\begin{table}%t8
\caption{\label{tab:lowmasscomp2}Detached eclipsing binaries that may have a low mass component.}
%\centering
\par
\begin{tabular}{lllllllll}
\hline\hline \noalign{\smallskip}
ID & Subset & Right ascension & Declination & \multicolumn{3}{c}{Calibrated magnitudes} & Period & Type \\ 
& &(J2000.0) & (J2000.0) & $R$ & $B-R$ & $R-I$ & (days) & \\
\hline
V-1106 & 6G & 16:18:55.35 &--53:28:34.7387 & 18.83 & 2.19 & 0.73 & 0.4983 & EA \\
V-992 & 6A & 16:18:45.09 &--53:39:45.9131 & 19.46 & 2.46 & 1.48 & 0.4095 & EA \\
V-790 & 4H & 16:17:28.84 &--53:10:42.0607 & 17.83 & 2.09 & 0.37 & 0.4711 & EA \\
V-244 & 2C & 16:19:37.54 &--53:18:34.5958 & 18.35 & 2.84 & 1.14 & 0.5610 & EA \\
V-755 & 4G & 16:17:58.34 &--53:11:39.78 & 20.63 & 3.00 & 1.28 & 0.6861 & EA \\
V-611 & 4A & 16:18:02.91 &--53:23:07.2723 & 18.33 & 2.37 & 0.50 & 0.7061 & EA \\
V-979 & 6A & 16:18:46.94 &--53:41:25.8984 & 18.57 & 2.91 & 0.43 & 0.8337 & EA \\
V-894 & 5E & 16:18:05.07 &--53:31:34.5940 & 19.24 & 1.60 & 1.65 & 0.7043 & EA \\
V-52 & 1B & 16:20:11.65 &--53:24:02.0859 & 16.28 & 1.86 & 0.19 & 1.1242 & EA \\
\hline
\end{tabular}
\end{table}