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Status of the JWST/MIRI Focal Plane System and Cooler

Status of the JWST/MIRI Focal Plane System and Cooler

Publication date: 15 January 2009

Authors: Ressler, M.E. et al.

Journal: Bulletin of the American Astronomical Society
Volume: 41
Issue: 1
Page: 255

Copyright: The American Astronomical Society

AAS Meeting #213, #426.10

The Mid-Infrared Instrument (MIRI) is a multipurpose imager, coronagraph, and spectrometer for the James Webb Space Telescope. It provides wavelength coverage from 5 through 28 microns and is an integral contributor to all four of JWST's primary science themes. MIRI is being developed as a partnership between NASA and ESA, with JPL providing the Focal Plane System (FPS, consisting of the detectors, control electronics, and flight software) and the cooler, and a consortium of European astronomical institutes providing the optical bench and structure. The flight FPS is being prepared for delivery to the European Consortium for its integration into the optical bench, while the cooler is nearing its Critical Design Review. We describe the capabilities of the FPS and cooler, present test results and the predicted sensitivity performance of the FPS, and update the current status of each these systems. The research described in this poster was carried out at the Jet Propulsion Laboratory, California Institute of Technology, under a contract with the National Aeronautics and Space Administration.

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