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Fig. 5
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Spatial distribution of the Shapley supercluster’s galaxies. Upper panel: each black dot corresponds to a spectroscopic galaxy selected from Quintana et al. (2020) such that R2 < 18 mag and 9000 < υ < 18 900 km/s. Lower panel: same galaxies after correcting for the FoG effect following Sec. 2.3.
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