- 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
- Files:
-
-
(pdf, 3.8mb)
-
- Publisher copy:
- 10.1093/mnras/stz1418
-
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- 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:
- Copyright holder:
- Lee et al.
- Copyright date:
- 2019
- Notes:
- © 2019 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society.
Journal article
Exoplanetary Monte Carlo radiative transfer with correlated-k I. Benchmarking transit and emission observables
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