Non-linear transient models and transient corrections methods for IR low-background photo-detectors

Details Non-linear transient models and transient corrections methods for IR low-background photo-detectors Non-linear transient models and transient corrections methods for IR low-background photo-detectors

Jul 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004aspc..314..566c&link_type=abstract

Astronomical Data Analysis Software and Systems (ADASS) XIII, Proceedings of the conference held 12-15 October, 2003 in Strasbou

Astronomy and Astrophysics

Astronomy

2

Scientific paper

Physical models are used to reproduce and correct transient effects of infrared (IR) photo-detectors in time series after incoming illumination changes. Such photo-detectors, working at low background for IR astronomy in space, cover the ranges 6-15 μm (Si:Ga), 40-110 μm (unstressed Ge:GA) and 120-210 μm (stressed Ge:Ga) and are working at low temperature. We discuss detectors models (direct models) and transients corrections (inversion methods). Some have been successfully applied to ISO data, others are in preparation for SIRTF (MIPS) -- launched in August 2003 -- and ASTRO-F (FIS) -- to be launched in 2005. New results for MIPS 160 μm and the FTS of ASTRO-F/FIS are evidenced.

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