From left to right: Radial distribution of dark matter subhalos at z = 0 for various mass bins and dark matter models. The triangles represent bins with a group mass of log[M_200c/(M_⊙ h⁻¹)] = 10.7 (green), 11.2 (gray), 12.6 (gold), and 13.1 (red), respectively. The solid, colored lines reflect the gNFW best-fit model. The corresponding errors are computed with the standard deviation of the measurements, for each mass bin.