\begin{table}%t1
\caption{Well-observed SNe~Ia in the Hubble flow.}\label{data.tab}
%\centerline
{
\begin{tabular}{l l l c c c c}
\hline \hline
SN & Filters & Ref. & $E(B-V)_{{\rm gal}}^{a}$ & $E(B-V)_{{\rm host}}$ & $v_{{\rm CMB}}$ $^{b}$ &
$F_{{\rm max}}^{{\rm bol}}$ \\
 &  &  &  &  & (km~s$^{-1}$) & (erg s$^{-1}$ cm$^{-2}$)  \\ 
\hline
SN1992bc & $BVRI$  & 1        & 0.022 & 0.000 & 5870  & (1.565 $\pm$ 0.124) $\times$ $10^{-11}$ \\ 
SN1992bo & $BVRI$  & 1        & 0.027 & 0.000 & 5151  & (9.106 $\pm$ 0.967) $\times$ $10^{-12}$ \\ 
SN1993H  & $BVRI$  & 1        & 0.060 & 0.050 & 7112  & (4.640 $\pm$ 0.613) $\times$ $10^{-12}$ \\
SN1995E  & $BVRI$  & 2        & 0.027 & 0.740 & 3478  & (5.726 $\pm$ 0.622) $\times$ $10^{-11}$ \\
SN1995ac & $BVRI$  & 2        & 0.042 & 0.080 & 14~651 & (3.425 $\pm$ 0.477) $\times$ $10^{-12}$ \\ SN1995bd & $BVRI$  & 2        & 0.495 & 0.150 & 4266  & (2.542 $\pm$ 0.521) $\times$ $10^{-11}$ \\
SN1996bo & $BVRI$  & 2        & 0.078 & 0.280 & 4857  & (2.382 $\pm$ 0.237) $\times$ $10^{-11}$ \\ 
SN1999aa & $UBVRI$ & 3, 4, 5  & 0.040 & 0.000 & 4546  & (2.333 $\pm$ 0.446) $\times$ $10^{-11}$ \\
SN1999aw & $BVRI$  & 5, 6     & 0.032 & 0.000 & 11~754 & (3.525 $\pm$ 0.700) $\times$ $10^{-12}$ \\
SN1999dq & $UBVRI$ & 3        & 0.024 & 0.139 & 4029  & (3.871 $\pm$ 0.730) $\times$ $10^{-11}$ \\
SN1999ee & $UBVRI$ & 7        & 0.020 & 0.280 & 3169  & (5.781 $\pm$ 0.881) $\times$ $10^{-11}$ \\
SN1999gp & $UBVRI$ & 3, 8     & 0.056 & 0.070 & 7783  & (9.270 $\pm$ 1.082) $\times$ $10^{-12}$ \\
\hline
\end{tabular}}
\medskip
$^a$ Taken from \citet{schlegel98} dust maps. \\
$^b$ Heliocentric velocities from NED transformed to the cosmic microwave background frame. To account for peculiar velocities we assume throughout this work an error of 400~km~s$^{-1}$ for all CMB~distances. \\
References: (1)~-- \citet{hamuy96c}; (2)~-- \citet{riess99a}; (3)~-- \citet{jha02}; (4)~-- \citet{krisciunas00}; (5)~-- \citet{regnault00}; (6)~--~\citet{strolger02}; (7)~-- \citet{stritzinger02}; (8)~-- \citet{krisciunas01}.
\end{table}