\begin{table}%t1
\caption{\label{tab:deepsurveys}Deep imaging surveys of young ($<$100~Myr), nearby
  ($<$100~pc) stars dedicated to the search for planetary mass
  companions and published in the literature.}
\par
  %\centerline
{
\begin{tabular}{llllll}     % 7 columns 
\hline\hline
Tel/Instr.       &  Mode        & FoV          & \#   & Mass      &  Ref.     \\ 
                 & \& Filter    & (arcsec)     &      & (\Mjup)   &          \\
\hline
3.6 m/ADONIS   & CI, $H-K$       & $13\times13$ & 29       & 5        & (1)                 \\ 
NTT/Sharp        & Sat-DI, $K$    & $11\times11$ & 23       & 5        & (2)                 \\ 
NTT/Sofi         & Sat-DI, $H$    & $13\times13$ & 10       & 5        & (2)                 \\ 
HST/NICMOS       & DI, $H$        & $19\times19$ & 45       & 1        & (3)                 \\
VLT/NaCo         & Sat-DI, $H-K$   & $14\times14$ & 28       & 5        & (4)                 \\ 
VLT/NaCo         & SDI, $H$       & $5\times5$   & 45       & 1        & (5)                 \\ 
VLT/NaCo         & DI, $L'$       & $28\times28$ & 22       & 1        & (6)                 \\ 
Gemini/NIRI      & ADI, $H$       & $22\times22$ & 85$^*$   & 1        & (7)                 \\
\hline                  
\end{tabular}}
\par
\medskip
-- References: (1) Chauvin et~al. (\cite{Chauvin03}), 
(2) Neuh\"auser et~al. (\cite{Neuhauser03}), (3)~Lowrance et~al. (\cite{Lowrance05}), 
(4) Masciadri et~al. (\cite{Masciadri05}), (5) Biller et~al. (\cite{Biller07}), (6) Kasper et~al. (\cite{Kasper07}), (7) Lafreni\`ere et~al. (\cite{Lafreniere07}).
\par
-- ($^*$): For the
  Gemini/NIRI survey, half stars have age estimates younger than
  200~Myr (see Fig.~1, Lafreni\`ere et~al. \cite{Lafreniere07}). 
\end{table}