\begin{table}%t1
%\centering
\par
\caption{WEBDA parameters on well-studied open clusters.}
\label{tab1}
\begin{tabular}{lcccccccccc}
\hline\hline\noalign{\smallskip}
Cluster&[Fe/H]&Age (Myr)&$d_{\odot}$ (pc)&$R_{\rm ex}$ (\arcmin)&($m-M)_V$&($m-M)_J$&($m-M)_{K_{\rm S}}$&$E(B-V)$&$E(J-H)$&$E(J-K_{\rm S}$)\\
\noalign{\smallskip}\hline\noalign{\smallskip}
Pleiades, M~45&$+0.11$&~135&~150&66&~5.98&~5.910&~5.895&0.030&0.009&0.015\\
M~41, NGC~2287&$+0.04$&~243&~693&25&~9.29&~9.227&~9.214&0.027&0.008&0.013\\
Praesepe, M~44, NGC~2632&$+0.14$&~729&~187&72&~6.39&~6.412&~6.383&0.009&0.003&0.004\\
M~67, NGC~2682&$-0.15$&2564&~908&15&~9.98&~9.799&~9.794&0.059&0.018&0.029\\
NGC~6791&$+0.11$&4395&5853&~7&14.21&13.936&13.879&0.117&0.036&0.057\\
\noalign{\smallskip}\hline\noalign{\smallskip}
\end{tabular}
\begin{list}{Table Notes.}
\item Column 4: distance to the Sun; Col. 5: radius used for VizieR extraction.
\end{list}
\end{table}