\begin{table}%t7
%\centering
\par
\caption{Photometric solutions for AD Boo (all data) from the WD code
adopting linear limb darkening coefficients by van Hamme (\cite{vh93});
see Table~\ref{tab:adboo_ebop_vh}.
Gravity darkening exponents of 0.33 and bolometric albedo
coefficients of 0.5 were applied, as appropriate for convective envelopes.
$T_{\rm {eff},p}$ was assumed to be 6575~K.}\label{tab:adboo_wd_vh}
\small \begin{tabular}{lrrrr}
\hline \hline
                     &     $y$    &       $b$  &       $v$  &   $u$\\                   
\hline
$i$ ~ (\degr)       &  87.47     &   87.78    &   87.79    &  87.82\\           
                     & $\pm$5    &  $\pm$3   &  $\pm$3   & $\pm$6\\                 
\par
$\Omega_{\rm p}$           &   6.743    &    6.711   &    6.717   &   6.702\\  
                     &  $\pm$11   &   $\pm$8  &   $\pm$9  &  $\pm$14\\                
\par
$\Omega_{\rm s}$           &   7.646    &    7.696   &    7.675   &   7.636\\  
                     &  $\pm$16   &   $\pm$10  &   $\pm$9  &  $\pm$18\\                
\par
$r_{\rm p}$                &  0.1705    &   0.1713   &   0.1711   &  0.1716\\                 
\par
$r_{\rm s}$                &  0.1303    &   0.1293   &   0.1297   &  0.1305\\                 
\par
$k$                  &  0.764     &   0.755    &   0.758    &  0.761\\                  
\par
$r_{\rm p} + r_{\rm s}$          &  0.3008    &   0.3006   &   0.3008   &  0.3021\\                 
\par
$T_{\rm {eff},s}$    &  6078      &   6052     &   5999     &  5946\\
                     &$\pm$4     & $\pm$4    &$\pm$$  4$    &$\pm$4\\
\par
$L_{\rm s}/L_{\rm p}$            &  0.4205    &    0.3868  &   0.3615   &  0.3761 \\
\par
$\sigma$ ~ (mag.)   &  0.0064    &    0.0062  &   0.0066   &  0.0101\\
\hline
\end{tabular}            
\end{table}