\begin{table}%t2
\caption{\label{tab:lowz_phot} 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 \citet{b109}.  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.}
 %\centerline
 {\begin{tabular}{lcccccc}
 \hline \hline
 \noalign{\smallskip}
Name  &  $z$   & MJD$_{\rm{max}}^{{a}}$     &  $m_{{B}}^{{b}}$   & 
$(B - V)_{\rm{max}}^{{c}}$  & $s^{{d}}$ & $M_{{B}}^{{e}}$ \\
\hline
\noalign{\smallskip}
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)$^{5}$ \\
\hline
\end{tabular}}
\par
\medskip
\par
\small
\par
$^a$   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: \citet{blowz1}; 2:
\citet{blowz2}; 3: \citet{blowz3}; 4: \citet{blowz4}; 5: \citet{blowz5};
6: \citet{blowz6}; 7: \citet{b112}.
\end{table}