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Proceedings Paper

Si:Ga focal-plane arrays for satellite and ground-based telescopes
Author(s): Patrick Louis Mottier; Patrick Agnese; Pierre-Olivier Lagage
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Paper Abstract

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.

Paper Details

Date Published: 1 September 1991
PDF: 8 pages
Proc. SPIE 1512, Infrared and Optoelectronic Materials and Devices, (1 September 1991); doi: 10.1117/12.47149
Show Author Affiliations
Patrick Louis Mottier, CEA-LETI (France)
Patrick Agnese, CEA-DSM-SAp (France)
Pierre-Olivier Lagage, CEA-DSM-SAp (France)


Published in SPIE Proceedings Vol. 1512:
Infrared and Optoelectronic Materials and Devices
Ahmed Naumaan; Carlo Corsi; Joseph M. Baixeras; Alain J. Kreisler, Editor(s)

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