Please use this identifier to cite or link to this item: http://hdl.handle.net/2381/33095
Title: The Mid-Infrared Instrument for the James Webb Space Telescope, II: Design and Build
Authors: Wright, GS
Wright, D
Goodson, GB
Rieke, GH
Aitink-Kroes, G
Amiaux, J
Aricha-Yanguas, A
Azzollini, R
Banks, K
Barrado-Navascues, D
Belenguer-Davila, T
Bloemmart, JADL
Bouchet, P
Brandl, BR
Colina, L
Detre, O
Diaz-Catala, E
Eccleston, P
Friedman, SD
Garcia-Marin, M
Guedel, M
Glasse, A
Glauser, AM
Greene, TP
Groezinger, U
Grundy, T
Hastings, P
Henning, T
Hofferbert, R
Hunter, F
Jessen, NC
Justtanont, K
Karnik, AR
Khorrami, MA
Krause, O
Labiano, A
Lagage, P-O
Langer, U
Lemke, D
Lim, T
Lorenzo-Alvarez, J
Mazy, E
McGowan, N
Meixner, ME
Morris, N
Morrison, JE
Mueller, F
Rgaard-Nielson, H-UN
Olofsson, G
O'Sullivan, B
Pel, J-W
Penanen, K
Petach, MB
Pye, John P.
Ray, TP
Renotte, E
Renouf, I
Ressler, ME
Samara-Ratna, P
Scheithauer, S
Schneider, A
Shaughnessy, B
Stevenson, T
Sukhatme, K
Swinyard, B
Sykes, J
Thatcher, J
Tikkanen, Tuomo Ville
van Dishoeck, EF
Waelkens, C
Walker, H
Wells, M
Zhender, A
First Published: 5-Jun-2015
Publisher: The University of Chicago Press on behalf of the Astronomical Society of the Pacific
Citation: Publications of the Astronomical Society of the Pacific, 2015, 127 (953), pp. 595-611
Abstract: The Mid-InfraRed Instrument (MIRI) on the James Webb Space Telescope (JWST) provides measurements over the wavelength range 5 to 28.5 μm. MIRI has, within a single “package,” four key scientific functions: photometric imaging, coronagraphy, single-source low-spectral resolving power (R ∼ 100) spectroscopy, and medium-resolving power (R ∼ 1500 to 3500) integral field spectroscopy. An associated cooler system maintains MIRI at its operating temperature of < 6.7 K. This paper describes the driving principles behind the design of MIRI, the primary design parameters, and their realization in terms of the “as-built” instrument. It also describes the test program that led to delivery of the tested and calibrated Flight Model to NASA in 2012, and the confirmation after delivery of the key interface requirements.
DOI Link: 10.1086/682253
ISSN: 0004-6280
Links: http://www.jstor.org/stable/info/10.1086/682253
http://hdl.handle.net/2381/33095
Version: Publisher Version
Status: Peer-reviewed
Type: Journal Article
Rights: Copyright © 2015. The Astronomical Society of the Pacific. All rights reserved.
Description: Deposited with reference to the societies open access archiving policy
Appears in Collections:Published Articles, Dept. of Physics and Astronomy

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