\begin{table}%t2
\caption{\label{tab:orbit}Orbital parameters of HD~45364b and HD~45364c from different fits.}
\par
\small%\centering
\par
\begin{tabular}{llllll}
\hline\hline
\noalign{\smallskip}
& &\multicolumn{2}{l}{\cite{CorreiaUdry2008}} & \multicolumn{2}{l}{Simulation \texttt{F5}}  \\
Parameter& Unit & b & c  & b & c \\
\hline
$M \sin i$ & $[{M}_{{\rm Jup}}]$ 		& 0.1872 & 0.6579 			& 0.1872 & 0.6579 		 		\\
$M_*$ &  $[M_{\odot}]$ 				&\multicolumn{2}{c}{0.82} 		& \multicolumn{2}{c}{0.82} 			\\
$a$ &$[\mbox{AU}]$				& 0.6813 & 0.8972 			& 0.6804 & 0.8994  	 	\\
$e$ 	&		& 			$ 0.17\pm 0.02$ & $0.097 \pm0.012$ 	& 0.036  & 0.017  		\\
$\lambda$ & $[\mbox{deg}]$ 			& $105.8 \pm1.4$ & $269.5\pm0.6$ 	& 352.5 & 153.9 		\\
$\varpi$\tablefootmark{a} & $[\mbox{deg}]$ 			& $162.6 \pm6.3$ & $7.4\pm4.3$ 		& 87.9& 292.2		\\
$\sqrt{\chi^2}$ &				& \multicolumn{2}{c}{2.79} 		& \multicolumn{2}{c}{2.76\tablefootmark{b} (3.51)} 	\\
Date  &[JD]					& \multicolumn{2}{c}{2~453~500} 		& \multicolumn{2}{c}{2~453~500}  	\\
\hline
\end{tabular}
\tablefoot{\tablefoottext{a}{Note that $\varpi$ is not well constrained for nearly circular orbits.}
\tablefoottext{b}{radial velocity amplitude was scaled down by~$8\%$.}}
\end{table}