Fig. 2.
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Detection probability as a function of richness (bottom axis) and redshift (top axis) for the AMICO-DR3 galaxy clusters, shown with dotted and dashed lines, respectively. As the catalogue contains very few clusters with high richness (greater than 70), clusters are divided into five logarithmically spaced richness bins and seven linearly spaced redshift bins. The error bars represent the standard errors of the detection probability.
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