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Table 1

Ejecta model properties from WH07 (upper part) and S16 (lower part).

Model Mej Ekin Vm 1 H 4 He 16 O 24Mg 28Si 40Ca 56Nit=0 Msh
(M) (erg) (km s−1) (M) (M) (M) (M) (M) (M) (M) (M) (km s−1)
Models from Woosley & Heger (2007)

s12A 9.39 1.10(51) 3432 5.27 3.40 3.45(−1) 1.87(−2) 4.53(−2) 3.30(−3) 5.04(−2) 3.8 1667
s15A 10.96 1.14(51) 3233 5.52 4.00 8.24(−1) 3.80(−2) 6.67(−2) 4.41(−3) 8.30(−2) 5.4 1808
s20A 14.11 1.15(51) 2862 5.86 4.96 1.94 7.54(−2) 2.07(−1) 9.20(−3) 1.46(−1) 7.0 1588
s25A 13.94 1.22(51) 2966 4.03 4.74 3.33 1.74(−1) 2.74(−1) 1.29(−2) 1.57(−1) 9.0 1981
s29A 12.53 1.27(51) 3192 1.97 3.52 4.79 1.61(−1) 1.52(−1) 9.68(−3) 1.31(−1) 11.0 3343

Models from Sukhbold et al. (2016)

s9 7.38 1.11(50) 1229 4.54 2.67 6.04(−2) 6.02(−3) 7.84(−3) 6.67(−4) 3.88(−3) 2.0 851
s9p5 7.78 1.82(50) 1533 4.75 2.83 9.69(−2) 8.52(−3) 1.41(−2) 1.24(−3) 1.66(−2) 2.2 948
s10 8.19 6.06(50) 2727 4.94 2.97 9.65(−2) 5.39(−3) 1.33(−2) 1.37(−3) 2.48(−2) 3.0 1832
s10p5 8.67 4.64(50) 2320 5.13 3.19 1.41(−1) 6.92(−3) 1.49(−2) 1.24(−3) 1.67(−2) 3.0 1493
s11 9.12 3.11(50) 1851 5.32 3.37 1.97(−1) 9.61(−3) 2.06(−2) 1.41(−3) 1.63(−2) 3.0 1151
s12 9.32 6.68(50) 2684 5.27 3.41 3.29(−1) 1.72(−2) 2.89(−2) 2.11(−3) 3.17(−2) 4.0 1906
s12p5 9.51 1.36(51) 3791 5.22 3.45 4.56(−1) 3.51(−2) 4.58(−2) 3.03(−3) 5.07(−2) 4.0 2643
s13p5 10.07 1.24(51) 3518 5.32 3.69 5.90(−1) 4.04(−2) 5.18(−2) 3.58(−3) 5.93(−2) 4.0 2328
s14p5 10.37 1.08(51) 3235 5.23 3.81 7.63(−1) 3.87(−2) 5.69(−2) 3.83(−3) 7.28(−2) 4.5 2259
s15p2 10.95 8.37(50) 2771 5.24 3.93 9.97(−1) 4.41(−2) 8.65(−2) 7.77(−3) 6.33(−2) 5.0 1997
s15p7 11.54 8.18(50) 2670 5.53 4.13 1.06 4.68(−2) 8.92(−2) 7.28(−3) 6.75(−2) 5.5 1988
s16p5 12.30 7.56(50) 2485 5.84 4.37 1.19 5.16(−2) 9.93(−2) 7.14(−3) 6.69(−2) 5.5 1770
s17p5 12.87 6.36(50) 2228 5.87 4.54 1.51 8.69(−2) 7.56(−2) 4.79(−3) 6.72(−2) 6.0 1629
s18p5 13.26 6.28(50) 2181 5.73 4.65 1.89 1.42(−1) 6.41(−2) 3.09(−3) 6.26(−2) 6.5 1638
s20p1 (a) 14.03 8.28(50) 2436 5.81 4.93 1.98 9.27(−2) 2.33(−1) 9.91(−3) 9.06(−2) 7.0 1875
s21p5 14.30 7.06(50) 2227 5.38 4.94 2.49 7.98(−2) 1.18(−1) 1.09(−2) 7.22(−2) 8.5 1930
s25p2 (a) 13.22 1.32(51) 3169 3.42 4.43 3.53 6.83(−2) 4.19(−1) 1.27(−2) 1.12(−1) 9.0 3168
s26p5 (a) 13.75 8.48(50) 2490 3.45 4.46 3.77 9.38(−2) 2.59(−1) 1.20(−2) 1.09(−1) 9.5 2527

Notes. The table columns give the ejecta mass, the ejecta kinetic energy, as well as the cumulative yields of H, He, O, Mg, Si, Ca, and 56Ni prior to decay. We specify whether the Si-rich and the O-rich shells merged before core collapse (this did not occur in the WH07 models, and only in three of the S16 models). The last two columns give the choice of mass cut Msh for the shell shuffling, as well as the associated velocity that bounds 99% of the total 56Ni mass in the corresponding model. The selected models from S16 were exploded with the W18 engine. (a) This indicates that the progenitor underwent Si-O shell merging prior to core collapse. The contamination of Si and Ca in the O-rich shell is strong in models s20p1 and s25p2 but moderate in model s26p5 (i.e., only the inner parts of the O-rich shell are contaminated by Si-rich material in model s26p5).

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