STIS Sensitivity Calibration

Details STIS Sensitivity Calibration STIS Sensitivity Calibration

Dec 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997aas...191.1811b&link_type=abstract

American Astronomical Society, 191st AAS Meeting, #18.11; Bulletin of the American Astronomical Society, Vol. 29, p.1240

Astronomy and Astrophysics

Astronomy

Scientific paper

Point source sensitivity curves are derived for the first order modes G140L, G230L, G230LB, G430L, and G750L, which collectively span a wavelength range from 1140 Angstroms to 10320 Angstroms. The curves are determined by comparing wide slit (52" x 2") observations of the spectrophotometric standard star GD153 to a pure hydrogen white dwarf model. The calibration is checked by comparing a calibrated STIS observation of the spectrophotometric standard star BD+75D325 to FOS flux values. Absolute spectrophotometric accuracies produced by routine processing of STIS data will be summarize.

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