\begin{table}%t5
\caption{\label{tab:5}Our derived values for the mass of the planet and the major semiaxis for the four-planet fitting.}
\small%%\centerline

 {
\begin{tabular}{ccccc}
\hline\hline
\multirow{2}{*}{Planet}&
This work&
This work&
Fischer et~al. &
Fischer et~al. \\
&
$M_{\rm P}\sin~ i$ ($M_{J}$)&
\textit{a} (AU)&
$M_{\rm P}\sin~ i$ ($M_{J}$)&
\textit{a} (AU)\\
\hline
&&&& \\[-8pt]
e&
0.0361 $\pm$ 0.0014&
0.0383 $\pm$ 0.0008&
0.034 $\pm$ 0.0036&
0.038 $\pm$ $1.0\times10^{-6}$\\
b&
0.8285 $\pm$ 0.0036&
0.1148 $\pm$ $1.0\times10^{-6}$&
0.824 $\pm$ 0.007&
0.115 $\pm$ $1.1\times10^{-6}$\\
c&
0.1661 $\pm$ 0.0035&
0.2402 $\pm$ $2.1\times10^{-5}$&
0.169 $\pm$ 0.008&
0.240 $\pm$ $4.5\times10^{-5}$\\
d&
3.8201 $\pm$ 0.0117&
5.7705 $\pm$ 0.0004&
3.835 $\pm$ 0.08&
5.77 $\pm$ 0.11\\
\hline
\end{tabular}}
\medskip
For comparison, we also show the values obtained by Fischer et~al. (\cite{Fischer & Marcy}) for their five-planet model, where we have removed the fifth body.
\end{table}