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Figure 13. the percentage of dual AGN is plotted against the projected separation between AGN for BAT and SDSS obtained data, respectively.  We compare this with Figure 11 and note that the SDSS obtained values (in red) have the same distribution, and similar error spread. We note that the X-ray fraction for the 1-15 kpc bin seems much higher as compared to that of the radio data. We also have that most of the SDSS-selected data points have an average below $10\%$ in the X-ray band as compared to an average of above $10\%$ for the radio data (see Figure 11). In both cases separations between 1- 30 kpc yield the most data points. (figure from \cite{Koss_2012} )