Frequently Asked Questions about Fouks models and transient correction methods for the ISOCAM LW Detector

Details Frequently Asked Questions about Fouks models and transient correction methods for the ISOCAM LW Detector Frequently Asked Questions about Fouks models and transient correction methods for the ISOCAM LW Detector

Feb 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003esasp.511..335c&link_type=abstract

Exploiting the ISO Data Archive. Infrared Astronomy in the Internet Age, held in Siguenza, Spain 24-27 June, 2002. Edited by

Astronomy and Astrophysics

Astronomy

Scientific paper

At low temperature and at very low (astrophysical) incoming flux, most of the IR detectors are affected by transient response, which delay the response and can strongly bias the estimated flux. The LW detector of ISOCAM is also affected by such an effect. It has been shown that an important component of the transient effects of this detector can be described with high accuracy using a non linear and non symmetrical model coming from the physics. An inversion method is also available. In this FAQ, we review the limitations of this model and the known problems occurring with the correction method, and we give several advices to process the data.

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