Si:Ga focal-plane arrays for satellite and ground-based telescopes

Details Si:Ga focal-plane arrays for satellite and ground-based telescopes Si:Ga focal-plane arrays for satellite and ground-based telescopes

Sep 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991spie.1512...60m&link_type=abstract

Proc. SPIE Vol. 1512, p. 60-67, Infrared and Optoelectronic Materials and Devices, Ahmed Naumaan; Carlo Corsi; Joseph M. Baixera

Astronomy and Astrophysics

Astronomy

2

Scientific paper

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.

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