Fig. 7.
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Posterior distributions of the parameters of the mass-amplitude relation in Eq. (18). The contours show the 68th and 95th percentiles of the distributions. For comparison, also shown are the results for α, β, and γ obtained by Bellagamba et al. (2019) (green squares) and when assuming a flat WMAP9 cosmology, fixing ΩM = 0.3 and h = 0.7.
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