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Proceedings Paper • Open Access

Fine guidance sensor/near-infrared imager and slitless spectrograph on James Webb Space Telescope: pupil alignment methodology and metrology
Author(s): M. Maszkiewicz; N. Rowlands; D. Aldridge; A. Beaton; S. Delamer; Sheng-Hai Zheng; R. Ohl IV; P. Coulter

Paper 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.

Paper Details

Date Published: 25 September 2017
PDF: 9 pages
Proc. SPIE 10562, International Conference on Space Optics — ICSO 2016, 1056223 (25 September 2017); doi: 10.1117/12.2296043
Show Author Affiliations
M. Maszkiewicz, Canadian Space Agency (Canada)
N. Rowlands, COM DEV International Systems (Canada)
D. Aldridge, COM DEV International Systems (Canada)
A. Beaton, COM DEV International Systems (Canada)
S. Delamer, COM DEV International Systems (Canada)
Sheng-Hai Zheng, COM DEV International Systems (Canada)
R. Ohl IV, NASA Goddard Space Flight Ctr. (United States)
P. Coulter, NASA Goddard Space Flight Ctr. (United States)

Published in SPIE Proceedings Vol. 10562:
International Conference on Space Optics — ICSO 2016
Bruno Cugny; Nikos Karafolas; Zoran Sodnik, Editor(s)

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