Point-spread function modeling for the James Webb Space Telescope

Colin Cox; Philip Hodge

doi:10.1117/12.672010

10 June 2006 Point-spread function modeling for the James Webb Space Telescope

Colin Cox, Philip Hodge

Proceedings Volume 6265, Space Telescopes and Instrumentation I: Optical, Infrared, and Millimeter; 62650W (2006) https://doi.org/10.1117/12.672010
Event: SPIE Astronomical Telescopes + Instrumentation, 2006, Orlando, Florida , United States

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.

Citation Download Citation

Colin Cox and 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); https://doi.org/10.1117/12.672010

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