Fine guidance sensor/near-infrared imager and slitless spectrograph on James Webb Space Telescope: pupil alignment methodology and metrology

M. Maszkiewicz; N. Rowlands; D. Aldridge; A. Beaton; S. Delamer; Sheng-Hai Zheng; R. Ohl IV; P. Coulter

doi:10.1117/12.2296043

25 September 2017 Fine guidance sensor/near-infrared imager and slitless spectrograph on James Webb Space Telescope: pupil alignment methodology and metrology

M. Maszkiewicz, N. Rowlands, D. Aldridge, A. Beaton, S. Delamer, Sheng-Hai Zheng, R. Ohl IV, P. Coulter

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Proceedings Volume 10562, International Conference on Space Optics — ICSO 2016; 1056223 (2017) https://doi.org/10.1117/12.2296043
Event: International Conference on Space Optics — ICSO 2016, 2016, Biarritz, France

Abstract

The JWST is an international collaboration among the NASA, the European Space Agency (ESA), and the Canadian Space Agency (CSA). It is a large (6.5 m primary mirror diameter), infrared (0.6-27 ?m) observatory that will study the first galaxies of the early Universe, the birth of stars and protoplanetary systems as well as exoplanets.

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M. Maszkiewicz, N. Rowlands, D. Aldridge, A. Beaton, S. Delamer, Sheng-Hai Zheng, R. Ohl IV, and P. Coulter "Fine guidance sensor/near-infrared imager and slitless spectrograph on James Webb Space Telescope: pupil alignment methodology and metrology", Proc. SPIE 10562, International Conference on Space Optics — ICSO 2016, 1056223 (25 September 2017); https://doi.org/10.1117/12.2296043

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