Fig. 5

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Detection probability as a function of luminosity L500 in the 0.5–2 keV band and redshift ɀ. The data points with error bars are the L500 for the clusters with >2σ measurements. Details of the computation of L500 are presented in Sect. 5. The white curve shows the flux limit at 1.5 × 10–14 erg s–1 cm–2, corresponding to an average completeness level of ~40%.

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