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First Detection of Hydroxyl Radical Emission from an Exoplanet Atmosphere: High-dispersion Characterization of WASP-33b Using Subaru/IRD

Abstract:

The chemical characterisation of exoplanet atmospheres plays a crucial role in profoundly enriching our comprehension of exoplanets. By deciphering the array of molecular species shaping the chemical composition of a given exoplanet atmosphere, we unlock invaluable insights into its chemical evolution, climate, physical dynamics, and even its potential for harbouring life. High-resolution molecular spectroscopy provides the fundamental data needed for robustly identifying molecules in exopla...

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Publication status:
Published
Peer review status:
Peer reviewed

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Publisher copy:
10.3847/2041-8213/abec71

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Role:
Author
ORCID:
0000-0003-4698-6285
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Role:
Author
ORCID:
0000-0003-3309-9134
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Role:
Author
ORCID:
0000-0002-9308-2353
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Role:
Author
ORCID:
0000-0001-6391-9266
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Role:
Author
ORCID:
0000-0003-3618-7535


Publisher:
American Astronomical Society
Journal:
The Astrophysical Journal Letters More from this journal
Volume:
910
Issue:
1
Pages:
L9-L9
Publication date:
2021-03-23
DOI:
EISSN:
2041-8213
ISSN:
2041-8205


Language:
English
Keywords:
Pubs id:
1171448
Local pid:
pubs:1171448
Source identifiers:
W3133886174
Deposit date:
2026-02-16
ARK identifier:
This ORA record was generated from metadata provided by an external service. It has not been edited by the ORA Team.

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