Fig. A.1.
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Best fit SED models of ALMA-selected galaxies. The black squares report the multiband photometric data. Flux upper limits at 5-σ for C1, C3, and C4, obtained from 3-mm continuum images are also reported. Red, blue, and orange lines represent the dust emission, and the young (star age <10 Myr) and old (>10 Myr) stellar components, respectively. The gray lines show random extraction from the posterior probability distribution of the total galaxy SED.
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