Spectral energy distributions from the IR to the radio for the integrated Magellanic clouds. The Draine & Li (2007) dust model spectra as observed in the different photometric bands (blue squares) is fitted to the observed data points (black stars) from 1.27 to 240 μm. Synchrotron and free-free spectra are adjusted on the WMAP and radio data. The sum of the three component fit is displayed as a dashed line. Error bars correspond to 1σ uncertainties.