Fig. 8
SN rates as a function of B−K galaxy colour for SNe Ia (top panel) and CC SNe (bottom panel). For comparison we report the same measurements obtained in the local Universe by Mannucci et al. (2005) and by Li et al. (2011). The mass estimates for the galaxies by Mannucci et al. (2005) and Li et al. (2011) have been converted to a Salpeter IMF and B−K colours are all in AB mag.
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