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Fig. 7

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Impact of the change in the evolution factor of the L500M500 relation (Sect. 4.5). The L500 and M500 values were estimated using the iterative procedure described in Sect. 4.1. Left: Ratio of L500 estimated with the recalibrated L500M500 relation evolving as E(z)−2 (Eq. (9)) to the value obtained with REXCESS relation (E(z)−7/3 evolution). Ratios are colour-coded according to cluster luminosity and plotted as a function of redshifts. Right: Same for the mass, M500. The curves show the theoretical ratio for different luminosity ratios (see Sect. 4.5).

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