\begin{table}%T2
\caption{Photometric and astrometric measurements of 2M1207 and its GPCC obtained with the myopic deconvolution algorithm \textit{MISTRAL} (Conan et al. \cite{Conan00}). The transformations between the two filters $K_{\rm s}$ and $K$ were found smaller than the measuring errors.}\label{t2}      
%\centerline
{
\begin{tabular}{lllllllllll}
\hline\hline
Source		         &SpT 	&Age	&$J$       &   $H $  &   $K$   & $L~\!'$  &    $\Delta$	   & PA  \\
                         &	&(Myr)	&(mag)	 &(mag)  & (mag) & (mag)   & (mas) &  ($^\circ$)\\
\hline
2MASSWJ1207334$-$393254    &M 8    &8$^{+4}_{-3}$	& $13.00\pm0.03~^a$	 & $12.39\pm0.03~^a$	 & $11.95\pm0.03~^a$  &$11.38\pm0.10~^b$   &     & \\
giant planet candidate   &L5$-$L9.5	&               & ${\ge}18.5~^a$              & $18.09\pm0.21~^a$    & $16.93\pm0.11~^a$  &$15.28\pm0.14~^b$   &778 & 125.8   \\
\hline 
\end{tabular}}
\par
\medskip
$^{{a}}$ From the 2MASS All-Sky Catalog of Point Sources (Cutri et al. \cite{Cutri03}) and NACO contrast measurements (this paper).\\
$^{{b}}$ From $L~\!'$ Keck $I$ photometry (Jayawardhana et al. \cite{Jayawardhana03}) and NACO contrast measurements (this paper).
\end{table}