The Trihybrid dataset for 12C14N

The dataset is an archive of ExoMol page, https://exomol.com/data/molecules/CN/12C-14N/Trihybrid.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 CN_12C14N_Trihybrid.md for detailed information.

Definitions file

12C-14N__Trihybrid.def[7.29 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/CN/12C-14N/Trihybrid/

Trihybrid: partition function

Trihybrid Experimental-Perturbative-Variational line list for CN in standard ExoMol format

12C-14N__Trihybrid.pf[25.39 KB]The partition function of CN, (12C)(14N), obtained using the Trihybrid line list.

References:
1. Syme, A. M., McKemmish, L. K., "Full spectroscopic model and trihybrid experimental perturbation variational line list for CN", Monthly Notices of the Royal Astronomical Society 505, 4383-4395 (2021). [https://doi.org/10.1093/mnras/stab1551][21SyMcxx.CN]

Trihybrid: line list

Trihybrid Experimental-Perturbative-Variational line list for CN in standard ExoMol format

12C-14N__Trihybrid.trans.bz2[10.86 MB]Trihybrid (12C)(14N) external line list transition file.

12C-14N__Trihybrid.states.bz2[522.19 KB]The states file (energy levels list) for the Trihybrid line list for (12C)(14N).

References:
1. Brooke, J. S. A., Ram, R. S., Western, C. M., Li, G., Schwenke, D. W., Bernath, P. F., "Einstein a coefficients and oscillator strengths for the A 2Π-X 2Σ+ (Red) and B 2Σ+ - X 2Σ+ (Violet) systems and rovibrational transitions in the X 2Σ+ state of CN", Astrophysical Journal Supplement Series 210, 23 (2014). [http://dx.doi.org/10.1088/0067-0049/210/2/23][14BrRaWe.CN]
2. Syme, A.-M., McKemmish, L. K., "Experimental energy levels of 12C14N through MARVEL analysis", Monthly Notices of the Royal Astronomical Society 499, 25-39 (2020). [https://doi.org/10.1093/mnras/staa2791][20SyMcxx.CN]
3. Syme, A. M., McKemmish, L. K., "Full spectroscopic model and trihybrid experimental perturbation variational line list for CN", Monthly Notices of the Royal Astronomical Society 505, 4383-4395 (2021). [https://doi.org/10.1093/mnras/stab1551][21SyMcxx.CN]