Fig. 23.

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Number of MAMBO proto-clusters and the sky-filling factor in a Δz (50%) redshift interval as a function of redshift and proto-cluster mass limit. The numbers are only shown for the sample with Mpc ≥ 1014 M⊙ as a dotted line. Solid lines show the fraction of the sky covered by the proto-clusters, and the dashed lines display the combined sky area of the proto-clusters. The thick lines with larger data points show the results for the core regions, while the thin lines show those for the region out to rpc. For the core regions of the Mpc ≥ 3 × 1014 M⊙ proto-clusters, the dashed and solid lines overlap.
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