Lower 1/f noise will allow long integration times or frame averaging. This will improve the sensitivity (i.e., signal-to-noise ratio) of the instrument. The increase of VLWIR detector operating temperatures will reduce the size, weight and power (SWaP) of infrared imagers and spectrometers. This will broaden the application areas of these instruments, in particular for low cost CubeSats/SmallSat for Earth and planetary science missions.
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