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Fig. 1.
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Redshift (top panel) and intrinsic richness (bottom panel) distributions of the AMICO galaxy clusters in KiDS-1000 (blue histograms), with S/N > 3.5 and z ∈ [0.1, 0.8], and in KiDS-DR3 (red hatched histograms), following the S/N and redshift selections employed in B19. In both panels, no λ* selections have been applied.
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