Correlation functions for the C0xG1025 sample, continued from Fig. 1. These are measured using the C0 cluster sample (0.1 <  z <  0.2, log₁₀(L_X [erg/s]) >  42.7) in combination with the G1025 galaxy sample (10.25 <  log₁₀(M^*[M_⊙]) <  12). A comparison is provided using the measurement from Zu & Weinberg (2013), showing the group-galaxy cross-correlation for the sample of Yang et al. (2007), with brightest group galaxies in the stellar mass range (11.2 <  log₁₀(M_BGG^*[M_⊙]) <  11.4) and all SDSS galaxies. This result is shown as a dotted line.