HST-COS far-ultraviolet detector: final ground calibration

Details HST-COS far-ultraviolet detector: final ground calibration HST-COS far-ultraviolet detector: final ground calibration

Dec 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001spie.4498..141v&link_type=abstract

Proc. SPIE Vol. 4498, p. 141-151, UV/EUV and Visible Space Instrumentation for Astronomy and Solar Physics, Oswald H. Siegmund;

Astronomy and Astrophysics

Astronomy

3

Scientific paper

The flight microchannel plate detectors to be used in the Cosmic Origins Spectrograph, a fourth generation instrument for the Hubble Space Telescope, have been calibrated in the laboratory before being integrated into the spectrograph. This paper presents the results of these calibrations that include measurements of the detector quantum efficiency, spatial resolution, spatial linearity, flat field, electronic livetime and the local count rate limit.

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