Spectrometer Catalog - MadatecSpectrometer Catalog A Full Range of Spectroscopy Solutions MADAtec Srl Tel. +39-0236542401 e-mail: [email protected] ITALY 1 …

Spectrometer CatalogA Full Range of Spectroscopy Solutions

MADAtec SrlWWW.MADATEC.COMTel. +39-0236542401e-mail: [email protected]

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By offering various services in industrial design, custom software development, end-user training, and regulatory compliance testing & certification, we work with our customers from concept to completion. We design, engineer, prototype, and manufacture an extensive range of photonic instrumentation for biomedical, analytical, and countless other applications.

B&W Tek, Inc. is an advanced instrumentation company producing optical spectroscopy and laser instrumentation for biomedical, physical, chemical, and research communities. Originally established as a producer of green lasers, we’ve grown into a leading total solutions provider for the photonics industry, coupling our core technologies with custom design and manufacturing capabilities.

About B&W Tek, Inc. Table of Contents

Since we were established in 1997, we’ve emphasized strong vertical integration for better efficiency and growth. This allows us to provide high quality products at a lower cost to our customers. B&W Tek, Inc’s key building blocks are diffraction limited, spectrum stabilized, and high power lasers as well as our UV, Vis, & NIR spectrometers, sampling accessories, and broadband light sources. By combining these core technologies, B&W Tek, Inc. provides total solutions with endless possibilities!

About B&W Tek -------------------------------------------------------- Page 1 Regulatory Compliance & QA / QC ----------------------------- Page 3 OEM Philosophy ---------------------------------------------------- Page 4

How Our Spectrometers Work Crossed Czerny-Turner Optical Design ------------------------- Pages 5+6 Unfolded Czerny-Turner Optical Design ------------------------ Pages 7+8 Concave Holographic Optical Design --------------------------- Pages 9+10

Spectrometer Modules Quest™ U ------------------------------------------------------------ Pages 11+12 Quest™ X ------------------------------------------------------------ Pages 13+14 Glacier™ X ---------------------------------------------------------- Pages 15+16 Prime™ X ----------------------------------------------------------- Pages 17+18 i-Trometer™ --------------------------------------------------------- Pages 19+20 Cypher™ H ---------------------------------------------------------- Pages 21+22 Sol™ 1.7 ------------------------------------------------------------- Pages 23+24 Sol™ 2.2 ------------------------------------------------------------- Pages 25+26 Sol™ 2.2A ----------------------------------------------------------- Pages 27+28 Sol™ 2.6 ------------------------------------------------------------- Pages 29+30

Accessories Light Sources -------------------------------------------------------- Pages 31+32 Sampling Accessories----------------------------------------------- Page 33 Fibers & Fiber Assemblies ---------------------------------------- Page 34

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As part of our mission to provide a total solution, we’ve developed the OEM Product Development Cycle to ensure we meet our customers’ goals at each milestone. Our project management and engineering team work closely with our customers to understand not only the product requirements, but their overall business goals. Our extremely flexible and adaptable solutions are the perfect answer for every OEM need.

Our resources for OEM development include a Research and Development team of over 30 engineers, all with advanced degrees in multiple disciplines. Leading these teams are senior engineers with over 30 years of industrial experience and a strong focus on vertical integration. Our combined 65,000 square feet of modern manufacturing facilities and laboratory space house multi-million dollar equipment, facilitating high-quality, low-cost manufacturing.

At B&W Tek, we guarantee superior performance, quality, and solid regulatory compliance standards on each product that leaves the facility. We operate in ISO 13485 & ISO 9001 certified facilities equipped with clean room environments, and apply an extensive Overall Quality Control Test (OQCT) to make sure our products and services pass or exceed domestic or international standards and regulations. Our Mock FDA Quality Systems Inspections Technique (QSIT) allows us to conduct Installation Qualifications (IQs), Operational Qualifications (OQs), and Performance Qualifications (PQs) checks, as well as software verifications and validations. We also apply Six Sigma methodologies to ensure each product passes all tests at each production process level.

Regulatory Compliance OEM Philosophy

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• ISO 9001 & ISO 13485 certified• FDA & CDRH registration and compliance • CE Safety Standards • UL Safety Standards• Manufacturing FDA Class II and III devices• Application of Six Sigma methodologies

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Workings of a Crossed Czerny-Turner Spectrometer:

Detector

As the dispersed light strikes the detector’s pixels, the electronics digitize the data to be displayed

Each pixel represents a portion of the spectrum and as the incident light strikes the individual pixels across the CCD, the electronics can then translate and display their intensity using our software, BWSpec™.

The quantum efficiency (QE), dynamic range (DR), and noise level of the array detector largely dictates the spectrometer sensitivity, dynamic range and signal-to-noise ratio. The spectral acquisition speed of the spectrometer is mainly determined by the detector response over a wavelength region.

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4Grating

Determines wavelength range and spectral resolution

The groove frequency of the grating determines two key aspects of the spectrometer’s performance: the spectral resolution and the wavelength coverage. The higher the groove frequency, the more resolution the instrument will achieve; however, the wavelength coverage will be less. Inversely, decreasing the groove frequency increases wavelength coverage at the sacrifice of spectral resolution. With over twenty-five gratings to choose from, we can customize your application needs. The blaze angle or blaze wavelength of the grating is also a key parameter in optimizing the spectrometer’s performance. The blaze angle determines the maximum efficiency the grating will have in a specific wavelength region. We have a variety of blaze angles available per groove frequency to match your application needs.

SMA 905:

Precision Fiber CouplerBy coupling the SMA 905 adapter with a fiber or lens, light will be guided to the slit and optically matched. This ensures reproducibility for light coupling from the fiber or lens into the optical bench.

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Slit

Determines the photon flux and optical resolutionLight entering into a spectrometer’s optical bench via a fiber or lens is focused onto a pre-mounted and aligned slit, which ultimately determines the optical resolution and throughput of the spectrometer after grating selection.

Collimating Mirror

Collimates and redirects the light beam towards the grating3

Focusing Mirror

Refocuses the dispersed light onto the detector

When working in the UV-Vis spectrum, both mirrors are F# matched focusing mirrors coated with AlMg2,which produces approximately 95% reflectance. Aluminum (Al) provides reflectance and Magnesium (Mg2) protects the aluminum from oxidation.

When working in the NIR, both mirrors are F# matched focusing mirrors coated with a special coating that enhances the NIR signal.

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Thermoelectric Cooler

Reduces dark noise and increases the dynamic rangeCooling an array detector with a built-in Thermoelectric Cooler (TEC) is an effective way to reduce dark current and noise, as well as to enhance the dynamic range and detection limit. For Si detectors, dark current halves when its temperature is decreased every 5 - 7°C. For InGaAs detectors, dark current halves when its temperature is decreased every 7 - 10°C. This allows the spectrometer to operate at long integration times and detect weak optical signals.

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For more technical information on how a spectrometer worksplease visit our knowledge section at www.bwtek.com/technical

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Workings of an Unfolded Czerny-Turner Spectrometer:

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Detector As the dispersed light strikes the detector’s pixels, the electronics digitize the data to be displayed

Each pixel represents a portion of the spectrum and as the incident light strikes the individual pixels across the CCD, the electronics can then translate and display their intensity using our software, BWSpec™.

The quantum efficiency (QE), dynamic range (DR), and noise level of the array detector largely dictates the spectrometer sensitivity, dynamic range and signal-to-noise ratio. The spectral acquisition speed of the spectrometer is mainly determined by the detector response over a wavelength region.

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SMA 905:

Precision Fiber CouplerBy coupling the SMA 905 adapter with a fiber or lens, light will be guided to the slit and optically matched. This ensures reproducibility for light coupling from the fiber or lens into the optical bench.

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Slit

Determines the photon flux and optical resolution

Light entering into a spectrometer’s optical bench via a fiber or lens is focused onto a pre-mounted and aligned slit, which ultimately determines the optical resolution and throughput of the spectrometer after grating selection.

Focusing Mirror

Refocuses the dispersed light onto the detector 5

Collimating Mirror

Collimates and redirects the light beam towards the gratingWhen working in the UV-Vis spectrum, both mirrors are F# matched focusing mirrors coated with AlMg2, which produces approximately 95% reflectance. Aluminum (Al) provides reflectance and Magnesium (Mg2) protects the aluminum from oxidation.

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Grating

Determines wavelength range and spectral resolution The groove frequency of the grating determines two key aspects of the spectrometer’s performance: the spectral resolution and the wavelength coverage. The higher the groove frequency, the more resolution the instrument will achieve; however, the wavelength coverage will be less. Inversely, decreasing the groove frequency increases wavelength coverage at the sacrifice of spectral resolution. With over twenty-five gratings to choose from, we can customize your application needs. The blaze angle or blaze wavelength of the grating is also a key parameter in optimizing the spectrometer’s performance. The blaze angle determines the maximum efficiency the grating will have in a specific wavelength region. We have a variety of blaze angles available per groove frequency to match your application needs.

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SMA 905:

Precision Fiber CouplerBy coupling the SMA 905 adaptor with a fiber or lens, light will be guided to the slit and optically matched. This ensures reproducibility for light coupling from the fiber or lens into the optical bench.

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Concave Holographic Grating

Collects, disperses and refocuses lightThis one compact optical component collects, disperses, and refocuses light onto the detector by combining two optical components, i.e. the grating and focusing mirror found in standard optical benches. The optimized holographic grating delivers excellent efficiency and stray-light reduction and is able to provide a faster F#, delivering higher throughput.

Slit

Determines the photon flux and spectral resolutionLight entering into a spectrometer’s optical bench via a fiber or lens is focused onto a pre-mounted and aligned slit. This ultimately determines the spectral resolution and throughput of the spectrometer after grating selection.

Folding Mirror

Redirects the light beam towards the grating3The folding mirror redirects the light from the slit towards the holographic grating to be defracted and refocused. This mirror is coated with AlMg2 which produces approximately 95% reflectance when working in the UV-Vis spectrum. Aluminum (Al) provides reflectance and Magnesium (Mg2) protects the Aluminum from oxidation.

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Workings of a Concave Holographic Spectrometer:

Detector As the dispersed light strikes the detector’s pixels, the electronics digitize the data to be displayed

Each pixel represents a portion of the spectrum. As the incident light strikes the individual pixels across the CCD, the electronics can then translate and display their intensity using our software, BWSpec™.

The quantum efficiency (QE), dynamic range (DR), and noise level of the array detector largely dictates the spectrometer sensitivity, dynamic range, and signal-to-noise ratio. The spectral acquisition speed of the spectrometer is mainly determined by the detector response over a wavelength region.

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Quest™ UTemperature Compensated, High Performance, Low Stray UV Light CCD Spectrometer

• Thermal Drift ~15 Counts/oC (Typical) • Low Stray UV Light• UV and UV / Vis Standard• 0.3nm Spectral Resolution• 16-Bit Digitizer• 1ms Minimum Integration Time• >2.0 MHz Readout Speed• Plug-and-Play USB 2.0

Features:

The QuestTM U series is optimized for UV performance with a low stray UV light optical bench featuring a high performance, non-cooled linear CCD array spectrometer, with a >2.0 MHz readout speed. External event sensing, control and external trigger input are standard. A 2048 element detector, built-in 16-bit digitizer, temperature compensation, and a USB 2.0 interface are standard. An enhanced RS232 communication is also available. This spectrometer will continuously deliver optimized high throughput results.

Temperature compensation greatly reduces the Thermal Drift to ~15 Counts/oC which decreases baseline drift and sustains the dynamic range.

The Quest™ U is available in two standard spectral configurations; 200nm - 400nm and 200nm - 850nm. Custom configurations are available for OEM applications.

Applications

About the Quest™ U

• UV, Vis, and NIR: Spectroscopy / Spectroradiometry / Spectrophotometry• WL Identification• Absorbance• Reflectance• OEM Optical Instrumentation Building Blocks

General Specifications:

Detector

Grating

Slit

Power Input USB at < 350 mA

Detector Type Response enhanced 2048 element linear silicon CCD array

Detector Pixel Format 2048 x 1 elements @ 14μm x 200μm per element

Spectrograph F# 3.6

Spectrograph Optical Layout Czerny-Turner

Dynamic Range 275 typical

Digitizer Resolution 16-bit or 65,535:1

Readout Speed >2.0 MHz

Data Transfer Speed Up to 660 spectra per second via USB 2.0

Integration Time 1 - 65,535ms

Thermal Drift ~29 Counts/oC (Max)

Aux Port External Trigger, Digital IOs

Operating Temperature 5°C - 35°C

Operational Relative Humidity 85% Noncondensing

Weight ~0.37 kg (0.8 lbs)

Dimensions 124mm x 91mm x 35mm (4.9in x 3.6in x 1.4in)

Computer Interface USB 2.0 / 1.1 and Enhanced RS232

Operating Systems Windows: XP, Vista (32-bit), 7 (32-bit)

The Quest™ U features a non-cooled 2048 element linear silicon CCD array detector with a pixel format of 2048 x 1 elements @ 14µm per element with effective (active) pixels > 2000. Each pixel represents a portion of the spectrum. As the dispersed incident light strikes the individual pixels across the CCD, the electronics can then translate and display the intensity using our BWSpec™ software.

The extension of the QE curve after the UV enhancement.

Specifications Wavelength Range 200nm - 850nm

Pixels 2048Pixel Size 14µm x 200µm

Well Depth ~65,000 eDigitization Rate >2.0 MHz

The groove frequency of the grating determines two key aspects of the spectrometer’s performance: the wavelength coverage and the spectral resolution.

Light entering into a spectrometer’s optical bench via a fiber or lens is focused onto a pre-mounted and aligned slit.

Slit Option Dimensions Approx. Resolution 200-400nm

10mm 10mm wide x 1mm high 0.325mm 25mm wide x 1mm high 0.550mm 50mm wide x 1mm high 0.8100mm 100mm wide x 1mm high 1.3200mm 200mm wide x 1mm high 3.0

Custom Slit Widths Available

RS232 communication also available. Contact B&W Tek for technical specifications.Phone: 1-302-368-7824 · Web: www.bwtek.com

Best Efficiency

Spectral Coverage (nm) Grating

UV 200 - 400 1800/250UV - Vis 200 - 850 600/250

Custom Configurations Available

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Quest™ XTemperature Compensated, High Performance, Compact CCD Spectrometer

• Thermal Drift ~15 Counts/oC (Typical)

• UV - NIR (200nm - 1050nm)

• 0.5nm Spectral Resolution

• 16-Bit Digitizer

• 1ms Minimum Integration Time

• >2.0 MHz Readout Speed

• Plug-and-Play USB 2.0

Features:

The QuestTM X series features a high performance, non-cooled linear CCD array spectrometer, with a >2.0 MHz readout speed. External event sensing, control and external trigger input are standard. A 2048 element detector, built-in 16-bit digitizer, temperature compensation, and USB 2.0 interface are standard. An enhanced RS232 communication is also available. This spectrometer will continuously deliver optimized high throughput results.

Temperature compensation greatly reduces the Thermal Drift to ~15 Counts/oC which decreases baseline drift and sustains the dynamic range.

The QuestTM X is ideal for most UV, Vis, and NIR applications with our standard spectral configurations which start at 200nm and reach up to 1050nm. With our slit options, resolutions between 0.5nm and 3.0nm can be achieved. Flexible custom configurations and application support are available for OEM applications.

Applications

About the Quest™ X

• UV, Vis, and NIR: Spectroscopy / Spectroradiometry / Spectrophotometry• WL Identification• Absorbance• Reflectance• OEM Optical Instrumentation Building Blocks


Detector

Grating

Slit

Power Input USB at < 350mA

Detector Type Response enhanced 2048 elementlinear silicon CCD array

Detector Pixel Format 2048 x 1 elements @ 14μm x 200μm per element

Spectrograph F# 3.6

Spectrograph Optical Layout Crossed Czerny-Turner



Readout Speed >2.0 MHz


Integration Time 1 - 65,535ms

Thermal Drift ~29 Counts/oC (Max)

Aux Port External Trigger, Digital IOs





Computer Interface USB 2.0 / 1.1 and Enhanced RS232


The Quest™ X features a non-cooled 2048 element linear silicon CCD array detector with a pixel format of 2048 x 1 elements @ 14µm per element with effective (active) pixels > 2000. Each pixel represents a portion of the spectrum. As the dispersed incident light strikes the individual pixels across the CCD, the electronics can then translate and display the intensity using our BWSpec™ software.




Well Depth ~65,000 eDigitization Rate >2.0 MHz


Best Efficiency


UV / NIR 200 - 850 600/250Vis / NIR 350 - 1050 600/400

Vis 380 - 750 900/500Vis / NIR 550 - 1050 830/800

NIR 750 - 1050 1200/750Custom Configurations Available



10mm 10mm wide x 1mm high 1.025mm 25mm wide x 1mm high 1.250mm 50mm wide x 1mm high 2.0100mm 100mm wide x 1mm high 3.0200mm 200mm wide x 1mm high Call


RS232 communication also available. Contact B&W Tek for technical specifications.Phone: 1-302-368-7824 · Web: www.bwtek.com

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Glacier™ XTE Cooled 16-bit USB Linear CCD Array Spectrometer

• UV - NIR Ranges• 0.6nm - 4.0nm Resolution Range• TE Cooled / Regulated• 16-Bit Digitizer• 500 kHz Readout Speed • Plug-and-Play USB 2.0 • OEM Version Available

Features:

The Glacier™ X series is a high performance, thermoelectric cooled (TEC) linear CCD array spectrometer solution. Equipped with 2048 elements, built-in 16-bit digitizer, and high-speed USB 2.0 interface, this TE Cooled spectrometer will continuously deliver optimized high throughput results.

Compared to non-cooled CCD spectrometers, the Glacier™ X offers higher dynamic range, significantly reduced dark counts, and superior long-term operation stability, making it ideal for low light level detection and long-term monitoring applications.

Wavelength configurations are available from as low as 200nm to as high as 1050nm with standard configuration resolutions of 0.6nm to 4.0nm. Flexible custom configurations and application support are available for OEM applications.

Applications

About the Glacier™ X

• UV, Vis, and NIR: Spectroscopy / Spectroradiometry / Spectrophotometry

• WL Identification• Absorbance• Reflectance• OEM Optical Instrumentation Building Blocks


DetectorThe Glacier™ X features a TE Cooled 2048 element linear silicon CCD array detector with a pixel format of 2048 x 1 elements @ 14µm per element with effective (active) pixels > 2000. Each pixel represents a portion of the spectrum. As the dispersed incident light strikes the individual pixels across the CCD, the electronics can then translate and display the intensity using our BWSpec™ software.

Grating Slit

DC Power Input 5V DC < 1.5 Amps

AC Adapter Input 100 - 240VAC 50/60 Hz, 0.5A @ 120VAC

Detector Type Response Enhanced 2048 element linear silicon CCD array

Pixels 2048 x 1 elements @ 14μm x 200μm per element

Spectrograph F# 3.2




Readout Speed 500 kHz


Integration Time 5 ~ 65,535ms x multiplier

External Trigger Aux Port



TE Cooling 14°C

Weight 0.60 kg (1.32 lbs)

Dimensions 127.0mm x 39.0mm x 90.7mm (5in x 1.5in x 3.6in)

Computer Interface USB 2.0 / 1.1





Well Depth ~90,000 eDigitization Rate 500 kHz

Best Efficiency


UV / Vis 200-400 1800/250UV - NIR 200-800 716/222UV / Vis 250-600 1200/250

UV 280-370 3600/240UV - NIR 300-900 600/400UV - NIR 350-1050 700/530

Vis 380-750 900/500Vis / NIR 400-800 1200/500Vis / NIR 450-1050 830/800

Vis 550-700 1800/500Vis / NIR 600-800 1714/650Vis / NIR 750-1050 1200/750



10mm 10mm wide x 1mm high 1.125mm 25mm wide x 1mm high 1.450mm 50mm wide x 1mm high 2.2100mm 100mm wide x 1mm high Call200mm 200mm wide x 1mm high Call

Custom Slit Widths Available

Thermoelectric CoolerCooling an array detector with a built-in Thermoelectric Cooler (TEC) is an effective way to reduce dark current and noise, as well as enhance the dynamic range and detection limit.

The graph shows the dark current and noise for an uncooled vs. cooled CCD detector at an integration time of 30 seconds. When operating at room temperature, the dark current nearly saturates the uncooled CCD. When the CCD is cooled down to 14oC by the TEC, the dark current is reduced by four times and the dark shot noise is reduced by two times. This allows the spectrometer to operate at long integration times and detect weak optical signals.

Room Temperature Cooled to 14oC

Dark Current: Uncooled vs. Cooled CCD Detectors at 30 Seconds



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Prime™ XFiber Coupled Back-Thinned CCD Array Spectrometer

• Over 90% Peak QE

• Over 60% QE at 200nm

• High UV, Vis, and NIR Response

• 512 or 1024 Elements

• -10oC TE Cooled

• Optional Shutter Available

Features:

The Prime™ X is a high performance linearly summed spectrometer featuring a high sensitivity -10oC TE Cooled, back-thinned 512 x 58 CCD array. A 1024 x 58 CCD array is also available for increased range and resolution. Both spectrometers have fiber-coupled input, built-in 16-bit digitizer, external trigger and high speed USB 2.0 interface.

With its high dynamic range and high signal-to-noise ratio, low dark counts and long term operational stability, this model will meet your UV to NIR application needs.

Flexible custom configurations and application support are available for OEM applications.

About the Prime™ X

General Specifications:AC Power Input 100 - 240VAC 50/60 Hz, 2.0A @ 120VAC

Detector Type Back-thinned CCD array

Pixels 512 @ equivalent 24mm x 1392mm (24x58)1024 @ equivalent 24mm x 1392mm (24x58)

Spectrograph F# 3.5


Dynamic Range 75,000 (typical) with line binning

Digitizer Resolution 16 bit or 65,535:1


Data Transfer Speed BWSpec 3.26: >50 spectra/second via USB 2.0

Integration Time (512) BWSpec 3.26: 27 - 65,535ms x multiplier(1024) BWSpec 3.26: 50 - 65,535ms x multiplier


Operating Temperature 0°C to 35°C

TE Cooling -10°C

Weight Spectrometer: 1.4 kg (3.1 lbs)Power Supply: 0.9 kg (2 lbs)

Dimensions

Spectrometer: 107mm x 178mm x 89mm (4.2in x 7.0in x 3.5in)Power Supply: 249mm x 169mm x 57mm (9.8in x 6.6in x 2.2in)



Applications• Low Light Level UV and NIR Spectroscopy • Raman and Fluorescence Spectroscopy • Remote Sensing • DNA Sequencing • Semiconductor End Point Inspection • LED Sorting and Characterizations • LCD Display Measurements

Detector

Grating

Slit

The Prime™ X back-thinned CCD offers very high quantum efficiency over the spectrum 200nm - 1000nm. Featuring a large full-well capacity, low readout noise and MPP technology in the electronics for dark current reduction, this CCD is ideal for low light level applications.

Specifications 512 Pixel Array 1024 Pixel Array

Wavelength Range 380nm - 1050nm 200nm - 1050nmPixels 512 x 58 1024 x 58

Pixel Size 24µm x 24µmWell Depth ~30,000 e (typical)

Digitization Rate 250 kHz


Best Efficiency


512 Pixel ArrayVis / NIR 500-920 400/400

Vis 380-750 400/4001024 Pixel Array

UV 200-400 1200/250UV-NIR 203-900 400/400

NIR 750-1050 600/1000Custom Configurations Available

Slit Option Dimensions512 Pixel Array

Approx. Resolution380-750nm

1024 Pixel ArrayApprox. Resolution

750-1050nm

10mm 10mm wide x 1mm high Call Call25mm 25mm wide x 1mm high 2.6 1.550mm 50mm wide x 1mm high 3.8 2.5100mm 100mm wide x 1mm high 10.0 5.0200mm 200mm wide x 1mm high Call Call



Thermoelectric CoolerCooling an array detector with a built-in thermoelectric cooler (TEC) is an effective way to reduce dark current and noise as well as enhance the dynamic range and detection limit.

The graphs show dark current and noise for uncooled and cooled CCD detectors at an integration time of 30 seconds. At room temperature, the dark current takes up much of the well depth. When the CCD is cooled down to just -10oC by the TEC, the dark current is reduced by sixteen times, and the dark shot noise is reduced by four times. This allows the spectrometer to operate at long integration times and to detect weak optical signals.

Room Temperature Cooled to -10oC

Dark Current: Uncooled vs. Cooled CCD Detectors at 30 Seconds

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i-trometer™Miniature Back-Thinned CCD Spectrometer

• High UV, Vis, NIR Response

• Wide Dynamic Range

• High Throughput

• High Stray Light Rejection

• Plug-and-Play USB 2.0 Interface

Features:

The i-trometer™ is a miniature back-thinned 2048 x 64 CCD array, linearly summed spectrometer designed for meeting the needs of wide dynamic range spectral applications. A holographic aberration corrected flat field concave grating and optimized optical bench minimizes stray light and improves throughput.

The i-trometer™ employs a high UV-NIR response CCD detector array leading to high detection sensitivity. The spectrometer offers wide detection dynamic range, superior quantum efficiency (QE), high signal-to-noise (S/N) ratio and is ideal for various UV/Vis/short-wave NIR spectroscopic applications. The optical input to the spectrometer can select from a single or bundled fiber option, providing ease of use and high throughput coupling for low light level detection. The i-trometer™ also features plug-and-play USB interface for high speed data transferring.

Applications

About the i-trometer™

• UV / Vis / Short-wave NIR Spectroscopy• UV / Vis / NIR Lamp Characterization• HPLC Detection• Solar Monitoring


Detector


Slit

DC Power Input 5V DC @ < 0.8 Amps Max


Detector Type Back-thinned CCD array

Pixels 2048 @ equivalent 14mm x 896mm (14x64)

Spectrograph F# 3.0

Spectrograph Optical Layout Concave Holographic, Aberration Corrected, Flat Field

Dynamic Range 33,300

Digitizer Resolution 16-bit or 65,535 to 1



Integration Time 7ms to >= 20,000ms


Operating Temperature 15°C to 35°C





The i-trometer™ features a back-thinned CCD array where pixels are vertically binned, making an equivalent format of 2048 x 64 element @ 14mm x 896mm with effective (active) pixels > 2000. Each pixel represents a portion of the spectrum. As the dispersed incident light strikes the back of this thinned piece of substrate, photons captured by individual pixels across the CCD are then translated by the electronics and their intensity is displayed using our BWSpec™ software.


Pixels 2048 x 64Pixel Size 14µm x 14µm

Well Depth ~200,000 eDigitization Rate 375 kHz

Slit Option Dimensions Approx. Resolution190-1100nm

10mm 10mm wide x 1mm high 2.025mm 25mm wide x 1mm high 2.550mm 50mm wide x 1mm high 3.2100mm 100mm wide x 1mm high 6.0200mm 200mm wide x 1mm high Call



Best Efficiency

Spectral Coverage (nm) Grating Option

UV / Vis 180-450 Group 1UV - NIR 190-800 Group 2Vis / NIR 400-800 Group 2UV / Vis 200-550 Group 3UV - NIR 190-1100 Group 4UV / Vis 350-750 Group 5UV - NIR 350-1050 Group 5


This one compact optical component collects, disperses, and refocuses light onto the detector by combining two optical components (i.e. grating and focusing mirror found in standard optical benches).

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Cypher™ HFiber Coupled UV - NIR Enhanced PDA Spectrometer

• Enhanced QE in NIR

• High UV Response as Low as 185nm

• High Dynamic Range

• 512 or 1024 Element Linear PDA

Features:

The Cypher™ H is a high performance linear PDA spectrometer with high speed plug-and-play USB 2.0 interface, 512 or 1024 element linear PDA array, optimized high throughput spectrograph, 16-bit built-in digitizer, and fiber coupled input capability.

The PDA offers high dynamic range, high signal-to-noise ratio and enhanced UV and NIR sensitivity; making it ideal for the detection of small changes in light intensity at high light levels. With its Concave Holographic grating, the Cypher™ H offers excellent efficiency, wavelength coverage from UV to NIR, and spectral resolution of 2.6nm or higher. Flexible custom configurations are also available.

Applications

About the Cypher™ H

• UV and NIR Applications• LED and Other Display Devices Testing• Color Measurement• Small Light Difference Detection


Detector


Slit

Power Input 5V DC @ < 0.8 Amps


Detector Type Self-scanning photodiode linear array

Pixels 512 @ 25mm x 2500mm1024 @ 25mm x 2500mm

Spectrograph F# 3.0

Spectrograph Optical Layout Concave Holographic, Aberration Corrected, Flat Field

Dynamic Range 5 x 104 typical




Integration Time 3 - 65,535ms x multiplier







As the dispersed light strikes individual pixels across the photodiode array (PDA), electronics translate and display intensity using our BWSpec™ software. The advantage of a PDA over a CCD is its high dynamic range, which allows it to be used for high light level applications.


Pixels 512, 1024Pixel Size 25µm x 2500µm

Well Depth ~156,000,000 eDigitization Rate 250 kHz

This one compact optical component collects, disperses, and refocuses light onto the detector by combining two optical components: grating and focusing mirror (found in standard optical benches).

Best Efficiency

Spectral Coverage (nm)

Grating Option

UV - Vis 185-800 Group 1Vis - NIR 350-1050 Group 1



Slit Option Dimensions Approx. Resolution350-1050nm

25mm 25mm wide x 2mm high 2.750mm 50mm wide x 2mm high 4.5100mm 100mm wide x 2mm high 7.2200mm 200mm wide x 2mm high Call


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Sol™ 1.7Short and Long Wavelength Enhanced NIR TE Cooled InGaAs Array Spectrometer

• 900nm - 1700nm Spectral Range

• Built-In 16-Bit Digitizer

• TE Cooled / Stabilized

• User Selectable High Dynamic / High Sensitivity Mode

Features:

The Sol™ 1.7 is a high performance linear InGaAs array spectrometer featuring 256, 512 (standard), and 1024 pixels, and TE Cooling down to 5oC, all while providing high throughput and large dynamic range.

Each spectrometer features an SMA 905 fiber optic input, a built-in 16-bit digitizer, and is USB 2.0 plug-and-play compatible. With our spectral acquisition software, you can select between high sensitivity and high dynamic range mode within your pre-configured spectral range. Customized spectral resolution and application support are available.

Applications

About the Sol™ 1.7

• Process Monitoring• NIR Spectroscopy• Quality Control• On-line Analyzer• Material Identification


Detector

Grating

Slit

AC Power Input 100 - 240VAC 50/60 Hz, 0.5A @ 120VAC

Detector Type Linear InGaAs Array

Pixels 512 x 1 @ 25μm x 500μm per element

Spectrograph F# 3.5


Dynamic Range High Dynamic Mode: 13,000:1 High Sensitivity Mode: 6,250:1




Integration Time BWSpec 3.26: 1ms - 65,535ms x multiplier



TE Cooling Single-Stage: 5°C (default)

Weight Spectrometer: ~1.4 kg (3.1 lbs) Power Supply: ~0.8 kg (1.8 lbs)

Dimensions

Spectrometer: 180mm x 109mm x 69mm (7.1in x 4.3in x 2.7in) Power Supply: 189mm x 169mm x 76mm (7.5in x 6.6in x 3.0in)

Computer Interface USB 2.0 / 1.1 or RS232


The standard Sol™ 1.7 features a TE Cooled 512 element linear InGaAs photo diode array detector with a pixel format of 512 x 1 elements @ 25µm pixel width and 500µm pixel height with 512 effective (active) pixels. Each pixel represents a portion of the spectrum. As the incident light strikes the individual pixels across the photo diode array, the electronics translate and display their intensity using our BWSpec™ software.

Using BWSpec™, the detector mode can be switched between High Sensitivity and High Dynamic modes, allowing for greater control over the detector’s sensitivity.


Pixels 512, Others AvailablePixel Size 25µm x 500µm

Well Depth High Dynamic: ~100 Me High Sensitivity: ~40 Me

Digitzation Rate 500 kHz


Sol 1.7 - S Sol 1.7 - L

Spectral Response - Tungsten

Best Efficiency

Spectral Coverage (nm) Grating Ordering

CodeNIR 900-1700 150/1250 SNIR 900-1700 150/1250 L


S = Shorter wavelength enhanced versionL = Longer wavelength enhanced version


Slit Option Dimensions Resolution25mm 25mm wide x 1mm high ~4.0nm50mm 50mm wide x 1mm high ~5.0nm100mm 100mm wide x 1mm high ~8.4nm


Using a 512 Pixel Array


Cooling an array detector with a built-in thermoelectric cooler (TEC) is an effective way to reduce dark current and noise as well as enhance the dynamic range and detection limit.

When the InGaAs detector array is cooled down to 5oC by the TEC from a room temperature of 25oC, the dark current is reduced by 6.25 times and the dark noise is reduced by a factor of 2.5. This allows the spectrometer to operate at longer exposure times and detect weaker optical signals.

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Sol™ 2.21100 - 2200nm NIR TE Cooled InGaAs Array Spectrometer


• 9nm FWHM Spectral Resolution or customized


• Optional Shutter Available

• Optional RS232 Interface

Features:

The Sol™ 2.2 is a high performance linear InGaAs array spectrometer featuring 512 (standard) and 1024 pixels with TE Cooling down to -10oC, all while providing high throughput and large dynamic range.

Each spectrometer features an SMA 905 fiber optic input, a built-in 16-bit digitizer, and is USB 2.0 plug-and-play compatible. Using the included software, the user can choose between high sensitivity and high dynamic range mode. Flexible custom configurations and application support are available for OEM applications.

Applications




Detector

Grating Slit

AC Power Input 100 - 240VAC 50/60 Hz, 0.5A @ 120VAC

Detector Type Extended wavelength InGaAs linear array

Pixels 512 x 1 @ 25mm x 250mm per element

Spectrograph F# 3.5


Dynamic Range High Dynamic Mode: 13,000:1 High Sensitivity Mode: 6,250:1




Integration Time 10µs to > 30ms



TE Cooling Two-Stage: -10°C

Weight Spectrometer: 1.4 kg (3.1 lbs) Power Supply: 0.8 kg (1.8 lbs)

Dimensions

Spectrometer: 192mm x 109mm x 69mm (7.5in x 4.3in x 2.7in) Power Supply: 189mm x 169mm x 76mm (7.5in x 6.6in x 3.0in)

Computer Interface USB 2.0 / 1.1 or RS232


The standard Sol™ 2.2 features a TE Cooled 512 element linear InGaAs photo diode array detector with a pixel format of 512 x 1 elements @ 25µm pixel width and 250µm pixel height with 512 effective (active) pixels. Each pixel represents a portion of the spectrum. As the dispersed incident light strikes the individual pixels across the photo diode, the electronics translate and display their intensity using our BWSpec™ software.

Using BWSpec™, the detector mode can be switched between High Sensitivity and High Dynamic modes allowing for a greater control over the detector’s sensitivity.


Pixels 512 (standard), 1024Pixel Size 25µm x 250µm

Well Depth High Dynamic: ~130 Me High Sensitivity: ~5 Me


Thermoelectric CoolerCooling an array detector with a built-in thermoelectric cooler (TEC) is an effective way to reduce dark current and noise as well as enhance the dynamic range and detection limit.

When the InGaAs detector array is cooled down to -10oC by the TEC from a room temperature of 25oC, the dark current is reduced by 12.25 times and the dark noise is reduced by 3.5 times. This allows the spectrometer to operate at longer exposure times and to detect weaker optical signals.

Best Efficiency



Slit Option Dimensions Resolution512 Pixel Array

25mm 25mm wide x 1mm high ~6.0nm50mm 50mm wide x 1mm high ~9.0nm100mm 100mm wide x 1mm high ~14.0nm

1024 Pixel Array

25mm 25mm wide x 1mm high Call50mm 50mm wide x 1mm high Call100mm 100mm wide x 1mm high Call




27 28

Sol™ 2.2A1100 - 2200nm NIR TE Cooled InGaAs Array Spectrometer


• Built-In Autozero (Noise Level Reduction)

• Built-In 3-Stage Cooler

• Low Dark Noise and High Sensitivity

• Four Sensitivity & Dynamic Range Modes for Specific Application Needs

Features:

The Sol™ 2.2A is a high performance linear InGaAs array spectrometer featuring 256 pixels and providing high throughput and large dynamic range with TE Cooling down to -15oC via a built-in 3-Stage Cooler.

Each spectrometer features an SMA 905 fiber optic input, built-in 16-bit digitizer, is USB 2.0 plug-and-play compatible, and has a built-in autozero function which automatically reduces dark current and dark non-uniformity, resulting in an increased signal-to-noise ratio.

Software control allows the user to choose from four types of operation modes: Maximum Dynamic, High Dynamic, High Sensitivity, and Maximum Sensitivity. Customized spectral resolution and application support are also available.

Applications

About the Sol™ 2.2A



Detector

Grating

Slit

DC Power Input DC 5V / 13A


Detector Type Extended wavelength InGaAs linear array


Spectrograph F# 3.5


Dynamic Range

Maximum Dynamic Mode: 20,000:1High Dynamic Mode: 10,000:1 High Sensitivity Mode: 2,500:1Maximum Sensitivity Mode: 250:1



Data Transfer Speed >300 spectra per second via USB 2.0

Integration Time 250µs to >= 64ms



TE Cooling 3-Stage: -15°C @ Relative Humidity = 90%





The standard Sol™ 2.2A features a TE Cooled 256 element linear InGaAs photo diode array detector with a pixel format of 256 x 1 elements @ 50µm pixel width and 250µm pixel height with 256 effective (active) pixels. Each pixel represents a portion of the spectrum. As the dispersed incident light strikes the individual pixels across the photo diode, the photons captured by each pixel are then translated by electronics and their intensity is displayed using our BWSpec™ software.

Autozero is an automatic function of the detector which reduces the dark current and dark non-uniformity by minimizing the offset voltage on each pixel during the exposure time. This results in an increase in the signal-to-noise ratio by as much as 50 times compared to units without this feature.

Using BWSpec™, the detector mode can be switched among Maximum Dynamic Range, High Dynamic Range, High Sensitivity, and Maximum Sensitivity, allowing for greater control over different applications.



Well Depth

Maximum Dynamic Mode: ~250 MeHigh Dynamic: ~125 Me

High Sensitivity: ~12.5 MeMaximum Sensitivity Mode: 1.25 Me



Best Efficiency




Slit Option Dimensions Resolution50mm 50mm wide x 1mm high ~12.0nm100mm 100mm wide x 1mm high ~20.0nm


Using A 256 Pixel Array

Thermoelectric CoolerCooling an array detector with a built-in thermoelectric cooler (TEC) is an effective way to reduce dark current and noise as well as to enhance the dynamic range and detection limit.

When the InGaAs detector array is cooled down to -15oC by the TEC from a room temperature of 25oC, the dark current is reduced by 16 times and the dark noise is reduced by 4 times. This allows the spectrometer to operate at longer exposure times and to detect weaker optical signals.

29 30

Sol™ 2.61550nm - 2550nm* NIR TE Cooled InGaAs Array Spectrometer

• 1550nm - 2550nm* Spectral Range

• Built-In Autozero (Noise Level Reduction)


• Low Dark Noise and High Sensitivity

• Four Sensitivity & Dynamic Range Modes for Specific Application Needs

Features:

The Sol™ 2.6 is a high performance linear InGaAs array spectrometer featuring 256 pixels and providing high throughput and large dynamic range with TE Cooling down to -15oC via a built-in 3-Stage Cooler.

Each spectrometer features an SMA 905 fiber optic input, built-in 16-bit digitizer, is USB 2.0 plug-and-play compatible, and has a built-in autozero function which automatically reduces dark current and dark non-uniformity, resulting in an increased signal-to-noise ratio.

Software control allows the user to choose from four types of operation modes: Maximum Dynamic, High Dynamic, High Sensitivity, and Maximum Sensitivity. Customized spectral resolution and application support are also available.

Applications


• Process Monitoring• NIR Spectroscopy• Quality Control• On-line Analyzer• Biological Applications


Detector

GratingSlit

DC Power Input DC 5V / 13A


Detector Type Extended Wavelength InGaAs Linear Array


Spectrograph F# 3.5


Dynamic Range

Maximum Dynamic Mode: 20,000:1High Dynamic Mode: 10,000:1High Sensitivity Mode: 2,500:1Maximum Sensitivity Mode: 250:1



Data Transfer Speed >300 spectra per second via USB 2.0

Integration Time 250µs to >= 64 seconds



TE Cooling Three-Stage: -15°C @ Relative Humidity = 90%

Relative Humidity <= 80%





*Custom Ranges Available

The standard Sol™ 2.6 features a TE Cooled 256 element linear InGaAs photo diode array detector with a pixel format of 256 x 1 elements @ 50µm pixel width and 250µm pixel height with 256 effective (active) pixels. Each pixel represents a portion of the spectrum. As the dispersed incident light strikes the individual pixels across the photo diode, the photons captured by each pixel are then translated by electronics and their intensity is displayed using our BWSpec™ software.

Autozero is a automatic function of the detector which reduces the dark current and dark non-uniformity by minimizing the offset voltage on each pixel during the exposure time. This results in an increase in the signal-to-noise ratio by as much as 50 times compared to units without this feature.

Using BWSpec™, the detector mode can be switched among Maximum Dynamic Range, High Dynamic Range, High Sensitivity, and Maximum Sensitivity, allowing for greater control over different applications.

Specifications Wavelength Range 1550nm - 2550nm*


Well Depth

Maximum Dynamic Mode: ~250 MeHigh Dynamic Mode: ~125 Me

High Sensitivity Mode: ~12.5 MeMaximum Sensitivity Mode: ~1.25 Me


*Custom Ranges Available


Cooling an array detector with a built-in thermoelectric cooler (TEC) is an effective way to reduce dark current and noise, as well as enhance the dynamic range and detection limit.

When the InGaAs detector array is cooled down to -15oC by the TEC from a room temperature of 25oC, the dark current is reduced by ~32 times and the dark noise is reduced by a factor of ~5.7. This allows the spectrometer to operate at longer exposure times and to detect weaker optical signals.


Best Efficiency




Slit Option Dimensions Resolution75mm 75mm wide x 1mm high ~15.0nm


Using A 256 Pixel Array

31 32

BDS100 Deuterium/Tungsten Light Source

BDS130 Deuterium/Tungsten Light Source

The BDS100 is a DC powered turnkey SMA 905 fiber coupled UV/Vis/NIR light source with spectral output from 200 to > 1100nm. The 3W UV Lamp is an electrode-less, RF induced deuterium lamp which shares a single optical path with the 3W tungsten halogen lamp. Features include a safety shutter and individual On/Off controls for both the deuterium and tungsten sources.

The BDS130 is an AC powered turnkey SMA 905 fiber coupled UV/Vis/NIR light source with a spectral output of 190 to > 2500nm. A 30W deuterium lamp and a 5W tungsten halogen lamp share a single optical path. Features include a safety shutter and individual On/Off controls for both the deuterium and tungsten lamps.

BPS101 Tungsten Halogen Light Source

BPS120 Tungsten Halogen Light Source

The BPS101 is a DC powered high performance SMA 905 fiber coupled constant current tungsten halogen light source with a spectral output of 350 to > 2600nm. A user replaceable 5W input power bulb has a ~10,000 hour lifetime with a color temperature of 2800 K. Constant current provides precision current control for stable performance. A remote control port provides On/Off modulation, operating current monitoring, and external operating current control.

The BPS120 is a DC powered high performance SMA 905 fiber coupled constant current tungsten halogen light source with a spectral output of 350 to > 2600nm. A replaceable 20W input power bulb has a ~5,000 hour lifetime with a color temperature of 2900K. Constant current provides precision current control for stable performance. A remote control port provides On/Off modulation, operating current monitoring, and external operating current control.

Accessories Accessories

ICL Irradiance Lamps

SCL100 Spectral Calibration

The ICL series Calibrated Lamp Standards are tungsten coiled-coil filaments enclosed in quartz envelopes. Calibrated Lamps provide reliable spectral irradiance calibration data. Calibrated 100W lamps can cover 350-1050nm and 350-1700nm. Calibrated 1000W lamps can cover 350-1700nm, 350-2200nm, and 250-1100nm. Lamps are seasoned and calibration is traceable to the National Institute of Standards and Technology (NIST) scale of spectral irradiance. The lamps are provided with Calibration Data and respective lamp holders for easy installation and adjustment.

The SCL100 is a series of DC powered compact SMA 905 fiber coupled Spectral Calibration Light Sources. The SCL100 can be used for wavelength calibration of monochromators, spectrometers, and spectroradiometers. By exciting these various gases, they will produce narrow intense lines of the corresponding element(s). There are 6 lamp models to select from: Argon (Ar), Krypton (Kr), Mercury (Hg), Mercury/Argon (Hg/Ar), Neon (Ne), and Xenon (Xe).

For more information and additional accessories, please visit our website at www.bwtek.com

BPX100 Pulsed Xenon Light Source

The BPX100 is an AC powered compact SMA 905 fiber coupled 5W Xenon flash lamp module with a spectral output of 185 - 2000nm. By passing an electrical current through a Xenon gas, the BPX100 produces both continuous and line spectra. Low pulse-to-pulse variations and long operating life characteristics makes the BPX100 ideal as an excitation light source for fluorescence spectroscopy and UV rich sources for reflectance and transmittance spectrophotometry.

BPS2.0 Tungsten Halogen Light Source

The BPS2.0 is a DC powered, high performance, SMA 905 fiber coupled, constant current tungsten halogen light source with a spectral output of 350 to > 2600nm. A user replaceable 20W bulb has a ~2,000 hour lifetime with a color temperature of 2900K. Constant current provides precision current control for stable performance.

The BPS2.0 incorporates a fan for thermal stability for low drift. A remote control port provides On/Off modulation, operating current monitoring, and external operating current control.

33 34

Accessories

Fiber Patch Cords

BFA & BRS Bifurcated Fibers

Fiber Dip Probe

The Fiber Patch Cords (FPC) series are fiber optic cables terminated with fiber optic connectors on both ends and are available in single strand UV or NIR grade fused silica optical fiber with various core diameters for use in the spectral range 190nm - 2400nm.

Fiber core sizes range from 50um to 1000um. Standard lengths are 1.5 meters with custom available.

The Bifurcated Fiber Assembly (BFA) series combines optical fibers at a common end with the fiber bundle bifurcated into two separate channels. These channels can connect to a light source and a spectrometer or split an incoming signal into two separate spectrometer channels. When a collimating lens is attached to the common end of the assembly and positioned correctly, the specular reflectance for 0° angle of incidence can also be measured.

The fiber dip probe (FDP) series can be used for measuring the transmittance and absorbance of liquid solutions. The fiber dip probe can be inserted into liquids for in-situ %T/Abs measurements. Typical applications include observing changes in solutions for kinetic reaction studies or dissolution testing.

Fiber Reflectance Probe

The Fiber Reflectance Probe (FRP) series combines 7 optical fibers at the sample end into a bifurcated fiber. This bifurcated fiber splits into one fiber and 6 stacked fibers with the single fiber connecting to a light source and the 6 stacked fibers connecting to a spectrometer. These stacked fibers align to the spectrometer’s slit for increased signal input. When properly setup, the FRP can measure diffuse or specular reflectance from surfaces.

BCH100A & BCH103A Cuvette Holders

BIP2.0 Integrating Sphere

The BCH100A & BCH103A cuvette sample holders are designed for fiber optic illumination/detection. A standard 12.5 x 12.5mm (OD) (1 cm path length) cuvette can be used for liquid sample transmittance and absorbance. Two SMA 905 fiber couplers with collimated optics come with the BCH100A and three come with the BCH103. Both can be used with any B&W Tek, Inc. fiber, array spectrometer and BPS or BDS light sources. The BCH100A comes with two straight through SMA 905 ports. The BCH103A can be used for fluorescence when setup for right angle measurements with respect to illumination.

The BIP2.0 is a compact, fiber coupled integrating sphere with an integrated 20W tungsten halogen lamp which emits over the UV-NIR Spectrum. The two inch diameter integrating sphere is machined from PTFE, which is highly reflective (99% from 400-800nm), and Lambertian, over the broad spectral range of 250-2500nm.

The BIP2.0 incorporates a fan for thermal stability for low drift and operates on 12 V DC. It is designed for measuring diffused reflectance using any B&W Tek, Inc. array spectrometer.

Accessories

BIS1.5 Integrating Sphere

The BIS1.5 is a compact, integrating sphere designed as a sampling accessory for measuring diffused transmittance using any B&W Tek, Inc. array spectrometer. The 1.5 inch diameter integrating sphere is machined from PTFE, which is highly reflective (99% from 400-800nm), and Lambertian, over the broad spectral range of 250-2500nm.

For more information and additional accessories, please visit our website at www.bwtek.com

BFH105 Inline Filter Holder

The BFH105 inline filter holder is designed to hold up to three standard Ø 1 in x 5 mm filters (sold separately). The BFH105 has two SMA 905 fiber connections with collimated optics and can be used with any B&W Tek, Inc. array spectrometers and BDS or BPS light sources.

B&W Tek, Inc. · 19 Shea Way, Newark, DE 19713, USAPhone: 1-302-368-7824 · Fax: 1-302-368-7830 · Web: www.bwtek.comCopyright 2011 B&W Tek, Inc.

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Spectrometer Catalog - MadatecSpectrometer Catalog A Full Range of Spectroscopy Solutions MADAtec Srl Tel. +39-0236542401 e-mail: [email protected] ITALY 1 …