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The Mid-Infrared Instrument for the James Webb Space Telescope, I: Introduction

Rieke, G. H. (author)
University of Arizona
Wright, G. S. (author)
Royal Observatory
Boker, T. (author)
European Space Agency (ESA)
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Bouwman, J. (author)
Max Planck Gesellschaft zur Förderung der Wissenschaften e.V. (MPG),Max Planck Society for the Advancement of Science (MPG)
Colina, L. (author)
Centro de Astrobiologia (CAB)
Glasse, A. (author)
Royal Observatory
Gordon, K. D. (author)
Universiteit Gent,Ghent university,Space Telescope Science Institute (STScI)
Greene, T. P. (author)
NASA Ames Research Center
Gudel, M. (author)
Eidgenössische Technische Hochschule Zürich (ETH),Swiss Federal Institute of Technology in Zürich (ETH),Universität Wien,University of Vienna
Henning, T. (author)
Max Planck Gesellschaft zur Förderung der Wissenschaften e.V. (MPG),Max Planck Society for the Advancement of Science (MPG)
Justtanont, Kay, 1965 (author)
Chalmers tekniska högskola,Chalmers University of Technology
Lagage, P. O. (author)
Centre national de la recherche scientifique (CNRS)
Meixner, M. E. (author)
Johns Hopkins University,Space Telescope Science Institute (STScI)
Norgaard-Nielsen, H. U. (author)
Danmarks Tekniske Universitet,Technical University of Denmark
Ray, T. P. (author)
Dublin Institute for Advanced Studies
Ressler, M. E. (author)
van Dishoeck, E. F. (author)
Universiteit Leiden (UL),Leiden University (UL)
Waelkens, C. (author)
Katholieke Universiteit Leuven
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 (creator_code:org_t)
IOP Publishing, 2015
2015
English.
In: Publications of the Astronomical Society of the Pacific. - : IOP Publishing. - 0004-6280 .- 1538-3873. ; 127:953, s. 584-594
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  • Journal article (peer-reviewed)
Abstract Subject headings
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  • MIRI (the Mid-Infrared Instrument for the James Webb Space Telescope [JWST]) operates from 5 to 28: 5 mu m and combines over this range: (1) unprecedented sensitivity levels; (2) subarcsecond angular resolution; (3) freedom from atmospheric interference; (4) the inherent stability of observing in space; and (5) a suite of versatile capabilities including imaging, low- and medium-resolution spectroscopy (with an integral field unit), and coronagraphy. We illustrate the potential uses of this unique combination of capabilities with various science examples: (1) imaging exoplanets; (2) transit and eclipse spectroscopy of exoplanets; (3) probing the first stages of star and planet formation, including identifying bioactive molecules; (4) determining star formation rates and mass growth as galaxies are assembled; and (5) characterizing the youngest massive galaxies.

Subject headings

NATURVETENSKAP  -- Fysik -- Astronomi, astrofysik och kosmologi (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Astronomy, Astrophysics and Cosmology (hsv//eng)

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