The UCL-4000 dataset for 12C16O2
Authors/Creators
-
Tennyson, J.1
-
Yurchenko, S. N.1
- Al-Refaie, A. F.
- Clark, V. H. J.
-
Chubb, K. L.2
- 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.1
- Wang, Y.
- Wright, S.
- Yurchenko, O. P.
- Mellor, T. M.
- Freedman, R. S.
- Rocchetto, M.1
- Min, M.
- Barstow, J. K.1
- Molliere, P.3
- Al-Refaie, A. F1
- Phillips, M. W.
- 1. University College London
- 2. SRON Netherlands Institute for Space Research
- 3. Max Planck Institute for Astronomy
Description
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.
Spectroscopic Model12C-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]
UCL-4000: line list
UCL hot ro-vibrational line list for Carbon dioxide (CO2).
UCL-4000: partition function12C-16O2__UCL-4000__00000-01000.trans.bz2[307.45 MB]
UCL-4000 (12C)(16O)2 line list transitions: 00000-01000 cm-112C-16O2__UCL-4000__01000-02000.trans.bz2[343.16 MB]
UCL-4000 (12C)(16O)2 line list transitions: 01000-02000 cm-112C-16O2__UCL-4000__02000-03000.trans.bz2[426.2 MB]
UCL-4000 (12C)(16O)2 line list transitions: 02000-03000 cm-112C-16O2__UCL-4000__03000-04000.trans.bz2[513.8 MB]
UCL-4000 (12C)(16O)2 line list transitions: 03000-04000 cm-112C-16O2__UCL-4000__04000-05000.trans.bz2[578.45 MB]
UCL-4000 (12C)(16O)2 line list transitions: 04000-05000 cm-112C-16O2__UCL-4000__05000-06000.trans.bz2[654.58 MB]
UCL-4000 (12C)(16O)2 line list transitions: 05000-06000 cm-112C-16O2__UCL-4000__06000-07000.trans.bz2[748.52 MB]
UCL-4000 (12C)(16O)2 line list transitions: 06000-07000 cm-112C-16O2__UCL-4000__07000-08000.trans.bz2[821.39 MB]
UCL-4000 (12C)(16O)2 line list transitions: 07000-08000 cm-112C-16O2__UCL-4000__08000-09000.trans.bz2[882.7 MB]
UCL-4000 (12C)(16O)2 line list transitions: 08000-09000 cm-112C-16O2__UCL-4000__09000-10000.trans.bz2[951.73 MB]
UCL-4000 (12C)(16O)2 line list transitions: 09000-10000 cm-112C-16O2__UCL-4000__10000-11000.trans.bz2[1022.44 MB]
UCL-4000 (12C)(16O)2 line list transitions: 10000-11000 cm-112C-16O2__UCL-4000__11000-12000.trans.bz2[1.09 GB]
UCL-4000 (12C)(16O)2 line list transitions: 11000-12000 cm-112C-16O2__UCL-4000__12000-13000.trans.bz2[1.23 GB]
UCL-4000 (12C)(16O)2 line list transitions: 12000-13000 cm-112C-16O2__UCL-4000__13000-14000.trans.bz2[1.43 GB]
UCL-4000 (12C)(16O)2 line list transitions: 13000-14000 cm-112C-16O2__UCL-4000__14000-15000.trans.bz2[1.67 GB]
UCL-4000 (12C)(16O)2 line list transitions: 14000-15000 cm-112C-16O2__UCL-4000__15000-16000.trans.bz2[1.92 GB]
UCL-4000 (12C)(16O)2 line list transitions: 15000-16000 cm-112C-16O2__UCL-4000__16000-17000.trans.bz2[2.08 GB]
UCL-4000 (12C)(16O)2 line list transitions: 16000-17000 cm-112C-16O2__UCL-4000__17000-18000.trans.bz2[1.98 GB]
UCL-4000 (12C)(16O)2 line list transitions: 17000-18000 cm-112C-16O2__UCL-4000__18000-19000.trans.bz2[1.73 GB]
UCL-4000 (12C)(16O)2 line list transitions: 18000-19000 cm-112C-16O2__UCL-4000__19000-20000.trans.bz2[1.43 GB]
UCL-4000 (12C)(16O)2 line list transitions: 19000-20000 cm-112C-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 hot ro-vibrational line list for Carbon dioxide (CO2).
UCL-4000: opacity12C-16O2__UCL-4000.pf[122.07 KB]
UCL-4000 (12C)(16O)2 line list Partition function for T=0-5000 KReferences:
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 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]
Files
CO2_12C16O2_UCL-4000.md
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Additional details
Funding
- European Commission
- ExoplANETS A - Exoplanet Athmosphere New Emission Transmission Spectra Analysis 776403
- UK Research and Innovation
- UCL Astrophysics Consolidated Grant 2018-2021 ST/R000476/1
- European Commission
- ExoMolHD - ExoMolHD: Precision spectroscopic data for studies of exoplanets and other hot atmospheres 883830
- European Commission
- EXOMOL - ExoMol: molecular line lists for exoplanet atmospheres 267219
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.]