Resources
Andor’s iDus InGaAs 2.2 array detector series provides the most optimized platform for Spectroscopy applications between 1.6 and 2.2 µm. The TE-cooled, in-vacuum sensors reach cooling temperatures of -90°C where best Signal-to-Noise ratio can be achieved.
Andor's iDus InGaAs 2.2 array detector series provides the most optimized platform for Spectroscopy applications up to 2.2 µm. The TE-cooled, in-vacuum InGaAs camera sensors reach cooling temperatures of -90°C where best Signal-to-Noise ratio can be achieved. Indeed dark current will improve moderately below -90°C where scene black body radiation will dominate, while Quantum Efficiency of the sensor will be greatly impacted at these lower temperatures and lead to a lower Signal-to-Noise ratio.
0.8 to 2.2 µm - Operating wavelength range
Peak QE of > 70% - High detector sensitivity
TE cooling to -90°C - Negligible dark current without the inconvenience of LN2
UltraVac™ - Permanent vacuum integrity, critical for deep cooling and sensor performance
Single window design - Delivers maximum photon throughput
25 µm pixel width option - Ideal for high-resolution NIR spectroscopy
Simple USB 2.0 connection - USB plug and play – no controller box. Inputs & Outputs: External Trigger, Fire and Shutter TTL readily accessible. I2C for the more adventurous user
Software selectable output amplifiers - Allows user to optimize operation with choice of High Dynamic Range (HDR) or High Sensitivity (HS) modes of operation
Minimum exposure time of 1.4 µs - Enables higher time-resolution and minimization of dark current contribution for applications with reasonable signal level
XW-RECR - Coolant re-circulator for enhanced cooling performance
ACC-XW-CHIL-160 - Oasis 160 Ultra Compact Chiller Unit (tubing to be ordered separately)
ACC-6MM-TUBING-2xxxxM - 6 mm tubing option for ACC-XW-CHIL-160
SR-ASZ-0033 - SR-750 Adapter Flange for InGaAs detector.
ACC-SD-VDM1000 - Shutter Driver for NS25B Bistable Shutter (not needed for Shamrock spectrographs)
ACC-SHT-NS25B - Bistable Shutter, Standalone (not needed for Shamrock spectrographs)