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Fig. 2.
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Marginalized distribution for ρ, σ0, and σ1 as a function of the mean redshift and mean mass of each analysed bin derived with Eq. (2). The fraction of (un)relaxed clusters (1 − ρ) ρ remains constant across redshifts, while we find a positive correlation of σ0 with redshift and a negative correlation of σ1 with mass.
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