“…The ƒO2 influences key aspects of the SCLM such as melting, composition, speciation of volatiles (e.g., C, H, O) and multivalent elements (e.g., Fe, V, Cr), stability of C-bearing phases (diamond, graphite and carbonates), mineral/melt partitioning, degassing and metal fertility, as demonstrated by several studies (e.g., Mungall, 2002;McCammon and Kopylova, 2004;Frost and McCammon, 2008;Berry et a., 2013;Richards, 2015;Brounce et al, 2015;Yaxley et al, 2012Yaxley et al, , 2017Woodland and Seitz, 2018;Griffin et al, 2018;Aulbach et al, 2019;Tassara et al, 2020;Moretti and Neuville, 2021 and references therein). Most of the information about the redox evolution of the SCLM, ƒO2 mechanisms and distribution comes from experiments (e.g., Ballhaus et al, 1991;Holycross and Cottrell, 2022), quantification via proxies/oxybarometers in mantle-derived rocks such as mid-ocean ridge basalts and peridotites (e.g., V/Sc, Li and Lee, 2004;Lee et al, 2005; garnet and spinel oxybarometers, Miller et al, 2016) and modelling of element-…”