dc.contributor.author | Goyal, J | |
dc.contributor.author | Mayne, N | |
dc.contributor.author | Sing, D | |
dc.contributor.author | Drummond, B | |
dc.contributor.author | Tremblin, PLR | |
dc.contributor.author | Amundsen, DS | |
dc.contributor.author | Evans, T | |
dc.contributor.author | Carter, A | |
dc.contributor.author | Spake, J | |
dc.contributor.author | Baraffe, I | |
dc.contributor.author | Nikolov, NK | |
dc.contributor.author | MANNERS, J | |
dc.contributor.author | Chabrier, G | |
dc.contributor.author | Hébrard, ECF | |
dc.date.accessioned | 2019-06-11T09:32:46Z | |
dc.date.issued | 2019-03-14 | |
dc.description.abstract | The paper ‘A library of ATMO forward model transmission spectra for hot Jupiter exoplanets’ was published in MNRAS 474, 4, 5158–5185.
In the original manuscript (Goyal et al. 2018), we presented a grid of forward model transmission spectra for hot Jupiter exoplanets. However, we recently identified an error in the treatment of rainout in our 1D atmosphere model ATMO. The correction of this error led to changes in the equilibrium chemical abundances using rainout condensation and thereby the transmission spectra. We note that this error only affects the online library2,3 that includes rainout condensation, the library with local condensation (without rainout) is unaffected. We further note that the gas phase equilibrium scheme used in ATMO has been compared by Drummond et al. (2016) with the analytical schemes of Burrows & Sharp (1999) and Heng & Tsai (2016). The gas phase chemistry with and without local condensation has also been verified in Baudino et al. (2017) against the petitCODE (Mollière et al. 2015, 2017) and Exo-REM (Baudino et al. 2015) models. Therefore, issues with the previous version of the grid were confined to the implementation of rainout. | en_GB |
dc.identifier.citation | Vol. 486 (1), pp. 783 - 795 | en_GB |
dc.identifier.doi | 10.1093/mnras/stz755 | |
dc.identifier.uri | http://hdl.handle.net/10871/37453 | |
dc.language.iso | en | en_GB |
dc.publisher | Oxford University Press (OUP) / Royal Astronomical Society | en_GB |
dc.relation.url | http://hdl.handle.net/10871/30324 | en_GB |
dc.rights | © 2019 The Author(s).
Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved | en_GB |
dc.subject | errata | en_GB |
dc.subject | addenda | en_GB |
dc.subject | techniques: spectroscopic | en_GB |
dc.subject | planets and satellites: atmospheres | en_GB |
dc.subject | planets and satellites: composition | en_GB |
dc.subject | planets and satellites: gaseous planets | en_GB |
dc.title | Erratum: A library of ATMO forward model transmission spectra for hot Jupiter exoplanets | en_GB |
dc.type | Article | en_GB |
dc.date.available | 2019-06-11T09:32:46Z | |
dc.description | This is the final version. Available from OUP via the DOI in this record | en_GB |
dc.description | The article to which this is the erratum is in ORE at http://hdl.handle.net/10871/30324 | en_GB |
dc.identifier.eissn | 1365-2966 | |
dc.identifier.journal | Monthly Notices of the Royal Astronomical Society | en_GB |
dc.rights.uri | http://www.rioxx.net/licenses/all-rights-reserved | en_GB |
dcterms.dateAccepted | 2019-03-04 | |
rioxxterms.version | VoR | en_GB |
rioxxterms.licenseref.startdate | 2019-03-14 | |
rioxxterms.type | Journal Article/Review | en_GB |
refterms.dateFCD | 2019-06-10T16:54:45Z | |
refterms.versionFCD | AM | |
refterms.dateFOA | 2019-06-11T09:32:55Z | |
refterms.panel | B | en_GB |