Fig. 4.
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Posterior distributions of the halo occupation function, ⟨Nh⟩, for different dark matter cosmologies (left panel), mass selections (middle panel), and redshifts (right panel). Different dark matter models are tested in box 50/B, with a mass selection of Mmin > 109 M⊙ h−1. The other two panels consider the CDM cosmology in box 50/A.
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