Table 3.
Characteristics of the selected sample of observations, ranked in order of increasing of M(H).
| SN | Type | Redshift | μ | E(B − V)tot | Explosion date | Refs. (spectra) | Refs. (photometry) |
|---|---|---|---|---|---|---|---|
| [mag] | [mag] | [MJD] | |||||
| iPTF13bvn | Ib | 0.00449 | 31.76 | 0.071 | 56459 | [1]; [2]; [3] | [1]; [4]; [5] |
| SN 2011dh | IIb | 0.00168 | 29.42 | 0.07 | 55713 | [6] | [6] |
| SN 1993J | IIb | 0.000113 | 27.82 | 0.2 | 49074 | [7]; [8] | [7]; [9]; [10] |
| SN 2006Y | II-L | 0.03358 | 35.73 | 0.115 | 53766 | [11] | [12]; [13] |
| SN 2017eaw | II-P | 0.002192 | 29.47 | 0.30 | 57885 | [14] | [15]; [16] |
Notes. Data downloaded from https://www.wiserep.org/ (Yaron & Gal-Yam 2012).
References. [1] Cao et al. 2013; [2] Fremling et al. 2014; [3] Fremling et al. 2016; [4] Srivastav et al. 2014; [5] Zheng et al. 2022; [6] Ergon et al. 2014; [7] Barbon et al. 1995; [8] Matheson et al. 2000; [9] Richmond et al. 1994; [10] Richmond et al. 1996; [11] Gutiérrez et al. 2017; [12] Anderson et al. 2014b; [13] Hiramatsu et al. 2021; [14] Szalai et al. 2019; [15] Tsvetkov et al. 2018; [16] Van Dyk et al. 2019.
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