\begin{table}%t2
\caption{\label{tab3}Summary of the photometric information (magnitudes and 1-$\sigma$~errors) for our source.}
%\centering
\par
\begin{tabular}{lccccccccccccc}
\hline\hline\noalign{\smallskip}
$U_{\rm VIMOS}$\tablefootmark{\dag} &\wb\  & \wv\ & $R$   & \wi\ & \wz\ & $J$s  & $H$   & $K$s  &3.6 $\mu\rm m$&4.5 $\mu\rm m$&5.8 $\mu\rm  m$&8.0 $\mu\rm  m$&24 $\mu\rm  m$ \\[2pt]
\hline
29.49        &29.86      &27.86 &27.11&25.22 &24.61       &24.68 &24.80&24.21 &22.82      &23.00     &23.37     &23.18 & 22.61 \\
1$\sigma$ l.m&1$\sigma$ l.m& 0.179     & 0.195   & 0.039 & 0.031     & 0.116    & 0.151   & 0.140    & 0.014    &  0.024   & 0.235    & 0.198 & 1$\sigma$ l.m.   \\
\hline
\end{tabular}
\tablefoot {
\tablefoottext{\dag}{Other two WFI U bands are available, U35 and U38 with slightly different filter shape. The lower limits are 27.84 and~26.75, respectively much shallower than the limit provided by the~$U_{\rm VIMOS}$.}}
\vspace*{4.5mm}
\end{table}