\begin{table}%t5
\caption{\label{sedresults}Results of our SED disc modelling.}
%\centerline
{\small
\begin{tabular}{lcccccc}
\hline \hline
          & $R_{\rm in}$--$R_{\rm out}$ & $m$         & $\alpha$ & iron & $T_{\rm bb}$  & $i$\\
          & AU                      & $10^{-5}$$M_{\odot}$ &          & \%   & K &   $^{\circ}$ \\
\hline 
HD~52961: A   &  10--500  &  $1.7$ & $-1.5$ & 0  & 160  &  0--90\\
HD~52961: B   &  10--500  &  $0.7$ & $-1.5$ & 10  & 160  &  $< $$65$\\
EP~Lyr: A  &  40--300  &  $6$   & $-1.0$  & 0  & $-$  &  0--90\\
\hline
\end{tabular}}
\medskip
\par
Note: Given are the inner and outer radius ($R_{\rm in}$--$R_{\rm out}$),
the total disc mass $m$ for the homogeneous disc model, the surface-density distribution power law $\alpha$, the percentage of iron in the homogeneous disc model,
the blackbody temperature and the inclination of the system.
\end{table}