\begin{table}%t1
\caption{\label{tablehbr}$\HBR$  and parameters of the p mode envelope for CoRoT targets.}
%\centerline
{
\begin{tabular}{rllrllccccc}
\hline\hline
Star & Type &  $m\ind{V}$& $t$ & $\numax$ & $\HWHM$ & $\dnumoy$ & $\alpha$ & $\gamma$ & $\HBR$ & $\ampmax$\\
&&& (day) &\multicolumn{2}{c}{\dotfill (mHz) \dotfill}& (\muHz) & \\
\hline
HD~49385$^a$   & G0IV& 7.41 & 136.9 &   1.00 & 0.54 & 56 & 0.95 & 9.7& 0.90 &  452\\
HD~49933$^{b1}$& F5V & 5.78 & 136.9 &   1.79 & 0.86 & 85 & 1.10 &10.1& 0.75 &  562\\
HD~49933$^{b2}$&     &      & 60.7  &        &      &    &      &    &      &  237\\
HD~175726$^c$  & G0V & 6.72 & 27.2  &   2.05 & 0.82 & 97 & 1.20 & 8.5& 0.11 &  6.9\\
HD~181420$^d$  & F2V & 6.57 & 156.6 &   1.60 & 0.76 & 76 & 1.15 &10.3& 0.42 &  242\\
HD~181906$^e$  & F8V & 7.6  & 156.6 &   1.92 & 0.88 & 85 & 1.00 &10.3& 0.15 &   47\\
HD~181907$^f$  &G8III& 5.8  & 156.6 & 0.0286 &0.0176& 3.5& 1.10 & 5.0& 1.99 &   40\\
Sun/VIRGO$^g$& G2V &      & 182.1 &   3.25  & 1.04 & 135& 1.30 & 8.0& 2.50 & $7.5\times  10^3$\\
\hline
%\multicolumn{7}{c}{Doppler observation}\\ \hline
%Procyon  &FIV/V & 0.4&  12.5 &   0.90 & 0.38 & 55 & 2.4 & 7.2& 1.58 &   69\\
%Sun/GOLF & G2V  &    & 121.2 &   3.25 & 0.57 & 135& 2.5 & 4.7& 6.5  &17252\\ % OK
%\hline
\end{tabular}}
\par
\medskip  
$\numax$ is the location of the frequency of maximum power; $\HWHM$ is the full-width at half-maximum of the mode envelope; $\dnumoy$ is the mean value of the large separation; $\alpha$ represents the optimized filter width, in unit $\HWHM$;  $\gamma$ represents $\HWHM$ in unit $\dnu$; $\HBR$ measures the mean seismic amplitude in the time series compared to the noise, by the ratio in the Fourier spectrum, at the maximum-oscillation frequency, of the smoothed mode height to the background power density;  $\ampmax$ measures the \fonction.
\par
References:
$^a$~Deheuvels et~al. (private comm.);
$^{b1}$~Benomar et~al. (private comm.);
$^{b2}$~Appourchaux et~al. (\cite{2008A&A...488..705A});
$^c$~Mosser et~al. (\cite{mosser2009});
$^d$~Barban et~al. (\cite{barban2009});
$^e$~Garcia et~al. (\cite{garcia2009});
$^f$~Carrier et~al. (\cite{carrier2009});
$^g$~Frohlich et~al. (\cite{1997SoPh..170....1F}).\vspace*{2mm}
\end{table}