From left to right and top to bottom: Stellar mass density (Σ_⋆), star formation rate density (Σ_SFR), dust attenuation ($A_{\mathrm{v}}^{\mathrm{ISM}}$), sSFR, and mass-weighted age normalized median radial profiles inferred using Cigale for BlueSFGs (in blue), RedSFGs (in red), and QGs (in yellow). Error bars represent the 68th and 32th quantiles of the distributions in each radial bin. In the Σ_⋆ panel we indicate the (normalized) half-mass effective radius for each population with a vertical dashed line.