The top-left plot shows the sample-split scheme, where galaxies are categorized by position on the ﹩{{\rm{log}}}_{10}({M}_{\star ,R\gt 10\,{\rm{kpc}}}/{M}_{\odot })﹩ vs. ﹩{{\rm{log}}}_{10}({M}_{\star ,R\gt 20\,{\rm{kpc}}}/{M}_{\odot })﹩ plane. The two samples have similar inner stellar masses (M_{⋆,R<10 kpc}); the green circles represent galaxies with more extended outskirts (extended), and the purple diamonds represent more compact galaxies (compact). As before, the total sample is in gray circles. The top-right plot displays the radial profiles of stellar mass density (M_⊙ kpc^–2), with the thick lines representing the median profiles. The green solid lines and purple dashed lines correspond to the extended and compact samples, respectively. The gray-filled bar represents the total sample. Similar to Figure 3, the histograms show the M_* (bottom left), σ_⋆,cen (bottom middle), and redshift (bottom right). We also show the p-values (with errors from resampling the original sample in their respective uncertainties. For M_{⋆,R>20 kpc}, we assume a 0.1 dex error) of the K-S tests on the M_* (bottom left) and σ_⋆,cen (bottom middle) distributions between the two subsamples on the first two histograms. The Jupyter notebook for reproducing this figure can be found here: ✎. This repository is also available on Zenodo (https://doi.org/10.5281/zenodo.17979404).