\begin{table}%t4
\caption{\label{lpv-prop}Properties of the long period variables.}
%\centerline
{
\small 
\begin{tabular}{l l c c r c c c c}
\hline\hline\noalign{\smallskip}
ID    & $\alpha$~[hms] & $\delta$~[dms] &  $d~[\arcsec]$ &   $P$~[d]  &   $SNR$    &    $V$    &  $V-I$\\ 
\hline
 V84  &   13:12:36.2   &  18:07:32.3    &   306.6   &    22.4     &   15.5   &   14.766  &  1.175    \\ 
 V85  &   13:12:50.7   &  18:10:39.7    &    69.7   &    19.8     &   19.2   &   13.962  &  1.357    \\ 
 V86  &   13:12:52.7   &  18:10:28.0    &    39.4   &    22.2     &   12.9   &   $\sim$14.2  &    \dots     \\ 
\hline
\end{tabular}}
\medskip
Notes: for variable V86, only instrumental $V$ magnitude average is shown 
because the star was saturated in the $I$ band. The signal-to-noise ratio (SNR)  was calculated in the $[0,20]$~d$^{-1}$ frequency range.
\end{table}