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Table 1

Ejecta properties for our set of explosion models.

Model MZAMS (M) MpreSN (M) Mej (M) Ekin [foe] Vm [km s−1] 4He (M) 12C (M) 14N (M) 16O (M) 24Mg (M) 28Si (M) 40Ca (M) 56Nit=o (M) 58Ni (M)
he2p6 13.85 2.15 0.79 0.13 4134 0.71 0.02 4.78(−3) 2.28(−2) 1.58(−3) 3.35(−3) 2.40(−4) 1.22(−2) 1.53(−3)
he2p9 14.82 2.37 0.93 0.37 6336 0.77 0.04 5.15(−3) 5.03(−2) 3.82(−3) 1.01(−2) 5.62(−4) 2.32(−2) 1.48(−3)
he3p3 16.07 2.67 1.20 0.55 6777 0.84 0.06 6.21(−3) 1.51(−1) 1.75(−2) 2.76(−2) 1.00(−3) 4.00(−2) 3.61(−3)
he3p5 16.67 2.81 1.27 0.41 5704 0.87 0.07 6.31(−3) 1.72(−1) 1.60(−2) 2.13(−2) 7.34(−4) 2.92(−2) 2.43(−3)
he4p0 18.11 3.16 1.62 0.63 6272 0.92 0.10 6.46(−3) 3.10(−1) 2.98(−2) 4.70(−2) 1.35(−3) 4.45(−2) 3.47(−3)
he4p5 19.50 3.49 1.89 1.17 7884 0.95 0.13 6.52(−3) 4.19(−1) 3.73(−2) 6.14(−2) 2.40(−3) 8.59(−2) 6.09(−3)
he5p0 20.82 3.81 2.21 1.51 8286 0.97 0.15 6.60(−3) 5.92(−1) 5.20(−2) 5.55(−2) 2.26(−3) 9.77(−2) 7.56(−3)
he6p0 23.33 4.44 2.82 1.10 6269 0.95 0.25 6.20(−3) 9.74(−1) 1.01(−1) 5.88(−2) 2.12(−3) 7.04(−2) 5.00(−3)
he7p0 25.68 5.04 3.33 1.38 6456 0.90 0.39 5.42(−3) 1.29(0) 1.07(−1) 9.47(−2) 3.42(−3) 1.02(−1) 4.19(−3)
he8p0 27.91 5.63 3.95 0.71 4251 0.84 0.49 5.17(−3) 1.71(0) 1.10(−1) 4.89(−2) 2.00(−3) 5.46(−2) 3.46(−3)
he12p0 35.74 7.24 5.32 0.81 3911 0.23 1.00 1.42(−4) 3.03(0) 8.73(−2) 7.41(−2) 3.42(−3) 7.90(−2) 2.47(−3)

he2p5MdZ 13.51 2.5 1.10 0.43 6237 0.87 0.05 4.08(−3) 9.20(−2) 3.41(−3) 1.33(−2) 8.39(−4) 3.48(−2) 2.58(−3)
he3p0MdZ 15.14 3.0 1.45 0.72 7077 0.98 0.08 7.12(−3) 2.07(−1) 1.29(−2) 3.82(−2) 2.25(−3) 5.64(−2) 2.51(−3)
he3p5MdZ 16.67 3.5 1.93 1.21 7941 1.06 0.10 7.34(−3) 4.26(−1) 4.25(−2) 7.14(−2) 3.57(−3) 1.02(−1) 5.02(−3)
he4p0MdZ 18.11 4.0 2.34 1.20 7168 1.11 0.13 7.45(−3) 6.71(−1) 5.88(−2) 8.93(−2) 4.53(−3) 1.07(−1) 4.75(−3)
he4p5MdZ 19.50 4.5 2.78 1.20 6573 1.15 0.16 6.60(−3) 9.62(−1) 7.91(−2) 9.27(−2) 4.33(−3) 1.01(−1) 4.44(−3)

Notes. The upper part describes the models already used in D21 while the lower part describes new models arising from progenitors evolved without wind mass loss. The table columns correspond to the ZAMS mass, the preSN mass, the ejecta mass, the ejecta kinetic energy (1 foe ≡ 1051 erg), the mean expansion rate , the cumulative yields of 4He, 12C, 14N, 16O, 24Mg, 28Si, 40Ca, 56Ni prior to decay, and 58Ni. All 56Ni masses used here were taken from the KEPLER approximation to the P-HOTB neutrino simulation (see discussion in D21).

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