Fig. 6


Distribution of the bright XXL cluster sample in the M500,MT vs. redshift plane. Although many low mass systems are detected at low redshift (~20% of the sample with M500,MT< × 1014 M), the high redshift subsample mostly contains similar mass clusters. The dashed line shows the 50% completeness limit in the WMAP9 cosmology from the model described in Sect. 6.1.

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