The AYT2 dataset for 1H232S

The dataset is an archive of ExoMol page, https://exomol.com/data/molecules/H2S/1H2-32S/AYT2.<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 H2S_1H232S_AYT2.md for detailed information.</strong> <br> <strong>Definitions file</strong> <strong>1H2-32S__AYT2.def</strong>[8.09 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/H2S/1H2-32S/AYT2/<br> <strong>AYT2: line list</strong> <em>Ro-vibrational line list for H2S</em><br> <strong>H2S__AYT2.readme</strong>[4.0 KB]<br>Documentation for the AYT2 line list for H2S <strong>1H2-32S__AYT2.states.bz2</strong>[2.17 MB]<br>Labelled ro-vibrational states of H2S <strong>1H2-32S__AYT2__00000-01000.trans.bz2</strong>[54.34 MB]<br>(1H)2(32S) line list transitions: 0-01000 cm-1 <strong>1H2-32S__AYT2__01000-02000.trans.bz2</strong>[53.49 MB]<br>(1H)2(32S) line list transitions: 01000-02000 cm-1 <strong>1H2-32S__AYT2__02000-03000.trans.bz2</strong>[54.8 MB]<br>(1H)2(32S) line list transitions: 02000-03000 cm-1 <strong>1H2-32S__AYT2__03000-04000.trans.bz2</strong>[56.38 MB]<br>(1H)2(32S) line list transitions: 03000-04000 cm-1 <strong>1H2-32S__AYT2__04000-05000.trans.bz2</strong>[59.56 MB]<br>(1H)2(32S) line list transitions: 04000-05000 cm-1 <strong>1H2-32S__AYT2__05000-06000.trans.bz2</strong>[64.14 MB]<br>(1H)2(32S) line list transitions: 05000-06000 cm-1 <strong>1H2-32S__AYT2__06000-07000.trans.bz2</strong>[70.21 MB]<br>(1H)2(32S) line list transitions: 06000-07000 cm-1 <strong>1H2-32S__AYT2__07000-08000.trans.bz2</strong>[78.34 MB]<br>(1H)2(32S) line list transitions: 07000-08000 cm-1 <strong>1H2-32S__AYT2__08000-09000.trans.bz2</strong>[87.14 MB]<br>(1H)2(32S) line list transitions: 08000-09000 cm-1 <strong>1H2-32S__AYT2__09000-10000.trans.bz2</strong>[91.38 MB]<br>(1H)2(32S) line list transitions: 09000-10000 cm-1 <strong>1H2-32S__AYT2__10000-11000.trans.bz2</strong>[71.09 MB]<br>(1H)2(32S) line list transitions: 10000-11000 cm-1 <strong>1H2-32S__AYT2__11000-12000.trans.bz2</strong>[49.53 MB]<br>(1H)2(32S) line list transitions: 11000-12000 cm-1 <strong>1H2-32S__AYT2__12000-13000.trans.bz2</strong>[33.42 MB]<br>(1H)2(32S) line list transitions: 12000-13000 cm-1 <strong>1H2-32S__AYT2__13000-14000.trans.bz2</strong>[21.45 MB]<br>(1H)2(32S) line list transitions: 13000-14000 cm-1 <strong>1H2-32S__AYT2__14000-15000.trans.bz2</strong>[13.12 MB]<br>(1H)2(32S) line list transitions: 14000-15000 cm-1 <strong>1H2-32S__AYT2__15000-16000.trans.bz2</strong>[7.43 MB]<br>(1H)2(32S) line list transitions: 15000-16000 cm-1 <strong>1H2-32S__AYT2__16000-17000.trans.bz2</strong>[3.81 MB]<br>(1H)2(32S) line list transitions: 16000-17000 cm-1 <strong>1H2-32S__AYT2__17000-18000.trans.bz2</strong>[1.83 MB]<br>(1H)2(32S) line list transitions: 17000-18000 cm-1 <strong>1H2-32S__AYT2__18000-19000.trans.bz2</strong>[795.5 KB]<br>(1H)2(32S) line list transitions: 18000-19000 cm-1 <strong>1H2-32S__AYT2__19000-20000.trans.bz2</strong>[292.97 KB]<br>(1H)2(32S) line list transitions: 19000-20000 cm-1 <strong>1H2-32S__AYT2__20000-21000.trans.bz2</strong>[130.91 KB]<br>(1H)2(32S) line list transitions: 20000-21000 cm-1 <strong>1H2-32S__AYT2__21000-22000.trans.bz2</strong>[82.11 KB]<br>(1H)2(32S) line list transitions: 21000-22000 cm-1 <strong>1H2-32S__AYT2__22000-23000.trans.bz2</strong>[61.75 KB]<br>(1H)2(32S) line list transitions: 22000-23000 cm-1 <strong>1H2-32S__AYT2__23000-24000.trans.bz2</strong>[49.0 KB]<br>(1H)2(32S) line list transitions: 23000-24000 cm-1 <strong>1H2-32S__AYT2__24000-25000.trans.bz2</strong>[39.22 KB]<br>(1H)2(32S) line list transitions: 24000-25000 cm-1 <strong>1H2-32S__AYT2__25000-26000.trans.bz2</strong>[30.76 KB]<br>(1H)2(32S) line list transitions: 25000-26000 cm-1 <strong>1H2-32S__AYT2__26000-27000.trans.bz2</strong>[23.9 KB]<br>(1H)2(32S) line list transitions: 26000-27000 cm-1 <strong>1H2-32S__AYT2__27000-28000.trans.bz2</strong>[17.68 KB]<br>(1H)2(32S) line list transitions: 27000-28000 cm-1 <strong>1H2-32S__AYT2__28000-29000.trans.bz2</strong>[13.12 KB]<br>(1H)2(32S) line list transitions: 28000-29000 cm-1 <strong>1H2-32S__AYT2__29000-30000.trans.bz2</strong>[9.37 KB]<br>(1H)2(32S) line list transitions: 29000-30000 cm-1 <strong>1H2-32S__AYT2__30000-31000.trans.bz2</strong>[6.3 KB]<br>(1H)2(32S) line list transitions: 30000-31000 cm-1 <strong>1H2-32S__AYT2__31000-32000.trans.bz2</strong>[3.79 KB]<br>(1H)2(32S) line list transitions: 31000-32000 cm-1 <strong>1H2-32S__AYT2__32000-33000.trans.bz2</strong>[1.97 KB]<br>(1H)2(32S) line list transitions: 32000-33000 cm-1 <strong>1H2-32S__AYT2__33000-34000.trans.bz2</strong>[1.09 KB]<br>(1H)2(32S) line list transitions: 33000-34000 cm-1 <strong>1H2-32S__AYT2__34000-35000.trans.bz2</strong>[454 bytes]<br>(1H)2(32S) line list transitions: 34000-35000 cm-1 <strong>References:</strong><br> 1. Azzam, A. A. A., Tennyson, J., Yurchenko, S. N., Naumenko, O. V., "ExoMol molecular line lists – XVI: The rotation-vibration spectrum of hot H2S", Monthly Notices of the Royal Astronomical Society 460, 4063-4074 (2016). [http://dx.doi.org/10.1093/mnras/stw1133][16AzTeYu.H2S]<br> <strong>AYT2: partition function</strong> <em>Ro-vibrational line list for H2S</em><br> <strong>H2S__AYT2.readme</strong>[4.0 KB]<br>Documentation for the AYT2 line list for H2S <strong>1H2-32S__AYT2.pf</strong>[76.17 KB]<br>Partition function for H2S calculated from the AYT2 line list. <strong>References:</strong><br> <strong>AYT2: opacity</strong> <em>Ro-vibrational line list for H2S</em><br> <strong>1H2-32S__AYT2.R1000_0.3-50mu.ktable.ARCiS.fits.gz</strong>[445.05 MB]<br>ARCiS k-tables at R= 1000 (0.3-50mu) in fits format (gzipped): AYT2 (1H)2(32S) line list. <strong>1H2-32S__AYT2.R1000_0.3-50mu.ktable.petitRADTRANS.h5</strong>[370.98 MB]<br>petitRADTRANS k-tables at R= 1000 (0.3-50mu) in HDF5 format: AYT2 (1H)2(32S) line list. <strong>1H2-32S__AYT2.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: AYT2 (1H)2(32S) line list. <strong>1H2-32S__AYT2.R15000_0.3-50mu.xsec.TauREx.h5</strong>[348.39 MB]<br>TauREx k-tables at R= 15000 (0.3-50mu) in HDF5 format: AYT2 (1H)2(32S) line list. <strong>References:</strong><br> 1. Azzam, A. A. A., Tennyson, J., Yurchenko, S. N., Naumenko, O. V., "ExoMol molecular line lists – XVI: The rotation-vibration spectrum of hot H2S", Monthly Notices of the Royal Astronomical Society 460, 4063-4074 (2016). [http://dx.doi.org/10.1093/mnras/stw1133][16AzTeYu.H2S]<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>