Fig. 3.
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Comparison of the Ωm and σ8 distribution for XODs from the D1 and D3 datasets. Left: D1 with eight free parameters. Right: D3 with six free parameters, having fixed cluster evolution to be self-similar. Both datasets verify the dn/dz test. Each dataset contains 70 000 XODs. The white zones show the regions excluded by each selection. Fixing cluster evolution does not significantly restrict the a priori range of possible cosmological values.
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