\begin{table}%t4
%%\centering

\par
\caption{\label{pipeline_res}Pipeline results for real data: rotation period, mean large separation, frequency-range of the p~modes, position of maximum amplitude, and bolometric maximum amplitude per radial mode.}
\begin{tabular}{cccccccccc}
\hline \hline \noalign{\smallskip}
Star& Period (days)&$\langle \Delta \nu \rangle$ ($\mu$Hz) & $\epsilon$ ($\mu$Hz)& $f_{\rm min}$ ($\mu$Hz) & $f_{\rm max}$ ($\mu$Hz)& $\nu_{\rm max}$ ($\mu$Hz)& $\epsilon$ ($\mu$Hz)& A$_{\rm max}$ (ppm)&  $\epsilon$ (ppm)\\
\hline
Sun & 27.8 & 135.46 & 3.26 & 2040&4920 & 3074.7&1.02 & 2.99& 0.13 \\
HD49933 (1) & 3.2 & 86.14& 1.58& 720& 3060& 1699.88& 1.05&4.08 &0.15\\
HD49933 (2) & 3.3 & 86.33& 1.73& 720& 3000& 1804.34& 0.28&3.90 &0.08\\
HD181906& 2.8 & 86.53& 1.69& 1200& 2460& 1896.9& 1.2& 2.85& 0.13\\
HD181420&  2.6 & 75.35& 1.53& 480& 2760& 1536.26& 0.42 & 3.89&0.1\\
\hline
\end{tabular}
\vspace*{5mm}
\end{table}