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Fig. 10

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log(NRichσ2) versus log(TX) for the z ≥ 0.5 clusters (all C1 but XLSSC 046 which is C2). The + sign indicates XLSSC 027 and translates to the red disk when replacing the galaxy velocity dispersion by the weak lensing estimate from Gavazzi Soucail (2007). The continuous line is the fit (computed without XLSSC 027 and XLSSC 018): log(NRichσ2) = (1.05 ± 0.13) log(TX) + (7.05 ± 0.07).

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