Mean completeness and purity along with associated errors as a function of galaxy magnitude (panel a)), projected separation, in r200 units, of the galaxy from the cluster center (panel b)), halo mass (panel c)) and richness (panel d)), cluster redshift (panel e)), and cluster redshift accuracy σc/σ0 (panel f)). Richness refers to cluster galaxies brighter than H∗(zp) + 1.5 and within r200 radius of each halo. All values refer to σ0 = 0.03 and a probability threshold Pthr = 20%.
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