Sensitivity Calibration of Far-Ultraviolet Imaging Spectrograph

Details Sensitivity Calibration of Far-Ultraviolet Imaging Spectrograph Sensitivity Calibration of Far-Ultraviolet Imaging Spectrograph

Dec 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004jass...21..383k&link_type=abstract

Journal of Astronomy and Space Sciences. Vol. 21, no. 4, 383-390

Astronomy and Astrophysics

Astronomy

Far-Ultraviolet, White Dwarf, Effective Area

Scientific paper

We describe the in-flight sensitivity calibration of the Far ultraviolet Imaging Spectrograph (FIMS, also known as SPEAR) onboard the first Korean science satellite, STSAT-1, which was launched in September 2003. The sensitivity calibration is based on a comparison of the FIMS observations of the hot white dwarf G191B2B, and two O-type stars Alpha-Cam, HD93521 with the HUT (Hopkins Ultraviolet Telescope) observations. The FIMS observations for the calibration targets have been conducted from November 2003 through May 2004. The effective areas calculated from the targets are compared with each other.

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