Table 2: The photometric properties of the low-z spectra analyzed in this study. The published photometry from these objects was re-fit to determine the magnitudes and lightcurve shape parameters shown here. SN 1991M did not have published photometry in B-band, so the parameters for this object were not determined. The SNLS models did not fit the sub-luminous SN 1991bg with any accuracy; the values given here for this unusual object are from Altavilla et al. (2004). The precision of the derived values for the unusual SN 2000cx are also in doubt and were not used in any of the analysis in this paper. Uncertainties in each quantity are given in brackets.

Name		 z MJD $_{\rm {max}}^{{a}}$ mBb $(B - V)_{\rm {max}}^{{c}}$ sd MBe

1981B		 0.0060 44 671.84(0.09) 11.83(0.01) -0.06(0.01) 0.95(0.01) -19.58(0.22)1
1986G 0.0027 46 560.53(0.05) 11.91(0.01) 0.83(0.01) 0.73(0.01) $\cdots$
1989B 0.0024 47 564.39(0.27) 12.12(0.02) 0.30(0.02) 0.94(0.01) -19.03(0.31)1
1990N 0.0034 48 081.92(0.03) 12.53(0.01) -0.09(0.01) 1.07(0.01) -19.59(0.23)1
1991M 0.0072 $\cdots$ $\cdots$ $\cdots$ $\cdots$ $\cdots$
1991T 0.0060 48 374.25(0.04) 11.30(0.01) -0.04(0.01) 1.05(0.01) -20.07(0.27)2
1991bg 0.0030 48 604.50(1.0) 14.75(0.04) 0.00(0.08) .68(0.10) $\cdots$
1992A 0.0063 48 639.71(0.02) 12.41(0.01) -0.09(0.01) 0.85(0.01) -18.73(0.22)7
1994D 0.0015 49 431.41(0.01) 11.64(0.01) -0.19(0.01) 0.84(0.01) -19.44(0.22)7
1994Q 0.0294 49 494.35(0.90) 16.16(0.09) -0.14(0.04 1.11(0.04) $\cdots$
1996X 0.0070 50 190.65(0.10) 12.86(0.01) -0.12(0.01) 0.90(0.01) -19.38(0.22)7
1997br 0.0053 50 558.57(0.03) 13.23(0.02) 0.12(0.01) 0.89(0.01) $\cdots$
1997cn 0.0162 50 593.36(0.32) 18.12(0.02) 0.92(0.01) 0.89(0.02) $\cdots$
1998aq 0.0037 50 930.16(0.02) 12.18(0.01) -0.25(0.01) 0.98(0.01) -19.87(0.23)6
1998bu 0.0030 50 951.89(0.04) 11.97(0.01) 0.15(0.01) 0.99(0.01) -19.18(0.26)1
1999aa 0.0144 51 231.82(0.03) 14.59(0.01) -0.18(0.01) 1.12(0.01) $\cdots$
1999ac 0.0095 51 250.07(0.08) 13.99(0.01) -0.08(0.01) 1.02(0.01) $\cdots$
1999aw 0.0380 51 253.34(0.08) 16.59(0.01) -0.17(0.01) 1.22(0.01) $\cdots$
1999ee 0.0114 51 468.89(0.01) 14.69(0.01) 0.11(0.01) 1.05(0.01) -19.70(0.30)3
2000e 0.0047 51 576.44(0.03) 12.68 (0.01) 0.01(0.01) 1.03(0.01) -20.08(0.25)7
2000cx 0.0079 51 752.03(0.03) 12.92(0.01) -0.09(0.01) 0.91(0.01) $\cdots$
2002bo 0.0042 52 356.43(0.04) 13.82(0.01) 0.29(0.01) 0.95(0.01) -19.04(0.46)7
2003du 0.0064 52 766.22(0.19) 13.36(0.01) -0.25(0.01) 1.02(0.01) -19.53(0.45)5
a Date of maximum luminosity (rest-frame B');
b Maximum apparent magnitude in rest-frame B' magnitudes, corrected for Milky Way extinction with E(B-V) values from Schlegel et al. (1998); c B-V color at (B-band) maximum luminosity;
d Stretch values, based on fitting a fiducial s = 1.0 Type Ia template;
e Absolute peak luminosities (B'), not adjusted for lightcurve shape-luminosity corrections. These made use of the following distance modulus references - 1: Gibson et al. (2000); 2: Saha et al. (2001); 3: Stritzinger et al. (2002); 4: Candia et al. (2003); 5: Anupama et al. (2005); 6: Riess et al. (2005); 7: Tully (1988).

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