Optical performance modeling of the James Webb Space Telescope

Allison A. Barto; Paul A. Lightsey

doi:10.1117/12.550088

12 October 2004 Optical performance modeling of the James Webb Space Telescope

Allison A. Barto, Paul A. Lightsey

Proceedings Volume 5487, Optical, Infrared, and Millimeter Space Telescopes; (2004) https://doi.org/10.1117/12.550088
Event: SPIE Astronomical Telescopes + Instrumentation, 2004, Glasgow, United Kingdom

Abstract

The James Webb Space Telescope (JWST) is a large space based astronomical telescope that will operate at cryogenic temperatures, and utilizes a segmented primary mirror with active control. To achieve the science goals for JWST, the image quality over a wide spectral range is necessary. Several metrics related to the quality of the PSF have been used to capture the optical requirement to meet the science goals. We will present the performance predictions for the JWST based on the results of the detailed allocations of the optical requirements.

Citation Download Citation

Allison A. Barto and Paul A. Lightsey "Optical performance modeling of the James Webb Space Telescope", Proc. SPIE 5487, Optical, Infrared, and Millimeter Space Telescopes, (12 October 2004); https://doi.org/10.1117/12.550088

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