\begin{table}%t5 \caption{\label{stats}Detection limit for 50$\%$ and 90$\%$ for different periods.} \par \small%\centerline { \begin{tabular}{l l l l l } \hline \hline ST, \vsini & Period & 50$\%$ & 90$\%$ & $N$-st.$^\star$ \\ & [days] & [\Mjup] & [\Mjup] & \\ \hline early A, \vsini~$\leq$ 70~\kms & 3 & 1.2 & -- & 2 \\ & 10 & 1.7 & -- & 2 \\ & 200 & 4.7 & -- & 2 \\ & 500 & 6.4 & -- & 2 \\ early A, \vsini~70--130~\kms & 3 & 4.6 & 7.2 & 9 \\ & 10 & 6.9 & 10.7 & 9 \\ \hline A, \vsini~$\leq$ 70~\kms & 3 & 3.5 & -- & 2 \\ A, \vsini~70--130~\kms & 3 & 4.5 & 6.3 & 10 \\ & 10 & 6.7 & 9.5 & 10 \\ A, \vsini~$\geq$ 130~\kms & 3 & 11.2 & & 13 \\ \hline F, \vsini~$\leq$ 15~\kms & 3 & 0.1 & 0.8 & 28 \\ & 10 & 0.2 & 1.2 & 28 \\ & 200 & 0.4 & 3.2 & 25 \\ & 500 & 0.6 & 2.7 & 22 \\ F, \vsini~15--60~\kms & 3 & 0.6 & 0.8 & 13 \\ & 10 & 0.9 & 1.2 & 13 \\ & 200 & 2.8 & 3.3 & 12 \\ & 500 & 3.8 & 4.5 & 12 \\ F, \vsini~$\geq$ 60~\kms & 3 & 1.9 & 10.2 & 10 \\ & 10 & 2.8 & & 10 \\ & 200 & 7.5 & & 9 \\ & 500 & 10.1 & & 9 \\ \hline \end{tabular}} \medskip $^\star$ Number of stars considered to estimate these detection limits. Note: only stars with more than 12~measurements (6~epochs) were considered, binaries were excluded, and numbers outside the planetary mass domain ($>$$13$~\Mjup) are not given. \end{table}