Yurchenko, SN;
Tennyson, J;
Barton, EJ;
(2017)
Molecular line shape parameters for exoplanetary atmospheric applications.
Journal of Physics: Conference Series
, 810
(1)
, Article 012010. 10.1088/1742-6596/810/1/012010.
Text
Tennyson_Yurchenko_2017_J._Phys.%253A_Conf._Ser._810_012010.pdf - Published Version Download (334kB) |
Abstract
We describe the recent updates to the ExoMol database regarding the molecular spectral line shapes. ExoMol provides comprehensive molecular line lists with a special emphasis on the applications involving characterization of hot atmospheres such as those found in exoplanets and cool stars. Among important requirements of such applications are (i) the broadening parameters for hydrogen and helium dominating atmospheres and (ii) very broad ranges of temperature and pressures. The current status of the available line shape data in the literature, demands from the exoplanetary community and their specific needs are discussed.
Type: | Article |
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Title: | Molecular line shape parameters for exoplanetary atmospheric applications |
Open access status: | An open access version is available from UCL Discovery |
DOI: | 10.1088/1742-6596/810/1/012010 |
Publisher version: | http://doi.org/10.1088/1742-6596/810/1/012010 |
Language: | English |
Additional information: | Presented at XXIII International Conference on Spectral Line Shapes - 19–24 June 2016, Torun, Poland. Content from this work may be used under the terms of the Creative Commons Attribution 3.0 licence. Any further distribution of this work must maintain attribution to the author(s) and the title of the work, journal citation and DOI. Published under licence by IOP Publishing Ltd |
UCL classification: | UCL UCL > Provost and Vice Provost Offices > UCL BEAMS UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences > Dept of Physics and Astronomy |
URI: | https://discovery.ucl.ac.uk/id/eprint/1551489 |
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