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A full range of small-footprint, fiber optic spectrometers covering 150 - 2500 nm with FWHM resolution starting at 0.1 nm
 
Solar resistant, UV/VIS and VIS/NIR fibers with a range of jacketing and termination options
 
Driver platforms for embedded and other system designs supporting Windows, Mac OS and Linux
 
O2 and pH sensors for both aqueous and atmospheric applications
 
For use with the S2000 and multi-channel systems
 

The Ocean Optics line of high-sensitivity back-thinned 2D FFT-CCD spectrometers for low light-level, UV-sensitive and other scientific applications now includes the uncooled Maya2000 and Maya2000 Pro, which offer greater than 90% quantum efficiency, high dynamic range and excellent deep-UV response (<190 nm).

Advantages of Back-thinned FFT-CCD Detectors

Back-Thinned CCD area image sensors have high UV response, great signal-to-noise characteristics and wide dynamic range, making them especially suited for low light level applications. Because of their great native UV response, FFT-CCD detectors do not require the application of UV-sensitive coatings, which is common with standard CCD-array detectors. That’s important because batch-to-batch variation can be problematic with some UV coatings.

  • Maya2000 Pro has >75% quantum efficiency; Maya2000 has 90% QE

  • USB 2.0 interface

  • Low-noise electronics

  • Optical resolution to ~0.035 nm (FWHM); resolution depends on groove density of grating and size of entrance aperture (slit)

  • 14 grating options (ask us about options that provide expanded range).

  • Slits available in widths of 5 µm, 10 µm, 25 µm, 50 µm, 100 µm and 200 µm

  • Optional propriety order-sorting filters to eliminate second- and third-order effects

  • Maya2000 offers the detector collection lens option for enhanced signal collection

  • Fully controllable strobe signals (single or continuous)

  • 10 onboard digital user-programmable GPIOs

Maya2000 Nitrogen Purgebox

The Nitrogen Purgebox gives you the ability to measure under nitrogen flushed conditions. Use it for applications where oxygen is negatively influencing your measurements - like deep UV (below 190 nm). The Nitrogen Purgebox helps eliminate absorption from oxygen.

Under the Hood - Maya2000
Detector Hamamatsu S9840
Architecture: Back-thinned, 2D
Thermoelectric cooling: No
# of Pixels: All: 2080x20
Active: 2048x14
Pixel size: 14 um square
Detector active area (mm): 28.672 horizontal x 0.196 vertical
Well depth: 130Ke-
Peak QE >90%
QE @ 250 nm 55%
Spectrometer
Integration time: 6 ms - 10 seconds
A/D converter: 16 bit, 500 kHz
Dynamic range (typical): 5700:1
Signal-to-noise ratio: 350:1
Non-linearity (uncorrected): ~4.0%
Linearity (corrected): >99.7%
Column sensitivity: ~0.45 Counts/e-

Under the Hood - Maya2000 Pro
Detector Hamamatsu S10420
Architecture: Back-thinned, 2D
Thermoelectric cooling: No
# of Pixels: All: 2068x70
Active: 2048x64
Pixel size: 14 um square
Detector active area (mm): 28.672 horizontal x 0.896 vertical
Well depth: 200Ke-
Peak QE 75%
QE @ 250 nm 60%
Spectrometer
Integration time: 6 ms - 5 seconds
A/D converter: 16 bit, 500 kHz
Dynamic range (typical): 12000:1
Signal-to-noise ratio: 450:1
Non-linearity (uncorrected): ~4.0%
Linearity (corrected): >99.7%
Column sensitivity: ~0.32 Counts/e-
 

 
 

Contact us: +1 727-733-2447 | oem@oceanoptics.com
Contents and images are Copyright Ocean Optics, Inc. 2012 or used by permission.
All logos and product names used are trademarks of Ocean Optics, Inc. All rights reserved.