ExoMol line list for H_2_^18^O and H_2_^17^O Virtual Observatory Resource

Authors
  1. Polyansky O.L.
  2. Kyuberis A.A.
  3. Lodi L.
  4. Tennyson J.
  5. Yurchenko S.N.,Ovsyannikov R.I.
  6. Zobov N.F.
  7. Published by
    CDS
Abstract

Hot line lists for two isotopologues of water, H_2_^18^O and H_2_^17^O, are presented. The calculations employ newly constructed potential energy surfaces (PES), which take advantage of a novel method for using the large set of experimental energy levels for H_2_^16^O to give high-quality predictions for H_2_^18^O and H_2_^17^O. This procedure greatly extends the energy range for which a PES can be accurately determined, allowing an accurate prediction of higher lying energy levels than are currently known from direct laboratory measurements. This PES is combined with a high-accuracy, ab initio dipole moment surface of water in the computation of all energy levels, transition frequencies and associated Einstein A coefficients for states with rotational excitation up to J=50 and energies up to 30000cm^-1^. The resulting HotWat78 line lists complement the well-used BT2 H_2_^16^O line list.

Keywords
  1. Atomic physics
Bibliographic source Bibcode
2017MNRAS.466.1363P
See also HTML
https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/466/1363
IVOA Identifier IVOID
ivo://CDS.VizieR/J/MNRAS/466/1363

Access

Web browser access HTML
http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/MNRAS/466/1363
https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/466/1363
http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/466/1363
IVOA Table Access TAP
http://tapvizier.cds.unistra.fr/TAPVizieR/tap
Run SQL-like queries with TAP-enabled clients (e.g., TOPCAT).

History

2017-01-26T08:23:32Z
Resource record created
2017-01-26T07:24:54Z
Updated
2017-01-26T08:23:32Z
Created

Contact

Name
CDS support team
Postal Address
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
E-Mail
cds-question@unistra.fr