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) |