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Figure 14. The log of the X-ray luminosity is plotted against AGN separation. We compare this with Figure 12 and we observe a similar trend. Both plots show that the binned average luminosity versus separation seems to be somewhat stable for separations between 20 - 80 kpc. With separations less than 20 kpc yielding higher luminosities in both cases (X-ray and radio). Figure from \cite{Koss_2011} (figure credit \cite{Koss_2012})