The Cooled VGA SWIR InGaAs Camera from Photonic Science utilizes specific InGaAs focal plane arrays with low defective pixel count and low dark current.
The InGaAs camera has efficient cooling and stable offset, thus enabling reproducible acquisition for accurate metrology measurements in the SWIR spectrum.
Gigabit Ethernet Vision- and Camera Link-compliant interface facilitates simple integration into present systems.
OEM versions with unique form factors or cooling options are available for integration into particular systems or instruments.
Key Features
- 16-bit image processing or 14-bit digitization
- Readout noise down to generally <30 electrons
- Over 200 fps with a region of interest (ROI)
- Outstanding linearity response to varying intensities and or exposures
- Camera Link interface and Gigabit Ethernet
- Software option: Labview VIs and SDK kit
Specifications
. |
. |
Spectral Range |
900 - 1700 nm |
Resolution |
640 x 512 |
Sensor Size |
9.6 mm x 7.68 mm |
Frame Rate |
174 fps at full VGA resolution
570 fps at ¼ VGA resolution
7,200 fps at 640x4 resolution (spectroscopy or line mode) |
Pitch |
15 μm x 15 μm |
Full Well Capacity |
20 k - 23 k electrons (high gain mode)
80 k - 105 k electrons (mid-gain mode)
1.0 M - 1.5 M electrons (low gain mode) |
Read Out Noise |
28 - 38 electrons (high gain mode)
50 - 77 electrons (mid-gain mode)
500 - 800 electrons (low gain mode) |
Reading Mode |
Integrate Then Read, Integrate While Reading |
Dark Current |
<0.7 fA with air cooling & <0.1 fA with water cooling |
Sensor Temperature (ºC) |
-25 °C with air cooling, -50 °C with water cooling (lower dark current) |
Corrections |
Non-uniformity, bright pixel, gain, offset, flatfield |
ADC |
14-bit with 16-bit digital processing |
Exposure |
30 microseconds up to >1 minute |
QE at 1500 nm |
80% |
Applications
Available with Passive Cooling
- SWIR airborne payload
- SWIR handheld vision improvement
- Semiconductor inspection
- Photoluminescence for solar cells
Air Cooling or Water Cooling for Long Exposure
- Spectroscopy
- Astronomy
- Laser beam profiling
- Hyperspectral imaging