Published July 19, 2018 | Version 20180719
Dataset Open

The MoLLIST dataset for 16O1H+

Description

The dataset is an archive of ExoMol page, https://exomol.com/data/molecules/OH_p/16O-1H_p/MoLLIST.
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 OH_p_16O1H+_MoLLIST.md for detailed information.

Definitions file

16O-1H_p__MoLLIST.def[5.7 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/OH_p/16O-1H_p/MoLLIST/

MoLLIST: line list

Empirical Diatomic line lists MoLLIST from Bernath lab (bernath.uwaterloo.ca) in standard ExoMol format [Tennyson and Yurchenko (2016)]

16O-1H_p__MoLLIST.states.bz2[8.92 KB]
MoLLIST (16O)(1H)+ line list: States, compiled by Yixin Wang

16O-1H_p__MoLLIST.trans.bz2[118.86 KB]
MoLLIST (16O)(1H)+ line list: Transition file, compiled by Yixin Wang

References:
1. Hodges, J. N., Bernath, P. F., "Fourier Transform Spectroscopy of the A3 - X3 Transition of OH+", The astrophysical journal 840, 81-88 (2017). [http://iopscience.iop.org/article/10.3847/1538-4357/aa6bf5/meta]
2. Bernath, P.F., "MoLLIST: Molecular Line Lists, Intensities and Spectra", Journal of Quantitative Spectroscopy and Radiative Transfer 240, 106687 (2020). [https://doi.org/10.1016/j.jqsrt.2019.106687]

MoLLIST: partition function

Empirical Diatomic line lists MoLLIST from Bernath lab (bernath.uwaterloo.ca) in standard ExoMol format [Tennyson and Yurchenko (2016)]

16O-1H_p__MoLLIST.pf[122.07 KB]
MoLLIST (16O)(1H)+ line list: Partition function, compiled by Yixin Wang

References:
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). [http://dx.doi.org/10.1086/190980][84SaTaxx.FeH]

MoLLIST: opacity

Empirical Diatomic line lists MoLLIST from Bernath lab (bernath.uwaterloo.ca) in standard ExoMol format [Tennyson and Yurchenko (2016)]

16O-1H_p__MoLLIST.R1000_0.3-50mu.ktable.ARCiS.fits.gz[352.85 MB]
ARCiS k-tables at R= 1000 (0.3-50mu) in fits format (gzipped): MoLLIST (16O)(1H)+ line list.

16O-1H_p__MoLLIST.R1000_0.3-50mu.ktable.petitRADTRANS.h5[370.98 MB]
petitRADTRANS k-tables at R= 1000 (0.3-50mu) in HDF5 format: MoLLIST (16O)(1H)+ line list.

16O-1H_p__MoLLIST.R1000_0.3-50mu.ktable.NEMESIS.kta[232.01 MB]
NEMESIS k-tables at R= 1000 (0.3-50mu) in NEMESIS-kta format: MoLLIST (16O)(1H)+ line list.

16O-1H_p__MoLLIST.R15000_0.3-50mu.xsec.TauREx.h5[348.39 MB]
TauREx k-tables at R= 15000 (0.3-50mu) in HDF5 format: MoLLIST (16O)(1H)+ line list.

References:
1. Hodges, J. N., Bernath, P. F., "Fourier Transform Spectroscopy of the A3 - X3 Transition of OH+", The astrophysical journal 840, 81-88 (2017). [http://iopscience.iop.org/article/10.3847/1538-4357/aa6bf5/meta]
2. Bernath, P.F., "MoLLIST: Molecular Line Lists, Intensities and Spectra", Journal of Quantitative Spectroscopy and Radiative Transfer 240, 106687 (2020). [https://doi.org/10.1016/j.jqsrt.2019.106687]
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). [http://dx.doi.org/10.1051/0004-6361/202038350][20ChRoYu.]

Files

OH_p_16O1H+_MoLLIST.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). \[[https://doi.org/10.1016/j.jqsrt.2020.107228](https://doi.org/10.1016/j.jqsrt.2020.107228)\]
  • Hodges, J. N., Bernath, P. F., "Fourier Transform Spectroscopy of the A3 - X3 Transition of OH+", The astrophysical journal 840, 81-88 (2017). [http://iopscience.iop.org/article/10.3847/1538-4357/aa6bf5/meta]
  • Bernath, P.F., "MoLLIST: Molecular Line Lists, Intensities and Spectra", Journal of Quantitative Spectroscopy and Radiative Transfer 240, 106687 (2020). [https://doi.org/10.1016/j.jqsrt.2019.106687]
  • 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). [http://dx.doi.org/10.1086/190980][84SaTaxx.FeH]
  • 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.]