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Fig. 6

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AGN fraction (fAGN) contours in the projected pair separation Rn/rvir,nei vs. the clustercentric distance R/r200,cl for the galaxies with 0.04 ≤ z < 0.0927 and −20.0 ≥ Mr > −20.5. Four cases are given; the early-type target galaxies having an early-type neighbor (E-e), the early-type target galaxies having a late-type neighbor (E-l), the late-type target galaxies having an early-type neighbor (L-e), and the late-type target galaxies having a late-type neighbor (L-l). The points with error bars above the x-axes denote the average virial radius of BCGs.

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