\begin{table}%t5
\caption{\label{table:info}The properties of the massive star clusters.}
%\centerline
{
\begin{tabular}{c c c c c c}
\hline\hline
Name  & $M_V$$^{a}$ & $R_{\rm eff}$ & $\sigma$ & age & Mass \\
      & (mag) &  (pc)         & (km~s$^{-1}$)   & Gyr &  ($10^{7}~{\cal{M}}_{\odot}$) \\
\hline
NGC~7252:W3 & $-$16.2 & $17.5\pm1.8$ & $45\pm5$ & $0.4\pm0.15$ &
$8\pm2$ \\
NGC~7252:W30 & $-$14.6 & $9.3\pm1.7$ & $27.5\pm2.5$ & $0.4\pm0.15$ & $1.59\pm0.26$\\
NGC~1316:G114 & $-$13.0 & $4.08\pm0.55$ & $42.1\pm2.8$ & $3\pm1$ & $1.64\pm0.13$\\
\hline
\end{tabular}}
\smallskip
\begin{list}{}{}
\item[$^{{a}}$] We have corrected for foreground extinction of
NGC~7252 and NGC~1316 of $A_{V} = 0.03$  and
$A_{V} = 0.0$  respectively.
\end{list}
\end{table}