Fig. 11.
Comparisons of projected cross-correlation functions derived for mass groups of M8 (circles) and M9 (squares). Each panel represents the result for redshifts z0, z1, z2, and z3. Redshift-matched AGN samples and galaxy samples brighter than $M_{90\%}$ are used. Solid lines represent the power-law model fitted to the data points. (Color online)

Comparisons of projected cross-correlation functions derived for mass groups of M8 (circles) and M9 (squares). Each panel represents the result for redshifts z0, z1, z2, and z3. Redshift-matched AGN samples and galaxy samples brighter than |$M_{90\%}$| are used. Solid lines represent the power-law model fitted to the data points. (Color online)

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