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Fig. 18.
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Mass-richness relation for GAEA H for the redshift range z = 1.5 − 2 (top) and z = 3 − 3.25 (bottom). The small black dots show all proto-clusters, and the blue dots are the ones above the cut, which is shown as a solid black line. The linear regression fit to the relation is shown by a dashed line. M200 is in units of M⊙.
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