\begin{table}%t3
\caption{\label{spv-prop}Properties of the short period stars.}
%\centerline
 {\small \begin{tabular}{l c c r r r}
\hline\hline
ID & $\alpha$~[hms]&$\delta$~[dms]&$d~[\arcsec]$&$f$~[d$^-1$]&$SNR$\\
\hline
V73   &   13:13:03.1   &   18:09:26.1   &   119.9 &14.26581 &  10.2   \\
 V74   &   13:12:49.7   &   18:07:26.3   &   181.9   &    22.03949      &   13.7   \\
 V75   &   13:13:09.4   &   18:09:39.5   &   203.9   &    22.60022      &   11.8   \\
 V76   &   13:13:05.0   &   18:08:35.3   &   168.4   &    24.10224      &   10.4   \\
 V77*  &   13:13:20.8   &   18:15:34.9   &   488.3   &    13.00995      &   23.0   \\
 V78*  &   13:12:49.8   &   18:08:56.0   &   106.9   &    22.25488      &   12.7   \\
 V79*  &   13:12:46.6   &   18:11:36.9   &   150.6   &    21.59184      &    9.7   \\
\hline
 V80*  &   13:12:57.4   &   18:10:13.8   &    31.3   &    14.83029      &   14.2   \\
 V81*  &   13:13:02.7   &   18:06:29.4   &   244.5   &    14.01180      &    9.5   \\
 V82*  &   13:12:56.5   &   18:13:10.0   &   181.1   &    45.33103      &    8.4   \\
 V83*  &   13:12:50.1   &   18:07:42.9   &   164.5   &     8.01907      &    8.2   \\
\hline
\end{tabular}}
\medskip
Notes: new discoveries are marked with asterisks. The signal-to-noise ratio (SNR) was calculated in the  $[0,50]$~d$^{-1}$ frequency range. See Table~\ref{rrlprop} for other notations.
\end{table}