Fig. 6.
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Left: M1 − z non-parametric reconstruction using GWTC-3 events. For each redshift value, the mass distribution has been normalised, and the shaded areas mark the 68% credible regions. Right: Posterior distribution for μ and σ of a Gaussian distribution obtained from the non-parametric reconstruction using the remapping procedure presented in Rinaldi et al. (2025b).
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