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Fig. 1.

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Distributions of properties of sample used in this study. Galaxies with values below (above) the median are marked in yellow (blue). The median value is shown with the dashed vertical line, except for the distance to the MS for which we show a cut 3.5 times higher than (below) the MS. Top left: Stellar mass, M. Top right: Distance to MS as reported in Valentino et al. (2020). Bottom left: Infrared luminosity, LIR. Bottom right: Specific star formation rate (sSFR).

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