Table 8
Explosion parameters for 33 CSP-I SE SNe from the semi-analytic and hydrodynamical modeling of their bolometric light curves.
SN | Type | M ej | E K | M(56Ni) | M ej | E K | M(56Ni) | 56Ni mixing |
(M⊙) | (1051 erg) | (M⊙) | (M⊙) | (1051 erg) | (M⊙) | |||
|
||||||||
Arnett modelHydrodynamical model | ||||||||
2004ex | IIb | 3.2(0.1) | 0.6(0.1) | 0.09(0.01) | 2.5 | 0.8 | 0.10 | 0.88 |
2004ff | IIb | 2.2(0.7) | 0.8(0.3) | 0.12(0.02) | 1.9 | 1.0 | 0.135 | 0.88 |
2004gq | Ib | 2.3(1.5) | 2.0(1.3) | 0.08(0.02) | 3.4 | 3.0 | 0.11 | 0.98 |
2004gt | Ic | 4.1(1.3) | 1.3(0.4) | 0.16(0.02) | 3.4 | 1.2 | 0.16 | 1.00 |
2004gv | Ib | 6.0(1.0) | 2.5(0.4) | 0.15(0.01) | 3.4 | 2.0 | 0.16 | 0.68 |
2005aw | Ic | 2.7(0.1) | 2.3(0.1) | 0.14(0.02) | 4.3 | 2.5 | 0.17 | 0.95 |
2005em | Ic | 0.7(0.5) | 0.2(0.1) | 0.11(0.01) | 1.1 | 0.25 | 0.13 | 1.00 |
2006T | IIb | 5.5(0.4) | 1.5(0.1) | 0.11(0.02) | 3.4 | 1.5 | 0.12 | 0.65 |
2006ba | IIb | 2.6(0.4) | 0.5(0.1) | 0.12(0.02) | 1.9 | 1.0 | 0.19 | 1.00 |
2006bf | IIb | 3.0(0.5) | 0.8(0.1) | 0.09(0.02) | 1.9 | 0.6 | 0.11 | 1.00 |
2006ep | Ib | 0.8(0.6) | 0.3(0.2) | 0.09(0.02) | 1.9 | 1.0 | 0.12 | 1.00 |
2006ir | Ic | 1.4(0.1) | 1.1(0.1) | 0.19(0.03) | 4.3 | 2.5 | 0.20 | 0.73 |
2006lc | Ib | 8.3(1.0) | 2.9(0.4) | 0.16(0.04) | 3.4 | 1.3 | 0.14 | 0.45 |
2007C | Ib | 3.4(0.8) | 1.3(0.3) | 0.08(0.02) | 6.2 | 2.8 | 0.07 | 0.50 |
2007Y | Ib | 3.1(0.8) | 0.8(0.2) | 0.03(0.01) | 1.9 | 0.6 | 0.03 | 0.75 |
2007ag | Ic | 2.4(0.4) | 1.0(0.2) | 0.10(0.01) | 2.5 | 0.6 | 0.12 | 1.00 |
2007hn | Ic | 1.8(0.7) | 0.5(0.2) | 0.17(0.02) | 1.5 | 0.4 | 0.25 | 1.00 |
2007kj | Ib | 2.8(0.4) | 1.2(0.2) | 0.07(0.01) | 2.5 | 1.2 | 0.066 | 0.75 |
2007rz | Ic | 1.7(0.9) | 1.0(0.5) | 0.08(0.02) | ... | ... | 0.08 | ... |
2008aq | IIb | 4.3(1.4) | 1.5(0.5) | 0.05(0.01) | 3.4 | 0.9 | 0.04 | 0.85 |
2008gc | Ib | 2.6(0.2) | 0.6(0.1) | 0.35(0.04) | 2.5 | 0.6 | 0.35 | 0.85 |
2009K | IIb | 9.1(2.3) | 2.5(0.6) | 0.20(0.08) | 2.5 | 0.8 | 0.18 | 0.70 |
2009Z | IIb | 3.8(0.2) | 1.8(0.1) | 0.25(0.01) | 2.5 | 1.3 | 0.28 | 0.82 |
2009bb | Ic-BL | 3.4(0.4) | 6.2(0.8) | 0.20(0.02) | 4.3 | 8.0 | 0.25 | 0.90 |
2009ca | Ic-BL | 4.7(1.6) | 6.5(2.3) | 1.73(0.19) | 6.2 | 10.0 | 2.40 | 1.00 |
2009dt | Ic | 1.7(0.6) | 0.4(0.1) | 0.12(0.02) | 1.9 | 0.4 | 0.13 | 1.00 |
|
||||||||
2004ew | Ib | 3.7(0.4) | 0.8(0.1) | 0.12(0.01) | ... | ... | 0.150 | 0.80 |
2004fe | Ic | 1.3(1.0) | 0.7(0.6) | 0.08(0.01) | 2.5 | 2.0 | 0.10 | 1.00 |
2005Q | IIb | 4.9(1.3) | 1.6(0.4) | 0.22(0.05) | 2.5 | 1.0 | 0.22 | 0.80 |
2005bj | IIb | 3.9(0.5) | 1.6(0.2) | 0.25(0.03) | 6.2 | 3.0 | 0.23 | 0.70 |
2006fo | Ib | 5.1(1.8) | 1.7(0.6) | 0.23(0.03) | 3.4 | 1.5 | 0.25 | 0.75 |
2008hh | Ic | 2.9(1.2) | 2.4(1.0) | 0.10(0.01) | 4.3 | 3.0 | 0.12 | 1.00 |
2009dp | Ic | 1.8(1.2) | 1.1(0.7) | 0.12(0.02) | 1.9 | 1.0 | 0.25 | 1.00 |
|
||||||||
Full SN sample | ||||||||
IIb (10) | 4.3(2.0) | 1.3(0.6) | 0.15(0.07) | 2.9(1.3) | 1.2(0.7) | 0.16(0.07) | 0.83(0.12) | |
Ib (10) | 3.8(2.1) | 1.4(0.9) | 0.14(0.09) | 3.2(1.3) | 1.6(0.9) | 0.14(0.09) | 0.75(0.18) | |
Ic (11) | 2.1(1.0) | 1.2(0.7) | 0.13(0.04) | 2.8(1.2) | 1.4(1.0) | 0.16(0.06) | 0.97(0.09) | |
Ic-BL (2) | 4.1(0.9) | 6.3(0.2) | 0.96(1.09) | 5.2(1.3) | 9.0(1.4) | 1.32(1.52) | 0.95(0.07) | |
|
||||||||
SNe with observed bolometric peak | ||||||||
IIb (7) | 4.7(2.2) | 1.5(0.6) | 0.15(0.07) | 2.7(0.5) | 1.0(0.3) | 0.15(0.08) | 0.80(0.09) | |
Ib (6) | 3.9(2.7) | 1.6(1.0) | 0.10(0.05) | 2.8(0.7) | 1.5(0.9) | 0.10(0.05) | 0.77(0.20) | |
Ic (4) | 2.5(1.2) | 1.2(0.8) | 0.14(0.04) | 2.9(1.2) | 1.5(0.9) | 0.17(0.06) | 0.99(0.03) | |
Ic-BL (1) | 3.4(0.0) | 6.2(0.0) | 0.20(0.00) | 4.3(0.0) | 8.0(0.0) | 0.25(0.00) | 0.90(0.00) |
Notes. A single horizontal line separates the objects observed in both optical and NIR from those observed only in the optical. Uncertainties on the average of each sub-sample are the standard deviations.
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