\begin{table}%t6
\caption{The  candidates  found  in   the  two cases discussed   in Sect.~\ref{s:diffapproach}. The case of the whole data-sets put together
is  indicated with  $ALL$ (1st  column), that one  for the $only$
CFHT data-set  is indicated with $CFHT$  (2nd column). A cross (x)
indicates that the candidate was found in that case,  a trait ($-$) that
it is absent. In the 3rd column, the $ID$ of the stars taken from
S03 is shown. Follow the $V$ calibrated  magnitude, the $(B-V)$ color,
the right ascension, ($\alpha$),  and the declination,  ($\delta$), of
the stars.
\label{tab:candidates}}
%\begin{center}
\par
\begin{tabular}{c c c c c c c}
\hline\hline
$ALL$ & $CFHT$ & $ID(Stetson)$ & $V$ & $(B-V)$ & $\alpha(2000)$ & $\delta(2000)$ \\
\hline\noalign{\smallskip}
 x & - & $6598$ & $18.176$ & $0.921$ & $19^{\rm h}$ $20${m} $48\fs65$ & $+37^{\circ}$ $47\arcmin$ $41\farcs1$ \\
 x & - & $4304$ & $17.795$ & $0.874$ & $19^{\rm h}$ $20${m} $41\fs39$ & $+37^{\circ}$ $43\arcmin$ $28\farcs9$ \\
 x & - & $4699$ & $17.955$ & $0.846$ & $19^{\rm h}$ $20${m} $42\fs67$ & $+37^{\circ}$ $43\arcmin$ $31\farcs5$ \\
 x & x & $1239$ & $19.241$ & $1.058$ & $19^{\rm h}$ $20${m} $25\fs42$ & $+37^{\circ}$ $47\arcmin$ $45\farcs2$ \\
 - & x & $4300$ & $18.665$ & $0.697$ & $19^{\rm h}$ $20${m} $41\fs38$ & $+37^{\circ}$ $45\arcmin$ $23\farcs3$ \\
 - & x & $7591$ & $18.553$ & $0.959$ & $19^{\rm h}$ $20${m} $51\fs51$ & $+37^{\circ}$ $48\arcmin$ $58\farcs7$ \\
\hline
\end{tabular}
%\end{center}
\par
\end{table}