Fig. A.1.
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Mean goodness of fit (quantified by the χ2) of the NFW (grey), Einasto (orange), and Y24 (blue) models in each considered dark matter scenario. Top to bottom: DMO and FP runs, respectively. In each panel, the solid lines show the mean value as a function of mass for the 50/A resolution, except for WDM1, where 50/B was considered, while the shaded band indicates the standard deviation.
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