Monthly Notices of the Royal Astronomical Society · 2011 · 364 citations · 28 references
Natural SciencesAstronomyChemistryComputational ChemistryMolecular PhysicsSpectroscopyAb Initio MethodsAstrochemical ModelingMolecular Energy LevelsBrown DwarfsGround State PropertiesLine List ConstructionPotential Energy Surface AnalysisRo-vibrational InteractionsRotational-vibrational TransitionsTemperature Effects On Spectra
We present ‘BYTe’, a comprehensive ‘hot’ line list for the ro-vibrational transitions of ammonia, 14NH3, in its ground electronic state. This line list has been computed variationally using the program suite trove, a new spectroscopically determined potential energy surface and an ab initio dipole moment surface. BYTe, is designed to be used at all temperatures up to 1500 K. It comprises 1138 323 351 transitions in the frequency range from 0 to 12 000 cm−1, constructed from 1373 897 energy levels below 18 000 cm−1 having J values ≤36. Comparisons with laboratory data confirm the accuracy of the line list which is suitable for modelling a variety of astrophysical problems including the atmospheres of extrasolar planets and brown dwarfs.
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A Nongray Theory of Extrasolar Giant Planets and Brown Dwarfs
Adam Burrows, Mark S. Marley, W. B. Hubbard et al. · The Astrophysical Journal · 1997 · 1.4K citations · Full text
Natural Sciences, Astronomy, Physics +14
A high-accuracy computed water line list
R. J. Barber, Jonathan Tennyson, G. J. Harris et al. · Monthly Notices of the Royal Astronomical Society · 2006 · 712 citations · Full text
The presence of methane in the atmosphere of an extrasolar planet
Gautam Vasisht, G. Tinetti · Nature · 2008 · 600 citations
Water vapour in the atmosphere of a transiting extrasolar planet
G. Tinetti, A. Vidal‐Madjar, Mao‐Chang Liang et al. · Nature · 2007 · 550 citations · Full text