10 June 2006 Point-spread function modeling for the James Webb Space Telescope
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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.
© (2006) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Colin Cox, Colin Cox, Philip Hodge, Philip Hodge, "Point-spread function modeling for the James Webb Space Telescope", Proc. SPIE 6265, Space Telescopes and Instrumentation I: Optical, Infrared, and Millimeter, 62650W (10 June 2006); doi: 10.1117/12.672010; https://doi.org/10.1117/12.672010


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