Paper
1 September 1991 In-flight performance of the faint object camera of the Hubble Space Telescope
Perry E. Greenfield, Francesco Paresce, David A. Baxter, Philip Hodge, Richard N. Hook, Peter Jakobsen, Robert Ian Jedrzejewski, Anatonella Nota, William Brian Sparks, Nigel Mark Towers, Robin J. Laurance, Duccio Macchetto
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Abstract
An overview of the Faint Object Camera and its performance to date is presented. In particular, the detector's efficiency, the spatial uniformity of response, distortion characteristics, detector and sky background, detector linearity, spectrography, and operation are discussed. The effect of the severe spherical aberration of the telescope's primary mirror on the camera's point spread function is reviewed, as well as the impact it has on the camera's general performance. The scientific implications of the performance and the spherical aberration are outlined, with emphasis on possible remedies for spherical aberration, hardware remedies, and stellar population studies.
© (1991) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Perry E. Greenfield, Francesco Paresce, David A. Baxter, Philip Hodge, Richard N. Hook, Peter Jakobsen, Robert Ian Jedrzejewski, Anatonella Nota, William Brian Sparks, Nigel Mark Towers, Robin J. Laurance, and Duccio Macchetto "In-flight performance of the faint object camera of the Hubble Space Telescope", Proc. SPIE 1494, Space Astronomical Telescopes and Instruments, (1 September 1991); https://doi.org/10.1117/12.46711
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Cited by 3 scholarly publications.
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KEYWORDS
Optical fiber cables

Cameras

Sensors

Stars

Point spread functions

Distortion

Space telescopes

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