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Fig. A.1


SN rates per unit stellar mass vs. sSFR for different CC SN types in three different groups of galaxies based on their sSFR: the first group of passive galaxies with a zero mean SFR, the second group of galaxies with −12.0 < log (sSFR) < −9.5 and the third group of galaxies with log (sSFR) > −9.5. The circles are from SUDARE, the triangles from Mannucci et al. (2005) and the pentagons from Graur et al. (2015).

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