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ZENODO
Dataset . 2020
License: CC BY
Data sources: Datacite
image/svg+xml art designer at PLoS, modified by Wikipedia users Nina, Beao, JakobVoss, and AnonMoos Open Access logo, converted into svg, designed by PLoS. This version with transparent background. http://commons.wikimedia.org/wiki/File:Open_Access_logo_PLoS_white.svg art designer at PLoS, modified by Wikipedia users Nina, Beao, JakobVoss, and AnonMoos http://www.plos.org/
ZENODO
Dataset . 2020
License: CC BY
Data sources: ZENODO
image/svg+xml art designer at PLoS, modified by Wikipedia users Nina, Beao, JakobVoss, and AnonMoos Open Access logo, converted into svg, designed by PLoS. This version with transparent background. http://commons.wikimedia.org/wiki/File:Open_Access_logo_PLoS_white.svg art designer at PLoS, modified by Wikipedia users Nina, Beao, JakobVoss, and AnonMoos http://www.plos.org/
ZENODO
Dataset . 2020
License: CC BY
Data sources: Datacite
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The UCL-4000 dataset for 12C16O2

Authors: Tennyson, J.; Yurchenko, S. N.; Al-Refaie, A. F.; Clark, V. H. J.; Chubb, K. L.; Conway, E. K.; Dewan, A.; +23 Authors

The UCL-4000 dataset for 12C16O2

Abstract

The dataset is an archive of ExoMol page, https://exomol.com/data/molecules/CO2/12C-16O2/UCL-4000.Please check the reference details according to the following description or directly from the website. 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. Definitions file 12C-16O2__UCL-4000.def[9.47 KB] References: 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] Spectroscopic Model https://exomol.com/models/CO2/12C-16O2/UCL-4000/ UCL-4000: line list UCL hot ro-vibrational line list for Carbon dioxide (CO2). 12C-16O2__UCL-4000__00000-01000.trans.bz2[307.45 MB]UCL-4000 (12C)(16O)2 line list transitions: 00000-01000 cm-1 12C-16O2__UCL-4000__01000-02000.trans.bz2[343.16 MB]UCL-4000 (12C)(16O)2 line list transitions: 01000-02000 cm-1 12C-16O2__UCL-4000__02000-03000.trans.bz2[426.2 MB]UCL-4000 (12C)(16O)2 line list transitions: 02000-03000 cm-1 12C-16O2__UCL-4000__03000-04000.trans.bz2[513.8 MB]UCL-4000 (12C)(16O)2 line list transitions: 03000-04000 cm-1 12C-16O2__UCL-4000__04000-05000.trans.bz2[578.45 MB]UCL-4000 (12C)(16O)2 line list transitions: 04000-05000 cm-1 12C-16O2__UCL-4000__05000-06000.trans.bz2[654.58 MB]UCL-4000 (12C)(16O)2 line list transitions: 05000-06000 cm-1 12C-16O2__UCL-4000__06000-07000.trans.bz2[748.52 MB]UCL-4000 (12C)(16O)2 line list transitions: 06000-07000 cm-1 12C-16O2__UCL-4000__07000-08000.trans.bz2[821.39 MB]UCL-4000 (12C)(16O)2 line list transitions: 07000-08000 cm-1 12C-16O2__UCL-4000__08000-09000.trans.bz2[882.7 MB]UCL-4000 (12C)(16O)2 line list transitions: 08000-09000 cm-1 12C-16O2__UCL-4000__09000-10000.trans.bz2[951.73 MB]UCL-4000 (12C)(16O)2 line list transitions: 09000-10000 cm-1 12C-16O2__UCL-4000__10000-11000.trans.bz2[1022.44 MB]UCL-4000 (12C)(16O)2 line list transitions: 10000-11000 cm-1 12C-16O2__UCL-4000__11000-12000.trans.bz2[1.09 GB]UCL-4000 (12C)(16O)2 line list transitions: 11000-12000 cm-1 12C-16O2__UCL-4000__12000-13000.trans.bz2[1.23 GB]UCL-4000 (12C)(16O)2 line list transitions: 12000-13000 cm-1 12C-16O2__UCL-4000__13000-14000.trans.bz2[1.43 GB]UCL-4000 (12C)(16O)2 line list transitions: 13000-14000 cm-1 12C-16O2__UCL-4000__14000-15000.trans.bz2[1.67 GB]UCL-4000 (12C)(16O)2 line list transitions: 14000-15000 cm-1 12C-16O2__UCL-4000__15000-16000.trans.bz2[1.92 GB]UCL-4000 (12C)(16O)2 line list transitions: 15000-16000 cm-1 12C-16O2__UCL-4000__16000-17000.trans.bz2[2.08 GB]UCL-4000 (12C)(16O)2 line list transitions: 16000-17000 cm-1 12C-16O2__UCL-4000__17000-18000.trans.bz2[1.98 GB]UCL-4000 (12C)(16O)2 line list transitions: 17000-18000 cm-1 12C-16O2__UCL-4000__18000-19000.trans.bz2[1.73 GB]UCL-4000 (12C)(16O)2 line list transitions: 18000-19000 cm-1 12C-16O2__UCL-4000__19000-20000.trans.bz2[1.43 GB]UCL-4000 (12C)(16O)2 line list transitions: 19000-20000 cm-1 12C-16O2__UCL-4000.states.bz2[56.98 MB]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. References: 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] UCL-4000: partition function UCL hot ro-vibrational line list for Carbon dioxide (CO2). 12C-16O2__UCL-4000.pf[122.07 KB]UCL-4000 (12C)(16O)2 line list Partition function for T=0-5000 K References: 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] UCL-4000: opacity UCL hot ro-vibrational line list for Carbon dioxide (CO2). 12C-16O2__UCL-4000.R1000_0.3-50mu.ktable.ARCiS.fits.gz[402.28 MB]ARCiS k-tables at R= 1000 (0.3-50mu) in fits format (gzipped): UCL-4000 (12C)(16O)2 line list. 12C-16O2__UCL-4000.R1000_0.3-50mu.ktable.petitRADTRANS.h5[370.98 MB]petitRADTRANS k-tables at R= 1000 (0.3-50mu) in HDF5 format: UCL-4000 (12C)(16O)2 line list. 12C-16O2__UCL-4000.R1000_0.3-50mu.ktable.NEMESIS.kta[232.01 MB]NEMESIS k-tables at R= 1000 (0.3-50mu) in NEMESIS-kta format: UCL-4000 (12C)(16O)2 line list. 12C-16O2__UCL-4000.R15000_0.3-50mu.xsec.TauREx.h5[348.39 MB]TauREx k-tables at R= 15000 (0.3-50mu) in HDF5 format: UCL-4000 (12C)(16O)2 line list. References: 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.] 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]

{"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.]"]}

Keywords

ExoMolOP, ExoMol, partition function, opacity, line list

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This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
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