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Proceedings Paper

Point-spread function modeling for the James Webb Space Telescope
Author(s): Colin Cox; Philip Hodge
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Paper Abstract

We describe software which models the Point Spread Function of the James Webb Space Telescope. The software is designed to be expandable to incorporate optical and instrument data as they become available. An initial model of the detector used in the Near Infra-red Camera has been used to generate realistic stellar images.

Paper Details

Date Published: 10 June 2006
PDF: 6 pages
Proc. SPIE 6265, Space Telescopes and Instrumentation I: Optical, Infrared, and Millimeter, 62650W (10 June 2006); doi: 10.1117/12.672010
Show Author Affiliations
Colin Cox, Space Telescope Science Institute (United States)
Philip Hodge, Space Telescope Science Institute (United States)


Published in SPIE Proceedings Vol. 6265:
Space Telescopes and Instrumentation I: Optical, Infrared, and Millimeter
John C. Mather; Howard A. MacEwen; Mattheus W. M. de Graauw, Editor(s)

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