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Fig. 1

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Normalised multiplicity function of the superclusters for a range of overdensity parameters, f, constructed with the halos in the CS (black solid line), and with those in the GCS (grey dashed line). The value of f is indicated in each panel. Richer systems are abundant with decreasing f, which is equivalent to a longer linking length (upper left panel), while less rich systems are more common with higher f values (lower right panel).

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