The Villanueva dataset for 12C1H: partition functions

Metadata

Spectroscopic Model

12C-1H__Villanueva.model

Villanueva: line list

Villanueva's data set is the MoLLIST empirical line list converted to ExoMol by Geronimo Villanueva (NASA/GSFC)

  • 12C-1H__Villanueva.states.bz2
    MoLLIST empirical (12C)(1H) line list states file from T. Masseron et al. (2014) and converted to ExoMol by Geronimo Villanueva (NASA/GSFC) Feb/2019.
  • 12C-1H__Villanueva.trans.bz2
    MoLLIST empirical (12C)(1H) line list trans file from T. Masseron et al. (2014) and converted to ExoMol by Geronimo Villanueva (NASA/GSFC) Feb/2019.

References

  1. Masseron, T., Plez, B., Van Eck, S., Colin, R., Daoutidis, I., Godefroid, M., Coheur, P. -F., Bernath, P., Jorissen, A., Christlieb, N., "CH in stellar atmospheres: an extensive linelist", Astronomy and Astrophysics 571, A47 (2014). [link to article][14MaPlVa.CH]
  2. Bernath, P.F., "MoLLIST: Molecular Line Lists, Intensities and Spectra", Journal of Quantitative Spectroscopy and Radiative Transfer 240, 106687 (2020). [link to article]

Villanueva: partition function

Villanueva's data set is the MoLLIST empirical line list converted to ExoMol by Geronimo Villanueva (NASA/GSFC)

  • 12C-1H__Villanueva.pf
    Villanueva partition function is taken from MoLLIST, computed by population addition up to 500K and then patched with the values obtained using Sauval and Tatum, ApJSS 56, 193 (1984).

References

  1. Masseron, T., Plez, B., Van Eck, S., Colin, R., Daoutidis, I., Godefroid, M., Coheur, P. -F., Bernath, P., Jorissen, A., Christlieb, N., "CH in stellar atmospheres: an extensive linelist", Astronomy and Astrophysics 571, A47 (2014). [link to article][14MaPlVa.CH]
  2. Barklem, P. S., Collet, R., "Partition functions and equilibrium constants for diatomic molecules and atoms of astrophysical interest", Astronomy & Astrophysics 588, A96 (2016). [link to article][16BaCoxx.O2]