Notes. First column gives the labels used throughout the paper, with simulations divided into four different groups based on the assumption that is varied. Note that some simulations appear multiple times in the table, and the final two labels represent three simulations each. When applicable, the second column gives stellar rotation, and the third column gives the delay time (t_Ia; see Eq. (1)) for SNIa. The last two columns include notable features of each model and a list of yield table references for massive stars. Yield tables for AGB ejecta is omitted for brevity because all models apply yields (Pignatari et al. 2016; Ritter et al. 2018). Yield tables are abbreviated by number accordingly: [1] Pignatari et al. (2016); [2] Ritter et al. (2018); [3] Seitenzahl et al. (2013); [4] LC18. For [3*], we only apply yields from model N100 from Seitenzahl et al. (2013), i.e., SNIa yields at solar metallicity.