Open Access Paper
20 November 2017 The integral field unit for the James Webb space telescope's near-infrared spectrograph
David J. Purll, Daniel R. Lobb, Andrew R. Barnes, R. Gordon Talbot, Stephen Rolt, David J. Robertson, Martin F. Closs, Maurice te Plate
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Proceedings Volume 10565, International Conference on Space Optics — ICSO 2010; 105650J (2017) https://doi.org/10.1117/12.2309221
Event: International Conference on Space Optics—ICSO 2010, 2010, Rhodes Island, Greece
Abstract
The European Space Agency (ESA) is providing the Near Infrared Spectrograph (NIRSpec) developed by EADS Astrium GmbH to fly on the James Webb Space Telescope (JWST). NIRSpec covers the 0.6-5.0 µm domain. It will be primarily operated as a multi-object spectrograph, using a MEMS micro-shutter array (MSA) provided by NASA to select multiple objects from the field of view at an intermediate image plane formed by the NIRSpec fore-optics. The MSA apertures form multiple entrance slits of the spectrometer section.
© (2017) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
David J. Purll, Daniel R. Lobb, Andrew R. Barnes, R. Gordon Talbot, Stephen Rolt, David J. Robertson, Martin F. Closs, and Maurice te Plate "The integral field unit for the James Webb space telescope's near-infrared spectrograph", Proc. SPIE 10565, International Conference on Space Optics — ICSO 2010, 105650J (20 November 2017); https://doi.org/10.1117/12.2309221
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KEYWORDS
Mirrors

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Spectroscopy

Astronomical imaging

Cryogenics

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