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Fig. 10


SN rates per unit stellar mass [10-3 SNe yr-1 10-10M] as a function of the mass of the parent galaxy in the star-forming subsample for Type Ia (left panel) and CC SNe (right panel). In both panels the circles are from SUDARE, the triangles from Mannucci et al. (2005), the squares from Sullivan et al. (2006), the pentagons from Smith et al. (2012) and the diamonds from Graur et al. (2015). SN rates and masses have been rescaled to a Salpeter IMF.

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