Broadband SEDs of the NT disk-diffuse emission of the Small (left) and Large (right) Magellanic Cloud. Data points are shown as dots, and model predictions as curves. Emission components are plotted by the following line types: synchrotron, dot-long-dashed; thermal free-free, dot-short-dashed; total radio, solid; Comptonized CMB, long-dashed; Comptonized starlight (EBL+FGL), short-dashed; NT bremsstrahlung, dotted; and pionic, solid. For each type of NT leptonic yield, secondary, primary, and total emissions are denoted as curves with a progressively higher flux. For the Large Magellanic Cloud, in the X-ray and γ-ray range, a solid line on top of the emissions resulting from the various radiative processes indicates the cumulative emission.