\begin{table}%t3
\caption{\label{multi_data}Observations details. }
\small%\centerline
{
\begin{tabular}{lcccccc}
\hline\hline
                Instrument    & Frequency (filter) & Observing dates  & Total exposure time  & Depth              & Resolution  & References   \\                             
                             &       ($\mu$m)     &   (dd/mm/yy)     & (ks)                 & (mag)       & (arcsec)   &               \\
 \hline \noalign{\smallskip}
               HST/ACS       & 0.83 ({\it F814W})       &     $-$          & 2.4$-$2.7 per pointing &      25            &   1.0       &    \cite{MO07.1}$^{1}$\\ 
                             &                    &                  &                      &                    &             &    Smith et~al., in prep.        \\
	       SUBARU/CISCO  & 2.13   ($K'$)        &  17,~18/11/2000   &     9.22             &      22.1          &   0.6-0.8   &    \cite{TA03.1}        \\
               JCMT/SCUBA    & 850                &  03/09/1998      &     22               &      $-$           &   15.0      &    \cite{BO04.1}        \\ 
\hline
\noalign{\smallskip}
 \end{tabular}}
 \smallskip
 $^1$ Data products from their wide field survey in MS0451 are available at \protect\url{http://www.astro.caltech.edu/~smm/clusters/}.\\
 Further information on the data and survey can be found in Chap.~2 of the Ph.D. Thesis of Sean Moran.
\end{table}