Fig. B.2.
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n parameter of the coreNFW profile versus the ratio of stellar mass formed after and before re-ionisation. Grey circles with error bars show the results for EDGE2 galaxies and coloured plots indicate the fitted values for galaxies from the FIRE-2 suite. Colours indicate the fit quality via the median deviation of the model relative to the data. Galaxies with median relative deviation over 0.15% are displayed as empty circles, indicating unreliable fitting around the core radius. The dot-dashed grey line represents the fit to the EDGE2 simulations reported by Muni et al. (2024).
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