Fig. 6
(Left to right) AGN-galaxy and galaxy-galaxy two-point correlation functions computed from the COSMOS photometric catalog. To approximate the GROND sample selection and completeness, only sources with KAB < 19.3 are included. The best fit power-law of the first 14 bins (0 ≤ θ ≤ 42′′) of the galaxy-galaxy two-point correlation function is represented by the solid black line. The same fit is used in both figures for comparison.
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