The YT34to10 dataset for 12C1H4

The dataset is an archive of ExoMol page, https://exomol.com/data/molecules/CH4/12C-1H4/YT34to10.<br>Please check the reference details according to the following description or directly from the website.<br> <strong>NB: The html description skips data which are not included in the current version for the purpose of simplicity. Please check CH4_12C1H4_YT34to10.md for detailed information.</strong> <br> <strong>Definitions file</strong> <strong>12C-1H4__YT34to10.def</strong>[21.85 KB]<br> <strong>References:</strong><br> 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] <strong>Spectroscopic Model</strong> https://exomol.com/models/CH4/12C-1H4/YT34to10/<br> <strong>YT34to10: line list</strong> <strong>NB: These data are not included in the current version on Zenodo because the data are over Zenodo upload cap, 50GB</strong><br> <strong>Data can be accessed via:</strong> https://exomol.com/data/molecules/CH4/12C-1H4/YT34to10<br> <strong>References:</strong><br> 1. Yurchenko, S. N., Tennyson, J., "ExoMol line lists IV: The rotation-vibration spectrum of methane up to 1500 K", Monthly Notices of the Royal Astronomical Society 440, 1649-1661 (2014). [http://http://dx.doi.org/10.1093/mnras/stu326][14YuTexx.CH4]<br> 2. Yurchenko, S. N., Amundsen, D. S., Tennyson, J., Waldmann, I. P., "A hybrid line list for CH4 and hot methane continuum", Astronomy and Astrophysics 605, A95/1-9 (2017). [https://doi.org/10.1051/0004-6361/201731026][17YuAmTe.CH4]<br> <strong>YT34to10: partition function</strong> <em>Calculated line list and energy levels for (12C)(1H)4</em><br> <strong>12C-1H4__YT34to10.pf</strong>[25.39 KB]<br>Partition function of (12C)(1H)4 in 3 K intervals to 2000 K <strong>References:</strong><br> 1. Yurchenko, S. N., Tennyson, J., "ExoMol line lists IV: The rotation-vibration spectrum of methane up to 1500 K", Monthly Notices of the Royal Astronomical Society 440, 1649-1661 (2014). [http://http://dx.doi.org/10.1093/mnras/stu326][14YuTexx.CH4]<br> 2. Yurchenko, S. N., Amundsen, D. S., Tennyson, J., Waldmann, I. P., "A hybrid line list for CH4 and hot methane continuum", Astronomy and Astrophysics 605, A95/1-9 (2017). [https://doi.org/10.1051/0004-6361/201731026][17YuAmTe.CH4]<br> <strong>YT34to10: opacity</strong> <em>Calculated line list and energy levels for (12C)(1H)4</em><br> <strong>12C-1H4__YT34to10.R1000_0.3-50mu.ktable.ARCiS.fits.gz</strong>[353.53 MB]<br>ARCiS k-tables at R= 1000 (0.3-50mu) in fits format (gzipped): YT34to10 (12C)(1H)4 line list. <strong>12C-1H4__YT34to10.R1000_0.3-50mu.ktable.petitRADTRANS.h5</strong>[370.98 MB]<br>petitRADTRANS k-tables at R= 1000 (0.3-50mu) in HDF5 format: YT34to10 (12C)(1H)4 line list. <strong>12C-1H4__YT34to10.R1000_0.3-50mu.ktable.NEMESIS.kta</strong>[232.01 MB]<br>NEMESIS k-tables at R= 1000 (0.3-50mu) in NEMESIS-kta format: YT34to10 (12C)(1H)4 line list. <strong>12C-1H4__YT34to10.R15000_0.3-50mu.xsec.TauREx.h5</strong>[348.39 MB]<br>TauREx k-tables at R= 15000 (0.3-50mu) in HDF5 format: YT34to10 (12C)(1H)4 line list. <strong>References:</strong><br> 1. Yurchenko, S. N., Amundsen, D. S., Tennyson, J., Waldmann, I. P., "A hybrid line list for CH4 and hot methane continuum", Astronomy and Astrophysics 605, A95/1-9 (2017). [https://doi.org/10.1051/0004-6361/201731026][17YuAmTe.CH4]<br> 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). [http://dx.doi.org/10.1051/0004-6361/202038350][20ChRoYu.]<br>