ExoMol line lists -- XXXVIII. High-temperature molecular line list of silicon dioxide (SiO)
arXiv:2005.13586 · doi:10.1093/mnras/staa1287
Abstract
Silicon dioxide (SiO) is expected to occur in the atmospheres of hot rocky super-Earth exoplanets but a lack of spectroscopic data is hampering its possible detection. Here, we present the first, comprehensive molecular line list for SiO. The line list, named OYT3, covers the wavenumber range 0\,--\,6000~cm (wavelengths ~m) and is suitable for temperatures up to ~K. Almost 33 billion transitions involving 5.69 million rotation-vibration states with rotational excitation up to have been computed using robust first-principles methodologies. The OYT3 line list is available from the ExoMol database at http://www.exomol.com.
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