\begin{table}%t7
%\centering
\par
\caption{Radial velocities of the candidate binary systems identified in the
$\lambda$ Ori cluster sample.}\label{tab:vr_bin_lori} 
\small \begin{tabular}{ccccccccc}
\hline \hline
 & \multicolumn{8}{c}{JD-2453600.00}\\ 
   & 58.86 &  59.86 & 60.84 & 84.82 & 86.78  & 86.82 & 86.85 & 97.74\\ 
\hline\noalign{\smallskip}
ID & RV (km~s$^{-1}$) & RV (km~s$^{-1}$)  & RV (km~s$^{-1}$)  & RV(km~s$^{-1}$)  & RV (km~s$^{-1}$)  & RV (km~s$^{-1}$) & RV (km~s$^{-1}$) & RV (km~s$^{-1}$) \\ 
 \hline
L01  &  $25.41\pm1.06$ &  $29.09\pm1.25$ &  $24.36\pm1.05$ &  $25.65\pm0.97$ &  $24.05\pm0.74$ &  $25.03\pm1.16$ &  $24.98\pm0.91$ &  $24.31\pm1.46$ \\
L03  &  $19.48\pm0.41$ &  $20.98\pm0.49$ &  $20.13\pm0.37$ &  $20.91\pm0.41$ &  $20.89\pm0.54$ &  $20.91\pm0.75$ &  $21.01\pm0.62$ &  $32.16\pm0.92$ \\
L10a &  $27.18\pm0.66$ &  $29.27\pm1.44$ &  $28.14\pm0.73$ &  $-1.29\pm1.88$ &  $-2.48\pm1.90$ &  $-1.66\pm2.06$ &  $-1.33\pm1.90$ &  $26.59\pm0.66$ \\
L10b &  $27.18\pm0.66$ &  $29.27\pm1.44$ &  $28.14\pm0.73$ &  $30.49\pm2.80$ &  $29.34\pm2.99$ &  $29.71\pm2.57$ &  $29.19\pm2.58$ &  $26.59\pm0.66$ \\
L22  &  $24.40\pm1.43$ &  $28.26\pm2.58$ &  $29.54\pm1.31$ &  $24.54\pm1.67$ &  $27.19\pm1.15$ &  $27.57\pm0.97$ &  $27.60\pm0.88$ &  $23.27\pm1.33$ \\
L32  &  $25.41\pm2.88$ &  $24.66\pm3.28$ &  $16.12\pm3.85$ &  $28.19\pm2.63$ &  $25.35\pm2.98$ &  $24.67\pm3.96$ &  $25.16\pm2.67$ &  $34.81\pm5.05$ \\
\hline
\end{tabular}
\end{table}