The Mid-Infrared Instrument for the James Webb Space Telescope, III: MIRIM, The MIRI Imager
Artikel i vetenskaplig tidskrift, 2015
In this article, we describe the Mid-Infrared Imager Module (MIRIM), which provides broadband imaging in the 5-27 mu m wavelength range for the James Webb Space Telescope. The imager has a 0 ''.11 pixel scale and a total unobstructed view of 74 '' x 113 '' The remainder of its nominal 113 '' x 113 '' field is occupied by the coronagraphs and the low-resolution spectrometer. We present the instrument optical and mechanical design. We show that the test data, as measured during the test campaigns undertaken at CEA-Saclay, at the Rutherford Appleton Laboratory, and at the NASA Goddard Space Flight Center, indicate that the instrument complies with its design requirements and goals. We also discuss the operational requirements (multiple dithers and exposures) needed for optimal scientific utilization of the MIRIM.
SPECTROMETER
Författare
P. Bouchet
Centre national de la recherche scientifique (CNRS)
M. Garcia-Marin
Universität zu Köln
P. O. Lagage
Centre national de la recherche scientifique (CNRS)
J. Amiaux
Centre national de la recherche scientifique (CNRS)
J. L. Augueres
Centre national de la recherche scientifique (CNRS)
E Bauwens
KU Leuven
Jadl Blommaert
KU Leuven
Vlaamse Instelling voor Technologisch Onderzoek (VITO)
Vrije Universiteit Brüssel (VUB)
C. H. Chen
Space Telescope Science Institute (STScI)
O. Detre
Max-Planck-Gesellschaft
D. Dicken
Centre national de la recherche scientifique (CNRS)
D. Dubreuil
Centre national de la recherche scientifique (CNRS)
P. Galdemard
Centre national de la recherche scientifique (CNRS)
R. Gastaud
Le Commissariat à l’Énergie Atomique et aux Énergies Alternatives (CEA)
A. Glasse
Royal Observatory
K. D. Gordon
Universiteit Gent
Space Telescope Science Institute (STScI)
F. Gougnaud
Le Commissariat à l’Énergie Atomique et aux Énergies Alternatives (CEA)
P. Guillard
Université Paris-Sud
Kay Justtanont
Chalmers, Rymd- och geovetenskap, Radioastronomi och astrofysik
O. Krause
Max-Planck-Gesellschaft
D. Leboeuf
Le Commissariat à l’Énergie Atomique et aux Énergies Alternatives (CEA)
Y. Longval
Université Paris-Sud
L. Martin
Laboratoire d'Astrophysique de Marseille
E. Mazy
Universite de Liège
V. Moreau
Centre national de la recherche scientifique (CNRS)
G. Olofsson
Stockholms universitet
T. P. Ray
Dublin Institute for Advanced Studies
J. M. Rees
Université Pierre et Marie Curie (UPMC)
E. Renotte
Universite de Liège
M. E. Ressler
Jet Propulsion Laboratory, California Institute of Technology
S. Ronayette
Centre national de la recherche scientifique (CNRS)
S. Salasca
Le Commissariat à l’Énergie Atomique et aux Énergies Alternatives (CEA)
S. Scheithauer
Max-Planck-Gesellschaft
J. Sykes
University Of Leicester
M. P. Thelen
Jet Propulsion Laboratory, California Institute of Technology
M. Wells
Royal Observatory
D. Wright
G. S. Wright
Royal Observatory
Publicerad i
Publications of the Astronomical Society of the Pacific
0004-6280 (ISSN) 1538-3873 (eISSN)
Vol. 127 Nummer/häfte 953 s. 612-622Kategorisering
Ämneskategorier (SSIF 2011)
Astronomi, astrofysik och kosmologi
Identifikatorer
DOI
10.1086/682254