ExoMol molecular line lists - XXVI: spectra of SH and NS
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作者:
Yurchenko, Sergei N.
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UCL, Dept Phys & Astron, London WC1E 6BT, EnglandUCL, Dept Phys & Astron, London WC1E 6BT, England
Yurchenko, Sergei N.
[1
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Bond, Wesley
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UCL, Dept Phys & Astron, London WC1E 6BT, EnglandUCL, Dept Phys & Astron, London WC1E 6BT, England
Bond, Wesley
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Gorman, Maire N.
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UCL, Dept Phys & Astron, London WC1E 6BT, England
Aberystwyth Univ, Dept Phys, Aberystwyth SY23 3BZ, Ceredigion, WalesUCL, Dept Phys & Astron, London WC1E 6BT, England
Gorman, Maire N.
[1
,2
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Lodi, Lorenzo
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UCL, Dept Phys & Astron, London WC1E 6BT, EnglandUCL, Dept Phys & Astron, London WC1E 6BT, England
Lodi, Lorenzo
[1
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McKemmish, Laura K.
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UCL, Dept Phys & Astron, London WC1E 6BT, England
Univ New South Wales, Sch Chem, Kensington, NSW 2052, AustraliaUCL, Dept Phys & Astron, London WC1E 6BT, England
McKemmish, Laura K.
[1
,3
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Nunn, William
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UCL, Dept Phys & Astron, London WC1E 6BT, EnglandUCL, Dept Phys & Astron, London WC1E 6BT, England
Nunn, William
[1
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Shah, Rohan
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UCL, Dept Phys & Astron, London WC1E 6BT, EnglandUCL, Dept Phys & Astron, London WC1E 6BT, England
Shah, Rohan
[1
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Tennyson, Jonathan
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UCL, Dept Phys & Astron, London WC1E 6BT, EnglandUCL, Dept Phys & Astron, London WC1E 6BT, England
Tennyson, Jonathan
[1
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机构:
[1] UCL, Dept Phys & Astron, London WC1E 6BT, England
[2] Aberystwyth Univ, Dept Phys, Aberystwyth SY23 3BZ, Ceredigion, Wales
[3] Univ New South Wales, Sch Chem, Kensington, NSW 2052, Australia
Line lists for the sulphur-containing molecules SI I (the mercapto radical) and NS are computed as part of the ExoMol project. These line lists consider transitions within the X (2)Pi ground state for (SII)-S-32, (SII)-S-33, (SII)-S-34, (SII)-S-36 and, (SD)-S-32, and (NS)-N-14-S-32, (NS)-N-14-S-33, (NS)-N-14-S-34, (NS)-N-14-S-36, and (NS)-N-15-S-32. 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 (v(max) = 4, J(max) = 34.5) and calculated transitions wavenumbers; this is extrapolated such that all X (2)Pi rotational-vibrational-electronic (rovibronic) bound states are considered. For (SH)-S-32 the resulting line list contains about 81 000 transitions and 2300 rovibronic states, considering levels up to v(max) = 14 and J(max) = 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.
机构:
UCL, Dept Phys & Astron, London WC1E 6BT, England
SRON Netherlands Inst Space Res, Sorbonnelaan 2, NL-3584 CA Utrecht, NetherlandsUCL, Dept Phys & Astron, London WC1E 6BT, England
Chubb, Katy L.
Tennyson, Jonathan
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UCL, Dept Phys & Astron, London WC1E 6BT, EnglandUCL, Dept Phys & Astron, London WC1E 6BT, England
Tennyson, Jonathan
Yurchenko, Sergei N.
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机构:
UCL, Dept Phys & Astron, London WC1E 6BT, EnglandUCL, Dept Phys & Astron, London WC1E 6BT, England