\begin{table}%t3[!htp]
\caption{Membership probabilities  from proper motions  and positions in 
the CMD for the 11~stars with radial velocities implying membership of 
Palomar~13.}\label{tablemembership}
%\centering
\par
%\LTleft=\parindent 
%\LTright=\fill 
%\setlongtables 
\begin{tabular}{cccrrcccccc}
\hline 
\hline 
\multicolumn{1}{c}{ID}  & \multicolumn{1}{c}{$\alpha_{\rm J2000}$}
& \multicolumn{1}{c}{$\delta_{\rm J2000}$}  &
\multicolumn{1}{c}{$\mu$($\alpha$)} &
\multicolumn{1}{c}{$\mu$($\delta$)} & \multicolumn{1}{c}{P($\mu$)}  &
\multicolumn{1}{r}{\ensuremath{V_{\rm r}} FLAMES}    & \multicolumn{1}{c}{$U$}   & \multicolumn{1}{c}{$B$}   & \multicolumn{1}{c}{$V$}   & \multicolumn{1}{c}{CMD} \\
           & \multicolumn{1}{c}{[$^{\rm h\;\;m\;\;s}$]} & 
	     \multicolumn{1}{c}{[$^\circ\; ^\prime\; ^{\prime\prime}$]} & 
	     \multicolumn{1}{c}{[mas~yr$^{-1}$]}          & 
	     \multicolumn{1}{c}{[mas~yr$^{-1}$]}          & 
	     \multicolumn{1}{c}{[\%]}        & 
	     \multicolumn{1}{c}{[km~s$^{-1}$]}      & 
	     \multicolumn{1}{c}{[mag]}   & \multicolumn{1}{c}{[mag]}   & \multicolumn{1}{c}{[mag]}  \\
\multicolumn{1}{c}{(1)} & \multicolumn{1}{c}{(2)}       & \multicolumn{1}{c}{(3)}       & \multicolumn{1}{c}{(4)}             & \multicolumn{1}{c}{(5)}             & \multicolumn{1}{c}{(6)}       & \multicolumn{1}{c}{(7)}      & \multicolumn{1}{c}{(8)}   & \multicolumn{1}{c}{(9)}   & \multicolumn{1}{c}{(10)}  & \multicolumn{1}{c}{(11)} \\
\hline
  38 & 23 06 41.55 & 12 46 58.5 & $ 0.32 \pm 0.11$ & $ 0.05 \pm 0.19$ & 48 & 21.39 & $18.432 \pm 0.020$ & $18.335 \pm 0.010$ & $17.808 \pm 0.007$ &  RRL   \\
 112 & 23 06 39.37 & 12 47 35.1 & $-0.31 \pm 0.16$ & $ 0.59 \pm 0.29$ & 89 & 24.36 & $20.134 \pm 0.042$ & $20.070 \pm 0.021$ & $19.276 \pm 0.014$ &  SGB   \\
  22 & 23 06 37.31 & 12 49 26.8 & $-0.22 \pm 0.07$ & $-0.02 \pm 0.10$ & 96 & 24.82 & $18.148 \pm 0.023$ & $17.761 \pm 0.012$ & $16.897 \pm 0.007$ &  RGB   \\
  24 & 23 06 50.11 & 12 47 14.9 & $ 0.24 \pm 0.19$ & $ 1.6  \pm 0.16$ &  0 & 25.39 & $18.334 \pm 0.020$ & $17.983 \pm 0.011$ & $17.005 \pm 0.007$ &  off-r?\\
  41 & 23 06 49.95 & 12 45 28.7 & $-0.05 \pm 0.12$ & $-0.25 \pm 0.12$ & 79 & 25.76 & $18.854 \pm 0.022$ & $18.658 \pm 0.011$ & $17.795 \pm 0.007$ &  RGB   \\
  79 & 23 06 44.30 & 12 45 49.4 & $ 0.22 \pm 0.16$ & $-0.36 \pm 0.18$ & 65 & 25.76 & $19.418 \pm 0.027$ & $19.386 \pm 0.014$ & $19.021 \pm 0.012$ &  BS?   \\
 188 & 23 06 45.76 & 12 46 41.4 & $-0.18 \pm 0.20$ & $ 0.09 \pm 0.23$ & 99 & 25.96 & $20.535 \pm 0.058$ & $20.529 \pm 0.024$ & $19.834 \pm 0.018$ &  SGB   \\
  37 & 23 06 48.51 & 12 46 19.8 & $ 0.00 \pm 0.09$ & $ 0.32 \pm 0.09$ & 88 & 26.32 & $18.757 \pm 0.023$ & $18.537 \pm 0.011$ & $17.625 \pm 0.007$ &  RGB   \\
 127 & 23 06 31.29 & 12 43 36.0 & $-4.4  \pm 0.77$ & $-6.2  \pm 0.54$ &  0 & 26.44 & $21.740 \pm 0.185$ & $20.579 \pm 0.034$ & $19.305 \pm 0.018$ &  off-r \\
  66 & 23 06 48.28 & 12 45 47.2 & $-0.41 \pm 0.13$ & $ 0.03 \pm 0.14$ & 88 & 26.69 & $19.427 \pm 0.028$ & $19.361 \pm 0.014$ & $18.583 \pm 0.010$ &  SGB   \\
  88 & 23 06 43.82 & 12 45 36.4 & $-0.30 \pm 0.18$ & $-0.20 \pm 0.20$ & 93 & 27.97 & $19.842 \pm 0.033$ & $19.727 \pm 0.016$ & $18.970 \pm 0.011$ &  SGB   \\
\hline
\end{tabular}
\end{table}