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The formation of magmatic oxide ore deposits hosted in chemically-evolved layered gabbroic intrusions is attributed to a variety of petrological processes, but there is little to no consensus on the general applicability of each model. Complicating the matter further is that many layered gabbroic intrusions are spatially and temporally associated with alkaline A-type granites, suggesting that there is a petrogenetic relationship between the two types of chemically different rocks. Our experimental results show that petrological modelling using a starting composition of high-Ti basalt from the Emeishan large igneous province can produce evolved silicic liquids that resemble the compositions of microgranular enclaves from the syenitic unit of the bimodal, oxide ore-bearing Baima igneous complex. The experimental results confirm that bimodal gabbro-granitoid complexes can form from a common parental magma and that early crystallisation of Ti-rich magnetite can explain the formation of the oxide ore deposits in the lower parts of the layered gabbroic intrusions. We conclude that crystallisation of a typical high-Ti basaltic parental magma can produce world-class giant magmatic oxide ore deposits and that the occurrence of some alkaline granites may be an indicator of their presence.CITATION:Shellnutt, J G, Hsia, T W-Y, Liu, T-C and Iizuka, Y, 2015. Cogenetic formation of the peralkaline syenite and oxide ore-bearing layered gabbroic intrusion of the Baima igneous complex, Emeishan large igneous province, south-west China , in Proceedings PACRIM 2015 Congress, pp 317-324 (The Australasian Institute of Mining and Metallurgy: Melbourne).