Same as Fig. 8 but for models with different assumptions for SNIa, including two different time delays (t_Ia = 38 Myr and t_Ia = 100 Myr). In addition, we include one model without SNIa and one model in which yields (taken from Seitenzahl et al. 2013) are interpolated in metallicity (denoted Z dep. yields), but otherwise the same as the model with t_Ia = 38 Myr. All models take yields from LC18 with 150 km s⁻¹ stellar rotation for massive stars.