Fig. 2.
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Mass distribution for the highest accreting third (green) and lowest accreting third (red) of the sample. Left: Gas density. Center: DM density. Right: Baryon depletion. Top row: Profiles stacked over each subsample, together with the whole population (grey lines). Second row: Each class normalised by the ensemble average. Third row: Logarithmic slopes of the profiles, together with an indication of the radius of minimum slope. Bottom row: Correlation between the profiles and accretion rate Γ200m controlling for M200m.
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