Paper
10 December 2001 HST-COS far-ultraviolet detector: final ground calibration
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Abstract
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.
© (2001) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
John V. Vallerga, Jason B. McPhate, Adrian P. Martin, Geoffrey A. Gaines, Oswald H. W. Siegmund, Erik Wilkinson, Steven Penton, and Stephane Beland "HST-COS far-ultraviolet detector: final ground calibration", Proc. SPIE 4498, UV/EUV and Visible Space Instrumentation for Astronomy and Solar Physics, (10 December 2001); https://doi.org/10.1117/12.450052
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Cited by 13 scholarly publications.
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KEYWORDS
Sensors

Microchannel plates

Calibration

Quantum efficiency

Spatial resolution

Spectrographs

Diodes

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