Absolute magnitude of galaxies brighter than M_r = −19.5 with 0.04 ≤ z < 0.0927 vs. clustercentric radius. The upper panel shows early types, and the lower panel shows late types. Orange and blue dots indicate AGN hosts and non-AGN galaxies, respectively. Solid lines are median magnitudes for AGN host galaxies, while dashed lines are those for non-AGN galaxies. Crosses are BCGs, and are not used in calculating median curves. Late types with axis ratio of b/a < 0.6 are eliminated. Vertical dashed lines indicate the cluster virial radius r_200,cl.