Fig. 12
Multiplicity function of AGN for two percolation radii, Rper = 10 h-1 Mpc a) and Rper = 20 h-1 Mpc b). The grey lines show the expected multiplicity of a random field with the same smoothed redshift distribution as the data. We see significant structures with 2−3 members at both radii and one significant structure consisting of 23 members for Rper = 20 h-1 Mpc.
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