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Table B.1

SNIa and SNcc yield models, taken from literature and used in this work.

Category Name Reference Remarks

SNIa

Classical W7 1 Deflagration, ρ9 = 2.12
Classical W70 1 Deflagration, ρ9 = 2.12, zero initial metallicity
Classical WDD1 1 Delayed-detonation, ρ9 = 2.12, ρT,7 = 1.7
Classical WDD2 1 Delayed-detonation, ρ9 = 2.12, ρT,7 = 2.2
Classical WDD3 1 Delayed-detonation, ρ9 = 2.12, ρT,7 = 3.0
Classical CDD1 1 Delayed-detonation, ρ9 = 1.37, ρT,7 = 1.7
Classical CDD2 1 Delayed-detonation, ρ9 = 1.37, ρT,7 = 2.2
Bravo DDTa 2, 3 Delayed-detonation, fits the Tycho SNR, ρT,7 = 3.9
Bravo DDTc 2, 3 Delayed-detonation, fits the Tycho SNR, ρT,7 = 2.2
Bravo DDTe 2, 3 Delayed-detonation, fits the Tycho SNR, ρT,7 = 1.3
Ca-rich gap CO.45HE.2 4 Ca-rich SNe, MCO = 0.45, MHe = 0.2
Ca-rich gap CO.5HE.2 4 Ca-rich SNe, MCO = 0.5, MHe = 0.2
Ca-rich gap CO.5HE.15 4 Ca-rich SNe, MCO = 0.5, MHe = 0.15
Ca-rich gap CO.5HE.2N.02 4 Ca-rich SNe, MCO = 0.5, MHe = 0.2, 2% N in He layer
Ca-rich gap CO.5HE.2C.03 4 Ca-rich SNe, MCO = 0.5, MHe = 0.2, 30% mixing core-He layer
Ca-rich gap CO.5HE.3 4 Ca-rich SNe, MCO = 0.5, MHe = 0.3
Ca-rich gap CO.55HE.2 4 Ca-rich SNe, MCO = 0.55, MHe = 0.2
Ca-rich gap CO.6HE.2 4 Ca-rich SNe, MCO = 0.6, MHe = 0.2
2D C-DEF 5 2D deflagration, ρ9 = 2.9
2D C-DDT 5 2D delayed-detonation, ρ9 = 2.9, ρT,7 = 1.0
2D O-DDT 5 2D delayed-detonation, ρ9 = 2.9, ρT,7 = 1.0, off-centre ignition
3D N1def 6 3D deflagration, ρ9 = 2.9, 1 ignition spot
3D N3def 6 3D deflagration, ρ9 = 2.9, 3 ignition spots
3D N5def 6 3D deflagration, ρ9 = 2.9, 5 ignition spots
3D N10def 6 3D deflagration, ρ9 = 2.9, 10 ignition spots
3D N20def 6 3D deflagration, ρ9 = 2.9, 20 ignition spots
3D N40def 6 3D deflagration, ρ9 = 2.9, 40 ignition spots
3D N100Ldef 6 3D deflagration, ρ9 = 1.0, 100 ignition spots
3D N100def 6 3D deflagration, ρ9 = 2.9, 100 ignition spots
3D N100Hdef 6 3D deflagration, ρ9 = 5.5, 100 ignition spots
3D N150def 6 3D deflagration, ρ9 = 2.9, 150 ignition spots
3D N200def 6 3D deflagration, ρ9 = 2.9, 200 ignition spots
3D N300Cdef 6 3D deflagration, ρ9 = 2.9, 300 centred ignition spots
3D N1600def 6 3D deflagration, ρ9 = 2.9, 1600 ignition spots
3D N1600Cdef 6 3D deflagration, ρ9 = 2.9, 1600 centred ignition spots
3D N1 7 3D delayed-detonation, ρ9 = 2.9, 1 ignition spot
3D N3 7 3D delayed-detonation, ρ9 = 2.9, 3 ignition spots
3D N5 7 3D delayed-detonation, ρ9 = 2.9, 5 ignition spots
3D N10 7 3D delayed-detonation, ρ9 = 2.9, 10 ignition spots
3D N20 7 3D delayed-detonation, ρ9 = 2.9, 20 ignition spots
3D N40 7 3D delayed-detonation, ρ9 = 2.9, 40 ignition spots
3D N100L 7 3D delayed-detonation, ρ9 = 1.0, 100 ignition spots
3D N100 7 3D delayed-detonation, ρ9 = 2.9, 100 ignition spots
3D N100H 7 3D delayed-detonation, ρ9 = 5.5, 100 ignition spots
3D N150 7 3D delayed-detonation, ρ9 = 2.9, 150 ignition spots
3D N200 7 3D delayed-detonation, ρ9 = 2.9, 200 ignition spots
3D N300C 7 3D delayed-detonation, ρ9 = 2.9, 300 centred ignition spots
3D N1600 7 3D delayed-detonation, ρ9 = 2.9, 1600 ignition spots
3D N1600C 7 3D delayed-detonation, ρ9 = 2.9, 1600 centred ignition spots
Sub-MCh 0.9_0.9 8 WD-WD violent merger, MWD ≃ 0.9, ρ9 = 1.4 × 10-2

SNcc

Nomoto Z0 9,10,11 Zinit = 0
Nomoto Z0_cut 9,10,11 Zinit = 0, restricted to 40 M
Nomoto Z0.001 9,10,11 Zinit = 0.001
Nomoto Z0.004 9,10,11 Zinit = 0.004
Nomoto Z0.008 11 Zinit = 0.008
Nomoto Z0.02 9,10,11 Zinit = 0.02
Nomoto Z0+PISNe 9,10,11,12 Zinit = 0, incl. contribution from PISNe (up to 300 M)
HW Z0+PISNe 13,14 Zinit = 0, incl. contribution from PISNe (up to 260 M)

Notes. The inner core densities ρ9 are given in units of 109 g/cm3. The transitional deflagration-to-detonation densities ρT,7 are given in units of 107 g/cm3. The masses of the CO core and of the He layer (respectively MCO and MHe, “Ca-rich gap” models), and the mass of each of the two merging WD (MWD, “DD channel” model) are given in units of M.

Reference. (1) Iwamoto et al. (1999); (2) Badenes et al. (2003); (3) Badenes et al. (2006); (4) Waldman et al. (2011); (5) Maeda et al. (2010); (6) Fink et al. (2014); (7) Seitenzahl et al. (2013b); (8) Pakmor et al. (2010); (9) Nomoto et al. (2006); (10) Kobayashi et al. (2006); (11) Nomoto et al. (2013); (12) Umeda & Nomoto (2002); (13) Heger & Woosley (2002); (14) Heger & Woosley (2010).

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