\begin{table}%T1
\caption[]{\label{tab:8788_ebop_vh}Photometric solutions for V636~Cen from JKTEBOP analyses of the 1987 and 1988
light curve observations (426 points per band). 
}
\centerline {\begin{tabular}{lrrrr} \hline
\hline\noalign{\smallskip}
                     &     $y$    &       $b$  &       $v$  &   $u$\\                 
\noalign{\smallskip}
\hline
\noalign{\smallskip}
$i$ \, (\degr)       &  89.65     &   89.62    &   89.62    &  89.63\vspace{-0.8mm}\\ 
                     & $\pm $7    &  $\pm $7   &  $\pm $8   & $\pm 9$\\               
$r_{\rm p}$                &  0.0746    &   0.0748   &   0.0750   &  0.0751\vspace{-0.8mm}\\
                     &  $\pm $5   &   $\pm $5  &   $\pm $6  &  $\pm $6\\              
$r_{\rm s}$                &  0.0613    &   0.0614   &   0.0613   &  0.0614\vspace{-0.8mm}\\
                     &  $\pm $3   &   $\pm $3  &   $\pm $3  &  $\pm $3\\                                                                                      $k$                  &   0.822    &   0.822    &   0.818    &   0.817\\ 
                     &  $\pm $5   &  $\pm $5   &  $\pm $6   & $\pm  $6\\              
$r_p + r_{\rm s}$          &  0.1359    &   0.1362   &   0.1363   &  0.1365\vspace{-0.8mm}\\
                     &  $\pm $6   &   $\pm $5  &   $\pm $7  &  $\pm $7\\
$u_{\rm p}$                &  0.59      &   0.68     &   0.77     &  0.81\\   
$u_{\rm s}$                &  0.73      &   0.84     &   0.95     &  0.99\\
$y_{\rm p}$                &  0.37      &   0.43     &   0.49     &  0.58\\
$y_{\rm s}$                &  0.44      &   0.51     &   0.59     &  0.70\\
$J_{\rm s}/J_{\rm p}$            &  0.417     &    0.370   &   0.286    &  0.236\vspace{-0.8mm}\\
                    &  $\pm$10   &   $\pm $9  &   $\pm $8  &  $\pm $7\\
$L_{\rm s}/L_{\rm p}$            &  0.265     &    0.233   &   0.176    &  0.144\vspace{-0.8mm}\\
                     & $\pm $3    &   $\pm $3  &  $\pm $3   & $\pm $3\\
$\sigma$ \, (mmag.)  &  11.3      &    11.4    &   13.2     &  14.5\\        
\hline
\end{tabular}            
}

\smallskip            
 {Note 1:}
Orbital parameters of $e = 0.1348$ and $\omega = 281\fdg60$ were assumed
(Table~\ref{tab:v636_orb}), and linear limb darkening coefficients by Van 
Hamme (\cite{vh93}) were adopted.

 {Note 2:}
The errors quoted for the free parameters are realistic values determined from 
1000 Monte Carlo simulations. $e$ and $\omega$ were perturbed corresponding
to their uncertainties, and the limb darkening coefficients within ${\pm} 0.05$.
\end{table}