A comparison between the absolute yields is done between 2 studies: one using the Anders & Grevess 1989 solar abundances (the present study) and the other making use of the Lodders 2004 solar abundances (previous study) for the initial composition of the stars.

1. 3 star average (15, 20, 25 Msun) (Boyes et al. medium weight elements)
a). AG89	b). Lodders04
2. 3 star average (15, 20, 25 Msun) (all medium weight elements)
a). AG89	b). Lodders04
3. 2 star average (15, 25 Msun) (Boyes et al. medium weight elements)
a). AG89	b). Lodders04
4. 2 star average (15, 25 Msun) (all medium weight elements)
a). AG89	b). Lodders04