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Fig. 5.

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Warm dust heated in star forming clouds (, left panel) and cold dust in thermal equilibrium within the ISM (, right panel) parameters obtained with MAGPHYS (da Cunha et al. 2008) using the full photometric coverage (ordinate) or removing WISE data (abscissa). The dashed line shows a linear relation between the two quantities and the black cross in the bottom right corner shows the average errors in the fit.

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