|


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- |
|