Paper
12 October 2004 Wavefront sensing using a multi-object spectrograph (NIRSpec)
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Abstract
An analysis is presented that illustrates how the James Webb Space Telescope (JWST) fine-phasing process can be carried out using the Near-Infrared Spectrograph (NIRSpec) data collected at the science focal plane. The analysis considers a multi-plane diffraction model which properly accounts for the microshutter diffractive element placed at the first relay position of the spectrograph. Wavefront sensing results are presented based on data collected from the NASA Goddard Microshutter Optical Testbed.
© (2004) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Bruce H. Dean, Rene A. Boucarut, Jeffrey Scott Smith, and Theo Hadjimichael "Wavefront sensing using a multi-object spectrograph (NIRSpec)", Proc. SPIE 5487, Optical, Infrared, and Millimeter Space Telescopes, (12 October 2004); https://doi.org/10.1117/12.550912
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CITATIONS
Cited by 2 scholarly publications.
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KEYWORDS
Wavefront sensors

Data modeling

Diffraction

James Webb Space Telescope

Phase retrieval

Spectrographs

Mirrors

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