Metadata

• 51V-16O__VOMYT.def: "Definitions" file (text format).
• 51V-16O__VOMYT.def.json: "Definitions" file (JSON format).

Spectroscopic Model

VOMYT: partition function

VO Linelist, utilising a spectroscopic model with the 13 lowest electronic states.

• 51V-16O__VOMYT.pf [210.9 KB]
  Partition function for (51V)(16O) in the temperature range 1 – 8000 K in 1 K steps from the VOMYT data set.

References

1. McKemmish, L. K., Yurchenko, S. N., Tennyson, J., "ExoMol line lists XVIII – The high temperature spectrum of VO", Monthly Notices of the Royal Astronomical Society 463, 771-793 (2016). [link to article][16McYuTe.VO]

VOMYT: line list

VO Linelist, utilising a spectroscopic model with the 13 lowest electronic states.

Show files

References

1. McKemmish, L. K., Yurchenko, S. N., Tennyson, J., "ExoMol line lists XVIII – The high temperature spectrum of VO", Monthly Notices of the Royal Astronomical Society 463, 771-793 (2016). [link to article][16McYuTe.VO]

VOMYT: opacity

VO Linelist, utilising a spectroscopic model with the 13 lowest electronic states.

• 51V-16O__VOMYT.R1000_0.3-50mu.ktable.ARCiS.fits.gz
  ARCiS k-tables at R= 1000 (0.3-50mu) in fits format (gzipped): VOMYT (51V)(16O) line list.
• 51V-16O__VOMYT.R1000_0.3-50mu.ktable.petitRADTRANS.h5
  petitRADTRANS k-tables at R= 1000 (0.3-50mu) in HDF5 format: VOMYT (51V)(16O) line list.
• 51V-16O__VOMYT.R1000_0.3-50mu.ktable.NEMESIS.kta
  NEMESIS k-tables at R= 1000 (0.3-50mu) in NEMESIS-kta format: VOMYT (51V)(16O) line list.
• 51V-16O__VOMYT.R15000_0.3-50mu.xsec.TauREx.h5
  TauREx k-tables at R= 15000 (0.3-50mu) in HDF5 format: VOMYT (51V)(16O) line list.

References

1. McKemmish, L. K., Yurchenko, S. N., Tennyson, J., "ExoMol line lists XVIII – The high temperature spectrum of VO", Monthly Notices of the Royal Astronomical Society 463, 771-793 (2016). [link to article][16McYuTe.VO]
2. 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.]

VOMYT: broadening coefficients

VO Linelist, utilising a spectroscopic model with the 13 lowest electronic states.

Show files

References

1. Buldyreva, J., Yurchenko, S.N., Tennyson, J., "Simple semi-classical model of pressure-broadened infrared/microwave linewidths in the temperature range 200-3000 K.", RAS Techniques and Instruments 1, 43-47 (2022). [link to article]
2. Guest, E.R., Tennyson, J., Yurchenko, S.N., "Modelling the Rotational Dependence of Line Broadening using Machine Learning", Journal of Molecular Spectroscopy (2024).