Fig. 8
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Completeness as a function of intrinsic unabsorbed flux limit for two 𝓛ext thresholds: the cluster catalog 𝓛ext > 3 (in black) and the cosmology sample 𝓛ext > 6 (in blue). The dashed curves show the corresponding number of clusters for both samples. The trade-off between completeness and the number of clusters in the primary cluster sample is clear in the figure.
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