\begin{table}%t6
\caption{Rotational variables belonging to the cluster. $V$ is the mean brightness value.
$T_0$ indicates the time of the maximum brightness.
The last column shows the membership
 probability (when available) or our photometric membership. The two
uncertain cases (V41 and V14) are also listed (see text).}
\small%\centering
\par
\begin{tabular}{llll ccc l ll ll}
\hline \hline
\multicolumn{1}{l}{Star} &
\multicolumn{1}{l}{Type}&
\multicolumn{1}{l}{$\alpha_{2000}$}&
\multicolumn{1}{l}{$\delta_{2000}$}&
\multicolumn{1}{c}{$V$} &
\multicolumn{1}{c}{$\langle B-V\rangle$} &
\multicolumn{1}{c}{$\langle V-I\rangle$} &
\multicolumn{1}{l}{Ref.} &
\multicolumn{1}{l}{$T_0$}&
\multicolumn{1}{l}{Period}&
\multicolumn{1}{l}{Ampl.} &
\multicolumn{1}{l}{Notes}  \\
 & & & &[mag] & [mag]& [mag] & &
\multicolumn{1}{l}{[HJD-2~452~400]}&
\multicolumn{1}{l}{[d]}&
\multicolumn{1}{l}{[mag]} &
\multicolumn{1}{l}{}  \\
\hline
 04803\_9 &    RO1 &  19.347698 &  37.796043 &   21.81 &    1.33  &    1.84 &    s & 61.799 &     1.1034 &  0.17 &         member (B06)  \\
       V82 &    RO1 &  19.344366 &  37.793381 &   19.01 &    1.00  &    1.02 &    k & 56.481 &     1.1568 &  0.04 &         likely memb.  \\
  06553\_9 &    RO1 &  19.349134 &  37.672577 &   19.26 &    1.04  &    1.13 &    s & 61.421 &     1.3485 &  0.08 &         likely memb.  \\
  01724\_9 &    RO1 &  19.344957 &  37.785362 &   20.73 &    1.29  &    1.69 &    s & 64.410 &     1.6130 &  0.17 &         likely memb.  \\
       V38 &    RO1 &  19.351021 &  37.768288 &   18.82 &    0.96  &         &    k & 55.630 &       1.96 &  0.13 &        member (92\%)  \\
  03079\_9 &    RO1 &  19.346190 &  37.754753 &   19.23 &    1.14  &    1.26 &    k & 66.630 &      2.640 &  0.07 &        member (93\%)  \\
       V14 &    RO1 &  19.347687 &  37.756874 &   18.58 &    0.93  &    1.05 &    k & 55.933 &       5.45 &  0.05 &    non-member (0\%)  \\
       V48 &    RO1 &  19.352076 &  37.718506 &   17.51 &    0.88  &         &    k & 65.223 &       5.65 &  0.09 &        member (96\%)  \\
       V17 &    RO1 &  19.344135 &  37.817928 &   17.92 &    1.20  &    1.28 &    k & 63.211 &      6.523 &  0.04 &        member (88\%)  \\
       V51 &    RO1 &  19.353382 &  37.748795 &   19.94 &    1.22  &    1.21 &    k & 63.624 &       6.72 &  0.09 &         likely memb.  \\
       V52 &    RO1 &  19.355795 &  37.771935 &   17.49 &    0.88  &    0.88 &    k & 64.345 &       7.06 &  0.03 &         likely memb.  \\
       V53 &    RO1 &  19.350233 &  37.743187 &   18.72 &    0.89  &    0.93 &    k & 69.294 &       7.47 &  0.04 &        member (86\%)  \\
  00436\_3 &    RO2 &  19.352205 &  37.878635 &   18.92 &    0.92  &    1.08 &    k & 60.018 &    0.26601 &  0.04 &         likely memb.  \\
  07483\_9 &    RO2 &  19.349997 &  37.746311 &   21.28 &    1.32  &    1.70 &    s & 60.465 &     0.4375 &  0.17 &         likely memb.  \\
       V41 &    RO2 &  19.347492 &  37.806892 &   19.09 &          &         &      & 60.000 &     0.4798 &  0.07 &        member (77\%)  \\
       V42 &    RO2 &  19.350058 &  37.714867 &   19.51 &    1.05  &    1.16 &    k & 60.323 &     0.5068 &  0.10 &        member (92\%)  \\
       V16 &    RO2 &  19.352108 &  37.802662 &   17.79 &    0.93  &    1.01 &    k & 67.713 &      2.182 &  0.03 &        member (96\%)  \\
\hline
\label{rotbel}
\end{tabular}
\end{table}