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          Institute: MPI für Astronomie     Collection: Publikationen_mpia     Display Documents



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ID: 421401.0, MPI für Astronomie / Publikationen_mpia
Design and development of MIRI, the mid-IR instrument for JWST
Authors:Wright, G. S.; Reike, G.; Barella, P.; Boeker, T.; Colina, L.; van Dishoeck, E.; Driggers, P.; Goodson, G.; Greene, T.; Heske, A.; Henning, T.; Lagage, P. O.; Meixner, M.; Norgaard-Nielsen, H.; Olofsson, G.; Ray, T.; Ressler, M.; Thatcher, J.; Waelkens, C.; Wright, D.; Zehnder, A.
Language:English
Publisher:SPIE
Place of Publication:Bellingham, Wash.
Date of Publication (YYYY-MM-DD):2008
Title of Proceedings:Space Telescopes and Instrumentation 2008: Optical, Infrared, and Millimeter
Start Page:70100T-70100T
End Page:10
Title of Series:SPIE
Volume (in Series):7010
Name of Conference/Meeting:Society of Photo-Optical Instrumentation Engineers (SPIE) Conference Series
Review Status:not specified
Audience:Experts Only
Abstract / Description:MIRI is the mid-IR instrument for the James Webb Space Telescope and provides imaging, coronography and integral field spectroscopy over the 5-28mum wavelength range. MIRI is the only instrument which is cooled to 7K by a dedicated cooler, much lower than the passively cooled 40K of the rest of JWST, which introduces unique challenges. The paper will describe the key features of the overall instrument design. The flight model design of the MIRI Optical System is completed, with hardware now in manufacture across Europe and the USA, while the MIRI Cooler System is at PDR level development. A brief description of how the different development stages of the optical and cooling systems are accommodated is provided, but the paper largely describes progress with the MIRI Optical System. We report the current status of the development and provide an overview of the results from the qualification and test programme.
Comment of the Author/Creator:Date: 2008, August 1, 2008
External Publication Status:published
Document Type:Conference-Paper
Communicated by:N. N.
Affiliations:MPI für Astronomie
Identifiers:URL:http://adsabs.harvard.edu/abs/2008SPIE.7010E..27W [ID No:1]
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