Table 2.
Physical parameters derived from the hydrodynamic modelling of bolometric LCs and expansion velocities for three SNe II in our sample when their bolometric LCs are constructed using different methods.
| SN | BLCs | MZAMS | Mej | E | MNi | 56Ni mixing |
|---|---|---|---|---|---|---|
| (M⊙) | (M⊙) | (foe) | (M⊙) | (%) | ||
| 2005dn | This work | 10.7 |
8.5 |
0.94 |
0.041 |
39 |
| Method 1 | 11.8 |
9.2 |
1.12 |
0.049 |
45 |
|
| 2007ab | This work | 11.2 |
8.8 |
1.15 |
0.033 |
22 |
| Method 1 | 10.9 |
8.6 |
1.42 |
0.051 |
26 |
|
| 2008if | This work | 10.1 |
8.2 |
1.00 |
0.042 |
21 |
| Method 1 | 10.2 |
8.3 |
1.33 |
0.065 |
33 |
|
Notes. BLCs indicates the method used to calculate the bolometric luminosity. MZAMS, Mej, E, and MNi refer to the progenitor initial mass, ejecta mass, explosion energy, and 56Ni mass, respectively. 56Ni mixing describes the spatial distribution of 56Ni within the ejecta and is presented in percentage of the pre-SN mass in mass coordinate. The reader is referred to Paper II for a full description of our modelling and fitting procedures.
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