\begin{table}%t7
%\centering
\par
\caption{\label{tab:results}Summary of results from the combined SDI and radial-velocity constraints for all stars.} 
\begin{tabular}{ccccccccc}
\hline\hline \noalign{\smallskip}
\multicolumn{1}{c}{Star}& \multicolumn{1}{c}{AO (0.5$''$)}& \multicolumn{1}{c}{AO (1.0$''$)}& \multicolumn{1}{c}{SDI (0.5$''$)} & \multicolumn{1}{c}{SDI (1.0$''$)} & \multicolumn{1}{c}{$RV$ 70\%}& \multicolumn{1}{c}{RV 90\%}& \multicolumn{1}{c}{$RV$ 95\%} \\
\hline
HD25874   & 9.5--71~$M_{\rm{J}}$ & 11.2--68~$M_{\rm{J}}$ & 11.2--68~$M_{\rm{J}}$ & 11.3--67~$M_{\rm{J}}$ & 2~$M_{\rm{J}}$ & 4~$M_{\rm{J}}$ &  9~$M_{\rm{J}}$ \\
HD32778   & 8.7--72~$M_{\rm{J}}$ &   9.0--71~$M_{\rm{J}}$ &   8.9--71~$M_{\rm{J}}$ &   9.3--71~$M_{\rm{J}}$ & -- & --  & --  \\
HD91204   & 9.5 | 70~$M_{\rm{J}}$ & 10.1 | 68~$M_{\rm{J}}$ & 10.0--68~$M_{\rm{J}}$ & 10.0--67~$M_{\rm{J}}$ & 3~$M_{\rm{J}}$ & 13~$M_{\rm{J}}$ & 30~$M_{\rm{J}}$  \\
HD120780 & 8.9--66~$M_{\rm{J}}$ &   9.8 | 60~$M_{\rm{J}}$ & 10.0--59~$M_{\rm{J}}$ & 10.3--57~$M_{\rm{J}}$ & 3~$M_{\rm{J}}$ & 35~$M_{\rm{J}}$ & 23~$M_{\rm{J}}$  \\
HD145825 & 9.3--57~$M_{\rm{J}}$ & 10.9--41~$M_{\rm{J}}$ & 10.6--44~$M_{\rm{J}}$ & 11.0--40~$M_{\rm{J}}$ & 3~$M_{\rm{J}}$ & 11~$M_{\rm{J}}$ & 15~$M_{\rm{J}}$ \\
\hline
\end{tabular}
\tablefoot{Columns~2 and 3 show the AO reduced contrast limits and their associated~T5 mass limits at the age of each star for angular separations of~0.5$''$ and 1.0$''$ respectively.  Columns~4 and~5 show the same results but for the SDI reduction.  Columns 6--8 show the minimum mass that was ruled out at confidence levels of 70,~90~and~95\% respectively.  These masses were for all separations and therefore show only the lowest mass reached by the simulations and are not constrained within a separation limit.  Note the lack of this data for HD32778 due to the limited radial-velocity data~set.}
\end{table}