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Fig. 5

image

Same as in the left panel of Fig. 4 for 20% loud clusters. The left panel shows the comparison with the previous model with one obtained adopting z2 = 0.6, and one with a lower mass integration limit, of 1013h-1M. The right panel shows the comparison with the model in Fig. 4 and one obtained using the Planck cosmological data.

This figure is made of several images, please see below:

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