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Fig. 6.
Probability of cluster detection as a function of redshift. The solid, dotted, dashed, and long-dashed curves denote the calculation for log10(M200c/M⊙) of 14, 14.5, 14.8, and 15, respectively. The gray curves show the same calculation for clusters with richness deviating from the mass-richness relation by +1.5σλ|μ.
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