Metadata

• 89Y-16O__SSYT.def: "Definitions" file (text format).
• 89Y-16O__SSYT.def.json: "Definitions" file (JSON format).

Spectroscopic Model

SSYT: line list

SSYT line list for (89Y)(16O) obtained using ab initio model with Duo

• 89Y-16O__SSYT.states.bz2
  States of the SSYT (89Y)(16O) rovibronic ab initio line list for the six lowest electronic states.
• 89Y-16O__SSYT.trans.bz2
  Transitions of the SSYT (89Y)(16O) rovibronic ab initio line list for the six lowest electronic states.

References

1. Smirnov, A. N, Solomonik, V. G., Yurchenko, S. N., Tennyson, J., "Spectroscopy of YO from first principles", Physical Chemistry Chemical Physics 21, 22794-22810 (2019). [link to article][19SmSoYu.YO]

SSYT: partition function

SSYT line list for (89Y)(16O) obtained using ab initio model with Duo

• 89Y-16O__SSYT.pf
  Partition funciton of the SSYT (89Y)(16O) rovibronic ab initio line list for the six lowest electronic states.

References

1. Smirnov, A. N, Solomonik, V. G., Yurchenko, S. N., Tennyson, J., "Spectroscopy of YO from first principles", Physical Chemistry Chemical Physics 21, 22794-22810 (2019). [link to article][19SmSoYu.YO]

SSYT: opacity

SSYT line list for (89Y)(16O) obtained using ab initio model with Duo

• 89Y-16O__SSYT.R1000_0.3-50mu.ktable.NEMESIS.kta
  NEMESIS k-tables at R= 1000 (0.3-50mu) in NEMESIS-kta format: SSYT (89Y)(16O) line list.
• 89Y-16O__SSYT.R15000_0.3-50mu.xsec.TauREx.h5
  TauREx cross sections at R= 15000 (0.3-50mu) in HDF5 format: SSYT (89Y)(16O) line list.
• 89Y-16O__SSYT.R1000_0.3-50mu.ktable.ARCiS.fits.gz
  ARCiS k-tables at R= 1000 (0.3-50mu) in fits format (gzipped): SSYT (89Y)(16O) line list.
• 89Y-16O__SSYT.R1000_0.3-50mu.ktable.petitRADTRANS.h5
  petitRADTRANS k-tables at R= 1000 (0.3-50mu) in HDF5 format: SSYT (89Y)(16O) line list.

References

1. Chubb, K. L., Rocchetto, M., Yurchenko, S. N., Min, M., Waldmann, I., Barstow, J. K., Molliere, P., Al-Refaie, A. F, Phillips, M. W., Tennyson, J., "The ExoMolOP database: Cross sections and k-tables for molecules of interest in high-temperature exoplanet atmospheres", Astronomy and Astrophysics 646, A21 (2020). [link to article][20ChRoYu.]
2. Smirnov, A. N, Solomonik, V. G., Yurchenko, S. N., Tennyson, J., "Spectroscopy of YO from first principles", Physical Chemistry Chemical Physics 21, 22794-22810 (2019). [link to article][19SmSoYu.YO]

SSYT: Specific heat - heat capacity

SSYT line list for (89Y)(16O) obtained using ab initio model with Duo

• 89Y-16O__SSYT.cp
  Heat capacity (specific heat) Cp of (89Y)(16O) in 200 K intervals to 5000 K

References

1. Smirnov, A. N, Solomonik, V. G., Yurchenko, S. N., Tennyson, J., "Spectroscopy of YO from first principles", Physical Chemistry Chemical Physics 21, 22794-22810 (2019). [link to article][19SmSoYu.YO]