Comparison between the physical properties obtained when fitting the UV-to-NIR rest-frame observations only (HST+JWST) and the ones obtained when adding the ALMA constraints. The solid black line is the one-to-one relationship. Results for the stellar mass, SFR, FUV attenuation, and β are shown from left to right. The black circles with error bars indicate the median error in each panel. The inset panels show the same figure for the most massive (logM_⋆^{no − IR}/M_⊙ >  8) sources in the sample.