Replication Data for: Chalcophile elements in Martian meteorites indicate low sulfur content in the Martian interior and a volatile element-depleted late veneer.

• Ratios of Cu, S, Se, Te, Re, Pt and Pd in Martian meteorites are relatively constant. • Martian meteorites show very limited eruptive losses of volatile Re, S, Se and Te. • The parent magmas of most Martian meteorites were sulfide-undersaturated. • Martian mantle and core have a low sulfur content. • Low Te/PGE ratios in Martian meteorites reflect a strongly volatile element-depleted Martian late veneer.