\begin{table} %t3 [b]
%\centering
\par
\caption{We give the name, ID number, 
$\alpha$, $\delta$, $V$, $V-I$, and $B-I$ for the stars with transit-like
light curves. 
All information except the adapted name in the first column 
is from Stetson \ea~(\cite{stetson03}).
The positions of the stars in the CMD is shown in Fig.~\ref{fig:cmd_n6791_transits}
and the light curves can be seen in Fig.~\ref{fig:planet_transits}.
As discussed in the text, the transits seen for T1--4, T6, and T9 are 
not likely to be due to transiting giant planets (they are marked by a $*$ symbol). 
\label{tab:n6791_transits}}
%\centering
\par
\begin{tabular}{lr|cc|ccc}
\hline\hline
\multicolumn{1}{c}{Name} & \multicolumn{1}{c}{ID} & $\alpha_{2000.0}$ & $\delta_{2000.0}$ & $V$ & $V-I$ & $B-I$ \\  
\hline
   T1$^*$&$ 4891   $& 19$^{\rm h}$20$^{\rm m}$43\fs37&$ +$37$^\circ$47\Secc31\farcs5 & 17.675 &  0.928 &  1.818 \\ %  4891  631 ; 631 = ISIS/DAO ID.
   T2$^*$&$ 6598   $& 19$^{\rm h}$20$^{\rm m}$48\fs65&$ +$37$^\circ$47\Secc41\farcs1 & 18.175 &  0.979 &  1.901 \\ %  6598 1002 ; = P5
   T3$^*$&$ 12616  $& 19$^{\rm h}$21$^{\rm m}$07\fs28&$ +$37$^\circ$47\Secc39\farcs9 & 17.718 &  0.915 &  1.809 \\ % 12616  661 ; = P3
   T4$^*$&$ 9049   $& 19$^{\rm h}$20$^{\rm m}$55\fs47&$ +$37$^\circ$44\Secc06\farcs1 & 17.493 &  1.005 &  1.839 \\ %  9049  454 ; = P0
   T5    &$ 3671   $& 19$^{\rm h}$20$^{\rm m}$39\fs07&$ +$37$^\circ$47\Secc26\farcs1 & 17.509 &  0.901 &  1.784 \\ %  3671  501 ; = P1
   T6$^*$&$ 3567   $& 19$^{\rm h}$20$^{\rm m}$38\fs63&$ +$37$^\circ$45\Secc33\farcs3 & 17.635 &  0.919 &  1.811 \\ %  3567  602 ; = P2
   T7    &$ 3723   $& 19$^{\rm h}$20$^{\rm m}$39\fs25&$ +$37$^\circ$45\Secc39\farcs3 & 18.002 &  0.954 &  1.827 \\ %  3723  878 ; = P4
   T8    &$ 9020   $& 19$^{\rm h}$20$^{\rm m}$55\fs40&$ +$37$^\circ$47\Secc23\farcs4 & 17.029 &  0.848 &  1.670 \\ %  9020  244 ; 
   T9$^*$&$ 12390  $& 19$^{\rm h}$21$^{\rm m}$06\fs48&$ +$37$^\circ$47\Secc27\farcs8 & 17.886 &  1.015 &  1.947 \\ % 12390  789 ; 
  T10$^*$&$ 8279   $& 19$^{\rm h}$20$^{\rm m}$53\fs42&$ +$37$^\circ$48\Secc14\farcs6 & 18.907 &  1.079 &  2.092 \\ 
 \hline 
\end{tabular}
\end{table}