The MoLLIST dataset for 25Mg19F (Q6712246)

The dataset is an archive of ExoMol page, https://exomol.com/data/molecules/MgF/25Mg-19F/MoLLIST.Please check the reference details according to the following description or directly from the website. NB: The html description skips data which are not included in the current version for the purpose of simplicity. Please check MgF_25Mg19F_MoLLIST.md for detailed information. Definitions file 25Mg-19F__MoLLIST.def[4.37 KB] References: 1. Tennyson, J., Yurchenko, S. N., Al-Refaie, A. F., Clark, V. H. J., Chubb, K. L., Conway, E. K., Dewan, A., Gorman, M. N., Hill, C., Lynas-Gray, A. E., Mellor, T., McKemmish, L. K., Owens, A., Polyansky, O. L., Semenov, M., Somogyi, W., Tinetti, G., Upadhyay, A., Waldmann, I., Wang, Y., Wright, S., Yurchenko, O. P., "The 2020 release of the ExoMol database: molecular line lists for exoplanet and other hot atmospheres", J. Quant. Spectrosc. Rad. Transf., 255, 107228 (2020). [https://doi.org/10.1016/j.jqsrt.2020.107228] Spectroscopic Model https://exomol.com/models/MgF/25Mg-19F/MoLLIST/ MoLLIST: line list Empirical Diatomic line lists MoLLIST from Bernath lab (bernath.uwaterloo.ca) in standard ExoMol format [Tennyson and Yurchenko (2016)] 25Mg-19F__MoLLIST.trans.bz2[76.55 KB]MoLLIST (25Mg)(19F) line list: Transition file, compiled by Yixin Wang 25Mg-19F__MoLLIST.states.bz2[10.41 KB]MoLLIST (25Mg)(19F) line list: States, compiled by Yixin Wang References: 1. Hou, S., Bernath, P. F., "Line list for the MgF ground state", Journal of Quantitative Spectroscopy Radiative Transfer 203, 511-516 (2017). [https://doi.org/10.1016/j.jqsrt.2017.03.019] MoLLIST: partition function Empirical Diatomic line lists MoLLIST from Bernath lab (bernath.uwaterloo.ca) in standard ExoMol format [Tennyson and Yurchenko (2016)] 25Mg-19F__MoLLIST.pf[122.07 KB]MoLLIST (25Mg)(19F) line list: Partition function, compiled by Yixin Wang References: 1. Sauval, A. J., Tatum, J. B., "A set of partition functions and equilibrium constants for 300 diatomic molecules of astrophysical interest", Astrophysical Journal Supplement Series 56, 193-209 (1984). [http://dx.doi.org/10.1086/190980][84SaTaxx.FeH]