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HST PanCET Program: A Complete Near-UV to Infrared Transmission Spectrum for the Hot Jupiter WASP-79b

Abstract:
The ExoMol database (www.exomol.com) provides molecular data for spectroscopic studies of hot atmospheres. These data are widely used to model atmospheres of exoplanets, cool stars and other astronomical objects, as well as a variety of terrestrial applications. The 2024 data release reports the current status of the database which contains recommended line lists for 91 molecules and 224 isotopologues giving a total of almost 10$^{12}$ individual transitions. New features of the database include extensive "MARVELization" of line lists to allow them to be used for high resolutions studies, extension of several line lists to ultraviolet wavelengths, provision of photodissociation cross sections and extended provision of broadening parameters. Some of the in-house data specifications have been rewritten in JSON and moved to conformity with other international standards. Data products, including specific heats, a database of lifetimes for plasma studies, and the ExoMolHR web app which allows exclusively high resolution data to be extracted, are discussed
Publication status:
Published
Peer review status:
Peer reviewed

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Publisher copy:
10.3847/1538-3881/ac0e99

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Author
ORCID:
0000-0002-4227-4953
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Author
ORCID:
0000-0003-4816-3469
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ORCID:
0000-0003-3726-5419
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ORCID:
0000-0002-8515-7204
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Author
ORCID:
0000-0003-3204-8183


Publisher:
IOP Publishing
Journal:
The Astronomical Journal More from this journal
Volume:
162
Issue:
4
Pages:
138-138
Publication date:
2021-09-10
DOI:
EISSN:
1538-3881
ISSN:
0004-6256


Language:
English
Keywords:
Pubs id:
1173866
Local pid:
pubs:1173866
Source identifiers:
W3154623012
Deposit date:
2026-03-24
ARK identifier:
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