(a, b) Global, (c, d) nuclear, and (e, f) disk SEDs for NGC 4631. The measured data are represented by squares, and the errors for the data are less than the size of the squares. Parts (a), (c), and (e) show the best‐fitting blackbodies with λ−β emissivities (with β variable). Parts (b), (d), and (f) show the best‐fitting two blackbody components with λ−2 emissivities, with the dotted lines represent the individual blackbody components. This format also applies to Figures 3–9, although only the global SEDs are shown in those cases.