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Proceedings Paper

Performance of the Advanced Camera for Surveys CCDs after two years on orbit
Author(s): Marco Sirianni; Max Mutchler; Mark Clampin; Holland Ford; Garth Illingworth; George Hartig; Doug van Orsow; Thomas Wheeler
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Paper Abstract

The Advanced Camera for Surveys (ACS), installed in the Hubble Space Telescope (HST) in March 2002, comprises three cameras: the Wide Field Camera (WFC), designed for deep near-IR survey imaging programs; the High Resolution Camera (HRC), a high angular resolution imager which fully samples the HST full spread function (PSF) in the visible; and the Solar Blind Camera (SBC), a far-UV imager. The WFC and HRC employ CCD detectors. Their performances are affected by the on-going damage due to the space radiation environment where they operate. We present an overview of the performance of the ACS CCD detectors, based on the first two years of flight science operations. We analyze the evolution with time of the basic detector performance that are subjected to degradation due to the on-going radiation damage. Comparison is made with ground testing prediction and with the amount of performance degradation seen in other CCD detectors on board of HST.

Paper Details

Date Published: 29 September 2004
PDF: 12 pages
Proc. SPIE 5499, Optical and Infrared Detectors for Astronomy, (29 September 2004); doi: 10.1117/12.552584
Show Author Affiliations
Marco Sirianni, European Space Agency (Netherlands)
Space Telescope Science Institute (United States)
Max Mutchler, Space Telescope Science Institute (United States)
Mark Clampin, NASA Goddard Space Flight Ctr. (United States)
Holland Ford, Johns Hopkins Univ. (United States)
Garth Illingworth, Univ. of California/Santa Cruz (United States)
George Hartig, Space Telescope Science Institute (United States)
Doug van Orsow, Space Telescope Science Institute (United States)
Thomas Wheeler, Space Telescope Science Institute (United States)


Published in SPIE Proceedings Vol. 5499:
Optical and Infrared Detectors for Astronomy
James D. Garnett; James W. Beletic, Editor(s)

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