The RACPPK dataset for 1H2: cooling functions
RACPPK: line list
A line list for the ground electronic state of H2 by Roueff et al (2019): The Einstein coefficients are the sum of the dipole and quadrupole contributions.
- 1H2__RACPPK.states.bz2
States of H2 from RACPPK dataset: ground electronic system. The energy term values are defined relative to the X1Sigma,v=0,J=0 state. The dissociation energy of the triplet is 36118.0695 cm-1, ZPE=155.52687 cm-1.
- 1H2__RACPPK.trans.bz2
Transition file for H2 from the RACPPK dataset: ground electronic system.
References
- Roueff, E., Abgrall, H., Czachorowski, P., Pachucki, K., Puchalski, M., Komasa, J., "The full infrared spectrum of molecular hydrogen", Astronomy and Astrophysics 630, A58 (2019). [link to article][19RoAbCz.H2]
- Roueff, E., Abgrall, H., Czachorowski, P., Pachucki, K., Puchalski, M., Komasa, J., "Visier CDSdata: The line list for full infrared spectrum of molecular hydrogen", Visier CDS (2019). [link to article][19RoAbCz1.H2]
RACPPK: partition function
A line list for the ground electronic state of H2 by Roueff et al (2019): The Einstein coefficients are the sum of the dipole and quadrupole contributions.
- 1H2__RACPPK.pf
Partition function of H2 from the RACPPK dataset: ground electronic system.
References
- Roueff, E., Abgrall, H., Czachorowski, P., Pachucki, K., Puchalski, M., Komasa, J., "The full infrared spectrum of molecular hydrogen", Astronomy and Astrophysics 630, A58 (2019). [link to article][19RoAbCz.H2]
RACPPK: Specific heat - heat capacity
A line list for the ground electronic state of H2 by Roueff et al (2019): The Einstein coefficients are the sum of the dipole and quadrupole contributions.
- 1H2__RACPPK.cp
Heat capacity (specific heat) Cp of (1H)2 in 200 K intervals to 10000 K
References
- Roueff, E., Abgrall, H., Czachorowski, P., Pachucki, K., Puchalski, M., Komasa, J., "The full infrared spectrum of molecular hydrogen", Astronomy and Astrophysics 630, A58 (2019). [link to article][19RoAbCz.H2]
RACPPK: cooling function
A line list for the ground electronic state of H2 by Roueff et al (2019): The Einstein coefficients are the sum of the dipole and quadrupole contributions.
- 1H2__RACPPK.cf
RACPPK Cooling function (erg.sr-1.s-1.molec-1) on a grid of 1 K
References
- Yurchenko, S. N., Al-Refaie, A. F., Tennyson, J., "ExoCross: a general program for generating spectra from molecular line lists", Astronomy & Astrophysics 614, A131/1-12 (2018). [link to article][l8YuAlTe.]
- Zhang, J, Tennyson, J., Yurchenko, S.N., "PyExoCross: a Python program for generating spectra and cross sections from molecular line lists", RASTI 3, 257-287 (2024). [link to article]