Magmatic gas delivered by intraplate, hot-spot related volcanism offers important insight into the abundance and distribution of volatiles in the Earth's upper mantle (Aiuppa et al., 2021) and hence into the rates and mechanisms of volatile exchange in and out our planet (Dasgupta & Hirschmann, 2010). Hot-spot magmatic gases have long been recognized (Gerlach, 1982;Symonds et al., 1994) to exbibit CO 2 -richer (and H 2 O-poorer) compositions relative to arc magmatic gases (Fischer, 2008;Fischer & Chiodini, 2015;Oppenheimer et al., 2014;Taran & Zelenski, 2015), attesting for the presence of a carbon-rich mantle reservoir (Aiuppa et al., 2021, and references therein) at depths higher than the shallow (<50 km) Depleted Mantle (DM) sampled by MORBs (Mid-Ocean Ridge Basalts;Hauri et al., 2019). Combined with the specific trace element and radiogenic isotope signatures of hot-spot volcanic rocks (Hoffman, 2003;Zindler & Hart, 1986), the composition of intraplate magmatic gases may thus provide unique information on volatiles' heterogeneities in mantle plumes. Unfortunately, however, the existing data set for hot-spot magmatic gases is still limited (Aiuppa et al., 2021), detailed information being available for only the