\begin{table}%t3
\caption{Photometry and proper motion of the most obvious 
candidate members in the field of NGC~5385.}\label{tab3}
%\centering
\par
\begin{tabular}{ccccccccc}
\hline
\hline
\multicolumn{1}{c}{ID} &
\multicolumn{1}{c}{TYC 4558-} &
\multicolumn{1}{c}{$\alpha (J2000.0)$}&
\multicolumn{1}{c}{$\delta (J2000.0)$}&
\multicolumn{1}{c}{$V$}  &
\multicolumn{1}{c}{$(B-V)$} &
\multicolumn{1}{c}{$(U-B)$}  &
\multicolumn{1}{c}{$\mu_\alpha \cos \delta$ [mas/yr]} &
\multicolumn{1}{c}{$\mu_\delta$ [mas/yr]}  \\
\hline
   1& 1641& 13:52:54.104& +76:09:59.63&  11.29& 0.50& 0.18&   --7.5 $\pm$ 1.9&  11.7 $\pm$ 2.1\\
   2& 1385& 13:52:08.976& +76:10:55.12&  11.52& 0.39& 0.14&    2.5 $\pm$ 2.0&  --3.0 $\pm$ 2.1\\
   3&  457& 13:51:58.757& +76:13:20.41&  11.39& 0.58& 0.32&  --44.6 $\pm$ 2.0&  --6.6 $\pm$ 2.1\\
   4&  399& 13:52:18.535& +76:10:45.58&  11.31& 0.68& 0.39&  --29.0 $\pm$ 2.3&  13.8 $\pm$ 2.3\\
   5& 1797& 13:51:49.975& +76:12:11.67&  11.32& 0.72& 0.56&  --23.6 $\pm$ 2.1&  17.0 $\pm$ 2.2\\
   6& 1873& 13:52:32.078& +76:08:07.41&  11.78& 0.64& 0.33&  --42.2 $\pm$ 2.2&  26.8 $\pm$ 2.3\\
   7&  217& 13:52:34.850& +76:11:10.84&  11.77& 1.04& 1.03&  --12.5 $\pm$ 2.3&   6.5 $\pm$ 2.4\\
\hline
\end{tabular} 
\end{table}