Fig. 7
Local density as a function of the cluster-centric radius. Open circles represent cluster members not detected in the FIR, yellow and orange filled circles represent MIPS-only and Herschel-detected SF galaxies, respectively. The vertical dash-dotted line at 1.05 Mpc shows the virial radius. The horizontal dashed lines at log Σ = 1.65 and 2.15 indicate the limits between the low-, intermediate-, and high-density environments. The red stars are the AGN candidates.
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