Identification of X-ray emission with galaxy groups from the v195 volume-limited catalog of Tempel et al. (2014). The sample was cleaned to remove groups with fewer than ten member galaxies. Groups that were only matched with an X-ray source using an MHD in degrees are marked with red circles, while groups that were only matched using an MHD in megaparsecs are marked with blue diamonds. Groups that were matched when using an both an MHD in megaparsecs or degrees are marked with green triangles. Unmatched groups are plotted in gray. The black line represents a σ(z) function above which we have 50% completeness for matches.