Yurchenko, SN;
Bond, W;
Gorman, MN;
Lodi, L;
McKemmish, LK;
Nunn, W;
Shah, R;
(2018)
ExoMol molecular line lists – XXVI: spectra of SH and NS.
Monthly Notices of the Royal Astronomical Society
, 478
(1)
pp. 270-282.
10.1093/mnras/sty939.
Preview |
Text
Yurchenko_sty939.pdf - Published Version Download (3MB) | Preview |
Abstract
Line lists for the sulphur-containing molecules SH (the mercapto radical) and NS are computed as part of the ExoMol project. These line lists consider transitions within the X2Π ground state for 32SH, 33SH, 34SH,36SH and, 32SD, and 14N32S, 14N33S, 14N34S, 14N36S, and 15N32S. Ab initio potential energy (PEC) and spin-orbit coupling (SOC) curves are computed and then improved by fitting to experimentally observed transitions. Fully ab initio dipole moment curves (DMCs) computed at high level of theory are used to produce the final line lists. For SH, our fit gives a root-mean-square (rms) error of 0.03 cm−1 between the observed (vmax = 4, Jmax = 34.5) and calculated transitions wavenumbers; this is extrapolated such that all X2Π rotational-vibrational-electronic (rovibronic) bound states are considered. For 32SH the resulting line list contains about 81 000 transitions and 2300 rovibronic states, considering levels up to vmax = 14 and Jmax = 60.5. For NS the refinement used a combination of experimentally determined frequencies and energy levels and led to an rms-fitting error of 0.002 cm−1. Each NS-calculated line list includes around 2.8 million transitions and 31 000 rovibronic states with a vibrational range up to v = 53 and rotational range up to J = 235.5, which covers up to 23 000 cm−1. Both line lists should be complete for temperatures up to 5000 K. Example spectra simulated using this line list are shown and comparisons made to the existing data in the CDMS data base. The line lists are available from the CDS (http://cdsarc.u-strasbg.fr) and ExoMol (www.exomol.com) data bases.
| Type: | Article |
|---|---|
| Title: | ExoMol molecular line lists – XXVI: spectra of SH and NS |
| Open access status: | An open access version is available from UCL Discovery |
| DOI: | 10.1093/mnras/sty939 |
| Publisher version: | https://doi.org/10.1093/mnras/sty939 |
| Language: | English |
| Additional information: | This version is the version of record. For information on re-use, please refer to the publisher’s terms and conditions. |
| Keywords: | molecular data, opacity, astronomical data bases: miscellaneous, planets and satellites: atmospheres, stars: low-mass |
| UCL classification: | UCL UCL > Provost and Vice Provost Offices > UCL BEAMS UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences > Dept of Physics and Astronomy |
| URI: | https://discovery.ucl.ac.uk/id/eprint/10046039 |
Archive Staff Only
 |
View Item |
