Table 6: Data of the double stars, p for primary, s for secondary, $f_\star $ is the relative V-flux of the component.
\begin{displaymath}\begin{tabular}{l c c r@{$~~\pm$} r c l | l c c r@{$~~\pm$} r c l } \hline\hline\noal... ...&\mycl{1}{(22)}&\mycl{2}{(23)}&\mycl{2}{(24)}&\mycl{1}{(25)}&\mycl{1}{(26)}&\mycl{1}{(27)}&\mycl{1}{(28)}\\ \myendtab \end{tabular}\end{displaymath}

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