Detectors and arrays of ISO's photopolarimeter

Details Detectors and arrays of ISO's photopolarimeter Detectors and arrays of ISO's photopolarimeter

Sep 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989spie.1130..222l&link_type=abstract

IN: New technologies for astronomy; Proceedings of the Meeting, Paris, France, Apr. 25, 26, 1989 (A90-37976 16-89). Bellingham,

Astronomy and Astrophysics

Astronomy

Astronomical Photometry, Infrared Space Observatory (Iso), Photometers, Polarimeters, Satellite-Borne Instruments, Design Analysis, Pixels, Signal To Noise Ratios, Spectrophotometry

Scientific paper

The 'Isophot' photometry experiment of the IR Space Observatory allows multiband/multiaperture photopolarimetry, as well as multicolor polarimetric imaging and spectrophotometry. In order to cover the 2.5-240 micron wavelength range, five different detector materials have been used, arranged as two-dimensional arrays, linear arrays, and single detectors; a total of 223 different detectors is included. Accounts are presently given of the sources of noise in detector assemblies, the design of an integrating preamplifier unit, and the anticipated effects of high-energy radiation effects on detectors.

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