\begin{table}%TA.3
%\centering
\small
  \caption{Properties of the SHT dataset that we use in our analysis. Note that not all candidate companions are listed here, as in our analysis we only consider single stars and binary systems. The six members at the bottom of the list were not explicitly observed by SHT. Due to the presence of (known) close companions these were not suitable for wavefront sensing. We have included these targets for our analysis to avoid a bias towards low binarity. \label{table: data_tokovinin}}
  \begin{tabular}{lccc cr ccc}
    \hline
    \hline
  HIP & $K_{\rm S,1}$ & $K_{\rm S,2}$ & $\Delta K_{\rm S}$ & $\rho$  & $\varphi$ & $M_1$     & $M_2$     & $q$ \\
      & mag       & mag       & mag          & arcsec  & deg       & $\msun$ & $\msun$ &     \\
    \hline
    \input{7719ta3}
    \hline
  \end{tabular}
\end{table}