\begin{table}%T1
\caption{\label{tab1}Magnitudes for the local sequence stars in the field of SN~2003du. The
stars are identified in Fig.~\ref{fig1}.}
%\centering
\par
\begin{tabular}{lrrrrr}
\hline\hline
ID & \multicolumn{1}{c}{$U$} & \multicolumn{1}{c}{$B$} & \multicolumn{1}{c}{$V$} & 
\multicolumn{1}{c}{$R$} & \multicolumn{1}{c}{$I$}\\
\hline
1 &~$13.80\pm 0.01$ &~$13.81\pm 0.02$ &~$13.19\pm 0.01$ &~$12.80\pm 0.003$ &~$12.43\pm 0.003$\\
2 &~$18.34\pm 0.01$ &~$17.67\pm 0.01$ &~$16.30\pm 0.01$ &~$15.31\pm 0.02$ &~$14.19\pm 0.02$\\
3 &~$13.85\pm 0.01$ &~$13.92\pm 0.02$ &~$13.37\pm 0.01$ &~$13.03\pm 0.01$ &~$12.72 \pm 0.01$\\
4 &~$17.76\pm 0.02$ &~$18.04\pm 0.02$ &~$17.57\pm 0.01$ &~$17.22\pm 0.003$ &~$16.90\pm 0.02$\\
5 &~$16.53\pm 0.01$ &~$16.32\pm 0.03$ &~$15.58\pm 0.02$ &~$15.15\pm 0.01$ &~$14.74\pm 0.01$\\
6 &~$18.25\pm 0.04$ &~$18.67\pm 0.01$ &~$18.20\pm 0.01$ &~$17.86\pm 0.01$ &~$17.50\pm 0.01$\\
7 &~$17.14\pm 0.02$ &~$17.05\pm 0.02$ &~$16.33\pm 0.02$ &~$15.91\pm 0.01$ &~$15.51\pm 0.01$\\
\hline
\end{tabular}
\end{table}