An astronomy camera for low background applications in the 1.0 to 2.5 micron spectral region

Computer Science – Performance

Scientific paper

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Astronomical Photography, Focal Plane Devices, Imaging Spectrometers, Infrared Spectrometers, Earth Observing System (Eos), Indium Arsenides, Mercury Cadmium Tellurides, Signal To Noise Ratios

Scientific paper

A description is given of a low-background astronomy camera system based on a short wavelength (1.0-2.5 micron) 128 x 128 focal plane array. The camera is designed to accept either a HgCdTe array for the 1-2.5 micron spectral region or an InSb array for the 3-5 micron spectral region. A cryogenic folded optical system is utilized to control excess stray light along with a cold eight-position filter wheel for spectral filtering. The camera head and electronics will also accept a 256 x 256 focal plane. Engineering evaluation of the system and two engineering runs at the JPL Table Mountain Observatory have been completed. System design, engineering performance, and sample imagery are presented.

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