Iso-correlation contours of the redshift-space two-point correlation function, corresponding to the values ξ(s⊥,s∥) = [0.1,0.2,0.4,1,3], for AGN with log (MBH [h-1M⊙]) > 6.3, at z = 0.2 (black contours). The other contours show the best-fit models, as in Fig. 3.
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