Table 4
Characteristics of the observed Type II SNe used in this paper, including the inferred time of explosion, the redshift, the distance, the reddening, and the reference from whence these quantities and observational data were taken.
| texpl | z | d | E(B−V) | Ref. | |
|---|---|---|---|---|---|
| [MJD] | [Mpc] | [mag] | |||
| SN 1987A | 46849.82 | 0.00088 | 0.05 | 0.15 | a |
| SN 1999em | 51474.3 | 0.0024 | 11.5 | 0.1 | b |
| SN 2012aw | 56002.6 | 0.0026 | 9.9 | 0.074 | c |
| SN 2004et | 53270.5 | 0.0009 | 7.73 | 0.3 | d |
| SN 2013ej | 56497.5 | 0.0022 | 10.2 | 0.06 | e |
| SN 2015bs | 56920.60 | 0.027 | 120.23 | 0.04 | f |
References. (a) Phillips et al. (1988, 1990); (b) Leonard et al. (2002) and Dessart & Hillier (2006); (c)Dall’Ora et al. (2014); (d) Sahu et al. (2006) – we use a lower reddening E(B − V) of 0.3 mag; We adopt the distance of Van Dyk et al. (2019). (e)Yuan et al. (2016); (f)Anderson et al. (2018).
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