Photometric Mapping with ISOPHOT using the "P32" Astronomical Observation Template

Details Photometric Mapping with ISOPHOT using the "P32" Astronomical Observation Template Photometric Mapping with ISOPHOT using the "P32" Astronomical Observation Template

Feb 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003esasp.511..365t&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

1

Scientific paper

The ``P32'' Astronomical Observation Template (AOT) provided a means to map large areas of sky (up to 45×45 arcmin) in the FIR at high redundancy and with sampling close to the Nyquist limit using the ISOPHOT C100 (3×3) and C200 (2×2) detector arrays on board ISO. However, the transient response behaviour of the Ga:Ge detectors, if uncorrected, can lead to severe systematic photometric errors and distortions of source morphology on maps. Here we demonstrate the photometric and imaging performance of an algorithm which can successfully correct for transient response artifacts in P32 observations.

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