Journal article icon

Journal article

Exoplanetary Monte Carlo radiative transfer with correlated-k I. Benchmarking transit and emission observables

Abstract:

Current observational data of exoplanets are providing increasing detail of their 3D atmospheric structures. As characterisation efforts expand in scope, the need to develop consistent 3D radiative-transfer methods becomes more pertinent as the complex atmospheric properties of exoplanets are required to be modelled together consistently. We aim to compare the transmission and emission spectra results of a 3D Monte Carlo Radiative Transfer (MCRT) model to contemporary radiative-transfer suite...

Expand abstract
Publication status:
Published
Peer review status:
Peer reviewed
Version:
Publisher's version

Actions


Access Document


Files:
Publisher copy:
10.1093/mnras/stz1418

Authors


More by this author
Institution:
University of Oxford
Division:
MPLS Division
Department:
Physics
Subgroup:
Atmos Ocean & Planet Physics
ORCID:
0000-0002-3052-7116
More by this author
Institution:
University of Oxford
Division:
MPLS Division
Department:
Physics
Subgroup:
Atmos Ocean & Planet Physics
ORCID:
0000-0003-4061-2514
Garland, R More by this author
Expand authors...
Publisher:
Oxford University Press Publisher's website
Journal:
Monthly Notices of the Royal Astronomical Society Journal website
Volume:
487
Issue:
2
Pages:
2082-2096
Publication date:
2019-05-23
Acceptance date:
2019-05-13
DOI:
ISSN:
0035-8711
Pubs id:
pubs:1003009
URN:
uri:1e10b480-65fe-40ec-96f6-ddee7fb3783e
UUID:
uuid:1e10b480-65fe-40ec-96f6-ddee7fb3783e
Local pid:
pubs:1003009
Keywords:

Terms of use


Metrics



If you are the owner of this record, you can report an update to it here: Report update to this record

TO TOP