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• W3098964749 abstract "Context. Ultraviolet (UV) absorption cross sections are an essential ingredient of photochemical atmosphere models. Exoplanet searches have unveiled a large population of short-period objects with hot atmospheres, very different from what we find in our solar system. Transiting exoplanets whose atmospheres can now be studied by transit spectroscopy receive extremely strong UV fluxes and have typical temperatures ranging from 400 to 2500 K. At these temperatures, UV photolysis cross section data are severely lacking." @default.
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• W3098964749 date "2013-03-01" @default.
• W3098964749 modified "2023-10-15" @default.
• W3098964749 title "High-temperature measurements of VUV-absorption cross sections of CO₂and their application to exoplanets" @default.
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• W3098964749 doi "https://doi.org/10.1051/0004-6361/201220945" @default.
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