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Fig. B.1.

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Correlation between R1 and stellar mass for central (left panel) and satellite (right panel) galaxies in the sample. The median values for each bin are plotted together with the 16% and 84% quantiles (shaded area). For bins with fewer than ten galaxies, single values are plotted. Both fits to the data are for stellar masses M > 108.5 M. For comparison, we plot the relation for R50 in purple.

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