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- W4300644446 abstract "The ``P32'' Astronomical Observation Template (AOT) provided a means to map large areas of sky (up to 45x45 arcmin) in the FIR at high redundancy and with sampling close to the Nyquist limit using the ISOPHOT C100 (3x3) and C200 (2x2) 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 describe the basic concepts of an algorithm which can successfully correct for transient response artifacts in P32 observations. Examples are given demonstrating the photometric and imaging performance of ISOPHOT P32 observations corrected using the algorithm." @default.
- W4300644446 created "2022-10-03" @default.
- W4300644446 creator A5036328991 @default.
- W4300644446 creator A5083486984 @default.
- W4300644446 date "2002-05-31" @default.
- W4300644446 modified "2023-10-18" @default.
- W4300644446 title "Photometric Mapping with ISOPHOT using the P32 Astronomical Observation Template" @default.
- W4300644446 doi "https://doi.org/10.48550/arxiv.astro-ph/0206002" @default.
- W4300644446 hasPublicationYear "2002" @default.
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