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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(BV) 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(BV) 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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