Empirical line lists BRYTS for the open shell molecule (YO)-Y-89-O-16 (yttrium oxide) and its isotopologues are presented. The line lists cover the six lowest electronic states: X-2 Sigma+, A(2)Pi, A '(2)Delta, B-2 Sigma+, C-2 Pi, and D-2 Sigma+ up to 60 000 cm(-1) (<0.167 mu m) for rotational excitation up to J = 400.5. An ab initio spectroscopic model consisting of potential energy curves (PECs), spin-orbit, and electronic angular momentum couplings is refined by fitting to experimentally determined energies of YO, derived from published YO experimental transition frequency data. The model is complemented by empirical spin-rotation and Lambda-doubling curves and ab initio dipole moment and transition dipole moment curves computed using multireference configuration interaction (MRCI). The ab initio PECs computed using the complete basis set limit extrapolation and the coupled-cluster CCSD(T) method with its higher quality provide an excellent initial approximation for the refinement. Non-adiabatic coupling curves for two pairs of states of the same symmetry A/C and B/D are computed using a state-averaged complete active space self-consistant field theory (CASSCF) and used to build diabatic representations for the A(2)Pi, C-2 Pi, B-2 Sigma+, and D-2 Sigma(+) curves. The experimentally derived energies of (YO)-Y-89-O-16 utilized in the fit are used to replace the corresponding calculated energy values in the BRYTS line list. Simulated spectra of YO show excellent agreement with the experiment, where it is available. Calculated lifetimes of YO are tuned to agree well with the experiment, where available.
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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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UCL, Dept Phys & Astron, London WC1E 6BT, EnglandUCL, Dept Phys & Astron, London WC1E 6BT, England
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Univ New South Wales, Sch Chem, Sydney, NSW 2052, Australia
UCL, Dept Phys & Astron, Gower St, London WC1E 6BT, EnglandUniv New South Wales, Sch Chem, Sydney, NSW 2052, Australia
McKemmish, Laura K.
Masseron, Thomas
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Inst Astrofis Canarias, E-38205 Tenerife, Spain
Univ La Laguna, Dept Astrofis, E-38206 Tenerife, SpainUniv New South Wales, Sch Chem, Sydney, NSW 2052, Australia
Masseron, Thomas
Jens Hoeijmakers, H.
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Univ Bern, Ctr Space & Habitabil, Gesell Str 6, CH-3012 Bern, Switzerland
Univ Geneva, Geneva Observ, Chemin Maillettes 51, CH-1290 Versoix, SwitzerlandUniv New South Wales, Sch Chem, Sydney, NSW 2052, Australia
Jens Hoeijmakers, H.
Perez-Mesa, Victor
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Inst Astrofis Canarias, E-38205 Tenerife, Spain
Univ La Laguna, Dept Astrofis, E-38206 Tenerife, SpainUniv New South Wales, Sch Chem, Sydney, NSW 2052, Australia
Perez-Mesa, Victor
Grimm, Simon L.
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Univ Bern, Ctr Space & Habitabil, Gesell Str 6, CH-3012 Bern, SwitzerlandUniv New South Wales, Sch Chem, Sydney, NSW 2052, Australia
Grimm, Simon L.
Yurchenko, Sergei N.
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UCL, Dept Phys & Astron, Gower St, London WC1E 6BT, EnglandUniv New South Wales, Sch Chem, Sydney, NSW 2052, Australia
Yurchenko, Sergei N.
Tennyson, Jonathan
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UCL, Dept Phys & Astron, Gower St, London WC1E 6BT, EnglandUniv New South Wales, Sch Chem, Sydney, NSW 2052, Australia