Table 4
Characteristics of our selected sample of Type Ib and Ic SNe.
| SN | Type | D | μ | texpl |  |
 |
 |
 |
z | Ref. |
|---|---|---|---|---|---|---|---|---|---|---|
| [Mpc] | [mag] | MJD [d] | [mag] | [mag] | ||||||
| sn2004gq | Ib | 25.1 | 32.00 | 53 346.9 | 0.06 | 3.1 | 0.08 | 3.1 | 0.0065 | CfA, CSP |
| sn2004gv | Ib | 79.6 | 34.50 | 53 345.3 | 0.03 | 3.1 | 0.03 | 3.1 | 0.0200 | CSP |
| sn2005hg | Ib | 86.0 | 34.67 | 53 665.8 | 0.09 | 3.1 | 0.00 | 3.1 | 0.0210 | CSP |
| iPTF13bvn | Ib | 25.5 | 32.04 | 56 459.2 | 0.04 | 3.1 | 0.17 | 3.1 | 0.0045 | (a) |
| sn2008D | Ib | 31.0 | 32.46 | 54 474.0 | 0.02 | 3.1 | 0.60 | 3.1 | 0.0065 | (b) |
| sn2009jf | Ibc(g) | 33.9 | 32.65 | 55 099.5 | 0.05 | 3.1 | 0.11 | 3.1 | 0.0079 | (c) |
| sn2017ein | Ibc(g) | 20.0 | 31.51 | 57 898.5 | 0.02 | 3.1 | 0.38 | 3.1 | 0.0027 | (d) |
| sn2007gr | Ic | 9.3 | 29.84 | 54 325.5 | 0.06 | 3.1 | 0.03 | 3.1 | 0.0017 | (e) |
| sn2004aw | Ic | 68.2 | 34.17 | 53 073.0 | 0.02 | 3.1 | 0.35 | 3.1 | 0.0160 | (f) |
Notes. In the following, CfA refers to Bianco et al. (2014) and CSP to Taddia et al. (2018). (g) The classification as Ibc arises because of the use of the intermediate model he9 at the junction between models thatare unambiguously associated with SNe Ib (he4–he8) and SNe Ic (he10–he12).
References. (a) Bersten et al. (2014); (b) Modjaz et al. (2009); (c)Valenti et al. (2011); (d)Van Dyk et al. (2018, we take the average of their values for the distance and the extinction); (e) Hunter et al. (2009); (f) Taubenberger et al. (2006).
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