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Table A.1.

Properties of the stellar progenitor models in the 3D CCSN simulations performed in the Garching group. The final fate (ff) column indicates the outcome of the simulation (0: failed SN, 1: successful SN).

model ff MCO/M ξ2.5 s c ( k B N A ) $ \frac{s_{\mathrm{c}}}{(k_B \, N_A)} $ μ4M4 μ4 Ref. progenitor Ref. 3D CCSN sim.
s9.0 1 1.40 4 ⋅ 10−5 0.53 2 ⋅ 10−5 2 ⋅ 10−5 Woosley & Heger (2015) Melson et al. (2020)
z9.6 1 1.37 8 ⋅ 10−5 0.89 3 ⋅ 10−5 2 ⋅ 10−5 Heger (2012), priv. comm. Melson et al. (2015b)
s12.28 1 2.23 0.0312 0.61 0.061 0.039 Yadav (2023), priv. comm. Janka & Kresse (2024)
m15 1 3.24 0.106 0.68 0.073 0.046 Heger et al. (2005) Summa et al. (2018)
s18.88 1 4.45 0.283 0.87 0.200 0.110 Yadav et al. (2020) Bollig et al. (2021)
s20 1 4.98 0.285 0.86 0.201 0.110 Woosley & Heger (2007) Melson et al. (2015a)

s40 0 13.59 0.544 1.05 0.470 0.207 Woosley & Heger (2007) Walk et al. (2020)
u75 0 31.16 0.882 1.53 0.793 0.321 Woosley et al. (2002) Walk et al. (2020)

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