GSMFs of galaxies in different environments by 0.1 dex bins in log-stellar mass, with single-Schechter function fits to each. The region shaded in grey marks our mass selection limit. Each panel shows GSMFs for galaxies in different types of environment: large-scale structure (top), groups (middle), and pairs (bottom), with the total GSMF for all galaxies shown as the black line in the top panel. Each set of GSMFs adds up to this total set. See fig. 3 in Kelvin et al. (2014) for GSMFs of galaxies by their morphological type.