Cross section data for 48Ti1H

Reminder: the cross sections provided by this page are calculated at zero-pressure (i.e. Doppler-broadened lines only). If you enter your email address below it will only be used to inform you of fixes to the service in case it fails. Alternatively, please email christian.hill@ucl.ac.uk.

The default format of the .sigma data file is a single column of cross section points (in cm2/molec), one for each wavenumber bin selected, starting at νmin and spaced by Δν. Select two-column output below if you want each cross section point preceded explicitly by the wavenumber at the centre of the bin it applies to.

Online absorption cross section service: this cross section has been generated from the line lists MoLLIST by P. F. Bernath [Burrows et al. (2005)] for the ExoMol project [Tennyson and Yurchenko (2012)] using the procedure described in [Hill et al. (2013)].

References

  1. Hill, C., Yurchenko, S. N., Tennyson, J., "Temperature-dependent molecular absorption cross sections for exoplanets and other atmospheres", Icarus 226, 1673-1677 (2013). [link to article][13HiYuTe.SO2]
  2. Tennyson, J., Yurchenko, S. N., "ExoMol: molecular line lists for exoplanet and other atmospheres", Monthly Notices of the Royal Astronomical Society 425, 21-33 (2012). [link to article][12TeYuxx]
  3. Burrows, A., Dulick, M., Bauschlicher, C. W., Bernath, P. F., Ram, R. S., Sharp, C. M., Milsom, J. A., "Spectroscopic constants, abundances, and opacities of the TiH molecule", Astrophysical Journal 624, 988-1002 (2005). [link to article][05BuDuBa.TiH]