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
5. 9 star average (13, 15, 17, 19, 20, 21, 23, 25, 27 Msun) (Boyes et al. medium weight elements)
a). AG89
6. 9 star average (13, 15, 17, 19, 20, 21, 23, 25, 27 Msun) (all medium weight elements)
a). AG89
7. odd star average (13, 15, 17, 19, 21, 23, 25, 27 Msun) (Boyes et al. medium weight elements)
a). AG89
8. odd star average (13, 15, 17, 19, 21, 23, 25, 27 Msun) (all medium weight elements)
a). AG89