\begin{table}%t2 \caption {\label{radvel}Heliocentric radial velocities measurements and their 1$\sigma$ errors ($V_{\rm r} \pm \delta V_{\rm r}$)$_{\rm here}$ for each program star.} %\centerline {\begin{tabular}{l l c c c c} \hline\hline \noalign{\smallskip} Cluster & Star & $(V_{\rm r}\pm\delta V_{\rm r})_{\rm here}$ & $(V_{\rm r}\pm\sigma V_{\rm r})_{\rm lit}$ \\ & &(km~s$^{-1}$) &(km~s$^{-1}$) \\ \hline Cr~110 & 2108 & 44.47 $\pm$ 0.54 & $45\pm8$\tablefootmark{a} \\ & 2129 & 38.74 $\pm$ 0.64 & $45\pm8$$^a$ \\ & 3144 & 37.81 $\pm$ 0.69 & $45\pm8$$^a$ \\ NGC~2099 (M~37) & 067 & 8.79 $\pm$ 0.10 & 8.04 $\pm$ 0.19\tablefootmark{b} \\ & 148 & 9.05 $\pm$ 0.36 & 8.73 $\pm$ 0.19$^b$ \\ & 508 & 9.40 $\pm$ 0.28 & 8.96 $\pm$ 0.19$^b$ \\ NGC~2420 & 041 & 74.23 $\pm$ 0.87 & 79.0 $\pm$ 4.2\tablefootmark{c} \\ & 076 & 75.49 $\pm$ 0.41 & 75.7 $\pm$ 8.6$^c$ \\ & 174 & 73.66 $\pm$ 1.17 & 68.0 $\pm$ 0.9$^c$ \\ NGC~2682 (M~67) & 141 & 35.23 $\pm$ 0.05 & 33.5 $\pm$ 2.3\tablefootmark{d} \\ & 223 & 34.92 $\pm$ 0.31 & 33.0 $\pm$ 1.1$^d$ \\ & 286 & 38.90 $\pm$ 0.46 & 33.2 $\pm$ 2.0$^d$ \\ NGC~7789 & 5237 & --51.06 $\pm$ 0.99 & --57.17 $\pm$ 0.23\tablefootmark{e} \\ & 7840 & --49.06 $\pm$ 0.81 & --49.21 $\pm$ 0.28$^e$ \\ & 8556 & --53.37 $\pm$ 0.81 & --54.10 $\pm$ 0.32$^e$ \\ \hline \end{tabular}} \par \tablefoot{Literature measurements, when available, are also reported with their uncertainties ($V_{\rm r} \pm \delta V_{\rm r}$)$_{\rm lit}$.} \tablefoottext{a}{Cluster average by \citet{ricardo}, based on 8 stars.} \tablefoottext{b}{\citet{mer08}, superseding \citet{mer96}.} \tablefoottext{c}{Average of measurements by \citet{liu87}, \citet{friel89} and \citet{scott95}.} \tablefoottext{d}{Average of measurements by \citet{mat86}, \citet{pil88}, \citet{friel89}, \citet{friel93}, \citet{sun92}, \citet{scott95}, \citet{melo01}, \citet{yong05}, \citet{yad08}.} \tablefoottext{e}{\citet{gim98a}.} \end{table}