Fig. C.1.

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Reproducing the scaling relations and histograms in Fig. 11, 12, and 13 using the modelled effective radii values from Su et al. (2021) for Fornax galaxies. Our main conclusion that the effective radii of Fornax galaxies are not significantly different from those found in the field for low stellar mass galaxies < 109 M⊙ remains unchanged.
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