\begin{table}%t1
      \caption{Basic log of the $I$- and $J$-band runs.} 
         \label{log}
     $$ 
       \small  \begin{tabular}{c c c c c c c c c}
            \hline
            \hline
            \noalign{\smallskip}
Telescope       & 
Instrument      & 
Filter          & 
Dates           & 
Exp. time       &
Area            &
{\it FWHM}            &
Compl.          &
Limit.
\\
                &               
                &               
                &                       
                & 
(s)             &
(arcmin$^2$)    &
(arcsec)        &
(mag)           &
(mag)
\\
            \noalign{\smallskip}
            \hline
            \noalign{\smallskip}
INT             & 
WFC             & 
RGO $I$         & 
2000 Dec. 30--2001 Jan. 1 (WFC00) & 
21 $\times$ 1~500              &
970             &
1.2--1.3        &
23.4            &
24.0
\\ % 5+10+6 repeticiones                
                & 
                & 
                & 
2003 Jan. 8 (WFC03) & 
20 $\times$ 1~200 &
970             &
1.0--1.1        &
23.3            &
24.1
\\ % 12 repeticiones            
{\em Antu}      & 
ISAAC           & 
$J$             & 
2001 Dec. 8,9,10,18 & 
4 $\times$ 60   &
680             &
0.4--0.7        &
20.6            &
21.8    
\\ % 7$+$10$+$10$+$2 bloques; 1 bloque = 2 x 16 x 60 s
                & 
                & 
                & 
2001 Dec. 8,9,10,18 & 
2 $\times$ 60$^{a}$     &
110             &
0.4--0.7        &
20.2            &
21.4    
\\ % 7$+$10$+$10$+$2 bloques; 1 bloque = 2 x 16 x 60 s
           \noalign{\smallskip}
            \hline
         \end{tabular}
     $$ 
\begin{list}{}{}
\item\hspace{1.3mm}[$^{a}$] These are areas along the borders of the ISAAC scans and have
  shorter 
integration times.
\end{list}
   \end{table}