Post-SM4 Sensitivity Calibration of the STIS Echelle Modes

Details Post-SM4 Sensitivity Calibration of the STIS Echelle Modes Post-SM4 Sensitivity Calibration of the STIS Echelle Modes

Jan 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012stis.rept....1b&link_type=abstract

Instrument Science Report STIS 2012-01, 21 pages

Physics

Hubble Telescope, Hst, Stis, Stsci

Scientific paper

On-orbit sensitivity curves for all echelle modes were derived for post - servicing mis- sion 4 data using observations of the DA white dwarf G191-B2B. Additionally, new echelle ripple tables and grating dependent bad pixel tables were created for the FUV and NUV MAMA. We review the procedures used to derive the adopted throughputs and implement them in the pipeline as well as the motivation for the modification of the additional reference files and pipeline procedures.

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