\begin{table}%t4
\caption{\label{tab:ewori_jktebop_vh}Photometric solutions for EW~Ori from the JKTEBOP code.}
%\centering
\par
\begin{tabular}{lrrrr} 
\hline
\hline\noalign{\smallskip}
                     &     $y$    &       $b$  &       $v$  &   $u$\\                   
\hline
$i$ ~ (\degr)       &  89.89     &   89.84    &   89.87    &   89.85\vspace{-0.8mm}\\   
                     & $\pm 5$    &  $\pm 4$   &  $\pm 5$   &  $\pm 5$\\                 
\par
$e\cos \omega$       &  0.04778   &   0.04775  &   0.04774  &   0.04767\vspace{-0.8mm}\\ 
                     &$\pm    3$  & $\pm    3$ & $\pm    3$ & $\pm    4$\\             
\par
$e\sin \omega$       &$-0.05926$  & $-0.05763$ & $-0.06064$ & $-0.05806$\vspace{-0.8mm}\\  
                     & $\pm 176$  &  $\pm 186$ & $\pm  206$ & $\pm  256$\\                
\par
$e$                  &  0.0761    &   0.0748   &   0.0772   &  0.0751\\                 
\par
$\omega$ ~ (\degr)  &  309.88    &   309.65   &   308.21   & 309.39 \\                 
\par
$r_{\rm p}$                &  0.0579    &   0.0579   &   0.0578   &  0.0578\\                 
\par
$r_{\rm s}$                &  0.0542    &   0.0543   &   0.0543   &  0.0546\\                 
\par
$k$                  &  0.9356    &   0.9391   &   0.9386   &   0.9446\vspace{-0.8mm}\\  
                     &  $\pm33$   &   $\pm43$  &   $\pm45$  &   $\pm59$\\                
\par
$r_{\rm p} + r_{\rm s}$          &  0.1121   &   0.1122  &   0.1121  &  0.1123\vspace{-0.8mm}\\  
                     &  $\pm 2$  &   $\pm 2$ &   $\pm 2$ &  $\pm 3$ \\               
\par
$u_{\rm p}$                &  0.56      &   0.66     &   0.74     &  0.76\\                   
\par
$u_{\rm s}$                &  0.59      &   0.68     &   0.77     &  0.81\\                   
\par
$y_{\rm p}$                &  0.37      &   0.42     &   0.48     &  0.57\\
\par
$y_{\rm s}$                &  0.38      &   0.43     &   0.50     &  0.59\\
\par
$J_{\rm s}/J_{\rm p}$            &  0.8737    &    0.8415  &   0.8154   &  0.8037\vspace{-0.8mm}\\
                     &  $\pm25$   &    $\pm30$ &   $\pm33$  &  $\pm41$\\
\par
$L_{\rm s}/L_{\rm p}$            &  0.7554    &    0.7357  &   0.7088   &  0.7011 \\
\par
$\sigma$ ~ (mmag.)  &  6.9       &    6.7     &   7.3      &  8.7   \\
\hline
\end{tabular}            
\tablefoot {Linear limb darkening coefficients by Van Hamme (\cite{vh93}) were adopted,
a mass ratio of 0.97 was assumed, and phase shift and  magnitude normalization 
were included as free parameters. \\
The errors quoted for the free parameters are the $formal$ errors determined 
from the iterative least squares solution procedure.}
\end{table}