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The OYT dataset for 12C1H335Cl
<p>The dataset is an archive of ExoMol page, https://exomol.com/data/molecules/CH3Cl/12C-1H3-35Cl/OYT.<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 CH3Cl_12C1H335Cl_OYT.md for detailed information.</strong> <br></p> <strong>Definitions file</strong> <blockquote> <p><strong>12C-1H3-35Cl__OYT.def</strong>[9.14 KB]<br></p> <p><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). [<a href="https://doi.org/10.1016/j.jqsrt.2020.107228">https://doi.org/10.1016/j.jqsrt.2020.107228</a>]</p> </blockquote> <strong>Spectroscopic Model</strong> <blockquote> <p><a href="https://exomol.com/models/CH3Cl/12C-1H3-35Cl/OYT/">https://exomol.com/models/CH3Cl/12C-1H3-35Cl/OYT/</a><br></p> </blockquote> <strong>OYT: line list</strong> <p><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/CH3Cl/12C-1H3-35Cl/OYT<br></p> <blockquote> <p><strong>References:</strong><br> 1. Owens, A., Yachmenev, A., Thiel, W., Fateev, A., Tennyson, J., Yurchenko, S. N., "ExoMol line lists – XXIX. The rotation-vibration spectrum of methyl chloride up to 1200 K", Monthly Notices of the Royal Astronomical Society 479, 3002-3010 (2018). <a href="[https://doi.org/10.1093/mnras/sty1542]">[https://doi.org/10.1093/mnras/sty1542]</a>[18OwYaTh.CH3Cl]<br></p> </blockquote> <strong>OYT: partition function</strong> <p><em>The OYT calculated high-temperature line list for CH3Cl</em><br></p> <blockquote> <p><strong>12C-1H3-35Cl__OYT.pf</strong>[50.78 KB]<br>OYT (12C)(1H)3(35Cl) partition function file</p> <p><strong>References:</strong><br> 1. Owens, A., Yachmenev, A., Thiel, W., Fateev, A., Tennyson, J., Yurchenko, S. N., "ExoMol line lists – XXIX. The rotation-vibration spectrum of methyl chloride up to 1200 K", Monthly Notices of the Royal Astronomical Society 479, 3002-3010 (2018). <a href="[https://doi.org/10.1093/mnras/sty1542]">[https://doi.org/10.1093/mnras/sty1542]</a>[18OwYaTh.CH3Cl]<br></p> </blockquote> <strong>OYT: super-line</strong> <p><strong>NB: These data are not included in current version on Zenodo</strong><br> <strong>Data can be accessed via:</strong> https://exomol.com/data/molecules/CH3Cl/12C-1H3-35Cl/OYT<br></p> <strong>OYT: opacity</strong> <p><em>The OYT calculated high-temperature line list for CH3Cl</em><br></p> <blockquote> <p><strong>12C-1H3-35Cl__OYT.R1000_0.3-50mu.ktable.ARCiS.fits.gz</strong>[298.77 MB]<br>ARCiS k-tables at R= 1000 (0.3-50mu) in fits format (gzipped): OYT (12C)(1H)3(35Cl) line list.</p> <p><strong>12C-1H3-35Cl__OYT.R1000_0.3-50mu.ktable.petitRADTRANS.h5</strong>[370.98 MB]<br>petitRADTRANS k-tables at R= 1000 (0.3-50mu) in HDF5 format: OYT (12C)(1H)3(35Cl) line list.</p> <p><strong>12C-1H3-35Cl__OYT.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: OYT (12C)(1H)3(35Cl) line list.</p> <p><strong>12C-1H3-35Cl__OYT.R15000_0.3-50mu.xsec.TauREx.h5</strong>[348.39 MB]<br>TauREx k-tables at R= 15000 (0.3-50mu) in HDF5 format: OYT (12C)(1H)3(35Cl) line list.</p> <p><strong>References:</strong><br> 1. Owens, A., Yachmenev, A., Thiel, W., Fateev, A., Tennyson, J., Yurchenko, S. N., "ExoMol line lists – XXIX. The rotation-vibration spectrum of methyl chloride up to 1200 K", Monthly Notices of the Royal Astronomical Society 479, 3002-3010 (2018). <a href="[https://doi.org/10.1093/mnras/sty1542]">[https://doi.org/10.1093/mnras/sty1542]</a>[18OwYaTh.CH3Cl]<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). <a href="[http://dx.doi.org/10.1051/0004-6361/202038350]">[http://dx.doi.org/10.1051/0004-6361/202038350]</a>[20ChRoYu.]<br></p> </blockquote>
The OY-Cis dataset for cis-31P21H2
<p>The dataset is an archive of ExoMol page, https://exomol.com/data/molecules/cis-P2H2/cis-31P2-1H2/OY-Cis.<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 cis-P2H2_cis-31P21H2_OY-Cis.md for detailed information.</strong> <br></p> <strong>Definitions file</strong> <blockquote> <p><strong>cis-31P2-1H2__OY-Cis.def</strong>[8.25 KB]<br></p> <p><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). [<a href="https://doi.org/10.1016/j.jqsrt.2020.107228">https://doi.org/10.1016/j.jqsrt.2020.107228</a>]</p> </blockquote> <strong>Spectroscopic Model</strong> <blockquote> <p><a href="https://exomol.com/models/cis-P2H2/cis-31P2-1H2/OY-Cis/">https://exomol.com/models/cis-P2H2/cis-31P2-1H2/OY-Cis/</a><br></p> </blockquote> <strong>OY-Cis: line list</strong> <p><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/cis-P2H2/cis-31P2-1H2/OY-Cis<br></p> <blockquote> <p><strong>References:</strong><br> 1. Owens, A., Yurchenko, S. N., "Theoretical rotation-vibration spectroscopy of cis- and trans-diphosphene (P2H2) and the deuterated species P2HD", Journal of Chemical Physics 150, 194308/1-9 (2019). <a href="[https://doi.org/10.1063/1.5092767]">[https://doi.org/10.1063/1.5092767]</a>[19OwYuxx.P2H2]<br></p> </blockquote> <strong>OY-Cis: partition function</strong> <p><em>OY-Cis ro-vibrational line list for cis-P2H2</em><br></p> <blockquote> <p><strong>cis-31P2-1H2__OY-Cis.pf</strong>[24.41 KB]<br>Partition function produced using the Cis-(31P)2(1H)2 line list.</p> <p><strong>References:</strong><br> 1. Owens, A., Yurchenko, S. N., "Theoretical rotation-vibration spectroscopy of cis- and trans-diphosphene (P2H2) and the deuterated species P2HD", Journal of Chemical Physics 150, 194308/1-9 (2019). <a href="[https://doi.org/10.1063/1.5092767]">[https://doi.org/10.1063/1.5092767]</a>[19OwYuxx.P2H2]<br></p> </blockquote> <strong>OY-Cis: opacity</strong> <p><em>OY-Cis ro-vibrational line list for cis-P2H2</em><br></p> <blockquote> <p><strong>cis-31P2-1H2__OY-Cis.R1000_0.3-50mu.ktable.ARCiS.fits.gz</strong>[295.65 MB]<br>ARCiS k-tables at R= 1000 (0.3-50mu) in fits format (gzipped): OY-Cis (31P)2(1H)2 line list.</p> <p><strong>cis-31P2-1H2__OY-Cis.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: OY-Cis (31P)2(1H)2 line list.</p> <p><strong>cis-31P2-1H2__OY-Cis.R15000_0.3-50mu.xsec.TauREx.h5</strong>[348.39 MB]<br>TauREx k-tables at R= 15000 (0.3-50mu) in HDF5 format: OY-Cis (31P)2(1H)2 line list.</p> <p><strong>cis-31P2-1H2__OY-Cis.R1000_0.3-50mu.ktable.petitRADTRANS.h5</strong>[370.98 MB]<br>petitRADTRANS k-tables at R= 1000 (0.3-50mu) in HDF5 format: OY-Cis (31P)2(1H)2 line list.</p> <p><strong>References:</strong><br> 1. Owens, A., Yurchenko, S. N., "Theoretical rotation-vibration spectroscopy of cis- and trans-diphosphene (P2H2) and the deuterated species P2HD", Journal of Chemical Physics 150, 194308/1-9 (2019). <a href="[https://doi.org/10.1063/1.5092767]">[https://doi.org/10.1063/1.5092767]</a>[19OwYuxx.P2H2]<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). <a href="[http://dx.doi.org/10.1051/0004-6361/202038350]">[http://dx.doi.org/10.1051/0004-6361/202038350]</a>[20ChRoYu.]<br></p> </blockquote>
The OY-Trans dataset for trans-31P21H2H
<p>The dataset is an archive of ExoMol page, https://exomol.com/data/molecules/trans-P2H2/trans-31P2-1H2/OY-Trans.<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 trans-P2H2_trans-31P21H2H_OY-Trans.md for detailed information.</strong> <br></p> <strong>Definitions file</strong> <blockquote> <p><strong>trans-31P2-1H2__OY-Trans.def</strong>[8.25 KB]<br></p> <p><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). [<a href="https://doi.org/10.1016/j.jqsrt.2020.107228">https://doi.org/10.1016/j.jqsrt.2020.107228</a>]</p> </blockquote> <strong>Spectroscopic Model</strong> <blockquote> <p><a href="https://exomol.com/models/trans-P2H2/trans-31P2-1H2/OY-Trans/">https://exomol.com/models/trans-P2H2/trans-31P2-1H2/OY-Trans/</a><br></p> </blockquote> <strong>OY-Trans: line list</strong> <p><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/trans-P2H2/trans-31P2-1H2/OY-Trans<br></p> <blockquote> <p><strong>References:</strong><br> 1. Owens, A., Yurchenko, S. N., "Theoretical rotation-vibration spectroscopy of cis- and trans-diphosphene (P2H2) and the deuterated species P2HD", Journal of Chemical Physics 150, 194308/1-9 (2019). <a href="[https://doi.org/10.1063/1.5092767]">[https://doi.org/10.1063/1.5092767]</a>[19OwYuxx.P2H2]<br></p> </blockquote> <strong>OY-Trans: partition function</strong> <p><em>Trans ro-vibrational line list for trans-P2H2</em><br></p> <blockquote> <p><strong>trans-31P2-1H2__OY-Trans.pf</strong>[24.41 KB]<br>Partition function produced using the Trans-(31P)2(1H)2 line list.</p> <p><strong>References:</strong><br> 1. Owens, A., Yurchenko, S. N., "Theoretical rotation-vibration spectroscopy of cis- and trans-diphosphene (P2H2) and the deuterated species P2HD", Journal of Chemical Physics 150, 194308/1-9 (2019). <a href="[https://doi.org/10.1063/1.5092767]">[https://doi.org/10.1063/1.5092767]</a>[19OwYuxx.P2H2]<br></p> </blockquote> <strong>OY-Trans: opacity</strong> <p><em>Trans ro-vibrational line list for trans-P2H2</em><br></p> <blockquote> <p><strong>trans-31P2-1H2__OY-Trans.R1000_0.3-50mu.ktable.ARCiS.fits.gz</strong>[296.04 MB]<br>ARCiS k-tables at R= 1000 (0.3-50mu) in fits format (gzipped): OY-Trans (31P)2(1H)2 line list.</p> <p><strong>trans-31P2-1H2__OY-Trans.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: OY-Trans (31P)2(1H)2 line list.</p> <p><strong>trans-31P2-1H2__OY-Trans.R15000_0.3-50mu.xsec.TauREx.h5</strong>[348.39 MB]<br>TauREx k-tables at R= 15000 (0.3-50mu) in HDF5 format: OY-Trans (31P)2(1H)2 line list.</p> <p><strong>trans-31P2-1H2__OY-Trans.R1000_0.3-50mu.ktable.petitRADTRANS.h5</strong>[370.98 MB]<br>petitRADTRANS k-tables at R= 1000 (0.3-50mu) in HDF5 format: OY-Trans (31P)2(1H)2 line list.</p> <p><strong>References:</strong><br> 1. Owens, A., Yurchenko, S. N., "Theoretical rotation-vibration spectroscopy of cis- and trans-diphosphene (P2H2) and the deuterated species P2HD", Journal of Chemical Physics 150, 194308/1-9 (2019). <a href="[https://doi.org/10.1063/1.5092767]">[https://doi.org/10.1063/1.5092767]</a>[19OwYuxx.P2H2]<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). <a href="[http://dx.doi.org/10.1051/0004-6361/202038350]">[http://dx.doi.org/10.1051/0004-6361/202038350]</a>[20ChRoYu.]<br></p> </blockquote>
The SAlTY dataset for 31P1H3
<p>The dataset is an archive of ExoMol page, https://exomol.com/data/molecules/PH3/31P-1H3/SAlTY.<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 PH3_31P1H3_SAlTY.md for detailed information.</strong> <br></p> <strong>Definitions file</strong> <blockquote> <p><strong>31P-1H3__SAlTY.def</strong>[12.33 KB]<br></p> <p><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). [<a href="https://doi.org/10.1016/j.jqsrt.2020.107228">https://doi.org/10.1016/j.jqsrt.2020.107228</a>]</p> </blockquote> <strong>Spectroscopic Model</strong> <blockquote> <p><a href="https://exomol.com/models/PH3/31P-1H3/SAlTY/">https://exomol.com/models/PH3/31P-1H3/SAlTY/</a><br></p> </blockquote> <strong>SAlTY: line list</strong> <p><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/PH3/31P-1H3/SAlTY<br></p> <blockquote> <p><strong>References:</strong><br> 1. Sousa-Silva, C., Al-Refaie, A. F., Tennyson, J., Yurchenko, S. N., "ExoMol line lists VII: The rotation-vibration spectrum of phosphine up to 1500 K", Monthly Notices of the Royal Astronomical Society 446, 2337-2347 (2014). <a href="[http://dx.doi.org/10.1093/mnras/stu2246]">[http://dx.doi.org/10.1093/mnras/stu2246]</a>[14SoAlTe.PH3]<br></p> </blockquote> <strong>SAlTY: partition function</strong> <p><em>A computed hot line list for phosphine.</em><br></p> <blockquote> <p><strong>SAlTY_readme.txt</strong>[1.62 KB]<br>Documentation for the line list of the SAlTY PH3 data set.</p> <p><strong>31P-1H3__SAlTY.pf</strong>[25.39 KB]<br>Partition Function for (31P)(1H)3</p> <p><strong>References:</strong><br> 1. Sousa-Silva, C., Al-Refaie, A. F., Tennyson, J., Yurchenko, S. N., "ExoMol line lists VII: The rotation-vibration spectrum of phosphine up to 1500 K", Monthly Notices of the Royal Astronomical Society 446, 2337-2347 (2014). <a href="[http://dx.doi.org/10.1093/mnras/stu2246]">[http://dx.doi.org/10.1093/mnras/stu2246]</a>[14SoAlTe.PH3]<br></p> </blockquote> <strong>SAlTY: opacity</strong> <p><em>A computed hot line list for phosphine.</em><br></p> <blockquote> <p><strong>31P-1H3__SAlTY.R1000_0.3-50mu.ktable.ARCiS.fits.gz</strong>[339.54 MB]<br>ARCiS k-tables at R= 1000 (0.3-50mu) in fits format (gzipped): SAlTY (31P)(1H)3 line list.</p> <p><strong>31P-1H3__SAlTY.R1000_0.3-50mu.ktable.petitRADTRANS.h5</strong>[370.98 MB]<br>petitRADTRANS k-tables at R= 1000 (0.3-50mu) in HDF5 format: SAlTY (31P)(1H)3 line list.</p> <p><strong>31P-1H3__SAlTY.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: SAlTY (31P)(1H)3 line list.</p> <p><strong>31P-1H3__SAlTY.R15000_0.3-50mu.xsec.TauREx.h5</strong>[348.39 MB]<br>TauREx k-tables at R= 15000 (0.3-50mu) in HDF5 format: SAlTY (31P)(1H)3 line list.</p> <p><strong>References:</strong><br> 1. Sousa-Silva, C., Al-Refaie, A. F., Tennyson, J., Yurchenko, S. N., "ExoMol line lists VII: The rotation-vibration spectrum of phosphine up to 1500 K", Monthly Notices of the Royal Astronomical Society 446, 2337-2347 (2014). <a href="[http://dx.doi.org/10.1093/mnras/stu2246]">[http://dx.doi.org/10.1093/mnras/stu2246]</a>[14SoAlTe.PH3]<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). <a href="[http://dx.doi.org/10.1051/0004-6361/202038350]">[http://dx.doi.org/10.1051/0004-6361/202038350]</a>[20ChRoYu.]<br></p> </blockquote>
The AIJS dataset for 1H14N16O3
<p>The dataset is an archive of ExoMol page, https://exomol.com/data/molecules/HNO3/1H-14N-16O3/AIJS.<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 HNO3_1H14N16O3_AIJS.md for detailed information.</strong> <br></p> <strong>Definitions file</strong> <blockquote> <p><strong>1H-14N-16O3__AIJS.def</strong>[7.6 KB]<br></p> <p><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). [<a href="https://doi.org/10.1016/j.jqsrt.2020.107228">https://doi.org/10.1016/j.jqsrt.2020.107228</a>]</p> </blockquote> <strong>Spectroscopic Model</strong> <blockquote> <p><a href="https://exomol.com/models/HNO3/1H-14N-16O3/AIJS/">https://exomol.com/models/HNO3/1H-14N-16O3/AIJS/</a><br></p> </blockquote> <strong>AIJS: line list</strong> <p><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/HNO3/1H-14N-16O3/AIJS<br></p> <blockquote> <p><strong>References:</strong><br> 1. Pavlyuchko, A. I., Yurchenko, S. N., Tennyson, J., "ExoMol molecular line lists – XI. The spectrum of nitric acid", Monthly Notices of the Royal Astronomical Society 452, 1702-1706 (2015). <a href="[http://dx.doi.org/10.1093/mnras/stv1376]">[http://dx.doi.org/10.1093/mnras/stv1376]</a>[15PaYuTe.HNO3]<br></p> </blockquote> <strong>AIJS: partition function</strong> <p><em>Line list for nitric acid (HNO3) for temperatures up to 500 K.</em><br></p> <blockquote> <p><strong>README_AIJS.txt</strong>[4.66 KB]<br>Documentation for the HNO3 line list of the AIJS dataset</p> <p><strong>1H-14N-16O3__AIJS.pf</strong>[12.7 KB]<br>Partition function for (1H)(14N)(16O)3</p> <p><strong>References:</strong><br> 1. Pavlyuchko, A. I., Yurchenko, S. N., Tennyson, J., "ExoMol molecular line lists – XI. The spectrum of nitric acid", Monthly Notices of the Royal Astronomical Society 452, 1702-1706 (2015). <a href="[http://dx.doi.org/10.1093/mnras/stv1376]">[http://dx.doi.org/10.1093/mnras/stv1376]</a>[15PaYuTe.HNO3]<br></p> </blockquote> <strong>AIJS: opacity</strong> <p><em>Line list for nitric acid (HNO3) for temperatures up to 500 K.</em><br></p> <blockquote> <p><strong>1H-14N-16O3__AIJS.R1000_0.3-50mu.ktable.ARCiS.fits.gz</strong>[306.7 MB]<br>ARCiS k-tables at R= 1000 (0.3-50mu) in fits format (gzipped): AIJS (1H)(14N)(16O)3 line list.</p> <p><strong>1H-14N-16O3__AIJS.R1000_0.3-50mu.ktable.petitRADTRANS.h5</strong>[370.98 MB]<br>petitRADTRANS k-tables at R= 1000 (0.3-50mu) in HDF5 format: AIJS (1H)(14N)(16O)3 line list.</p> <p><strong>1H-14N-16O3__AIJS.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: AIJS (1H)(14N)(16O)3 line list.</p> <p><strong>1H-14N-16O3__AIJS.R15000_0.3-50mu.xsec.TauREx.h5</strong>[348.39 MB]<br>TauREx k-tables at R= 15000 (0.3-50mu) in HDF5 format: AIJS (1H)(14N)(16O)3 line list.</p> <p><strong>References:</strong><br> 1. Pavlyuchko, A. I., Yurchenko, S. N., Tennyson, J., "ExoMol molecular line lists – XI. The spectrum of nitric acid", Monthly Notices of the Royal Astronomical Society 452, 1702-1706 (2015). <a href="[http://dx.doi.org/10.1093/mnras/stv1376]">[http://dx.doi.org/10.1093/mnras/stv1376]</a>[15PaYuTe.HNO3]<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). <a href="[http://dx.doi.org/10.1051/0004-6361/202038350]">[http://dx.doi.org/10.1051/0004-6361/202038350]</a>[20ChRoYu.]<br></p> </blockquote>
The ADJSAAM dataset for 1H2H+
<p>The dataset is an archive of ExoMol page, https://exomol.com/data/molecules/H2_p/1H-2H_p/ADJSAAM.<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 H2_p_1H2H+_ADJSAAM.md for detailed information.</strong> <br></p> <strong>Definitions file</strong> <blockquote> <p><strong>1H-2H_p__ADJSAAM.def</strong>[4.86 KB]<br></p> <p><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). [<a href="https://doi.org/10.1016/j.jqsrt.2020.107228">https://doi.org/10.1016/j.jqsrt.2020.107228</a>]</p> </blockquote> <strong>Spectroscopic Model</strong> <blockquote> <p><a href="https://exomol.com/models/H2_p/1H-2H_p/ADJSAAM/">https://exomol.com/models/H2_p/1H-2H_p/ADJSAAM/</a><br></p> </blockquote> <strong>ADJSAAM: line list</strong> <p><em>Ab initio line list for isotopologues of HD, HD+ and HeH+ by Amaral et al (2019)</em><br></p> <blockquote> <p><strong>1H-2H_p__ADJSAAM.states.bz2</strong>[6.36 KB]<br>Energy file for the ADJSAAM line list for HD+.</p> <p><strong>1H-2H_p__ADJSAAM.trans.bz2</strong>[112.05 KB]<br>Transition file for the ADJSAAM line list for HD+.</p> <p><strong>References:</strong><br> 1. Amaral, P. H. R., Diniz, L.G., Jones, K.A., Stanke, M., Alijah, A., Adamowicz, L., Mohallem, J.R., "Benchmark Rovibrational Linelists and Einstein A-coefficients for the Primordial Molecules and Isotopologues", The Astrophysical Journal 878, 95 (2019). <a href="[https://doi.org/10.3847/1538-4357/ab1f65]">[https://doi.org/10.3847/1538-4357/ab1f65]</a><br></p> </blockquote> <strong>ADJSAAM: partition function</strong> <p><em>Ab initio line list for isotopologues of HD, HD+ and HeH+ by Amaral et al (2019)</em><br></p> <blockquote> <p><strong>1H-2H_p__ADJSAAM.pf</strong>[195.31 KB]<br>Partition function file for the ADJSAAM line list for HD+.</p> <p><strong>References:</strong><br> 1. Amaral, P. H. R., Diniz, L.G., Jones, K.A., Stanke, M., Alijah, A., Adamowicz, L., Mohallem, J.R., "Benchmark Rovibrational Linelists and Einstein A-coefficients for the Primordial Molecules and Isotopologues", The Astrophysical Journal 878, 95 (2019). <a href="[https://doi.org/10.3847/1538-4357/ab1f65]">[https://doi.org/10.3847/1538-4357/ab1f65]</a><br></p> </blockquote> <strong>ADJSAAM: opacity</strong> <p><em>Ab initio line list for isotopologues of HD, HD+ and HeH+ by Amaral et al (2019)</em><br></p> <blockquote> <p><strong>1H-2H_p__ADJSAAM.R1000_0.3-50mu.ktable.ARCiS.fits.gz</strong>[405.32 MB]<br>ARCiS k-tables at R= 1000 (0.3-50mu) in fits format (gzipped): ADJSAAM (1H)(2H)+ line list.</p> <p><strong>1H-2H_p__ADJSAAM.R1000_0.3-50mu.ktable.petitRADTRANS.h5</strong>[370.98 MB]<br>petitRADTRANS k-tables at R= 1000 (0.3-50mu) in HDF5 format: ADJSAAM (1H)(2H)+ line list.</p> <p><strong>1H-2H_p__ADJSAAM.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: ADJSAAM (1H)(2H)+ line list.</p> <p><strong>1H-2H_p__ADJSAAM.R15000_0.3-50mu.xsec.TauREx.h5</strong>[348.39 MB]<br>TauREx k-tables at R= 15000 (0.3-50mu) in HDF5 format: ADJSAAM (1H)(2H)+ line list.</p> <p><strong>References:</strong><br> 1. Amaral, P. H. R., Diniz, L.G., Jones, K.A., Stanke, M., Alijah, A., Adamowicz, L., Mohallem, J.R., "Benchmark Rovibrational Linelists and Einstein A-coefficients for the Primordial Molecules and Isotopologues", The Astrophysical Journal 878, 95 (2019). <a href="[https://doi.org/10.3847/1538-4357/ab1f65]">[https://doi.org/10.3847/1538-4357/ab1f65]</a><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). <a href="[http://dx.doi.org/10.1051/0004-6361/202038350]">[http://dx.doi.org/10.1051/0004-6361/202038350]</a>[20ChRoYu.]<br></p> </blockquote>
The CATS dataset for 28Si1H2
<p>The dataset is an archive of ExoMol page, https://exomol.com/data/molecules/SiH2/28Si-1H2/CATS.<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 SiH2_28Si1H2_CATS.md for detailed information.</strong> <br></p> <strong>Definitions file</strong> <blockquote> <p><strong>28Si-1H2__CATS.def</strong>[8.4 KB]<br></p> <p><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). [<a href="https://doi.org/10.1016/j.jqsrt.2020.107228">https://doi.org/10.1016/j.jqsrt.2020.107228</a>]</p> </blockquote> <strong>Spectroscopic Model</strong> <blockquote> <p><a href="https://exomol.com/models/SiH2/28Si-1H2/CATS/">https://exomol.com/models/SiH2/28Si-1H2/CATS/</a><br></p> </blockquote> <strong>CATS: partition function</strong> <p><em>SiH2 line list CATS obtained using a refined PES and ab initio DMS, computed with TROVE</em><br></p> <blockquote> <p><strong>28Si-1H2__CATS.pf</strong>[48.83 KB]<br>A CATS partition function, (28Si)(1H)2.</p> <p><strong>References:</strong><br> 1. Clark, V. H. J., Owens, A., Tennyson, J., Yurchenko, S. N., "The high-temperature rotation-vibration spectrum and rotational clustering of silylene (SiH2)", Journal of Quantitative Spectroscopy and Radiative Transfer 246, 106929 (2021). <a href="[https://doi.org/10.1016/j.jqsrt.2020.106929]">[https://doi.org/10.1016/j.jqsrt.2020.106929]</a>[21ClOwTe.SiH2]<br></p> </blockquote> <strong>CATS: line list</strong> <p><em>SiH2 line list CATS obtained using a refined PES and ab initio DMS, computed with TROVE</em><br></p> <blockquote> <p><strong>28Si-1H2__CATS.states.bz2</strong>[6.9 MB]<br>A CATS .states file. (28Si)(1H)2 hot line list.</p> <p><strong>28Si-1H2__CATS__00000-01000.trans.bz2</strong>[80.78 MB]<br>CATS hot line list transitions, (28Si)(1H)2: 0-1000 cm-1.</p> <p><strong>28Si-1H2__CATS__01000-02000.trans.bz2</strong>[105.67 MB]<br>CATS hot line list transitions, (28Si)(1H)2: 1000-2000 cm-1.</p> <p><strong>28Si-1H2__CATS__02000-03000.trans.bz2</strong>[134.01 MB]<br>CATS hot line list transitions, (28Si)(1H)2: 2000-3000 cm-1.</p> <p><strong>28Si-1H2__CATS__03000-04000.trans.bz2</strong>[167.82 MB]<br>CATS hot line list transitions, (28Si)(1H)2: 3000-4000 cm-1.</p> <p><strong>28Si-1H2__CATS__04000-05000.trans.bz2</strong>[205.19 MB]<br>CATS hot line list transitions, (28Si)(1H)2: 4000-5000 cm-1.</p> <p><strong>28Si-1H2__CATS__05000-06000.trans.bz2</strong>[249.32 MB]<br>CATS hot line list transitions, (28Si)(1H)2: 5000-6000 cm-1.</p> <p><strong>28Si-1H2__CATS__06000-07000.trans.bz2</strong>[298.96 MB]<br>CATS hot line list transitions, (28Si)(1H)2: 6000-7000 cm-1.</p> <p><strong>28Si-1H2__CATS__07000-08000.trans.bz2</strong>[354.93 MB]<br>CATS hot line list transitions, (28Si)(1H)2: 7000-8000 cm-1.</p> <p><strong>28Si-1H2__CATS__08000-09000.trans.bz2</strong>[415.19 MB]<br>CATS hot line list transitions, (28Si)(1H)2: 8000-9000 cm-1.</p> <p><strong>28Si-1H2__CATS__09000-10000.trans.bz2</strong>[476.85 MB]<br>CATS hot line list transitions, (28Si)(1H)2: 9000-10000 cm-1.</p> <p><strong>References:</strong><br> 1. Clark, V. H. J., Owens, A., Tennyson, J., Yurchenko, S. N., "The high-temperature rotation-vibration spectrum and rotational clustering of silylene (SiH2)", Journal of Quantitative Spectroscopy and Radiative Transfer 246, 106929 (2021). <a href="[https://doi.org/10.1016/j.jqsrt.2020.106929]">[https://doi.org/10.1016/j.jqsrt.2020.106929]</a>[21ClOwTe.SiH2]<br></p> </blockquote> <strong>CATS: opacity</strong> <p><em>SiH2 line list CATS obtained using a refined PES and ab initio DMS, computed with TROVE</em><br></p> <blockquote> <p><strong>28Si-1H2__CATS.R1000_0.3-50mu.ktable.ARCiS.fits.gz</strong>[339.68 MB]<br>ARCiS k-tables at R= 1000 (0.3-50mu) in fits format (gzipped): CATS (28Si)(1H)2 line list.</p> <p><strong>28Si-1H2__CATS.R1000_0.3-50mu.ktable.petitRADTRANS.h5</strong>[370.98 MB]<br>petitRADTRANS k-tables at R= 1000 (0.3-50mu) in HDF5 format: CATS (28Si)(1H)2 line list.</p> <p><strong>28Si-1H2__CATS.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: CATS (28Si)(1H)2 line list.</p> <p><strong>28Si-1H2__CATS.R15000_0.3-50mu.xsec.TauREx.h5</strong>[348.39 MB]<br>TauREx k-tables at R= 15000 (0.3-50mu) in HDF5 format: CATS (28Si)(1H)2 line list.</p> <p><strong>References:</strong><br> 1. Clark, V. H. J., Owens, A., Tennyson, J., Yurchenko, S. N., "The high-temperature rotation-vibration spectrum and rotational clustering of silylene (SiH2)", Journal of Quantitative Spectroscopy and Radiative Transfer 246, 106929 (2021). <a href="[https://doi.org/10.1016/j.jqsrt.2020.106929]">[https://doi.org/10.1016/j.jqsrt.2020.106929]</a>[21ClOwTe.SiH2]<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). <a href="[http://dx.doi.org/10.1051/0004-6361/202038350]">[http://dx.doi.org/10.1051/0004-6361/202038350]</a>[20ChRoYu.]<br></p> </blockquote>
The UYT2 dataset for 32S16O3
<p>The dataset is an archive of ExoMol page, https://exomol.com/data/molecules/SO3/32S-16O3/UYT2.<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 SO3_32S16O3_UYT2.md for detailed information.</strong> <br></p> <strong>Definitions file</strong> <blockquote> <p><strong>32S-16O3__UYT2.def</strong>[9.62 KB]<br></p> <p><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). [<a href="https://doi.org/10.1016/j.jqsrt.2020.107228">https://doi.org/10.1016/j.jqsrt.2020.107228</a>]</p> </blockquote> <strong>Spectroscopic Model</strong> <blockquote> <p><a href="https://exomol.com/models/SO3/32S-16O3/UYT2/">https://exomol.com/models/SO3/32S-16O3/UYT2/</a><br></p> </blockquote> <strong>UYT2: line list</strong> <p><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/SO3/32S-16O3/UYT2<br></p> <blockquote> <p><strong>References:</strong><br> 1. Underwood, D. S., Tennyson, J., Yurchenko, S. N., Clausen, S., Fateev, A., "ExoMol line lists XVII: A line list for hot SO3", Monthly Notices of the Royal Astronomical Society 462, 4300-4313 (2016). <a href="[http://dx.doi.org/10.1093/mnras/stw1828]">[http://dx.doi.org/10.1093/mnras/stw1828]</a>[16UnTeYu.SO3]<br></p> </blockquote> <strong>UYT2: partition function</strong> <p><em>A calculated hot line list for 32S16O3</em><br></p> <blockquote> <p><strong>32S-16O3__UYT2.pf</strong>[24.41 KB]<br>UYT2 partition function, 0-1000 K</p> <p><strong>References:</strong><br> 1. Underwood, D. S., Tennyson, J., Yurchenko, S. N., Clausen, S., Fateev, A., "ExoMol line lists XVII: A line list for hot SO3", Monthly Notices of the Royal Astronomical Society 462, 4300-4313 (2016). <a href="[http://dx.doi.org/10.1093/mnras/stw1828]">[http://dx.doi.org/10.1093/mnras/stw1828]</a>[16UnTeYu.SO3]<br></p> </blockquote> <strong>UYT2: opacity</strong> <p><em>A calculated hot line list for 32S16O3</em><br></p> <blockquote> <p><strong>32S-16O3__UYT2.R1000_0.3-50mu.ktable.ARCiS.fits.gz</strong>[281.45 MB]<br>ARCiS k-tables at R= 1000 (0.3-50mu) in fits format (gzipped): UYT2 (32S)(16O)3 line list.</p> <p><strong>32S-16O3__UYT2.R1000_0.3-50mu.ktable.petitRADTRANS.h5</strong>[370.98 MB]<br>petitRADTRANS k-tables at R= 1000 (0.3-50mu) in HDF5 format: UYT2 (32S)(16O)3 line list.</p> <p><strong>32S-16O3__UYT2.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: UYT2 (32S)(16O)3 line list.</p> <p><strong>32S-16O3__UYT2.R15000_0.3-50mu.xsec.TauREx.h5</strong>[348.39 MB]<br>TauREx k-tables at R= 15000 (0.3-50mu) in HDF5 format: UYT2 (32S)(16O)3 line list.</p> <p><strong>References:</strong><br> 1. Underwood, D. S., Tennyson, J., Yurchenko, S. N., Clausen, S., Fateev, A., "ExoMol line lists XVII: A line list for hot SO3", Monthly Notices of the Royal Astronomical Society 462, 4300-4313 (2016). <a href="[http://dx.doi.org/10.1093/mnras/stw1828]">[http://dx.doi.org/10.1093/mnras/stw1828]</a>[16UnTeYu.SO3]<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). <a href="[http://dx.doi.org/10.1051/0004-6361/202038350]">[http://dx.doi.org/10.1051/0004-6361/202038350]</a>[20ChRoYu.]<br></p> </blockquote>
The OYKYT dataset for 12C1H319F
<p>The dataset is an archive of ExoMol page, https://exomol.com/data/molecules/CH3F/12C-1H3-19F/OYKYT.<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 CH3F_12C1H319F_OYKYT.md for detailed information.</strong> <br></p> <strong>Definitions file</strong> <blockquote> <p><strong>12C-1H3-19F__OYKYT.def</strong>[9.14 KB]<br></p> <p><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). [<a href="https://doi.org/10.1016/j.jqsrt.2020.107228">https://doi.org/10.1016/j.jqsrt.2020.107228</a>]</p> </blockquote> <strong>Spectroscopic Model</strong> <blockquote> <p><a href="https://exomol.com/models/CH3F/12C-1H3-19F/OYKYT/">https://exomol.com/models/CH3F/12C-1H3-19F/OYKYT/</a><br></p> </blockquote> <strong>OYKYT: line list</strong> <p><em>The OYKYT calculated high-temperature water line list of CH3F</em><br></p> <blockquote> <p><strong>12C-1H3-19F__OYKYT__00000-00100.trans.bz2</strong>[30.5 MB]<br>OYKYT (12C)(1H)3(19F) line list transitions: 00000-00100 cm-1</p> <p><strong>12C-1H3-19F__OYKYT__00100-00200.trans.bz2</strong>[33.2 MB]<br>OYKYT (12C)(1H)3(19F) line list transitions: 00100-00200 cm-1</p> <p><strong>12C-1H3-19F__OYKYT__00200-00300.trans.bz2</strong>[34.88 MB]<br>OYKYT (12C)(1H)3(19F) line list transitions: 00200-00300 cm-1</p> <p><strong>12C-1H3-19F__OYKYT__00300-00400.trans.bz2</strong>[36.85 MB]<br>OYKYT (12C)(1H)3(19F) line list transitions: 00300-00400 cm-1</p> <p><strong>12C-1H3-19F__OYKYT__00400-00500.trans.bz2</strong>[39.21 MB]<br>OYKYT (12C)(1H)3(19F) line list transitions: 00400-00500 cm-1</p> <p><strong>12C-1H3-19F__OYKYT__00500-00600.trans.bz2</strong>[42.27 MB]<br>OYKYT (12C)(1H)3(19F) line list transitions: 00500-00600 cm-1</p> <p><strong>12C-1H3-19F__OYKYT__00600-00700.trans.bz2</strong>[45.9 MB]<br>OYKYT (12C)(1H)3(19F) line list transitions: 00600-00700 cm-1</p> <p><strong>12C-1H3-19F__OYKYT__00700-00800.trans.bz2</strong>[52.09 MB]<br>OYKYT (12C)(1H)3(19F) line list transitions: 00700-00800 cm-1</p> <p><strong>12C-1H3-19F__OYKYT__00800-00900.trans.bz2</strong>[60.05 MB]<br>OYKYT (12C)(1H)3(19F) line list transitions: 00800-00900 cm-1</p> <p><strong>12C-1H3-19F__OYKYT__00900-01000.trans.bz2</strong>[70.18 MB]<br>OYKYT (12C)(1H)3(19F) line list transitions: 00900-01000 cm-1</p> <p><strong>12C-1H3-19F__OYKYT__01000-01100.trans.bz2</strong>[82.33 MB]<br>OYKYT (12C)(1H)3(19F) line list transitions: 01000-01100 cm-1</p> <p><strong>12C-1H3-19F__OYKYT__01100-01200.trans.bz2</strong>[87.8 MB]<br>OYKYT (12C)(1H)3(19F) line list transitions: 01100-01200 cm-1</p> <p><strong>12C-1H3-19F__OYKYT__01200-01300.trans.bz2</strong>[94.17 MB]<br>OYKYT (12C)(1H)3(19F) line list transitions: 01200-01300 cm-1</p> <p><strong>12C-1H3-19F__OYKYT__01300-01400.trans.bz2</strong>[103.0 MB]<br>OYKYT (12C)(1H)3(19F) line list transitions: 01300-01400 cm-1</p> <p><strong>12C-1H3-19F__OYKYT__01400-01500.trans.bz2</strong>[112.57 MB]<br>OYKYT (12C)(1H)3(19F) line list transitions: 01400-01500 cm-1</p> <p><strong>12C-1H3-19F__OYKYT__01500-01600.trans.bz2</strong>[118.23 MB]<br>OYKYT (12C)(1H)3(19F) line list transitions: 01500-01600 cm-1</p> <p><strong>12C-1H3-19F__OYKYT__01600-01700.trans.bz2</strong>[121.32 MB]<br>OYKYT (12C)(1H)3(19F) line list transitions: 01600-01700 cm-1</p> <p><strong>12C-1H3-19F__OYKYT__01700-01800.trans.bz2</strong>[126.59 MB]<br>OYKYT (12C)(1H)3(19F) line list transitions: 01700-01800 cm-1</p> <p><strong>12C-1H3-19F__OYKYT__01800-01900.trans.bz2</strong>[134.9 MB]<br>OYKYT (12C)(1H)3(19F) line list transitions: 01800-01900 cm-1</p> <p><strong>12C-1H3-19F__OYKYT__01900-02000.trans.bz2</strong>[144.93 MB]<br>OYKYT (12C)(1H)3(19F) line list transitions: 01900-02000 cm-1</p> <p><strong>12C-1H3-19F__OYKYT__02000-02100.trans.bz2</strong>[158.81 MB]<br>OYKYT (12C)(1H)3(19F) line list transitions: 02000-02100 cm-1</p> <p><strong>12C-1H3-19F__OYKYT__02300-02400.trans.bz2</strong>[193.42 MB]<br>OYKYT (12C)(1H)3(19F) line list transitions: 02300-02400 cm-1</p> <p><strong>12C-1H3-19F__OYKYT__02400-02500.trans.bz2</strong>[214.67 MB]<br>OYKYT (12C)(1H)3(19F) line list transitions: 02400-02500 cm-1</p> <p><strong>12C-1H3-19F__OYKYT__02500-02600.trans.bz2</strong>[244.0 MB]<br>OYKYT (12C)(1H)3(19F) line list transitions: 02500-02600 cm-1</p> <p><strong>12C-1H3-19F__OYKYT__02600-02700.trans.bz2</strong>[268.96 MB]<br>OYKYT (12C)(1H)3(19F) line list transitions: 02600-02700 cm-1</p> <p><strong>12C-1H3-19F__OYKYT__02700-02800.trans.bz2</strong>[296.23 MB]<br>OYKYT (12C)(1H)3(19F) line list transitions: 02700-02800 cm-1</p> <p><strong>12C-1H3-19F__OYKYT__02800-02900.trans.bz2</strong>[332.49 MB]<br>OYKYT (12C)(1H)3(19F) line list transitions: 02800-02900 cm-1</p> <p><strong>12C-1H3-19F__OYKYT__02900-03000.trans.bz2</strong>[356.96 MB]<br>OYKYT (12C)(1H)3(19F) line list transitions: 02900-03000 cm-1</p> <p><strong>12C-1H3-19F__OYKYT__03000-03100.trans.bz2</strong>[365.46 MB]<br>OYKYT (12C)(1H)3(19F) line list transitions: 03000-03100 cm-1</p> <p><strong>12C-1H3-19F__OYKYT__03100-03200.trans.bz2</strong>[369.35 MB]<br>OYKYT (12C)(1H)3(19F) line list transitions: 03100-03200 cm-1</p> <p><strong>12C-1H3-19F__OYKYT__03200-03300.trans.bz2</strong>[373.11 MB]<br>OYKYT (12C)(1H)3(19F) line list transitions: 03200-03300 cm-1</p> <p><strong>12C-1H3-19F__OYKYT__03300-03400.trans.bz2</strong>[390.55 MB]<br>OYKYT (12C)(1H)3(19F) line list transitions: 03300-03400 cm-1</p> <p><strong>12C-1H3-19F__OYKYT__03400-03500.trans.bz2</strong>[422.14 MB]<br>OYKYT (12C)(1H)3(19F) line list transitions: 03400-03500 cm-1</p> <p><strong>12C-1H3-19F__OYKYT__03500-03600.trans.bz2</strong>[451.48 MB]<br>OYKYT (12C)(1H)3(19F) line list transitions: 03500-03600 cm-1</p> <p><strong>12C-1H3-19F__OYKYT__03600-03700.trans.bz2</strong>[490.12 MB]<br>OYKYT (12C)(1H)3(19F) line list transitions: 03600-03700 cm-1</p> <p><strong>12C-1H3-19F__OYKYT__03700-03800.trans.bz2</strong>[542.08 MB]<br>OYKYT (12C)(1H)3(19F) line list transitions: 03700-03800 cm-1</p> <p><strong>12C-1H3-19F__OYKYT__03800-03900.trans.bz2</strong>[599.13 MB]<br>OYKYT (12C)(1H)3(19F) line list transitions: 03800-03900 cm-1</p> <p><strong>12C-1H3-19F__OYKYT__03900-04000.trans.bz2</strong>[654.83 MB]<br>OYKYT (12C)(1H)3(19F) line list transitions: 03900-04000 cm-1</p> <p><strong>12C-1H3-19F__OYKYT__04000-04100.trans.bz2</strong>[706.59 MB]<br>OYKYT (12C)(1H)3(19F) line list transitions: 04000-04100 cm-1</p> <p><strong>12C-1H3-19F__OYKYT__04100-04200.trans.bz2</strong>[753.79 MB]<br>OYKYT (12C)(1H)3(19F) line list transitions: 04100-04200 cm-1</p> <p><strong>12C-1H3-19F__OYKYT__04200-04300.trans.bz2</strong>[801.3 MB]<br>OYKYT (12C)(1H)3(19F) line list transitions: 04200-04300 cm-1</p> <p><strong>12C-1H3-19F__OYKYT__04300-04400.trans.bz2</strong>[855.69 MB]<br>OYKYT (12C)(1H)3(19F) line list transitions: 04300-04400 cm-1</p> <p><strong>12C-1H3-19F__OYKYT__04600-04700.trans.bz2</strong>[704 bytes]<br>OYKYT (12C)(1H)3(19F) line list transitions: 04600-04700 cm-1</p> <p><strong>12C-1H3-19F__OYKYT__04400-04500.trans.bz2</strong>[896.88 MB]<br>OYKYT (12C)(1H)3(19F) line list transitions: 04400-04500 cm-1</p> <p><strong>12C-1H3-19F__OYKYT__04500-04600.trans.bz2</strong>[924.18 MB]<br>OYKYT (12C)(1H)3(19F) line list transitions: 04500-04600 cm-1</p> <p><strong>12C-1H3-19F__OYKYT.states.bz2</strong>[42.02 MB]<br>OYKYT (12C)(1H)3(19F) states</p> <p><strong>12C-1H3-19F__OYKYT__04600-04700.trans.bz2</strong>[704 bytes]<br>OYKYT (12C)(1H)3(19F) line list transitions: 04600-04700 cm-1</p> <p><strong>References:</strong><br> 1. Owens, A., Yachmenev, A., Küpper, J., Yurchenko, S. N., Thiel, W., "The rotation-vibration spectrum of methyl fluoride from first principles", Physical Chemistry Chemical Physics 21, 3496-3505 (2019). <a href="[https://doi.org/10.1039/C8CP01721B]">[https://doi.org/10.1039/C8CP01721B]</a>[19OwYaKu.CH3F]<br></p> </blockquote> <strong>OYKYT: partition function</strong> <p><em>The OYKYT calculated high-temperature water line list of CH3F</em><br></p> <blockquote> <p><strong>12C-1H3-19F__OYKYT.pf</strong>[12.7 KB]<br>partition function of (12C)(1H)3(19F) computed for OYKYT</p> <p><strong>References:</strong><br> 1. Owens, A., Yachmenev, A., Küpper, J., Yurchenko, S. N., Thiel, W., "The rotation-vibration spectrum of methyl fluoride from first principles", Physical Chemistry Chemical Physics 21, 3496-3505 (2019). <a href="[https://doi.org/10.1039/C8CP01721B]">[https://doi.org/10.1039/C8CP01721B]</a>[19OwYaKu.CH3F]<br></p> </blockquote> <strong>OYKYT: opacity</strong> <p><em>The OYKYT calculated high-temperature water line list of CH3F</em><br></p> <blockquote> <p><strong>12C-1H3-19F__OYKYT.R1000_0.3-50mu.ktable.ARCiS.fits.gz</strong>[271.88 MB]<br>ARCiS k-tables at R= 1000 (0.3-50mu) in fits format (gzipped): OYKYT (12C)(1H)3(19F) line list.</p> <p><strong>12C-1H3-19F__OYKYT.R1000_0.3-50mu.ktable.petitRADTRANS.h5</strong>[370.98 MB]<br>petitRADTRANS k-tables at R= 1000 (0.3-50mu) in HDF5 format: OYKYT (12C)(1H)3(19F) line list.</p> <p><strong>12C-1H3-19F__OYKYT.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: OYKYT (12C)(1H)3(19F) line list.</p> <p><strong>12C-1H3-19F__OYKYT.R15000_0.3-50mu.xsec.TauREx.h5</strong>[348.39 MB]<br>TauREx k-tables at R= 15000 (0.3-50mu) in HDF5 format: OYKYT (12C)(1H)3(19F) line list.</p> <p><strong>References:</strong><br> 1. Owens, A., Yachmenev, A., Küpper, J., Yurchenko, S. N., Thiel, W., "The rotation-vibration spectrum of methyl fluoride from first principles", Physical Chemistry Chemical Physics 21, 3496-3505 (2019). <a href="[https://doi.org/10.1039/C8CP01721B]">[https://doi.org/10.1039/C8CP01721B]</a>[19OwYaKu.CH3F]<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). <a href="[http://dx.doi.org/10.1051/0004-6361/202038350]">[http://dx.doi.org/10.1051/0004-6361/202038350]</a>[20ChRoYu.]<br></p> </blockquote>
The ADJSAAM dataset for 4He1H+
<p>The dataset is an archive of ExoMol page, https://exomol.com/data/molecules/HeH_p/4He-1H_p/ADJSAAM.<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 HeH_p_4He1H+_ADJSAAM.md for detailed information.</strong> <br></p> <strong>Definitions file</strong> <blockquote> <p><strong>4He-1H_p__ADJSAAM.def</strong>[4.95 KB]<br></p> <p><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). [<a href="https://doi.org/10.1016/j.jqsrt.2020.107228">https://doi.org/10.1016/j.jqsrt.2020.107228</a>]</p> </blockquote> <strong>Spectroscopic Model</strong> <blockquote> <p><a href="https://exomol.com/models/HeH_p/4He-1H_p/ADJSAAM/">https://exomol.com/models/HeH_p/4He-1H_p/ADJSAAM/</a><br></p> </blockquote> <strong>ADJSAAM: line list</strong> <p><em>Ab initio line list for isotopologues of HD, HD+ and HeH+ by Amaral et al (2019)</em><br></p> <blockquote> <p><strong>4He-1H_p__ADJSAAM.trans.bz2</strong>[15.86 KB]<br>Transition file from the ADJSAAM line list for (4He)(1H)+.</p> <p><strong>4He-1H_p__ADJSAAM.states.bz2</strong>[1.92 KB]<br>Energy (States) file from the ADJSAAM line list for (4He)(1H)+.</p> <p><strong>References:</strong><br> 1. Amaral, P. H. R., Diniz, L.G., Jones, K.A., Stanke, M., Alijah, A., Adamowicz, L., Mohallem, J.R., "Benchmark Rovibrational Linelists and Einstein A-coefficients for the Primordial Molecules and Isotopologues", The Astrophysical Journal 878, 95 (2019). <a href="[https://doi.org/10.3847/1538-4357/ab1f65]">[https://doi.org/10.3847/1538-4357/ab1f65]</a><br></p> </blockquote> <strong>ADJSAAM: partition function</strong> <p><em>Ab initio line list for isotopologues of HD, HD+ and HeH+ by Amaral et al (2019)</em><br></p> <blockquote> <p><strong>4He-1H_p__ADJSAAM.pf</strong>[195.31 KB]<br>Partition function file from the ADJSAAM line list for (4He)(1H)+.</p> <p><strong>References:</strong><br> 1. Amaral, P. H. R., Diniz, L.G., Jones, K.A., Stanke, M., Alijah, A., Adamowicz, L., Mohallem, J.R., "Benchmark Rovibrational Linelists and Einstein A-coefficients for the Primordial Molecules and Isotopologues", The Astrophysical Journal 878, 95 (2019). <a href="[https://doi.org/10.3847/1538-4357/ab1f65]">[https://doi.org/10.3847/1538-4357/ab1f65]</a><br></p> </blockquote> <strong>ADJSAAM: opacity</strong> <p><em>Ab initio line list for isotopologues of HD, HD+ and HeH+ by Amaral et al (2019)</em><br></p> <blockquote> <p><strong>4He-1H_p__ADJSAAM.R1000_0.3-50mu.ktable.ARCiS.fits.gz</strong>[351.92 MB]<br>ARCiS k-tables at R= 1000 (0.3-50mu) in fits format (gzipped): ADJSAAM (4He)(1H)+ line list.</p> <p><strong>4He-1H_p__ADJSAAM.R1000_0.3-50mu.ktable.petitRADTRANS.h5</strong>[370.98 MB]<br>petitRADTRANS k-tables at R= 1000 (0.3-50mu) in HDF5 format: ADJSAAM (4He)(1H)+ line list.</p> <p><strong>4He-1H_p__ADJSAAM.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: ADJSAAM (4He)(1H)+ line list.</p> <p><strong>4He-1H_p__ADJSAAM.R15000_0.3-50mu.xsec.TauREx.h5</strong>[348.39 MB]<br>TauREx k-tables at R= 15000 (0.3-50mu) in HDF5 format: ADJSAAM (4He)(1H)+ line list.</p> <p><strong>References:</strong><br> 1. Amaral, P. H. R., Diniz, L.G., Jones, K.A., Stanke, M., Alijah, A., Adamowicz, L., Mohallem, J.R., "Benchmark Rovibrational Linelists and Einstein A-coefficients for the Primordial Molecules and Isotopologues", The Astrophysical Journal 878, 95 (2019). <a href="[https://doi.org/10.3847/1538-4357/ab1f65]">[https://doi.org/10.3847/1538-4357/ab1f65]</a><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). <a href="[http://dx.doi.org/10.1051/0004-6361/202038350]">[http://dx.doi.org/10.1051/0004-6361/202038350]</a>[20ChRoYu.]<br></p> </blockquote>
The CLT dataset for 7Li1H+
<p>The dataset is an archive of ExoMol page, https://exomol.com/data/molecules/LiH_p/7Li-1H_p/CLT.<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 LiH_p_7Li1H+_CLT.md for detailed information.</strong> <br></p> <strong>Definitions file</strong> <blockquote> <p><strong>7Li-1H_p__CLT.def</strong>[4.65 KB]<br></p> <p><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). [<a href="https://doi.org/10.1016/j.jqsrt.2020.107228">https://doi.org/10.1016/j.jqsrt.2020.107228</a>]</p> </blockquote> <strong>Spectroscopic Model</strong> <blockquote> <p><a href="https://exomol.com/models/LiH_p/7Li-1H_p/CLT/">https://exomol.com/models/LiH_p/7Li-1H_p/CLT/</a><br></p> </blockquote> <strong>CLT: line list</strong> <p><em>The CLT data set for line lists and cooling functions of HD+, LiH and LiH+</em><br></p> <blockquote> <p><strong>7Li-1H_p__CLT.states.bz2</strong>[724 bytes]<br>Energy levels file for the CLT line list for (7Li)(1H)+</p> <p><strong>7Li-1H_p__CLT.trans.bz2</strong>[3.27 KB]<br>Transitions file for the CLT line list for (7Li)(1H)+</p> <p><strong>README.txt</strong>[1.65 KB]<br>Documentation for the CLT data set for (7Li)(1H)+</p> <p><strong>References:</strong><br> 1. Coppola, C. M., Lodi, L., Tennyson, J., "Radiative cooling functions for primordial molecules", Monthly Notices of the Royal Astronomical Society 415, 487-493 (2011). <a href="[http://dx.doi.org/10.1111/j.1365-2966.2011.18723.x]">[http://dx.doi.org/10.1111/j.1365-2966.2011.18723.x]</a>[11CoLiTe.LiH+]<br></p> </blockquote> <strong>CLT: cooling function</strong> <p><strong>NB: These data are not included in current version on Zenodo</strong><br> <strong>Data can be accessed via:</strong> https://exomol.com/data/molecules/LiH_p/7Li-1H_p/CLT<br></p> <strong>CLT: opacity</strong> <p><em>The CLT data set for line lists and cooling functions of HD+, LiH and LiH+</em><br></p> <blockquote> <p><strong>7Li-1H_p__CLT.R1000_0.3-50mu.ktable.ARCiS.fits.gz</strong>[89.44 MB]<br>ARCiS k-tables at R= 1000 (0.3-50mu) in fits format (gzipped): CLT (7Li)(1H)+ line list.</p> <p><strong>7Li-1H_p__CLT.R1000_0.3-50mu.ktable.petitRADTRANS.h5</strong>[370.98 MB]<br>petitRADTRANS k-tables at R= 1000 (0.3-50mu) in HDF5 format: CLT (7Li)(1H)+ line list.</p> <p><strong>7Li-1H_p__CLT.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: CLT (7Li)(1H)+ line list.</p> <p><strong>7Li-1H_p__CLT.R15000_0.3-50mu.xsec.TauREx.h5</strong>[348.39 MB]<br>TauREx k-tables at R= 15000 (0.3-50mu) in HDF5 format: CLT (7Li)(1H)+ line list.</p> <p><strong>References:</strong><br> 1. Coppola, C. M., Lodi, L., Tennyson, J., "Radiative cooling functions for primordial molecules", Monthly Notices of the Royal Astronomical Society 415, 487-493 (2011). <a href="[http://dx.doi.org/10.1111/j.1365-2966.2011.18723.x]">[http://dx.doi.org/10.1111/j.1365-2966.2011.18723.x]</a>[11CoLiTe.LiH+]<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). <a href="[http://dx.doi.org/10.1051/0004-6361/202038350]">[http://dx.doi.org/10.1051/0004-6361/202038350]</a>[20ChRoYu.]<br></p> </blockquote>
The eXeL dataset for 1H316O+
<p>The dataset is an archive of ExoMol page, https://exomol.com/data/molecules/H3O_p/1H3-16O_p/eXeL.<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 H3O_p_1H316O+_eXeL.md for detailed information.</strong> <br></p> <strong>Definitions file</strong> <blockquote> <p><strong>1H3-16O_p__eXeL.def</strong>[10.77 KB]<br></p> <p><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). [<a href="https://doi.org/10.1016/j.jqsrt.2020.107228">https://doi.org/10.1016/j.jqsrt.2020.107228</a>]</p> </blockquote> <strong>Spectroscopic Model</strong> <blockquote> <p><a href="https://exomol.com/models/H3O_p/1H3-16O_p/eXeL/">https://exomol.com/models/H3O_p/1H3-16O_p/eXeL/</a><br></p> </blockquote> <strong>eXeL: line list</strong> <p><em>H3O+ line list eXeL obtained using refined PES and DMS, computed with TROVE</em><br></p> <blockquote> <p><strong>1H3-16O_p__eXeL.states.bz2</strong>[17.72 MB]<br>eXeL (1H)3(16O)+ states</p> <p><strong>1H3-16O_p__eXeL__00000-00100.trans.bz2</strong>[33.37 MB]<br>eXeL eXeL (1H)3(16O)+ line list transitions: 00000-00100 cm-1</p> <p><strong>1H3-16O_p__eXeL__00100-00200.trans.bz2</strong>[22.22 MB]<br>eXeL eXeL (1H)3(16O)+ line list transitions: 00100-00200 cm-1</p> <p><strong>1H3-16O_p__eXeL__00200-00300.trans.bz2</strong>[22.93 MB]<br>eXeL eXeL (1H)3(16O)+ line list transitions: 00200-00300 cm-1</p> <p><strong>1H3-16O_p__eXeL__00300-00400.trans.bz2</strong>[23.69 MB]<br>eXeL eXeL (1H)3(16O)+ line list transitions: 00300-00400 cm-1</p> <p><strong>1H3-16O_p__eXeL__00400-00500.trans.bz2</strong>[24.45 MB]<br>eXeL eXeL (1H)3(16O)+ line list transitions: 00400-00500 cm-1</p> <p><strong>1H3-16O_p__eXeL__00500-00600.trans.bz2</strong>[25.27 MB]<br>eXeL eXeL (1H)3(16O)+ line list transitions: 00500-00600 cm-1</p> <p><strong>1H3-16O_p__eXeL__00600-00700.trans.bz2</strong>[26.11 MB]<br>eXeL eXeL (1H)3(16O)+ line list transitions: 00600-00700 cm-1</p> <p><strong>1H3-16O_p__eXeL__00700-00800.trans.bz2</strong>[27.07 MB]<br>eXeL eXeL (1H)3(16O)+ line list transitions: 00700-00800 cm-1</p> <p><strong>1H3-16O_p__eXeL__00800-00900.trans.bz2</strong>[28.04 MB]<br>eXeL eXeL (1H)3(16O)+ line list transitions: 00800-00900 cm-1</p> <p><strong>1H3-16O_p__eXeL__00900-01000.trans.bz2</strong>[29.08 MB]<br>eXeL eXeL (1H)3(16O)+ line list transitions: 00900-01000 cm-1</p> <p><strong>1H3-16O_p__eXeL__01000-01100.trans.bz2</strong>[30.19 MB]<br>eXeL eXeL (1H)3(16O)+ line list transitions: 01000-01100 cm-1</p> <p><strong>1H3-16O_p__eXeL__01100-01200.trans.bz2</strong>[31.3 MB]<br>eXeL eXeL (1H)3(16O)+ line list transitions: 01100-01200 cm-1</p> <p><strong>1H3-16O_p__eXeL__01200-01300.trans.bz2</strong>[32.54 MB]<br>eXeL eXeL (1H)3(16O)+ line list transitions: 01200-01300 cm-1</p> <p><strong>1H3-16O_p__eXeL__01300-01400.trans.bz2</strong>[33.86 MB]<br>eXeL eXeL (1H)3(16O)+ line list transitions: 01300-01400 cm-1</p> <p><strong>1H3-16O_p__eXeL__01400-01500.trans.bz2</strong>[35.1 MB]<br>eXeL eXeL (1H)3(16O)+ line list transitions: 01400-01500 cm-1</p> <p><strong>1H3-16O_p__eXeL__01500-01600.trans.bz2</strong>[36.39 MB]<br>eXeL eXeL (1H)3(16O)+ line list transitions: 01500-01600 cm-1</p> <p><strong>1H3-16O_p__eXeL__01600-01700.trans.bz2</strong>[37.67 MB]<br>eXeL eXeL (1H)3(16O)+ line list transitions: 01600-01700 cm-1</p> <p><strong>1H3-16O_p__eXeL__01700-01800.trans.bz2</strong>[38.85 MB]<br>eXeL eXeL (1H)3(16O)+ line list transitions: 01700-01800 cm-1</p> <p><strong>1H3-16O_p__eXeL__01800-01900.trans.bz2</strong>[40.01 MB]<br>eXeL eXeL (1H)3(16O)+ line list transitions: 01800-01900 cm-1</p> <p><strong>1H3-16O_p__eXeL__01900-02000.trans.bz2</strong>[41.23 MB]<br>eXeL eXeL (1H)3(16O)+ line list transitions: 01900-02000 cm-1</p> <p><strong>1H3-16O_p__eXeL__02000-02100.trans.bz2</strong>[42.43 MB]<br>eXeL eXeL (1H)3(16O)+ line list transitions: 02000-02100 cm-1</p> <p><strong>1H3-16O_p__eXeL__02100-02200.trans.bz2</strong>[43.64 MB]<br>eXeL eXeL (1H)3(16O)+ line list transitions: 02100-02200 cm-1</p> <p><strong>1H3-16O_p__eXeL__02200-02300.trans.bz2</strong>[44.92 MB]<br>eXeL eXeL (1H)3(16O)+ line list transitions: 02200-02300 cm-1</p> <p><strong>1H3-16O_p__eXeL__02300-02400.trans.bz2</strong>[46.37 MB]<br>eXeL eXeL (1H)3(16O)+ line list transitions: 02300-02400 cm-1</p> <p><strong>1H3-16O_p__eXeL__02400-02500.trans.bz2</strong>[47.84 MB]<br>eXeL eXeL (1H)3(16O)+ line list transitions: 02400-02500 cm-1</p> <p><strong>1H3-16O_p__eXeL__02500-02600.trans.bz2</strong>[49.47 MB]<br>eXeL eXeL (1H)3(16O)+ line list transitions: 02500-02600 cm-1</p> <p><strong>1H3-16O_p__eXeL__02600-02700.trans.bz2</strong>[51.17 MB]<br>eXeL eXeL (1H)3(16O)+ line list transitions: 02600-02700 cm-1</p> <p><strong>1H3-16O_p__eXeL__02700-02800.trans.bz2</strong>[52.94 MB]<br>eXeL eXeL (1H)3(16O)+ line list transitions: 02700-02800 cm-1</p> <p><strong>1H3-16O_p__eXeL__02800-02900.trans.bz2</strong>[54.8 MB]<br>eXeL eXeL (1H)3(16O)+ line list transitions: 02800-02900 cm-1</p> <p><strong>1H3-16O_p__eXeL__02900-03000.trans.bz2</strong>[56.78 MB]<br>eXeL eXeL (1H)3(16O)+ line list transitions: 02900-03000 cm-1</p> <p><strong>1H3-16O_p__eXeL__03000-03100.trans.bz2</strong>[58.76 MB]<br>eXeL eXeL (1H)3(16O)+ line list transitions: 03000-03100 cm-1</p> <p><strong>1H3-16O_p__eXeL__03100-03200.trans.bz2</strong>[60.73 MB]<br>eXeL eXeL (1H)3(16O)+ line list transitions: 03100-03200 cm-1</p> <p><strong>1H3-16O_p__eXeL__03200-03300.trans.bz2</strong>[62.58 MB]<br>eXeL eXeL (1H)3(16O)+ line list transitions: 03200-03300 cm-1</p> <p><strong>1H3-16O_p__eXeL__03300-03400.trans.bz2</strong>[64.38 MB]<br>eXeL eXeL (1H)3(16O)+ line list transitions: 03300-03400 cm-1</p> <p><strong>1H3-16O_p__eXeL__03400-03500.trans.bz2</strong>[66.22 MB]<br>eXeL eXeL (1H)3(16O)+ line list transitions: 03400-03500 cm-1</p> <p><strong>1H3-16O_p__eXeL__03500-03600.trans.bz2</strong>[68.11 MB]<br>eXeL eXeL (1H)3(16O)+ line list transitions: 03500-03600 cm-1</p> <p><strong>1H3-16O_p__eXeL__03600-03700.trans.bz2</strong>[69.98 MB]<br>eXeL eXeL (1H)3(16O)+ line list transitions: 03600-03700 cm-1</p> <p><strong>1H3-16O_p__eXeL__03700-03800.trans.bz2</strong>[71.75 MB]<br>eXeL eXeL (1H)3(16O)+ line list transitions: 03700-03800 cm-1</p> <p><strong>1H3-16O_p__eXeL__03800-03900.trans.bz2</strong>[73.63 MB]<br>eXeL eXeL (1H)3(16O)+ line list transitions: 03800-03900 cm-1</p> <p><strong>1H3-16O_p__eXeL__03900-04000.trans.bz2</strong>[75.62 MB]<br>eXeL eXeL (1H)3(16O)+ line list transitions: 03900-04000 cm-1</p> <p><strong>1H3-16O_p__eXeL__04000-04100.trans.bz2</strong>[77.8 MB]<br>eXeL eXeL (1H)3(16O)+ line list transitions: 04000-04100 cm-1</p> <p><strong>1H3-16O_p__eXeL__04100-04200.trans.bz2</strong>[80.16 MB]<br>eXeL eXeL (1H)3(16O)+ line list transitions: 04100-04200 cm-1</p> <p><strong>1H3-16O_p__eXeL__04200-04300.trans.bz2</strong>[82.61 MB]<br>eXeL eXeL (1H)3(16O)+ line list transitions: 04200-04300 cm-1</p> <p><strong>1H3-16O_p__eXeL__04300-04400.trans.bz2</strong>[85.15 MB]<br>eXeL eXeL (1H)3(16O)+ line list transitions: 04300-04400 cm-1</p> <p><strong>1H3-16O_p__eXeL__04400-04500.trans.bz2</strong>[87.88 MB]<br>eXeL eXeL (1H)3(16O)+ line list transitions: 04400-04500 cm-1</p> <p><strong>1H3-16O_p__eXeL__04500-04600.trans.bz2</strong>[90.66 MB]<br>eXeL eXeL (1H)3(16O)+ line list transitions: 04500-04600 cm-1</p> <p><strong>1H3-16O_p__eXeL__04600-04700.trans.bz2</strong>[93.47 MB]<br>eXeL eXeL (1H)3(16O)+ line list transitions: 04600-04700 cm-1</p> <p><strong>1H3-16O_p__eXeL__04700-04800.trans.bz2</strong>[96.33 MB]<br>eXeL eXeL (1H)3(16O)+ line list transitions: 04700-04800 cm-1</p> <p><strong>1H3-16O_p__eXeL__04800-04900.trans.bz2</strong>[99.07 MB]<br>eXeL eXeL (1H)3(16O)+ line list transitions: 04800-04900 cm-1</p> <p><strong>1H3-16O_p__eXeL__04900-05000.trans.bz2</strong>[101.79 MB]<br>eXeL eXeL (1H)3(16O)+ line list transitions: 04900-05000 cm-1</p> <p><strong>1H3-16O_p__eXeL__05000-05100.trans.bz2</strong>[104.61 MB]<br>eXeL eXeL (1H)3(16O)+ line list transitions: 05000-05100 cm-1</p> <p><strong>1H3-16O_p__eXeL__05100-05200.trans.bz2</strong>[107.54 MB]<br>eXeL eXeL (1H)3(16O)+ line list transitions: 05100-05200 cm-1</p> <p><strong>1H3-16O_p__eXeL__05200-05300.trans.bz2</strong>[110.31 MB]<br>eXeL eXeL (1H)3(16O)+ line list transitions: 05200-05300 cm-1</p> <p><strong>1H3-16O_p__eXeL__05300-05400.trans.bz2</strong>[113.04 MB]<br>eXeL eXeL (1H)3(16O)+ line list transitions: 05300-05400 cm-1</p> <p><strong>1H3-16O_p__eXeL__05400-05500.trans.bz2</strong>[115.86 MB]<br>eXeL eXeL (1H)3(16O)+ line list transitions: 05400-05500 cm-1</p> <p><strong>1H3-16O_p__eXeL__05500-05600.trans.bz2</strong>[118.75 MB]<br>eXeL eXeL (1H)3(16O)+ line list transitions: 05500-05600 cm-1</p> <p><strong>1H3-16O_p__eXeL__05600-05700.trans.bz2</strong>[121.8 MB]<br>eXeL eXeL (1H)3(16O)+ line list transitions: 05600-05700 cm-1</p> <p><strong>1H3-16O_p__eXeL__05700-05800.trans.bz2</strong>[125.06 MB]<br>eXeL eXeL (1H)3(16O)+ line list transitions: 05700-05800 cm-1</p> <p><strong>1H3-16O_p__eXeL__05800-05900.trans.bz2</strong>[128.54 MB]<br>eXeL eXeL (1H)3(16O)+ line list transitions: 05800-05900 cm-1</p> <p><strong>1H3-16O_p__eXeL__05900-06000.trans.bz2</strong>[132.25 MB]<br>eXeL eXeL (1H)3(16O)+ line list transitions: 05900-06000 cm-1</p> <p><strong>1H3-16O_p__eXeL__06000-06100.trans.bz2</strong>[136.23 MB]<br>eXeL eXeL (1H)3(16O)+ line list transitions: 06000-06100 cm-1</p> <p><strong>1H3-16O_p__eXeL__06100-06200.trans.bz2</strong>[140.19 MB]<br>eXeL eXeL (1H)3(16O)+ line list transitions: 06100-06200 cm-1</p> <p><strong>1H3-16O_p__eXeL__06200-06300.trans.bz2</strong>[144.13 MB]<br>eXeL eXeL (1H)3(16O)+ line list transitions: 06200-06300 cm-1</p> <p><strong>1H3-16O_p__eXeL__06300-06400.trans.bz2</strong>[147.94 MB]<br>eXeL eXeL (1H)3(16O)+ line list transitions: 06300-06400 cm-1</p> <p><strong>1H3-16O_p__eXeL__06400-06500.trans.bz2</strong>[151.69 MB]<br>eXeL eXeL (1H)3(16O)+ line list transitions: 06400-06500 cm-1</p> <p><strong>1H3-16O_p__eXeL__06500-06600.trans.bz2</strong>[155.47 MB]<br>eXeL eXeL (1H)3(16O)+ line list transitions: 06500-06600 cm-1</p> <p><strong>1H3-16O_p__eXeL__06600-06700.trans.bz2</strong>[159.47 MB]<br>eXeL eXeL (1H)3(16O)+ line list transitions: 06600-06700 cm-1</p> <p><strong>1H3-16O_p__eXeL__06700-06800.trans.bz2</strong>[163.4 MB]<br>eXeL eXeL (1H)3(16O)+ line list transitions: 06700-06800 cm-1</p> <p><strong>1H3-16O_p__eXeL__06800-06900.trans.bz2</strong>[167.36 MB]<br>eXeL eXeL (1H)3(16O)+ line list transitions: 06800-06900 cm-1</p> <p><strong>1H3-16O_p__eXeL__06900-07000.trans.bz2</strong>[171.27 MB]<br>eXeL eXeL (1H)3(16O)+ line list transitions: 06900-07000 cm-1</p> <p><strong>1H3-16O_p__eXeL__07000-07100.trans.bz2</strong>[175.26 MB]<br>eXeL eXeL (1H)3(16O)+ line list transitions: 07000-07100 cm-1</p> <p><strong>1H3-16O_p__eXeL__07100-07200.trans.bz2</strong>[179.33 MB]<br>eXeL eXeL (1H)3(16O)+ line list transitions: 07100-07200 cm-1</p> <p><strong>1H3-16O_p__eXeL__07200-07300.trans.bz2</strong>[183.26 MB]<br>eXeL eXeL (1H)3(16O)+ line list transitions: 07200-07300 cm-1</p> <p><strong>1H3-16O_p__eXeL__07300-07400.trans.bz2</strong>[187.58 MB]<br>eXeL eXeL (1H)3(16O)+ line list transitions: 07300-07400 cm-1</p> <p><strong>1H3-16O_p__eXeL__07400-07500.trans.bz2</strong>[192.02 MB]<br>eXeL eXeL (1H)3(16O)+ line list transitions: 07400-07500 cm-1</p> <p><strong>1H3-16O_p__eXeL__07500-07600.trans.bz2</strong>[196.82 MB]<br>eXeL eXeL (1H)3(16O)+ line list transitions: 07500-07600 cm-1</p> <p><strong>1H3-16O_p__eXeL__07600-07700.trans.bz2</strong>[201.97 MB]<br>eXeL eXeL (1H)3(16O)+ line list transitions: 07600-07700 cm-1</p> <p><strong>1H3-16O_p__eXeL__07700-07800.trans.bz2</strong>[207.06 MB]<br>eXeL eXeL (1H)3(16O)+ line list transitions: 07700-07800 cm-1</p> <p><strong>1H3-16O_p__eXeL__07800-07900.trans.bz2</strong>[212.24 MB]<br>eXeL eXeL (1H)3(16O)+ line list transitions: 07800-07900 cm-1</p> <p><strong>1H3-16O_p__eXeL__07900-08000.trans.bz2</strong>[217.38 MB]<br>eXeL eXeL (1H)3(16O)+ line list transitions: 07900-08000 cm-1</p> <p><strong>1H3-16O_p__eXeL__08000-08100.trans.bz2</strong>[215.62 MB]<br>eXeL eXeL (1H)3(16O)+ line list transitions: 08000-08100 cm-1</p> <p><strong>1H3-16O_p__eXeL__08100-08200.trans.bz2</strong>[207.44 MB]<br>eXeL eXeL (1H)3(16O)+ line list transitions: 08100-08200 cm-1</p> <p><strong>1H3-16O_p__eXeL__08200-08300.trans.bz2</strong>[199.27 MB]<br>eXeL eXeL (1H)3(16O)+ line list transitions: 08200-08300 cm-1</p> <p><strong>1H3-16O_p__eXeL__08300-08400.trans.bz2</strong>[191.24 MB]<br>eXeL eXeL (1H)3(16O)+ line list transitions: 08300-08400 cm-1</p> <p><strong>1H3-16O_p__eXeL__08400-08500.trans.bz2</strong>[183.1 MB]<br>eXeL eXeL (1H)3(16O)+ line list transitions: 08400-08500 cm-1</p> <p><strong>1H3-16O_p__eXeL__08500-08600.trans.bz2</strong>[175.51 MB]<br>eXeL eXeL (1H)3(16O)+ line list transitions: 08500-08600 cm-1</p> <p><strong>1H3-16O_p__eXeL__08600-08700.trans.bz2</strong>[168.23 MB]<br>eXeL eXeL (1H)3(16O)+ line list transitions: 08600-08700 cm-1</p> <p><strong>1H3-16O_p__eXeL__08700-08800.trans.bz2</strong>[161.06 MB]<br>eXeL eXeL (1H)3(16O)+ line list transitions: 08700-08800 cm-1</p> <p><strong>1H3-16O_p__eXeL__08800-08900.trans.bz2</strong>[154.18 MB]<br>eXeL eXeL (1H)3(16O)+ line list transitions: 08800-08900 cm-1</p> <p><strong>1H3-16O_p__eXeL__08900-09000.trans.bz2</strong>[147.51 MB]<br>eXeL eXeL (1H)3(16O)+ line list transitions: 08900-09000 cm-1</p> <p><strong>1H3-16O_p__eXeL__09000-09100.trans.bz2</strong>[141.06 MB]<br>eXeL eXeL (1H)3(16O)+ line list transitions: 09000-09100 cm-1</p> <p><strong>1H3-16O_p__eXeL__09100-09200.trans.bz2</strong>[135.05 MB]<br>eXeL eXeL (1H)3(16O)+ line list transitions: 09100-09200 cm-1</p> <p><strong>1H3-16O_p__eXeL__09200-09300.trans.bz2</strong>[129.25 MB]<br>eXeL eXeL (1H)3(16O)+ line list transitions: 09200-09300 cm-1</p> <p><strong>1H3-16O_p__eXeL__09300-09400.trans.bz2</strong>[123.7 MB]<br>eXeL eXeL (1H)3(16O)+ line list transitions: 09300-09400 cm-1</p> <p><strong>1H3-16O_p__eXeL__09400-09500.trans.bz2</strong>[118.33 MB]<br>eXeL eXeL (1H)3(16O)+ line list transitions: 09400-09500 cm-1</p> <p><strong>1H3-16O_p__eXeL__09500-09600.trans.bz2</strong>[113.29 MB]<br>eXeL eXeL (1H)3(16O)+ line list transitions: 09500-09600 cm-1</p> <p><strong>1H3-16O_p__eXeL__09600-09700.trans.bz2</strong>[108.18 MB]<br>eXeL eXeL (1H)3(16O)+ line list transitions: 09600-09700 cm-1</p> <p><strong>1H3-16O_p__eXeL__09700-09800.trans.bz2</strong>[103.43 MB]<br>eXeL eXeL (1H)3(16O)+ line list transitions: 09700-09800 cm-1</p> <p><strong>1H3-16O_p__eXeL__09800-09900.trans.bz2</strong>[98.83 MB]<br>eXeL eXeL (1H)3(16O)+ line list transitions: 09800-09900 cm-1</p> <p><strong>1H3-16O_p__eXeL__09900-10000.trans.bz2</strong>[94.36 MB]<br>eXeL eXeL (1H)3(16O)+ line list transitions: 09900-10000 cm-1</p> <p><strong>References:</strong><br> 1. Yurchenko, S. N., Tennyson, J., Miller, S., Melnikov, V. V., O'Donoghue, J., Moore, L., "ExoMol line lists: XL. Rovibrational molecular line list for the hydronium ion (H3O+)", Monthly Notices of the Royal Astronomical Society 497, 2340-2351 (2020). <a href="[https://doi.org/10.1093/mnras/staa2034]">[https://doi.org/10.1093/mnras/staa2034]</a>[20YuTeMi.H3O+]<br></p> </blockquote> <strong>eXeL: partition function</strong> <p><em>H3O+ line list eXeL obtained using refined PES and DMS, computed with TROVE</em><br></p> <blockquote> <p><strong>1H3-16O_p__eXeL.pf</strong>[48.83 KB]<br>eXeL (1H)3(16O)+ Partition function</p> <p><strong>References:</strong><br> 1. Yurchenko, S. N., Tennyson, J., Miller, S., Melnikov, V. V., O'Donoghue, J., Moore, L., "ExoMol line lists: XL. Rovibrational molecular line list for the hydronium ion (H3O+)", Monthly Notices of the Royal Astronomical Society 497, 2340-2351 (2020). <a href="[https://doi.org/10.1093/mnras/staa2034]">[https://doi.org/10.1093/mnras/staa2034]</a>[20YuTeMi.H3O+]<br></p> </blockquote> <strong>eXeL: super-line</strong> <p><strong>NB: These data are not included in current version on Zenodo</strong><br> <strong>Data can be accessed via:</strong> https://exomol.com/data/molecules/H3O_p/1H3-16O_p/eXeL<br></p> <strong>eXeL: opacity</strong> <p><em>H3O+ line list eXeL obtained using refined PES and DMS, computed with TROVE</em><br></p> <blockquote> <p><strong>1H3-16O_p__eXeL.R1000_0.3-50mu.ktable.ARCiS.fits.gz</strong>[338.4 MB]<br>ARCiS k-tables at R= 1000 (0.3-50mu) in fits format (gzipped): eXeL (1H)3(16O)+ line list.</p> <p><strong>1H3-16O_p__eXeL.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: eXeL (1H)3(16O)+ line list.</p> <p><strong>1H3-16O_p__eXeL.R15000_0.3-50mu.xsec.TauREx.h5</strong>[348.39 MB]<br>TauREx k-tables at R= 15000 (0.3-50mu) in HDF5 format: eXeL (1H)3(16O)+ line list.</p> <p><strong>1H3-16O_p__eXeL.R1000_0.3-50mu.ktable.petitRADTRANS.h5</strong>[370.98 MB]<br>petitRADTRANS k-tables at R= 1000 (0.3-50mu) in HDF5 format: eXeL (1H)3(16O)+ line list.</p> <p><strong>References:</strong><br> 1. 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). <a href="[http://dx.doi.org/10.1051/0004-6361/202038350]">[http://dx.doi.org/10.1051/0004-6361/202038350]</a>[20ChRoYu.]<br> 2. Yurchenko, S. N., Tennyson, J., Miller, S., Melnikov, V. V., O'Donoghue, J., Moore, L., "ExoMol line lists: XL. Rovibrational molecular line list for the hydronium ion (H3O+)", Monthly Notices of the Royal Astronomical Society 497, 2340-2351 (2020). <a href="[https://doi.org/10.1093/mnras/staa2034]">[https://doi.org/10.1093/mnras/staa2034]</a>[20YuTeMi.H3O+]<br></p> </blockquote>
The MoLLIST dataset for 16O1H+
<p>The dataset is an archive of ExoMol page, https://exomol.com/data/molecules/OH_p/16O-1H_p/MoLLIST.<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 OH_p_16O1H+_MoLLIST.md for detailed information.</strong> <br></p> <strong>Definitions file</strong> <blockquote> <p><strong>16O-1H_p__MoLLIST.def</strong>[5.7 KB]<br></p> <p><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). [<a href="https://doi.org/10.1016/j.jqsrt.2020.107228">https://doi.org/10.1016/j.jqsrt.2020.107228</a>]</p> </blockquote> <strong>Spectroscopic Model</strong> <blockquote> <p><a href="https://exomol.com/models/OH_p/16O-1H_p/MoLLIST/">https://exomol.com/models/OH_p/16O-1H_p/MoLLIST/</a><br></p> </blockquote> <strong>MoLLIST: line list</strong> <p><em>Empirical Diatomic line lists MoLLIST from Bernath lab (bernath.uwaterloo.ca) in standard ExoMol format [Tennyson and Yurchenko (2016)]</em><br></p> <blockquote> <p><strong>16O-1H_p__MoLLIST.states.bz2</strong>[8.92 KB]<br>MoLLIST (16O)(1H)+ line list: States, compiled by Yixin Wang</p> <p><strong>16O-1H_p__MoLLIST.trans.bz2</strong>[118.86 KB]<br>MoLLIST (16O)(1H)+ line list: Transition file, compiled by Yixin Wang</p> <p><strong>References:</strong><br> 1. Hodges, J. N., Bernath, P. F., "Fourier Transform Spectroscopy of the A3 - X3 Transition of OH+", The astrophysical journal 840, 81-88 (2017). <a href="[http://iopscience.iop.org/article/10.3847/1538-4357/aa6bf5/meta]">[http://iopscience.iop.org/article/10.3847/1538-4357/aa6bf5/meta]</a><br> 2. Bernath, P.F., "MoLLIST: Molecular Line Lists, Intensities and Spectra", Journal of Quantitative Spectroscopy and Radiative Transfer 240, 106687 (2020). <a href="[https://doi.org/10.1016/j.jqsrt.2019.106687]">[https://doi.org/10.1016/j.jqsrt.2019.106687]</a><br></p> </blockquote> <strong>MoLLIST: partition function</strong> <p><em>Empirical Diatomic line lists MoLLIST from Bernath lab (bernath.uwaterloo.ca) in standard ExoMol format [Tennyson and Yurchenko (2016)]</em><br></p> <blockquote> <p><strong>16O-1H_p__MoLLIST.pf</strong>[122.07 KB]<br>MoLLIST (16O)(1H)+ line list: Partition function, compiled by Yixin Wang</p> <p><strong>References:</strong><br> 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). <a href="[http://dx.doi.org/10.1086/190980]">[http://dx.doi.org/10.1086/190980]</a>[84SaTaxx.FeH]<br></p> </blockquote> <strong>MoLLIST: opacity</strong> <p><em>Empirical Diatomic line lists MoLLIST from Bernath lab (bernath.uwaterloo.ca) in standard ExoMol format [Tennyson and Yurchenko (2016)]</em><br></p> <blockquote> <p><strong>16O-1H_p__MoLLIST.R1000_0.3-50mu.ktable.ARCiS.fits.gz</strong>[352.85 MB]<br>ARCiS k-tables at R= 1000 (0.3-50mu) in fits format (gzipped): MoLLIST (16O)(1H)+ line list.</p> <p><strong>16O-1H_p__MoLLIST.R1000_0.3-50mu.ktable.petitRADTRANS.h5</strong>[370.98 MB]<br>petitRADTRANS k-tables at R= 1000 (0.3-50mu) in HDF5 format: MoLLIST (16O)(1H)+ line list.</p> <p><strong>16O-1H_p__MoLLIST.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: MoLLIST (16O)(1H)+ line list.</p> <p><strong>16O-1H_p__MoLLIST.R15000_0.3-50mu.xsec.TauREx.h5</strong>[348.39 MB]<br>TauREx k-tables at R= 15000 (0.3-50mu) in HDF5 format: MoLLIST (16O)(1H)+ line list.</p> <p><strong>References:</strong><br> 1. Hodges, J. N., Bernath, P. F., "Fourier Transform Spectroscopy of the A3 - X3 Transition of OH+", The astrophysical journal 840, 81-88 (2017). <a href="[http://iopscience.iop.org/article/10.3847/1538-4357/aa6bf5/meta]">[http://iopscience.iop.org/article/10.3847/1538-4357/aa6bf5/meta]</a><br> 2. Bernath, P.F., "MoLLIST: Molecular Line Lists, Intensities and Spectra", Journal of Quantitative Spectroscopy and Radiative Transfer 240, 106687 (2020). <a href="[https://doi.org/10.1016/j.jqsrt.2019.106687]">[https://doi.org/10.1016/j.jqsrt.2019.106687]</a><br> 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). <a href="[http://dx.doi.org/10.1051/0004-6361/202038350]">[http://dx.doi.org/10.1051/0004-6361/202038350]</a>[20ChRoYu.]<br></p> </blockquote>
The MoLLIST dataset for 27Al35Cl
<p>The dataset is an archive of ExoMol page, https://exomol.com/data/molecules/AlCl/27Al-35Cl/MoLLIST.<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 AlCl_27Al35Cl_MoLLIST.md for detailed information.</strong> <br></p> <strong>Definitions file</strong> <blockquote> <p><strong>27Al-35Cl__MoLLIST.def</strong>[4.37 KB]<br></p> <p><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). [<a href="https://doi.org/10.1016/j.jqsrt.2020.107228">https://doi.org/10.1016/j.jqsrt.2020.107228</a>]</p> </blockquote> <strong>Spectroscopic Model</strong> <blockquote> <p><a href="https://exomol.com/models/AlCl/27Al-35Cl/MoLLIST/">https://exomol.com/models/AlCl/27Al-35Cl/MoLLIST/</a><br></p> </blockquote> <strong>MoLLIST: line list</strong> <p><em>Empirical Diatomic line lists MoLLIST from Bernath lab (bernath.uwaterloo.ca) in standard ExoMol format [Tennyson and Yurchenko (2016)]</em><br></p> <blockquote> <p><strong>27Al-35Cl__MoLLIST.states.bz2</strong>[28.92 KB]<br>MoLLIST (27Al)(35Cl) line list: States, compiled by Yixin Wang</p> <p><strong>27Al-35Cl__MoLLIST.trans.bz2</strong>[206.98 KB]<br>MoLLIST (27Al)(35Cl) line list: Transition file, compiled by Yixin Wang</p> <p><strong>References:</strong><br> 1. Bernath, P.F., "MoLLIST: Molecular Line Lists, Intensities and Spectra", Journal of Quantitative Spectroscopy and Radiative Transfer 240, 106687 (2020). <a href="[https://doi.org/10.1016/j.jqsrt.2019.106687]">[https://doi.org/10.1016/j.jqsrt.2019.106687]</a><br></p> </blockquote> <strong>MoLLIST: partition function</strong> <p><em>Empirical Diatomic line lists MoLLIST from Bernath lab (bernath.uwaterloo.ca) in standard ExoMol format [Tennyson and Yurchenko (2016)]</em><br></p> <blockquote> <p><strong>27Al-35Cl__MoLLIST.pf</strong>[122.07 KB]<br>MoLLIST (27Al)(37Cl) line list: Partition function, compiled by Yixin Wang</p> <p><strong>References:</strong><br> 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). <a href="[http://dx.doi.org/10.1086/190980]">[http://dx.doi.org/10.1086/190980]</a>[84SaTaxx.FeH]<br></p> </blockquote> <strong>MoLLIST: opacity</strong> <p><em>Empirical Diatomic line lists MoLLIST from Bernath lab (bernath.uwaterloo.ca) in standard ExoMol format [Tennyson and Yurchenko (2016)]</em><br></p> <blockquote> <p><strong>27Al-35Cl__MoLLIST.R1000_0.3-50mu.ktable.ARCiS.fits.gz</strong>[158.16 MB]<br>ARCiS k-tables at R= 1000 (0.3-50mu) in fits format (gzipped): MoLLIST (27Al)(35Cl) line list.</p> <p><strong>27Al-35Cl__MoLLIST.R1000_0.3-50mu.ktable.petitRADTRANS.h5</strong>[370.98 MB]<br>petitRADTRANS k-tables at R= 1000 (0.3-50mu) in HDF5 format: MoLLIST (27Al)(35Cl) line list.</p> <p><strong>27Al-35Cl__MoLLIST.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: MoLLIST (27Al)(35Cl) line list.</p> <p><strong>27Al-35Cl__MoLLIST.R15000_0.3-50mu.xsec.TauREx.h5</strong>[348.39 MB]<br>TauREx k-tables at R= 15000 (0.3-50mu) in HDF5 format: MoLLIST (27Al)(35Cl) line list.</p> <p><strong>References:</strong><br> 1. Bernath, P.F., "MoLLIST: Molecular Line Lists, Intensities and Spectra", Journal of Quantitative Spectroscopy and Radiative Transfer 240, 106687 (2020). <a href="[https://doi.org/10.1016/j.jqsrt.2019.106687]">[https://doi.org/10.1016/j.jqsrt.2019.106687]</a><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). <a href="[http://dx.doi.org/10.1051/0004-6361/202038350]">[http://dx.doi.org/10.1051/0004-6361/202038350]</a>[20ChRoYu.]<br></p> </blockquote>
The CoYuTe dataset for 14N1H3
<p>The dataset is an archive of ExoMol page, https://exomol.com/data/molecules/NH3/14N-1H3/CoYuTe.<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 NH3_14N1H3_CoYuTe.md for detailed information.</strong> <br></p> <strong>Definitions file</strong> <blockquote> <p><strong>14N-1H3__CoYuTe.def</strong>[16.5 KB]<br></p> <p><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). [<a href="https://doi.org/10.1016/j.jqsrt.2020.107228">https://doi.org/10.1016/j.jqsrt.2020.107228</a>]</p> </blockquote> <strong>Spectroscopic Model</strong> <blockquote> <p><a href="https://exomol.com/models/NH3/14N-1H3/CoYuTe/">https://exomol.com/models/NH3/14N-1H3/CoYuTe/</a><br></p> </blockquote> <strong>CoYuTe: line list</strong> <p><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/NH3/14N-1H3/CoYuTe<br></p> <blockquote> <p><strong>References:</strong><br> 1. Al Derzi, A. R., Furtenbacher, T., Tennyson, J., Yurchenko, S. N., Császár, A. G., "MARVEL analysis of the measured high-resolution spectra of 14NH3", unknown journal 161, 117-130 (2015). <a href="[https://doi.org/10.1016/j.jqsrt.2015.03.034]">[https://doi.org/10.1016/j.jqsrt.2015.03.034]</a>[15AlFuTe.NH3]<br> 2. Coles, P. A., Yurchenko, S. N., Tennyson, J., "ExoMol molecular line lists – XXXV. A rotation-vibration line list for hot ammonia", Monthly Notices of the Royal Astronomical Society 490, 4638-4647 (2019). <a href="[https://doi.org/10.1093/mnras/stz2778]">[https://doi.org/10.1093/mnras/stz2778]</a>[19CoYuTe.NH3]<br></p> </blockquote> <strong>CoYuTe: partition function</strong> <p><em>Hot Temperature line list for (14N)(1H)3, 0-20000 cm-1.</em><br></p> <blockquote> <p><strong>14N-1H3__CoYuTe.pf</strong>[48.83 KB]<br>Partition function (T=0-2000K) of the CoYuTe line list for (14N)(1H)3</p> <p><strong>References:</strong><br> 1. Coles, P. A., Yurchenko, S. N., Tennyson, J., "ExoMol molecular line lists – XXXV. A rotation-vibration line list for hot ammonia", Monthly Notices of the Royal Astronomical Society 490, 4638-4647 (2019). <a href="[https://doi.org/10.1093/mnras/stz2778]">[https://doi.org/10.1093/mnras/stz2778]</a>[19CoYuTe.NH3]<br></p> </blockquote> <strong>CoYuTe: super-line</strong> <p><strong>NB: These data are not included in current version on Zenodo</strong><br> <strong>Data can be accessed via:</strong> https://exomol.com/data/molecules/NH3/14N-1H3/CoYuTe<br></p> <strong>CoYuTe: ExoCross input file</strong> <p><strong>NB: These data are not included in current version on Zenodo</strong><br> <strong>Data can be accessed via:</strong> https://exomol.com/data/molecules/NH3/14N-1H3/CoYuTe<br></p> <strong>CoYuTe: opacity</strong> <p><em>Hot Temperature line list for (14N)(1H)3, 0-20000 cm-1.</em><br></p> <blockquote> <p><strong>14N-1H3__CoYuTe.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: CoYuTe (14N)(1H)3 line list.</p> <p><strong>14N-1H3__CoYuTe.R15000_0.3-50mu.xsec.TauREx.h5</strong>[348.39 MB]<br>TauREx cross sections at R= 15000 (0.3-50mu) in HDF5 format: CoYuTe (14N)(1H)3 line list.</p> <p><strong>14N-1H3__CoYuTe.R1000_0.3-50mu.ktable.ARCiS.fits.gz</strong>[397.89 MB]<br>ARCiS k-tables at R= 1000 (0.3-50mu) in fits format (gzipped): CoYuTe (14N)(1H)3 line list.</p> <p><strong>14N-1H3__CoYuTe.R1000_0.3-50mu.ktable.petitRADTRANS.h5</strong>[370.98 MB]<br>petitRADTRANS k-tables at R= 1000 (0.3-50mu) in HDF5 format: CoYuTe (14N)(1H)3 line list.</p> <p><strong>References:</strong><br> 1. Coles, P. A., Yurchenko, S. N., Tennyson, J., "ExoMol molecular line lists – XXXV. A rotation-vibration line list for hot ammonia", Monthly Notices of the Royal Astronomical Society 490, 4638-4647 (2019). <a href="[https://doi.org/10.1093/mnras/stz2778]">[https://doi.org/10.1093/mnras/stz2778]</a>[19CoYuTe.NH3]<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). <a href="[http://dx.doi.org/10.1051/0004-6361/202038350]">[http://dx.doi.org/10.1051/0004-6361/202038350]</a>[20ChRoYu.]<br></p> </blockquote> <strong>CoYuTe: other States files</strong> <p><strong>NB: These data are not included in current version on Zenodo</strong><br> <strong>Data can be accessed via:</strong> https://exomol.com/data/molecules/NH3/14N-1H3/CoYuTe<br></p>
The MoLLIST dataset for 27Al19F
<p>The dataset is an archive of ExoMol page, https://exomol.com/data/molecules/AlF/27Al-19F/MoLLIST.<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 AlF_27Al19F_MoLLIST.md for detailed information.</strong> <br></p> <strong>Definitions file</strong> <blockquote> <p><strong>27Al-19F__MoLLIST.def</strong>[4.37 KB]<br></p> <p><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). [<a href="https://doi.org/10.1016/j.jqsrt.2020.107228">https://doi.org/10.1016/j.jqsrt.2020.107228</a>]</p> </blockquote> <strong>Spectroscopic Model</strong> <blockquote> <p><a href="https://exomol.com/models/AlF/27Al-19F/MoLLIST/">https://exomol.com/models/AlF/27Al-19F/MoLLIST/</a><br></p> </blockquote> <strong>MoLLIST: line list</strong> <p><em>Empirical Diatomic line lists MoLLIST from Bernath lab (bernath.uwaterloo.ca) in standard ExoMol format [Tennyson and Yurchenko (2016)]</em><br></p> <blockquote> <p><strong>27Al-19F__MoLLIST.trans.bz2</strong>[317.85 KB]<br>MoLLIST (27Al)(19F) line list: Transition file, compiled by Yixin Wang</p> <p><strong>27Al-19F__MoLLIST.states.bz2</strong>[29.38 KB]<br>MoLLIST (27Al)(19F) line list: States, compiled by Yixin Wang</p> <p><strong>References:</strong><br> 1. Bernath, P.F., "MoLLIST: Molecular Line Lists, Intensities and Spectra", Journal of Quantitative Spectroscopy and Radiative Transfer 240, 106687 (2020). <a href="[https://doi.org/10.1016/j.jqsrt.2019.106687]">[https://doi.org/10.1016/j.jqsrt.2019.106687]</a><br></p> </blockquote> <strong>MoLLIST: partition function</strong> <p><em>Empirical Diatomic line lists MoLLIST from Bernath lab (bernath.uwaterloo.ca) in standard ExoMol format [Tennyson and Yurchenko (2016)]</em><br></p> <blockquote> <p><strong>27Al-19F__MoLLIST.pf</strong>[122.07 KB]<br>MoLLIST (27Al)(19F) line list: Partition function, compiled by Yixin Wang</p> <p><strong>References:</strong><br> 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). <a href="[http://dx.doi.org/10.1086/190980]">[http://dx.doi.org/10.1086/190980]</a>[84SaTaxx.FeH]<br></p> </blockquote> <strong>MoLLIST: opacity</strong> <p><em>Empirical Diatomic line lists MoLLIST from Bernath lab (bernath.uwaterloo.ca) in standard ExoMol format [Tennyson and Yurchenko (2016)]</em><br></p> <blockquote> <p><strong>27Al-19F__MoLLIST.R1000_0.3-50mu.ktable.ARCiS.fits.gz</strong>[206.18 MB]<br>ARCiS k-tables at R= 1000 (0.3-50mu) in fits format (gzipped): MoLLIST (27Al)(19F) line list.</p> <p><strong>27Al-19F__MoLLIST.R1000_0.3-50mu.ktable.petitRADTRANS.h5</strong>[370.98 MB]<br>petitRADTRANS k-tables at R= 1000 (0.3-50mu) in HDF5 format: MoLLIST (27Al)(19F) line list.</p> <p><strong>27Al-19F__MoLLIST.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: MoLLIST (27Al)(19F) line list.</p> <p><strong>27Al-19F__MoLLIST.R15000_0.3-50mu.xsec.TauREx.h5</strong>[348.39 MB]<br>TauREx k-tables at R= 15000 (0.3-50mu) in HDF5 format: MoLLIST (27Al)(19F) line list.</p> <p><strong>References:</strong><br> 1. Bernath, P.F., "MoLLIST: Molecular Line Lists, Intensities and Spectra", Journal of Quantitative Spectroscopy and Radiative Transfer 240, 106687 (2020). <a href="[https://doi.org/10.1016/j.jqsrt.2019.106687]">[https://doi.org/10.1016/j.jqsrt.2019.106687]</a><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). <a href="[http://dx.doi.org/10.1051/0004-6361/202038350]">[http://dx.doi.org/10.1051/0004-6361/202038350]</a>[20ChRoYu.]<br></p> </blockquote>
The AYTY dataset for 1H212C16O
<p>The dataset is an archive of ExoMol page, https://exomol.com/data/molecules/H2CO/1H2-12C-16O/AYTY.<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 H2CO_1H212C16O_AYTY.md for detailed information.</strong> <br></p> <strong>Definitions file</strong> <blockquote> <p><strong>1H2-12C-16O__AYTY.def</strong>[14.89 KB]<br></p> <p><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). [<a href="https://doi.org/10.1016/j.jqsrt.2020.107228">https://doi.org/10.1016/j.jqsrt.2020.107228</a>]</p> </blockquote> <strong>Spectroscopic Model</strong> <blockquote> <p><a href="https://exomol.com/models/H2CO/1H2-12C-16O/AYTY/">https://exomol.com/models/H2CO/1H2-12C-16O/AYTY/</a><br></p> </blockquote> <strong>AYTY: line list</strong> <p><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/H2CO/1H2-12C-16O/AYTY<br></p> <blockquote> <p><strong>References:</strong><br> 1. Al-Refaie, A. F., Yachmenev, A., Tennyson, J.Yurchenko, S. N., "ExoMol line lists VIII: A variationally computed line list for hot formaldehyde", Monthly Notices of the Royal Astronomical Society 448, 1704-1714 (2015). <a href="[http://dx.doi.org/10.1093/mnras/stv091]">[http://dx.doi.org/10.1093/mnras/stv091]</a>[15AlYaTe.H2CO]<br></p> </blockquote> <strong>AYTY: partition function</strong> <p><em>A variationally computed line list for hot formaldehyde</em><br></p> <blockquote> <p><strong>1H2-12C-16O__AYTY.pf</strong>[25.39 KB]<br>Partition Function for (1H)2(12C)(16O)</p> <p><strong>References:</strong><br> 1. Al-Refaie, A. F., Yachmenev, A., Tennyson, J.Yurchenko, S. N., "ExoMol line lists VIII: A variationally computed line list for hot formaldehyde", Monthly Notices of the Royal Astronomical Society 448, 1704-1714 (2015). <a href="[http://dx.doi.org/10.1093/mnras/stv091]">[http://dx.doi.org/10.1093/mnras/stv091]</a>[15AlYaTe.H2CO]<br></p> </blockquote> <strong>AYTY: opacity</strong> <p><em>A variationally computed line list for hot formaldehyde</em><br></p> <blockquote> <p><strong>1H2-12C-16O__AYTY.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: AYTY (1H)2(12C)(16O) line list.</p> <p><strong>1H2-12C-16O__AYTY.R15000_0.3-50mu.xsec.TauREx.h5</strong>[348.39 MB]<br>TauREx cross sections at R= 15000 (0.3-50mu) in HDF5 format: AYTY (1H)2(12C)(16O) line list.</p> <p><strong>1H2-12C-16O__AYTY.R1000_0.3-50mu.ktable.ARCiS.fits.gz</strong>[337.15 MB]<br>ARCiS k-tables at R= 1000 (0.3-50mu) in fits format (gzipped): AYTY (1H)2(12C)(16O) line list.</p> <p><strong>1H2-12C-16O__AYTY.R1000_0.3-50mu.ktable.petitRADTRANS.h5</strong>[370.98 MB]<br>petitRADTRANS k-tables at R= 1000 (0.3-50mu) in HDF5 format: AYTY (1H)2(12C)(16O) line list.</p> <p><strong>References:</strong><br> 1. Al-Refaie, A. F., Yurchenko, S. N., Yachmenev, A., Tennyson, J., "ExoMol line lists IX: A variationally computed line-list for hot formaldehyde", Monthly Notices of the Royal Astronomical Society 448, 1704-1714 (2015). <a href="[https://doi.org/10.1093/mnras/stv091]">[https://doi.org/10.1093/mnras/stv091]</a>[15AlYuTe.H2CO]<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). <a href="[http://dx.doi.org/10.1051/0004-6361/202038350]">[http://dx.doi.org/10.1051/0004-6361/202038350]</a>[20ChRoYu.]<br></p> </blockquote> <strong>AYTY: other States files</strong> <p><strong>NB: These data are not included in current version on Zenodo</strong><br> <strong>Data can be accessed via:</strong> https://exomol.com/data/molecules/H2CO/1H2-12C-16O/AYTY<br></p>
The MoLLIST dataset for 12C31P
<p>The dataset is an archive of ExoMol page, https://exomol.com/data/molecules/CP/12C-31P/MoLLIST.<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 CP_12C31P_MoLLIST.md for detailed information.</strong> <br></p> <strong>Definitions file</strong> <blockquote> <p><strong>12C-31P__MoLLIST.def</strong>[5.57 KB]<br></p> <p><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). [<a href="https://doi.org/10.1016/j.jqsrt.2020.107228">https://doi.org/10.1016/j.jqsrt.2020.107228</a>]</p> </blockquote> <strong>Spectroscopic Model</strong> <blockquote> <p><a href="https://exomol.com/models/CP/12C-31P/MoLLIST/">https://exomol.com/models/CP/12C-31P/MoLLIST/</a><br></p> </blockquote> <strong>MoLLIST: line list (external)</strong> <p><em>Empirical Diatomic line lists MoLLIST from Bernath lab (bernath.uwaterloo.ca) in standard ExoMol format [Tennyson and Yurchenko (2016)]</em><br></p> <blockquote> <p><strong>CP_README__MoLLIST.txt</strong>[1.63 KB]<br>Documentation for CP external line list of the MoLLIST dataset</p> <p><strong>12C-31P__MoLLIST.states.bz2</strong>[15.45 KB]<br>MoLLIST (12C)(31P) external line list states file</p> <p><strong>12C-31P__MoLLIST.trans.bz2</strong>[271.63 KB]<br>MoLLIST (12C)(31P) external line list transition file</p> <p><strong>References:</strong><br> 1. Ram, R. S., Brooke, J. S. A., Western, C. M., Bernath, P. F., "Einstein A values and oscillator strengths of the A 2Π – X 2Σ+ system of CP", Journal of Quantitative Spectroscopy and Radiative Transfer 138, 107-115 (2014). <a href="[http://dx.doi.org/10.1016/j.jqsrt.2014.01.030]">[http://dx.doi.org/10.1016/j.jqsrt.2014.01.030]</a>[14RaBrWe.CP]<br> 2. Bernath, P.F., "MoLLIST: Molecular Line Lists, Intensities and Spectra", Journal of Quantitative Spectroscopy and Radiative Transfer 240, 106687 (2020). <a href="[https://doi.org/10.1016/j.jqsrt.2019.106687]">[https://doi.org/10.1016/j.jqsrt.2019.106687]</a><br> 3. Qin, Z., Bai, T., Liu, L., "Line lists for the X 2Σ+ - X 2Σ+, A 2Π - A 2Π and A 2Π - X 2Σ+ transitions of CP", Journal of Quantitative Spectroscopy and Radiative Transfer 258, 107352 (2021). <a href="[https://doi.org/10.1016/j.jqsrt.2020.107352]">[https://doi.org/10.1016/j.jqsrt.2020.107352]</a>[21QiBaLi.CP]<br></p> </blockquote> <strong>MoLLIST: partition function (external)</strong> <p><em>Empirical Diatomic line lists MoLLIST from Bernath lab (bernath.uwaterloo.ca) in standard ExoMol format [Tennyson and Yurchenko (2016)]</em><br></p> <blockquote> <p><strong>CP_README__MoLLIST.txt</strong>[1.63 KB]<br>Documentation for CP external line list of the MoLLIST dataset</p> <p><strong>12C-31P__MoLLIST.pf</strong>[7.62 KB]<br>MoLLIST (12C)(31P) external line list partition function</p> <p><strong>References:</strong><br> 1. Ram, R. S., Brooke, J. S. A., Western, C. M., Bernath, P. F., "Einstein A values and oscillator strengths of the A 2Π – X 2Σ+ system of CP", Journal of Quantitative Spectroscopy and Radiative Transfer 138, 107-115 (2014). <a href="[http://dx.doi.org/10.1016/j.jqsrt.2014.01.030]">[http://dx.doi.org/10.1016/j.jqsrt.2014.01.030]</a>[14RaBrWe.CP]<br> 2. Bernath, P.F., "MoLLIST: Molecular Line Lists, Intensities and Spectra", Journal of Quantitative Spectroscopy and Radiative Transfer 240, 106687 (2020). <a href="[https://doi.org/10.1016/j.jqsrt.2019.106687]">[https://doi.org/10.1016/j.jqsrt.2019.106687]</a><br> 3. Qin, Z., Bai, T., Liu, L., "Line lists for the X 2Σ+ - X 2Σ+, A 2Π - A 2Π and A 2Π - X 2Σ+ transitions of CP", Journal of Quantitative Spectroscopy and Radiative Transfer 258, 107352 (2021). <a href="[https://doi.org/10.1016/j.jqsrt.2020.107352]">[https://doi.org/10.1016/j.jqsrt.2020.107352]</a>[21QiBaLi.CP]<br></p> </blockquote> <strong>MoLLIST: opacity</strong> <p><em>Empirical Diatomic line lists MoLLIST from Bernath lab (bernath.uwaterloo.ca) in standard ExoMol format [Tennyson and Yurchenko (2016)]</em><br></p> <blockquote> <p><strong>12C-31P__MoLLIST.R1000_0.3-50mu.ktable.ARCiS.fits.gz</strong>[286.78 MB]<br>ARCiS k-tables at R= 1000 (0.3-50mu) in fits format (gzipped): MoLLIST (12C)(31P) line list.</p> <p><strong>12C-31P__MoLLIST.R1000_0.3-50mu.ktable.petitRADTRANS.h5</strong>[370.98 MB]<br>petitRADTRANS k-tables at R= 1000 (0.3-50mu) in HDF5 format: MoLLIST (12C)(31P) line list.</p> <p><strong>12C-31P__MoLLIST.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: MoLLIST (12C)(31P) line list.</p> <p><strong>12C-31P__MoLLIST.R15000_0.3-50mu.xsec.TauREx.h5</strong>[348.39 MB]<br>TauREx k-tables at R= 15000 (0.3-50mu) in HDF5 format: MoLLIST (12C)(31P) line list.</p> <p><strong>References:</strong><br> 1. Ram, R. S., Brooke, J. S. A., Western, C. M., Bernath, P. F., "Einstein A values and oscillator strengths of the A 2Π – X 2Σ+ system of CP", Journal of Quantitative Spectroscopy and Radiative Transfer 138, 107-115 (2014). <a href="[http://dx.doi.org/10.1016/j.jqsrt.2014.01.030]">[http://dx.doi.org/10.1016/j.jqsrt.2014.01.030]</a>[14RaBrWe.CP]<br> 2. Bernath, P.F., "MoLLIST: Molecular Line Lists, Intensities and Spectra", Journal of Quantitative Spectroscopy and Radiative Transfer 240, 106687 (2020). <a href="[https://doi.org/10.1016/j.jqsrt.2019.106687]">[https://doi.org/10.1016/j.jqsrt.2019.106687]</a><br> 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). <a href="[http://dx.doi.org/10.1051/0004-6361/202038350]">[http://dx.doi.org/10.1051/0004-6361/202038350]</a>[20ChRoYu.]<br></p> </blockquote>
The JnK dataset for 12C32S
<p>The dataset is an archive of ExoMol page, https://exomol.com/data/molecules/CS/12C-32S/JnK.<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 CS_12C32S_JnK.md for detailed information.</strong> <br></p> <strong>Definitions file</strong> <blockquote> <p><strong>12C-32S__JnK.def</strong>[6.85 KB]<br></p> <p><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). [<a href="https://doi.org/10.1016/j.jqsrt.2020.107228">https://doi.org/10.1016/j.jqsrt.2020.107228</a>]</p> </blockquote> <strong>Spectroscopic Model</strong> <blockquote> <p><a href="https://exomol.com/models/CS/12C-32S/JnK/">https://exomol.com/models/CS/12C-32S/JnK/</a><br></p> </blockquote> <strong>JnK: line list</strong> <p><em>Calculated line lists for CS (updated August 2015). Energy levels replaced by experimental values, through the MARVEL procedure where available.</em><br></p> <blockquote> <p><strong>CS__JnK.readme</strong>[2.89 KB]<br>Documentation for calculated line lists of CS.</p> <p><strong>12C-32S__JnK.states.bz2</strong>[118.35 KB]<br>States file for the JnK (12C)(32S) calculated line list.</p> <p><strong>12C-32S__JnK.trans.bz2</strong>[2.25 MB]<br>Transitions file for the JnK (12C)(32S) calculated line list.</p> <p><strong>References:</strong><br> 1. Paulose, G., Barton, E. J., Yurchenko, S. N., Tennyson, J., "ExoMol molecular line lists – XII. Line lists for eight isotopologues of CS", Monthly Notices of the Royal Astronomical Society 454, 1931-1939 (2015). <a href="[http://dx.doi.org/10.1093/mnras/stv1543]">[http://dx.doi.org/10.1093/mnras/stv1543]</a>[15PaBaYu.CS]<br></p> </blockquote> <strong>JnK: partition function</strong> <p><em>Calculated line lists for CS (updated August 2015). Energy levels replaced by experimental values, through the MARVEL procedure where available.</em><br></p> <blockquote> <p><strong>CS__JnK.readme</strong>[2.89 KB]<br>Documentation for calculated line lists of CS.</p> <p><strong>12C-32S__JnK.pf</strong>[73.24 KB]<br>Partition function for (12C)(32S) calculated from the energy levels of the JnK line list.</p> <p><strong>References:</strong><br> 1. Paulose, G., Barton, E. J., Yurchenko, S. N., Tennyson, J., "ExoMol molecular line lists – XII. Line lists for eight isotopologues of CS", Monthly Notices of the Royal Astronomical Society 454, 1931-1939 (2015). <a href="[http://dx.doi.org/10.1093/mnras/stv1543]">[http://dx.doi.org/10.1093/mnras/stv1543]</a>[15PaBaYu.CS]<br></p> </blockquote> <strong>JnK: cross section</strong> <p><strong>NB: These data are not included in current version on Zenodo</strong><br> <strong>Data can be accessed via:</strong> https://exomol.com/data/molecules/CS/12C-32S/JnK<br></p> <strong>JnK: opacity</strong> <p><em>Calculated line lists for CS (updated August 2015). Energy levels replaced by experimental values, through the MARVEL procedure where available.</em><br></p> <blockquote> <p><strong>12C-32S__JnK.R1000_0.3-50mu.ktable.ARCiS.fits.gz</strong>[326.77 MB]<br>ARCiS k-tables at R= 1000 (0.3-50mu) in fits format (gzipped): JnK (12C)(32S) line list.</p> <p><strong>12C-32S__JnK.R1000_0.3-50mu.ktable.petitRADTRANS.h5</strong>[370.98 MB]<br>petitRADTRANS k-tables at R= 1000 (0.3-50mu) in HDF5 format: JnK (12C)(32S) line list.</p> <p><strong>12C-32S__JnK.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: JnK (12C)(32S) line list.</p> <p><strong>12C-32S__JnK.R15000_0.3-50mu.xsec.TauREx.h5</strong>[348.39 MB]<br>TauREx k-tables at R= 15000 (0.3-50mu) in HDF5 format: JnK (12C)(32S) line list.</p> <p><strong>References:</strong><br> 1. Paulose, G., Barton, E. J., Yurchenko, S. N., Tennyson, J., "ExoMol molecular line lists – XII. Line lists for eight isotopologues of CS", Monthly Notices of the Royal Astronomical Society 454, 1931-1939 (2015). <a href="[http://dx.doi.org/10.1093/mnras/stv1543]">[http://dx.doi.org/10.1093/mnras/stv1543]</a>[15PaBaYu.CS]<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). <a href="[http://dx.doi.org/10.1051/0004-6361/202038350]">[http://dx.doi.org/10.1051/0004-6361/202038350]</a>[20ChRoYu.]<br></p> </blockquote>
The Barton dataset for 39K37Cl
<p>The dataset is an archive of ExoMol page, https://exomol.com/data/molecules/KCl/39K-37Cl/Barton.<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 KCl_39K37Cl_Barton.md for detailed information.</strong> <br></p> <strong>Definitions file</strong> <blockquote> <p><strong>39K-37Cl__Barton.def</strong>[4.65 KB]<br></p> <p><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). [<a href="https://doi.org/10.1016/j.jqsrt.2020.107228">https://doi.org/10.1016/j.jqsrt.2020.107228</a>]</p> </blockquote> <strong>Spectroscopic Model</strong> <blockquote> <p><a href="https://exomol.com/models/KCl/39K-37Cl/Barton/">https://exomol.com/models/KCl/39K-37Cl/Barton/</a><br></p> </blockquote> <strong>Barton: line list</strong> <p><em>Calculated line lists for NaCl and KCl</em><br></p> <blockquote> <p><strong>KCl_README__Barton.txt</strong>[1.96 KB]<br>Documentation for the line list and partition function of the Barton KCl data set.</p> <p><strong>39K-37Cl__Barton.states.bz2</strong>[639.74 KB]<br>States file for the Barton (39K)(37Cl) calculated line list.</p> <p><strong>39K-37Cl__Barton.trans.bz2</strong>[14.81 MB]<br>Transitions file for the Barton (39K)(37Cl) calculated line list.</p> <p><strong>References:</strong><br> 1. Barton, E. J., Chui, C., Golpayegani, S., Yurchenko, S. N., Tennyson, J., Frohman, D. J., Bernath, P. F., "ExoMol molecular line lists V: The ro-vibrational spectra of NaCl and KCl", Monthly Notices of the Royal Astronomical Society 442, 1821-1829 (2014). <a href="[http://dx,doi,org/10.1093/mnras/stu944]">[http://dx,doi,org/10.1093/mnras/stu944]</a>[14BaChGo.NaCl]<br></p> </blockquote> <strong>Barton: partition function</strong> <p><em>Calculated line lists for NaCl and KCl</em><br></p> <blockquote> <p><strong>KCl_README__Barton.txt</strong>[1.96 KB]<br>Documentation for the line list and partition function of the Barton KCl data set.</p> <p><strong>39K-37Cl__Barton.pf</strong>[73.24 KB]<br>Partition function for (39K)(37Cl) calculated from the energy levels of the Barton line list.</p> <p><strong>References:</strong><br> 1. Barton, E. J., Chui, C., Golpayegani, S., Yurchenko, S. N., Tennyson, J., Frohman, D. J., Bernath, P. F., "ExoMol molecular line lists V: The ro-vibrational spectra of NaCl and KCl", Monthly Notices of the Royal Astronomical Society 442, 1821-1829 (2014). <a href="[http://dx,doi,org/10.1093/mnras/stu944]">[http://dx,doi,org/10.1093/mnras/stu944]</a>[14BaChGo.NaCl]<br></p> </blockquote>
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