Sulphur-bearing species in the coma of comet 67P/Churyumov–Gerasimenko

By U. Calmonte, K. Altwegg, H. Balsiger, J. Berthelier, A. Bieler, G. Cessateur, F. Dhooghe, E. Dishoeck, B. Fiethe, S. Fuselier and 8 more. 2016

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Organics in comet 67P – a first comparative analysis of mass spectra from ROSINA–DFMS, COSAC and Ptolemy (2017, background): “We note that the absence of a peak around 32 Da does not exclude the existence of sulphur-bearing species as organo-sulphur (CH2S, CH4S, C2H6S) and CS2 fragmentation patterns do not produce significant amounts of S+ (e.g. Calmonte et al. 2016).”
Elemental and molecular abundances in comet 67P/Churyumov-Gerasimenko (2019, methodology): “The same period in 2015 May has been analysed in previous works on the sulphur-bearing species (Calmonte et al. 2016), hydrocarbons and oxygenated compounds (Schuhmann et al. 2019a,b), halogens (Dhooghe et al. 2017), noble gases, and N2 (Rubin et al. 2018).”
Astrochemistry and compositions of planetary systems (2020, background): “In the solar system, the accounting is clearer: C I chondrites contain a nearly solar abundance of S (Lodders 2010), and so does the comet 67P/Churyumov–Gerasimenko Calmonte et al. (2016).”