Fig. 8.
Richness distribution of CODEX clusters (solid black histogram) compared to a subsample of CODEX clusters with flux above 10−12 ergs cm−2 s−1 (dashed black histogram), z < 0.3 CODEX clusters (dotted black histogram), and the matched MCXC clusters (solid gray histogram). The comparison shows a deficiency in the low richness identifications present in the MCXC catalog.
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