DOI: 10.5281/zenodo.5716763
title: The VOMYT dataset for 51V16O

description: The dataset is an archive of ExoMol page, https://exomol.com/data/molecules/VO/51V-16O/VOMYT.<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 VO_51V16O_VOMYT.md for detailed information.</strong> <br> <strong>Definitions file</strong> <strong>51V-16O__VOMYT.def</strong>[6.48 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/VO/51V-16O/VOMYT/<br> <strong>VOMYT: partition function</strong> <em>New VO Linelist, utilising a spectroscopic model with the 13 lowest electronic states.</em><br> <strong>51V-16O__VOMYT.pf</strong>[203.12 KB]<br>Partition function for (51V)(16O) in the temperature range 1 – 8000 K in 1 K steps from the VOMYT data set. <strong>References:</strong><br> 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]<br> <strong>VOMYT: line list</strong> <em>New VO Linelist, utilising a spectroscopic model with the 13 lowest electronic states.</em><br> <strong>51V-16O__VOMYT.readme</strong>[2.24 KB]<br>README documentation for the VOMYT data set for (51V)(16O) <strong>51V-16O__VOMYT.states.bz2</strong>[8.27 MB]<br>States file for the VOMYT linelist for (51V)(16O) <strong>51V-16O__VOMYT__00000-05000.trans.bz2</strong>[263.74 MB]<br>Transitions file in the region 0 – 5000 cm-1 for the VOMYT linelist for (51V)(16O) <strong>51V-16O__VOMYT__05000-10000.trans.bz2</strong>[366.24 MB]<br>Transitions file in the region 5000 – 10000 cm-1 for the VOMYT linelist for (51V)(16O) <strong>51V-16O__VOMYT__10000-15000.trans.bz2</strong>[439.65 MB]<br>Transitions file in the region 10000 – 15000 cm-1 for the VOMYT linelist for (51V)(16O) <strong>51V-16O__VOMYT__15000-20000.trans.bz2</strong>[503.12 MB]<br>Transitions file in the region 15000 – 20000 cm-1 for the VOMYT linelist for (51V)(16O) <strong>51V-16O__VOMYT__20000-25000.trans.bz2</strong>[587.59 MB]<br>Transitions file in the region 20000 – 25000 cm-1 for the VOMYT linelist for (51V)(16O) <strong>51V-16O__VOMYT__25000-30000.trans.bz2</strong>[676.67 MB]<br>Transitions file in the region 25000 – 30000 cm-1 for the VOMYT linelist of (51V)(16O) <strong>51V-16O__VOMYT__30000-35000.trans.bz2</strong>[452.39 MB]<br>Transitions file in the region 30000 – 35000 cm-1 for the VOMYT linelist for (51V)(16O) <strong>References:</strong><br> 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]<br> <strong>VOMYT: opacity</strong> <em>New VO Linelist, utilising a spectroscopic model with the 13 lowest electronic states.</em><br> <strong>51V-16O__VOMYT.R1000_0.3-50mu.ktable.ARCiS.fits.gz</strong>[445.29 MB]<br>ARCiS k-tables at R= 1000 (0.3-50mu) in fits format (gzipped): VOMYT (51V)(16O) line list. <strong>51V-16O__VOMYT.R1000_0.3-50mu.ktable.petitRADTRANS.h5</strong>[370.98 MB]<br>petitRADTRANS k-tables at R= 1000 (0.3-50mu) in HDF5 format: VOMYT (51V)(16O) line list. <strong>51V-16O__VOMYT.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: VOMYT (51V)(16O) line list. <strong>51V-16O__VOMYT.R15000_0.3-50mu.xsec.TauREx.h5</strong>[348.39 MB]<br>TauREx k-tables at R= 15000 (0.3-50mu) in HDF5 format: VOMYT (51V)(16O) line list. <strong>References:</strong><br> 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]<br> 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.]<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)\\]", "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.]"]}