\begin{table}%t3
\caption{\label{tab:hotjupresults}Constraints on the ``Hot'' planets from Fischer \& Valenti (\cite{fischervalenti2005}) and results from the synthetic population.} 
%%\centerline

 {\small \begin{tabular}{llll}
\hline \hline
Feature & 0.1~AU & 0.01~AU & Obs. const. (FV05)\\
\hline
Nb. of detectable synth. planets with the FV05 bias outside feeding limit & \multicolumn{2}{c}{3382}  & -- \\
Detection probability with FV05 bias excluding ``Hot'' planets ($\pfv$) [\%] & \multicolumn{2}{c}{4.8} & $4.5\pm0.7$ \\
Nb. of ``Hot'' synth. planets detectable with the FV05 bias   &  259 & 407 & -- \\
Detection probability with FV05 bias including ``Hot'' planets ($\pfvwhot$) [\%]  & 5.2 &5.4 & $\geq$$5.5\pm0.8$\\
Fraction of ''Hot'' detectable planets of all FV05 detectable planets ($\ffv$) [\%]&  7.1 & 10.7& $\geq$$ 19 \pm 6 $\\ 
\hline
\end{tabular}}
\medskip
The two columns 0.1 and 0.01~AU represent the results if such final semimajor axes for the synthetic ``Hot'' planets are assumed.
\end{table}