The throughput and sensitivity of the JWST mid-infrared instrument
Övrigt konferensbidrag, 2010
The Verification Model (VM) of MIRI has recently completed an extensive programme of cryogenic testing, with the Flight Model (FM) now being assembled and made ready to begin performance testing in the next few months. By combining those VM test results which relate to MIRI's scientific performance with measurements made on FM components and sub-assemblies, we have been able to refine and develop the existing model of the instrument's throughput and sensitivity. We present the main components of the model, its correlation with the existing test results and its predictions for MIRI's performance on orbit. © 2010 SPIE.
MIRI
Astronomy
Infrared
Space instrumentation
JWST
Sensitivity
Författare
A. Glasse
UK Astronomy Technology Centre
E Bauwens
KU Leuven
J. Bouwman
Max Planck Institut fur Astronomie
O. Detre
Max Planck Institut fur Astronomie
S Fischer
Universitat zu Koln
M. Garcia-Marin
Universitat zu Koln
Kay Justtanont
Chalmers, Rymd- och geovetenskap, Onsala rymdobservatorium
A. Labiano
European Space Astronomy Centre
T. Nakos
Universiteit Gent
M. E. Ressler
Jet Propulsion Laboratory, California Institute of Technology
G. H. Rieke
University of Arizona
S. Scheithauer
Max Planck Institut fur Astronomie
M. Wells
UK Astronomy Technology Centre
G. Wright
UK Astronomy Technology Centre
Proceedings of SPIE - The International Society for Optical Engineering
0277786X (ISSN) 1996756X (eISSN)
Vol. 7731 77310K978-081948221-1 (ISBN)
Ämneskategorier (SSIF 2011)
Fysik
DOI
10.1117/12.856975
ISBN
978-081948221-1