\begin{table}%t2
\caption{\label{t2}Properties of the targeted member stars.}             
%\centerline
{          
\begin{tabular}{ccccccc}     
\hline\hline       
& $\alpha$  & $\delta$ & $V_0$ & $(B-V)_0$ & $(V-K)_0$ & $S/N$$^a$  \\
\raisebox{1.5ex}[-1.5ex]{ID} & (J2000.0) & (J2000.0)  & [mag] & [mag] & [mag] & [pixel$^{-1}$] \\
%
\hline
Pal3-2    & 10 05 31.57 & +00 04 17.0 & 18.11 & 1.13 &  2.73 & 7 / 44 \\
Pal3-3    & 10 05 37.08 & +00 04 27.9 & 18.22 & 1.11 &  2.57 & 7 / 32  \\
Pal3-5    & 10 05 30.70 & +00 04 04.2 & 18.35 & 1.07 &  2.52 & 7 / 36 \\
Pal3-6$^b$& 10 05 29.71 & +00 05 39.2 & 18.50 & 0.95 &  3.47 & 7 / 31 \\
Pal3-8    & 10 05 31.05 & +00 04 17.3 & 18.64 & 1.01 &  3.45 &  6 \\
Pal3-15   & 10 05 34.63 & +00 04 06.9 & 19.20 & 0.89 & \dots &  5 \\
Pal3-16   & 10 05 31.84 & +00 04 16.5 & 19.24 & 0.89 & \dots &  6 \\
Pal3-17   & 10 05 32.87 & +00 04 36.1 & 19.32 & 0.85 & \dots &  6 \\
Pal3-18   & 10 05 33.19 & +00 03 57.1 & 19.30 & 0.90 & \dots &  6 \\
Pal3-21   & 10 05 34.04 & +00 05 13.5 & 19.43 & 0.88 & \dots &  7 \\
Pal3-22   & 10 05 31.12 & +00 04 16.9 & 19.49 & 0.89 & \dots &  6 \\
Pal3-24   & 10 05 32.91 & +00 04 26.1 & 19.69 & 0.86 & \dots &  5 \\
Pal3-26   & 10 05 32.59 & +00 04 32.3 & 19.77 & 0.83 & \dots &  6 \\
Pal3-29   & 10 05 32.73 & +00 04 36.7 & 19.85 & 0.84 & \dots &  5 \\
Pal3-35   & 10 05 30.25 & +00 03 37.6 & 20.02 & 0.81 & \dots &  6 \\
Pal3-36   & 10 05 29.92 & +00 04 53.9 & 20.03 & 0.80 & \dots & 5 \\
Pal3-38   & 10 05 28.79 & +00 03 45.5 & 20.10 & 0.80 & \dots &  4 \\
Pal3-40   & 10 05 28.83 & +00 04 36.5 & 20.11 & 0.79 & \dots &  5 \\
Pal3-41   & 10 05 29.97 & +00 04 03.8 & 20.14 & 0.79 & \dots &  5 \\
\hline                  
\end{tabular}}
\par
\medskip
$^a$ The second number for the first 4 stars gives the $S/N$ from the MIKE spectra.\\
$^b$ AGB star (Hilker \cite{Hilker06}).
\end{table}