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Proceedings Paper

Progress with the design and development of MIRI, the mid-IR instrument for JWST
Author(s): G. S. Wright; G. Rieke; T. Boeker; L. Colina; E. van Dishoeck; P. Driggers; S. Friedman; A. Glasse; G. Goodson; T. Greene; M. Guedel; T. Henning; P.-O. Lagage; J. Lorenzo-Alvarez; M. Meixner; H. Norgaard-Nielsen; G. Olofsson; T. Ray; M. Ressler; K. Sukhatme; J. Thatcher; C. Waelkens; D. Wright
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Paper Abstract

MIRI is one of four instruments to be built for the James Webb Space Telescope. It provides imaging, coronography and integral field spectroscopy over the 5-28.5um 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, and consists of both an Optical System and a Cooler System. This paper will describe the key features of the overall instrument design and then concentrate on the status of the MIRI Optical System development. The flight model design and manufacture is complete, and final assembly and test of the integrated instrument is now underway. Prior to integration, all of the major subassemblies have undergone individual environmental qualification and performance tests and end-end testing of a flight representative model has been carried out. The paper will provide an overview of results from this testing and describe the current status of the flight model build and the plan for performance verification and ground calibration.

Paper Details

Date Published: 4 August 2010
PDF: 10 pages
Proc. SPIE 7731, Space Telescopes and Instrumentation 2010: Optical, Infrared, and Millimeter Wave, 77310E (4 August 2010); doi: 10.1117/12.857262
Show Author Affiliations
G. S. Wright, UK Astronomy Technology Ctr. (United Kingdom)
G. Rieke, Steward Observatory, The Univ. of Arizona (United States)
T. Boeker, European Space Research and Technology Ctr. (Netherlands)
L. Colina, Consejo Superior de Investigaciones Científicas (Spain)
E. van Dishoeck, Leiden Observatory, Leiden Univ. (Netherlands)
P. Driggers, NASA Goddard Space Flight Ctr. (United States)
S. Friedman, Space Telescope Science Institute (United States)
A. Glasse, UK Astronomy Technology Ctr. (United Kingdom)
G. Goodson, Jet Propulsion Lab. (United States)
T. Greene, NASA Ames Research Ctr. (United States)
M. Guedel, Univ. of Vienna (Austria)
T. Henning, Max-Planck-Institut für Astronomie (Germany)
P.-O. Lagage, Service d'Astrophysique, CEA (France)
J. Lorenzo-Alvarez, European Space Research and Technology Ctr. (Netherlands)
M. Meixner, Space Telescope Science Institute (United States)
H. Norgaard-Nielsen, Danish Space Research Institute (Denmark)
G. Olofsson, Stockholm Observatory (Sweden)
T. Ray, The Dublin Institute for Advanced Studies (Ireland)
M. Ressler, Jet Propulsion Lab. (United States)
K. Sukhatme, Jet Propulsion Lab. (United States)
J. Thatcher, EADS Astrium Ltd. (United Kingdom)
C. Waelkens, Instituut voor Sterrenkunde, Katholieke Univ. Leuven (Belgium)
D. Wright, EADS Astrium Ltd. (United Kingdom)


Published in SPIE Proceedings Vol. 7731:
Space Telescopes and Instrumentation 2010: Optical, Infrared, and Millimeter Wave
Jacobus M. Oschmann; Mark C. Clampin; Howard A. MacEwen, Editor(s)

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