\begin{table}%t4
\caption{\label{tbl:planets}Planetary solutions from radial velocity orbit fitting. See  text for details.} 
%\centerline
 {\begin{tabular}{lrrr}
\hline\hline
Parameters  & \multicolumn{2}{c}{Solutions using filtering  algorithm}& Adopted solution\\
& \multicolumn{1}{c}{with the Pre-whitening} & \multicolumn{1}{c}{with the rotation harmonics}&   \\
\hline
\multicolumn{4}{c}{{\bf \corotp}}\\
Period [days]  &  0.85353 $\pm 2\times 10^{-5}$&0.8536 (fixed)&$0.853585\pm2.4\times 10^{-5}$ ($^\ddagger$)\\
$T_{\rm tr}$ [JD] & $2~454~446.7311$ (fixed)&$2~454~446.721\pm0.028$&2~454~446.731 $\pm$ 0.003 ($\ddagger$)\\
$T_{0}$ [JD] & &$2~454~446.508\pm0.029$&\\
$K$ [m~s$^{-1}$] & (4.16 $\pm$  0.27)$^\dagger$ 3.33 $\pm$  0.27 ($\pm 1$)$^\star$&(1.9 $\pm$  0.4)$^\dagger$ 3.8 $\pm$  0.8&$3.5\pm0.6$\\
$e$               & 0.07  $\pm$ 0.067 & 0 (fixed)&0\\
$\omega$ [deg]    & 91.55 $\pm$ 49.27 &180 (fixed)&180\\
\\
$m$  [\Me]       &$4.5\pm1$&$5.2\pm 1$ &4.8 $\pm$ 0.8\\
$a$ [AU] &&&0.017 \\
\hline
\multicolumn{4}{c}{{\bf \corotc}}\\
Period [days]  & 3.701 $\pm$ 0.004  &3.692 $\pm$ 0.008&3.698 $\pm$ 0.003\\
$T_{0}$ [JD] & $2~454~445.34\pm1.07$  &$2~454~444.73\pm0.87$&2~454~445.0 $\pm$ 0.7\\
$K$ [m~s$^{-1}$] & (5.5 $\pm$  0.3)$^\dagger$  $4.4\pm0.3$ ($\pm $1)$^\star$  &(3.5 $\pm$  0.4)$^\dagger$  $3.8\pm0.5$&$4.0\pm0.5$\\
$e$               & 0.028 $\pm$ 0.048  &0 (fixed)&0\\
$\omega$ [deg]    & 140 $\pm$ 98  &180 (fixed)&180\\
\\
$m$  [\Me]       & 9.4 $\pm$ 2.1 ($^\ast$) & 8.1 $\pm$ 0.9 ($^\ast$)&8.4 $\pm$ 0.9 \\
$a$ [AU] && &0.046\\
\hline
$\sigma \rm (O{-}C)$ [\ms]& 1.81 &2.82&\\
$\chi_{\rm red}$&1.2&1.3&\\
\hline
\end{tabular}}
\par
Notes: ($^\dagger$) Uncorrected amplitude solution from filtering effects. ($^\star$) Systematic error resulting from the filtering process. ($^\ddagger$) Adopted from \citet{Leger09}, ($^\ast$) assuming \corotp and \corotc are on  coplanar orbits ($\sin i=80^0 $).
\end{table}