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Fig. D.1

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SED of LMC as observed with gray points and without CMB with black points (subtracted from the best model), and radio data in light blue (from Tables A.1) with 30% increased uncertainties. Data points from the literature (Israel et al. 2010; Planck Collaboration XVII 2011) are overlaid in green. The best fit model spectra are overlaid for the global model and individual emission components. On the right, the corner plot displays probability distributions of each model parameter, with the MCMC best-fit values indicated above each histogram.

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