\begin{table}%T1
\caption{\label{table:0}Observations and data reduction summary.}               
\small%\centerline
{
\begin{tabular}{c@{ }c@{ }c@{ }c@{ }c@{ }c@{ }c@{  }c@{  }c@{\hspace{4pt}}c}
\hline \hline  
 Target & Run & Date & Instrument & Window size (px) & DIT (s) & N.~Frames & Filter &
Apertures (px) & Inner annuli (px)\\
\hline
GJ~436b & A & May 17, 2007 & SofI & $872\times132$ & 0.239 & 36~058 &
$K_{\rm S}$ & 23 & 35\\
XO-1b & A & April 27, 2007 & SofI & $352\times152$ & 0.8 & 17~066 &
$J$ & 11 & 19\\
XO-1b & B & May 1, 2007 & SofI & $892\times180$ & 0.8 & 20~100 & $J$ &
8 & 20\\
XO-1b & C & May 1, 2007 & ISAAC & $64\times544$ &
0.17$-$0.13$^a$ & 110~161 & $K_{\rm S}$ & 7 & 10 \\
XO-1b & D & May 5, 2007 & ISAAC & $64\times544$ & 0.08 & 186~095 & $J$+Block &
21 & 21\\
\hline
\end{tabular}}
\smallskip
$^a$ The DIT (Detector Integration Time) was reduced during the observations to
  avoid reaching the non-linear limit of the detector in improving sky
  conditions. 
\end{table}