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dc.contributor.authorChubb, Katy L.
dc.contributor.authorRocchetto, Marco
dc.contributor.authorYurchenko, Sergei N.
dc.contributor.authorMin, Michiel
dc.contributor.authorWaldmann, Ingo
dc.contributor.authorBarstow, Joanna K.
dc.contributor.authorMolliere, Paul
dc.contributor.authorAl-Refaie, Ahmed F.
dc.contributor.authorPhillips, Mark W.
dc.contributor.authorTennyson, Jonathan
dc.date.accessioned2021-12-06T16:30:02Z
dc.date.available2021-12-06T16:30:02Z
dc.date.issued2021-02-02
dc.identifier276907280
dc.identifier96dcbfca-d57d-4996-9429-4426aa3cabde
dc.identifier000616956200001
dc.identifier85100398687
dc.identifier.citationChubb , K L , Rocchetto , M , Yurchenko , S N , Min , M , Waldmann , I , Barstow , J K , Molliere , P , Al-Refaie , A F , Phillips , M W & Tennyson , J 2021 , ' The ExoMolOP database : cross sections and k-tables for molecules of interest in high-temperature exoplanet atmospheres ' , Astronomy & Astrophysics , vol. 646 , 21 . https://doi.org/10.1051/0004-6361/202038350en
dc.identifier.issn0004-6361
dc.identifier.otherORCID: /0000-0002-4552-4559/work/104252887
dc.identifier.urihttps://hdl.handle.net/10023/24479
dc.descriptionFunding: This project has received funding from the European Union’s Horizon 2020 Research and Innovation Programme, under Grant Agreement 776403, and from the European Research Council (ERC) under the European Union’s Horizon 2020 research and innovation programme under grant agreement No 758892, ExoAI. P.M. acknowledges support from the European Research Council under the European Union’s Horizon 2020 research and innovation program under grant agreement No. 832428. J.T. and S.Y. thank the STFC Project No. ST/R000476/1.en
dc.description.abstractHere we present a publicly available database of opacities for molecules of astrophysical interest named ExoMolOP that has been compiled for over 80 species, and is based on the latest line list data from the ExoMol, HITEMP, and MoLLIST databases. These data are generally suitable for characterising high-temperature exoplanet or cool stellar and substellar atmospheres, and have been computed at a variety of pressures and temperatures, with a few molecules included at room temperature only from the HITRAN database. The data are formatted in di fferent ways for four di fferent exoplanet atmosphere retrieval codes; ARCiS, TauREx, NEMESIS, and petitRADTRANS, and include both cross sections (at R = λ/Δλ = 15 000) and k-tables (at R = λ/Δλ = 1000) for the 0.3-50 μm wavelength region. Opacity files can be downloaded and used directly for these codes. Atomic data for alkali metals Na and K are also included, using data from the NIST database and the latest line shapes for the resonance lines. Broadening parameters have been taken from the literature where available, or have been estimated from the parameters of a known molecule with similar molecular properties where no broadening data are available.
dc.format.extent19
dc.format.extent801799
dc.language.isoeng
dc.relation.ispartofAstronomy & Astrophysicsen
dc.subjectMolecular dataen
dc.subjectOpacityen
dc.subjectRadiative transferen
dc.subjectPlanets and satellites: atmospheresen
dc.subjectPlanets and satellites: gaseous planetsen
dc.subjectInfrared: planetary systemsen
dc.subjectQB Astronomyen
dc.subjectQC Physicsen
dc.subject3rd-DASen
dc.subject.lccQBen
dc.subject.lccQCen
dc.titleThe ExoMolOP database : cross sections and k-tables for molecules of interest in high-temperature exoplanet atmospheresen
dc.typeJournal articleen
dc.contributor.institutionUniversity of St Andrews. School of Physics and Astronomyen
dc.identifier.doihttps://doi.org/10.1051/0004-6361/202038350
dc.description.statusPeer revieweden
dc.identifier.urlhttps://arxiv.org/abs/2009.00687en


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