Table 1.
Characteristics of observed Type II SNe used in this paper.
| texpl | z | d | E(B − V) | Ref. | |
|---|---|---|---|---|---|
| [MJD] | [Mpc] | [mag] | |||
| SN 2005cs | 53547.6 | 0.0016 | 8.9 | 0.04 | a |
| SN 2003cn | 52719.5 | 0.0181 | 78.7 | 0.059 | b |
| SN 2006qr | 54062.8 | 0.0145 | 63.68 | 0.124 | b |
| SN 2007oc | 54388.5 | 0.0048 | 18.11 | 0.014 | b |
| SN 1999em | 51474.3 | 0.0024 | 11.5 | 0.1 | c |
| SN 2012aw | 56002.6 | 0.0026 | 9.9 | 0.074 | d |
| SN 2004et | 53270.5 | 0.0009 | 5.5 | 0.3 | e |
| SN 2013ej | 56497.5 | 0.0022 | 10.2 | 0.06 | f |
| SN 2014G | 56669.6 | 0.0045 | 24.5 | 0.21 | g |
| SN 1979C | 43975.0 | 0.0046 | 16.86 | 0.023 | h |
| SN 1998S | 50875.2 | 0.003 | 17.0 | 0.22 | i |
Notes. These include the inferred time of explosion, the redshift, the distance, the reddening, and the reference from where these quantities and observational data were taken.
References. The references used are a: Pastorello et al. (2009) and Dessart et al. (2008); b: Anderson et al. (2014); c: Leonard et al. (2002) and Dessart & Hillier (2006); d: Dall’Ora et al. (2014); e: Sahu et al. (2006) – we use a lower reddening E(B − V) of 0.3 mag; f: Yuan et al. (2016); g: Terreran et al. (2016); h: Panagia et al. (1980); i: Fassia et al. (2000).
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