ExoMol line lists – IV. The rotation–vibration spectrum of methane up to 1500 K
about
Using experimental data and a contracted basis Lanczos method to determine an accurate methane potential energy surface from a least squares optimization.Spectrum of hot methane in astronomical objects using a comprehensive computed line list.Ab initio variational predictions for understanding highly congested spectra: rovibrational assignment of 108 new methane sub-bands in the icosad range (6280-7800 cm(-1)).Perspective: Accurate ro-vibrational calculations on small molecules.A global potential energy surface and dipole moment surface for silane.An efficient method for energy levels calculation using full symmetry and exact kinetic energy operator: tetrahedral molecules.A highly accurate ab initio potential energy surface for methane.Study of the electronic and rovibronic structure of the X ²Σ⁺, A ²Π, and B ²Σ⁺ states of AlO.Automatic differentiation method for numerical construction of the rotational-vibrational Hamiltonian as a power series in the curvilinear internal coordinates using the Eckart frame.Accurate ab initio dipole moment surfaces of ozone: First principle intensity predictions for rotationally resolved spectra in a large range of overtone and combination bands.A hybrid variational-perturbation calculation of the ro-vibrational spectrum of nitric acidExoMol line lists – VII. The rotation–vibration spectrum of phosphine up to 1500 KExoMol line lists – VIII. A variationally computed line list for hot formaldehydeExoMol line lists – XXII. The rotation-vibration spectrum of silane up to 1200 KFirst light of the VLT planet finder SPHEREExplicitly correlated MRCI-F12 potential energy surfaces for methane fit with several permutation invariant schemes and full-dimensional vibrational calculationsCFBDSIR 2149-0403: young isolated planetary-mass object or high-metallicity low-mass brown dwarf?A library of ATMO forward model transmission spectra for hot Jupiter exoplanetsTransmission spectral properties of clouds for hot Jupiter exoplanetsTreatment of overlapping gaseous absorption with the correlated-kmethod in hot Jupiter and brown dwarf atmosphere modelsThe UK Met Office global circulation model with a sophisticated radiation scheme applied to the hot Jupiter HD 209458b
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ExoMol line lists – IV. The rotation–vibration spectrum of methane up to 1500 K
description
article
@en
im März 2014 veröffentlichter wissenschaftlicher Artikel
@de
wetenschappelijk artikel
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наукова стаття, опублікована в березні 2014
@uk
name
ExoMol line lists – IV. The rotation–vibration spectrum of methane up to 1500 K
@en
ExoMol line lists – IV. The rotation–vibration spectrum of methane up to 1500 K
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type
label
ExoMol line lists – IV. The rotation–vibration spectrum of methane up to 1500 K
@en
ExoMol line lists – IV. The rotation–vibration spectrum of methane up to 1500 K
@nl
prefLabel
ExoMol line lists – IV. The rotation–vibration spectrum of methane up to 1500 K
@en
ExoMol line lists – IV. The rotation–vibration spectrum of methane up to 1500 K
@nl
P2860
P356
P1476
ExoMol line lists – IV. The rotation–vibration spectrum of methane up to 1500 K
@en
P2860
P304
P356
10.1093/MNRAS/STU326
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2014-03-01T00:00:00Z
P818
P819
2014MNRAS.440.1649Y