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Detectability of biosignatures in anoxic atmospheres with the James Webb Space Telescope: a TRAPPIST-1e case study

Abstract:

The James Webb Space Telescope (JWST) may be capable of finding biogenic gases in the atmospheres of habitable exoplanets around low-mass stars. Considerable attention has been given to the detectability of biogenic oxygen, which could be found using an ozone proxy, but ozone detection with JWST will be extremely challenging, even for the most favorable targets. Here, we investigate the detectability of biosignatures in anoxic atmospheres analogous to those that likely existed on the early Ea...

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Publication status:
Published
Peer review status:
Peer reviewed

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Publisher copy:
10.3847/1538-3881/aad564

Authors


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Institution:
University of Oxford
Division:
MPLS Division
Department:
Physics
Sub department:
Atmos Ocean & Planet Physics
Role:
Author
More by this author
Institution:
University of Oxford
Division:
MPLS
Department:
Physics
Sub department:
Atmos Ocean & Planet Physics
Oxford college:
St Anne's College
Role:
Author
ORCID:
0000-0002-6772-384X
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Grant:
Cross-campus Astrobiology Program
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Grant:
Virtual Planetary Laboratory (grant NNA13AA93A
Publisher:
American Astronomical Society
Journal:
Astronomical Journal More from this journal
Volume:
156
Issue:
3
Article number:
114
Publication date:
2018-08-23
Acceptance date:
2018-07-20
DOI:
EISSN:
1538-3881
ISSN:
0004-6256
Keywords:
Pubs id:
pubs:909550
UUID:
uuid:29246a9d-53dc-4518-9ec9-270e4f403ff9
Local pid:
pubs:909550
Source identifiers:
909550
Deposit date:
2018-08-23

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