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

Actions


Access Document


Files:
Publisher copy:
10.1093/mnras/stz1418

Authors


More by this author
Institution:
University of Oxford
Division:
MPLS Division
Department:
Physics
Sub department:
Atmos Ocean & Planet Physics
Role:
Author
ORCID:
0000-0002-3052-7116
More by this author
Institution:
University of Oxford
Division:
MPLS
Role:
Author
ORCID:
0000-0003-4061-2514
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
Source identifiers:
1003009
Keywords:
Pubs id:
pubs:1003009
UUID:
uuid:1e10b480-65fe-40ec-96f6-ddee7fb3783e
Local pid:
pubs:1003009
Deposit date:
2019-06-04

Terms of use


Views and Downloads






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

TO TOP