The MPI-Mainz UV/VIS Spectral Atlas

of Gaseous Molecules of Atmospheric Interest

www.uv-vis-spectral-atlas-mainz.org

Hannelore Keller-Rudek1, Geert K. Moortgat2, Rolf Sander2, Rüdiger Sörensen1

1Satellite Group

2Atmospheric Chemistry Division

Max-Planck Institute for Chemistry
Mainz, Germany

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When referring to the Spectral Atlas, please cite our publication:

Keller-Rudek, H., Moortgat, G. K., Sander, R., and Sörensen, R.: The MPI-Mainz UV/VIS spectral atlas of gaseous molecules of atmospheric interest, Earth Syst. Sci. Data, 5, 365–373, (2013), DOI: 10.5194/essd-5-365-2013

Cross Sections / Carbon-oxides / CO2 / Venot(2018)_150K_114.2-178.4nm

DATAFILE: CO2_Venot(2018)_150K_114.2-178.4nm.txt
NAME: carbon dioxide
FORMULA: CO2
AUTHOR(YEAR): Venot(2018)
T: 150K
λ: 114.2-178.4nm
BIBLIOGRAPHY: O. Venot, Y. Bénilan, N. Fray, M.-C. Gazeau, F. Lefèvre, E. Es-sebbar, E. Hébrard, M. Schwell, C. Bahrini, F. Montmessin, M. Lefèvre, I.P. Waldmann, "VUV-absorption cross section of carbon dioxide from 150 to 800 K and applications to warm exoplanetary atmospheres", Astronom. Astrophys. 609, A34 (2018); DOI: 10.1051/0004-6361/201731295
COMMENTS: High-resolution (0.03 nm) absorption measurements using synchrotron radiation as a light source

Absorption cross sections as listed in the Supporting Information

The results presented in the earlier publication of

O. Venot, N. Fray, Y. Bénilan, M.-C. Gazeau, E. Hébrard, G. Larcher, M. Schwell, M. Dobrijevic, and F. Selsis "High-temperature measurements of VUV-absorption cross sections of CO2 and their application to exoplanets", Astronom. Astrophys. 551, A131 (2013); DOI: 10.1051/0004-6361/201220945

have been reevaluated

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