Powered by OpenAIRE graph
Found an issue? Give us feedback
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/ ZENODOarrow_drop_down
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 . 2016
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 . 2016
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 . 2016
License: CC BY
Data sources: ZENODO
versions View all 2 versions
addClaim

The VOMYT dataset for 51V16O

Authors: Tennyson, J.; Yurchenko, S. N.; Al-Refaie, A. F.; Clark, V. H. J.; Chubb, K. L.; Conway, E. K.; Dewan, A.; +21 Authors

The VOMYT dataset for 51V16O

Abstract

The dataset is an archive of ExoMol page, https://exomol.com/data/molecules/VO/51V-16O/VOMYT.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 VO_51V16O_VOMYT.md for detailed information. Definitions file 51V-16O__VOMYT.def[6.48 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/VO/51V-16O/VOMYT/ VOMYT: partition function New VO Linelist, utilising a spectroscopic model with the 13 lowest electronic states. 51V-16O__VOMYT.pf[203.12 KB]Partition function for (51V)(16O) in the temperature range 1 – 8000 K in 1 K steps from the VOMYT data set. References: 1. McKemmish, L. K., Yurchenko, S. N., Tennyson, J., "ExoMol line lists XVIII – The high temperature spectrum of VO", Monthly Notices of the Royal Astronomical Society 463, 771-793 (2016). [http://dx.doi.org/10.1093/mnras/stw1969][16McYuTe.VO] VOMYT: line list New VO Linelist, utilising a spectroscopic model with the 13 lowest electronic states. 51V-16O__VOMYT.readme[2.24 KB]README documentation for the VOMYT data set for (51V)(16O) 51V-16O__VOMYT.states.bz2[8.27 MB]States file for the VOMYT linelist for (51V)(16O) 51V-16O__VOMYT__00000-05000.trans.bz2[263.74 MB]Transitions file in the region 0 – 5000 cm-1 for the VOMYT linelist for (51V)(16O) 51V-16O__VOMYT__05000-10000.trans.bz2[366.24 MB]Transitions file in the region 5000 – 10000 cm-1 for the VOMYT linelist for (51V)(16O) 51V-16O__VOMYT__10000-15000.trans.bz2[439.65 MB]Transitions file in the region 10000 – 15000 cm-1 for the VOMYT linelist for (51V)(16O) 51V-16O__VOMYT__15000-20000.trans.bz2[503.12 MB]Transitions file in the region 15000 – 20000 cm-1 for the VOMYT linelist for (51V)(16O) 51V-16O__VOMYT__20000-25000.trans.bz2[587.59 MB]Transitions file in the region 20000 – 25000 cm-1 for the VOMYT linelist for (51V)(16O) 51V-16O__VOMYT__25000-30000.trans.bz2[676.67 MB]Transitions file in the region 25000 – 30000 cm-1 for the VOMYT linelist of (51V)(16O) 51V-16O__VOMYT__30000-35000.trans.bz2[452.39 MB]Transitions file in the region 30000 – 35000 cm-1 for the VOMYT linelist for (51V)(16O) References: 1. McKemmish, L. K., Yurchenko, S. N., Tennyson, J., "ExoMol line lists XVIII – The high temperature spectrum of VO", Monthly Notices of the Royal Astronomical Society 463, 771-793 (2016). [http://dx.doi.org/10.1093/mnras/stw1969][16McYuTe.VO] VOMYT: opacity New VO Linelist, utilising a spectroscopic model with the 13 lowest electronic states. 51V-16O__VOMYT.R1000_0.3-50mu.ktable.ARCiS.fits.gz[445.29 MB]ARCiS k-tables at R= 1000 (0.3-50mu) in fits format (gzipped): VOMYT (51V)(16O) line list. 51V-16O__VOMYT.R1000_0.3-50mu.ktable.petitRADTRANS.h5[370.98 MB]petitRADTRANS k-tables at R= 1000 (0.3-50mu) in HDF5 format: VOMYT (51V)(16O) line list. 51V-16O__VOMYT.R1000_0.3-50mu.ktable.NEMESIS.kta[232.01 MB]NEMESIS k-tables at R= 1000 (0.3-50mu) in NEMESIS-kta format: VOMYT (51V)(16O) line list. 51V-16O__VOMYT.R15000_0.3-50mu.xsec.TauREx.h5[348.39 MB]TauREx k-tables at R= 15000 (0.3-50mu) in HDF5 format: VOMYT (51V)(16O) line list. References: 1. McKemmish, L. K., Yurchenko, S. N., Tennyson, J., "ExoMol line lists XVIII – The high temperature spectrum of VO", Monthly Notices of the Royal Astronomical Society 463, 771-793 (2016). [http://dx.doi.org/10.1093/mnras/stw1969][16McYuTe.VO] 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). [http://dx.doi.org/10.1051/0004-6361/202038350][20ChRoYu.]

{"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)\\]", "McKemmish, L. K., Yurchenko, S. N., Tennyson, J., \"ExoMol line lists XVIII \u2013 The high temperature spectrum of VO\", Monthly Notices of the Royal Astronomical Society 463, 771-793 (2016). [http://dx.doi.org/10.1093/mnras/stw1969][16McYuTe.VO]", "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

  • BIP!
    Impact byBIP!
    selected citations
    These citations are derived from selected sources.
    This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
    0
    popularity
    This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
    Average
    influence
    This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
    Average
    impulse
    This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
    Average
    OpenAIRE UsageCounts
    Usage byUsageCounts
    visibility views 2
  • 2
    views
    Powered byOpenAIRE UsageCounts
Powered by OpenAIRE graph
Found an issue? Give us feedback
visibility
selected citations
These citations are derived from selected sources.
This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Citations provided by BIP!
popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
views
OpenAIRE UsageCountsViews provided by UsageCounts
0
Average
Average
Average
2