A comparison between the remnant mass plots 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 masive stars being considered.

A. The reaction rate ratio is constant (i.e., R3alpa and R12C(a,g) are changed by the same amount):
1a). AG89 - 15 Msun star	1b). Lodders04 - 15 Msun star
2a). AG89 - 20 Msun star	2b). Lodders04 - 20 Msun star
3a). AG89 - 25 Msun star	3b). Lodders04 - 25 Msun star
B. Only R3alpha varies (i.e., R12C(a,g) constant):
1a). AG89 - 15 Msun star	1b). Lodders04 - 15 Msun star
2a). AG89 - 20 Msun star	2b). Lodders04 - 20 Msun star
3a). AG89 - 25 Msun star	3b). Lodders04 - 25 Msun star
C. Only R12C(a,g) varies (i.e R3alpha constant):
1a). AG89 - 13 Msun star
2a). AG89 - 15 Msun star	2b). Lodders04 - 15 Msun star
3a). AG89 - 17 Msun star
4a). AG89 - 19 Msun star
5a). AG89 - 20 Msun star	5b). Lodders04 - 20 Msun star
6a). AG89 - 21 Msun star
7a). AG89 - 23 Msun star
8a). AG89 - 25 Msun star	8b). Lodders04 - 25 Msun star
9a). AG89 - 27 Msun star