Table 1: The low redshift spectra analyzed in this study. The dates correspond to the epoch relative to maximum luminosity in the B-band. Many of these spectra are available in the SUSPECT archive as well as their listed publications.
Name Date(s) Reference
1981B 0, 20 Branch et al. (1983)
1986G -5, -4, -3, 0 Phillips et al. (1987)
1989B -7, -5, -3, -2, -1, 3, 5, 8, 9, 11, 12, 13, 16, 17, 18, 19 Barbon et al. (1990), Wells et al. (1994)
1990N -14, -7, 2, 3, 17 Mazzali et al. (1993)
1991M 3 Gomez & Lopez (1998)
1991T -12, -11, -10, -8, -7, -6, 0, 10, 15 Mazzali et al. (1995)
1991bg 0, 1, 2 Turatto et al. (1996)
1992A -5, -1, 3, 5, 6, 7, 9, 11, 16, 17 Kirshner et al. (1993)
1994D -11, -10, -9, -8, -7, -5, -4, -2, 2, 4, 10, 11, 12, 13, 20 Patat et al. (1996)
1994Q 10 Gomez & Lopez (1998)
1996X -2, -1, 0, 1, 2, 7 Salvo et al. (2001)
1997br -9, -8, -7, -6, -4, 8 Li et al. (1999)
1997cn 3 Turatto et al. (1998)
1998aq -8, 0, 1, 2, 3, 4, 5, 6, 7 Branch et al. (2003)
1998bu -4, -3, -2, 8, 9, 10, 11, 12, 13 Capellaro et al. (2001)
1999aa -11, -3, -1, 5, 6 Garavini et al. (2004)
1999ac -15, -9, 0, 2, 8, 11 Garavini et al. (2004)
1999aw 3, 5, 5, 12 Strolger et al. (2002)
1999by -5, -4, -3, -2, 3, 4, 5, 6, 7, 8, 11 Garnavich et al. (2004)
1999ee -11, -9, -8, -6, -4, -2, -1, 0, 3, 5, 7, 8, 9, 12, 14 Hamuy et al. (2002)
2000E -2, 3, 5, 14 Valentini et al. (2003)
2000cx -4, -3, -2, -1, 0, 1, 5, 6, 7, 9, 11 Li et al. (2001)
2002bo -14, -13, -11, -7, -6, -5, -4, -3, -2, -1, 4 Benetti et al. (2004)
2003du -11, -7, 13 Anupama et al. (2005)


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