ExoMol line lists for SO2 Virtual Observatory Resource

Authors
  1. Underwood D.S.
  2. Tennyson J.
  3. Yurchenko S.N.
  4. Huang X.
  5. Schwenke D.W.,Lee T.J.
  6. Clausen S.
  7. Fateev A.
  8. Published by
    CDS
Abstract

Sulphur dioxide is well-known in the atmospheres of planets and satellites, where its presence is often associated with volcanism, and in circumstellar envelopes of young and evolved stars as well as the interstellar medium. This work presents a line list of 1.3 billion 32S16O2 vibration-rotation transitions computed using an empirically-adjusted potential energy surface and an ab initio dipole moment surface. The list gives complete coverage up to 8000cm^-1^ (wavelengths longer than 1.25um) for temperatures below 2000K. Infrared absorption cross sections are recorded at 300 and 500C are used to validated the resulting ExoAmes line list. The line list is made available in electronic form as supplementary data to this article and at www.exomol.com.

Keywords
  1. Atomic physics
Bibliographic source Bibcode
2016MNRAS.459.3890U
See also HTML
https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/459/3890
IVOA Identifier IVOID
ivo://CDS.VizieR/J/MNRAS/459/3890

Access

Web browser access HTML
http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/MNRAS/459/3890
https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/459/3890
http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/459/3890
IVOA Table Access TAP
http://tapvizier.cds.unistra.fr/TAPVizieR/tap
Run SQL-like queries with TAP-enabled clients (e.g., TOPCAT).

History

2016-10-21T10:04:44Z
Resource record created
2016-10-21T09:06:07Z
Updated
2016-10-21T10:04:44Z
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