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Atmospheric Characterization of Directly Imaged Exoplanets with JWST/MIRI

Abstract:

The Mid-Infrared instrument (MIRI) on board the James Webb Space Telescope will perform the first ever characterization of young giant exoplanets observed by direct imaging in the 5–28 μm spectral range. This wavelength range is key for both determining the bolometric luminosity of the cool known exoplanets and for accessing the strongest ammonia bands. In conjunction with shorter wavelength observations, MIRI will enable a more accurate characterization of the exoplanetary atmospheric proper...

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Publication status:
Published
Peer review status:
Peer reviewed
Version:
Publisher's Version

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Publisher copy:
10.3847/1538-3881/aae651

Authors


Danielski, C More by this author
More by this author
Institution:
University of Oxford
Division:
MPLS Division
Department:
Physics
Subgroup:
Atmos Ocean & Planet Physics
ORCID:
0000-0003-4061-2514
Lagage, P-O More by this author
Boccaletti, A More by this author
Gastaud, R More by this author
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Publisher:
American Astronomical Society Publisher's website
Journal:
Astronomical Journal Journal website
Volume:
156
Issue:
6
Pages:
Article: 276
Publication date:
2018-11-21
Acceptance date:
2018-09-28
DOI:
EISSN:
1538-3881
ISSN:
0004-6256
Pubs id:
pubs:923305
URN:
uri:5bcb77a4-0cea-428a-ab02-0f8c111a55f2
UUID:
uuid:5bcb77a4-0cea-428a-ab02-0f8c111a55f2
Local pid:
pubs:923305

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