Distributions of (from top to bottom) mass-weighted ages, stellar masses, SFRs, and dust attenuation of clumps detected in Hα (in gold) and F275W (in dark pink), and star-forming complexes (in purple). We limit the histograms to the 95th percentiles of ⟨ t_⋆⟩_M and A_V, and to the 15th percentile of SFR. These percentiles are calculated for the combined (all clumps and complexes) samples and the ranges are kept the same in all histograms of the same variable. Left panels show the general samples, tail clumps and complexes are in the middle panels and extraplanar clumps are on the right. Histograms are normalized to have the same area.