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Fig. 9


Top: pressure profiles for all our clusters rescaled using an overdensity of 500, colour coded with respect to the redshift bin to which each curve belongs, compared with the best-fit results in Arnaud et al. (2010; black solid line). Bottom: stacked pressure profiles (in logarithmic space) compared with the best fit of Arnaud et al. (2010); the panel at the bottom shows the ratio with respect to the “universal” pressure profile.

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