\begin{table}%t8
\caption{Nearby type Ia supernovae.\label{table:nearbydata}}
\begin{tabular}{lccccccc}
\hline
{Name} & 
{$z$ $^{a}$} & 
{Bands} &
{$m^*_B$} & 
{$s$} &
{$c$} &
{$\mu_B$ $^{b}$} &
{Phot. ref.$^{c}$}  
\\\hline
1990af & 0.050 & {\it BV} & 17.723 $\pm$ 0.006 & 0.737 $\pm$ 0.001 & --0.001 $\pm$  0.009 & 36.632 $\pm$  0.045 & (H96) \\
1990O & 0.031 & {\it BV} & 16.196 $\pm$ 0.023$^d$ & 1.035 $\pm$ 0.033$^d$ & 0.017 $\pm$  0.023$^d$ & 35.532 $\pm$  0.091 & (H96) \\
1992ae & 0.075 & {\it BV} & 18.392 $\pm$ 0.037$^d$ & 0.939 $\pm$ 0.021$^d$ & --0.023 $\pm$  0.025$^d$ & 37.642 $\pm$  0.049 & (H96) \\
1992ag & 0.026 & {\it BV} & 16.241 $\pm$ 0.021$^d$ & 1.030 $\pm$ 0.027$^d$ & 0.155 $\pm$  0.018$^d$ & 35.353 $\pm$  0.094 & (H96) \\
1992aq & 0.101 & {\it BV} & 19.299 $\pm$ 0.028$^d$ & 0.839 $\pm$ 0.032$^d$ & --0.048 $\pm$  0.020$^d$ & 38.437 $\pm$  0.055 & (H96) \\
1992bc & 0.020 & {\it BV} & 15.086 $\pm$ 0.007 & 1.033 $\pm$ 0.007 & --0.031 $\pm$  0.008 & 34.494 $\pm$  0.111 & (H96) \\
1992bh & 0.045 & {\it BV} & 17.592 $\pm$ 0.016 & 0.985 $\pm$ 0.016 & 0.095 $\pm$  0.014 & 36.728 $\pm$  0.057 & (H96) \\
1992bl & 0.043 & {\it BV} & 17.275 $\pm$ 0.033$^d$ & 0.784 $\pm$ 0.016$^d$ & --0.014 $\pm$  0.020$^d$ & 36.276 $\pm$  0.059 & (H96) \\
1992bo & 0.018 & {\it BV} & 15.753 $\pm$ 0.012 & 0.739 $\pm$ 0.006 & 0.055 $\pm$  0.011 & 34.576 $\pm$  0.121 & (H96) \\
1992bp & 0.079 & {\it BV} & 18.281 $\pm$ 0.011 & 0.873 $\pm$ 0.014 & --0.043 $\pm$  0.012 & 37.465 $\pm$  0.041 & (H96) \\
1992br & 0.088 & {\it BV} & 19.398 $\pm$ 0.073$^d$ & 0.650 $\pm$ 0.029$^d$ & 0.032 $\pm$  0.037$^d$ & 38.121 $\pm$  0.046 & (H96) \\
1992bs & 0.063 & {\it BV} & 18.177 $\pm$ 0.041$^d$ & 1.001 $\pm$ 0.018$^d$ & --0.034 $\pm$  0.019$^d$ & 37.540 $\pm$  0.046 & (H96) \\
1992P & 0.026 & {\it BV} & 16.037 $\pm$ 0.018$^d$ & 1.139 $\pm$ 0.084$^d$ & --0.005 $\pm$  0.018$^d$ & 35.565 $\pm$  0.141 & (H96) \\
1993ag & 0.050 & {\it BV} & 17.799 $\pm$ 0.014 & 0.915 $\pm$ 0.018 & 0.096 $\pm$  0.017 & 36.827 $\pm$  0.060 & (H96) \\
1993B & 0.071 & {\it BV} & 18.377 $\pm$ 0.054$^d$ & 0.988 $\pm$ 0.022$^d$ & 0.041 $\pm$  0.026$^d$ & 37.604 $\pm$  0.048 & (H96) \\
1993H & 0.025 & {\it BV} & 16.735 $\pm$ 0.017 & 0.699 $\pm$ 0.012 & 0.250 $\pm$  0.015 & 35.192 $\pm$  0.092 & (H96, A04) \\
1993O & 0.053 & {\it BV} & 17.614 $\pm$ 0.011 & 0.901 $\pm$ 0.010 & --0.014 $\pm$  0.011 & 36.794 $\pm$  0.047 & (H96) \\
1994M & 0.024 & {\it BV} & 16.205 $\pm$ 0.041$^d$ & 0.854 $\pm$ 0.019$^d$ & 0.040 $\pm$  0.022$^d$ & 35.228 $\pm$  0.094 & (R99) \\
1994S & 0.016 & {\it BV} & 14.760 $\pm$ 0.017 & 1.018 $\pm$ 0.026 & 0.016 $\pm$  0.017 & 34.071 $\pm$  0.146 & (R99) \\
1995ac & 0.049 & {\it BV} & 17.026 $\pm$ 0.009 & 1.042 $\pm$ 0.013 & 0.010 $\pm$  0.010 & 36.383 $\pm$  0.051 & (R99, A04) \\
1995bd & 0.016 & {\it BV} & 15.246 $\pm$ 0.009 & 0.992 $\pm$ 0.009 & 0.293 $\pm$  0.008 & 34.083 $\pm$  0.138 & (R99, A04) \\
1996ab & 0.125 & {\it BV} & 19.525 $\pm$ 0.027$^d$ & 0.957 $\pm$ 0.033$^d$ & --0.074 $\pm$  0.015$^d$ & 38.885 $\pm$  0.049 & (R99) \\
1996bl & 0.035 & {\it BV} & 16.611 $\pm$ 0.010 & 0.983 $\pm$ 0.015 & 0.037 $\pm$  0.011 & 35.837 $\pm$  0.069 & (R99) \\
1996bo & 0.016 & {\it U{\it BV}} & 15.816 $\pm$ 0.006 & 0.881 $\pm$ 0.003 & 0.343 $\pm$  0.007 & 34.405 $\pm$  0.133 & (R99, A04) \\
1996bv & 0.017 & {\it BV} & 15.380 $\pm$ 0.019$^d$ & 0.989 $\pm$ 0.024$^d$ & 0.225 $\pm$  0.009$^d$ & 34.319 $\pm$  0.133 & (R99) \\
1996C & 0.030 & {\it BV} & 16.636 $\pm$ 0.029$^d$ & 1.045 $\pm$ 0.111$^d$ & 0.122 $\pm$  0.010$^d$ & 35.822 $\pm$  0.210 & (R99) \\
1997dg & 0.030 & {\it U{\it BV}} & 16.821 $\pm$ 0.014$^d$ & 0.917 $\pm$ 0.024$^d$ & 0.005 $\pm$  0.010$^d$ & 35.994 $\pm$  0.080 & (J02) \\
1997Y & 0.017 & {\it U{\it BV}} & 15.284 $\pm$ 0.020$^d$ & 0.916 $\pm$ 0.024$^d$ & 0.008 $\pm$  0.014$^d$ & 34.452 $\pm$  0.136 & (J02) \\
1998ab & 0.028 & {\it U{\it BV}} & 16.048 $\pm$ 0.010 & 0.938 $\pm$ 0.008 & 0.071 $\pm$  0.007 & 35.150 $\pm$  0.079 & (J02) \\
1998dx & 0.054 & {\it U{\it BV}} & 17.660 $\pm$ 0.055$^d$ & 0.733 $\pm$ 0.039$^d$ & --0.028 $\pm$  0.019$^d$ & 36.606 $\pm$  0.054 & (J02) \\
1998eg & 0.024 & {\it U{\it BV}} & 16.089 $\pm$ 0.009 & 0.940 $\pm$ 0.029 & 0.036 $\pm$  0.012 & 35.250 $\pm$  0.102 & (J02) \\
1998V & 0.017 & {\it U{\it BV}} & 15.094 $\pm$ 0.011$^d$ & 0.909 $\pm$ 0.016$^d$ & 0.030 $\pm$  0.006$^d$ & 34.216 $\pm$  0.128 & (J02) \\
1999aw & 0.039 & {\it BV} & 16.732 $\pm$ 0.005 & 1.205 $\pm$ 0.008 & 0.044 $\pm$  0.006 & 36.284 $\pm$  0.057 & (S02) \\
1999cc & 0.032 & {\it U{\it BV}} & 16.791 $\pm$ 0.009 & 0.840 $\pm$ 0.013 & 0.043 $\pm$  0.010 & 35.789 $\pm$  0.074 & (J02) \\
1999ek & 0.018 & {\it U{\it BV}} & 15.584 $\pm$ 0.004 & 0.892 $\pm$ 0.007 & 0.153 $\pm$  0.005 & 34.489 $\pm$  0.124 & (J02, K04b) \\
1999gp & 0.026 & {\it U{\it BV}} & 16.005 $\pm$ 0.004 & 1.104 $\pm$ 0.007 & 0.083 $\pm$  0.004 & 35.342 $\pm$  0.084 & (J02, K01) \\
2000ca & 0.025 & {\it U{\it BV}} & 15.510 $\pm$ 0.007 & 1.006 $\pm$ 0.013 & --0.066 $\pm$  0.006 & 34.931 $\pm$  0.091 & (K04a) \\
2000cf & 0.036 & {\it U{\it BV}} & 17.091 $\pm$ 0.027$^d$ & 0.868 $\pm$ 0.024$^d$ & 0.054 $\pm$  0.013$^d$ & 36.113 $\pm$  0.066 & (J02) \\
2000cn & 0.023 & {\it U{\it BV}} & 16.544 $\pm$ 0.007 & 0.732 $\pm$ 0.006 & 0.190 $\pm$  0.006 & 35.146 $\pm$  0.094 & (J02) \\
2000dk & 0.016 & {\it U{\it BV}} & 15.323 $\pm$ 0.005 & 0.724 $\pm$ 0.006 & 0.052 $\pm$  0.005 & 34.129 $\pm$  0.133 & (J02) \\
2000fa & 0.022 & {\it U{\it BV}} & 15.832 $\pm$ 0.014 & 0.953 $\pm$ 0.010 & 0.081 $\pm$  0.009 & 34.941 $\pm$  0.101 & (J02) \\
2001ba & 0.031 & {\it BV} & 16.182 $\pm$ 0.006 & 1.000 $\pm$ 0.011 & --0.043 $\pm$  0.008 & 35.558 $\pm$  0.075 & (K04a) \\
2001cn & 0.015 & {\it U{\it BV}} & 15.271 $\pm$ 0.013$^d$ & 0.911 $\pm$ 0.012$^d$ & 0.208 $\pm$  0.007$^d$ & 34.118 $\pm$  0.142 & (K04b) \\
2001cz & 0.017 & {\it U{\it BV}} & 15.035 $\pm$ 0.006 & 1.004 $\pm$ 0.010 & 0.120 $\pm$  0.007 & 34.162 $\pm$  0.127 & (K04b) \\
\end{tabular}
$^a$ { CMB-centric redshift.}\\
$^b$ { Computed with $H_0 = 70$ km~s$^{-1}$~Mpc$^{-1}$. Uncertainty only accounts for photometric uncertainties.}\\
$^c$ { Photometry references: 
H96: \citet{Hamuy96b}, 
R99: \citet{Riess99a}, 
K01: \citet{Krisciunas01},  
J02: \citet{Jha02}, 
A04: \citet{Altavilla04},  
K04a: \citet{Krisciunas04a}, 
K04b: \citet{Krisciunas04b},
S02: \citet{Strolger02}.
}\\
$^d${ First photometric measurement after $B$-band maximum, see discussion in Sect.~\ref{section:snIa-sample}.}
\end{table}