2016
DOI: 10.1016/j.jms.2016.05.002
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The ExoMol database: Molecular line lists for exoplanet and other hot atmospheres

Abstract: The ExoMol database (www.exomol.com) provides extensive line lists of molecular transitions which are valid over extended temperature ranges. The status of the current release of the database is reviewed and a new data structure is specified. This structure augments the provision of energy levels (and hence transition frequencies) and Einstein A coefficients with other key properties, including lifetimes of individual states, temperature-dependent cooling functions, Land? g-factors, partition functions, cross … Show more

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Cited by 419 publications
(317 citation statements)
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References 275 publications
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“…Einstein-A coefficients were calculated using the program GAIN [53] which was developed as part of TROVE [29] . Our two line lists are provided in the ExoMol [54] format are available from the ExoMol website ( www.exomol.com ); details of NH 3 specific formatting are the same as for BYTe [11] . Fig.…”
Section: Intensity Simulationsmentioning
confidence: 99%
“…Einstein-A coefficients were calculated using the program GAIN [53] which was developed as part of TROVE [29] . Our two line lists are provided in the ExoMol [54] format are available from the ExoMol website ( www.exomol.com ); details of NH 3 specific formatting are the same as for BYTe [11] . Fig.…”
Section: Intensity Simulationsmentioning
confidence: 99%
“…Shabram et al 2011, Fig. 5) could also contribute, as many studies pre-date the latest NH 3 and HCN line-lists (Tennyson et al 2016). This initial evidence has motivated retrievals to include nitrogen chemistry for other planets.…”
Section: Introductionmentioning
confidence: 99%
“…For very large lists it is recommended that these are stored separately to minimize disk usage. 106,107 For both energies and intensities, calculations start from electronic structure calculations giving an initial ab initio PES and dipole moment surfaces (DMSs). There is increasing evidence that best results require the consideration of effects, such as QED, 108 which are usually considered to be too small to be important for chemically important molecules.…”
Section: Heavier Systemsmentioning
confidence: 99%
“…Many of these species are closed shell polyatomic molecules composed of elements such H, C, O, N and S. My own ExoMol project 125 has already produced more than 20 such line lists, see the work of Tennyson et al 106 for a review of the current status. Other groups notably from Reims 55 and NASA Ames 126,127 are also computing line lists for hot species, with more experimentally driven line list being provided by Bernath and co-workers.…”
Section: Line Lists For Hot Moleculesmentioning
confidence: 99%