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Table 3:

Total nucleosynthetic yields of selected species or groups of species.

Model 		1 2 3 4 5 6
  C/O core detonation
$M_{\rm C/O,~fuel}$ 8.1 $\times$ 10-1 9.2 $\times$ 10-1 1.03 1.13 1.28 1.39
$M_{\rm IGEs}$ 1.8 $\times$ 10-1 3.6 $\times$ 10-1 5.7 $\times$ 10-1 8.2 $\times$ 10-1 1.11 1.33
$M_{\rm IMEs}$ 4.8 $\times$ 10-1 4.4 $\times$ 10-1 3.7 $\times$ 10-1 2.6 $\times$ 10-1 1.2 $\times$ 10-1 3.1 $\times$ 10-2
$M_{\ensuremath{^{56}{\rm Ni}} }$ 1.7 $\times$ 10-1 3.4 $\times$ 10-1 5.5 $\times$ 10-1 7.8 $\times$ 10-1 1.05 1.10
$M_{\ensuremath{^{52}{\rm Fe}} }$ 7.6 $\times$ 10-3 9.9 $\times$ 10-3 9.6 $\times$ 10-3 7.9 $\times$ 10-3 4.2 $\times$ 10-3 1.7 $\times$ 10-3
$M_{\ensuremath{^{48}{\rm Cr}} }$ 3.9 $\times$ 10-4 4.6 $\times$ 10-4 4.5 $\times$ 10-4 3.8 $\times$ 10-4 2.1 $\times$ 10-4 7.1 $\times$ 10-5
$M_{\rm\ensuremath{^{16}{\rm O}} }$ 1.4 $\times$ 10-1 1.1 $\times$ 10-1 8.0 $\times$ 10-2 4.2 $\times$ 10-2 3.1 $\times$ 10-2 1.2 $\times$ 10-2
$M_{\rm\ensuremath{^{12}{\rm C}} }$ 6.6 $\times$ 10-3 4.4 $\times$ 10-3 2.7 $\times$ 10-3 8.8 $\times$ 10-4 5.9 $\times$ 10-3 7.4 $\times$ 10-4
  Helium shell detonation
$M_{\rm He,~fuel}$ 1.3 $\times$ 10-1 8.4 $\times$ 10-2 5.5 $\times$ 10-2 3.9 $\times$ 10-2 1.3 $\times$ 10-2 3.5 $\times$ 10-3
$M_{\rm IGEs}$ 2.9 $\times$ 10-2 (23%) 2.2 $\times$ 10-2 (26%) 1.7 $\times$ 10-2 (30%) 1.3 $\times$ 10-2 (33%) 4.2 $\times$ 10-3 (32%) 1.1 $\times$ 10-3 (31%)
$M_{\rm IMEs}$ 1.3 $\times$ 10-2 (10%) 8.2 $\times$ 10-3 (10%) 5.3 $\times$ 10-3 (10%) 5.7 $\times$ 10-3 (15%) 1.9 $\times$ 10-3 (14%) 7.3 $\times$ 10-4 (21%)
$M_{\ensuremath{^{56}{\rm Ni}} }$ 8.4 $\times$ 10-4 (1%) 1.1 $\times$ 10-3 (1%) 1.7 $\times$ 10-3 (3%) 4.4 $\times$ 10-3 (11%) 1.5 $\times$ 10-3 (11%) 5.7 $\times$ 10-4 (16%)
$M_{\ensuremath{^{52}{\rm Fe}} }$ 7.6 $\times$ 10-3 (6%) 7.0 $\times$ 10-3 (8%) 6.2 $\times$ 10-3 (11%) 3.5 $\times$ 10-3 (9%) 1.2 $\times$ 10-3 (10%) 2.0 $\times$ 10-4 (6%)
$M_{\ensuremath{^{48}{\rm Cr}} }$ 1.1 $\times$ 10-2 (9%) 7.8 $\times$ 10-3 (9%) 4.4 $\times$ 10-3 (8%) 2.2 $\times$ 10-3 (6%) 6.8 $\times$ 10-4 (5%) 1.5 $\times$ 10-4 (4%)
$M_{\ensuremath{^{44}{\rm Ti}} }$ 7.9 $\times$ 10-3 (6%) 5.4 $\times$ 10-3 (6%) 3.4 $\times$ 10-3 (6%) 1.8 $\times$ 10-3 (5%) 4.9 $\times$ 10-4 (4%) 6.2 $\times$ 10-5 (2%)
$M_{\ensuremath{^{40}{\rm Ca}} }$ 4.7 $\times$ 10-3 (4%) 3.2 $\times$ 10-3 (4%) 2.2 $\times$ 10-3 (4%) 2.2 $\times$ 10-3 (6%) 6.8 $\times$ 10-4 (5%) 2.4 $\times$ 10-4 (7%)
$M_{\ensuremath{^{4}{\rm He}} }$ 8.4 $\times$ 10-2 (66%) 5.3 $\times$ 10-2 (63%) 3.3 $\times$ 10-2 (60%) 2.0 $\times$ 10-2 (52%) 6.9 $\times$ 10-3 (54%) 1.7 $\times$ 10-3 (48%)

ML 		2.0 $\times$ 10-1 3.7 $\times$ 10-1 5.7 $\times$ 10-1 8.0 $\times$ 10-1 1.06 1.10
$E_{\rm kin}$ [1051 erg] 0.90 1.04 1.20 1.40 1.59 1.68

Notes.  $M_{\rm C/O,~fuel}$ and $M_{\rm He,~fuel}$are the total masses of initial fuel in the C/O core and the helium shell, respectively. For the helium detonation the values in brackets give the fraction of an isotope mass to the total shell mass  $M_{\rm He,~fuel}$. ML is the total mass of all radioactive species that could power a light curve:  \ensuremath{^{56}{\rm Ni}}, \ensuremath {^{52}{\rm Fe}}, and  \ensuremath {^{48}{\rm Cr}}. All masses are given in units of  \ensuremath{M_\odot}. $E_{\rm kin}$ is the asymptotic total kinetic energy.


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