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Fig. 10.

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Linear relation between the shift of the IRX-βFUV relation at z = 0 (namely that of Overzier et al. 2010) vs. the mass-weighted age in years derived from the analysis of the galaxies studied here. Red symbols correspond to ALMA-detected objects, while blue objects correspond to upper limits from ALMA. We note, however, that these upper limits apply to ALMA, but not to the parameters presented in this figure: ageMstar and βz.

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