Fig. 12.
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Global specific SFR. The galaxies with null sSFR were given the value sSFR = 10−4.15 Gyr−1 (the value of the minimum minus the standard deviation) so that they could appear in the plots. The dotted line marks the limit between star-forming and quenched galaxies, adopted in Peng et al. (2010). Top: distribution of the total sSFR for each type (violin plot as in Fig. 4). Bottom: sSFR versus stellar mass.
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