Table 6.
Mass fractions of stable isotopes or elements of interest relative to 16O from the solar distribution (Asplund et al. 2009), the simulation G14a from Jones et al. (2016a) post-processed including weak reaction rates from Nabi & Klapdor-Kleingrothaus (2004), and the IMF-weighted average per-explosion FeCCSN ejecta from Nomoto et al. (2006, at Z = 0 and Z = 0.001 and Z = 0.004) together with the maximum allowed number of ECSNe as a fraction of the number of FeCCSNe for each set of assumed FeCCSN yields.
| Isotope/element |
 |
G14aNKK | N06 (Z = 0) | N06 (Z = 0.001) | N06 (Z = 0.004) | |||
|---|---|---|---|---|---|---|---|---|
| Xi/X(16O) |
 |
Xi/X(16O) |
 |
Xi/X(16O) |
 |
|||
| 48Ca | 2.52e-05 | 5.79e-03 | 6.87e-13 | 2.63e-02 | 9.93e-08 | 2.72e-02 | 3.04e-07 | 2.34e-02 |
| 50Ti | 2.94e-05 | 1.06e-02 | 9.12e-13 | 1.69e-02 | 2.98e-07 | 1.74e-02 | 1.13e-06 | 1.47e-02 |
| 54Cr | 7.12e-05 | 2.35e-02 | 4.92e-09 | 1.85e-02 | 8.02e-07 | 1.90e-02 | 2.56e-06 | 1.61e-02 |
| 66Zn | 8.55e-05 | 1.54e-02 | 2.07e-07 | 3.33e-02 | 7.33e-06 | 3.18e-02 | 2.68e-05 | 2.10e-02 |
| 67Zn | 1.27e-05 | 8.37e-05 | 4.82e-09 | 5.26e-01 | 9.38e-07 | 5.17e-01 | 4.40e-06 | 3.96e-01 |
| 68Zn | 5.92e-05 | 3.02e-03 | 8.56e-09 | 1.10e-01 | 6.27e-06 | 1.03e-01 | 2.71e-05 | 5.69e-02 |
| 70Zn | 2.01e-06 | 1.87e-05 | 5.01e-15 | 4.27e-01 | 5.87e-08 | 4.29e-01 | 1.44e-07 | 3.84e-01 |
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