Fig. 9.

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Global SFR. The galaxies with SFR = 0 M⊙ yr−1 were given the value SFR = 10−2.67 M⊙ yr−1 (the value of the minimum minus the standard deviation) so that they could appear in the plots. Top: distribution of the SFR by morphological types (violin plot as in Fig. 4). Bottom: SFR versus stellar mass, coloured by morphological type. The dashed lines refer to the SFMS, parametrised as in González Delgado et al. (2016, in green), Renzini & Peng (2015, in orange) and Duarte Puertas et al. (2017, in blue). The black dots mark the median value of our data in bins of mass, taking into account only late spirals (Sb, Sc, Sd) that had originally SFR ≠ 0.
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