\begin{table}%T7
\caption{Long period variable stars that are likely members 
 of NGC~6791 (ordered by increasing right ascension). Column~9 shows the membership probability (when available) or our photometric membership.}
 \small%\centering
\par
\begin{tabular}{lllccclllr}
\hline \hline
\noalign{\smallskip}
\multicolumn{1}{l}{Star} &
\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}{Ampl.} &
\multicolumn{1}{l}{Notes}&
\multicolumn{1}{r}{Distance}\\
 & & & [mag] & [mag] & [mag] & & [mag] & & arcmin \\
\hline
  02138\_8  &   19.341864 &  37.749653 &   19.68 &    1.12  &    1.18 &    k &   0.06 &         likely memb.  &   4.6  \\
  02444\_8  &   19.342766 &  37.810604 &   18.34 &    0.93  &    1.00 &    k &   0.02 &        member (78\%)  &   4.4  \\
  00510\_9  &   19.343704 &  37.796719 &   18.67 &    0.94  &    0.98 &    k &   0.03 &        member (83\%)  &   3.4  \\
  01610\_9  &   19.344818 &  37.740486 &   19.09 &    1.01  &    1.05 &    k &   0.02 &         likely memb.  &   3.0  \\
       V94  &   19.345139 &  37.743549 &   17.54 &    0.88  &    0.92 &    k &   0.03 &        member (90\%)  &   2.7  \\
       V95  &   19.345295 &  37.792412 &   19.16 &    1.03  &    1.10 &    k &   0.07 &        member (93\%)  &   2.3  \\
 V56(=V96)  &   19.345908 &  37.763525 &   17.01 &    0.95  &    0.97 &    k &   0.04 &        member (98\%)  &   1.6  \\
  04392\_3  &   19.345982 &  37.870571 &   17.90 &    0.88  &    0.92 &    k &   0.02 &         likely memb.  &   6.1  \\
       V75  &   19.346651 &  37.766308 &   17.38 &    0.94  &    0.98 &    s &   0.01 &         likely memb.  &   1.0  \\
  04133\_9  &   19.347109 &  37.777020 &   18.47 &    0.94  &    0.98 &    k &   0.04 &        member (98\%)  &   0.7  \\
 V76(=V85)  &   19.347192 &  37.764169 &   18.19 &    1.03  &    1.15 &    k &   0.11 &        member (97\%)  &   0.8  \\
       V86  &   19.347258 &  37.808815 &   19.44 &    1.06  &    1.14 &    k &   0.03 &        member (83\%)  &   2.3  \\
       V87  &   19.347996 &  37.749668 &   18.12 &    0.91  &    0.93 &    k &   0.03 &        member (98\%)  &   1.3  \\
  05740\_9  &   19.348534 &  37.808022 &   17.96 &    0.93  &         &    k &   0.03 &        member (95\%)  &   2.2  \\
  06725\_9  &   19.349329 &  37.724495 &   17.77 &    0.91  &         &    k &   0.02 &        member (91\%)  &   3.0  \\
  06796\_9  &   19.349415 &  37.769268 &   18.46 &    0.92  &    1.04 &    k &   0.03 &        member (92\%)  &   1.0  \\
       V90  &   19.349686 &  37.746449 &   18.11 &    0.86  &    0.94 &    k &   0.01 &        member (94\%)  &   1.9  \\
  07680\_9  &   19.350193 &  37.718224 &   18.32 &    0.89  &    0.97 &    k &   0.03 &        member (98\%)  &   3.5  \\
       V31  &   19.350683 &  37.785912 &   17.12 &    1.00  &    1.02 &    k &   0.01 &        member (97\%)  &   2.1  \\
  09376\_9  &   19.351952 &  37.831886 &   18.21 &    1.00  &    1.02 &    k &   0.01 &        member (92\%)  &   4.6  \\
  09611\_9  &   19.352139 &  37.773365 &   17.97 &    0.85  &    0.91 &    k &   0.01 &        member (76\%)  &   2.9  \\
       V58  &   19.354042 &  37.801240 &   17.52 &    0.89  &    0.94 &    k &   0.05 &        member (87\%)  &   4.6  \\
 02268\_10  &   19.359475 &  37.731544 &   18.59 &    0.95  &    0.99 &    k &   0.02 &         likely memb.  &   8.5  \\
 \hline
\label{lptab}
\end{tabular}
\end{table}