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1 September 1991 Si:Ga focal-plane arrays for satellite and ground-based telescopes
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Since 1984, infrared sensors devices have been developed in the CEA-LETI laboratories for astronomical observation in the 4-17 micrometers wavelength band using Si:Ga detectors. These devices are to equip ISOCAM, a camera which will operate from ISO (Infrared Space Observatory), the European satellite expected to be launched in May 1993, and C10(mu) , a French astronomical camera which will be based at the CFHT (Canadian French Hawaii Telescope). In this paper, a brief description of the devices and their operating conditions, as well as main preliminary results, are given.
© (1991) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Patrick Louis Mottier, Patrick Agnese, and Pierre-Olivier Lagage "Si:Ga focal-plane arrays for satellite and ground-based telescopes", Proc. SPIE 1512, Infrared and Optoelectronic Materials and Devices, (1 September 1991);

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