\begin{table}%T3
\caption{\label{results}Output parameters derived from the spot modeling. }
\small%\centerline
{
\begin{tabular}{rccccccc}
  \hline\hline
  Star &\multicolumn{2}{c}{Inclination}& Spot contrast& \multicolumn{2}{c}{Spot angular radius}& Lifetime& Mean rotation \\
       & $i\ind{spot}$ &  $i\ind{seismo}$& $\langle\contrast\ind{max}\rangle$&median & range&  $\tau$ & $\Tmoy$ \\
       &\multicolumn{2}{c}{\dotfill\ (deg) \dotfill}&($~^0\!/_{00}$)&\multicolumn{2}{c}{\dotfill\ (deg) \dotfill}&\multicolumn{2}{c}{\dotfill\ (day) \dotfill}\\
\hline\noalign{\smallskip}
HD~49933  & $50\pm 25^\circ$& $55\pm10^\circ$ (a)& 1  & 1.8 & $1\to2.5^\circ$& $2.5\to3.5$& $_rm 3.45^{+0.05}_{-0.05}$ \\
HD~175726 & $55\pm 25^\circ$&  --                & 8  & 4.7 & $3  \to7^\circ$& $5  \to  7$       & $\rm 3.95^{+0.1}_{-0.1}$   \\
HD~181420 & $60\pm 25^\circ$& $45\pm 4^\circ$ (b)& 0.8& 1.6 &$0.8 \to2^\circ$& $1.5\to  3$    & $\rm 2.25^{+0.03}_{-0.01}$ \\
HD~181906 & $45\pm 25^\circ$& $24\pm 3^\circ$ (c)& 1  & 1.8 &$1.0 \to 2.5^\circ$& $1.5\to  3$ & $\rm 2.71^{+0.03}_{-0.01}$ \\
\hline
\end{tabular}}
\smallskip
Inclinations derived from the spot model are compared to the seismic values inferred from the fit of the Fourier spectra of p~modes: (a)~Appourchaux et~al. (2008); (b) Barban et~al. (2009); (c) Garcia et~al. (2009).
\end{table}