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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Department of Physics and Astronomy, University College London, Gower Street, London,WC1E 6BT, United KingdomDepartment of Physics and Astronomy, University College London, Gower Street, London,WC1E 6BT, United Kingdom
Yurchenko, Sergei N
Szajna, Wojciech
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Materials Spectroscopy Laboratory, Institute of Physics, University of Rzeszów, Pigonia 1 Street, Rzeszów,PL-35-310, PolandDepartment of Physics and Astronomy, University College London, Gower Street, London,WC1E 6BT, United Kingdom
Szajna, Wojciech
Hakalla, Rafal
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Materials Spectroscopy Laboratory, Institute of Physics, University of Rzeszów, Pigonia 1 Street, Rzeszów,PL-35-310, PolandDepartment of Physics and Astronomy, University College London, Gower Street, London,WC1E 6BT, United Kingdom
Hakalla, Rafal
Semenov, Mikhail
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Department of Physics and Astronomy, University College London, Gower Street, London,WC1E 6BT, United KingdomDepartment of Physics and Astronomy, University College London, Gower Street, London,WC1E 6BT, United Kingdom
Semenov, Mikhail
Sokolov, Andrei
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Department of Physics and Astronomy, University College London, Gower Street, London,WC1E 6BT, United KingdomDepartment of Physics and Astronomy, University College London, Gower Street, London,WC1E 6BT, United Kingdom
Sokolov, Andrei
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Tennyson, Jonathan
Gamache, Robert R
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Department of Physics and Astronomy, University College London, Gower Street, London,WC1E 6BT, United KingdomDepartment of Physics and Astronomy, University College London, Gower Street, London,WC1E 6BT, United Kingdom
Gamache, Robert R
Pavlenko, Yakiv
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Instituto de Astrofísica de Canarias (IAC), Calle Vía Láctea s/n, Tenerife,E-38200, Spain
Main Astronomical Observatory, Academy of Sciences of the Ukraine, 27 Zabolotnoho, Kyiv,UA-03143, UkraineDepartment of Physics and Astronomy, University College London, Gower Street, London,WC1E 6BT, United Kingdom
Pavlenko, Yakiv
Schmidt, Mirek R
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Nicolaus Copernicus Astronomical Center, Polish Academy of Sciences, Rabianska 8, Toruń,PL-87-100, PolandDepartment of Physics and Astronomy, University College London, Gower Street, London,WC1E 6BT, United Kingdom