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dc.contributor.authorGoyal, J
dc.contributor.authorMayne, N
dc.contributor.authorSing, D
dc.contributor.authorDrummond, B
dc.contributor.authorTremblin, PLR
dc.contributor.authorAmundsen, DS
dc.contributor.authorEvans, T
dc.contributor.authorCarter, A
dc.contributor.authorSpake, J
dc.contributor.authorBaraffe, I
dc.contributor.authorNikolov, NK
dc.contributor.authorMANNERS, J
dc.contributor.authorChabrier, G
dc.contributor.authorHébrard, ECF
dc.date.accessioned2019-06-11T09:32:46Z
dc.date.issued2019-03-14
dc.description.abstractThe 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.citationVol. 486 (1), pp. 783 - 795en_GB
dc.identifier.doi10.1093/mnras/stz755
dc.identifier.urihttp://hdl.handle.net/10871/37453
dc.language.isoenen_GB
dc.publisherOxford University Press (OUP) / Royal Astronomical Societyen_GB
dc.relation.urlhttp://hdl.handle.net/10871/30324en_GB
dc.rights© 2019 The Author(s). Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserveden_GB
dc.subjecterrataen_GB
dc.subjectaddendaen_GB
dc.subjecttechniques: spectroscopicen_GB
dc.subjectplanets and satellites: atmospheresen_GB
dc.subjectplanets and satellites: compositionen_GB
dc.subjectplanets and satellites: gaseous planetsen_GB
dc.titleErratum: A library of ATMO forward model transmission spectra for hot Jupiter exoplanetsen_GB
dc.typeArticleen_GB
dc.date.available2019-06-11T09:32:46Z
dc.descriptionThis is the final version. Available from OUP via the DOI in this recorden_GB
dc.descriptionThe article to which this is the erratum is in ORE at http://hdl.handle.net/10871/30324en_GB
dc.identifier.eissn1365-2966
dc.identifier.journalMonthly Notices of the Royal Astronomical Societyen_GB
dc.rights.urihttp://www.rioxx.net/licenses/all-rights-reserveden_GB
dcterms.dateAccepted2019-03-04
rioxxterms.versionVoRen_GB
rioxxterms.licenseref.startdate2019-03-14
rioxxterms.typeJournal Article/Reviewen_GB
refterms.dateFCD2019-06-10T16:54:45Z
refterms.versionFCDAM
refterms.dateFOA2019-06-11T09:32:55Z
refterms.panelBen_GB


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