Fig. 5
SEDs of the Magellanic Clouds in the FIR to mm regime, once the free-free and synchrotron emission removed. This SED is fitted from 100 μm to 9.1 mm with a dust model with DCD/TLS effects. The spectral shape of the DCD effect is shown in light blue, while the TLS effects are displayed in dark blue and the total emission is displayed in red.
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