The MoLLIST dataset for 56Fe1H (Q6711487)

The dataset is an archive of ExoMol page, https://exomol.com/data/molecules/FeH/56Fe-1H/MoLLIST. Please check the reference details according to the following description or directly from the website.Definitions file:56Fe-1H__MoLLIST.defRoot references for ExoMol database: 1. J. Tennyson, S.N. Yurchenko A.F. Al-Refaie, V.H.J. Clark, K.L. Chubb,E.K. Conway, A. Dewan, M.N. Gorman, C. Hill, A.E. Lynas-Gray, T. Mellor, L.K. McKemmish, A. Owens, O.L. Polyansky, M. Semenov, W. Somogyi, G. Tinetti, A. Upadhyay, I. Waldmann, Y. Wang, S. Wright and O.P. Yurchenko, 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.]MoLLIST: line list (external)Empirical Diatomic line lists MoLLIST from Bernath lab (bernath.uwaterloo.ca) in standard ExoMol format [Tennyson and Yurchenko (2016)]:FeH_README__MoLLIST.txtDocumentation for FeH external line list of the MoLLIST dataset56Fe-1H__MoLLIST.states.bz2MoLLIST (56Fe)(1H) external line list states file56Fe-1H__MoLLIST.trans.bz2MoLLIST (56Fe)(1H) external line list transition file by Dulick et al. (2003)References:1. Dulick, M., Bauschlicher, C. W,. Burrows, A., Sharp, C. M., Ram, R. S., Bernath, P. F., "Line intensities and molecular opacities of the FeH F 4Δi - X 4Δi transition", The Astrophysical Journal 594, 651-663 (2003). [http://dx.doi.org/10.1086/376791][03DuBaBu.FeH]2. Bernath, P.F., "MoLLIST: Molecular Line Lists, Intensities and Spectra", Journal of Quantitative Spectroscopy and Radiative Transfer 240, 106687 (2020). [https://doi.org/10.1016/j.jqsrt.2019.106687]MoLLIST: partition function (external)Empirical Diatomic line lists MoLLIST from Bernath lab (bernath.uwaterloo.ca) in standard ExoMol format [Tennyson and Yurchenko (2016)]:56Fe-1H__MoLLIST.pfMoLLIST (56Fe)(1H) external line list partition functionReferences:1. Bernath, P.F., "MoLLIST: Molecular Line Lists, Intensities and Spectra", Journal of Quantitative Spectroscopy and Radiative Transfer 240, 106687 (2020). [https://doi.org/10.1016/j.jqsrt.2019.106687]MoLLIST: opacityEmpirical Diatomic line lists MoLLIST from Bernath lab (bernath.uwaterloo.ca) in standard ExoMol format [Tennyson and Yurchenko (2016)]:56Fe-1H__MoLLIST.R1000_0.3-50mu.ktable.ARCiS.fits.gzARCiS k-tables at R= 1000 (0.3-50mu) in fits format (gzipped): MoLLIST (56Fe)(1H) line list.56Fe-1H__MoLLIST.R1000_0.3-50mu.ktable.petitRADTRANS.h5petitRADTRANS k-tables at R= 1000 (0.3-50mu) in HDF5 format: MoLLIST (56Fe)(1H) line list.56Fe-1H__MoLLIST.R1000_0.3-50mu.ktable.NEMESIS.ktaNEMESIS k-tables at R= 1000 (0.3-50mu) in NEMESIS-kta format: MoLLIST (56Fe)(1H) line list.56Fe-1H__MoLLIST.R15000_0.3-50mu.xsec.TauREx.h5TauREx k-tables at R= 15000 (0.3-50mu) in HDF5 format: MoLLIST (56Fe)(1H) line list.References:1. Wende, S., Reiners, A., Seifahrt, A., Bernath, P. F., "CRIRES spectroscopy and empirical line-by-line identification of FeH molecular absorption in an M dwarf", Astronomy and Astrophysics 523, A58 (2010). [http://dx.doi.org/10.1051/0004-6361/201015220][10WEReSe.FeH]2. Bernath, P.F., "MoLLIST: Molecular Line Lists, Intensities and Spectra", Journal of Quantitative Spectroscopy and Radiative Transfer 240, 106687 (2020). [https://doi.org/10.1016/j.jqsrt.2019.106687]3. 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). [http://dx.doi.org/10.1051/0004-6361/202038350][20ChRoYu.]