Fig. 9.
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Rest-frame velocity distribution relative to the mean cluster velocity of the 120 galaxies having R < 20 (left panel), and of the 395 galaxies within 1 Mpc from the cluster centre (right panel). The smooth curve is the probability density function obtained with a kernel density estimator. In both panels, the dashed line indicates the rest-frame velocity of the BCG: (VBCG − ⟨V⟩)/(1 + z) = 333 km s−1.
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