5 March 2003 NGST MIRI instrument
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The MIRI is the mid-IR (5-28μm) instrument for NGST and provides for imaging, cororographic, high- and low-resolution spectroscopic capabilities. Unlike to the other instruments on NGST, the MIRI must be cooled - to reduce the thermal background from the optics and because the detectors require an operating temperature of about 7k.. In this paper we summarise the science goals, the proposed overall opto-mechanical concept, the thermal design aspects, the detectors and the expected sensitivity of the instrument.
© (2003) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Gillian S. Wright, Gillian S. Wright, Fabio Bortoletto, Fabio Bortoletto, Carl F. Bruce, Carl F. Bruce, Ewine F. van Dishoeck, Ewine F. van Dishoeck, Avinash R. Karnik, Avinash R. Karnik, Pierre-Olivier Lagage, Pierre-Olivier Lagage, Melora E. Larson, Melora E. Larson, Dietrich Lemke, Dietrich Lemke, Goran Oloffson, Goran Oloffson, Edward A. Miller, Edward A. Miller, Thomas F. E. Henning, Thomas F. E. Henning, Sam Heys, Sam Heys, Tom Ray, Tom Ray, J. Rodriguez, J. Rodriguez, Eugene Serabyn, Eugene Serabyn, Ian Walters, Ian Walters, } "NGST MIRI instrument", Proc. SPIE 4850, IR Space Telescopes and Instruments, (5 March 2003); doi: 10.1117/12.461607; https://doi.org/10.1117/12.461607

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