\begin{table}%T4
 \caption{\label{tableHD49933prior}Priors used for HD~49933 data analysis. $\nu_{\rm s}$ is the rotational splitting, $i$ the star inclination angle, $\delta\nu_{02}$ the small frequency separation, $\Delta\nu$ the large separation. The value of $\epsilon$ and $D_0$ depend on the model and set the position of the first prior frequency (see Eq.~(\ref{Assymptotic_relation})).}
\par
\small%\centerline
{
\begin{tabular}{cccc}
\hline\hline
Parameter & Prior nature & Values \\ 
\hline
$\nu_{\rm s}$ & Gaussian & $3.4\pm0.34$ $\mu {\rm{Hz}}$ \\
$i$ & Uniform & $[0^\circ{-}90^\circ]$ \\
$\delta \nu_{02}$ & Gaussian & $6 \pm 3$~$\mu {\rm{Hz}}$\\
$\Delta\nu$ & Gaussian & $85.6 \pm 0.8$~$\mu {\rm{Hz}}$\\
$\epsilon$ & Fixed & 1.55 ($M_{\rm A}$) / 1.05 ($M_{\rm B}$)\\
$D_0$ & Fixed & 1 $\mu {\rm{Hz}}$\\ 
\hline
\end{tabular}}
%\centerline
{
\begin{tabular}{cccc}
Parameter             & Prior nature & $x_{\rm min}$ & $x_{\rm max}$ \\
 \hline\noalign{\smallskip}
$h$ (ppm$^2$/$ \mu Hz)$ & Jeffrey      &     1    &   10 \\
$V_{l=1}$             & Jeffrey      &     1.5  &   5  \\
$V_{l=2}$             & Jeffrey      &     0.5  &   5  \\
$\Gamma$ $(\mu {\rm{Hz}})$     & Jeffrey      &     5    &   25  \\
\hline
\end{tabular}}
\smallskip
$\nu_{\rm s}$ is the rotational splitting, $i$ the star inclination angle, $\delta\nu_{02}$ the small frequency separation, $\Delta\nu$ the large separation. The value of $\epsilon$ and $D_0$ depend on the model and set the position of the first prior frequency (see Eq.~(\ref{Assymptotic_relation})). 
\end{table}