Fig. 5.
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Zoomed-in view of Fig. 3, the median radial profiles of the mass density for the ICM gas phase for all the clusters (left panel), and the most massive ones (M3 mass bin, right panel). We highlight the comparison with X-COP observations (Ghirardini et al. 2019), those of a sample of 31 nearly clusters by Eckert et al. (2012), and the Coma cluster (Mirakhor & Walker 2020).
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