Fig. 15.
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Distribution of the δi, V values (see text and Fig. 14). The solid line histogram refers to the observed galaxies. The dashed line histogram refers to the galaxies of the simulated clusters, normalized to the number of observed galaxies. The blue vertical dashed lines mark the |δi, V|> 3 regions in which most of the real galaxies are expected to be in the 3D substructure.
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