\begin{table}%t1
\caption{\label{sterren}List of stellar parameters for our sample sources.}
%\centerline
{\small
\begin{tabular}{llrrcccrrcl}
\hline \hline
Name & $\alpha$ (J2000) & $\delta$ (J2000)  & $T_{\rm eff}$ & $\log g$ & [Fe/H] & $P_{\rm orb}$ & $e$ & $E(B-V)_{\rm tot}$ & $L_{\rm IR}/L_*$ & $d$\\ 
     & (h m s)          & ($^\circ$ $'$ $''$)   & (K)       & (cgs)    &        & (days)      &     &                & (\%)         & (kpc)\\
\hline
EP~Lyr      & 19 18 17.5 & $+$27 50 38  & 7000 & 2.0 & $-1.5$   &       &      & $0.51\pm0.01$ & $3\pm0$ & $3.2\pm1.0$\\ 
HD~52961    & 07 03 39.6 & $+$10 46 13  & 6000 & 0.5 & $-4.8$   & 1310  & 0.21 & $0.06\pm0.02$ & $12\pm1$ & $1.6\pm0.5$\\ 
\hline
\end{tabular}}
\par
\medskip
Note: Listed are the name, equatorial coordinates $\alpha$ and $\delta$(J2000), effective
temperature $T_{\rm eff}$, surface gravity $\log g$, and metallicity [Fe/H] of our sample stars.
For the model parameters we refer to \citet{deruyter06}. Also given are the orbital period and the
eccentricity \citep[see references in][]{deruyter06,gielen07}. The total reddening $E(B-V)_{\rm tot}$, the energy ratio $L_{\rm IR}/L_*$ and the calculated distance,
assuming a luminosity of $L_*=3000\pm2000$~$L_{\odot}$.
\end{table}