DOI: 10.5281/zenodo.5716785
title: The UCL-4000 dataset for 12C16O2

description: The dataset is an archive of ExoMol page, https://exomol.com/data/molecules/CO2/12C-16O2/UCL-4000.<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 CO2_12C16O2_UCL-4000.md for detailed information.</strong> <br> <strong>Definitions file</strong> <strong>12C-16O2__UCL-4000.def</strong>[9.47 KB]<br> <strong>References:</strong><br> 1. Tennyson, J., Yurchenko, S. N., Al-Refaie, A. F., Clark, V. H. J., Chubb, K. L., Conway, E. K., Dewan, A., Gorman, M. N., Hill, C., Lynas-Gray, A. E., Mellor, T., McKemmish, L. K., Owens, A., Polyansky, O. L., Semenov, M., Somogyi, W., Tinetti, G., Upadhyay, A., Waldmann, I., Wang, Y., Wright, S., Yurchenko, O. P., "The 2020 release of the ExoMol database: molecular line lists for exoplanet and other hot atmospheres", J. Quant. Spectrosc. Rad. Transf., 255, 107228 (2020). [https://doi.org/10.1016/j.jqsrt.2020.107228] <strong>Spectroscopic Model</strong> https://exomol.com/models/CO2/12C-16O2/UCL-4000/<br> <strong>UCL-4000: line list</strong> <em>UCL hot ro-vibrational line list for Carbon dioxide (CO2).</em><br> <strong>12C-16O2__UCL-4000__00000-01000.trans.bz2</strong>[307.45 MB]<br>UCL-4000 (12C)(16O)2 line list transitions: 00000-01000 cm-1 <strong>12C-16O2__UCL-4000__01000-02000.trans.bz2</strong>[343.16 MB]<br>UCL-4000 (12C)(16O)2 line list transitions: 01000-02000 cm-1 <strong>12C-16O2__UCL-4000__02000-03000.trans.bz2</strong>[426.2 MB]<br>UCL-4000 (12C)(16O)2 line list transitions: 02000-03000 cm-1 <strong>12C-16O2__UCL-4000__03000-04000.trans.bz2</strong>[513.8 MB]<br>UCL-4000 (12C)(16O)2 line list transitions: 03000-04000 cm-1 <strong>12C-16O2__UCL-4000__04000-05000.trans.bz2</strong>[578.45 MB]<br>UCL-4000 (12C)(16O)2 line list transitions: 04000-05000 cm-1 <strong>12C-16O2__UCL-4000__05000-06000.trans.bz2</strong>[654.58 MB]<br>UCL-4000 (12C)(16O)2 line list transitions: 05000-06000 cm-1 <strong>12C-16O2__UCL-4000__06000-07000.trans.bz2</strong>[748.52 MB]<br>UCL-4000 (12C)(16O)2 line list transitions: 06000-07000 cm-1 <strong>12C-16O2__UCL-4000__07000-08000.trans.bz2</strong>[821.39 MB]<br>UCL-4000 (12C)(16O)2 line list transitions: 07000-08000 cm-1 <strong>12C-16O2__UCL-4000__08000-09000.trans.bz2</strong>[882.7 MB]<br>UCL-4000 (12C)(16O)2 line list transitions: 08000-09000 cm-1 <strong>12C-16O2__UCL-4000__09000-10000.trans.bz2</strong>[951.73 MB]<br>UCL-4000 (12C)(16O)2 line list transitions: 09000-10000 cm-1 <strong>12C-16O2__UCL-4000__10000-11000.trans.bz2</strong>[1022.44 MB]<br>UCL-4000 (12C)(16O)2 line list transitions: 10000-11000 cm-1 <strong>12C-16O2__UCL-4000__11000-12000.trans.bz2</strong>[1.09 GB]<br>UCL-4000 (12C)(16O)2 line list transitions: 11000-12000 cm-1 <strong>12C-16O2__UCL-4000__12000-13000.trans.bz2</strong>[1.23 GB]<br>UCL-4000 (12C)(16O)2 line list transitions: 12000-13000 cm-1 <strong>12C-16O2__UCL-4000__13000-14000.trans.bz2</strong>[1.43 GB]<br>UCL-4000 (12C)(16O)2 line list transitions: 13000-14000 cm-1 <strong>12C-16O2__UCL-4000__14000-15000.trans.bz2</strong>[1.67 GB]<br>UCL-4000 (12C)(16O)2 line list transitions: 14000-15000 cm-1 <strong>12C-16O2__UCL-4000__15000-16000.trans.bz2</strong>[1.92 GB]<br>UCL-4000 (12C)(16O)2 line list transitions: 15000-16000 cm-1 <strong>12C-16O2__UCL-4000__16000-17000.trans.bz2</strong>[2.08 GB]<br>UCL-4000 (12C)(16O)2 line list transitions: 16000-17000 cm-1 <strong>12C-16O2__UCL-4000__17000-18000.trans.bz2</strong>[1.98 GB]<br>UCL-4000 (12C)(16O)2 line list transitions: 17000-18000 cm-1 <strong>12C-16O2__UCL-4000__18000-19000.trans.bz2</strong>[1.73 GB]<br>UCL-4000 (12C)(16O)2 line list transitions: 18000-19000 cm-1 <strong>12C-16O2__UCL-4000__19000-20000.trans.bz2</strong>[1.43 GB]<br>UCL-4000 (12C)(16O)2 line list transitions: 19000-20000 cm-1 <strong>12C-16O2__UCL-4000.states.bz2</strong>[56.98 MB]<br>UCL-4000 (12C)(16O)2 line list States. 18957 Calculated (Ca) energy levels were replaced with more accurate HITRAN2020 (HI) values. Uncertainties are provided both for Ca and HI. <strong>References:</strong><br> 1. Yurchenko, S. N., Mellor, T. M., Freedman, R. S., Tennyson, J., "ExoMol line lists -- XXXIX. Ro-vibrational molecular line list for CO2", Monthly Notices of the Royal Astronomical Society 496, 5282-5291 (2020). [https://doi.org/10.1093/mnras/staa1874][20YuMeFr.CO2]<br> <strong>UCL-4000: partition function</strong> <em>UCL hot ro-vibrational line list for Carbon dioxide (CO2).</em><br> <strong>12C-16O2__UCL-4000.pf</strong>[122.07 KB]<br>UCL-4000 (12C)(16O)2 line list Partition function for T=0-5000 K <strong>References:</strong><br> 1. Yurchenko, S. N., Mellor, T. M., Freedman, R. S., Tennyson, J., "ExoMol line lists -- XXXIX. Ro-vibrational molecular line list for CO2", Monthly Notices of the Royal Astronomical Society 496, 5282-5291 (2020). [https://doi.org/10.1093/mnras/staa1874][20YuMeFr.CO2]<br> <strong>UCL-4000: opacity</strong> <em>UCL hot ro-vibrational line list for Carbon dioxide (CO2).</em><br> <strong>12C-16O2__UCL-4000.R1000_0.3-50mu.ktable.ARCiS.fits.gz</strong>[402.28 MB]<br>ARCiS k-tables at R= 1000 (0.3-50mu) in fits format (gzipped): UCL-4000 (12C)(16O)2 line list. <strong>12C-16O2__UCL-4000.R1000_0.3-50mu.ktable.petitRADTRANS.h5</strong>[370.98 MB]<br>petitRADTRANS k-tables at R= 1000 (0.3-50mu) in HDF5 format: UCL-4000 (12C)(16O)2 line list. <strong>12C-16O2__UCL-4000.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: UCL-4000 (12C)(16O)2 line list. <strong>12C-16O2__UCL-4000.R15000_0.3-50mu.xsec.TauREx.h5</strong>[348.39 MB]<br>TauREx k-tables at R= 15000 (0.3-50mu) in HDF5 format: UCL-4000 (12C)(16O)2 line list. <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). [http://dx.doi.org/10.1051/0004-6361/202038350][20ChRoYu.]<br> 2. Yurchenko, S. N., Mellor, T. M., Freedman, R. S., Tennyson, J., "ExoMol line lists -- XXXIX. Ro-vibrational molecular line list for CO2", Monthly Notices of the Royal Astronomical Society 496, 5282-5291 (2020). [https://doi.org/10.1093/mnras/staa1874][20YuMeFr.CO2]<br>
description: {"references": ["Tennyson, J., Yurchenko, S. N., Al-Refaie, A. F., Clark, V. H. J., Chubb, K. L., Conway, E. K., Dewan, A., Gorman, M. N., Hill, C., Lynas-Gray, A. E., Mellor, T., McKemmish, L. K., Owens, A., Polyansky, O. L., Semenov, M., Somogyi, W., Tinetti, G., Upadhyay, A., Waldmann, I., Wang, Y., Wright, S., Yurchenko, O. P., \"The 2020 release of the ExoMol database: molecular line lists for exoplanet and other hot atmospheres\", J. Quant. Spectrosc. Rad. Transf., 255, 107228 (2020). \\[[https://doi.org/10.1016/j.jqsrt.2020.107228](https://doi.org/10.1016/j.jqsrt.2020.107228)\\]", "Yurchenko, S. N., Mellor, T. M., Freedman, R. S., Tennyson, J., \"ExoMol line lists -- XXXIX. Ro-vibrational molecular line list for CO2\", Monthly Notices of the Royal Astronomical Society 496, 5282-5291 (2020). [https://doi.org/10.1093/mnras/staa1874][20YuMeFr.CO2]", "Chubb, K. L., Rocchetto, M., Yurchenko, S. N., Min, M., Waldmann, I., Barstow, J. K., Molliere, P., Al-Refaie, A. F, Phillips, M. W., Tennyson, J., \"The ExoMolOP database: Cross sections and k-tables for molecules of interest in high-temperature exoplanet atmospheres\", Astronomy and Astrophysics 646, A21 (2020). [http://dx.doi.org/10.1051/0004-6361/202038350][20ChRoYu.]"]}