\begin{table}%TA.1

%\centering
\small
  \caption{Properties of the KO5 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 members \object{HIP~68532} and \object{HIP~69113} (marked with a star) both have two companions with a similar separation, position angle, and brightness. In our analysis we consider these "double companions'' as a single companion. \label{table: data_adonis}}
%\setlength{\LTcapwidth}{1.0\textwidth}
\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{7719ta1}
  \hline
\end{tabular}
\end{table}