The STIS Pipeline - Determination of Calibration Switch Settings

Details The STIS Pipeline - Determination of Calibration Switch Settings The STIS Pipeline - Determination of Calibration Switch Settings

Oct 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998stis.rept...28d&link_type=abstract

STIS Instrument Science Report ISR 98-28, 15 pages

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Hubble Space Telescope, Hst, Space Telescope Science Institute, Stis, Space Telescope Imaging Spectrograph

Scientific paper

There are many possible calibrations that can be performed on STIS data, so care must be taken in determining the rules that are used to select what calibrations are performed on a given dataset. In some cases, a given calibration is never performed (because we have found that it is not necessary), while others are always performed (because they are very basic calibrations). The execution of most calibrations, however, is determined by the mode of observation (imaging vs. spectroscopy, supported vs. available, CCD vs. MAMA). In this ISR, we present the rules used to set the defaults for the calibration switches for the various modes of STIS. Users may change the default settings (to optimize the processing for their particular science) and reprocess the data as needed.

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