Fig. 6.
Left: distance of matched AGN from the cluster centre, as a function of 150 MHz luminosity, for the R14 catalogue (red) and the W12 catalogue (blue). Middle: as for the left-hand plot, but as a function of rest-frame KS magnitude. Right: fraction of AGN associated with groups/clusters that are hosted by the cluster centre galaxy (BCG) as a function of radio luminosity (colours as for left panel).
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