Correlation between R₁ and stellar mass for all galaxies in the sample (orange symbols). The median values in each bin are plotted together with the 16% and 84% quantiles (shaded area). For bins with fewer than ten galaxies, single galaxies are plotted as small dots. The orange solid line depicts the double power-law fit for M_★ > 10^8.6 M_⊙ (extrapolated below that mass). We show the relation between R₅₀ and stellar mass for all galaxies in the sample in purple. For visual comparison, the galaxies in the sample of Trujillo et al. (2020) are represented with small dots, both R₁ and R₅₀. The distribution of the residuals around the best-fit linear relation for all galaxies is shown in the inset. The distribution has been fitted with a Gaussian (solid line) with a dispersion of σ_Δlog10R1 = 0.06 dex.