate
2 meters
silicone monocoil
4 cm
2 cm
$159
QP50-2-UV/BX
300-1100 nm
50 µm ± 5 µm
polyimide
2 meters
stainless-steel BX
4 cm
2 cm
$149
QP50-2-UV-VIS
300-1100 nm
50 µm ± 5 µm
polyimide
2 meters
silicone monocoil
4 cm
2 cm
$150
QP50-2-VIS-NIR
400-2500 nm
50 µm ± 5 µm
polyimide
2 meters
silicone monocoil
4 cm
2 cm
$150
QP100-2-UV/BX
300-1100 nm
100 µm ± 3 µm
polyimide
2 meters
stainless-steel BX
4 cm
2 cm
$149
QP100-2-UV-VIS
300-1100 nm
100 µm ± 3 µm
polyimide
2 meters
silicone monocoil
4 cm
2 cm
$150
QP100-2-VIS/BX
400-2500 nm
100 µm ± 3 µm
polyimide
2 meters
stainless-steel BX
4 cm
2 cm
$149
QP100-2-VIS-NIR
400-2500 nm
100 µm ± 3 µm
polyimide
2 meters
silicone monocoil
4 cm
2 cm
$150
QP200-2-SR/BX
200-1100 nm
200 µm ± 4 µm
polyimide
2 meters
stainless-steel BX
8 cm
2 cm
$179
QP200-2-UV/BX
300-1100 nm
200 µm ± 4 µm
polyimide
2 meters
stainless-steel BX
8 cm
4 cm
$149
QP200-2-UV-VIS
300-1100 nm
200 µm ± 4 µm
polyimide
2 meters
silicone monocoil
8 cm
4 cm
$150
QP200-2-VIS/BX
400-2500 nm
200 µm ± 4 µm
polyimide
2 meters
stainless-steel BX
8 cm
4 cm
$149
QP200-2-VIS-NIR
400-2500 nm
200 µm ± 4 µm
polyimide
2 meters
silicone monocoil
8 cm
4 cm
$150
QP230-0.25-XSR
180-900 nm
230 µm ± 10 µm
aluminum
25 centimeters
stainless-steel BX
4 cm
2 cm
$149
QP230-1-XSR
180-900 nm
230 µm ± 10 µm
aluminum
1 meter
stainless-steel BX
4 cm
2 cm
$179
QP230-2-XSR
180-900 nm
230 µm ± 10 µm
aluminum
2 meters
stainless-steel BX
4 cm
2 cm
$199
QP300-1-SR
200-1100 nm
300 µm ± 6 µm
polyimide
1 meter
silicone monocoil
12 cm
6 cm
$150
QP400-025-SR
200-1100 nm
400 µm ± 8 µm
polyimide
25 centimeters
silicone monocoil
16 cm
8 cm
$119
QP400-025-SR/BX
200-1100 nm
400 µm ± 8 µm
polyimide
25 centimeters
stainless-steel BX
16 cm
8 cm
$119
QP400-1-UV-VIS
300-1100 nm
400 µm ± 8 µm
polyimide
1 meter
silicone monocoil
16 cm
8 cm
$150
QP400-2-SR
200-1100 nm
400 µm ± 8 µm
polyimide
2 meters
silicone monocoil
16 cm
8 cm
$179
QP400-2-SR/BX
200-1100 nm
400 µm ± 8 µm
polyimide
2 meters
stainless-steel BX
16 cm
8 cm
$179
QP400-2-UV/BX
300-1100 nm
400 µm ± 8 µm
polyimide
2 meters
stainless-steel BX
16 cm
8 cm
$169
QP400-2-UV-VIS
300-1100 nm
400 µm ± 8 µm
polyimide
2 meters
silicone monocoil
16 cm
8 cm
$169
QP400-2-VIS/BX
400-2500 nm
400 µm ± 8 µm
polyimide
2 meters
stainless-steel BX
16 cm
8 cm
$169
QP400-2-VIS-NIR
400-2500 nm
400 µm ± 8 µm
polyimide
2 meters
silicone monocoil
16 cm
8 cm
$169
QP450-0.25-XSR
180-900 nm
455 µm ± 10 µm
aluminum
25 centimeters
stainless-steel BX
8 cm
4 cm
$159
QP450-1-XSR
180-900 nm
455 µm ± 10 µm
aluminum
1 meter
stainless-steel BX
8 cm
4 cm
$199
QP450-2-XSR
180-900 nm
455 µm ± 10 µm
aluminum
2 meters
stainless-steel BX
8 cm
4 cm
$239
QP600-025-SR
200-1100 nm
600 µm ± 10 µm
polyimide
25 centimeters
silicone monocoil
24 cm
12 cm
$129
QP600-025-SR/BX
200-1100 nm
600 µm ± 10 µm
polyimide
25 centimeters
stainless-steel BX
24 cm
12 cm
$119
QP600-025-UV
300-1100 nm
600 µm ± 10 µm
polyimide
25 centimeters
silicone monocoil
24 cm
12 cm
$119
QP600-025-VIS-N
400-2500 nm
600 µm ± 10 µm
polyimide
25 centimeters
silicone monocoil
24 cm
12 cm
$119
QP600-1-SR
200-1100 nm
600 µm ± 10 µm
polyimide
1 meter
silicone monocoil
24 cm
12 cm
$179
QP600-1-SR/BX
200-1100 nm
600 µm ± 10 µm
polyimide
1 meter
stainless-steel BX
24 cm
12 cm
$179
QP600-1-UV-VIS
300-1100 nm
600 µm ± 10 µm
polyimide
1 meter
silicone monocoil
24 cm
12 cm
$179
QP600-2-SR
200-1100 nm
600 µm ± 10 µm
polyimide
2 meters
silicone monocoil
24 cm
12 cm
$219
QP600-2-SR/BX
200-1100 nm
600 µm ± 10 µm
polyimide
2 meters
stainless-steel BX
24 cm
12 cm
$219
QP600-2-UV/BX
300-1100 nm
600 µm ± 10 µm
polyimide
2 meters
stainless-steel BX
24 cm
12 cm
$209
QP600-2-UV-VIS
300-1100 nm
600 µm ± 10 µm
polyimide
2 meters
silicone monocoil
24 cm
12 cm
$209
QP600-2-VIS/BX
400-2500 nm
600 µm ± 10 µm
polyimide
2 meters
stainless-steel BX
24 cm
12 cm
$209
QP600-2-VIS-NIR
400-2500 nm
600 µm ± 10 µm
polyimide
2 meters
silicone monocoil
24 cm
12 cm
$209
QP1000-2-UV/BX
300-1100 nm
1000 µm ± 20 µm
acrylate
2 meters
stainless-steel BX
30 cm
15 cm
$359
QP1000-2-UV-VIS
300-1100 nm
1000 µm ± 20 µm
acrylate
2 meters
silicone monocoil
30 cm
15 cm
$359
QP1000-2-VIS/BX
400-2500 nm
1000 µm ± 20 µm
acrylate
2 meters
stainless-steel BX
30 cm
15 cm
$359
QP1000-2-VIS-NI
400-2500 nm
1000 µm ± 20 µm
acrylate
2 meters
silicone monocoil
30 cm
15 cm
$359
* LTBR stands for Long Term Bend Radius, the bend radius allowed long term (such as for storage) before damaging the fiber.
** STBR stands for Short Term Bend Radius, the momentary bend radius allowed before damaging the fiber.
142
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Premium-grade Assemblies
Premium-grade Bifurcated Optical Fiber Assemblies
Our 2-meter Premium-grade Bifurcated Optical Fiber Assemblies are
Y-shaped assemblies with two fibers of the same diameter side-byside in the common end of the assembly. From the breakout of the
assembly, the two fibers diverge into two legs,
which can be UV-VIS, VIS-NIR or one of each -a “mixed” assembly. Premium-grade assemblies
feature premium SMA 905 Connectors (at right).
Item Code
Wavelength
Range
Core Diameter
Buffer /
Coating
Assembly
Length
Jacketing
LTBR*
STBR**
Price
QBIF50-UV-VIS
300-1100 nm
50 µm ± 5 µm
polyimide
2 meters
silicone monocoil
4 cm
2 cm
$299
QBIF200-UV-VIS
300-1100 nm
200 µm ± 4 µm
polyimide
2 meters
silicone monocoil
8 cm
4 cm
$299
QBIF200-VIS/BX
400-2500 nm
200 µm ± 4 µm
polyimide
2 meters
stainless-steel BX
8 cm
4 cm
$299
QBIF200-VIS-NIR
400-2500 nm
200 µm ± 4 µm
polyimide
2 meters
silicone monocoil
8 cm
4 cm
$299
QBIF400-UV-VIS
300-1100 nm
400 µm ± 8 µm
polyimide
2 meters
silicone monocoil
16 cm
8 cm
$329
QBIF400-VIS-NIR
400-2500 nm
400 µm ± 8 µm
polyimide
2 meters
silicone monocoil
16 cm
8 cm
$329
QBIF600-UV-VIS
300-1100 nm
600 µm ± 10 µm
polyimide
2 meters
silicone monocoil
24 cm
12 cm
$369
QBIF600-VIS/BX
400-2500 nm
600 µm ± 10 µm
polyimide
2 meters
stainless-steel BX
24 cm
12 cm
$369
QBIF600-VIS-NIR
400-2500 nm
600 µm ± 10 µm
polyimide
2 meters
silicone monocoil
24 cm
12 cm
$369
QBIF200-MIXED
300-1100 nm &
200 µm ± 4 µm
polyimide
2 meters
silicone monocoil
8 cm
4 cm
$299
400 µm ± 8 µm
polyimide
2 meters
silicone monocoil
16 cm
8 cm
$329
400-2500 nm
QBIF400-MIXED
300-1100 nm &
Fibers & Probes
400-2500 nm
Unjacketed Bulk Optical Fiber
We offer spooled, unjacketed optical fiber primarily for those interested in making their own assemblies.
We offer various core diameters from 50 µm to 600 µm. To improve the fiber’s strength and flexibility,
we triple-coat it with a polyimide buffer before spooling. We offer all types of unjacketed optical fiber:
High OH (high hydroxyl content for UV-VIS), Low OH (very low hydroxyl content for VIS-NIR) and
Solarization-resistant (for UV-VIS). Each fiber type is optimized for use in a particular wavelength range.
Item Code
Wavelength
Range
Core
Diameter
Buffer /
Coating
Fiber
Type
Length
LTBR*
STBR**
Price /
Meter
FIBER-50-UV
300-1100 nm
50 µm ± 5 µm
polyimide
UV-VIS
specify meter length
4 cm
2 cm
$15.78
FIBER-50-VIS
400-2500 nm
50 µm ± 5 µm
polyimide
VIS-NIR
specify meter length
4 cm
2 cm
$15.78
FIBER-100-UV
300-1100 nm
100 µm ± 3 µm
polyimide
UV-VIS
specify meter length
4 cm
2 cm
$15.78
FIBER-100-VIS
400-2500 nm
100 µm ± 3 µm
polyimide
VIS-NIR
specify meter length
4 cm
2 cm
$15.78
FIBER-200-SR
200-1100 nm
200 µm ± 4 µm
polyimide
UV/SR-VIS
specify meter length
4 cm
2 cm
$15.00
FIBER-200-UV
300-1100 nm
200 µm ± 4 µm
polyimide
UV-VIS
specify meter length
8 cm
4 cm
$12.63
FIBER-200-VIS
400-2500 nm
200 µm ± 4 µm
polyimide
VIS-NIR
specify meter length
8 cm
4 cm
$12.63
FIBER-300-SR
200-1100 nm
300 µm ± 6 µm
polyimide
UV/SR-VIS
specify meter length
12 cm
6 cm
$19.38
FIBER-300-UV
300-1100 nm
300 µm ± 6 µm
polyimide
UV-VIS
specify meter length
12 cm
6 cm
$18.75
FIBER-300-VIS
400-2500 nm
300 µm ± 6 µm
polyimide
VIS-NIR
specify meter length
12 cm
6 cm
$18.75
FIBER-400-SR
200-1100 nm
400 µm ± 8 µm
polyimide
UV/SR-VIS
specify meter length
16 cm
8 cm
$28.75
FIBER-400-UV
300-1100 nm
400 µm ± 8 µm
polyimide
UV-VIS
specify meter length
16 cm
8 cm
$23.38
FIBER-400-VIS
400-2500 nm
400 µm ± 8 µm
polyimide
VIS-NIR
specify meter length
16 cm
8 cm
$23.38
FIBER-500-SR
200-1100 nm
500 µm ± 10 µm
polyimide
UV/SR-VIS
specify meter length
20 cm
10 cm
$40.00
FIBER-500-UV
300-1100 nm
500 µm ± 10 µm
polyimide
UV-VIS
specify meter length
20 cm
10 cm
$31.25
FIBER-500-VIS
400-2500 nm
500 µm ± 10 µm
polyimide
VIS-NIR
specify meter length
20 cm
10 cm
$31.25
FIBER-600-SR
200-1100 nm
600 µm ± 10 µm
polyimide
UV/SR-VIS
specify meter length
24 cm
12 cm
$20.34
FIBER-600-UV
300-1100 nm
600 µm ± 10 µm
polyimide
UV-VIS
specify meter length
24 cm
12 cm
$36.88
FIBER-600-VIS
400-2500 nm
600 µm ± 10 µm
polyimide
VIS-NIR
specify meter length
24 cm
12 cm
$36.88
FIBER-1000-UV
300-1100 nm
1000 µm ± 20 µm
acrylate
UV-VIS
specify meter length
30 cm
15 cm
$96.25
FIBER-1000-VIS
400-2500 nm
1000 µm ± 20 µm
acrylate
VIS-NIR
specify meter length
30 cm
15 cm
$96.25
* LTBR stands for Long Term Bend Radius, the bend radius allowed long term (such as for storage) before damaging the fiber.
** STBR stands for Short Term Bend Radius, the momentary bend radius allowed before damaging the fiber.
Tel: 727.733.2447 • Email: [email protected]
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Laboratory-grade Assemblies
Laboratory-grade Patch Cord Optical Fiber Assemblies
Our Laboratory-grade Optical Fiber Assemblies offer high quality at an affordable price. These
off-the-shelf assemblies come in various lengths and wavelength ranges, and in bifurcated
and splitter designs. Our standard Laboratory-grade Assemblies act as both illumination
and read fibers and connect easily to our spectrometers, light sources and accessories.
Solarization-resistant Assemblies (these have -SR in the item code) are for applications
below 300 nm. UV radiation below 300 nm degrades transmission in standard silica
fibers, resulting in solarization (increased light absorption in the UV fiber that can
invalidate data). For applications below 200 nm, we recommend our Premiumgrade Xtreme Solarization-resistant Fiber and Probe Assemblies (see page 146).
Fibers & Probes
Item Code
Wavelength
Range
Core Diameter
Buffer /
Coating
Assembly
Length
LTBR*
STBR**
Price
P8-2-SMA
400-2500 nm
8 µm ± 0.5 µm
acrylate
2 meters
4 cm
2 cm
$99
P50-2-UV-VIS
300-1100 nm
50 µm ± 5 µm
polyimide
2 meters
4 cm
2 cm
$99
P50-2-VIS-NIR
400-2500 nm
50 µm ± 5 µm
polyimide
2 meters
4 cm
2 cm
$99
P100-2-UV-VIS
300-1100 nm
100 µm ± 3 µm
polyimide
2 meters
4 cm
2 cm
$99
P100-2-VIS-NIR
400-2500 nm
100 µm ± 3 µm
polyimide
2 meters
4 cm
2 cm
$99
P100-5-UV-VIS
300-1100 nm
100 µm ± 3 µm
polyimide
5 meters
4 cm
2 cm
$149
P100-5-VIS-NIR
400-2500 nm
100 µm ± 3 µm
polyimide
5 meters
4 cm
2 cm
$149
P100-10-UV-VIS
300-1100 nm
100 µm ± 3 µm
polyimide
10 meters
4 cm
2 cm
$199
P100-10-VIS-NIR
400-2500 nm
100 µm ± 3 µm
polyimide
10 meters
4 cm
2 cm
$199
P200-2-UV-VIS
300-1100 nm
200 µm ± 4 µm
polyimide
2 meters
8 cm
4 cm
$99
P200-2-VIS-NIR
400-2500 nm
200 µm ± 4 µm
polyimide
2 meters
8 cm
4 cm
$99
P200-5-UV-VIS
300-1100 nm
200 µm ± 4 µm
polyimide
5 meters
8 cm
4 cm
$149
P200-5-VIS-NIR
400-2500 nm
200 µm ± 4 µm
polyimide
5 meters
8 cm
4 cm
$149
P200-10-UV-VIS
300-1100 nm
200 µm ± 4 µm
polyimide
10 meters
8 cm
4 cm
$199
P200-10-VIS-NIR
400-2500 nm
200 µm ± 4 µm
polyimide
10 meters
8 cm
4 cm
$199
P300-1-SR
200-1100 nm
300 µm ± 6 µm
polyimide
1 meter
12 cm
6 cm
$99
P400-025-SR
200-1100 nm
400 µm ± 8 µm
polyimide
25 centimeters
16 cm
8 cm
$99
P400-1-SR
200-1100 nm
400 µm ± 8 µm
polyimide
1 meter
16 cm
8 cm
$119
P400-1-UV-VIS
300-1100 nm
400 µm ± 8 µm
polyimide
1 meter
16 cm
8 cm
$109
P400-2-SR
200-1100 nm
400 µm ± 8 µm
polyimide
2 meters
16 cm
8 cm
$129
P400-2-UV-VIS
300-1100 nm
400 µm ± 8 µm
polyimide
2 meters
16 cm
8 cm
$119
P400-2-VIS-NIR
400-2500 nm
400 µm ± 8 µm
polyimide
2 meters
16 cm
8 cm
$119
P400-5-UV-VIS
300-1100 nm
400 µm ± 8 µm
polyimide
5 meters
16 cm
8 cm
$179
P400-5-VIS-NIR
400-2500 nm
400 µm ± 8 µm
polyimide
5 meters
16 cm
8 cm
$179
P400-10-UV-VIS
300-1100 nm
400 µm ± 8 µm
polyimide
10 meters
16 cm
8 cm
$279
P400-10-VIS-NIR
400-2500 nm
400 µm ± 8 µm
polyimide
10 meters
16 cm
8 cm
$279
P600-025-SR
200-1100 nm
600 µm ± 10 µm
polyimide
25 centimeters
24 cm
12 cm
$109
P600-025-VIS-NIR
400-2500 nm
600 µm ± 10 µm
polyimide
25 centimeters
24 cm
12 cm
$99
P600-1-SR
200-1100 nm
600 µm ± 10 µm
polyimide
1 meter
24 cm
12 cm
$119
P600-2-SR
200-1100 nm
600 µm ± 10 µm
polyimide
2 meters
24 cm
12 cm
$169
P600-2-UV-VIS
300-1100 nm
600 µm ± 10 µm
polyimide
2 meters
24 cm
12 cm
$159
P600-2-VIS-NIR
400-2500 nm
600 µm ± 10 µm
polyimide
2 meters
24 cm
12 cm
$159
P600-5-UV-VIS
300-1100 nm
600 µm ± 10 µm
polyimide
5 meters
24 cm
12 cm
$249
P600-5-VIS-NIR
400-2500 nm
600 µm ± 10 µm
polyimide
5 meters
24 cm
12 cm
$249
P600-10-UV-VIS
300-1100 nm
600 µm ± 10 µm
polyimide
10 meters
24 cm
12 cm
$349
P600-10-VIS-NIR
400-2500 nm
600 µm ± 10 µm
polyimide
10 meters
24 cm
12 cm
$349
P1000-2-UV-VIS
300-1100 nm
1000 µm ± 20 µm
acrylate
2 meters
30 cm
15 cm
$299
P1000-2-VIS-NIR
400-2500 nm
1000 µm ± 20 µm
acrylate
2 meters
30 cm
15 cm
$299
* LTBR stands for Long Term Bend Radius, the bend radius allowed long term (such as for storage) before damaging the fiber.
** STBR stands for Short Term Bend Radius, the momentary bend radius allowed before damaging the fiber.
Specifications
Type:
Fiber profile:
Fiber core:
Fiber cladding:
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144
Laboratory-grade Patch Cord Optical Fiber Assemblies
Step-index multimode (all diameter assemblies except for (8 µm) and
Step-index single mode (8 µm diameter assemblies)
Pure silica core
Fluorine-doped silica cladding
Connector(s):
Assembly jacketing
Temperature range:
Numerical aperture:
Laboratory-grade SMA 905 Connectors
zip tube blue PVDF
-20 °C to 80 °C
Multimode: 0.22 ± 0.02 (yields acceptance angle of 24.8° in air);
Single mode: 0.14 ± 0.02 (yields acceptance angle of 14.94° in air)
For all your sensing needs, visit OceanOptics.com
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Laboratory-grade Assemblies
Laboratory-grade Bifurcated and Splitter Optical Fiber Assemblies
These 2-meter Bifurcated Optical Fiber Assemblies (right,
top) are Y-shaped assemblies that have two fibers of the
same diameter side-by-side in the common end, or the
tail of the assembly. From the nexus or breakout of the
assembly, the two fibers diverge into two separate legs.
You may specify that both fibers in the assembly are
UV-VIS, VIS-NIR or one of each -- a “mixed” bifurcated
assembly.
A splitter (right, bottom) is a 2-meter, Y-shaped assembly
with a stainless steel breakout located midway from the
ends of the assembly. Each splitter is made up of three
separate optical fibers, all of the same diameter, and
epoxied at the nexus of the Y-shaped assembly. A splitter
can route light from two different sources to illuminate
one sample or from one source to illuminate two
samples. Splitters have lower transmission efficiency than
other fiber assemblies due to their design.
Item Code
Wavelength
Range
Core Diameter
Buffer /
Coating
Assembly
Length
LTBR*
STBR**
Price
BIF50-UV-VIS
300-1100 nm
50 µm ± 5 µm
polyimide
2 meters
4 cm
2 cm
BIF50-VIS-NIR
400-2500 nm
50 µm ± 5 µm
polyimide
2 meters
4 cm
2 cm
$249
$249
BIF200-UV-VIS
300-1100 nm
200 µm ± 4 µm
polyimide
2 meters
8 cm
4 cm
$249
BIF200-VIS-NIR
400-2500 nm
200 µm ± 4 µm
polyimide
2 meters
8 cm
4 cm
$249
BIF400-UV-VIS
300-1100 nm
400 µm ± 8 µm
polyimide
2 meters
16 cm
8 cm
$279
BIF400-VIS-NIR
400-2500 nm
400 µm ± 8 µm
polyimide
2 meters
16 cm
8 cm
$279
BIF400-MIXED
300-1100 nm &
400 µm ± 8 µm
polyimide
2 meters
16 cm
8 cm
$279
400-2500 nm
BIF600-UV-VIS
300-1100 nm
600 µm ± 10 µm
polyimide
2 meters
24 cm
12 cm
$329
BIF600-VIS-NIR
400-2500 nm
600 µm ± 10 µm
polyimide
2 meters
24 cm
12 cm
$329
$499
Splitter Optical Fiber Assemblies
SPLIT200-UV-VIS
300-1100 nm
200 µm ± 4 µm
polyimide
2 meters
8 cm
4 cm
SPLIT200-VIS-NIR
400-2500 nm
200 µm ± 4 µm
polyimide
2 meters
8 cm
4 cm
$499
SPLIT400-UV-VIS
300-1100 nm
400 µm ± 8 µm
polyimide
2 meters
16 cm
8 cm
$499
SPLIT400-VIS-NIR
400-2500 nm
400 µm ± 8 µm
polyimide
2 meters
16 cm
8 cm
$499
Fibers & Probes
Bifurcated Optical Fiber Assemblies
Keyed SMA Optical Fiber Assemblies, Round to Keyed Linear
PL100-2-UV-VIS
300-1100 nm
100 µm ± 3 µm
polyimide
2 meters
4 cm
2 cm
$299
PL100-2-VIS-NIR
400-2500 nm
100 µm ± 3 µm
polyimide
2 meters
4 cm
2 cm
$299
PL100-2-MIXED
300-1100 nm &
100 µm ± 3 µm
polyimide
2 meters
4 cm
2 cm
$299
200 µm ± 4 µm
polyimide
2 meters
8 cm
4 cm
$299
400-2500 nm
PL200-2-MIXED
300-1100 nm &
400-2500 nm
* LTBR stands for Long Term Bend Radius, the bend radius allowed long term (such as for storage) before damaging the fiber.
** STBR stands for Short Term Bend Radius, the momentary bend radius allowed before damaging the fiber.
Specifications
Type:
Fiber profile:
Fiber core:
Fiber cladding:
Connector(s):
Assembly jacketing:
Breakout:
Operating temp. range:
Numerical aperture:
Laboratory Grade Bifurcated, Splitter and Keyed
Optical Fiber Assemblies
Step-index multimode
Pure silica core
Fluorine-doped silica cladding
Laboratory-grade SMA 905 Connectors
zip tube blue PVDF
Midway of assembly at 1 meter
-20 °C to 80 °C
0.22 ± 0.02 (yields acceptance angle of 24.8° in air)
Tel: 727.733.2447 • Email: [email protected]
145
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Xtreme Solarization-resistant Assemblies
High Transparency and Durability
Xtreme Solarization-resistant Optical Fiber and Probe Assemblies
for spectroscopy are manufactured using a proprietary process
that provides enhanced UV transmission -- signal will transmit to
180 nm -- and remarkable resistance to UV degradation,
making it ideal for deep-UV applications (<300 nm). Ocean
Optics is the only spectroscopy manufacturer to offer XSR Fiber.
Solarization in Typical Fibers
UV radiation below 300 nm degrades transmission in standard
silica fibers, resulting in solarization (increased light absorption
in the UV fiber that can invalidate data). For applications below
300 nm, we recommend Premium-grade XSR Xtreme Solarizationresistant Fiber and Probe Assemblies, which are available for
immediate delivery in standard lengths. Shorter lengths for
solarization-resistant assemblies maximize UV throughput.
Custom lengths are available; however, we recommend
speaking with our Applications Scientists before ordering.
QR450-7-XSR Premium-grade
XSR Xtreme Solarization-resistant
Reflection Probe Assembly
Fibers & Probes
High Production Values
Our XSR products are part of our high-quality Premium-grade
line of optical fibers and probes. XSR Fiber and Probe
Assemblies are robust and durable; each assembly has an
aluminum coating, a stainless-steel BX jacketing, and our highquality SMA 905 Connectors with captive end cap that protects
fiber tips against scratches and contaminants. And like all of our
optical fibers, the XSR assemblies are precisely polished to work
with our miniature fiber optic spectrometers and accessories.
QP230-2-XSR Premium-grade
XSR Xtreme Solarization-resistant
Patch Cord Optical Fiber Assembly
Absorbance Spectra of Various Fiber Types
after 72 Hours of UV Exposure
2.2
2.0
1.8
235 µm XSR Fiber
200 µm UV/SR
Absorbance Units
1.6
200 µm UV-VIS Fiber
Specifications
1.4
Type:
1.2
1.0
Wavelength range:
Fiber profile:
Fiber core:
Fiber cladding:
Fiber buffer/coating:
Operating temp. range:
Numerical aperture:
Connector(s):
Assembly jacketing
0.8
0.6
0.4
0.2
0
180
205
230
255
280
305
330
355
380
405
WAVELENGTH (nm)
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QP450-2-XSR
Premium-grade XSR
Xtreme Solarizationresistant Patch Cord
Optical Fiber Assembly
Premium Grade Xtreme XSR Solarization-resistant
Optical Fiber Assemblies and
Reflection/Backscattering Probes
180-900 nm
Step-index multimode
Pure silica core
Fluorine-doped silica cladding
Aluminum
-50 °C to 250 °C
0.22 ± 0.02 (yields acceptance angle of 24.8° in air)
Premium-grade SMA 905 Connectors
Stainless-steel BX
Item Code
Product Type
Assembly Length
Core Diameter
LTBR*
STBR**
QP230-0.25-XSR
Optical Fiber Assembly
25 centimeters
230 µm
4 cm
2 cm
Price
QP230-1-XSR
Optical Fiber Assembly
1 meter
230 µm
4 cm
2 cm
$179
QP230-2-XSR
Optical Fiber Assembly
2 meters
230 µm
4 cm
2 cm
$199
QP450-0.25-XSR
Optical Fiber Assembly
25 centimeters
450 µm
8 cm
4 cm
$159
QP450-1-XSR
Optical Fiber Assembly
1 meter
450 µm
8 cm
4 cm
$199
QP450-2-XSR
Optical Fiber Assembly
2 meters
450 µm
8 cm
4 cm
$239
$149
QR230-7-XSR/BX
Reflection/backscattering Probe
2 meters
230 µm
4 cm
2 cm
$599
QR450-7-XSR
Reflection/backscattering Probe
2 meters
450 µm
8 cm
4 cm
$999
* LTBR stands for Long Term Bend Radius, the bend radius allowed long term (such as for storage) before damaging the fiber.
** STBR stands for Short Term Bend Radius, the momentary bend radius allowed before damaging the fiber.
146
For all your sensing needs, visit OceanOptics.com
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Flame Loop Fiber Optic Probe
Heat-resistant Fiber Optic Probe
The FL-400 Flame Loop Fiber Optic Probe couples to our spectrometers to measure in situ emission spectra of
samples such as dissolved metals and high-temperature plasmas. The FL-400 consists of a high-temperature
400 µm gold-jacketed UV-VIS optical fiber in an 8-inch-long nickel sleeve. The assembly operates in
temperatures up to 700 °C. The probe connects to the 21-02 Splice Bushing and a P400-2-UV-VIS Optical
Fiber, which couples to a spectrometer to measure emission spectra. (Components are sold separately.)
Use as a Flame Loop Probe or Use as a Heat-resistant Fiber Probe
The FL-400 is especially beneficial as an emission spectroscopy teaching tool to observe atomic emission lines
of dissolved metals. You simply dip the loop in your sample material and pass the loop over an open flame to
take emission measurements. To use the FL-400 as a heat-resistant emission probe, remove the flame loop
and insert the FL-400 into a high-temperature environment to monitor emission.
FL-400:
$499
P400-2-UV-VIS: $119
21-02:
$13
Probe Assembly Specifications
400 µm core diameter
Fused silica core and doped, fused silica cladding
Gold
1 single-strand, multimode fiber
300-1100 nm
Nickel
17.78 cm length, 20-gauge probes with 0.902 mm OD
-269 °C to 700 °C
0.22
SMA 905
Fibers & Probes
Fiber diameter:
Fiber core/cladding:
Fiber jacketing:
Fiber type:
Wavelengths covered:
Probe sleeve (ferrule):
Probe dimensions:
Temperature range:
Numerical aperture:
Connector:
Cosine-corrected Irradiance Probe
CC-3-UV Angular Response
3500
Spectralon
See pages 142 and 144 for selecting
a fiber to couple to a cosine corrector
to create an irradiance probe.
Lambert’s Cosine Law
3000
COUNTS
2500
2000
1500
1000
500
0
CC-3 and CC-3-UV Cosine Correctors collect radiation from a
180° solid angle. When screwed onto the end of an optical fiber,
the cosine corrector and optical fiber become an irradiance probe,
measuring the intensity of light normal to the probe surface defined
by the diffusing material. The probe then couples to one of our
spectrometers to make a complete spectroradiometer for relative
and absolute spectral intensity measurements, such as measuring
UV-A and UV-B in natural solar environments, evaluating emissive
color sources and analyzing light sources such as LEDs and lasers.
The CC-3 has an opaline glass diffuser for VIS-NIR; the CC-3-UV
utilizes Spectralon for UV-NIR. Each disc sits flush at the end of
6.35-mm outer diameter barrel, which is threaded on one side for
SMA 905 Connectors.
CC-3:
$99
CC-3-UV: $129
Tel: 727.733.2447 • Email: [email protected]
0
10
20
30
40
50
60
70
80
90
100
ANGLE
The response of the Spectralon (red trace) used in the
CC-3-UV nearly matches that of Lambert’s Cosine Law.
Specifications
Diffusing material:
Wavelength range:
Disc thickness:
Dimensions:
Field of view:
Connector:
CC-3
Opaline glass
350-1000 nm
7.9 mm
6.35 mm OD
180°
SMA 905
CC-3-UV
Spectralon
200-1100 nm
7.9 mm
6.35 mm OD
180°
SMA 905
147
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Reflection/Backscattering Probes
Our R-series Fiber Optic Reflection Probes are used for measuring
specular or diffuse reflectance from a surface, fluorescence from
solid surfaces, or backscattering and fluorescence in solutions and
powders. These probes come in all four fiber types (XSR, UV/SR,
UV-VIS and VIS-NIR), or a combination of fiber types. (See page
139 for more on each fiber type.)
Standard Reflection/Backscattering Probes
Our standard reflection probes use a 6-around-1 closepacking design to ensure parallel orientation of the fibers.
Stainless Steel Ferrule
Our Standard Reflection/Backscattering Probes are based on a
natural close-packing arrangement of optical fibers. Typically,
the arrangement is a tight bundle of seven optical fibers -- six
illumination fibers around one read fiber. This arrangement
ensures parallel orientation of the fibers. The center or read fiber
splits from the other six fibers and couples to a spectrometer.
The outer six illumination fibers connect to the light source.
Fibers & Probes
PEEK Probe Ferrule
The RP200-7-UV-VIS consists of a bundle of 200-µm
fibers in a six-around-one design, but has a PEEK
ferrule for applications where samples may be
corrosive to the standard stainless-steel
ferrule.
Reflection/Backscattering
Probes with Reference Leg
The R200-REF consists of an R200-7 and an
additional fiber to monitor the illumination (or
reference) source, which is useful for any experiment
in which variation or instability in the spectral output
of the light source needs to be monitored.
Reflection/Backscattering Probes for
Expanded Wavelength Coverage
The R200-MIXED has 14 fibers -- six UV-VIS and six VIS-NIR
illumination fibers, plus one UV-VIS and one VIS-NIR read
fiber (see bundle photo at right). It couples easily to a dualchannel spectrometer in which each channel is set for a
different wavelength range.
Angled Probes for Solutions & Powders
Our angled probes also have a six-around-one design, but employ a 30°
window to remove specular reflection effects when the probe is immersed
in dense solutions and powders. We offer the angled probe with two
different diameter fibers, 200 µm and 400 µm. These backscattering
probes are especially useful for fluorescence measurements.
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For all your sensing needs, visit OceanOptics.com
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Reflection/Backscattering Probes
Item Code
Wavelength
Range
Core Diameter
Fiber Bundle
Fiber Jacketing
Probe
Ferrule
LTBR* STBR** Price
Standard Reflection/Backscattering Probes
QR200-7-UV-VIS
300-1100 nm
200 µm ± 4 µm
6 illumination fibers around 1 read silicone monocoil
6.35 mm OD 8 cm
4 cm
$399
QR200-7-VIS-NIR
400-2500 nm
200 µm ± 4 µm
6 illumination fibers around 1 read silicone monocoil
6.35 mm OD 8 cm
4 cm
$399
QR230-7-XSR/BX
180-900 nm
230 µm
6 illumination fibers around 1 read, stainless-steel BX
6.35 mm OD
$599
with aluminum coating
QR400-7-SR
200-1100 nm
400 µm ± 8 µm
6 illumination fibers around 1 read silicone monocoil
6.35 mm OD 16 cm
8 cm
$699
QR400-7-SR/BX
200-1100 nm
400 µm ± 8 µm
6 illumination fibers around 1 read stainless-steel BX
6.35 mm OD 16 cm
8 cm
$549
QR400-7-UV/BX
300-1100 nm
400 µm ± 8 µm
6 illumination fibers around 1 read stainless-steel BX
6.35 mm OD 16 cm
8 cm
$549
QR400-7-UV-VIS
300-1100 nm
400 µm ± 8 µm
6 illumination fibers around 1 read silicone monocoil
6.35 mm OD 16 cm
8 cm
$650
QR400-7-VIS/BX
400-2500 nm
400 µm ± 8 µm
6 illumination fibers around 1 read stainless-steel BX
6.35 mm OD 16 cm
8 cm
$549
QR400-7-VIS-NIR
400-2500 nm
400 µm ± 8 µm
6 illumination fibers around 1 read silicone monocoil
6.35 mm OD 16 cm
8 cm
$649
QR450-7-XSR
180-900 nm
450 µm
6 illumination fibers around 1 read, stainless-steel BX
6.35 mm OD
$999
with aluminum coating
200-1100 nm
600 µm ± 10 µm
6 illumination fibers around 1 read silicone monocoil
3.18 mm OD 24 cm
12 cm
$899
QR600-7-UV-125F
300-1100 nm
600 µm ± 10 µm
6 illumination fibers around 1 read silicone monocoil
3.18 mm OD 24 cm
12 cm
$849
QR600-7-VIS-125
400-2500 nm
600 µm ± 10 µm
6 illumination fibers around 1 read silicone monocoil
3.18 mm OD 24 cm
12 cm
$849
R200-7-UV-VIS
300-1100 nm
200 µm ± 4 µm
6 illumination fibers around 1 read zip tube blue PVDF 6.35 mm OD 8 cm
4 cm
$399
R200-7-VIS-NIR
400-2500 nm
200 µm ± 4 µm
6 illumination fibers around 1 read zip tube blue PVDF 6.35 mm OD 8 cm
4 cm
$399
R400-7-SR
200-1100 nm
400 µm ± 8 µm
6 illumination fibers around 1 read zip tube blue PVDF 6.35 mm OD 16 cm
8 cm
$549
R400-7-UV-VIS
300-1100 nm
400 µm ± 8 µm
6 illumination fibers around 1 read zip tube blue PVDF 6.35 mm OD 16 cm
8 cm
$499
R400-7-VIS-NIR
400-2500 nm
400 µm ± 8 µm
6 illumination fibers around 1 read zip tube blue PVDF 6.35 mm OD 16 cm
8 cm
$499
R600-7-SR-125F
200-1100 nm
600 µm ± 10 µm
6 illumination fibers around 1 read zip tube blue PVDF 3.18 mm OD 24 cm
12 cm
$699
R600-7-UV-125F
300-1100 nm
600 µm ± 10 µm
6 illumination fibers around 1 read zip tube blue PVDF 3.18 mm OD 24 cm
12 cm
$699
R600-7-VIS-125F
400-2500 nm
600 µm ± 10 µm
6 illumination fibers around 1 read zip tube blue PVDF 3.18 mm OD 24 cm
12 cm
$699
RP200-7-UV-VIS
300-1100 nm
200 µm ± 4 µm
6 illumination fibers around 1 read zip tube blue PVDF PEEK ferrule, 8 cm
6.35 mm OD
4 cm
$499
Reflection/Backscattering Probes with Reference Leg
QR200-REF-UV-VI
300-1100 nm
200 µm ± 4 µm
6 illumination fibers around 1 read silicone monocoil
plus 1 fiber to monitor illumination
6.35 mm OD 8 cm
4 cm
$549
QR200-REF-VIS-N
400-2500 nm
200 µm ± 4 µm
6 illumination fibers around 1 read silicone monocoil
plus 1 fiber to monitor illumination
6.35 mm OD 8 cm
4 cm
$549
R200-REF-UV-VIS
300-1100 nm
200 µm ± 4 µm
6 illumination fibers around 1 read zip tube blue PVDF 6.35 mm OD 8 cm
plus 1 fiber to monitor illumination
4 cm
$549
R200-REF-VIS-NI
400-2500 nm
200 µm ± 4 µm
6 illumination fibers around 1 read zip tube blue PVDF 6.35 mm OD 8 cm
plus 1 fiber to monitor illumination
4 cm
$549
Fibers & Probes
QR600-7-SR-125F
Reflection/Backscattering Probes for Expanded Wavelength Coverage
QR200-12-MIXED
300-1100 nm &
400-2500 nm
200 µm ± 4 µm
6 UV-VIS & 6 VIS-NIR illumination silicone monocoil
fibers around 1 UV-VIS &
1 VIS-NIR fibers
6.35 mm OD 8 cm
4 cm
$749
R200-12-MIXED
300-1100 nm &
400-2500 nm
200 µm ± 4 µm
6 UV-VIS & 6 VIS-NIR illumination zip tube blue PVDF 6.35 mm OD 8 cm
fibers around 1 UV-VIS
& 1 VIS-NIR fibers
4 cm
$749
$599
Angled Probes for Solutions & Powders
QR200-ANGLE-U
300-1100 nm
200 µm ± 4 µm
6 illumination fibers around 1 read silicone monocoil
6.35 mm OD 8 cm
4 cm
QR200-ANGLE-V
400-2500 nm
200 µm ± 4 µm
6 illumination fibers around 1 read silicone monocoil
6.35 mm OD 8 cm
4 cm
$599
QR400-ANGLE-U
300-1100 nm
400 µm ± 8 µm
6 illumination fibers around 1 read silicone monocoil
6.35 mm OD 16 cm
8 cm
$749
6.35 mm OD 16 cm
QR400-ANGLE-V
400-2500 nm
400 µm ± 8 µm
6 illumination fibers around 1 read silicone monocoil
8 cm
$749
R200-ANGLE-UV
300-1100 nm
200 µm ± 4 µm
6 illumination fibers around 1 read zip tube blue PVDF 6.35 mm OD 8 cm
4 cm
$499
R200-ANGLE-VIS
400-2500 nm
200 µm ± 4 µm
6 illumination fibers around 1 read zip tube blue PVDF 6.35 mm OD 8 cm
4 cm
$499
R400-ANGLE-UV
300-1100 nm
400 µm ± 8 µm
6 illumination fibers around 1 read zip tube blue PVDF 6.35 mm OD 16 cm
8 cm
$599
R400-ANGLE-VIS
400-2500 nm
400 µm ± 8 µm
6 illumination fibers around 1 read zip tube blue PVDF 6.35 mm OD 16 cm
8 cm
$599
* LTBR stands for Long Term Bend Radius, the bend radius allowed long term (such as for storage) before damaging the fiber.
** STBR stands for Short Term Bend Radius, the momentary bend radius allowed before damaging the fiber.
Specifications
Fiber profile:
Fiber core:
Fiber cladding:
Fiber buffer/coating:
Operating temp. range:
Numerical aperture:
Step-index multimode
Pure silica core
Fluorine-doped silica cladding
Polyimide coating except where noted
-20 °C to 80 °C
0.22 ± 0.02 (yields an acceptance angle of 24.8° in air)
Tel: 727.733.2447 • Email: [email protected]
Probe ferrule material:
Probe connector(s):
Breakout:
Total probe length:
Stainless steel except where noted
Premium-grade SMA 905 Connectors for QR-series probes,
Laboratory-grade SMA 905 Connectors for R-series probes
Midway of assembly at 1 meter
2 meters for fiber assembly, 76.2 mm long for probe ferrule =
2.076 meters; custom lengths available
149
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Transmission Dip Probes
In Situ Monitoring
Our T300-RT and T200-RT Transmission Dip Probes couple
to our spectrometers and light sources to measure
absorbance and transmission in solutions. These probes
are especially useful for embedding into process streams
for in situ, real-time sample monitoring.
Theory of Operation
Fibers & Probes
In transmission dip probes, light is transmitted from
the illumination fiber through a plano-convex lens
and through the sample compartment to a flat,
second-surface mirror. The light reflects from this
mirror and is focused by the lens onto the read
fiber. The advantage of the transmission probe
is its compact optical design, which fits into a
6.35-mm (1/4") outer diameter stainless steel
body, or ferrule. The trade-offs with these
probes are that they measure both
transmitted light and backscattered light
from the sample and have internal
reflections that limit the dynamic range
of the measurement. Still, at less than $1,000, transmission
probes are a cost-effective option for many on-line and lab
applications.
T300-RT Design
The stainless steel RT-series tips screw
onto the end of the T300-RT or T200-RT.
Transmission Dip Probe Operation
Second-surface mirror
The T300-RT-UV-VIS Transmission Dip Probe consists of two
300-µm solarization-resistant optical fibers -- one
illumination optical fiber and one read optical fiber -- in a
3.175-mm (1/8") outer diameter stainless steel assembly
that slides into a 127-mm long, 6.35-mm (1/4") outer
diameter stainless steel ferrule. Each leg of the assembly
has an SMA 905 termination so that one leg can be
attached to a light source and the other to a spectrometer.
T200-RT Design
The T200-RT-VIS-NIR Transmission Dip Probe has the same
optical design as the T300-RT-UV-VIS, but is made with two
200-µm VIS-NIR optical fibers in its assembly.
Illumination fiber
Process Applications
Read fiber
Plano-convex lens
Specifications
Fiber type:
Pressure limit:
Temperature limit:
Outer diameter:
Probe length:
Fiber length:
Breakout:
Optics:
Probe wetted materials:
Pathlength:
Fiber jacketing:
Connector:
Probe sleeve:
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T300: 300 µm UV/SR fiber type (200-1100 nm)
T200: 200 µm VIS-NIR fiber type (400-2500 nm)
100 psi
100 °C without sleeve
6.35 mm
127 mm
2 meters
1.5 meters from the end of the probe
Fused silica
Stainless steel, fused silica, EPO-TEK 353ND
2, 4, 5 or 10 mm
PVC Monocoil
SMA 905
Stainless steel
Both probes fit into a standard 1/4" Swagelok fitting for
installation into a pipe or reactor. Probe optics are mounted
with an epoxy that offers superior chemical resistance to
most solvents and can tolerate high temperatures.
Screw-on Tips: Choose Your Pathlength
Available separately are the screw-on, interchangeable
probe tips necessary to use either probe. The RT-series tips
come in pathlengths of 2 mm, 4 mm, 5 mm or 10 mm so
that sampling setups can be configured for optically dense
or dilute solutions.
T300-RT-UV-VIS:
$750
T200-RT-VIS-NIR:
$750
RT-2MM:
$240
RT-4MM:
$240
RT-5MM:
$240
RT-10MM:
$240
For all your sensing needs, visit OceanOptics.com
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Transmission Dip Probes
Dip Probe for Hostile Environments
The TP300-UV-VIS Transmission Dip Probe
couples to our spectrometers and light
sources to measure the absorbance and
transmission of solutions in harsh
environments.
Probe Assembly
The TP300-UV-VIS consists of two 300-µm
optical fibers -- one illumination optical fiber
and one read optical fiber -- in a 3.175-mm
(1/8") outer diameter stainless steel assembly
sealed into a PEEK polymer sleeve. You have
the option of choosing solarization-resistant
fibers or VIS-NIR fibers for your assembly.
PEEK Polymer Sleeve
The TP300 comes
with the TPSLEEVE
PEEK sleeve.
The T300SLEEVE
stainless steel sleeve
is available.
Theory of Operation
The TP300 works the same way as the T300-RT and
T200-RT probes. Light travels from the light source
into the illumination leg of the probe and through a
lens near the end of the probe. The light then
transmits through the sample compartment to a
second-surface mirror. The light reflects and travels
back through the sample compartment a second time
and is then focused by the lens onto the read fiber
and through the read leg of the probe to the
spectrometer.
Adjustable-pathlength Tips
Fibers & Probes
The sleeve is designed for environments with
temperatures up to 200 °C. The PEEK
material is also radiation-resistant and has
low flammability and excellent chemical
resistance. The PEEK sleeve (TPSLEEVE) comes
with the TP300-UV-VIS. An additional
stainless steel sleeve (T300SLEEVE) is available.
The RTP-series Tips (above)
are for transmission and
absorbance measurements.
The RT-PH Tip (left) turns
the TP300 Probe into a pH
Sensor (see page 76).
There are two adjustable-pathlength tips (2-mm to
10-mm pathlengths or 10-mm to 20-mm pathlengths)
available for the TP300-UV-VIS. Additionally, an RT-PH
tip for mounting pH films in the optical path can be
used for pH-sensing applications.
TP300-UV-VIS:
$750
TP300-VIS-NIR:
$750
T300SLEEVE:
$250
TPSLEEVE:
$250
RTP-2-10 Tip:
$240
RTP-10-20 Tip:
$240
RT-PH Tip:
$240
Specifications
Fiber type:
Outer diameter:
Length:
Optics:
TP300-UV-VIS -- 300 µm UV/SR fiber type (200-1100 nm)
TP300-VIS-NIR -- VIS-NIRfiber type (400-2500 nm)
3.175 mm
107.9 mm for probe, 2 meters for fiber
Fused silica
Tel: 727.733.2447 • Email: [email protected]
Pathlength:
Outer materials:
Temperature limit:
Pressure limit:
Adjustable from 2-10 mm or from 10-20 mm
RT-PH - fixed 16-mm pathlength
PVDF for jacketing, PEEK polymer for sleeve
200 °C with PEEK sleeve
100 psi
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Industrial Process Probes
Industrial Environments up to 250 psi, 300 °C
Our TI300-series Transmission Industrial Dip Probes can be
used in environments with pressure limits up to 250 psi and at
temperatures up to 300 °C. The TI300-UV-VIS uses 300 µm
diameter solarization-resistant optical fiber
(200-1100 nm), while the TI300-VIS-NIR uses 300 µm
diameter VIS-NIR optical fiber (400-2200 nm). The
TI300 probes couple to our spectrometers and
light sources to measure solutions absorbance
and transmission in industrial applications.
Sampling Tips Use O-rings,
Replacing Epoxy
Fibers & Probes
With our other transmission probe
offerings, we use high-grade epoxy to
adhere the sampling optics to the
sampling tips. However, most epoxies lose their adhesive
properties in continuous heat over 220 °C. With the TI300s,
we mounted the probe optics into the sampling tips using
Parker perfluoroelastomer (Parofluor ULTRA) O-ring seals. The
material in these special O-rings offers broad chemical
resistance, excellent thermal stability and temperature
resistance up to 300 °C. The other materials in the screw-on,
interchangeable sampling tips are grade 303 stainless steel, a
back-coated quartz mirror and a quartz lens. The tips come in
pathlengths of 2, 5, 10, 25 and 50 mm so that sampling
setups can be configured for optically dense or dilute solutions.
Probe Ferrule & Jacketing
The TI300s use a fully interlocked stainless-steel jacketing over
Teflon tubing and have an outer diameter of 0.68 cm. The
immersible part of the probe, the ferrule, is also made from
303 stainless steel and measures 12.7 cm in length, with an
outer diameter of 1.27 cm.
How it Works
Specifications
Fiber type:
Wavelength range:
Pressure limit:
Temperature limit:
Sampling tip body:
Sampling tip optics:
Sampling tip O-ring:
Probe ferrule:
Probe jacketing:
Length:
Breakout distance:
Immersible length:
Optical pathlengths:
Connectors:
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TI300-UV-VIS -- 300 µm diameter
UV/SR fiber type (200-1100 nm)
TI300-VIS-NIR -- 300 µm diameter VIS-NIR
fiber type (400-2500 nm)
TI300-UV-VIS -- 200-1100 nm
TI300-VIS-NIR -- 400-2500 nm
250 psi
300 °C
303 stainless steel
Quartz back-coated mirror and quartz lens
Parker perfluoroelastomer (Parofluor ULTRA)
O-ring seal
12.7 mm outer diameter 303 stainless steel
Fully interlocked stainless-steel jacketing over
Teflon tubing; total 6.8 mm outer diameter
Fiber -- 2 meters
Ferrule -- 12.7 cm without tip
Tips -- 2.6 cm to 4.99 cm, depending on tip
1 meter from the end of the probe
12.7 cm
2, 5, 10, 25 and 50 mm pathlengths available
SMA 905
In a TI300 probe, there are two 300-µm optical fibers -- one
illumination optical fiber and one read optical fiber -- in a
12.7-mm diameter stainless-steel ferrule. Light transmits via
the illumination fiber through a plano-convex lens and the
sample compartment to a flat, second-surface mirror (see
diagram on page 150). The light reflects from this mirror,
travels back through the sample compartment and is focused
by the lens onto the read fiber and through the read leg of the
probe to the spectrometer. The trade-offs with these probes are
that they measure both transmitted light and backscattered
light from the sample and have internal reflections that limit
the dynamic range of the measurement. But at less than
$1,600 (for the TI300 probe and one sampling tip), a TI300
probe, with its high pressure and temperature limits, is a great
option for many industrial applications.
TI300-UV-VIS:
$1,299
TI300-VIS-NIR:
$1,299
RT-TI-2MM:
$299
RT-TI-5MM:
$299
RT-TI-25MM:
$299
RT-TI-50MM:
$299
For all your sensing needs, visit OceanOptics.com
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Vacuum Feedthroughs
Feedthroughs with Industry-standard Flanges
These Vacuum Feedthroughs are welded into industry standard flanges, and designed for monitoring highvacuum applications from inside a vacuum system with external equipment, such as our spectrometers. The
optical fiber inside of the VFT is hermetically sealed into a stainless steel shell. These VFTs come in two standard
flange types: Conflat Flanges and ISO KF Flanges. The flanges use surgical-grade stainless steel with glassceramic seals. The flange-to-seal’s metal-to-glass design allows the entire assembly to perform up to either 250
°C and 10-10 Torr for the Conflat Flanges or 150 °C and 10-8 Torr for the ISO KF Flanges.
Item
VFT-1000-UV-133
VFT-1000-UV-16
VFT-1000-UV-40
Range
Flange Type
Price
200-µm diameter UV-VIS
300-1100 nm
1.33" OD Conflat
$279
VFT-200-VIS-133
200-µm diameter VIS-NIR
400-2500 nm
1.33" OD Conflat
$279
VFT-400-UV-133
400-µm diameter UV-VIS
300-1100 nm
1.33" OD Conflat
$440
VFT-400-VIS-133
400-µm diameter VIS-NIR
400-2500 nm
1.33" OD Conflat
$440
VFT-600-UV-133
600-µm diameter UV-VIS
300-1100 nm
1.33" OD Conflat
$450
VFT-600-VIS-133
600-µm diameter VIS-NIR
400-2500 nm
1.33" OD Conflat
$450
VFT-1000-UV-133
1000-µm diameter UV-VIS
300-1100 nm
1.33" OD Conflat
$485
VFT-1000-VIS-133
1000-µm diameter VIS-NIR 400-2500 nm
1.33" OD Conflat
$485
VFT-200-UV-275
200-µm diameter UV-VIS
2.73" OD Conflat
$450
300-1100 nm
VFT-200-VIS-275
200-µm diameter VIS-NIR
400-2500 nm
2.73" OD Conflat
$450
VFT-400-UV-275
400-µm diameter UV-VIS
300-1100 nm
2.73" OD Conflat
$455
VFT-400-VIS-275
400-µm diameter VIS-NIR
400-2500 nm
2.73" OD Conflat
$455
VFT-600-UV-275
600-µm diameter UV-VIS
300-1100 nm
2.73" OD Conflat
$465
VFT-600-VIS-275
600-µm diameter VIS-NIR
400-2500 nm
2.73" OD Conflat
$465
VFT-1000-UV-275
1000-µm diameter UV-VIS
300-1100 nm
2.73" OD Conflat
$499
VFT-1000-VIS-275
1000-µm diameter VIS-NIR 400-2500 nm
2.73" OD Conflat
$499
VFT-200-UV-16
200-µm diameter UV-VIS
300-1100 nm
1.18" OD KF16 ISO
$430
VFT-200-VIS-16
200-µm diameter VIS-NIR
400-2500 nm
1.18" OD KF16 ISO
$430
VFT-400-UV-16
400-µm diameter UV-VIS
300-1100 nm
1.18" OD KF16 ISO
$435
VFT-400-VIS-16
400-µm diameter VIS-NIR
400-2500 nm
1.18" OD KF16 ISO
$435
VFT-600-UV-16
600-µm diameter UV-VIS
300-1100 nm
1.18" OD KF16 ISO
$445
VFT-600-VIS-16
600-µm diameter VIS-NIR
400-2500 nm
1.18" OD KF16 ISO
$445
VFT-1000-UV-16
1000-µm diameter UV-VIS
300-1100 nm
1.18" OD KF16 ISO
$480
VFT-1000-VIS-16
1000-µm diameter VIS-NIR 400-2500 nm
1.18" OD KF16 ISO
$480
VFT-200-UV-40
200-µm diameter UV-VIS
2.16" OD KF40 ISO
$445
300-1100 nm
VFT-200-VIS-40
200-µm diameter VIS-NIR
400-2500 nm
2.16" OD KF40 ISO
$445
VFT-400-UV-40
400-µm diameter UV-VIS
300-1100 nm
2.16" OD KF40 ISO
$450
VFT-400-VIS-40
400-µm diameter VIS-NIR
400-2500 nm
2.16" OD KF40 ISO
$450
VFT-600-UV-40
600-µm diameter UV-VIS
300-1100 nm
2.16" OD KF40 ISO
$460
VFT-600-VIS-40
600-µm diameter VIS-NIR
400-2500 nm
2.16" OD KF40 ISO
$460
VFT-1000-UV-40
1000-µm diameter UV-VIS
300-1100 nm
2.16" OD KF40 ISO
$495
VFT-1000-VIS-40
1000-µm diameter VIS-NIR 400-2500 nm
2.16" OD KF40 ISO
$495
VFT-series Feedthroughs
Our general-purpose VFT-series
Vacuum Feedthroughs are designed to
penetrate NEMA enclosures. The VFT
screws into a 3/8-24 external threaded
hole in the vacuum chamber, or bolts
into a smooth hole with the provided
nut and washer.
Item
Fibers & Probes
VFT-1000-UV-275
Fiber Type
VFT-200-UV-133
Fiber Type
Range
Price
VFT-200-SR
200-µm diameter SR fiber
200-1100 nm
$299
VFT-200-VIS
200-µm diameter VIS-NIR fiber
400-2500 nm
$299
VFT-400-SR
400-µm diameter SR fiber
200-1100 nm
$299
VFT-400-VIS
400-µm diameter VIS-NIR fiber
400-2500 nm
$299
VFT-600-SR
600-µm diameter SR fiber
200-1100 nm
$299
VFT-600-VIS
600-µm diameter VIS-NIR fiber
400-2500 nm
$299
VFT-1000-UV
1000-µm diameter UV-VIS fiber
300-1100 nm
$299
VFT-1000-VIS
1000-µm diameter VIS-NIR fiber
400-2500 nm
$299
Specifications
Temperature limit:
Vacuum range:
Numerical aperture:
VFTs with Conflat Flanges
250 °C
1 x 10-10 Torr
0.22, and acceptance angle of 24.8°
VFTs with KF ISO Flanges
150 °C
1 x 10-8 Torr
0.22, and acceptance angle of 24.8°
Tel: 727.733.2447 • Email: [email protected]
VFT-Series
140 °C
1 x 10-9 Torr
0.22, and acceptance angle of 24.8°
153
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Bare Fiber Adapter Kit
The BFA-KIT Bare Fiber Adapter Kit is for the fiber tinkerer
who wants to polish bare (unjacketed) optical fiber. The kit
comes with fiber polishing holders for various sizes of
optical fibers.
The Bare Fiber Adapter Kit includes the following:
6 fiber polishing holders for various sizes of optical
fiber: (1 each for 100 µm, 200 µm, 300 µm, 400 µm,
600 µm and 1000 µm optical fibers)
a BFA-KIT-CHUCK connect-and-release adapter (which
can be purchased separately as well) to fasten the
SMAs onto bare optical fiber
several pieces of wire for cleaning out the polishing
holders and connect-and-release adapter
An SMA-PUCK polishing puck is not included
with the BFA-KIT, but is available separately.
The puck is used to polish the surface of
an optical fiber.
Fibers & Probes
Need a special SMA 905 Connector? We can
drill out an SMA 905 Connector from 149 µm to
2705 µm. Custom-drilled connectors are
available for $50 each.
BFA-KIT:
BFA-KIT-CHUCK:
SMA-PUCK:
The SMA-PUCK,
sold separately
from the BFA-KIT.
$249
$169
$129
How to Use the BFA-KIT
Select the fiber polishing holder
that corresponds to the diameter
of your bare optical fiber.
Attach the fiber polishing holder to the
front of the BFA-KIT-CHUCK connectand-release adapter.
Thread your bare
optical fiber through the
back of the chuck and
into the holder and
fasten. The holder
allows you to easily
work with the fiber for
various purposes, such
as polishing.
Fiber Tinkerer’s Kit
The FT-KIT Fiber Tinkerer Kit (left) includes
an assortment of randomly selected,
unterminated UV-VIS and VIS-NIR optical
fibers. Each fiber included in the kit will
be at least one meter in length. The Fiber
Termination Kit (TERM-KIT) on the
following page includes all the tools
needed to terminate and polish fiber.
FT-KIT:
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$99
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Fiber Termination Kit
Inspect & Repair Fibers
The TERM-KIT Termination Kit provides you with all the tools you
need to properly polish and terminate an optical fiber. The TERMKIT is great for inspecting, repairing and polishing optical fiber
assemblies. If you would like unterminated fibers for use
with the TERM-KIT, the FT-KIT Fiber Tinkerer Kit includes
an assortment of optical fibers in lengths of at
least one meter (see page 154 for details).
Included in Each TERM-KIT
Fibers & Probes
4 SMA 905 Connectors for 50 µm or
100 µm fibers
4 SMA 905 Connectors for 200 µm
optical fibers
4 SMA 905 Connectors for 400 µm optical fibers
4 SMA 905 Connectors for 600 µm optical fibers
4 SMA 905 Connectors for 1000 µm optical fibers
polishing puck
glass polishing plate (15 cm x 15 cm)
dozens of polishing papers
5-cavity crimp tool (for 2.6, 3.4, 3.8, 4.5 and 6.4 mm cavities)
scoring tool
inspection scope
2-hour cure epoxy
optical wipes
TERM-KIT: $599
Terminators
Our SMA 905 Connector Kits are an
excellent complement to the standard
Termination Kit (above). We offer six
different kits, each with 10 SMA 905
Connectors of the same size, drilled for
precise alignment with our optical fiber.
The difference between each kit is the
diameter size of the SMA 905 Connector.
We offer 150 µm, 270 µm, 380 µm,
490 µm, 710 µm and 1300 µm
diameter connectors.
TERMKIT-SMA-710
TERMKIT-SMA-270
TERMKIT-QSMA-710
TERMKIT-QSMA-270
Item
Fiber Type
TERMKITSMA-150
10 SMA Connectors for 100-micron and 50-micron fibers
50 µm and 100 µm
$75
TERMKITSMA-270
10 SMA Connectors for 200-micron fibers
200 µm
$75
TERMKITSMA-380
10 SMA Connectors for 300-micron fibers
300 µm
$75
TERMKITSMA-490
10 SMA Connectors for 400-micron fibers
400 µm
$75
TERMKITSMA-710
10 SMA Connectors for 600-micron fibers
600 µm
$75
TERMKITSMA-130
10 SMA Connectors for 1000-micron fibers
1000 µm
$75
TERMKITQSMA-150
10 Premium SMA Connectors for 100-micron and 50-micron fibers
50 µm and 100 µm
$170
TERMKITQSMA-270
10 Premium SMA Connectors for 200-micron fibers
200 µm
$170
TERMKITQSMA-380
10 Premium SMA Connectors for 300-micron fibers
300 µm
$170
TERMKITQSMA-490
10 Premium SMA Connectors for 400-micron fibers
400 µm
$170
TERMKITQSMA-710
10 Premium SMA Connectors for 600-micron fibers
600 µm
$170
TERMKITQSMA-130
10 Premium SMA Connectors for 1000-micron fibers
1000 µm
$170
Tel: 727.733.2447 • Email: [email protected]
For Use with
Fiber Diameters of
Price
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Optical Fiber Kits
Fiber Optic Kit -- UV-VIS
The FVA-UV Fiber Optic Variable
Attenuator helps control the
amount of light transmitted
between two fibers.
Fibers & Probes
We’ve taken our most popular laboratory-grade optical fiber
assemblies and accessories and combined them into cost-saving
Optical Fiber Kits -- perfect for testing, teaching or just plain
tinkering. The FOP-UV Optical Fiber Kit consists of five patch cord
optical fiber assemblies, the Fiber Optic Variable Attenuator, a
CC-3-UV Cosine Corrector, a fiber wrench and more. By buying
a kit instead of each product separately, you save over $400. The
table below lists the items in the kit.
FOP-UV KIT:
$999
Price
FOP-UV Items
Description
P50-2-UV-VIS
(1) 50 µm diameter optical fiber; UV-VIS
$99
P200-2-UV-VIS
(1) 200 µm diameter optical fiber; UV-VIS
$99
P400-025-SR
(2) 400 µm diameter optical fibers; UV, SR
$198
P600-2-UV-VIS
(1) 600 µm diameter optical fiber; UV-VIS
$159
21-02
(2) Splice bushings
21-01
(2) Bulkhead bushings
FVA-UV
(1) Fiber Optic Variable Attenuator
FOT-SMAWRENCH
(1) Fiber Wrench
CC-3-UV
(1) Cosine Corrector
FCBARREL
(2) 6.35-mm OD barrel for FC connectors
FIBER-WRAP
(3) 2-foot-long pieces of fiber wrap
74-UV
(1) Collimating Lens
Total, if purchased separately:
$26
$18
The FIBER-WRAP is
used to bundle and
protect optical fibers.
$10
$129
$58
$10
$159
$1,464
The CC-3-UV Cosine Corrector
attaches to optical fiber to
create an irradiance probe.
The 21-01 SMA Bulkhead
Bushing allows you to position
an optical fiber on a throughpanel such as a chamber wall.
The FOP-VIS Optical Fiber Kit consists of five patch cord optical
fiber assemblies, the Fiber Optic Variable Attenuator, CC-3
Cosine Corrector, fiber wrap, a fiber wrench and more. By
buying a kit instead of each product separately, you save nearly
$500. The table below lists the items included in the kit.
FOP-VIS KIT:
$999
156
The FC-BARREL accepts FCterminated fibers for use with our
lenses, lamps and other fixtures.
$499
Fiber Optic Kit -- VIS-NIR
The 21-02 Splice Bushing is an
in-line adapter that mates two
SMA 905 Connectors, such as
those on optical fibers.
FOP-VIS Items
Description
P50-2-VIS-NIR
(1) 50 µm diameter optical fiber; VIS-NIR
P200-2-VIS-NIR
(1) 200 µm diameter optical fiber; VIS-NIR
P400-2-VIS-NIR
(2) 400 µm diameter optical fibers; VIS-NIR
$238
P600-2-VIS-NIR
(1) 600 µm diameter optical fiber; VIS-NIR
$159
21-02
(2) Splice bushings
21-01
(2) Bulkhead bushings
FVA-UV
(1) Fiber Optic Variable Attenuator
FOT-SMAWRENCH
(1) Fiber Wrench
$10
CC-3
(1) Cosine Corrector
$99
FCBARREL
(2) 6.35-mm OD barrel for FC connectors
$58
FIBER-WRAP
(3) 2-foot-long pieces of fiber wrap
74-UV
(1) Collimating Lens
Total, if purchased separately:
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The 74-UV Collimating Lens can
be screwed onto the end of a
fiber to collimate light.
Price
$99
The FOT-SMAWRENCH slips over
SMA 905 Connectors to secure
fibers to spectrometers, collimating
lenses and accessories.
$99
$26
$18
$499
The P400-2-UV-VIS
Laboratory-grade Optical
Fiber in the FOP-VIS Kit.
$10
$159
$1,474
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Fiber & Probe Fixtures & Holders
C-Mounts
Our C-MOUNT-MIC Adapter Assembly with adjustable focusing barrel has
an SMA 905 Connector in its center for attaching to optical fibers. The
internal C-mount threads of this assembly allow you to adapt fiber optic
spectrometers to other optical devices such as microscopes and telescopes.
The MFA-C-MOUNT also connects to optical devices such as microscopes
and telescopes, but its center connector is designed to accept probes with
6.35-mm (1/4") outer diameter ferrules.
C-MOUNT-MIC:
$125
MFA-C-MOUNT:
$458
The MFA-C-Mount.
The C-MOUNT-MIC
Adapter Assembly.
Phototubus Microscope Adapter
The MFA-PT Phototubus Microscope Adapter adapts to a Phototubus outlet
on microscopes and accepts SMA 905-terminated optical fibers.
MFA-PT:
$424
The MFA-PT Phototubus
Microscope Adapter.
Right-angle Collimating Lens Holder
Fibers & Probes
The 74-90-UV is an assembly for mounting lenses at right angles, and is
especially useful for applications involving awkward optical fiber routing. It
has a mirror located under its cap bonded with high-temperature epoxy,
and reflects light from the collimating lens to 90°. Two ports accommodate
74-series Collimating Lenses (not included).
74-90-UV: $139
The 74-90-UV Right-angle
Collimating Lens Holder with
collimating lenses and
optical fiber (not included).
Reflection Probe Holders
The RPH-1 (far right) and RPH-2 (near right) are anodized aluminum platforms
with holes drilled at 45° and 90° angles to the surface. The RPH-1 holds
6.35-mm (1/4") diameter probes but with the RPH-ADP -- an adapter that fits on
the RPH-1 -- you can secure 3.17 mm (1/8") diameter probes as well. The RPH-2
is for use only with probes with SMA 905 Connectors. The Curved Surface Probe
Holders accommodate 6.35-mm (1/4") outer diameter probes for measuring
reflection of curved surfaces. The CSH (right) has a hole drilled at a 90° angle to
the surface. The CSH-45 has a hole drilled at a 45° angle to the surface.
RPH-1:
$75
RPH-ADP:
$69
RPH-2:
$102
CSH:
$107
CSH-45:
$122
RPH-2
RPH-1
CSH
Optical Stages
The Single-Point Reflection Stage (at right) is a probe holder for reflection
measurements of optical layers and other substrates up to 150 mm in diameter. The
probe holder accommodates fiber optic probes and other sampling devices up to
6.35 mm in diameter.
STAGE
The Stage-RTL-T is also a sampling system for analysis of substrate materials. The
STAGE-RTL-T can be configured for reflection and transmission measurements. For
details on both stages, see page 109.
STAGE:
$631
STAGE-RTL-T: $2,303
Tel: 727.733.2447 • Email: [email protected]
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Fiber & Probe Accessories
Bulkhead Bushing
The 21-01 SMA Bulkhead Bushing assembly is a device mount for optical fibers. The bulkhead
bushing allows you to position an optical fiber on a through-panel such as a
chamber wall. For example, to monitor a chamber, you could configure a
sampling optic that consists of an SMA 905-terminated optical fiber
screwed into the bulkhead bushing and mounted to a chamber window.
21-01: $9
Splice Bushings
The 21-02 SMA Splice Bushings are in-line adapters that connect SMA 905-terminated
optical fibers (or any two objects with SMA 905 terminations). A splice bushing consists
of a 0.75" screw with female ends. The standard 21-02 is made of nickel-plated brass
while the 21-02-SS is made of stainless steel. They are useful for coupling patch cords
to fiber optic probes and other devices, or for any multiple-fiber application where
coupling our standard optical fibers and accessories is preferable to creating
costly and complex fiber optic assemblies.
21-02:
$13
21-02-SS: $49
Fibers & Probes
Bulkhead & Splice Bushing Combo
The 21-02-BH SMA Bulkhead Splice Bushing is an in-line adapter that
connects SMA 905-terminated optical fibers through a chamber wall or
panel. The 21-02-BH features an O-ring for sealing against the inside of
the panel wall and a nut and lockwasher for mounting to the outside of
the panel wall.
21-02-BH: $23
FC Barrel
Our collimating lenses come standard with SMA 905 Connectors and interface to our
SMA-terminated fibers. If you have FC-terminated fiber, you could remove the inner
6.35-mm OD SMA barrel and replace it with this FC Barrel to connect to our products.
FCBARREL: $29
Finger Fiber Wrench
The FOT-SMAWRENCH is a wrench that slips over the hex nut of the SMA 905 Connector
used in Laboratory-grade Optical Fibers and helps to easily attach the fiber to connectors
on spectrometers, light sources, collimating lenses and many other accessories.
FOT-SMAWRENCH: $10
Modemixer/Modestripper
The Modemixer/Modestripper is an in-line, 3-mm Suprasil rod that connects two
SMA 905-terminated optical fibers to mix core modes and eliminate clad modes
throughout 180-2100 nm.
ADP-SMA-SMA: $268
Fiber Wrap
Fiber Safety Wrap is a protective spiral wrap used to bundle and protect optical fibers.
The durable wrap comes in 2-foot sections of red, yellow and green.
FIBER-WRAP: $10
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Thin Films & Optics
Overview
161
Thin Films & Optics Capabilities
162
Thin Films & Optics Applications
163
Specular Reflectance Standards
163
Collimation Testers
163
Optical Flats
164
Absorbing Glass Filters
Thin Films & Optics
160
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Overview: Thin Films & Optics
Precision, Experience & New Technology
The thin films and optics division that we established nearly five years
ago provides the most versatile of in-house manufacturing arts: the
innovation to create patented patterned dichroic filters for display and
scientific applications, and the expertise to produce optics and
coatings in OEM volumes. We are often our own best customer,
applying the kind of spectroscopy-savvy insight that few optics
suppliers can provide to the development of filters and optics that
enhance our spectrometers and accessories. Our “colored light”
products are among the most robust in the world, making them ideal
for theatrical and architectural applications. One such product is the
SeaChanger Color Engine, a color-changing device for stage lighting.
Substrates:
up to 455 mm diameter
Image size:
up to 250 mm square
Pattern resolution:
to 2 µm features
Spatial resolution:
to 1 µm
Temperature tolerance:
-80 °F to 700 °F
Coating wavelength range:
200-2500 nm
Coatings used in patterning:
see coating types
below
Specifications
Optics
Specifications
Thin Films
Thin Films & Optics
It all starts with a patented dichroic filter array process (see sidebar
below), which creates patterns precise enough to project still images.
There's much more, including both custom and off-the-shelf filters
and precision optics for markets ranging from the entertainment
industry to the military; optical metrology products such as lasercollimation testers and optical flats; and optical services from
machining and microlithography to etching and QC testing.
Curvature:
plano, concave, convex
Deviation/wedge:
<0.002 mm
Wavefront:
<1/20 wave
Flatness:
λ/10 at 633 nm
Irregularity:
<1/20 wave
Mechanical tolerance:
<0.010 mm
Parallelism:
<30 arc seconds
Surface quality:
better than <10-5
Coating Types
Antireflective
Beamsplitter
Dichroic, Dielectric,
and Interference
(UV to NIR)
Fluorides
High-reflective
Metals
Oxides
Custom
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Surface roughness:
<10 angstrom RMS
Size of finished optic:
1 mm to 200 mm
High-precision Optics
Beamsplitters
Collimation Testers
Filters
Flats
Laser Mirrors and Optics
Lenses and Windows
Mirrors
Prisms & Spheres
Reticles
Patented Coating
Technology
We have pioneered an optical coatings
production method that combines
optical thin film deposition techniques
with microlithographic procedures. This
patented process enables micron-scale
precision patterning of optical thin film
dichroic coatings -- which selectively
transmit or reflect light according to its
wavelength -- on a single substrate.
With this process, we create
multipatterned arrays of optical filters
for use in various products, including
micromechanical and optical
waveguide-based devices and dense
wavelength division multiplexers. The
process also can be applied to
multipart bonded filter applications
common to the manufacture of digital
data projectors, LCD display panels
and CCD camera detectors. In fact,
many optical coatings can be
patterned, including dielectric multiplelayer reflectors, bandpass filters,
dichroic edge filters and broadband
anti-reflection coatings. Our technique
also is used to deposit enhanced metal
reflectors, low-reflectivity opaque metals
and electrically conductive transparent
patterns.
For all your sensing needs, visit OceanOptics.com
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Thin Films & Optics Capabilities
Our expertise in electro-optics, spectroscopy, optical fibers and precision optics offers great value to researchers
and OEMs seeking a flexible, full-service supplier. We offer a range of skills, techniques and services to provide
you with state-of-the-art, one-stop-shopping optical manufacturing. Since all grinding, polishing, coating and
assembly operations are performed in-house, we have absolute control over the entire process, whether for
prototype or production optics.
Raw Materials
We select only top-grade materials for machining into the optical component you need for
your application. Glasses and ceramics include Borosilicate glass, fused quartz, Zerodur
and ULE.
Machining & Finishing
Our full-size machine shop creates metal components and assemblies with equipment
such as CNC mills and lathes and other machine shop tools. Our shaping and finishing
capabilities -- double-side grinding, cutting and polishing equipment for plano, concave
and convex optics -- apply to materials up to 200 mm in diameter or 220 mm in length.
Reticles
Thin Films & Optics
Our etch-and-fill reticles can be fabricated with line widths from 0.005 mm to 0.5 mm.
Etchings are available with black, white or red fill. The middle photo in the column at right
is a close-up of a 0.015 mm line-width etching. In addition to etch & fill, reticles can be
constructed of dielectric and metal vacuum deposited materials.
Assembly
Our in-house machining capabilities allow us to provide a wide range of assembly services,
including optical cementing, thin film and surface mounting, thin film bonding, soldering
and wiring.
Coating & Microlithography
Our patented optical coating technology combines optical thin film deposition techniques
with microlithographic procedures to provide a variety of precise, cost-effective, optical thin
film coatings. This high-precision patterning can be applied to whatever filtering
configuration the customer requests, and provides color filtering, spatial resolution,
transmission efficiency and durability that's superior to dye-colored gels and other
commonly used filtering technologies. All of the coatings listed below can be deposited
onto optical substrates using this patented process.
Dichroic, Dielectric,
and Interference
(UV to NIR)
Oxides
Beamsplitter
Antireflective
Fluorides
High-reflective
Metals
QC Standards
Our standards program adheres to ISO 9001 guidelines and strict quality control procedures. We meet military compliance requirements (MIL-PRF-13830) and adhere to SPC
and Total Quality Management document control and manufacturing practices.
QC Testing
We perform optical-surface, spectral, environmental and mechanical testing on all products
to ensure the highest quality. Our full-service metrology department has at its disposal
equipment such as interferometers, a radius bench, alignment telescopes and
spectrophotometers.
Tel: 727.733.2447 • Email: [email protected]
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Thin Films & Optics Applications
Our expertise in a wide range of optical applications offers great value to researchers and OEMs seeking a flexible, fullservice supplier. We offer applications know-how that few manufacturers can match. Because of our applications knowledge
and our high manufacturing standards -- a surface accuracy to 1/20λ and a scratch-to-dig rating of 10:5 -- we can meet
most any optical specification. Our custom products can be integrated into many applications, including those listed below.
Thin Films & Optics
Applications
Entertainment/
Lighting
Consumer
Electronics
AR coatings for
GOBOs
Broadband antireflection coated filters for
entertainment
lighting
Coatings for light
envelopes
Dichroic filters for
stage lighting
Filters for special
effects lighting
Hot and cold mirrors
for lighting fixtures
Large-format still
images
Dielectric coatings for
personal digital
assistant screens
RGB filters for LCD
and projection
displays
Patterned GOBOs for
projection systems
Color technology for
HDTV, high-def
monitors, and rearprojection TVs
UVA-B-C filters in
cameras
Reticles
Binoculars
Bore-sighting devices
Fire control
Precision optics for
E-O systems
Instrumentation
Metrology
Optical
Networking
Bandpass filters for
medical fiber optic
instruments
Hyper-spectral
imaging filters for
CCD cameras
RGB color filters for
CCD detectors
Second- and thirdorder blocking filters
for spectroscopy
Spectroscopic kits for
optics inspection
Optics for optical
benches in
spectrometers
Flats for inspecting
optics
Collimation Testers for
examining and
adjusting the
collimation of laser
beams
Spectroscopic kits for
optics inspection
Reflectance standards, NISTtraceable
Long Trace Profilometer for large flats
and aspheres
AR coatings for network components
Bandpass filters, gain
flatteners and
rejection filters for
DWDM
Coatings for MEMS,
waveguide relays
and switches
Filters for wavelength
add/drop couplers
Tunable filters for
transmitters and
receivers
Examples of Custom Products
Variable Saturation Filters
Excellent optical transmission
efficiency for superior brightness
Temperature and humidity
stability for consistent color
Used in entertainment, display
and lighting fixtures
Reticles
Used for targeting systems,
firearm scopes and binoculars
Etch-and-fill or dielectric-andmetallic patterns
Superior line and image quality
Patterned MEMs Windows
Patterned MEMs Windows on a
variety of custom-sized wafers
Antireflective coatings available
in ranges from 200-2500 nm
Patterns aligned with great
precision on both wafer surfaces
Technologies for Entertainment and Consumer Applications
Our patterned dichroic filters can be patterned with such precision that it’s possible to
project even large-format still images with remarkable resolution and clarity. With that
same technology, we’ve developed a line of “colored light” products for theatrical, worship
and architectural lighting installations, anchored by the award-winning SeaChanger Color
Engine (at right). SeaChanger is a four-filter color changer designed as an accessory for
ETC Source Four Ellipsoidals, the world’s most popular stage lights. SeaChanger fills a
niche between inexpensive but maintenance-intensive color gel scrollers -- the traditional
color-changer technology for stage lighting -- and higher priced moving lights, and has
appeared everywhere from church productions to Broadway musicals. We’ve also
www.SeaChangerOnline.com
produced filters for the next generation of micro-mirror-based digital display technologies,
as well as precision mirror coatings and optics designed to improve the safety and
performance of a wide range of consumer products.
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Specular Reflectance Standards
We offer three specular reflectance standards for use as
references when measuring the reflection of surfaces with high
or low specular reflectivity. The superior coatings on the
substrates are environmentally stable; they are able to withstand
high temperatures and mechanical stresses. Reflectivity values
for the standards are built into our software to provide a
reference for any specular measurement.
With the STAN-SSH High-reflectivity Specular Reflectance
Standard (above), you receive a certificate of calibration in paper
and electronic formats.
We offer a STAN-SSH High-reflectivity Specular Reflectance
Standard designed as a standard reference when measuring the
optical substrates, optical coatings, machined metals and
semiconductor materials. (A NIST version of the STAN-SSH is
also available.) The STAN-SSL Low-reflectivity Specular
Reflectance Standard can be used as a reference when
measuring samples such as thin film coatings, anti-reflective
coatings, blocking filters and substrates. For details on the
specular reflectance standards, see page 108.
STAN-SSH:
$499
STAN-SSH-NIST: $999
STAN-SSL:
$499
Thin Films & Optics
Collimation Testers
Use Shear-plate Collimation Testers to examine the collimation of
laser light, and as tools for measuring the wavefront curvature and
divergence/convergence magnitude of optical components such as
large-radius optics. Each tester consists of a wedged, high-quality
optical flat housed in a heavy-duty anodized aluminum frame. Each
tester is available in apertures ranging from 10 mm to 200 mm in
diameter, and is useable from 350-2500 nm.
The testers are remarkably easy to use: When a planar wavefront is
incident at an angle of 45°, two reflected wavefronts result. The
lateral separation of these wavefronts is referred to as shear.
Fringes -- parallel patterns of light and dark areas -- will be seen in
the overlapping region of the two images. Collimating the laser
beam is a matter of adjusting the collimating system until the fringe
pattern is parallel to the shadow of the collimation tester's reference
wire. See page 111 for details on all of our collimation testers.
Optical Flats
Each Optical Flat is a finely polished optical reference
surface that can be used to visually inspect the flatness
of optical components such as mirrors, filters, prisms
and windows. We offer single-sided optical flats in
either fused silica or Zerodur, each of which can be
enhanced with an aluminum coating to increase
contrast and improve the visual reference. There are
nearly 50 different flats available, ranging from 1" to 6"
in diameter and with flatness accuracies as precise as
1/20 wave. For a complete list of prices and
specifications, see page 110.
Tel: 727.733.2447 • Email: [email protected]
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Absorbing Glass Filters
Schott Glass Filters
Schott glass filters absorb light energy in certain
regions of the spectrum. These filters fit easily
into our light sources, cuvette holders and in-line
filter holders. Please check for availability.
High-pass Filters
High-pass Filters are transmissive approximately
50% at the nominal cutoff wavelength, >99% at
wavelengths 50 nm higher than the cutoff, and
less than 0.1% at 50 nm lower than the cutoff.
High-pass filters are used to eliminate secondand third-order effects, test for stray light, and
block excitation energy in fluorescence
experiments.
Schott Standard Filters
Thin Films & Optics
Colored Glass
ND Filters
Balancing Filters
Balancing Filters absorb energy in some regions
while transmitting in others. The BG 34 filter, for
example, reduces the light’s intensity at 600 nm
from a tungsten bulb while transmitting all of
the light at the blue and red regions, where
detector sensitivity in our spectrometers is lower.
BG 3
BG 40
GG 420
OG 570
UG 11
D0.15
BG 4
BG 42
KG 1
OG 590
VG 3
D0.3
BG 7
FG 3
KG 2
RG 6
VG 4
D0.6
BG 12
FG 4
KG 3
RG 9
VG 6
D1.0
BG 13
FG 10
KG 4
RG 610
VG 9
D1.3
BG 14
FG 12
KG 5
RG 630
VG 9
D1.6
BG 18
FG 13
NG 1
RG 645
VG 10
D2.0
Bandpass Filters
BG 20
FG 16
NG 3
RG 665
WG 225
D2.3
BG 23
FG 17
NG 4
RG 695
WG 280
D2.6
Bandpass Filters pass energy in a certain region
and block energy above and below that region.
BG 24 A
GG 375
NG 5
RG 715
WG 295
D3.0
BG 25
GG 385
NG 9
RG 725
WG 305
D3.3
OF2, OF1 & Inline-OF Filters
BG 26
GG 395
NG 10
RG 780
WG 320
D3.6
BG 28
GG 400
NG 11
RG 830
WG 335
D4.0
BG 34
GG 435
NG 12
RG 850
WG 345
D4.3
BG 36
GG 455
OG 515
RG 1000
WG 360
D4.6
BG 38
GG 475
OG 530
UG 1
BG 39
GG 495
OG 550
UG 5
We offer OF2 Filters (see top photo) for
installing into the optical path of the
spectrometer setup. We also offer OF1 Filters
(see top photo in the column below) that are
installed permanently in the SMA 905 Connector
of the spectrometer. The OF1 filters are limited
to the filters listed on page 16 and come in
4.75 mm diameter and 2 mm thickness.
D5.0
Please check with us on filter availability.
High-pass Filters
OF2-WG305
pass >305 nm
square 25.4 x 25.4 x 3 mm
$50
OF2-GG375
pass >375 nm
square 25.4 x 25.4 x 3 mm
$50
OF2-GG395
pass >395 nm
square 25.4 x 25.4 x 3 mm
$50
OF2-GG475
pass >475 nm
square 50.8 x 50.8 x 3 mm or
$50
OF2-OG515
pass >515 nm
square 25.4 x 25.4 x 3 mm
$50
OF2-OG550
pass >550 nm
square 25.4 x 25.4 x 3 mm
$50
square 25.4 x 25.4 x 3 mm
Balancing Filters
OF2-FG3
enhance blue and red
square 25.4 x 25.4 x 3 mm
$50
OF2-BG34R
enhance blue and red
round 12.7 mm OD
$50
Bandpass Filters
OF2-KG3
>325 nm and <700 nm
square 25.4 x 25.4 x 3 mm
$50
OF2-U360
>340 nm and <380 nm
square 25.4 x 25.4 x 3 mm
$50
OF2-RG780
>780 nm and 50%
square 25.4 x 25.4 x 3 mm
$50
transmission <2.7 µm
Filter Kit for use with LS-1 Light Source
OF2-LS
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164
BG34, GG395, OG550, Teflon diffusers
$100
In addition, our
INLINE-FH Filter
Holder (middle left)
and FH-SMA Filter
Holder (bottom left)
also hold the filters
listed in these
tables, and are cut
to 8 mm diameter
and from 1 mm to
7 mm thick to fit
these fixtures. Filters
used in the INLINEFH and FH-SMA
Filter Holders are
$100 each. See
page 113 for
details.
For all your sensing needs, visit OceanOptics.com
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Resources
Overview
167
Setup: Solutions Absorbance
168
Setup: Upwelling/Downwelling
169
Setup: O2 Sensing
170
Setup: Gas Absorbance
171
Setup: Fluorescence
172
Setup: LED Analysis
173
Setup: Laser Analysis
174
Setup: LIBS
175
Setup: Metrology
176
Setup: UV-VIS Reflection
177
Setup: Reflected Color
178
Spectral Identity
183
Indices
Resources
166
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Overview: Resources
Our Know-how = More Resources for You
85,000+ Spectrometers,
1,000s of Applications
Find out more about our products, experience and support through the following:
We’ve sold over 85,000+
Ocean Optics optical-sensing
systems since 1992, which has
provided us with a body of
applications knowledge that is
unmatched in the industry. Our
spectrometers are used in
applications such as these:
Live Demonstrations
Each year we exhibit at nearly 100 tradeshows around the world (OceanOptics.com/
Tradeshows.asp). At home, we conduct
formal seminars and can customize training
sessions to your requirements.
Resources
Science Curricula
Our Educational Spectroscopy Grant
Program rewards educators and researchers
for their use of spectroscopy in curricula or
research. Information about grant-winning
projects is posted at OceanOptics.com/
Applications/GrantWinners.asp.
R&D Services
Our Applications Group will take ownership
of your most challenging application needs.
The Group provides optical and electronic
design services, software engineering and
spectral modeling, testing and validation,
and rapid prototyping capabilities.
Reference Library
We have amassed nearly 500 technical
papers featuring our spectrometers and
accessories. Citations are on our website at
OceanOptics.com/Applications.asp.
Technical Information on the Web
We believe in easy access to information. That’s why we don’t hide our prices and that’s
why we provide easily accessible technical documentation on our website, so that you can
view manuals before you buy the instrument. We also include the manufacturer’s name
and the model number for components that go into our instruments. We want to provide
you with all of the information you need not only to make the right purchasing decision,
but also to get the best performance out of your Ocean Optics products.
OceanOptics.com/Technical.asp. Choose the TECHNICAL button on our website to
view and download information about our products and technology, including manuals
and operating instructions, software downloads and system specifications.
Operating Instructions. We provide hundreds of pages of easy-to-access operating
instructions and specifications of our products so that you can read before you buy at
OceanOptics.com/Technical/OperatingInstructions.asp.
Software Downloads. Easily download the latest operating and application software,
device drivers and code, utility programs and microcode at
OceanOptics.com/Technical/SoftwareDownloads.asp.
Spectrometer System Specifications. Spectrometer system performance depends on
a host of factors, such as the detector, optical bench, grating, entrance aperture size
and sampling optics, just to list a few. To help you understand how to configure
spectrometer systems, visit OceanOptics.com/Technical/SystemSpecifications.asp.
Applications Database. Choose the APPLICATIONS button from any Ocean Optics
webpage to view an up-to-date bibliographic listing of journal and magazine articles
that reference our products. Visit OceanOptics.com/Applications/References.asp.
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166
Air and soil in situ
monitoring
Astronomy
Biological and chemical
warfare agent detection
Biotechnology
Blood oximetry
Cancer detection
Chemistry
Color measurement
Crystal growth
Display technologies
Dissolved oxygen
Elemental analysis
Endpoint detection
Exhaust emission analysis
Flow injection analysis
Fluorescence of corals
Food processing
Forensics
Gemstone grading
General R&D
Headspace monitoring
Laser characterization
LED quality control
Life sciences
Manufacturing
Medical research
Non-destructive testing
Optical filter transmission
pH monitoring
Pharmaceuticals
Physics/Optics
Physiological applications
Plasma monitoring
Process control
Radiometry
Raman spectroscopy
Reaction kinetics
Semiconductor processing
Shelf life of food and
beverages
Stack emissions
Thin film thickness
Tissue composition
For all your sensing needs, visit OceanOptics.com
The ABCs of Absorbance
Setup : Solutions Absorbance
Like thousands of other educators,
chemists at Miami (Ohio) University have
equipped their labs with Ocean Optics
spectrometers and accessories for basic
spectroscopic measurements such as
solutions absorbance.
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USB4000-UV-VIS
Of particular interest is a PC-based setup
for measuring the UV-VIS absorption
spectrum of iodine crystals from
500-580 nm. This experiment is readily
performed using an S2000 Spectrometer,
LS-1 Tungsten Halogen Light Source,
fiber optic patch cords and a 10-cm
pathlength cuvette holder. Substitute a
USB4000 Spectrometer (see drawing at
right) to eliminate the external A/D card
that completes the Miami University
system.
DH2000-BAL
QP400-025-SR
(read fiber)
CV-Q-10
QP400-025-SR
(illumination fiber)
CUV-UV
Overview
Absorbance measurements are used to quantify the concentration of gases and
solutions (the latter is described here) that absorb light in a media that transmits
light. The signal in absorbance units is proportional to the molar absorptivity,
pathlength and concentration of the sample (see Beer’s Law, page 178).
Spectrometer
Solutions absorbance experiments are not
limited to cuvette holder setups. Flow
cells, on-line dip probes and other
sampling optics are available, with the
latter especially useful for in situ
applications. For example, one Ocean
Optics customer uses a UV-VIS
spectrometer and dip probe to measure
the absorbance of vanadium
oxytrichloride (VOCI3), a potentially toxic
liquid used in the production of rubber
(the absorptivity of VOCI3 relates to its
stability). Because the VOCI3 reacts with
moisture in the air and forms vanadic
and hydrochloric acids, it must be
measured in a moisture-free
environment. In situ measurements
eliminate the need for potentially risky
sample collection.
The USB4000-UV-VIS Spectrometer is ideal for absorbance measurements from
200-850 nm. The spectrometer is configured with Grating #1, which has peak
efficiency at 300 nm. This configuration provides adequate resolution (~1.5 nm
FWHM) for most solutions absorbance measurements. The built-in OFLV-200-850
Order-sorting Filter eliminates second-and third-order effects that otherwise yield
false peaks in absorbance spectra. The preferred light source is the DH2000-BAL
Deuterium Tungsten Halogen Light Source. The DH2000 is a less expensive source,
but lacks the filtering technology that eliminates problems associated with the
D-alpha line in the deuterium source.
Resources
Another option is the CHEM4-UV-VIS Lab
Spectrophotometer, which consists of a
200-850 nm USB-interface spectrometer,
a combination deuterium tungsten
halogen light source and 1-cm cuvette
holder, high-speed electronics and
software.
Sampling Optics
For absolute absorbance measurements, use the 1-cm pathlength CUV-UV Cuvette
Holder and the CV-Q-10 Quartz Cuvette. For relative absorbance, direct-attach
USB accessories, dip probes and flow cells are available. We recommend
QP400-025-SR Premium-grade Solarization-resistant Optical Fibers as illumination
and read fibers. Use NIST-traceable STAN-ABS Photometric Absorbance Standards
to provide certifiable results.
Components
1.
USB4000-UV-VIS General Lab Spectrometer
Page
Price
34
$2,649
25 µm Slit as entrance aperture
15
included
Grating #1, 200-850 nm range
16
included
DET4-200-850 Detector with UV4 Detector Window Upgrade
17
included
and OFLV-200-850 Order-sorting Filter
2.
DH2000-BAL Deuterium Tungsten Halogen Light Source
122
$3,588
3.
(2) QP400-025-SR Premium-grade SR Assemblies
142
$238
4.
CUV-UV Cuvette Holder
90
$399
5.
CV-Q-10 Quartz Cuvette
93
$75
6.
STAN-ABS-UV Photometric Absorbance Standards
93
$370
7.
SpectraSuite Spectroscopy Operating Software
80
$199
8.
ASP Annual Service Package
62
$250
Total:
Tel: 727.733.2447 • Email: [email protected]
$7,768
167
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Setup: Upwelling/Downwelling
In the small Pacific island of New
Caledonia, a multinational team of
researchers has used Ocean Optics
spectrometers to measure the effects of
strip mining on coastal erosion, sea grass
growth and coral reef health.
HR4000
DH2000-CAL
Measuring Mining Effects
The team focused on the relationship
between above-water reflectance and
turbidity profiles. The latter relates to
fluxes in the presence of metals and
various pollutants -- and thus, to sea
grass growth and coral reef health.
QP400-2-UV-VIS
CC-3-UV
Overview
Upwelling radiation is radiation -- either reflected solar or emitted terrestrial -- that
is directed upward from the earth's surface. Downwelling radiation is radiation that
is directed toward the earth's surface from the sun or atmosphere. The relationship
between the two (albedo) can be used to derive spectral information from
vegetation, forest canopies, seabeds and more.
Resources
Spectrometer
An HR4000 Spectrometer with an HC-1 grating provides an elegant solution for
upwelling and downwelling measurements. The HC-1 is a variable-blazed grating
that covers the 200-1050 nm wavelength range; optical resolution is ~1.5 nm
(FWHM) with a 50 µm slit as the entrance aperture. An OFLV-200-1100 Ordersorting Filter eliminates second- and third-order effects.
Sampling Optics
The spectrometer connects to a patch cord that screws into the CC-3-UV Cosine
Corrector. The CC-3-UV can be used as part of a configuration for measuring
absolute spectral irradiance. You’ll need a DH2000-CAL (or LS-1-CAL for
300-1050 nm only) to calibrate the absolute spectral response of the system and
SpectraSuite Spectroscopy Operating Software to calculate spectral intensity and
photopic data in lumens, lux or candela. An alternative to the CC-3-UV is a
Gershun tube, which has fixtures for adjusting the area of light from 1° to 28° and
attaches directly to the spectrometer or to an optical fiber.
Components
1.
HR4000 High-resolution Spectrometer
Page
Price
21
$3,999
50 µm Slit as entrance aperture
22
$150
Grating HC-1, 200-1050 nm range
23
$600
DET4-200-1100 Detector with OFLV-200-1100 Order-sorting
24
$400
$169
Filter and UV4 Detector Window Upgrade
2.
QP400-2-UV-VIS Premium-grade Patch Cord Assembly
142
3.
CC-3-UV Cosine Corrector
104
$129
4.
DH2000-CAL Radiometric Calibration Standard
132
$3,275
5.
SpectraSuite Spectroscopy Operating Software
80
6.
ASP Annual Service Package
62
Total:
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168
$199
$250
$9,171
For all your sensing needs, visit OceanOptics.com
A USB4000 Spectrometer set from 3601100 nm measures reflectance and
irradiance. The USB4000 connects to a
patch cord that screws into a Gershun
Tube, which has fixtures for adjusting the
area of light entering the fiber -- in this
case, to reduce the field of view to 3°.
Upwelling irradiance and downwelling
radiance measurements -- the spectral
distribution of the underwater light field -add valuable data.
The researchers also have measured the
concentration of chlorophyll pigment in
coastal waters and the reflectance of
sand and mud collected at Caribbean,
Mediterranean and Pacific beaches. The
sand application used a dual-channel
spectrometer for visible (410-900 nm)
reflectance measurements of various
natural sands. Reflectance spectra were
deduced from successive measurements
of upwelling irradiance using a
Spectralon plate and downwelling
radiance captured under natural light.
Ultimately, researchers will use satellite
monitoring, spectroradiometric
measurements and numerical models to
better understand the nature of
particulate transport in coral reef
lagoons, especially as it relates to erosion
rates in coastal areas.
O2 Medical Diagnostics
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Setup: Oxygen Sensing
Researchers at two Irish universities have
monitored dissolved oxygen in cellular
media in order to validate the optimum
gassing technique to induce hypoxia in
irradiated cells.
MFPF100-1
Scientists from University College Cork
and Cork University Hospital measured
irradiated HeLa cells -- a strain of human
cells used for biological studies -- under
both oxic (rich in oxygen) and hypoxic
(lacking oxygen) conditions. With oxygen
present, the irradiation injury to the cells
was greater than when optimum levels of
21-02
Splice Bushing
QBIF600-VIS-NIR
FOXY-R
Overview
The FOXY Sensor has been used for
other hypoxia experiments, including an
application where clinicians determine
how much of a diseased human limb
targeted for amputation can be saved;
the presence of oxygen correlates to
tissue health. Monitoring dissolved
oxygen in both human and animal tissue
is a common application for the FOXY
Sensor, which offers the advantages of
being minimally invasive, not consuming
the sample, and working well in viscous
media.
Ultimately, the cellular hypoxia
researchers determined that oxygen
measurements of the cellular
environment made with the FOXY Sensor
matched the predicted hypoxic saturation
values, depending on the amount and
duration of nitrogen flushed through the
sample chamber. The FOXY Sensor
proved to be a valuable tool in
confirming the desired level of hypoxia.
Oxygen is sensed by measuring the decrease in fluorescence intensity of a
fluorophore bound to the tip of an optical fiber. The sensor responds to the partial
pressure of oxygen in gases, liquids and even viscous samples.
Spectrometer
Used with Ocean Optics Fiber Optic Oxygen Sensors and custom probes, the
MultiFrequency Phase Fluorometer (MFPF), manufactured by TauTheta, is a flexible
platform for measurement of luminescence lifetime, phase and intensity. This
frequency-domain luminescence monitor uses LED excitation and avalanche
photodiode detection with filter-based wavelength selection for easy experimental
set-up and control. The MFPF is especially useful for oxygen sensing applications
where sensitivity to drift is important and where sample set-ups must be undisturbed
for long periods of time. Because it utilizes phase-shift technology, it is invariant to
fiber bending and stray light, has a wide dynamic range of optical intensity, and
has low optical and electronic crosstalk as well as low drift and phase noise.
Resources
hypoxia (~90%) were reached. To induce
hypoxia, and thus mitigate any oxygenenhancement injury, the cells were
gassed with nitrogen. This hypoxia was
confirmed with a FOXY Fiber Optic
Oxygen Sensor and a USB2000
Spectrometer.
Sampling Optics
The MFPF is embedded with LED excitation sources and transmits light at ~475 nm
to one leg of a QBIF600-VIS-NIR Bifurcated Optical Fiber Assembly. The bifurcated
assembly connects to the oxygen sensor probe via a 21-02 SMA Splice Bushing. If
the excited formulation at the probe tip encounters an oxygen molecule, the
fluorescence signal decreases. The fluorescence is collected by the probe and is
transmitted to the spectrometer via the other leg of the bifurcated assembly.
OOISensors Software calculates partial pressure of the oxygen from this signal. For
more on sensor operation, see page 65.
Components
Page
Price
67
$5,000
QBIF600-VIS-NIR Premium-grade Bifurcated Fiber Assembly
72
$369
21-02 Splice Bushing
72
$13
4.
FOXY-R Fiber Optic Oxygen Sensor Probe
71
$499
5.
OOISensors Software
75
$199
6.
ASP Annual Service Package
62
$250
1.
MFPF100-1 MultiFrequency Phase Fluorometer
2.
3.
Total:
Tel: 727.733.2447 • Email: [email protected]
$6,330
169
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Volcano Emissions
Setup: Gas Absorbance
HR4000
D2000
For example, on the Caribbean island of
Montserrat, researchers use three S2000
Spectrometers to collect UV absorbance
(from 245-380 nm) of SO2 in gas
emissions. The spectrometers are set up
at three plume sites, each of which is
about 3.5 km from the volcano's dome.
The spectrometers are small, making
them simple to transport and deploy at
the volcano site. The entire setup costs
less than $10,000, within most budget
limits and almost "disposable" (this is a
volcano, after all).
QP400-2-UV-VIS
CUV-UV-10
QP400-2-UV-VIS
Overview
Resources
Active volcanoes emit various gases
including sulphur dioxide (SO2), a
colorless, pungent gas that can irritate
the skin and the mucous membranes of
the eyes, nose and throat. Volcanologists
regularly monitor SO2, which absorbs in
the UV.
Absorbance measurements are used to quantify the concentration of solutions
and gases (as described here) that absorb light in a media that transmits light.
The signal in absorbance units is proportional to the molar absorptivity,
pathlength and concentration of the sample. (See more on Beer’s Law on
page 178.)
The Montserrat researchers configured a
system that makes efficient use of lightcollection optics and provides good
optical resolution (~3.5 nm FWHM).
Each spectrometer is connected to a
1000 µm optical fiber, which screws into
a telescope mount.
Spectrometer
A setup for measuring benzene gas, for example, would call for an HR4000
High-resolution Spectrometer with an H7 grating and a 200-300 nm wavelength
range. Optical bench accessories include an L4 Detector Collection Lens for
increased light throughput, and a UV4 Detector Upgrade to transmit light in the
UV. With a 5 µm slit, optical resolution of ~0.07 nm (FWHM) is possible. The
preferred light source for work in the ultraviolet is the D2000 Deuterium Light
Source.
Sampling Optics
The 10-cm pathlength CUV-UV-10 Cuvette Holder, the CV-Q-10 Cylindrical Cell
and QP400-025-SR Premium-grade Solarization-resistant Optical Fibers (one
fiber illuminates, the other reads signal) comprise the system’s sampling optics.
For applications requiring shorter pathlengths or open-air monitoring (see
sidebar), use an optical fibers-and-collimating lenses configuration.
Components
1.
Page
Price
21
$3,999
Grating H7, 2400 lines per mm, 200-300 nm range
23
included
5 µm Slit as entrance aperture
22
$150
L4 Detector Collection Lens
24
$150
HR4000 High-resolution Spectrometer
DET4-UV Detector with UV4 Detector Upgrade
24
126
D2000 Deuterium Light Source
3.
CUV-UV-10 Cuvette Holder
90
$549
4.
CV-Q-100 Cylindrical Cell
93
$165
5.
(2) QP400-2-UV-VIS Premium-grade Patch Cord Assemblies
142
$338
6.
SpectraSuite Spectroscopy Operating Software
80
$199
7.
ASP Annual Service Package
62
Total:
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$150
2.
170
$2,172
$250
$8,122
For all your sensing needs, visit OceanOptics.com
At the Montserrat Volcano Observatory
(www.mvo.ms) sampling sites, spectra are
collected every 4-6 seconds and
transmitted to researchers at the
observatory via modem; one complete
scan of the plume takes 4-6 minutes.
Depending on wind direction, data from
two of the three spectrometers is used to
calculate plume height, by comparing the
angles at which peaks in the SO2 plume
are measured.
All That Glitters . . .
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Setup: Fluorescence
By some accounts, fluorescence of
minerals has been observed for more
than a century. For early miners,
fluorescence of minerals such as calcite
helped to target drilling operations to the
richest bodies of ore. For amateur
geologists, mineral fluorescence is a
more esoteric pursuit: samples that
fluoresce simply look really cool.
USB4000-FL
PX-2
Consider genthelvite, an opaque mineral
that fluoresces bright green under UV
radiation and remains phosphorescent
for a short period. In 2003, mineralogists
Earl Verbeek and Herb Yeates measured
fluorescence of both genthelvite and
willemite (another fluorescent mineral)
found in deposits at a site in New Jersey.
QP1000-2-UV-VIS
LVF and LVF-CUV-ADP
(part of LVF-UV-KIT)
CUV-ALL
R400-7-VIS-NIR
Overview
Fluorescence measurements require a sensitive detector and an effective filter for
discriminating between powerful excitation source wavelengths and weak spectral
emissions from the sample.
Spectrometer
We offer several spectrometers useful for fluorescence, but recommend the highsensitivity, preconfigured USB4000-FL Spectrometer for most general fluorescence
applications. The USB4000-FL is set to 360-1000 nm and comes with a 200-µm slit
and an L4 Detector Collection Lens for increased light throughput.
Sampling Optics
Your standard excitation source option is our PX-2 Pulsed Xenon Source. Our
proprietary LVF Linear Variable Filters are excellent tools for spectrally shaping the
excitation energy from broadband sources used for fluorescence. Various sampling
optics are available for detecting picomolar-range concentrations of fluorophores
from surfaces and in solutions and powders.
Spectrometer Components
Spectrometer integration times were set
for 1000 ms to measure the dim
(although visible to the naked eye)
genthelvite fluorescence, compared with
a 10 ms integration to measure the
brighter willemite fluorescence.
1.
Page
Price
46
$2,499
200 µm Slit as entrance aperture
15
included
Grating #3, 380-1000 nm range
16
included
L4 Detector Collection Lens
17
included
SAG+UPG Mirrors
16
$250
Page
Price
USB4000-FL Spectrofluorometer
Components for Use with Solutions
To ensure that the light emitted from the
samples came from the minerals
themselves, Verbeek and Yeates
measured the samples in a light-tight
enclosure and filtered out excitation
source wavelengths and ambient light.
Why does genthelvite fluoresce? Verbeek
and Yeates identified the source as
divalent manganese -- a substitute for
zinc in the genthelvite structure that is
also responsible for the color in amethyst.
2.
PX-2 Pulsed Xenon Source
3.
CUV-ALL-UV 4-way Cuvette Holder
4.
LVF-UV-KIT Linear Variable Filter Kit
114
$999
6.
(2) QP1000-2-UV-VIS Premium-grade Patch Cord Assemblies
142
$718
7.
(2) 74-MSP Mirrored Screw Plugs
90
$198
8.
SpectraSuite Spectroscopy Operating Software
80
$199
Page
Price
Components for Use with Solids
127
$769
90
$809
2.
PX-2 Pulsed Xenon Source
127
$769
3.
R400-7-VIS-NIR Reflection/Backscattering Probe
148
$499
4.
SpectraSuite Spectroscopy Operating Software
80
$199
Tel: 727.733.2447 • Email: [email protected]
171
Resources
In a paper submitted to the FranklinOgdensburg Mineralogical Society,
Verbeek and Yeates described using a
USB2000-VIS-NIR Spectrometer (3501000 nm), a high-power UV excitation
source and a 600 µm probe to observe
emission peaks of 511 nm for genthelvite
and 528 nm for willemite.
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QC of LED Curing Lights
Setup: LED Analysis
High-output LEDs may be a viable
alternative to other light sources for
curing ceramic materials used in
dentistry, according to researchers from
the University of Manchester in England.
USB4000
As researchers Adrian Bennett and David
Watts suggested in a 2003 article
submitted to the journal Dental Materials,
LEDs have longer lifetimes, are less prone
to degradation and temperature effects,
and require less power than tungsten
halogen curing units.
QP400-2-VIS-NIR
FOIS-1
LED-PS
LS-1-CAL-INT
Overview
To measure the absolute spectral intensity and color of LEDs, specify the
configuration described here or see page 56.
Resources
Spectrometer
We suggest a USB4000 Spectrometer with a 25 µm Slit and Grating #2
(350-1000 nm). An L4 Detector Collection Lens increases light-collection efficiency
and reduces stray light. An OFLV-350-1000 Order-sorting Filter eliminates secondand third-order effects. This optical bench configuration maximizes system sensitivity,
mitigating the light loss inherent with use of an integrating sphere -- the sampling
optic of choice for most LED applications. (You also can collect LED signal with a
CC-3-UV Cosine Corrector and fiber.)
Sampling Optics
The LED is mounted in the NIST-traceable LED-PS-NIST LED Power Supply, which
provides a white background for the LED and a controlled drive current to
characterize LED output. The FOIS-1 Integrating Sphere is placed over the
LED-PS-NIST and collects the LED output. The attached optical fiber collects the light
energy from the LED and transmits it to the spectrometer. The power and color of
the LED is determined by comparing the LED to a radiant standard -- the
LS-1-CAL-INT Calibrated Source, which fits into the sample port of the FOIS-1.
SpectraSuite Spectroscopy Operating Software calculates absolute irradiance and
spectral features such as dominant, central and centroid wavelength; hue, chroma
and saturation, X,Y,Z; L*, a*, b*; xyz; u’v’w’; CCT and more.
Components
1.
Page
Price
USB4000 Plug-and-Play Spectrometer
14
$2,199
Grating #2, 350-1000 nm range
16
included
25 µm Slit as entrance aperture
15
$150
L4 Detector Collection Lens
17
$150
17
$150
2.
LS-1-CAL-INT Tungsten Halogen Calibrated Light Source
DET4-350-1000 Detector with OFLV-350-1000 Order-sorting Filter
133
$749
3.
LED-PS LED Power Supply
104
$499
4.
FOIS-1 Integrating Sphere for Emission
105
$499
5.
QP400-2-VIS-NIR Premium-grade Patch Cord Assembly
142
$169
6.
SpectraSuite Spectroscopy Operating Software
80
$199
7.
ASP Annual Service Package
62
Total:
oo
172
$250
$5,014
For all your sensing needs, visit OceanOptics.com
To assess LED performance, Bennett and
Watts used a radiometrically calibrated
USB2000 Spectrometer to measure the
absolute spectral output and irradiance of
three LED curing units. The spectrometer
was radiometrically calibrated using the
LS-1-CAL Tungsten Halogen Light Source;
a FOIS-1 Integrating Sphere collected the
LED output and funneled it to an optical
fiber coupled to the spectrometer. The
spectral range of the LEDs also was
measured.
By most criteria, Bennett and Watts
concluded, the LED curing units
compared favorably with the tungsten
halogen curing units. However, longer
curing times may be necessary with LEDs,
which have lower irradiance than the
tungsten halogen sources.
Similar studies also have been performed
at the Indiana University School of
Dentistry.
Whatever their ultimate application, LEDs
can be analyzed for color and absolute
spectral intensity very easily and
inexpensively with Ocean Optics
spectrometers and accessories.
Laser Plume Analysis
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Setup: Laser Analysis
Ocean Optics spectrometers and
accessories are useful tools for measuring
the spectral output and power of lasers,
with configurations as simple as the setup
shown at right.
HR4000
But we also provide components for
applications involving what happens after
the laser fires. Consider laser welding,
which is now common to a number of
industries. An Ocean Optics customer
has used our PC Plug-in Spectrometer
and an optical fiber to measure the
plume created by a CO2 laser used in
welding metals such as copper and
stainless steel alloys. Researchers were
particularly interested in the processes
related to welding of dissimilar materials.
QP400-2-VIS-NIR
FOIS-1
Optical Post
Optical Post
Overview
Our HR4000 High-resolution Spectrometer is ideal for measuring the spectral
characteristics and intensity of continuous-wave and pulsed lasers. For high-power
lasers, an integrating sphere or cosine corrector attenuates the light to avoid
saturating the CCD array.
The HR4000 Spectrometer uses the “HR” Optical Bench, which was designed to
yield high optical resolution for resolving fine spectral features. For laser
characterization, we recommend a grating with a high groove density, such as the
H6 1200 mm-1 grating set to a 750-925 nm wavelength range and with a 5 µm
Slit as the entrance aperture. This configuration provides ~0.12 nm resolution
(FWHM). For better resolution consider an 1800 mm-1 or 2400 mm-1 grating.
Resources
Spectrometer
Sampling Optics
By measuring the concentration of
elements within the laser weld plume, as
well as the plume temperature, the
researchers were able to determine the
efficiency of the weld. Species
identification is useful in controlling the
welding of dissimilar alloys; plume
temperature can be correlated to laser
power and speed.
There are several possible sampling setups: a CC-3-UV Cosine Corrector with an
optical fiber; FOIS-1 Integrating Sphere with a fiber; or fiber assembly coupled to
the laser. Optical posts are used to hold fixtures in place.
Measurements
Our operating software can detect the laser wavelength peak; SpectraSuite
Spectroscopy Operating Software obtains peak, centroid and central wavelength
values, and full-width half-maximum values.
Components
1.
The UV-VIS spectrometer used in the
study had a wavelength range of
263-523 nm. One leg of a bifurcated
optical fiber carried light from a diode
laser to the weld site; the other leg
sampled the plume emission.
Ultimately, real-time monitoring of the
laser weld plume makes it far simpler to
correct process problems before large
numbers of parts are affected. This
increases manufacturing yields and
speeds up inspection processes.
Page
Price
21
$3,999
Grating #H6, 750-925 nm range
23
included
5 µm Slit as entrance aperture
22
$150
DET4-VIS Detector
24
Free
105
$499
HR4000 High-resolution Spectrometer
2.
FOIS-1 Integrating Sphere for Emission
3.
OPM-3 Three-inch Optical Post (2)
4.
QP400-2-VIS-NIR Premium-grade Patch Cord Assembly
5.
6.
89
$30
142
$169
SpectraSuite Spectroscopy Operating Software
80
$199
ASP Annual Service Package
62
Total:
Tel: 727.733.2447 • Email: [email protected]
$250
$5,296
173
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LIBS for Defense
Setup: LIBS
In an earlier LIBS application, closely
related spores of the genus Bacillus were
deposited on silver membrane filters for
analysis using broadband Laser-induced
Breakdown Spectroscopy (LIBS). The
observed spectral differences among the
spores -- Bacillus subtilis, Geobacillus
stearothermophilus and Bacillus
pumilus -- provide evidence of the power
of Ocean Optics’ Laser-induced
Breakdown Spectrometer in resolving
complex biological samples.
LIBS-LASER
LIBS2500
LIBS-LASER
power supply
LIBS-SC
LIBS-FIBER-BUN
Overview
Resources
The LIBS2500 Broadband Spectrometer is a detection system for real-time elemental
analysis in solids, solutions and gases. This high-resolution system provides full
spectral analysis from 200-980 nm, with optical resolution of ~0.1 nm (FWHM).
Principle of Operation
An Nd:YAG pulsed laser beam is focused on the sample area. The energy of the
laser generates a plasma, in which a trace amount of the sample has been ablated.
As the plasma decays or cools, the plasma emits light of wavelengths that are
distinct to each element. The emission is collected by a 7-fiber bundle and sent to
the spectrometers for analysis.
Spectrometers
The LIBS2500-7 uses seven high-resolution spectrometers, which connects to a PC
via one USB port. All seven spectrometers acquire data simultaneously; software
displays the results. However, you may require a system with less than seven
spectrometer channels. See page 48 for options on all LIBS2500 Systems.
Sampling Optics
The LIBS-LASER is a 50 mJ CFR Nd:YAG laser for metal and thin film samples and
sells for $14,500. The LIBS-LAS200MJ is a 200 mJ CFR Nd:YAG laser for most all
other materials and is priced at $22,500. Both lasers are manufactured by Big Sky
Laser. The LIBS-SC Sample Chamber has a manual x-y-z stage and a remote laser
safety lock. Signal is collected by a fiber bundle comprising (7) 600 µm UV-VIS
patch cords, each with a collimating focusing lens built into the fiber termination.
Measurements
OOILIBS Software allows users to set operating parameters such as the laser
Q-switch delay (the time between the firing of the laser and the beginning of
spectral acquisition) and signal averaging of laser pulses.
Components
Page
LIBS2500-7 7-Channel Laser-induced Breakdown Spectrometer
48
2.
LIBS-BUN-7 Optical Fiber Bundle
48
$985
3.
LIBS-LASER Nd:YAG 50 mJ Laser (from Big Sky Laser)
49
$14,500
4.
LIBS-SC Sample Chamber
49
$9,800
5.
OOILIBS Software
48
Total:
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Price
1.
174
$29,999
$500
$55,784
For all your sensing needs, visit OceanOptics.com
The presence of the spores’ unique
spectral lines, as well as different
combinations of spectral lines, provide
many opportunities for discrimination.
While most of the unique peaks occurred
in the G. stearothermophilus spectrum,
spectral differences were observed in the
spectra for all the spores. Spore
characteristics such as surface profile and
coat mineralization may account for these
differences.
The results reported for the Bacillus
spores, along with others obtained for
biological molecules including nucleic
acids and proteins, provide exciting
evidence of the discriminating capability
of our LIBS system. In fact, we are now
collaborating with others to develop a
man-portable LIBS system for field
detection of chemical and biological
warfare agents. The system will be able
to make a complete analysis every one to
two seconds, be small enough to carry in
a backpack, and require very little power
to operate.
Product developer Thickness Detection
Systems (TDS) of Salt Point, N.Y., has
integrated an Ocean Optics multichannel
spectrometer into a broadband
dissolution rate monitor (DRM) for
analyzing very thin resist films used in the
semiconductor and optics industries.
USB4000-VIS-NIR
DRMs help to determine the thickness of
thin film layers and the rate at which the
film resist material dissolves -- important
parameters in controlling thin film
production processes. In its initial testing,
Thickness Detection Solutions focused on
applications involving films of <300 nm
thickness, where existing monochromatic
and polychromatic interferometric testing
methods have had limited effectiveness.
STAN-SSH
RPH-1
R400-7-VIS-NIR
Overview
A thin film on a substrate can act as an etalon, creating an interference pattern
superimposed on the surface reflectivity when viewed in reflection. The spacing of the
pattern’s sinusoidal peaks, when combined with the refraction index of the material,
can be used to calculate the thickness of the material.
Spectrometer
The USB4000-VIS-NIR (350-1000 nm) is ideal for reflectometry of thin films. The
spectrometer is preconfigured with Grating #3, which is blazed at 500 nm; an
OFLV-350-1000 Filter to eliminate second- and third-order effects; and a 25 µm slit
for optical resolution of ~1.5 nm (FWHM).
Sampling Optics
The R400-7-VIS/NIR Reflection
Probe positioned at 90°
measures specular reflectance
from surfaces such as thin films.
An LS-1 Tungsten Halogen Lamp
and a STAN-SSH High-reflectivity
Specular Reflectance Standard
complete the sampling setup.
Measurements
Today, TDS offers 1-, 2-, 4- and 8channel configurations. TDS just recently
announced the commercial release of its
L-Series DRM product line for photoresist
R&D, formulation studies, photoresist
manufacturing QC, and polymer resin
manufacturing QC.
The L-series line includes multiwavelength
and multilayer analysis algorithms, which
enable discrete thickness measurements
to zero film thickness and provide
accurate data of non-linear dissolution
rate phenomena. For more details, visit
www.thicknessdetection.com.
LS-1
Interference Pattern of Thin Film
Resources
In testing, TDS used an SD2000 Dualchannel Spectrometer. Reflection
measurements were performed with an Rseries Reflection Probe. As TDS reports on
its website, results indicated that multiwavelength DRMs would be able to
determine film thicknesses at discrete
time intervals, to monitor photoresist
phenomena that are difficult to separate
with traditional DRMs, and to provide
additional value to the researcher “by
eliminating the need for discrete, static
optical thickness measurement tools.”
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Setup: Metrology
80
REFLECTIVITY (%)
Thin Film Thickness
70
60
50
40
375
475
575
675
775
875
WAVELENGTH (nm)
Spectra observed in our
operating software (see above) reveal oscillations caused by optical interference
within the layers of the thin film substrate. Analysis of the wavelength position of the
minima or maxima can determine either the thin film’s thickness (with the known
refractive index of the film) or its refractive index (with the known film thickness).
Keep in mind that the thickness of samples may not be uniform; we recommend
measuring several locations on the film.
Components
1.
Page
Price
34
$2,499
Grating #3, 600 lines per mm, blazed at 500 nm
16
included
25 µm Slit as entrance aperture
15
included
DET4-350-1000 Detector with OFLV-350-1000 Order-sorting Filter
17
included
USB4000-VIS-NIR General-purpose Spectrometer
2.
LS-1 Tungsten Halogen Light Source
128
$499
3.
R400-7-VIS-NIR Reflection/Backscattering Probe
148
$499
4.
RPH-1 Reflection Probe Holder
157
$75
5.
STAN-SSH High-reflectivity Specular Reflectance Standard
108
$499
Total:
Tel: 727.733.2447 • Email: [email protected]
$4,071
175
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Plants and Reflectance
Setup: UV-VIS Reflection
Spectral reflectance measurements of
fruits, vegetables and other plants have
long been performed using Ocean Optics
spectrometers, light sources and fiber
optic probes, with applications in the lab
and in the field.
USB4000-UV-VIS
DH2000-BAL
For example, researchers at the University
of Arkansas at Little Rock have measured
spectral reflectance of rice seedlings
(pictured) in relation to soil salinity and to
the chlorophyll content of individual rice
leaves -- two factors related to rice yield.
The experiment setup included an S2000
Spectrometer, LS-1 Tungsten Halogen
Light Source and R-series Fiber Optic
Reflection Probe.
RPH-1
R400-7-UV-VIS
Overview
Resources
Diffuse reflection measurements can be used to determine information about the
chemical content or color (see page 177) of a sample.
Spectrometer
The USB4000-UV-VIS (200-850 nm) is ideal for most UV-VIS reflectometry. The
spectrometer is preconfigured with Grating #1, which is efficient in the deep UV;
an OFLV-200-850 Order-sorting Filter to eliminate second- and third-order effects;
and a 25 µm slit for optical resolution of ~1.5 nm (FWHM).
Sampling Optics
The R400-7-UV-VIS Reflection Probe measures diffuse or specular reflectance from
surfaces, or backscattering from translucent materials and fluids. The RPH-1 Probe
Holder positions the R400-7 at either 45° for diffuse reflection or 90° for specular
reflection. (For reflection measurements with an integrating sphere, see page 106.)
For illumination, we recommend the DH2000-BAL Deuterium Tungsten Halogen
Light Source. If your application requires portability, use the smaller DT-MINI-2
Deuterium Tungsten Halogen Light Source. (Because the DT-MINI-2 is a low-power
source, configure your spectrometer with a 50 µm Slit and an L4 Detector
Collection Lens.)
Measurements
Reflectance standards include the WS-1 Diffuse Reflectance Standard (page 107)
for diffuse measurements and the STAN-SSH Specular Reflectance Standard (page
108) for specular measurements. Use our software to correct data for deviations
from 100% reflectivity of standards, field tiles or NIST-traceable materials.
Components
1.
Page
Price
34
$2,649
Grating #1, 200-850 nm range
16
included
25 µm Slit as entrance aperture
15
included
DET4-200-850 Detector with OFLV-200-850 Order-sorting Filter
17
included
USB4000-UV-VIS General Lab Spectrometer
2.
DH2000-BAL Deuterium Tungsten Halogen Light Source
122
$3,588
3.
R400-7-UV-VIS Reflection Probe
148
$499
4.
RPH-1 Reflection Probe Holder
157
5.
SpectraSuite Spectroscopy Operating Software
80
$199
6.
ASP Annual Service Package
62
$250
Total:
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One of our favorite plant applications is
a high school science fair-winning project
covering similar territory. Then-student
Naomi Levine used one of our old S1000
Spectrometers, a tungsten halogen
source, and a fiber optic probe to
measure the reflection at 90° of
philodendron plant leaves. Naomi
believed that correlating reflectance to
fertilization levels could be useful in
detecting over-fertilization in crops.
What Naomi discovered was that plant
reflectance at wavelengths >700 nm was
insensitive to the stress of over-fertilization
(samples were fertilized at 4x the
recommended amount), while the peak
within the 530-630 nm range was
noticeably sensitive to stress (manifest as
increased leaf reflection). She concluded
that the latter related to a decrease in
chlorophyll and to the effects of osmosis.
Osmosis caused water to collect between
the cell membrane and cell wall and
exposed more of the leaf surface, thus
increasing reflectance.
$75
$7,260
For all your sensing needs, visit OceanOptics.com
As for Naomi, she graduated from
Princeton University in 2003.
Nice Asp!
No, it’s not an asp, but we couldn’t resist.
Dr. Ted Rohr -- a wildlife biologist and
lecturer at RMIT University in Melbourne,
Australia -- is actually holding an
Australian Copperhead, which is one of
the most venomous snakes in the world.
USB4000
The Australian Copperhead is a frontfanged snake restricted to the cooler
parts of Southeastern Australia. It preys
on frogs, lizards, snakes and
small mammals.
Rohr is studying the capacity of these
snakes to undergo rapid color change -from several shades of brown or green to
black -- on the dorsal surface. Using a
USB2000 Spectrometer and a fiber optic
probe with a custom shield on its end
(the shield helps to maintain a fixed
distance to the sample point of interest),
Rohr measured the reflectance of
individual snake scales, both in the field
and in the laboratory.
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Setup: Reflected Color
LS-1
P400-2-VIS-NIR
ISP-REF
RPH-1
WS-1
R400-7-VIS-NIR
Overview
Spectrometer
A USB4000 with a 25 µm Slit and Grating #2 (350-1000 nm) works well for color
analysis. For those using an integrating sphere as the sampling optic, we
recommend an L4 Detector Collection Lens to improve sensitivity.
Resources
Color measurement involves determining the reflection spectrum of a sample and
applying it to a standard illuminant. The amount of light energy the sample reflects
is manipulated and reduced to tristimulus values X, Y and Z. These values
correspond to the physiological response of the three types of color receptors in the
human eye. X, Y and Z values are combined into uniform colorspace values such as
L*, a* and b*.
Sampling Optics
When taking reflective-color measurements, your data depends on sampling
geometry. The R400-7-VIS-NIR Reflection Probe provides illumination and detection
from the same direction. If you use the probe at a 45°, it measures diffuse
reflection. If you use the probe at a 90°, it measures specular reflection. The
distance from the probe to the surface determines the sample size. An alternative is
the ISP-REF Integrating Sphere, which provides 180° illumination and detection from
flat surfaces for measuring specular and diffuse reflection.
Measurements
According to Rohr, the snake’s ability to
change body color makes sense in a
cool-temperate environment, where
thermal conditions can change many
times during the season and even
throughout the day. Changing colors is a
perfect mechanism for adapting to
fluctuations in temperature. However,
body coloration is also important for
camouflage. Being black may be great in
order to absorb solar radiation, but it
makes the snake more obvious to birds
of prey -- and wary researchers!
Reflectivity is measured against a reference standard such as the WS-1 Diffuse
Reflectance Standard. SpectraSuite Spectroscopy Operating Software calculates a
variety of colorspace values from the reflection spectra.
Components for Color Measurements
1.
Page
Price
USB4000 Plug-and-Play Spectrometer
14
$2,199
Grating #2, 350-1000 nm range
16
included
25 µm Slit as entrance aperture
15
$150
L4 Detector Collection Lens
17
$150
17
$150
DET-4-350-1000 detector with OFLV Order-sorting Filter
2.
WS-1 Diffuse Reflectance Standard
107
3.
SpectraSuite Spectroscopy Operating Software
$299
80
$199
4.
5.
LS-1 Tungsten Halogen Light Source
128
$499
R400-7-VIS-NIR Reflection Probe
149
$499
6.
RPH-1 Reflection Probe Holder
157
7.
ASP Annual Service Package
62
Total:
Tel: 727.733.2447 • Email: [email protected]
$75
$250
$4,470
177
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Beer’s Law
Spectral Identity
It’s not uncommon for our customers to be unfamiliar with the absorbing or
emitting wavelength or wavelength range of their analytes. In the next few pages,
we’ve provided absorbance and emission data for many analytes. Our Applications
Scientists are another good resource for this information -- after all, we’ve
configured nearly than 85,000 spectrometers -- as are Internet searches and
commercial ventures specializing in spectral data.
Absorption Wavelength Bands for Chromophores
Resources
Chromophore
System
Max. Absorption
in nm
Acetylide
—C≡C—
175-180
6 000
Aldehyde
—CHO
210
strong
280-300
11-18
Amine
—NH²
Azido
Azo
>C=N—
195
190
2 800
5 000
—N=N—
285-400
3-25
Bromide
—Br
208
300
Carbonyl
>C=O
195
1 000
270-285
18-30
Carboxyl
—COOH
200-210
50-70
Disulfide
—S—S—
194
5 500
255
400
Ester
—COOR
205
50
Ether
—O—
185
1 000
Ethylene
—C=C—
190
8 000
Iodine
—I
260
400
Nitrate
—ONO²
270 (shoulder)
12
Nitrile
—C≡N
160
—
Nitrite
—ONO
220-230
1 000-2 000
10
strong
—NO²
210
Nitroso
—NO
302
100
Oxime
—NOH
190
5 000
Sulfone
—SO²—
180
—
Sulfoxide
>S=O
210
1 500
Thiocarbonyl
>C=S
205
strong
Thioether
—S—
194
4 600
—SH
—(C=C)²— (acrylic)
1 600
195
1 400
210-230
21 000
260
35 000
—(C=C)4—
300
52 000
—(C=C)²— (alicyclic)
330
118 000
230-260
3 000-8 000
C=C—C≡ C
219
6 500
C=C—C=N
220
23 000
C=C—C=O
210-250
10 000-20 000
C=C—NO²
Benzene
215
—(C=C)³—
—(C=C)5—
300-350
weak
229
9 500
184
46 700
204
6 900
255
170
Diphenyl
246
20 000
Naphthalene
222
112 000
275
5 600
Anthracene
178
300-400
Nitro
Thiol
oo
Absorb. Intensity
312
175
252
199 000
375
7 900
For all your sensing needs, visit OceanOptics.com
Beer-Lambert Law, more commonly known
as Beer’s Law, states that the optical
absorbance of a chromophore in a
transparent solvent varies linearly with
both the sample cell pathlength and the
chromophore concentration. Beer’s Law is
the simple solution to the more general
description of Maxwell’s far field equations
describing the interaction of light with
matter. In practice Beer’s Law is accurate
enough for a range of chromophores,
solvents and concentrations, and is a
widely used relationship in quantitative
spectroscopy.
Absorbance is measured in a spectrophotometer by passing a collimated beam of
light at wavelength λ through a plane
parallel slab of material that is normal to
the beam. For liquids, the sample is held
in an optically flat, transparent container
called a cuvette. Absorbance (A λ ) is
calculated from the ratio of light energy
incident passing through the sample
(I 0) to the energy that is incident on the
sample (I):
Aλ = -log (I/I 0 )
Beer’s Law follows:
Aλ = ελbc
ελ = molar absorptivity or extinction
coefficient of the chromophore at
wavelength λ (the optical density of a
1-cm thick sample of a 1 M solution).
ελ is a property of the material and
the solvent.
b = sample pathlength in centimeters
c = concentration of the compound in
the sample, in molarity (mol L-1)
In an absorbance experiment, light is
attenuated not only by the chromophore,
but also by reflections from the interface
between air and the sample, the sample
and the cuvette, and absorbance by the
solvent. These factors can be quantified
separately, but are often removed by
defining I 0 as the light passing through a
sample “blank” or “baseline” or reference
sample (for example, a cuvette filled with
solvent but zero concentration of the
chromophore is used as the blank).
Many factors can affect the validity of
Beer’s Law. It is usual to check for the
linearity of Beer’s Law for a chromophore
by measuring the absorbance of a series
of standards. This “calibration” can also
remove errors in the experiment, the
equipment and the batch of reagents
(such as cuvettes of unknown pathlength).
Determining
Optical Resolution
The optical resolution, measured as Full
Width Half Maximum (FWHM), of our
spectrometers depends on the groove
density of the grating and the width of
the entrance aperture (slit width or fiber
diameter).
In selecting these components, consider
two trade-offs. First, the optical resolution
improves as the groove density of the
grating increases, but at the expense of
spectral range and signal strength.
Second, the resolution improves as the
slit width or diameter of the fiber
decreases, but at the expense of signal
strength. The formula for calculating the
optical resolution follows:
Step 2
Choose a Slit. See the table below to find
the page on slit choices for your
spectrometer. Note the value in the Pixel
Resolution column in the slit chart.
Multiply the Dispersion (nm/pixel value
from Step 1) x Pixel Resolution of your
entrance aperture. This is your Optical
Resolution (in nm).
Absorption Wavelength Bands for Chromophores
Chromophore
Absorb. Intensity
251
66 000
Phenanthrene
292
14 000
Naphthacene
272
180 000
473
12 500
Pentacene
310
300 000
585
12 000
Pyridine
174
80 000
195
6 000
Quinoline
Isoquinoline
257
1 700
227
37 000
270
3 600
314
2 750
218
80 000
266
4 000
317
3 500
Absorption Wavelength Cutoffs for Solvents*
Solvent
Wavelength
Solvent
Wavelength
Acetic Acid
260
Hexadecane
Acetone
330
Hexane
210
Acetonitrile
190
Isobutyl alcohol
230
Benzene
280
Methanol
210
1-Butanol
210
2-Methoxyethanol
210
2-Butanol
260
Methylcyclohexane
210
Butyl acetate
254
Methylene chloride
235
Carbon disulfide
380
Methyl ethyl ketone
330
200
Carbon tetrachloride
265
Methyl isobutyl ketone
335
1-Chlorobutane
220
2-Methyl-1-propanol
230
Chloroform (stabilized
245
with ethanol)
Example
Here is an example of how to calculate
optical resolution of a USB4000
Spectrometer using Grating #3 and a
10- µm slit. With this data, you can
obtain the approximate optical resolution.
Step 1 650 nm ÷ 3648 = 0.178
Step 2 0.178 x 5.7 = 1.015 nm
FWHM = ~1.02 nm
Max. Absorption
in nm
N-Methylpyrrolidone
285
Nitromethane
380
Cyclohexane
210
Pentane
210
1,2-Dichloroethane
226
Pentyl acetate
212
Diethyl ether
218
1-Propanol
210
1,2-Dimethoxyethane
240
2-Propanol
210
N,N-Dimethylacetamide
268
Pyridine
330
N,N-Dimethylformamide
270
Tetrachloroethylene
290
Dimethylsulfoxide
265
(stabilized with thymol)
1,4-Dioxane
215
Tetrahydrofuran
Ethanol
210
Toluene
286
2-Ethoxyethanol
210
1,1,2-Trichloro-1,2,2-
231
220
Finding Your Values
Ethyl acetate
255
trifluoroethane
Spectrometer
Ethylene chloride
228
2,2,4-Trimethylpentane
Glycerol
207
o-Xylene
290
Heptane
197
Water
191
USB2000:
USB4000:
HR2000:
HR2000+:
HR4000:
QE65000:
NIR-512:
NIR256-2.1:
NIR256-2.5:
Grating
Entrance Aperture
Spectral Range Pixel Resolution
website
website
page 16
page 15
website
website
page 23
page 22
page 23
page 22
page 28
page 27
pages 32
page 32
pages 32
page 32
pages 32
page 32
Resources
Step 1
Choose a Grating from the Grating
Selection Chart. See the table below to
locate the page for the grating choices
for your spectrometer. Note the value in
the Spectral Range column in the chart.
Check the number of pixel elements in
the spectrometer’s detector. Divide the
Grating’s Spectral Range by the total
number of Detector Elements in the
detector. This is your Dispersion.
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Spectral Identity
215
* Solvents are transparent at wavelengths greater than the stated cutoff.
Tel: 727.733.2447 • Email: [email protected]
179
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Non-linearity & CCDs
Spectral Identity
Absorption/Emission for Fluorophores
Fluorophore
Absorption in nm
1,5 IAEDANS
336
490
4-Methylumbelliferone
385
502
512/598
563/668
542
568
6-Carboxyrhodamine 6G
518
543
6-CR 6G
518
543
6-JOE
520
548
7-Amino-4-Methylcoumarin
351
430
7-Aminoactinomycin D (7-AAD)
546
647
7-Hydroxy-4-methylcoumarin
360
449,455
Acridine Orange +DNA
502
526
Alexa Fluor 350™
346
442
5-Carboxynapthofluorescein
Emission in nm
(pH 10)
5-Carboxytetramethylrhodamine
Resources
(5-TAMRA)
342
441
Alexa Fluor 430™
431
540
Alexa Fluor 488™
495,492
519,520
Alexa Fluor 532™
531,532
553,554
Alexa Fluor 546™
556,557
572,573
Alexa Fluor 568™
577,578
603
Alexa Fluor 594™
590,594
617,618
Alexa Fluor 633™
632
650
Alexa Fluor 647™
647
666
Alexa Fluor 660™
668
698
Alexa Fluor 680™
679
702
630,645
655,660
345
425
Allophycocyanin (APC)
AMCA (Aminomethylcoumarin)
AMCA-X
347
444
353
442
ATTO-TAG™ FQ
486
591
BCECF (high pH)
492,503
520,528
BCECF (low pH)
482
520
Bodipy 505/515
502
510
Bodipy 558/568
558
569
Bodipy 564/570
564
570
Bodipy 576/589
579
590
Bodipy 581/591
584
592
Bodipy 630/650-X
625
642
Bodipy 650/665-X
647
665
Bodipy 665/676
Bodipy FI
605
676
504,505
511,513
Bodipy TMR
542
574
Bodipy TR
589
617
Calcein
494
517
Calcein Blue
373
440
Calcium Crimson™
588,589
611,615
Calcium Green
501,506
531
506
531
Calcium Green-1 Ca2+ Dye
Calcium Orange
549
575
Calcofluor White
385,395,405
437,440,445
Cascade Blue™
377
420
398
423
399
CFP - Cyan Fluorescent Protein
oo
180
430,433,436,(453)
474,475,476,(501)
For all your sensing needs, visit OceanOptics.com
All CCD detectors exhibit a non-linearity
in their response to light; i.e., doubling
the number of photons received during
the sample interval results in slightly less
than a doubling of the voltage output.
The effects of non-linearity, if left
uncorrected, will be slight but detectable
errors in the calculation of normalized
values (absorbance, transmission or
irradiance).
The non-linearity is a consequence of the
R-C circuit used to read out the electrons
that are left on the CCD capacitor (the
charge well). The effect is independent of
light level, integration time and optics. It
depends only on the charge in the
charge well.
The pattern of non-linearity is different for
the various detector models used in our
spectrometers. The magnitude of the
linearity varies from detector to detector,
but fortunately it is the same for all pixels
in the detector. This makes it possible to
1) measure the linearity, and 2) correct
for the errors in software.
For example, the ILX511 has a maximum
response at 2000 counts (half well
capacity). It drops to ~94% at 4000
counts and near zero counts. We can
establish this curve precisely using an
automated program that varies the
integration time to precisely control the
amount of light being sampled. This
program (OOINLCorrect) is available for
free download at our website at
OceanOptics.com/Technical/Software
Downloads.asp.
The linearity is captured from the
experiments as a plot of normalized
counts/sec versus counts for a constant
light source observed at a series of
integration times. The data is fit to a
7th order polynomial. The inverse of this
function is stored in the software and/or
on the EEPROM. When the linearity
correction feature is turned on, all spectra
are multiplied by the stored coefficients.
Uncorrected spectra are linear to ~92%.
Corrected spectra are linear to >99.8%.
Collimating Lenses
The 74-UV and 74-VIS Collimating Lenses
screw onto the end of SMA 905terminated fibers and other sampling
optics to convert divergent beams of
radiation (light) into a parallel beam. The
optical fibers we sell have a field of view
(FOV) of ~25° -- an acceptance angle
that may not be appropriate for some
experiments. Collimating lenses are
adjustable, providing FOV angles from
collimation (near 0°) to ~45°. Without the
collimating lenses, the light would
disperse more than is required for efficient
transmission and collection of the signal.
Focus the Next Collimating Lens
6. The illumination fiber is still connected
to the lamp and the lamp is on. Take
the second collimating lens in your
setup (removed from a cuvette holder,
for example) and screw it securely onto
the other end of the fiber. Point this end
of the fiber at least 2 meters from a
wall.
7. Repeat Steps 3, 4 and 5. Then remove
the lens from the end of the fiber and
install it back into your setup (back into
a cuvette holder, for example).
8. Continue to adjust the focus of the
other collimating lenses in your setup.
Absorption/Emission for Fluorophores (continued)
Fluorophore
Absorption in nm
Emission in nm
504/514
540
Cy2™
489
506
Cy3.5™
581
598
Cy3™
514
566
Cy5.5™
675
695
Cy5™
649
666
Cy7™
710,743
767,805
CL-NERF (Ratio Dye, pH)
Dabcyl
453
Dansyl Cadaverine
335
DAPI
359
461
Di-4-ANEPPS
496
705
Di-8-ANEPPS (non-ratio)
488
605
DiA (4-Di-16-ASP)
DIDS
Dil (DilC18(3))
Dinitrolphenol
518
498
713
456
591
341
415
549,551
565
349
DiO (DiOC18(3))
484,487
501,502
DM-NERF (Ratio Dye, high pH)
497/510
540
ELF 97
345
530
Eosin
524
545
Erythrosin
529,532
554,555
Ethidium Bromide
510,523
595,605
Ethidium homodimer -1 (EthD-1)
528
617
Europium (III) chloride
337
613
Fast Blue
360
440
480-506,506
520,527
Fluo-3
Fluo-4
494
516
490,494
520,525
Fluoro-Gold (Hydroxystilbamidine)
361
536
FluorX
494
520
FM 1-43™
479
598
Fura Red™ (high pH)
572
657
Fura-2, high calcium
335
505
363
512
Fluorescein (FITC)
Resources
Focus the Lamp’s Collimating Lens
In order to obtain accurate data, the light
entering and exiting a sample by means
of a fiber/collimating lens assembly must
be well collimated. Here are instructions
for adjusting the focus of the collimators
in a typical spectrometer setup.
1. Connect to the light source the fiber
that you’re going to use as the
illumination fiber in your setup. The
female SMA 905 Connector of the fiber
must be screwed all the way into the
male connector of the lamp.
2. Turn on the lamp and inspect the beam
emitted from the other end of the fiber
by pointing the fiber at a white piece of
paper. The distance is not too critical
but should be at least 3 inches from
the surface.
3. Loosen the setscrew on the fiber barrel
of the light source with an Allen wrench.
4. Slide the inner barrel of the collimating
lens until you see an even intensity
across the beam spot. The spot should
be uniform in intensity and color.
5. Once the inner barrel is positioned so
that a well-focused, uniform spot is
obtained, tighten the setscrew. Don’t
put down the fiber and then tighten the
setscrew as you may lose the focus.
oo
Spectral Identity
(Excitation ratio dye)
Fura-2, low calcium
(Excitation ratio dye)
GFP (S65T)
498
516
Hoechst 33258
345
487
Hoechst 33342
347
483
JC-1
514
529
JO-JO-1
530
545
JO-PRO-1
532
544
Lucifer Yellow
425,428
528,536,540
Lyso Tracker Green
504,534
511,551
Mag-Fura-2 (Ratio Dye, Ca2+)
369/329
508
Mag-Fura-2 (Ratio Dye Mg2+)
369/330
511/491
Mag-Fura-5 (Ratio Dye, Ca2+)
369/330
505/500
Mag-Fura-5 (Ratio Dye, Mg2+)
369/332
505/482
Magnesium Green
506,507
531
Marina Blue
362
459
Mitotracker Green FM
490
516
Tel: 727.733.2447 • Email: [email protected]
181
oo
oo
Phosphorescence &
Fluorescence
Spectral Identity
Absorption/Emission for Fluorophores (continued)
Fluorophore
Absorption in nm
Emission in nm
Mitotracker Orange
551
576
NBD
466
539
515-555,559
590,640
503
522
Oregon Green™ 488
490,493
514,520
Oregon Green™ 500
497
517
Oregon Green™ 514
506
526
PKH26 (Sigma)
551
567
POPO-3
533
574
PO-PRO-3
539
567
Nile Red
Oregon Green™
Propidium Iodid (PI)
(305), 536,538
617
Pyrene
360
387
QSY 7
560
591
Rhod-2
552
576
Rhodamine 110
496,497
520
Rhodamine 123
507
529
Rhodamine 6G
525
555
Rhodamine B
540
625
Rhodamine Green
502
527
Rhodamine Phalloidine
542
565
Rhodamine Red
570
590
R-phycoerythrin (PE)
565
578
Resources
SITS (Ion Channels)
336
436
SNAFL-1 (Ratio Dye, pH)
508/540
543/623
SNARF1 Excitation and emission
576/548
635/587
ratio dye
Sodium Green Na+, K+
506,507
532
SpectrumGreen (Vysis)
497/30, 509/31
538/44,524/56
559/38,560
588/48
SpectrumOrange (Vysis)
SPQ (6-methoxy-N-(3-sulfopropyl)
344
443
SYTO 11Dye for DNA, RNA
508,510
527,530
SYTO 13Dye for DNA, RNA
488,491
509,514
SYTOX Green (Nucleic Acid Stain
504
523
SYTOX Orange (Nucleic Acid Stain
547
570
Tetramethylrhodamine (TRITC)
555
576
Texas Red™
595
620
TO-PRO-1
515
531
TOTO-1
514
531,533
513,520
527,532
YFP (Yellow Fluorescent Protein)
oo
182
YO-PRO-1
491
506
YOYO-1
491
508,509
For all your sensing needs, visit OceanOptics.com
Phosphorescence and fluorescence are closely
related subcategories of luminescence. The
difference between the two is in the nature of
a material’s ground and excited states.
In a singlet excited state, the higher-energy
orbital electron spins opposite the lowerenergy orbital. The two electrons are
considered “paired.” In a triplet state, the
electrons are “unpaired,” and spin in the
same direction. A return to the ground state
from a singlet excited state does not require
one of the electrons to change its spin
orientation; a return from a triplet state to the
ground state does require an electron’s spin
orientation to change.
Fluorescence is the photonic emission that
occurs when the higher-energy electron in a
singlet state returns to the lower-orbit electron.
The laws of quantum mechanics permit this
rapid transition at a rate near 10-8 second.
The fluorescence lifetime is the average period
of time that a fluorophore remains in the
excited singlet state. By comparison,
phosphorescence emission occurs as the
electronically excited condition of a material in
the triplet state returns to the singlet ground
state. Again, the laws of quantum mechanics
prevail, and the probability of this transition is
lower. The lifetime of an excited triplet state is
much longer than that of an excited singlet
state, producing phosphorescence lifetimes
that range from milliseconds to seconds.
oo
INDEX by Item Code
21-01 . . . . . . . . . . . . . . . . . . . . . . . . . 156, 158
21-02. . . . . . . . . . . 65, 72, 147, 156, 158, 169
21-02-BH . . . . . . . . . . . . . . . . . . . . . . . . . . 158
21-02-SS . . . . . . . . . . . . . . . . . . . . . . . . . . 158
74-90-UV . . . . . . . . . . . . . . . . . . . . . . . 89, 157
74-ACH . . . . . . . . . . . . . . . . . . . . . 60, 89, 105
74-ACR . . . . . . . . . . . . . . . . . . . . . . . . . . . . 88
74-DA . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 88
74-MSP . . . . . . . . . . . . . . . . . . . . 90, 100, 171
74-UV . . . . . . . . . . . . 60, 88-90, 113, 156, 181
74-VIS . . . . . . . . . . . . . . . . . . . . . . . . . 88, 181
84-UV-25 . . . . . . . . . . . . . . . . . . . . . . . . . . . 88
-AACC-CON-US2 . . . . . . . . . . . . . . . . . . . . . . 62
ACC-CON-US4 . . . . . . . . . . . . . . . . . . . . . . 62
ACH-CUV-VAR . . . . . . . . . . . . . . . . . . . . . . 89
ADC-USB-SER . . . . . . . . . . . . . . . . . . . . . . 84
ADC1000-USB . . . . . . . . . . . . . . . . . . . 42, 84
ADC2000-PCI+ . . . . . . . . . . . . . . . . . . . . . . 84
ADP-SMA-SMA . . . . . . . . . . . . . . . . . . . . . 158
AR-1 . . . . . . . . . . . . . . . . . . . . . . . . . 120, 135
ASP . . . . 62, 134, 167-170, 172-173, 176-177
ASP-ES . . . . . . . . . . . . . . . . . . . . . . . . . . . . 62
ASP-NIR . . . . . . . . . . . . . . . . . . . . . . . . . . . 62
ASP-QE . . . . . . . . . . . . . . . . . . . . . . . . . . . . 62
ASP-R . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 62
ASP-R-E . . . . . . . . . . . . . . . . . . . . . . . . . . . 62
-B-
-CC-MOUNT-MIC . . . . . . . . . . . . . . . . . . . . . 157
CAL-2000 . . . . . . . . . . . . . . . . . . . . . 120, 134
CAL-2000-B. . . . . . . . . . . . . . . . . . . . . . . . 134
CBL-2 . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 84
CBL-PX-2 . . . . . . . . . . . . . . . . . . . . . . 62, 136
CBL-SER . . . . . . . . . . . . . . . . . . . . . . . . . . . 62
CC-3 . . . . . . . . . . . . . 104, 132, 133, 147, 156
CC-3-DA . . . . . . . . . . . . . . . . . . . . . . . 57, 104
CC-3-UV . . . . . . . 57, 104, 147, 168, 172-173
CD-SPECTRA . . . . . . . . . . . . . . . . . . . . . . . 79
CFV-PIP-SP. . . . . . . . . . . . . . . . . . . . . . . . 103
CFV-PUMP-SP . . . . . . . . . . . . . . . . . . . . . 103
CHEM4-UV-FIBER . . . . . . . 8-9, 36-37, 39, 76
CHEM4-UV-VIS . . . . . 8-9, 36-37, 39, 76, 167
CHEM4-VIS-FIBER . . . . . . 8-9, 36-37, 39, 76
CHEM4-VIS-NIR. . . . . . . . . 8-9, 36-37, 39, 76
CHEMSEN-CO . . . . . . . . . . . . . . . . . . . . . . 75
CHEMTEST-PH. . . . . . . . . . . . . . . . . . . . . . 76
CONN-FC . . . . . . . . . . . . . . . . . . . . . . . . . 141
CONN-LSMA . . . . . . . . . . . . . . . . . . . . . . . 141
CONN-PSMA, CONN-PSMA-O . . . . . . . . 141
CONN-QSMA, CONN-QSMA-O . . . . . . . . 141
CONN-SMA, CONN-SMA-O . . . . . . . . . . . 141
CONN-ST . . . . . . . . . . . . . . . . . . . . . . . . . 141
CSH, CSH-45 . . . . . . . . . . . . . . . . . . . . . . 157
CT-series . . . . . . . . . . . . . . . . . . . . . . . . . . 111
CUV-ALL-UV. . . . . . 45, 47, 90, 100, 103, 171
CUV-CCE . . . . . . . . . . . . . . . . . . . . . . . . . . 99
CUV-COVER . . . . . . . . . . . . . . . . . . . . . 90, 93
-DD-1000-B, D-1000-REM-B . . . . . . . . . . . . 136
D2000 . . . . . . . . . . . . . . . . . . . . 120, 126, 170
D2000-DUV . . . . . . . . . . . . . . . . . . . . 126, 136
D2000-S . . . . . . . . . . . . . . . . . . . . . . . . . . 126
D2000-S-DUV . . . . . . . . . . . . . . . . . . . . . . 126
DET2-UV . . . . . . . . . . . . . . . . . . . . . . . . . . . 24
DET2-VIS . . . . . . . . . . . . . . . . . . . . . . . . . . 24
DET4-200-1100 . . . . . . . . . . . . . . . . . . . . . . 24
DET4-200-850. . . . . . . . . . . . . . . . . . . 17, 176
DET4-350-1000. . . . . . . . . . . . . . 17, 172, 175
DET4-UV . . . . . . . . . . . . . . . . . . . . . . . . 17, 24
DET4-VIS . . . . . . . . . . . . . . . . . . . . . . . 17, 24
DH-BAL-KIT, DH-BAL-KIT-S . . . . . . . . . . . 122
DH2000 . . . . . . . . . . . 120, 122, 123, 136, 167
DH2000-BAL. . . 120, 122, 132, 136, 167, 176
DH2000-BD . . . . . . . . . . . . . . . . 123, 126, 136
DH2000-BH . . . . . . . . . . . . . . . . . . . . 123, 136
DH2000-CAL . . . . . . . . . . . . . . . 120, 132, 168
DH2000-DUV . . . . . . . . . . . . . . . . . . 123, 136
DH2000-DUV-B . . . . . . . . . . . . . 123, 126, 136
DH2000-FHS, DH2000-FHS-DUV . . . . . . 123
DH2000-RECAL . . . . . . . . . . . . . . . . . . . . 132
DH2000-S . . . . . . . . . . . . . . . . . . . . . 122, 123
DT-1000-B, DT-1000-BT . . . . . . . . . . . . . . 136
DT-1000-BT-CE, DT-1000-REM-B . . . . . . 136
DT-MINI . . . . . . . . . . . . . . . . . . . 120, 125, 136
DT-MINI-2 . . . . . . . 60, 62, 120, 125, 136, 176
DT-MINI-2-B . . . . . . . . . . . . . . . . . . . 125, 136
DT-MINI-2-GS . . . . . . . . . . . . . . 120, 125, 136
DT-MINI-B . . . . . . . . . . . . . . . . . . . . . 125, 136
DTS-1700, DTS-2500, DTS-NB . . . . . . . . . 40
DTS-PHAZIR-series . . . . . . . . . . . . . . . . . . 40
-EEDU-SPEC-BOOK . . . . . . . . . . . . . . . . . . . 36
EDU-SPEC-BOOK-S. . . . . . . . . . . . . . . . . . 36
EDU-SPEC-CD . . . . . . . . . . . . . . . . . . . . . . 36
EDU-SPEC-CD-S . . . . . . . . . . . . . . . . . . . . 36
EDU-SPEC-D . . . . . . . . . . . . . . . . . . . . . . . 36
EDU-SPEC-D-S. . . . . . . . . . . . . . . . . . . . . . 36
EPOXY-TEST . . . . . . . . . . . . . . . . . . . . . . 141
-FF-BY . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 76
F-CR . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 76
F-MCP . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 76
F-PR . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 76
F-TB. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 76
F-XXX . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 76
FCBARREL . . . . . . . . . . . . . . . . 136, 156, 158
FH-SMA. . . . . . . . . . . . . . . . . . . . . . . 113, 164
Tel: 727.733.2447 • Email: [email protected]
FHS-LVF . . . . . . . . . . . . . . . . . . . . . . . . . . 115
FHS-UV . . . . . . . . . . . . . . . . . . . . . . . . . . . 113
FHSA-RS232 . . . . . . . . . . . . . . . . . . . . . . . 113
FHSA-TTL . . . . . . . . . . . . . . . . . . . . . . . . . 113
FIA-1000-Z . . . . . . . . . . . . . . . . . . . . . . . . . 95
FIA-ASX260. . . . . . . . . . . . . . . . . . . . . . . . . 43
FIA-HEATER . . . . . . . . . . . . . . . . . . . . . . . . 43
FIA-LAB-2500 . . . . . . . . . . . . . . . . . . . . . . . 43
FIA-LOV. . . . . . . . . . . . . . . . . . . . . . . . . . . . 95
FIA-P200-SR, FIA-P400-SR . . . . . . . . . . . . 94
FIA-PMT-FL. . . . . . . . . . . . . . . . . . . . . 44, 101
FIA-PUMP-C . . . . . . . . . . . . . . . . . . . . . . . . 95
FIA-SIA . . . . . . . . . . . . . . . . . . . . . . . . . . . . 95
FIA-SIA-LOV . . . . . . . . . . . . . . . . . . . . . . . . 95
FIA-SMA-FL. . . . . . . . . . . . . . . . . . . . . . . . 100
FIA-Z-CELL-PEEK. . . . . . . . . . . . . . . . . . . . 94
FIA-Z-CELL-PLEX . . . . . . . . . . . . . . . . . . . . 94
FIA-Z-CELL-SS . . . . . . . . . . . . . . . . . . . . . . 94
FIA-Z-CELL-TEF . . . . . . . . . . . . . . . . . . . . . 94
FIA-Z-SMA-20-series. . . . . . . . . . . . . . . . . . 94
FIA-Z-SMA-50-series. . . . . . . . . . . . . . . . . . 94
FIA-Z-SMA-100-series. . . . . . . . . . . . . . . . . 94
FIA-Z-SMA-PEEK . . . . . . . . . . . . . . . . . . . . 94
FIA-Z-SMA-PLEX . . . . . . . . . . . . . . . . . . . . 94
FIA-Z-SMA-SS. . . . . . . . . . . . . . . . . . . . . . . 94
FIA-Z-SMA-TEF. . . . . . . . . . . . . . . . . . . . . . 94
FIA-Z-SMA-ULT. . . . . . . . . . . . . . . . . . . . . . 94
FIBER-50-series . . . . . . . . . . . . . . . . . . . . 143
FIBER-100-series . . . . . . . . . . . . . . . . . . . 143
FIBER-200-series . . . . . . . . . . . . . . . . . . . 143
FIBER-300-series . . . . . . . . . . . . . . . . . . . 143
FIBER-400-series . . . . . . . . . . . . . . . . . . . 143
FIBER-500-series . . . . . . . . . . . . . . . . . . . 143
FIBER-600-series . . . . . . . . . . . . . . . . . . . 143
FIBER-1000-series . . . . . . . . . . . . . . . . . . 143
FIBER-WRAP . . . . . . . . . . . . . . . . . . 156, 158
FILM . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 76
FILM300 . . . . . . . . . . . . . . . . . . . . . . . . . . . 76
FIRMWARE-FLG . . . . . . . . . . . . . . . . . . . . . 62
FL-400 . . . . . . . . . . . . . . . . . . . . . . . . . 36, 147
FLS-series . . . . . . . . . . . . . . . . . . . . . . . . . 110
FLZ-series . . . . . . . . . . . . . . . . . . . . . . . . . 110
FNY-PR . . . . . . . . . . . . . . . . . . . . . . . . . . . . 76
FOIS-1 . . . . . . . . . 56, 57, 104, 105, 172, 173
FOP-UV, FOP-VIS. . . . . . . . . . . . . . . . . . . 156
FOS-2X2-TTL . . . . . . . . . . . . . . . . . . . . . . 116
FOSPOR-18G, FOSPOR-21G . . . . . . . . . . 70
FOSPOR-AF, FOSPOR-AF-MG . . . . . . . . . 72
FOSPOR-AL300 . . . . . . . . . . . . . . . . . . . . . 71
FOSPOR-CAL . . . . . . . . . . . . . . . . . . . . . . . 74
FOSPOR-CAL-EXT . . . . . . . . . . . . . . . . . . . 74
FOSPOR-GF . . . . . . . . . . . . . . . . . . . . . . . . 72
FOSPOR-OR125. . . . . . . . . . . . . . . . . . . . . 70
FOSPOR-OR125-G, -GT. . . . . . . . . . . . . . . 70
FOSPOR-PI600. . . . . . . . . . . . . . . . . . . . . . 71
FOSPOR-R . . . . . . . . . . . . . . . . . . . . . . 71, 73
FOSPOR-RECOV . . . . . . . . . . . . . . . . . . . . 73
FOSPOR-RECOV-N . . . . . . . . . . . . . . . . . . 73
FOSPOR-SGS, FOSPOR-SGS-M . . . . . . . 72
FOSPOR-T1000 . . . . . . . . . . . . . . . . . . 71, 74
FOSPOR-T1000-RTD . . . . . . . . . . . . . . 71, 74
FOT-SMAWRENCH . . . . . . . . . 136, 156, 158
FOXY-18G, FOXY-21G . . . . . . . . . . . . . . . . 70
FOXY-AF, FOXY-AF-MG . . . . . . . . . . . . . . . 72
FOXY-AL300 . . . . . . . . . . . . . . . . . . . . . . . . 71
FOXY-CAL . . . . . . . . . . . . . . . . . . . . . . . . . . 74
FOXY-CAL-EXT. . . . . . . . . . . . . . . . . . . . . . 74
FOXY-FLOW-CELL . . . . . . . . . . . . . . . . . . . 73
FOXY-GF . . . . . . . . . . . . . . . . . . . . . . . . . . . 72
FOXY-OR125 . . . . . . . . . . . . . . . . . . . . . . . 70
FOXY-OR125-G . . . . . . . . . . . . . . . . . . . . . 70
FOXY-OR125-GT . . . . . . . . . . . . . . . . . . . . 70
FOXY-PI600 . . . . . . . . . . . . . . . . . . . . . . . . 71
FOXY-R . . . . . . . . . . . . . . . . . . 65, 71, 73, 169
FOXY-R-PNA. . . . . . . . . . . . . . . . . . . . . . . . 73
FOXY-RESP . . . . . . . . . . . . . . . . . . . . . . . . 72
183
Resources
BFA-KIT, BFA-KIT-CHUCK . . . . . . . . . . . . 154
BIF200-UV-VIS . . . . . . . . . . . . . . . . . . . . . 145
BIF200-VIS-NIR. . . . . . . . . . . . . . . . . . . . . 145
BIF400-MIXED . . . . . . . . . . . . . . . . . . . . . 145
BIF400-UV-VIS . . . . . . . . . . . . . . . . . 116, 145
BIF400-VIS-NIR. . . . . . . . . . . . . . . . . . . . . 145
BIF50-UV-VIS . . . . . . . . . . . . . . . . . . . . . . 145
BIF50-VIS-NIR. . . . . . . . . . . . . . . . . . . . . . 145
BIF600-MIXED . . . . . . . . . . . . . . . . . . . . . 145
BIF600-UV-VIS . . . . . . . . . . . . . . . . . . . . . 145
BIF600-VIS-NIR . . . . . . . . . . 65, 72, 125, 145
BOX-series . . . . . . . . . . . . . . . . . . . . . . . . . 62
CUV-COVER-TALL . . . . . . . . . . . . . . . . . . . 93
CUV-FL-DA . . . . . . . . . . . . . . . . . . . . . 90, 100
CUV-TLC-50F . . . . . . . . . . . . . . . . . . . . . . . 91
CUV-TLC-series . . . . . . . . . . . . . . . . . . . . . 91
CUV-UV. . . . . . . . . . . . . . . . . . . . . . . . 90, 167
CUV-UV-10 . . . . . . . . . . . . . . . 14, 34, 90, 170
CUV-VAR. . . . . . . . . . . . . . . . . . . . . . . . . . . 90
CUV-VAR-OPTION . . . . . . . . . . . . . . . . . . . 90
CV-Q-10 . . . . . . . . . . . . . . . . . . . 93, 167, 170
CV-Q-100 . . . . . . . . . . . . . . . . . . . . . . 93, 170
CVD-COVER . . . . . . . . . . . . . . . . . . . . . . . . 93
CVD-DIFFUSE. . . . . . . . . . . . . . . . . . . . . . 115
CVD-ROUND-series . . . . . . . . . . . . . . . . . . 93
CVD-UV1S, CVD-UV1S-SAM . . . . . . . . . . . 93
CVD-UV1U, CVD-UV1U-SAM. . . . . . . . . . . 93
CVD-VIS1M . . . . . . . . . . . . . . . . . . . . . . . . . 93
CVD-VIS1S . . . . . . . . . . . . . . . . . . . . . . . . . 93
CVF-Q-10 . . . . . . . . . . . . . . . . . . . . . . . . . . 93
CVFL-Q-10 . . . . . . . . . . . . . . . . . . . . . . . . . 93
CVS-Q-10 . . . . . . . . . . . . . . . . . . . . . . . . . . 93
oo
oo
INDEX by Item Code
FOXY-RECOV . . . . . . . . . . . . . . . . . . . . . . . 73
FOXY-RECOV-N . . . . . . . . . . . . . . . . . . . . . 73
FOXY-SGS, FOXY-SGS-M . . . . . . . . . . . . . 72
FOXY-T-MOD-1 . . . . . . . . . . . . . . . . . . . . . . 74
FOXY-T-MOD-K. . . . . . . . . . . . . . . . . . . . . . 74
FOXY-T1000, FOXY-T1000-RTD . . . . . 71, 74
FOXY-TK-W. . . . . . . . . . . . . . . . . . . . . . . . . 74
FOXY-TK1 . . . . . . . . . . . . . . . . . . . . . . . . . . 74
FOXY-TS1 . . . . . . . . . . . . . . . . . . . . . . . . . . 74
FR-BY . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 76
FR-CR . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 76
FR-MCP. . . . . . . . . . . . . . . . . . . . . . . . . . . . 76
FR-PR . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 76
FR-TB . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 76
FT-KIT . . . . . . . . . . . . . . . . . . . . . . . . 154, 155
FVA-ADP . . . . . . . . . . . . . . . . . . . . . . . . . . 117
FVA-UV . . . . . . . . . . . . . . . . . . . 117, 121, 156
-GGER-KIT . . . . . . . . . . . . . . . . . . . . . . . . . . 116
GRATING HC-1 . . . . . . . . 23, 28, 35, 60, 168
GRATING #1-#14 . . . . . . . . . . . . . . . . . . . . 16
GRATING #H1-H14 . . . . . . . . . . . . . . . . . . . 23
GRATING #N1-N2 . . . . . . . . . . . . . . . . . . . . 32
Resources
-HHC-1 . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 23
HG-1 . . . . . . . . . . . . . . . . . . . . . 120, 134, 135
HIOXY-18G, HIOXY-21G . . . . . . . . . . . . . . . 70
HIOXY-AF, HIOXY-AF-MG. . . . . . . . . . . . . . 72
HIOXY-AL300 . . . . . . . . . . . . . . . . . . . . . . . 71
HIOXY-CAL . . . . . . . . . . . . . . . . . . . . . . . . . 74
HIOXY-CAL-EXT . . . . . . . . . . . . . . . . . . . . . 74
HIOXY-GF . . . . . . . . . . . . . . . . . . . . . . . . . . 72
HIOXY-OR125 . . . . . . . . . . . . . . . . . . . . . . . 70
HIOXY-OR125-G, HIOXY-OR125-GT . . . . . 70
HIOXY-R . . . . . . . . . . . . . . . . . . . . . . . . 71, 73
HIOXY-RECOV, HIOXY-RECOV-N . . . . . . . 73
HIOXY-SGS, HIOXY-SGS-M . . . . . . . . . . . . 72
HIOXY-T1000, HIOXY-T1000-RTD . . . . 71, 74
HL-2000-series . . . . . . . . . 101, 120, 129, 136
HL-2000-CAL, HL-2000-CAL-ISP . . . 120, 133
HL-2000-RECAL . . . . . . . . . . . . . . . . . . . . 133
HPX-2000 . . . . . . . . . . . . . . . . . 120, 127, 136
HPX-2000-B, HPX-2000-BM . . . . . . . 127, 136
HR2000 . . . . . . . . . . . . . . . . . . . . 80, 124, 179
HR2000+ . . . . 13, 20, 22-25, 61, 80, 124, 179
HR4-BREAKOUT . . . . . . . . . . . . . 61, 62, 124
HR4-CBL-DB15 . . . . . . . . . . . . . . . . . . . . . . 62
HR4000 . . 13, 21-25, 52, 60-61, 80, 124, 179
HR4000CG-UV-NIR. . . . . . . . . . . . . . . . . . . 35
-IINLINE-FH . . . . . . . . . . . . . . . . . . . . . 113, 164
INLINE-OF. . . . . . . . . . . . . . . . . . . . . 113, 164
INLINE-TTL-S . . . . . . . . . . . . . . . . . . . . . . 116
ISP-30-6-I . . . . . . . . . . . . . . . . . . . . . . . . . 105
ISP-30-6-R. . . . . . . . . . . . . . . . . . . . . . . . . 106
ISP-50-8-I . . . . . . . . . . . . . . . . . . . . . 105, 133
ISP-50-8-R. . . . . . . . . . . . . . . . . . . . . . . . . 106
ISP-50-8-R-GT . . . . . . . . . . . . . . . . . . . . . 106
ISP-80-8-I . . . . . . . . . . . . . . . . . . . . . . . . . 105
ISP-80-8-R. . . . . . . . . . . . . . . . . . . . . . . . . 106
ISP-LED-ADP . . . . . . . . . . . . . . . . . . . . . . 105
ISP-PORT-1, ISP-PORT-2 . . . . . . . . 105, 106
ISP-REF, ISP-REF-B. . . . . . . . . . . . . 106, 177
ISS-2 . . . . . . . . . . . . . . . . . . . . . . . . . . . 37, 92
ISS-UV-VIS . . . . . . . . . . . . . . . . . . . . . . 37, 92
-LL2 . . . . . . . . . . . . . . . . . . . . . . . 13, 22, 24, 42
L4. . . . . . . . . 13, 17, 24, 65, 66, 169-172, 177
oo
184
LASER-785 . . . . . . . . . . . . . . . . . . . . . . 52, 53
LED-380 . . . . . . . . . . . . . . . . . . . . . . 130, 136
LED-395 . . . . . . . . . . . . . . . . . . . . . . 130, 136
LED-470 . . . . . . . . . . . . . . . . . . . . . . . . . . 130
LED-518 . . . . . . . . . . . . . . . . . . . . . . 130, 136
LED-590 . . . . . . . . . . . . . . . . . . . . . . 130, 136
LED-640 . . . . . . . . . . . . . . . . . . . . . . 130, 136
LED-KIT. . . . . . . . . . . . . . . . . . . . . . . 130, 136
LED-PS, LED-PS-NIST. . . . . . . . 56, 104, 172
LED-PS-RECAL . . . . . . . . . . . . . . . . . . . . 104
LED-WHITE. . . . . . . . . . . . . . . . . . . . 130, 136
LIBS2500-series. . . . . . . . . . . . 33, 48-50, 174
LIBS-BUN-series . . . . . . . . . . . . . . . . . . . . . 48
LIBS-CH-series . . . . . . . . . . . . . . . . . . . . . . 48
LIBS-ELITE . . . . . . . . . . . . . . . . . . . . . . . . . 50
LIBS-IM-USB . . . . . . . . . . . . . . . . . . . . . . . . 49
LIBS-LAS200MJ, LIBS-LASER. . . 48, 49, 174
LIBS-SC . . . . . . . . . . . . . . . . . . . . 48, 49, 174
LPC-1, LPC-5 . . . . . . . . . . . . . . . . . . . . . . . 98
LPC-CLEANKIT. . . . . . . . . . . . . . . . . . . . . . 98
LS-1 . . . . . . . . . . . 34, 120-121, 128, 175, 177
LS-1-B . . . . . . . . . . . . . . . . . . . . . . . . 128, 136
LS-1-CAL. . . . . . . . . . . . . . . . . . . 57, 120, 133
LS-1-CAL-INT . . . . . . . . . . . 56, 105, 133, 172
LS-1-LL . . . . . . . . . . . . . . . . . . . . . . . 128, 136
LS-1-LL-B . . . . . . . . . . . . . . . . . . . . . 128, 136
LS-1-RECAL . . . . . . . . . . . . . . . . . . . . . . . 133
LS-450. . . . . . . . . . . . . . . . . 62, 103, 130, 131
LS-475 . . . . . . . . . . . . . . . . . . . . . . . . . . . . 131
LTP-series . . . . . . . . . . . . . . . . . . . . . . . . . 112
LVF-series. . . . . . . . . . . . . . . . . . . . . . 114-115
-MMFA-C-MOUNT, MFA-PT . . . . . . . . . . . . . 157
MFPF100-1, MFPF100-2 . . . . . . . 65, 67, 169
MMS-RAMAN . . . . . . . . . . . . . . . . . 51, 55, 80
MPM-2000-series . . . . . . . . . . . . . . . . . . . 117
MONOSCAN2000 . . . . . . . . . . . . . . . . . . . 101
-NNC-512-NIR. . . . . . . . . . . . . . . . . . . . . . . . . 58
NC-NIR . . . . . . . . . . . . . . . . . . . . . . . . . . . . 58
NC-NIR-HR . . . . . . . . . . . . . . . . . . . . . . . . . 58
NC-UV-VIS . . . . . . . . . . . . . . . . . . . . . . . . . 58
NC-UV-VIS-NIR . . . . . . . . . . . . . . . . . . . . . . 58
NC-VIS . . . . . . . . . . . . . . . . . . . . . . . . . . . . 58
NC-VIS-NIR . . . . . . . . . . . . . . . . . . . . . . . . . 58
NIR-512 . . . . . . . . . . . . . . . . . 30-32, 135, 179
NIR256-2.1. . . . . . . . . . . . . . . . . . . 30-32, 179
NIR256-2.5. . . . . . . . . . . . . . . . . . . 30-32, 179
NTS-10, NTS-25, NTS-100 . . . . . . . . . . . . 118
NTS-ND-1, NTS-ND-2, NTS-ND-3 . . . . . . 118
NTS-NJ, NTS-SOFTWARE . . . . . . . . . . . . 118
-OOF1-GG375. . . . . . . . . . . . . . . . . . . 16, 23, 27
OF1-GG475. . . . . . . . . . . . . . . . . . . 16, 23, 27
OF1-OG515. . . . . . . . . . . . . . . . . . . 16, 23, 27
OF1-OG550. . . . . . . . . . . . . . . . . . . 16, 23, 27
OF1-OG590. . . . . . . . . . . . . . . . . . . 16, 23, 27
OF1-WG305 . . . . . . . . . . . . . . . . . . 16, 23, 27
OF2-BG34 . . . . . . . . . . . . . . . . . . . . . . . . . 164
OF2-BG34R. . . . . . . . . . . . . . . . . . . . . . . . 164
OF2-FG3 . . . . . . . . . . . . . . . . . . . . . . . . . . 164
OF2-GG375. . . . . . . . . . . . . . . . . . . . . . . . 164
OF2-GG395. . . . . . . . . . . . . . . . . . . . . . . . 164
OF2-GG475. . . . . . . . . . . . . . . . . . . . . . . . 164
OF2-KG3 . . . . . . . . . . . . . . . . . . . . . . . . . . 164
OF2-LS . . . . . . . . . . . . . . . . . . . . . . . 128, 164
OF2-OG515. . . . . . . . . . . . . . . . . . . . . . . . 164
OF2-OG550. . . . . . . . . . . . . . . . . . . . . . . . 164
OF2-RG780 . . . . . . . . . . . . . . . . . . . . . . . . 164
OF2-U360 . . . . . . . . . . . . . . . . . . . . . . . . . 164
OF2-WG305 . . . . . . . . . . . . . . . . . . . . . . . 164
OFLV-200-1100 . . . . . . . . . . . . . . . . . . . 24, 60
OFLV-200-850. . . . . . . . . 17, 34, 37, 167, 176
OFLV-350-1000. . . . 17, 34, 37, 172, 175, 177
OFLV-350-DW . . . . . . . . . . . . . . . . . . . . . . . 42
OFLV-DW . . . . . . . . . . . . . . . . . . . . . . . . . . 42
OFLV-QE . . . . . . . . . . . . . . . . . . 20, 26, 28, 45
OMNIDRIVER . . . . . . . . . . . . . . . . . . . . . . . 82
OMNI+SPAM . . . . . . . . . . . . . . . . . . . . . . . . 82
OOICHEM . . . . . . . . . . . . . . . . . . . . . . . 80-81
OOIIRRAD-C . . . . . . . . . . . . . . . . . . . . . 80-81
OOILIBS . . . . . . . . . . . . . . . . . . . . 48, 80, 174
OOISENSORS . . . . . . . . . . . . . . . 75, 80, 169
OOISPECLINE . . . . . . . . . . . . . . . . . . . . . . 83
OPM-1, -2, -3, -4 . . . . . . . . . . . . . . . . . 89, 173
OPM-M . . . . . . . . . . . . . . . . . . . . . . . . . . . . 89
OPM-SMA . . . . . . . . . . . . . . . . . . . . . . . . . . 89
-PP8-2-SMA . . . . . . . . . . . . . . . . . . . . . . . . . 144
P50-2-UV-VIS . . . . . . . . . . . . . . . . . . 144, 156
P50-2-VIS-NIR . . . . . . . . . . . . . . . . . 144, 156
P100-2-UV-VIS . . . . . . . . . . . . . . . . . . . . . 144
P100-2-VIS-NIR. . . . . . . . . . . . . . . . . . . . . 144
P100-5-UV-VIS . . . . . . . . . . . . . . . . . . . . . 144
P100-5-VIS-NIR. . . . . . . . . . . . . . . . . . . . . 144
P100-10-UV-VIS . . . . . . . . . . . . . . . . . . . . 144
P100-10-VIS-NIR. . . . . . . . . . . . . . . . . . . . 144
P200-2-UV-VIS . . . . . . . . . . . . . . 94, 144, 156
P200-2-VIS-NIR . . . . . . . . . . . . . 56, 144, 156
P200-5-UV-VIS . . . . . . . . . . . . . . . . . . . . . 144
P200-5-VIS-NIR. . . . . . . . . . . . . . . . . . . . . 144
P200-10-UV-VIS . . . . . . . . . . . . . . . . . . . . 144
P200-10-VIS-NIR. . . . . . . . . . . . . . . . . . . . 144
P300-1-SR. . . . . . . . . . . . . . . . . . . . . . 37, 144
P400-025-SR. . . . . . . . . . . . . . . . . . . 144, 156
P400-1-SR. . . . . . . . . . . . . . . . . . . . . . . . . 144
P400-1-UV-VIS . . . . . . . . . . . . . . . . . . . . . 144
P400-2-SR. . . . . . . . . . . . . . . . . . . . . . . . . 144
P400-2-UV-VIS . . . . . . . . . . . 37, 94, 144, 147
P400-2-VIS-NIR . . . . . . . . . 56, 144, 156, 177
P400-5-UV-VIS . . . . . . . . . . . . . . . . . . . . . 144
P400-5-VIS-NIR. . . . . . . . . . . . . . . . . . . . . 144
P400-10-UV-VIS . . . . . . . . . . . . . . . . . . . . 144
P400-10-VIS-NIR. . . . . . . . . . . . . . . . . . . . 144
P600-025-SR. . . . . . . . . . . . . . . . . . . . . . . 144
P600-025-VIS-NIR. . . . . . . . . . . . . . . . . . . 144
P600-1-SR. . . . . . . . . . . . . . . . . . . . . . 60, 144
P600-2-SR. . . . . . . . . . . . . . . . . . . . . . . . . 144
P600-2-UV-VIS . . . . . . . . . . . . . . . . . 144, 156
P600-2-VIS-NIR . . . . . . . . . . . . . . . . 144, 156
P600-5-UV-VIS . . . . . . . . . . . . . . . . . . . . . 144
P600-5-VIS-NIR. . . . . . . . . . . . . . . . . . . . . 144
P600-10-UV-VIS . . . . . . . . . . . . . . . . . . . . 144
P600-10-VIS-NIR. . . . . . . . . . . . . . . . . . . . 144
P1000-2-UV-VIS . . . . . . . . . . . . . . . . . . . . 144
P1000-2-VIS-NIR. . . . . . . . . . . . . . . . . . . . 144
PIP-10-2 . . . . . . . . . . . . . . . . . . . . . . . . . . . 98
PIP-UCK . . . . . . . . . . . . . . . . . . . . . . . . . . . 98
PIP-UCK-CS . . . . . . . . . . . . . . . . . . . . . . . . 98
PL100-2-series . . . . . . . . . . . . . . . . . . . . . 145
PL200-2-MIXED . . . . . . . . . . . . . . . . . . . . 145
PLASCALC-UV-NIR . . . . . . . . . . . . . . . . . . 59
PRO-CFC-1/2 . . . . . . . . . . . . . . . . . . . . . . . 96
PRO-CFC-3/8 . . . . . . . . . . . . . . . . . . . . . . . 96
PRO-FC-series . . . . . . . . . . . . . . . . . . 97, 100
PRO-MFC-series . . . . . . . . . . . . . . . . . . . . . 96
PROCESS-2000-series . . . . . . . . . . . . . . . . 41
PS-2636. . . . . . . . . . . . . . . . . . . . . . . . . . . . 39
PS-2555. . . . . . . . . . . . . . . . . . . . . . . . . . . . 39
PS-HG1-ADP. . . . . . . . . . . . . . . . . . . . . . . 135
PUMP-IT-1000. . . . . . . . . . . . . . . . . . . . . . . 99
PUMP-IT-PUMP . . . . . . . . . . . . . . . . . . . . . 99
PX-2 . . . . . . . . . . . . . . 45, 120, 127, 136, 171
PX-2-B. . . . . . . . . . . . . . . . . . . . . . . . 127, 136
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INDEX by Item Code
PX-2-FIRMWARE . . . . . . . . . . . . . . . . . . . . 62
-Q-
-SS1024DW-series . . . . . . . . . . . . . . . . . . 42, 84
S2-1024DW-series . . . . . . . . . . . . . . . . . . . 42
S2000 . . . . . . . . . . . . . . . . . 84, 167, 170, 176
SAG+UPG . . . . . . . . . . . . . . . . . . . . . . 16, 171
SAG+UPG-HR. . . . . . . . . . . . . . . . . . . . 23, 27
SHA-1 . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 61
SLIT-5 . . . . . . . . . . . . . . . . . . . . . . . 15, 22, 28
SLIT-10 . . . . . . . . . . . . . . . . . . . 15, 22, 27, 32
SLIT-25 . . . . . . . . . . . . . . . . . . . 15, 22, 27, 32
SLIT-50 . . . . . . . . . . . . . . . . . . . 15, 22, 27, 32
SLIT-100 . . . . . . . . . . . . . . . . . . 15, 22, 27, 32
SLIT-200 . . . . . . . . . . . . . . . . . . 15, 22, 27, 32
SMA-FC-ADP . . . . . . . . . . . . . . . . . . . . . . 141
SPAM. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 82
SMA-PUCK . . . . . . . . . . . . . . . . . . . . . . . . 154
SMA-ST-ADP. . . . . . . . . . . . . . . . . . . . . . . 141
SPEC-CADDY . . . . . . . . . . . . . . . . . . . . . . . 62
SPEC-CAL. . . . . . . . . . . . . . . . . . . . . . . . . 133
SPEC-CAL-UV . . . . . . . . . . . . . . . . . . . . . 132
SPEC-CAL-NIR . . . . . . . . . . . . . . . . . . . . . 132
SPECEl-2000 . . . . . . . . . . . . . . . . . . . . . . . 59
SPECLINE. . . . . . . . . . . . . . . . . . . . . . . . . . 83
SPECTRASUITE . . . . . . . . . . . . . . . . . . 78-81
SPLIT200-UV-VIS . . . . . . . . . . . . . . . . . . . 145
SPLIT200-VIS-NIR . . . . . . . . . . . . . . . . . . 145
SPLIT400-UV-VIS . . . . . . . . . . . . . . . . . . . 145
SPLIT400-VIS-NIR . . . . . . . . . . . . . . . . . . 145
STAGE . . . . . . . . . . . . . . . . . . . . . . . . 109,157
STAGE-RTL-T . . . . . . . . . . . . . . . . . . 109, 157
STAN-ABS-UV. . . . . . . . . . . . . . . . . . . 93, 167
STAN-ABS-VIS . . . . . . . . . . . . . . . . . . . . . . 93
STAN-FL-RED . . . . . . . . . . . . . . . . . . . 45, 100
STAN-HOLDER . . . . . . . . . . . . . . . . . . . . . 108
STAN-RAM532 . . . . . . . . . . . . . . . . . . . . . . 53
STAN-RAM785 . . . . . . . . . . . . . . . . . . . . . . 53
STAN-SSH . . . . . . . . . . . . 108, 163, 175, 176
STAN-SSH-NIST . . . . . . . . . . . . . . . . 108, 163
STAN-SSL . . . . . . . . . . . . . . . . . . . . . 108, 163
-RR-3000-532 . . . . . . . . . . . . . . . . . . . . . . 51, 54
R-3000-785 . . . . . . . . . . . . . . . . . . . . . . 51, 54
R-3000-HR-532 . . . . . . . . . . . . . . . . . . . 51, 54
TERM-KIT . . . . . . . . . . . . . . . . . . . . . 154, 155
TERMKITSMA-series . . . . . . . . . . . . . . . . 155
TERMKITQSMA-series . . . . . . . . . . . . . . . 155
TI300-UV-VIS . . . . . . . . . . . . . . . . . . . . . . 152
TI300-VIS-NIR . . . . . . . . . . . . . . . . . . . . . . 152
TP300-UV-VIS. . . . . . . . . . . . . . . . . . . 76, 151
TP300-VIS-NIR . . . . . . . . . . . . . . . . . . 76, 151
TPSLEEVE . . . . . . . . . . . . . . . . . . . . . . . . 151
-UUSB-650 . . . . . . . . . . . . . . . . . . . . . . . . . . . 38
USB-650-VIS-NIR . . . . . . . . . . . . . . . . . . . . 38
USB-ADP-DT2 . . . . . . . . . . . . . . . . . . 62, 124
USB-ADP-PC . . . . . . . . . . . . . . . . . . . . . . . 62
USB-ADC-PC-E. . . . . . . . . . . . . . . . . . . . . . 62
USB-ADP-PX2 . . . . . . . . . . . . . . . . . . 62, 127
USB-BP . . . . . . . . . . . . . . . . . . . . . . . . . . . . 62
USB-CBL-1 . . . . . . . . . . . . . . . . . . . . . . 62, 84
USB-CBL-PS. . . . . . . . . . . . . . . . . . . . . 61, 62
USB-DT . . . . . . . . . . . . . . . . . . . . 19, 120, 124
USB-DT-B . . . . . . . . . . . . . . . . . . . . . . . . . 124
USB-FHS. . . . . . . . . . . . . . . . . . . . . . . . . . . 19
USB-ISP-50-I. . . . . . . . . . . . . . . . . . . . . . . 105
USB-ISP-80-I. . . . . . . . . . . . . . . . . . . . . . . 105
USB-ISS-T. . . . . . . . . . . . . . . . . . . . . . . 19, 92
USB-ISS-UV-B. . . . . . . . . . . . . . . . . . . . . . 136
USB-ISS-UV-VIS. . . . . . . . . . . 19, 37, 92, 136
USB-ISS-VIS. . . . . . . . . . . . . . 19, 37, 92, 136
USB-ISS-VIS-B . . . . . . . . . . . . . . . . . . . . . 136
USB-LS-395 . . . . . . . . . . . . . . . . . 46, 68, 131
USB-LS-450 . . . . . . . . . . . . . 46, 68, 131, 169
USB-LS-450-TP . . . . . . . . . . . . . . 65, 74, 131
USB-LS-450-TP16. . . . . . . . . . . . . . . . . . . . 74
USB-LS-LED . . . . . . . . . . . . . . . . . . . . . . . 131
USB2000. . . . . . 17, 62, 80, 92, 105, 124, 131
USB2000-FLG. . . . . . . . . . . . . . . 47, 102, 103
USB4000 . . . 13, 14-19, 56, 80, 124, 167-168
USB4000-FL . . . . . . . . . . . 46, 65-66, 68, 171
USB4000-FL-395 . . . . . . . . . . . . . . 46, 66, 68
USB4000-FL-450 . . . . . . . . . . . 46, 65, 66, 68
USB4000-UV-VIS . . . . . . . . . 34, 37, 167, 176
USB4000-VIS-NIR. . . . . . . . . . . . . 34, 37, 175
UV2 . . . . . . . . . . . . . . . . . . . . . . . . . . . . 22, 24
UV4 . . . . . . 15, 17, 22, 24, 35, s167, 168, 170
Resources
QBIF50-UV-VIS . . . . . . . . . . . . . . . . . . . . . 143
QBIF200-MIXED . . . . . . . . . . . . . . . . . . . . 143
QBIF200-UV-VIS . . . . . . . . . . . . . . . . . . . . 143
QBIF200-VIS/BX . . . . . . . . . . . . . . . . . . . . 143
QBIF200-VIS-NIR . . . . . . . . . . . . . . . . . . . 143
QBIF400-MIXED . . . . . . . . . . . . . . . . . . . . 143
QBIF400-UV-VIS . . . . . . . . . . . . . . . . . . . . 143
QBIF400-VIS-NIR . . . . . . . . . . . . . . . . . . . 143
QBIF600-UV-VIS . . . . . . . . . . . . . . . . . . . . 143
QBIF600-VIS/BX . . . . . . . . . . . . . . . . . 65, 143
QBIF600-VIS-NIR . . . . . . . . . . . . 65, 143, 169
QE65000 . . . . . . . 13, 26-29, 45, 53, 124, 179
QP8-2-SMA . . . . . . . . . . . . . . . . . . . . . . . . 142
QP50-2-UV/BX . . . . . . . . . . . . . . . . . . . . . 142
QP50-2-UV-VIS . . . . . . . . . . . . . . . . . . . . . 142
QP50-2-VIS-NIR . . . . . . . . . . . . . . . . . . . . 142
QP100-2-UV/BX . . . . . . . . . . . . . . . . . . . . 142
QP100-2-UV-VIS . . . . . . . . . . . . . . . . . . . . 142
QP100-2-VIS/BX . . . . . . . . . . . . . . . . . . . . 142
QP100-2-VIS-NIR . . . . . . . . . . . . . . . . . . . 142
QP200-2-SR/BX . . . . . . . . . . . . . . . . . . . . 142
QP200-2-UV/BX . . . . . . . . . . . . . . . . . . . . 142
QP200-2-UV-VIS . . . . . . . . . . . . . . . . . . . . 142
QP200-2-VIS/BX . . . . . . . . . . . . . . . . . . . . 142
QP200-2-VIS-NIR . . . . . . . . . . . . . . . . . . . 142
QP230-0.25-XSR . . . . . . . . . . . . . . . 142, 146
QP230-1-XSR . . . . . . . . . . . . . . . . . . 142, 146
QP230-2-XSR . . . . . . . . . . . . . . . . . . 142, 146
QP300-1-SR . . . . . . . . . . . . . . . . . . . . . . . 142
QP400-025-SR . . . . . . . . . . 92, 142, 167, 170
QP400-025-SR/BX . . . . . . . . . . . . . . . . . . 142
QP400-1-UV-VIS . . . . . . . . . . . . . . . . . . . . 142
QP400-2-SR . . . . . . . . . . . . . . . . . . . . . . . 142
QP400-2-SR/BX . . . . . . . . . . . . . . . . . . . . 142
QP400-2-UV/BX . . . . . . . . . . . . . . . . . . . . 142
QP400-2-UV-VIS. . . . . . . . . 92, 142, 168, 170
QP400-2-VIS/BX . . . . . . . . . . . . . . . . . . . . 142
QP400-2-VIS-NIR . . . . . . . . . . . 142, 172, 173
QP450-0.25-XSR . . . . . . . . . . . . . . . 142, 146
QP450-1-XSR . . . . . . . . . . . . . . . . . . 142, 146
QP450-2-XSR . . . . . . . . . . . . . . . . . . 142, 146
QP600-025-SR . . . . . . . . . . . . . . . . . . . . . 142
QP600-025-SR/BX . . . . . . . . . . . . . . . . . . 142
QP600-025-UV . . . . . . . . . . . . . . . . . . . . . 142
QP600-025-VIS-N . . . . . . . . . . . . . . . . . . . 142
QP600-1-SR, -SR/BX . . . . . . . . . . . . . . . . 142
QP600-1-UV-VIS . . . . . . . . . . . . . . . . . . . . 142
QP600-2-SR . . . . . . . . . . . . . . . . . . . . . . . 142
QP600-2-SR/BX . . . . . . . . . . . . . . . . . . . . 142
QP600-2-UV/BX . . . . . . . . . . . . . . . . . . . . 142
QP600-2-UV-VIS . . . . . . . . . . . . . . . . . . . . 142
QP600-2-VIS/BX . . . . . . . . . . . . . . . . . . . . 142
QP600-2-VIS-NIR . . . . . . . . . . . . . . . . . . . 142
QP1000-2-UV/BX . . . . . . . . . . . . . . . . . . . 142
QP1000-2-UV-VIS . . . . . . . . . . . . . . . 142, 171
QP1000-2-VIS/BX . . . . . . . . . . . . . . . . . . . 142
QP1000-2-VIS-NI . . . . . . . . . . . . . . . . . . . 142
QR200-12-MIXED . . . . . . . . . . . . . . . . . . . 149
QR200-7-series . . . . . . . . . . . . . . . . . . . . . 149
QR200-ANGLE-series . . . . . . . . . . . . . . . . 149
QR200-REF-series . . . . . . . . . . . . . . . . . . 149
QR230-7-XSR/BX . . . . . . . . . . . . . . . 146, 149
QR400-7-series . . . . . . . . . . . . . . . . . . . . . 149
QR400-ANGLE-series . . . . . . . . . . . . . . . 149
QR450-7-XSR . . . . . . . . . . . . . . . . . . 146, 149
QR600-7-series . . . . . . . . . . . . . . . . . . . . . 149
R-3000-QE-532 . . . . . . . . . . . . . . . . . . . 51, 54
R-3000-QE-785 . . . . . . . . . . . . . . . . . . . 51, 54
R-LS-1 and R-LS-1-LL . . . . . . . . . . . . . . . 128
R200-12-MIXED . . . . . . . . . . . . . . . . . . . . 149
R200-7-series . . . . . . . . . . . . . . . . . . . . . . 149
R200-ANGLE-series . . . . . . . . . . . . . . . . . 149
R200-REF-series. . . . . . . . . . . . . . . . . . . . 149
R400-7-series. . . . . . . . . . . 149, 171, 175-177
R400-ANGLE-series . . . . . . . . . . . . . . . . . 149
R600-7-series . . . . . . . . . . . . . . . . . . . . . . 149
REFERENCE . . . . . . . . . . . . . . . . . . . . . . . 111
RESP-BL-series . . . . . . . . . . . . . . . . . . . . . 73
RESP-CL-series . . . . . . . . . . . . . . . . . . . . . 73
RFP200-UV-VIS . . . . . . . . . . . . . . . . . . . . . 76
RIP-PA-SH. . . . . . . . . . . . . . . . . . . . . . . . . . 52
RIP-RP2 . . . . . . . . . . . . . . . . . . . . . . . . . . . 52
RIP-RPB . . . . . . . . . . . . . . . . . . . . . . . . . . . 52
RIP-RPP . . . . . . . . . . . . . . . . . . . . . . . . . . . 52
RIP-RPR-H, RIP-RPR-S . . . . . . . . . . . . . . . 52
RIP-RPS . . . . . . . . . . . . . . . . . . . . . . . . . . . 52
RP200-7-UV-VIS . . . . . . . . . . . . . . . . 148, 149
RPH-1, RPH-2 . . . . . . . . . . . . . . 157, 175-177
RPH-ADP . . . . . . . . . . . . . . . . . . . . . . . . . 157
RSL-PLUS. . . . . . . . . . . . . . . . . . . . . . . 51, 54
RSS-VA, RSS-VA-ADP . . . . . . . . . . . . . . . 109
RT-2MM, -4MM, -5MM, -10MM . . . . . . . . . 150
RTP-2-10, RTP-10-20 . . . . . . . . . . . . . . . . 151
RT-PH . . . . . . . . . . . . . . . . . . . . . . . . . 76, 151
RT-TI-2MM, -5MM, -25MM, -50MM. . . . . . 152
-VVFT with Conflat Flanges . . . . . . . . . . . . . 153
VFT with KF16 ISO Flanges . . . . . . . . . . . 153
VFT with KF40 ISO Flanges . . . . . . . . . . . 153
VFT-series Vacuum Feedthroughs . . . . . . 153
-WWS-1-series. . . . . . . . . . . . . . . . 107, 176, 177
WT-12V . . . . . . . . . . . . . . . . . . . . . . . . 62, 136
WT-12V-E . . . . . . . . . . . . . . . . . . . . . . 62, 136
WT-12V-R-E . . . . . . . . . . . . . . . . . . . . 62, 136
WT-24V . . . . . . . . . . . . . . . . . . . . . . . . . . . 136
-X&ZXY(Z)-150 X150+. . . . . . . . . . . . . . . . . . . . 118
XY(Z)-200X150+ . . . . . . . . . . . . . . . . . . . . 118
XYZ-150 X150X100. . . . . . . . . . . . . . . . . . 118
XYZ-200X150X100 . . . . . . . . . . . . . . . . . . 118
Z-AXIS-100+ . . . . . . . . . . . . . . . . . . . . . . . 118
-TT200-RT-VIS-NIR . . . . . . . . . . . . . . . . . . . 150
T300-RT-UV-VIS . . . . . . . . . . . . . . . . . . . . 150
T300SLEEVE . . . . . . . . . . . . . . . . . . . . . . 151
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INDEX by Alphabetical Order
CAL-2000 Mercury Argon Calibration Source . . . . . . . . . . . . . . . . . . . 134
Calibrated Deuterium Tungsten Halogen Source . . . . . . . . . . . . 120, 132
Calibration
Adapter, Cuvette Wavelength. . . . . . . . . . . . . . . . . . . . . . . . . . . . 135
Service, In-house for Radiometric Sources . . . . . . . . . . . . . 132-133
Service, In-house for fiber optic oxygen sensors . . . . . . . . . . . . . . 74
Source . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 120, 134-135
Standards
Absorbance . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 93
Fluorescence. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 100
Radiometric . . . . . . . . . . . . . . . . . . . . . . . . . . . 57, 132-133, 168
Reflectance Diffuse . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 107
Reflectance Specular . . . . . . . . . . . . . . . . . . . . . . . 108-109, 163
Spectrometer Wavelength . . . . . . . . . . . . . . . . . . . . . . . 134-135
Capillary Electrophoresis . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 99
Carbon Monoxide Monitor . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 75
CC-3 Series Cosine Correctors . . . . . . . . . . . . . . . 57, 104, 133, 147,156
CCD-array Detectors . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 12
Hamamatsu in QE65000 . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 26, 28
In LIBS2500 . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 48
Non-linearity . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 180
RGB Color Filters for . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 162
Sony in HR2000+ . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 24
Toshiba, in HR4000 . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 21, 24
Toshiba, in USB4000 . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 15, 17
Centice Corporation . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 51, 55
CHEM4-series Spectrophotometers for Education . . . . . . . 8-9, 36-37, 76
Discount pricing & Cost Sharing . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 36
Chemiluminescence Assays . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 44
C-mount Adapter . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 157
Coating
Microlithography . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 161
Optical. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 162
Recoating Service . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 73
Sensor . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 64, 68
Services . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 64
Technology . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 160
Types . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 160
Collection Lens
For USB4000 Optical Bench . . . . . . . . . . . . . . . . . . . . . . . . . . 15, 17
For HR Optical Bench . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 22, 24
For QE65000 OPtical Bench . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 28
Collimating Lens . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 60, 86, 88, 156
Accessories . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 89, 157
Collimating Mirror. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 15, 22, 27
Collimation Testers . . . . . . . . . . . . . . . . . . . . . . . . . . . . 111, 160, 162-163
Color Measurement . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 177
Optical Bench Type . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 12
Tools for LED measurement. . . . . . . . . . . . . . . . . . . . . . 56, 105, 120
Color-correcting & Signal-attenuating Accessories . . . . . . . . . . . . . . . 128
Composite-grating . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 35
Compound ID Software . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 83
Conflat Flanges . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 153
Connectors, Custom-drilled . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 154
Contact Information
Customer Sales and Service . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 10
Distributors . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 4
Education Division . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 9
Ocean Optics Offices . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 5
OEM Opportunities . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 7
Cosine Correctors . . . . . . . . . . 57, 86, 104, 132-133, 147, 156, 168, 173
Cross Process Flow Cells . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 96
Curricula and Other Resources . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 9
Curved Surface Probe Holders . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 157
Custom Fiber
Fiber Options. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 140-141
Fiber & Probe Online Quoting Website . . . . . . . . . . . . . . . . . . . . 139
Filters . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 162
Custom Sensors & Technology . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 96
Customer Service . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 10
Cuvette. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 93
Covers for . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 93
Cylindrical Cell . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 170
Disposable . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 93
Holders
Adapter . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 115
Adjustable Collimating Lens and Cuvette Holder . . . . . . . . . . 89
Direct-attach . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 90, 100
For Absorbance and Fluorescence . . . . . . . . . . . . . . . . . . . . . 90
186
For all your sensing needs, visit OceanOptics.com
74-series Lens Fixtures . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 88
84-series Lens Fixture . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 88
Resources
-AA/D Converters . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 30, 37, 42, 80, 84
Absolute Irradiance. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 56-57, 81, 172
Absorbance . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . .
Accessories . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 87
Beer's Law . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 38, 178
Filters . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 15-16, 22-23, 27, 164
Gas . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 170
Set-up . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 167, 170
Solution. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 99, 167
With TLC-50F . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 91
Absorbance/Transmission Accessories . . . . . . . . . . . . . . . . . . . . . . . . . 87
Absorbing Glass Filters . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 164
Absorption Wavelength Bands for Chromophores . . . . . . . . . . . . 178-179
Absorption Wavelength Cutoffs for Solvents . . . . . . . . . . . . . . . . . . . . 179
Absorption/Emission for Fluorophores . . . . . . . . . . . . . . . . . . . . . 180-182
Accessories
Light Sources. . . . . . . . . . . . . . . . . . . . . . . . . . . . . see Light Sources
Sampling Accessories . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 85-118
USB4000 Direct-attach. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 19
Acrylic Sampling Chambers. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 73
ADC1000-USB A/D Converter. . . . . . . . . . . . . . . . . . . . . . . 42, 79, 80, 84
ADC2000-PCI+ PCI-bus A-to-D Converter . . . . . . . . . . . . . . . . . . . . . . 84
ADC-USB-SER Serial Cable . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 79, 84
Adjustable Collimating Lens Holder. . . . . . . . . . . . . . . . . 60, 89, 105, 113
ALine, Inc. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 103
Analog-to-Digital Converters . . . . . . . . . . . . . . . . . . . . . 30, 37, 42, 80, 84
Angled Probes . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 148
Antireflective Coatings . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 162
Applications. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 166-177
Database of . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 10
NIR Series . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 31
AR-1 Argon Wavelength Calibration Standard. . . . . . . . . . . . . . . . . . . 135
Asian Operations . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 5
ASP Annual Service Package . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 62
Astronomy . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 26, 166
Attenuation
Accessories . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 128
Spectra for each fiber type . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 139
Attenuator . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 117, 121, 129, 156
Automate Wet Lab Procedures . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 95
-BBack-thinned TE-cooled Detector for QE65000 . . . . . . . . . . . . . . . 12, 28
Balanced Deuterium Tungsten Light Source . . . . . . . . . . . . . . . . . . . . 122
Balancing Filters . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 121, 164
Bandpass Filters . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 114, 121, 162, 164
Bare Fiber Adapter Kit . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 154
Bare (Unjacketed) Fiber. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 143
Beamsplitter . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 112, 161
Beer's Law . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 9, 38, 81, 167, 178
BG34 Optical Filter. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 164
Bifurcated Optical Fiber Assembly. . . . . . . . . . . . . . . . . . . . 116, 145, 169
Laboratory grade . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 145
Premium grade . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 143
With splice bushing. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 72
Big Sky Laser Technologies. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 49
BK7 Glass . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 15, 22, 24, 88
Blaze Wavelength . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 16, 23, 28
Blocking Filters . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 16, 23, 27, 121
Breakout Box . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 61, 124
Bulbs, Power Supplies & Accessories . . . . . . . . . . . . . . . . . . . . . . . . . 136
Bulk Fiber. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 143, 154
Bulkhead & Splice Bushing Combo . . . . . . . . . . . . . . . . . . . . . . . . . . . 158
Bulkhead Bushing . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 156, 158
-C-
oo
oo
INDEX by Alphabetical Order
Temperature-regulated . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 91
Integrated Sampling Systems . . . . . . . . . . . . . . . . . . . . . . . . . 92
Wavelength Calibration Adapter . . . . . . . . . . . . . . . . . . . . . . 135
Mirror Plugs . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 91
Quartz . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 93
Cuvette Wavelength Calibration Adapter . . . . . . . . . . . . . . . . . . . . . . . 135
-D-
-EEducation
Division . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 9
Spectrometers . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 36-39
Spectroscopy Grant Program . . . . . . . . . . . . . . . . . . . . . . . . . . . 8, 36
Educator Training. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 9
Efficiency Curves
For Gratings H1-7, 9-12, 14 . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 18
For HC-1. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 23
For N1 and N2 Gratings . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 32
For QE65000 Detector . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 28-29
Electronic TTL Shutter . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 116
Ellipsometer System . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 59
Emission . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 104-105
Cosine Correctors. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 104
Tel: 727.733.2447 • Email: [email protected]
-FFC Barrel . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 136, 156, 158
Fedora Core. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 82
Feedthroughs. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 137, 153
Ferrule Options . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 141
Ferruled Fibers. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 94
FIA Cells Flow Injection Analysis System . . . . . . . . . . . . . . . . . . . . . . . 94
FIAlab Instruments . . . . . . . . . . . . . . . . . . . . . . 43-44, 86, 94-95, 100-101
FIA-PMT-FL Photomultiplier Flow-through Detection System . . . . 44, 101
FIA-SIA Micro Sequential Injection Analyzer . . . . . . . . . . . . . . . . . . . . . 95
FIA-SIA-LOV Lab-On-Valve System . . . . . . . . . . . . . . . . . . . . . . . . . . . 95
FIA-SMA-FL Fluorescence Flow Cell. . . . . . . . . . . . . . . . . . . . . . . . . . 100
FIA Cells. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 94
Fiber
Accessories . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 158
Adapter Kit . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 154
Assemblies
Anatomy . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 138
Custom Options . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 139-141
Laboratory-grade Optical Fiber . . . . . . . . . . . . . . . . . . . . . . . 144
Premium-grade Optical Fiber. . . . . . . . . . . . . . . . . . . . . 142-143
Xtreme Solarization-resistant . . . . . . . . . . . . . . . . . . . . . . . . 146
Boot Collar Colors . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 138
Bulk. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 143
Bundle for LIBS . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 48, 174
For CHEM4. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 37
Connector Adapters . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 141
Custom . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 139-141
Epoxy Options . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 141
Ferrule Options. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 141
For Use with FIA Cells . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 94
Fixtures & Holders . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 157
Jacketing Options . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 140
Laboratory-grade . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 144-145
Modemixer/Modestripper . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 158
Overview. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 138
Premium-grade . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 142-143
Quoting Website . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 139
Solarization-resistant . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 146
Termination Kit . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 155
Tinkerer's Kit. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 154
Wrap . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 158
Wrench . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 156, 158
Fiber Jacketing . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 138, 142-143, 149
Premium-grade Assemblies . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 142
Premium-grade Bifurcated Assemblies . . . . . . . . . . . . . . . . . . . . 143
Reflection/Backscattering Probes. . . . . . . . . . . . . . . . . . . . . . . . . 149
Fiber Optic
Dual Switch with TTL Line . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 116
Kits . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 156
Oxygen Probes, Chemical Compatibility . . . . . . . . . . . . . . . . . . . . 69
Oxygen Sensor Probes . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 70-71
pH Sensors. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 76
Probe . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 147
Scanning Monochromator . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 101
Variable Attenuator . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 117, 121
Fiber Type, Attenuation Spectra. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 139
Field of View . . . . . . . . . . . . . 56-57, 86, 88, 104-106, 116, 147, 168, 181
187
Resources
Data Acquisition . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 78-79
Datalogger . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 39
Deep Well Detector Spectrometer . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 42
Detector Sensitivity Comparison . . . . . . . . . . . . . . . . . . . . . . . . . . . 17, 24
Detectors
Hamamatsu G9204-512 InGaAs . . . . . . . . . . . . . . . . . . . . . . . . . . 32
Hamamatsu G9206-256 InGaAs . . . . . . . . . . . . . . . . . . . . . . . . . . 32
Hamamatsu G9204-512 InGaAs . . . . . . . . . . . . . . . . . . . . . . . . . . 32
Hamamatsu S3903 and S3904 . . . . . . . . . . . . . . . . . . . . . . . . . . . 42
Hamamatsu S7031 Back-thinned CCD . . . . . . . . . . . . . . . . . . 12, 28
Sony ILX511 Linear CCD . . . . . . . . . . . . . . . . . . . . . . . 12, 17, 24, 25
Toshiba TCD1304AP Linear CCD . . . . . . . . . . . . . . 17, 21-22, 24-25
Detectors, Accessories for . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . .
Deep Well Detector Spectrometers . . . . . . . . . . . . . . . . . . . . . . . . 42
HR-series Optical Bench Options. . . . . . . . . . . . . . . . . . . . . . . . . . 24
QE-series Optical Bench Options. . . . . . . . . . . . . . . . . . . . . . . . . . 28
Sensitivity Comparison, HR-series Options . . . . . . . . . . . . . . . . . . 24
Sensitivity Comparison, USB-series Options . . . . . . . . . . . . . . . . . 17
Detectors, Specifications for
HR-series . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 24
NIR-series. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 30
QE65000. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 28
USB-series . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 17
Deuterium Light Sources . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 120, 126
Deuterium Tungsten Halogen Light Sources . . . . . . . . 120, 123-125, 178
Device Drivers . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 82
DH2000 Deuterium Tungsten Light Sources. . . . . . . . 120, 123, 136, 167
DH2000-BAL Deuterium Tungsten Light Source. . . . . . . . . 122, 167, 176
DH2000-CAL Radiometric Calibration Standard . . . . . . . . . . . . . 132, 168
Dichroic Coatings & Filters . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 160-162
Diffuse Reflectance Standard . . . . . . . . . . . . . . . . . . . . . . . . 107, 176-177
Diffuser for Redirecting Excitation Light INLINE-TTL-S . . . . . . . . . . . . 115
Digital Transform Spectroscopy (DTS) . . . . . . . . . . . . . . . . . . . . . . . . . 40
Direct-attach Accessories
Cuvette Holder . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 90, 100
Filter Holder . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 19
Integrating Sphere . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 105
LED Light Source . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 131
Light Source . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 19, 36
Sampling System for Cuvttes . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 19
Test Tubes . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 19
For CHEM4-series . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 36
For USB4000 . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 19
Disposable
Cells for Fluorescence . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 103
Cuvettes, UV & VIS . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 93
Dissolved Oxygen Measurements. . . . . . . . . . . . . . . . . . . 64, 68, 73, 169
Distributors . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 6
Downwelling Measurement . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 168
DTS-PHAZIR-series NIR Spectrometers . . . . . . . . . . . . . . . . . . . . . . . . 40
Integrating Sphere . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 105
Sample Spectrometer Setups . . . . . . . . . . . . . . . . . . . . . . . . 171-174
Sampling Accessories . . . . . . . . . . . . . . . . . . . . . . . . 87-88, 104-105
Selected Fluorophores, Wavelengths of . . . . . . . . . . . . . . . . 180-182
Spectrometers . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 21, 44, 47-50, 59
Wavelength Library. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 83
Emissive Color. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 81, 104, 147
Entrance Slits . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 15, 22, 27, 32, 121
Epoxy Options . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 141
ETC Source Four Ellipsoidals . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 162
European Operations. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 5
Evident Technologies . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 102
EviDot & EviTag Nanocrystals . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 102
Excitation Sources
Laser . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 48-50, 52
LED. . . . . . . . . . . . . . . . . . . . . . . 26, 44, 51-53, 65-66, 120, 130-131
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Resources
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INDEX by Alphabetical Order
Filter Holders
& Cuvette Holder . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 113
CUV-TLC-FH . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 91
In-line . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 113, 115, 121, 164
For Linear Variable Filters. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 115
For Optical Fibers . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 113
Sample Holders . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 113
USB-FHS . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 19
Filtering Technology . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 114, 122, 167
Filters
Absorbing . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 15-17, 23, 27, 164
Balancing . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 121, 164
Bandpass . . . . . . . . . . . . . . . . . . . . . . . . . . . 114, 121, 160, 162, 164
Blocking . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 16, 23, 27, 121
Custom . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 162
Dichroic. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 160
Glass. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 164
High-pass . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 164
Inline-OF . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 113, 164
Linear Variable. . . . . . . . . . . . . . . . . . . . . . . . . . . . 109, 114-115, 121
Longpass Blocking . . . . . . . . . . . . . . . . . . . . . . . . 15-17, 23, 27, 164
Loose . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 121
For LS-1 Light Source . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 128
Order-sorting Filters OF1 . . . . . . . . . . . . . . . . . . . . . . 16, 23, 27, 164
Order-sorting Filters OF2 . . . . . . . . . . . . . . . . . . . . . . . . . . . 128, 164
Order-sorting Filters OFLV . . . . 15, 17, 22, 24, 27-28, 167, 172, 175
Use in Spectrometers . . . . . . . . . . . . . . . . . . . . . 16-17, 22-24, 27-28
Finger Fiber Wrench . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 158
Flame Loop Fiber Optic Probe . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 147
Flow
Cell Kit for Flow Injection Analysis . . . . . . . . . . . . . . . . . . . . . . . . . 95
Cells . . . . . . . . . . . . . . . . . . . . . . . . . . . 34, 43, 94-98, 100, 103, 167
Injection Analysis System . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 43
Injection PMT System. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 44
Fluid Analysis . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 86
Fluorescein, Spectra of . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 103
Fluorescence
Excitation Sources. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 130-131
Filters for. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 164
Flow Analysis System. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 44, 101
Flow Cell. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 97, 100
& Luminescence . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 182
Measurement Tools . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 44-47
Probes for . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 148
Process Flow Cells . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 97
Sampling Tools . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 100
Set-ups for . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 169, 171
Spectrometers . . . . . . . . . . . . . . . . . . . . . . . . 26, 45-47, 66, 130-131
Fluorophores, Emission Wavelengths of Selected . . . . . . . . . . . . 180-182
FluoroVette Micro-volume Cells . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 103
Focusing Mirror . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 15-16, 22-23, 27
FOIS-1 Fiber Optic Integrating Sphere . . . . . . 56-57, 104, 105, 172, 173
Forensics . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 48, 51, 166
FOSPOR Fiber Optic Oxygen Sensor Coating . . . . . . . . . . 46, 68, 70-72
FOXY Fiber Optic Oxygen Sensor Coating . . . . . . . . . . . . . . . . 46, 68-71
Fused Silica Optical Flats. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 110
-GGas Absorbance . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 21, 170
Gated Fluorescence Mode . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 47
Gated Spectrometer for Fluorescence. . . . . . . . . . . . . . . . . . . . . . . . . . 47
Gershun Tube Kit . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 87, 116
GOBOs. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 162
GRAMS SPC format . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 81
Grant Program . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 8-9, 36, 166
Gratings
Efficiency Curve, HC-1 Grating . . . . . . . . . . . . . . . . . . . . . . . . . . . 23
Efficiency Curves, "HR" Optical Bench Options . . . . . . . . . . . . . . . 25
Efficiency Curves, "NIR" Optical Bench Options . . . . . . . . . . . . . . 32
Efficiency Curves, "QE" Optical Bench Options . . . . . . . . . . . . . . . 29
Efficiency Curves, "S" Optical Bench Options . . . . . . . . . . . . . . . . 18
Grating HC-1 . . . . . . . . . . . . . . . . . . . . . . . . . 13, 23, 28, 35, 60, 168
Grating HC-1QE . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 28
Gratings H1-H14 . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 23, 28-29
Gratings N1-N2. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 30, 32
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188
Location in Optical Bench . . . . . . . . . . . . . . . . . . . . . . . . . 15, 22, 27
Selection Chart, "HR" Optical Bench . . . . . . . . . . . . . . . . . . . . . . . 23
Selection Chart, "NIR" Optical Bench. . . . . . . . . . . . . . . . . . . . . . . 32
Selection Chart, "QE" Optical Bench . . . . . . . . . . . . . . . . . . . . . . . 28
Selection Chart, "S" Optical Bench . . . . . . . . . . . . . . . . . . . . . . . . 16
-HHamamatsu
Back-thinned Area CCD Detector . . . . . . . . 12-13, 26, 28, 45, 51-52
InGaAs Linear Array Detectors . . . . . . . . . . . . . . . . . . . . . . . . 30, 32
Linear Photodiode Array Detectors . . . . . . . . . . . . . . . . . . . . . 42, 51
HC-1 Composite Grating . . . . . . . . . . . . . . . . . . . . 13, 23, 28, 35, 60, 168
Heat-resistant Fiber Optic Probe . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 147
HG-1 Mercury Argon Calibration Standard . . . . . . . . . . . . . . . . . . . . . 135
High-pass Filters . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 114, 121, 164
High-resolution Spectrometers
Break-out Box . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 61-62, 124
HR2000 High-resolution Spectrometer. . . . . . . . . . . . . . . . . . . . . . 48
HR2000+ High-resolution Spectrometer13, 20, 22-25, 61, 79, 80, 124,
179
HR4000 High-resolution Spectrometer12-13, 21-25, 35, 52, 60-61, 79,
80, 104, 124, 168, 170, 173, 179
HR4000CG-UV-NIR Broadband Spectrometer . . . . . . . . . . . . . . . 35
HIOXY Fiber Optic Oxygen Sensor Coating . . . . . . . . . . . . . . . 46, 68-74
Holders
Cuvette . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . see Cuvette Holders
Filter . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . see Filter Holders
Lens . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 157
Probe . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 157
Sample . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . see Sample Holders
"HR" Optical Bench Options . . . . . . . . . . . . . . . . . . . . . . . . . . . 20, 22-25
Choosing a Grating & Wavelength Range . . . . . . . . . . . . . . . . . . . 23
Collimating & Focusing Mirrors . . . . . . . . . . . . . . . . . . . . . . . . . 22-23
Detector . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 22, 24
Fixed Entrance Slit . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 22
Grating Selection Chart . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 23
HC-1 Grating Efficiency Curve . . . . . . . . . . . . . . . . . . . . . . . . . . . . 23
L2 or L4 Detector Collection Lens . . . . . . . . . . . . . . . . . . . . . . . . . 24
Longpass Absorbing Filters . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 23
Predicted Ranges & Resolution . . . . . . . . . . . . . . . . . . . . . . . . . . . 25
SAG+UPG-HR . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 23
SMA 905 Connector . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 22
Sony Detector. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 25
Toshiba Detector. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 25
HR2000+ High-resolution Spectrometer . . . . . 13, 20, 22-25, 61, 80, 124
HR4000 High-resolution Spectrometer . . . . 13, 21-25, 52, 60-61, 80, 124
HR4000CG Composite-grating Spectrometer . . . . . . . . . . . . . . . . . . . . 35
HR4-BREAKOUT Box . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 61-62, 124
-IIndustrial Process Probe . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 152
In-line Filter Holders. . . . . . . . . . . . . . . . . . . . . . . . . . . 113, 115, 121, 164
In-line Flow Cell . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 73
Inline-OF Filters . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 113, 164
Innovations in Educational Spectroscopy Grant Program . . . . . . . . . . . . 8
Instant Elemental Analysis . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 48
Integrated Sampling Systems . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 19, 92
Integrating Spheres . . . . . . . . 21, 56-57, 87, 105-106, 133, 172-173, 177
Irradiance . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 56-57, 120
Calibrated Light Sources . . . . . . . . . . . . . . . . . . . . . . . . . . . . 132-133
Probes . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 104, 147
Sample Setups . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 168, 172-173
Software . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 81
- J, K Java Programming Language . . . . . . . . . . . . . . . . . . . . . . . . . . 78, 80-82
KF ISO Flanges . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 153
-LL2 Detector Collection Lens . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 24, 42
L4 Detector Collection Lens . . . . . . . . . . . . . . . . 15, 17, 24, 46, 56, 65-66
Lab-On-Valve Technology . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 95
For all your sensing needs, visit OceanOptics.com
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INDEX by Alphabetical Order
-MMapping Tables . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 118
MeasureNet Technology Ltd . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 9
MEMS-based NIR Spectrometer . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 40
Mercury Argon Calibration Sources . . . . . . . . . . . . . . . . . . . . . . . . . . . 134
Metrology . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 48, 118, 160-162, 175
MFA-PT Phototubus Microscope Adapter . . . . . . . . . . . . . . . . . . . . . . 157
Micro Process Flow Cells . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 96
Micro Sequential Injection Analyzer. . . . . . . . . . . . . . . . . . . . . . . . . . . . 95
Microlithography . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 118, 160-161
Microscope Accessories . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 157
Miniature Deuterium Tungsten Halogen Light Source. . . . . . . . . . 60, 125
Mirrored Screw Plugs . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 90, 100, 171
Mirrors . . . . . . . . . . . . . . . . . . . . . . . . . 12, 15-16, 22-23, 27, 47, 110, 160
Monochromator . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 36, 72, 101
MonoScan2000 . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 101
MPM-2000 Fiber Optic Multiplexer . . . . . . . . . . . . . . . . . . . . . . . . . . . 117
MultiFrequency Phase Fluorometer . . . . . . . . . . . . . . . . . . . . 65, 67, 169
Tel: 727.733.2447 • Email: [email protected]
Multimodal Multiplex Spectrometer (MMS) Raman Spectrometer. . 51, 55
Multimode Diode Laser . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 21
Multiplexer, Optical . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 117
Multipoint Sampling . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 42, 117
-NN1 and N2 Grating Efficiency . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 32
NanoCalc Thin Film Reflectometry System . . . . . . . . . . . . . . . . . . . . . . 58
Nanocrystals . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 102
NanoDrop Technologies. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 7
Nanopositioner . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 118
"NIR" Optical Bench Options
Detectors . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 32
Fixed Entrance Slits . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 32
Grating Efficiency Graphs. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 32
N1 Grating Efficiency . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 32
N2 Grating Efficiency . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 32
NIR-series Applications . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 31
NIR Spectrometers
MEMS-based . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 40
NIR256 Extended-range . . . . . . . . . . . . . . . . . . . . . . . . . . 30-32, 179
NIR-512 Near-infrared. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 30-31
NIST-traceable
Absorbance Standards . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 93, 167
Calibration Standards . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 57, 132
LED-PS-NIST LED Power Supply . . . . . . . . . . . . . . . . . 56, 104, 172
Optical. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 111, 163
Radiometric Standards . . . . . . . . . . . . . . . . . . . . . . . . . . 57, 132-133
Raman Standards. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 53
Reflectance Standards . . . . . . . . . . . . . . . . . . . . . . . . . 107-109, 163
Non-Linearity, of CCDs . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 180
NTS-series Linear Nanopositioners . . . . . . . . . . . . . . . . . . . . . . . . . . . 118
-OOcean Optics Software & Hardware Compatibility . . . . . . . . . . . . . . . . 79
OEM . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 7
OF1 Filters . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 13, 16, 23, 27, 164
OF2 Filters . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 128, 164
OFLV Order-sorting Filters . . . . . . . . . . . . . . . . . 15, 17, 22-24, 27-28, 60
OFLV-200-850 . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 13, 17, 34, 167
OFLV-200-1100. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 35
OFLV-350-1000 . . . . . . . . . . . . . . . . . . 13, 17, 34, 56, 172, 175, 177
OFLV-350-DW . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 42
OFLV-DW . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 42
OFLV-H4 . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 13
OFLV-QE . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 13, 28
OMNI+SPAM . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 82
OmniDriver Spectroscopy Development Platform . . . . . . . . . . . . . . 78, 82
Onboard Microcontroller . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 21
OOILIBS Software . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 48, 174
OOINLCorrect Software. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 180
OOISensors Software. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 74-76, 169
Optical Bench Options . . . . . . . . . . . . . . 12, 15-18, 20, 22, 27, 34, 35, 38
Optical Benches
“HR” Optical Bench . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 20, 22-25
“NIR” Optical Bench . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 12, 32
Overview. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 12
“QE” Optical Bench . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 27-29
USB4000 Optical Bench . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 15-18
Optical Fiber Assemblies . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 139-146
Bifurcated Fiber Assemblies. . . . . . . . . . . . . . . . . . . . . . 72, 143, 145
Custom . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 139-141
For Use with FIA Cells . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 94
Jacketing Options . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 140
Kits . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 156
Laboratory Grade . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 144-145
Overview. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 138
Solarization-resistant Assemblies. . . . . . . . . . . . . . . . . . . . . . . . . 146
Splitter Optical Fiber Assemblies . . . . . . . . . . . . . . . . . . . . . . . . . 145
Optical Flats . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 110, 163
Optical Multiplexer . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 117
Optical O2 Sensors vs. Electrodes . . . . . . . . . . . . . . . . . . . . . . . . . . . . 64
Optical Post-mount Assembly . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 89
Optical Resolution . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 21, 48, 179
189
Resources
Laboratory-grade Assemblies
Bifurcated Optical Fiber Assemblies . . . . . . . . . . . . . . . . . . . 72, 145
Patch Cord Assemblies . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 144
Solarization-resistant Assemblies. . . . . . . . . . . . . . . . . . . . . . . . . 146
Splitter Optical Fiber Assemblies . . . . . . . . . . . . . . . . . . . . . . . . . 145
Labsphere . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 107
Lasers . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 49- 54, 104-105, 147
Analysis . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 21, 173
Characterization . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 31
Diodes. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 44
Laser-induced Breakdown Spectroscopy . . . . . . . . . . . . . . . . . 48-50, 174
LED Light-emitting Diodes
Analysis . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 172
Excitation Source . . . . . . . . . . . . . . . . . . . . . . . . . . . 19, 65, 130-131
Light Sources . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 19, 130-131
Options Available . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 130, 136
Measurement Tools . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 56, 104-105
Power Supply . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 56, 104, 172
LIBS2500 Laser-induced Breakdown Spectrometer . . . . . . . . 48-49, 174
Sample Chamber . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 49
System Software . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 48
Components . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 49
Imaging Module . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 49
Laser Options . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 49
Sample Chamber . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 49
Setup . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 172
LIBS-ELITE Laser Ablation System . . . . . . . . . . . . . . . . . . . . . . . . . . . . 50
Light, Ways to Modify. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 121
Light Sources . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 120
Balanced Deuterium Tungsten Source. . . . . . . . . . . . . . . . . . . . . 122
Bulbs, Power Supplies and Accessories . . . . . . . . . . . . . . . . . . . 136
Calibrated. . . . . . . . . . . . . . . . . . . . . . 56-57, 105,120, 133, 168, 172
Deuterium Sources. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 126
Deuterium Tungsten Halogen Sources . . . . . . . . . . . . . . . . . 123-124
LED Light Sources . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 130-131
Mini Deuterium Tungsten Halogen Sources. . . . . . . . . . . . . . 60, 125
Overview . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 120-121
Radiometric Calibration Standards . . . . . . . . . . . . . . . . . . . . 132-133
Tungsten Halogen Sources . . . . . . . . 20, 34, 128-129, 167, 175-177
Wavelength Calibration Standards . . . . . . . . . . . . . . . . . . . . 134-135
Xenon Sources . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 120, 127
Light-emitting Diodes . . . . . . . . . . . . . . . . see LED Light-emitting Diodes
Line Identification, Tools for Atomic Emission . . . . . . . . . . . . . . . . . 41, 83
Linear CCD Array Detector . . . . . . . . . . . . . . . . 13-15, 17, 22, 24, 32, 48
Linear Variable Filters . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 114, 121
Accessories. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 115
Linux Operating System. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 82
Lithium Ion Battery Pack . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 62
Long Pathlength Process Flow Cells . . . . . . . . . . . . . . . . . . . . . . . . . . . 97
Long Trace Profilometer. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 112
Longpass Filter . . . . . . . . . . . . . . . . . . . . . . . . . . . . 15-16, 22-23, 27, 121
LPC-series Longpass Flow Cells. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 98
LS-1 and LS-1-LL Spectral Output. . . . . . . . . . . . . . . . . . . . . . . . . . . . 128
LS-450 Blue LED. . . . . . . . . . . . . . . . . . . . . . . . . . . 62, 66, 103, 130, 136
LS-475 Blue LED Light Source . . . . . . . . . . . . . . . . . . . 62, 103, 131, 136
Luminescence Measurement. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 67
oo
oo
INDEX by Alphabetical Order
Optical Stages . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 157
Optics
Capabilities . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 161
High-precision. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 160
Transmission Tools . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 60
Order-sorting Filters . . . . . . . . . . . . . . . . . see OFLV Order-sorting Filters
Original Equipment Manufacturer . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 7
Overcoats. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 69, 72
Oxides. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 79, 160-161
Oxygen Acrylic Sampling Chambers . . . . . . . . . . . . . . . . . . . . . . . . . . . 73
Oxygen Medical Diagnostics . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 169
Oxygen Sensor Phase Fluorometer . . . . . . . . . . . . . . . . . . . . . . . . 65, 67
Oxygen Sensors
Accessories . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 64-75
Calibration. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 74
Care . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 63
Coating Formulations . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 68
Operation . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 65
Overcoats . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 72
Overview. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 64
Planar . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 72
Probes . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 70-71
Reconditioning/Recoating. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 73
Software . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 75
Spectrometers . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 66
Temperature Compensation . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 74
Oxygen Sensing With MultiFrequency Phase Fluorometer. . . 65, 67, 169
Ozone. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 69
Resources
-QQBIF-series Bifurcated Optical Fiber Assembly . . . . . . . . . . . . . . 72, 143
QE65000 Scientific-grade Spectrometer. . . . 12-13, 19, 26-28, 45, 51, 53
QR-series Reflection Probes . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 149
Q-series Premium-grade Patch Cord Assemblies . . . . . . . . . . . . . . . . 142
Quantum Dots . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 102
Quartz Cuvette Cells . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 93
-R-
Partnership . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 6-7
PASCO Scientific . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 9, 38-39
Patch Cord Optical Fiber Assembly . . . . . . . . . . . . . . . . . . . . . . . . . . . 130
PC Adapter Package for Temperature-regulated Cuvette Holder . . . . . 91
PCI -bus A/D Cards . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 78, 84
Peristaltic Pump . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 43, 95
pH Sensors . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 76
Phazir Handheld NIR Material Analyzer . . . . . . . . . . . . . . . . . . . . . . . . 40
Phenol Red pH Test Kit . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 76
Photodiode Detectors . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 12
Photoluminescence-quenching . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 68
Photometric Absorbance Standards . . . . . . . . . . . . . . . . . . . . . . . 93, 167
Photomultiplier Flow-through Detection System . . . . . . . . . . . . . . 44, 101
Phototubus Microscope Adapter . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 157
PIP-10-2 SpectroPipetter Microcell . . . . . . . . . . . . . . . . . . . . . . . . . . . . 98
Pixel Resolution, of Spectrometers . . . . . . . . . . . . 15, 22, 27, 32, 49, 179
Pixel Size
HR-series . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 13, 21
HR2000+ . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 20
NIR-series. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 30
QE65000 . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 13, 26
S-series . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 13-14
Planar Oxygen Sensors . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 72
PlasCalc Measurement System. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 59
Plasma Monitoring . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 59
PMT-FL Flow Through Fluorometer. . . . . . . . . . . . . . . . . . . . . . . . 44, 101
Pocket Carbon Monoxide Meter . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 75
Polychromix DTS NIR Spectrometer . . . . . . . . . . . . . . . . . . . . . . . . . . . 40
Positioning Stages . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 118
Positive Displacement Pump . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 99
Power Supplies . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 62
& Controller for LEDs . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 104
Premium Grade SMA Connectors . . . . . . . . . . . . . . . . . . . . . . . . . . . . 155
Premium-grade Assemblies
Bifurcated Optical Fiber Assemblies. . . . . . . . . . . . . . . . . . . . . . . 143
Patch Cord Assemblies . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 142
Solarization-resistant Assemblies. . . . . . . . . . . . . . . . . . . . . . . . . 146
Prisms . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 110, 160, 163
Probe
Accessories . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 158
Assemblies . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 138-146
Connector Adapters . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 141
Cosine-corrected Irradiance Probe . . . . . . . . . . . . . . . . . . . . . . . 147
Epoxy Options . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 141
Ferrule Options. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 141
Radiometric Calibration Standards
UV-NIR . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 132
VIS-NIR. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 133
Radiometric Reference Source . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 56
Raman
Analyzers for. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 54
Applications . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 51
Fiber Optic Probes . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 52
Handheld System . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 54
Key Applications . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 55
Laser for . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 52
Measurement Systems. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 54
Measurement Tools . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 52-53
Multimodal Multiplex Spectroscopy . . . . . . . . . . . . . . . . . . . . . 51, 55
Probes for . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 52
Selection Guide . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 51
Spectrometers for . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 26, 51, 53-55
Raman NIST-traceable Standards . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 53
Rayleigh . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 51-52
Red Tide Spectrometer . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 38
RedHat . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 82
Reference Wafer . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 111
Reflectance Standards
Diffuse . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 107, 176-177
Specular . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 108, 163, 176
Reflectance/Reflection
Probe Holder . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 34, 157, 175-177
Probe Holder Adapter . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 157
Probes . . . . . . . . . . . . . . . . . . . . . . . . . . . . 34, 76, 148-149, 175-176
Sampling System . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 109
Sampling Accessories, Color . . . . . . . . . . . . . . . . . . . . . . . . . 56, 107
Sampling Accessories, Metrology . . . . . . . . . 106, 108-109, 112, 175
Sampling Accessories, Optical . . . . . . . . . . . . . . . . . . . . . . . . . . . 108
Stage. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 109
Standards Holder . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 108
Standards, Reflectance Diffuse . . . . . . . . . . . . . . . . . . . . . . . . . . 107
Standards, Reflectance Specular . . . . . . . . . . . . . . . . . 108-109, 163
Reflective Indicator Dye Films . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 76
Relative Irradiance. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 36, 57, 81
Repair Fibers . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 155
Respiration Monitor . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 72
Respirometers . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 73
RESP-series Acrylic Sampling Chambers . . . . . . . . . . . . . . . . . . . . . . . 73
Reticles . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 161-162
Return Merchandise Authorization (RMA) . . . . . . . . . . . . . . . . . . . . . . . 10
Right-angle Collimating Lens Holder . . . . . . . . . . . . . . . . . . . . . . . 89, 157
RIP-series Raman Probes . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 52
RPB Laboratory Probe. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 52
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Fixtures . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 157
Flame Loop Fiber Optic Probe . . . . . . . . . . . . . . . . . . . . . . . . . . . 147
Heat-resistant Fiber Optic Probe . . . . . . . . . . . . . . . . . . . . . . . . . 147
Holder . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 157
Industrial Process Probe . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 152
Jacketing Options . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 140
Oxygen Sensor . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 70-72
Reflection/Backscattering Probes . . . . . . . . . . . . . . . . . . . . . 148-149
Transmission Dip Probe . . . . . . . . . . . . . . . . . . . . . . . . . . . . 150-151
Process2000 Process Control System . . . . . . . . . . . . . . . . . . . . . . . . . 41
Process-grade Assemblies . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 137
Pt-porphyrin Coating for FOSPOR Probe . . . . . . . . . . . . . . . . . . . . 65, 68
Pulsed Blue LED Light Source . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 131
Pulsed Xenon Lamps. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 120, 127
Pump, Positive Displacement . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 73, 99
PVC Monocoil . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 140, 150
oo
INDEX by Alphabetical Order
R-series Fiber Optic Reflection Probe . . . . . . . . . . 34, 148-149, 175-176
RSL-PLUS Handheld Raman Spectrometer . . . . . . . . . . . . . . . . . . 51, 54
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Tel: 727.733.2447 • Email: [email protected]
191
Resources
S1024DW Deep Well Series Spectrometers . . . . . . . . . . . . . . . . . . . . . 42
SAG+ High-reflectivity Mirrors . . . . . . . . . . . . . . . . 12, 16, 23, 27, 47, 171
Sample Cells . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 93
Sample Chamber, LIBS . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 49-50
Sample Holders
Filter . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 113
Fluorovette . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 103
Integrated Sampling Systems . . . . . . . . . . . . . . . . . . . . . . . . . . . . 92
USB4000 Direct-attach Accessories. . . . . . . . . . . . . . . . . . . . . . . . 19
Sample Setups
Fluorescence . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 171
Gas Absorbance . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 170
Laser Analysis . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 173
LED Analysis . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 172
LIBS . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 174
Metrology . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 175
Overview. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 166
Oxygen Sensing . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 169
Reflected Color. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 177
Solutions Absorbance. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 167
Spectral Identitiy . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 178
Upwelling/Downwelling . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 168
UV-VIS Reflection . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 176
Sampling Accessories . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 85-118
Absorbance Standards . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 93
Collimating Lens . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 88-89
Achromatic . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 88
For Collimation Over Long Distances . . . . . . . . . . . . . . . . . . . 88
Direct Attach . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 88
Collimating Lens, Accessories for . . . . . . . . . . . . . . . . . . . . . . . . . 89
Adjustable Collimating Lens Holder . . . . . . . . . . . . . . . . . . . . 89
Adjustable Collimating Lens and Cuvette Holder . . . . . . . . . . 89
Optical Posts and Post Mounts. . . . . . . . . . . . . . . . . . . . . . . . 89
Right-angle Reflector (excluding 74-UV) . . . . . . . . . . . . . . . . 89
Cuvette Holders . . . . . . . . . . . . . . . . . . . . . . . . . see Cuvette Holders
Cuvettes
Covers . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 93
Disposable . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 93
Quartz . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 93
Emission Sampling
Filter Holders . . . . . . . . . . . . . . . . . . . . . . . . . . . . . see Filter Holders
Filters . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . see Filters
Fluid Analysis . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 94-99
Fluorescence . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 100-103
Integrated Sampling Systems . . . . . . . . . . . . . . . . . . . . . . 19, 87, 92
Light Collection . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 104-105
Metrology . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 109-112
Collimation Testers . . . . . . . . . . . . . . . . . . . . . 111, 160, 162-163
Optical Flats . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 110, 163
Long Trace Profilometer . . . . . . . . . . . . . . . . . . . . . . . . . 87, 112
Reflection and Transmission Stage. . . . . . . . . . . . . . . . . . . . 109
Thin Film Reference Wafer . . . . . . . . . . . . . . . . . . . . . . . . . . 111
Variable-angle Reflection Sampling System . . . . . . . . . . . . . 109
Reflection Sampling Systems . . . . . . . . . . . . . . . . 106-109, 148-149
Diffuse Standards . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 107
Probes . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 76, 148-149
Reflection and Transmission Stage. . . . . . . . . . . . . . . . . . . . 109
Specular Standards . . . . . . . . . . . . . . . . . . . . . . . . 108-109, 163
Stage . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 109
Variable-angle Reflection Sampling System . . . . . . . . . . . . . 109
Sanitary Micro Flow Cell . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 96
Sarge . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 82
ScholAR Chemistry . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 9
Schott Glass Filters . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 164
Science Curricula. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 166
SeaChanger Color Engine. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 160, 162
Semiconductor Nanocrystals . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 102
Sensor Sensor In-house Temperature Calibration Services . . . . . . . . . 74
Sensors
Accessories . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 72-73
Coating Formulations
FOSPOR . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 68
FOXY. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 68
HIOXY . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 68
Coating Services . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 64
Operation . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 65
Oxygen . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . see Oxygen Sensors
pH . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 76
Probes. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 46, 63, 65, 68-72
Reconditioning/Recoating Service . . . . . . . . . . . . . . . . . . . . . . . . . 73
Software . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 75
Spectrometers . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 66-67
Temperature Compensation . . . . . . . . . . . . . . . . . . . . . . . . . . 74, 131
Setups. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 167-177
Shear-plate Collimation Testers . . . . . . . . . . . . . . . . . . . . . . . . . . 111, 163
Signal-attenuating Accessories . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 128
Silicon Wafer Reflectivity . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 31
Silicone Monocoil. . . . . . . . . . . . . . . . . . . . . . . . . . . . . 140, 142, 143, 149
Silicone Overcoats for to Oxygen Sensor Coatings . . . . . . . . . . . . . . . 72
Single-Point Reflection Stage . . . . . . . . . . . . . . . . . . . . . . . . . . . 109, 157
Slits, Optical Bench
HR2000+ . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 22
HR4000. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 22
NIR . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 32
QE65000. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 27
USB4000 . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 15
SMA 905 Connector . . . . . . . . . . . . . . . . . . 15, 22, 27, 32, 141, 143, 155
SMA 905 Bulkhead Bushing . . . . . . . . . . . . . . . . . . . . . . . . . . . . 156, 158
SMA-terminated Bifurcated Optical Fiber Assembly . . . . . . . . . . . . . . . 72
SMA-to-FC Adapter . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 141
SMA-to-ST Adapter . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 141
Software
LIBS-ELITE Software . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 50
NanoCalc Software. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 58
OmniDriver Development Platform. . . . . . . . . . . . . . . . . . . . . . 78, 82
OOILIBS Software . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 48
OOISensors . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 75
Overview . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 78-79
SPAM . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 82
SpecEl Software . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 59
SpecLine Software for Compound ID . . . . . . . . . . . . . . . . . . . . . . . 83
SpectraSuite Spectroscopy Software . . . . . . . . . . . . . . . . . 57, 80-81
UV-VIS Spectral Database . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 79
Solarization-resistant Optical Fiber . . . . . . . . . . . . . . . . . . . 144, 146, 152
SPAM . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 82
Spare Power Supplies . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 136
SpecEl Ellipsometer System . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 59
SpecLine Software for Compound ID . . . . . . . . . . . . . . . . . . . . . . . . . . 83
Spectral
Database . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 79
Diagnosis . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 41
Hyper Adapter. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 61
Identity . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 178-182
Library . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 45, 50, 53, 83
Matching System . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 54
Output Graphs for Light Sources . . . . . . . . . . . . . . . . . . . . . 122-135
Spectralon. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 105-107, 168
SpectraSuite Spectroscopy Software . . . . . . . . . . . . . . . . . . . . . 57, 80-81
Spectrometer
Absorbance, Educational . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 36-39
Absorbance, Flow Through . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 95
Absorbance, General-purpose UV-VIS . . . . . . . . . . . . . . . . . . 14, 42
Accessories . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 61-62
Bench Types . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 12
Calibration Standards (Wavelength) for . . . . . . . . . . . . . . . . 132-133
Comparison Chart . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 13
Deep Well Detector Spectrometers . . . . . . . . . . . . . . . . . . . . . . . . 42
Detector Types . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 12
DTS -series NIR . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 40
Educational Spectrometers . . . . . . . . . . . . . . . . . . . . . . . . . . . . 36-39
Emission Spectrometers . . . . . . . . . . . . . . . . . . . . . 21, 43, 46-50, 59
Flow Analysis . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 86
Fluorescence . . . . . . . . . . . . . . . . . . . . . . . . . 26, 45-47, 66, 130-131
Gated Spectrometer for Fluorescence . . . . . . . . . . . . . . . . . . . . . . 47
General Purpose UV-VIS and VIS-NIR . . . . . . . . . . . . . . . . . . . . . 34
High-resolution . . . . . . . . . . . . . . . . . . . . 12-13, 20-25, 35, 48, 60-61
HR2000+ . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 20
oo
Resources
oo
INDEX by Alphabetical Order
HR4000 . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 21-25
HR4000CG Composite-grating . . . . . . . . . . . . . . . . . . . . . 35, 79
Laser-induced Breakdown Spectrometer . . . . . . . . . . . . . 48-50, 174
LED Measurement Tools . . . . . . . . . . . . . . . . . . . . . . . . . . . . 56, 105
NIR . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 12, 30-32, 40, 179
Optical Benches . . . . . . . . . . . . . 12, 15-18, 20, 22-25, 27-29, 32, 35
Overview. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 12
Plasma Measurement System . . . . . . . . . . . . . . . . . . . . . . . . . . . . 59
Preconfigured . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 34-35, 47, 86
Process2000. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 41
QE65000 Scientific-grade. . . . 13, 19, 26-28, 45, 51, 53, 61, 80, 124
Raman Measurement . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 51-55
Red Tide . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 38
Reflectometry System . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 58
S1024DW Deep Well . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 42
Scientific-grade . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 45
Sample Setups. . . . . . . . . . . . . . . . . . . . . . . . 167, 171-172, 175-177
For Sensors . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 66
USB4000 . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 12-19, 34, 56
USB4000-FL . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 46, 65-66, 171
USB4000FLG . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 47
Spectroradiometric Systems . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 57
Spectroscopy Instructional Handbooks . . . . . . . . . . . . . . . . . . . . . . . . . 36
Specular Reflectance Standards . . . . . . . . . . . . . . . . . . . . . 108-109, 163
Splice Bushing . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 70, 72, 156, 158
Splitter Optical Fiber Assemblies . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 145
ST Connector . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 141
Stage . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 109, 157
Standards
Absorbance . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 93, 167
Calibration
Absorbance . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 93
Fluorescence. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 100
Radiometric . . . . . . . . . . . . . . . . . . . . . . . . . . . 57, 132-133, 168
Reflectance Diffuse . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 107
Reflectance Specular . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 108s
Spectrometer Wavelength . . . . . . . . . . . . . . . . . . . . . . . 134-135
Fluorescence . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 45, 100
NIST-traceable. . . . . . . . . . . . . . . . . . . . . . . . . . . . see NIST-traceble
Reflectance . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 107-108, 163, 176
Starna. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 93
-TTauTheta . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 67
Temperature Calibration Services, In-house . . . . . . . . . . . . . . . . . . . . . 74
Temperature-regulated Cuvette Holder . . . . . . . . . . . . . . . . . . . . . . . . . 91
Termination, Optical Fiber . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 155
Thermistor & Thermocouples . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 67, 74
Thin Film Measurement Systems and Components . . . . . . . . . . 160-164
Thin Film Reference Wafer . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 111
Thin Films & Optics . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 160-162
Capabilities . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 161
Coating Types. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 160
Specifications . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 160
Overview. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 160
Toshiba TCD1304AP CCD-array Detector . . . . . . . . . . . 17, 21-22, 24-25
Trade-in Program . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 8
Transmission Dip Probes . . . . . . . . . . . . . . . . . . . . . . . . . 36, 76, 150-152
Transmission of Optics Tools . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 60
Triggering . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 13-14, 30, 48, 61, 84, 127
Tungsten Halogen Light Sources . . . . . . . 20, 34, 128-129, 167, 175-177
Direct-attach Accessories . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 19
Optical Bench Options
Choosing a Grating & Wavelength Range . . . . . . . . . . . . . . . 16
Collimating & Focusing Mirrors . . . . . . . . . . . . . . . . . . . . . . . . 16
Detector Sensitivity Comparison . . . . . . . . . . . . . . . . . . . . . . . 17
Detector with OFLV Filter: . . . . . . . . . . . . . . . . . . . . . . . . . . . . 17
Fixed Entrance Slit . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 15
Grating Efficiency Curves . . . . . . . . . . . . . . . . . . . . . . . . . . . . 18
Grating Selection Chart. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 16
L4 Detector Collection Lens . . . . . . . . . . . . . . . . . . . . . . . . . . 17
Longpass Absorbing Filter. . . . . . . . . . . . . . . . . . . . . . . . . . . . 16
SAG+ Mirrors . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 16
SMA 905 Connector . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 15
UV4 Detector Window Upgrade . . . . . . . . . . . . . . . . . . . . . . . 17
Predicted Ranges & Resolution . . . . . . . . . . . . . . . . . . . . . . . 18
Sample Setups . . . . . . . . . . . . . . . . . . . . 167, 171-172, 175-177
USB-650 Red Tide Spectrometer . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 38
USB Cable . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 62, 84
UV Coating. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 28
UV2 and UV4 Detector Upgrade . . . . . . . . . . . . . . . . . . . . . 15, 17, 22, 24
UV-VIS
Fiber . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 139, 146
Preconfigured Spectrometers . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 34
Reflection, Setup . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 176
Spectral Database . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 79
Preconfigured Spectrometers . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 34
-VVacuum Feedthroughs . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 153
Variable
Attenuator . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 117, 121, 156
Bandwidth Filter . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 114
Longpass Order-sorting Filters. . . . . . . . . . . . . . . . . . . . . . 17, 24, 28
Order-sorting Filter . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 35
Saturation Filters . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 162
Variable-angle Reflection Sampling System . . . . . . . . . . . . . . . . . . . . 109
Vernier Software . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 9
VIS Cuvettes . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 93
VIS-NIR
Low OH Fibers . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 139
Optical Fiber Assemblies . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 40
Preconfigured Spectrometers . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 34
Spectrometers . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 34
Visual Basic . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 82
-WWarranty, Extended . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 62
Wavelength Calibration Cuvette Adapter . . . . . . . . . . . . . . . . . . . . . . . 135
Wavelength Calibration Standard
NIR . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 135
UV-VIS . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 134
White Standards. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 107
Wiener-Fourier . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 83
WS-1 Diffuse Reflectance Standard . . . . . . . . . . . . . . . . . . . 107, 176-177
-XXenon Pulsed & Continuous Light Sources . . . . . . . . . . . . 120, 127, 136
Xplorer GLX Handheld Computer . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 39
Xtreme Solarization-resistant (XSR) Optical Fiber Assemblies . . . . . . 146
XYZ Mapping Tables . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 118
-U-YUnipolar/Bipolar . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 99
Unjacketed Bulk Optical Fiber . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 143
Upwelling/Downwelling . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 168
USB Interface . . . . . . . . . 13-14, 20-21, 26, 30, 35-38, 40-41, 45-47, 101
USB Spectrometers
USB4000 . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 14-19, 56, 92
USB4000-FL. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 46, 66, 171
USB4000FLG . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 47
UV-VIS & VIS-NIR . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 34
USB4000 Spectrometer . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 14-19
Cables, Adapters, Power Supplies . . . . . . . . . . . . . . . . . . . . . . . . . 62
oo
192
YAG Laser, LIBS Laser Options . . . . . . . . . . . . . . . . . . . . . . . . . . . . 49-50
-ZZ Flow Cell . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 94-95
Zerodur Optical Flats . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 110
For all your sensing needs, visit OceanOptics.com
Standard & Extended Warranty Coverage
All products manufactured by Ocean Optics are warranted for
one year. Ocean Optics also offers an Annual Service Package
(ASP) that extends by one year the standard warranty on our
spectrometers. The holder of the ASP is entitled to several
benefits during the one-year period commencing with the
spectrometer invoice date:
Additional year of warranty protection and certification
Factory calibration and certification of your spectrometer,
including optical alignment, wavelength calibration,
linearity calibration, stray light measurement and signal-tonoise analysis, optical resolution evaluation and baseline
uniformity evaluation
Waiver of $250 labor charge for upgrades to your spectrometer configuration, such as changing a slit or grating
A spiffy new Maxwell’s Equations T-shirt – be the envy of all
your friends, like our Ocean Optics models!
Also available is a two-year extended warranty renewal option
for most of our spectrometers. Enjoy all the great ASP benefits
with the additional year of coverage at a steep discount.
The purchase of an ASP comes with the latest Maxwell's Equations T-shirt,
modeled by (left to right) Fernando Quinones, Accounting Specialist; Jada Mains,
Customer Support Coordinator; Nick Sebastian, Global Distribution Sales
Manager; and Ricardo Nobara De La Torre, Electrical Engineer.
Item
Description
For These Spectrometer Series
ASP
Extends the standard warranty from 1 year to 2 years. Price is per spectrometer
USB2000, S2000, PC2000, HR2000,
channel.
HR2000+, HR4000, USB4000
A 1-year warranty package available to customers whose original warranty has
USB2000, S2000, PC2000, HR2000,
expired. Price is per spectrometer channel.
HR2000+, HR4000, USB4000
1-year renewal option for holders of expiring ASPs; price is per channel.
USB2000, S2000, PC2000, HR2000,
ASP-ES
ASP-R
Price
$250
$300
$250
HR2000+, HR4000, USB4000
ASP-R-E
2-year renewal option for holders of expiring ASPs; price is per channel.
USB2000, S2000, PC2000, HR2000,
$350
HR2000+, HR4000, USB4000
ASP-NIR
Extends the standard warranty on NIR Spectrometers from 1 year to 2 years.
NIR256-2.1, NIR256-2.5, NIR512
ASP-QE
Extends the standard warranty on QE Spectrometers from 1 year to 2 years.
QE65000
$1,000
$750
Trademarks
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Dynasil is a registered trademark of Degussa-Huls Aktiengesellschaft.
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ETC and Source Four are registered trademarks of Electronic Theatre
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Fedora is a registered trademark of Red Hat, Inc.
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FluorX is a registered trademark of Panalytical B.V.
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Schott and Zerodur are registered trademarks of Schott Glaswerke
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SolidWorks is a registered trademark of SolidWorks Corporation.
Spectralon is a registered trademark of Labsphere, Inc.
Starna is a registered trademark of Starna Cells, Inc.
Java is a registered trademarks of Sun Microsystems, Inc.
Suprasil is a registered trademark of Heraeus Quarzglas GmbH & Co.
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Tygon is a registered trademark of Norton Company.
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VWR is a registered trademark of VWR International, Inc.
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Copyright © 2007 Ocean Optics, Inc.
All rights reserved. No part of this publication may be reproduced or transmitted in any form or by any means, electronic or
mechanical, including photocopy, recording, or stored in a retrieval system, without written permission from Ocean Optics, Inc.
Sensing a New World
Jaz is a new family of stackable, modular and flexible sensing
tools. You select from various Jaz modules to create a
networked community of smart sensing appliances with common
electronics and communications. With Jaz, we are proposing
nothing short of changing our world, and changing yours as well.
Be part of the evolution.
OceanOptics.com
830 Douglas Avenue
Dunedin, FL 34698
Phone: 727.733.2447
Fax: 727.733.3962
[email protected]
OceanOptics.com
727.733.2447
[email protected]
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