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Fig. B.1.

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Normalized statistical distances between our COSMIC models and the AGGC ΔRVmax distribution, with varying cutoff values for the minimum ΔRVmax and number of bins in the compared histograms (histograms shown in Figure 6). The colors indicate the qset value, while the markers indicate different statistical measures. Models with qset = 3 and models with α = 5.0 (D and E) consistently show lower distances to the observational data, which corroborates our finding that these models are better matched to the available data.

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