Aspects of LWS processing

Details Aspects of LWS processing Aspects of LWS processing

Mar 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999esasp.427...81l&link_type=abstract

The Universe as Seen by ISO. Eds. P. Cox & M. F. Kessler. ESA-SP 427., p. 81

Physics

6

Iso Lws, Spectroscopy, Calibration

Scientific paper

We present an outline of various stages of the Long Wavelength Spectrometer (LWS) data pipeline processing, from the conversion of the output from the detectors through to a calibrated spectrum. Normal calibration is based on a linear relationship between the Uranus data from the LWS and a theoretical model of the planet. For strong sources, however, some of the detectors behave non-linearly. We show that, using a strong source for which we have a good model as a calibrator, these data can be corrected. Examples of the resulting spectra are shown.

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