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Fig. 25


Distribution of the estimated bolometric luminosity, L500, as a function of the redshift for the first (red dots) and extended (green dots) cluster sample with X-ray spectroscopic parameters, the cluster sample (blue dots) with X-ray parameters based on the given flux in the 2XMMi-DR3 catalogue, and the MCXC cluster sample (black stars) (Piffaretti et al. 2011).

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