The 2020 release of the ExoMol database: Molecular line lists for exoplanet and other hot atmospheres

Jonathan Tennyson, Sergey Yurchenko, Ahmed Al-Refaie, Victoria Clark, Katie L. Chubb, Eamon Conway, Akhil Dewan, Maire Gorman, Christian Hill, Anthony Lynas-gray, Thomas Mellor, Laura K. McKemmish, Alec Owens, Oleg L. Polyansky, Mikhail Semenov, Wilfrid Somogyi, Giovanna Tinetti, Apoorva Upadhyay, Ingo Waldmann, Yixin WangSamuel Wright, Olga Yurchenko

Allbwn ymchwil: Cyfraniad at gyfnodolynErthygladolygiad gan gymheiriaid

135 Dyfyniadau(SciVal)
151 Wedi eu Llwytho i Lawr (Pure)

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The ExoMol database (www.exomol.com) provides molecular data for spectroscopic studies of hot atmospheres. While the data are intended for studies of exoplanets and other astronomical bodies, the dataset is widely applicable. The basic form of the database is extensive line lists; these are supplemented with partition functions, state lifetimes, cooling functions, Landé g-factors, temperature-dependent cross sections, opacities, pressure broadening parameters, k-coefficients and dipoles. This paper presents the latest release of the database which has been expanded to consider 80 molecules and 190 isotopologues totaling over 700 billion transitions. While the spectroscopic data are concentrated at infrared and visible wavelengths, ultraviolet transitions are being increasingly considered in response to requests from observers. The core of the database comes from the ExoMol project which primarily uses theoretical methods, albeit usually fine-tuned to reproduce laboratory spectra, to generate very extensive line lists for studies of hot bodies. The data have recently been supplemented by line lists derived from direct laboratory observations, albeit usually with the use of ab initiotransition intensities. A major push in the new release is towards accurate characterisation of transition frequencies for use in high resolution studies of exoplanets and other bodies.

Iaith wreiddiolSaesneg
Rhif yr erthygl107228
CyfnodolynJournal of Quantitative Spectroscopy and Radiative Transfer
Cyfrol255
Dyddiad ar-lein cynnar03 Medi 2020
Dynodwyr Gwrthrych Digidol (DOIs)
StatwsCyhoeddwyd - 01 Tach 2020

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