Detailed Performance of IR Detectors for WFC3

Details Detailed Performance of IR Detectors for WFC3 Detailed Performance of IR Detectors for WFC3

May 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003aas...202.0401h&link_type=abstract

American Astronomical Society Meeting 202, #04.01; Bulletin of the American Astronomical Society, Vol. 35, p.703

Computer Science

Performance

Scientific paper

Wide Field Camera 3 (WFC3), which is to be installed on the Hubble Space Telescope during Servicing Mission 4, will employ a 1Kx1K Rockwell HgCdTe detector in the focal plane of its IR channel. In-depth studies of the performance of these detectors have been made at the GSFC Detector Characterization Lab. These detectors represent a significant improvement in performance over earlier generations of IR detectors. We present here the results of detailed investigations of the on-board reference pixels, noise properties, bias stability and other features of these devices. The scientific performance of the flight-selected detectors is presented in a companion paper by Robberto et.al.

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