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Fig. 10


True vs. estimated richness for the 1208 halos in our sample. Richness refers to galaxies brighter than H(zp) + 1.5 and within r200 radius of each halo. Galaxies with a statistical photometric redshift accuracy σ0 = 0.03 are considered. Left: richness is estimated as Nestimated, where Pthr = 20% is considered. Right: richness is estimated as the sum of the membership probabilities. The mean logarithmic difference along with the rms dispersion around the mean are reported in the panels.

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