\begin{table}%t3
%\centering
\par
\caption{Limb darkened angular diameters and linear radii for the five program stars.\label{table_LD}}
\begin{tabular}{lcccccc}
\hline\hline
Star  & Baseline & Band ($\lambda_{\rm eff}$) & $\rho^{{a}}$ & $\theta_{\rm LD} \pm 
\sigma_{\rm stat} \pm \sigma_{\rm syst}$ [mas] & $R \pm  \sigma_{\rm tot} [R_{\odot}]$ & $\chi^2_{\rm red}$\\
\hline
\noalign{\smallskip}
$\tau$~Cet & B3-M0 & $K$ (2.179 $\mu$m) & 1.025  &  2.078 $\pm$ 0.014 $\pm$ 0.028 & 0.816 $\pm$ 0.013 & 0.57\\
\hline
\noalign{\smallskip}
$\epsilon$~Eri & UT1-UT3 + B3-M0 & $K$ (2.179 $\mu$m) & 1.027 &  2.148 $\pm$ 0.010 $\pm$ 0.027 & 0.743 $\pm$ 0.010 & 0.17\\
\hline
\noalign{\smallskip}
$\beta$ Leo & B3-M0 & $K$ (2.177 $\mu$m) & 1.014 & 1.449 $\pm$ 0.014 $\pm$ 0.023 & 1.728 $\pm$ 0.037 & 1.32\\
\hline
\noalign{\smallskip}
$\beta$~Pic & UT1-UT3 & $K$ (2.177 $\mu$m) & 1.014  &  0.849 $\pm$ 0.060 $\pm$ 0.100 & 1.759 $\pm$ 0.241 & 1.19\\
\hline
\noalign{\smallskip}
$\alpha$~PsA & UT1-UT3 + B3-M0 & $K$ (2.177 $\mu$m)& 1.014  &  2.222 $\pm$ 0.021 $\pm$ 0.015 & 1.835 $\pm$ 0.022 & 0.41 \\
 & E0-G1 & $K$ (2.177 $\mu$m) & 1.014 &  2.321 $\pm$ 0.042 $\pm$ 0.046 & 1.917 $\pm$ 0.054 & 0.44 \\
 & E0-G1 & $H$ (1.632 $\mu$m) & 1.016  &  2.235 $\pm$ 0.056 $\pm$ 0.046 & 1.846 $\pm$ 0.061 & 0.15 \\
 & All baselines & $K$ (2.177 $\mu$m) & 1.014  &  2.228 $\pm$ 0.011 $\pm$ 0.020 & 1.840 $\pm$ 0.023 & 0.62\\
\hline
\end{tabular}
\begin{list}{}{}
\item[$^{{a}}$] The linear 
limb-darkening coefficients were taken from Claret tables 
(Claret~\cite{claret00}) to compute the conversion factor $\rho$.
\end{list}
\end{table}