4.7 Article

ExoMol molecular line lists XXX: a complete high-accuracy line list for water

Journal

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
Volume 480, Issue 2, Pages 2597-2608

Publisher

OXFORD UNIV PRESS
DOI: 10.1093/mnras/sty1877

Keywords

molecular data; opacity; planets and satellites: atmospheres; stars: atmospheres; stars: low-mass; stars: brown dwarfs. astronomical data bases: miscellaneous

Funding

  1. ERC [267219]
  2. UK Natural Environment Research Council
  3. Russian Fund for Fundamental Studies [18-02-0057]
  4. STFC [ST/R000476/1, ST/M001334/1, ST/J001511/1] Funding Source: UKRI
  5. Natural Environment Research Council [NER/A/S/2003/00480] Funding Source: researchfish
  6. Science and Technology Facilities Council [ST/J001511/1, ST/R000476/1, ST/M001334/1] Funding Source: researchfish

Ask authors/readers for more resources

A new line list for (H2O)-O-1-O-6 is presented. This line list, which is called POKAZATEL, includes transitions between rotational-vibrational energy levels up to 41 000 cm(-1) and is the most complete to date. The potential energy surface (PES) used for producing the line list was obtained by fitting a high-quality ab initio PES to experimental energy levels with energies of 41 000 cm(-1) and for rotational excitations up to J = 5. The final line list comprises all energy levels up to 41 000 cm(-1) and rotational angular momentum J up to 72. An accurate ab initio dipole moment surface was used for the calculation of line intensities and reproduces high-precision experimental intensity data with an accuracy close to 1 percent. The final line list uses empirical energy levels, whenever they are available, to ensure that line positions are reproduced as accurately as possible. The POKAZATEL line list contains over 5 billion transitions and is available from the ExoMol website (www.exomol.com ) and the CDS data base.

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