Fig. 12
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Ratio of the HMF in wCDM with respect to ΛCDM for different values of w and at different redshifts, as predicted by e-MANTIS as well as multiple HMF predictions from other works. Left: FoF haloes with b = 0.2. Right: SO haloes with Δ = 200c. Only the dedicated emulators are able to fully capture the cosmological and redshift dependence of the HMF.
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