\begin{table}%t6
\caption{\label{tab:bkpeg_jktebop_vh}
Photometric solutions for BK~Peg from the {\sc jktebop} code.}
 %\centerline
{
\begin{tabular}{lrrrr} \hline
\hline\noalign{\smallskip}
                     &     $y$    &       $b$  &       $v$  &   $u$\\                   
\noalign{\smallskip}
\hline
\noalign{\smallskip}
$i$ ~ (\degr)       &  88.02     &   87.91    &   87.99    &   87.90\vspace{-0.8mm}\\   
                     & $\pm 5$    &  $\pm 5$   &  $\pm 4$   &  $\pm 7$\\                 
%c                      87.85         87.72        87.85        87.72
%sqrt                   87.99
%log                    87.99
$e\cos \omega$       &$-0.00364$  & $-0.00376$ & $-0.00363$ & $-0.00374$\vspace{-0.8mm}\\ 
                     &$\pm    6$  & $\pm    7$ & $\pm    6$ & $\pm   10$\\             
%c                     -0.00364      -0.00376     -0.00363     -0.00375
%sqrt                  -0.00364
%log                   -0.00364
$e\sin \omega$       &$ 0.00283$  & $ 0.00563$ & $ 0.00438$ & $ 0.00059$\vspace{-0.8mm}\\  
                     & $\pm 181$  &  $\pm 207$ & $\pm  183$ & $\pm  312$\\                
%c                      0.00133       0.00504      0.00340     -0.00050
%sqrt                   0.00264
%log                    0.00264
$e$                  &  0.0046    &   0.0068   &   0.0057   &  0.0038\\                 
%c                      0.0038        0.0063       0.0050      0.0038          
%sqrt                   0.0045
%log                    0.0045                                                     
$\omega$ ~ (\degr)  &  142.1     &   123.8    &   129.6    & 170.0  \\                 
%c                      160.0         126.7        136.9      187.7       
%sqrt                   144.0
%log                    144.0                                    
$r_{\rm p}$                &  0.1092    &   0.1096   &   0.1092   &  0.1100\\                 
%c                      0.1096        0.1098       0.1095      0.1104
%sqrt                   0.1094
%log                    0.1093
$r_{\rm s}$                &  0.0806    &   0.0819   &   0.0807   &  0.0813\\                 
%c                      0.0817        0.0834       0.0817      0.0826
%sqrt                   0.0807
%log                    0.0807                                    
$k$                  &  0.7379    &   0.7474   &   0.7394   &   0.7391\vspace{-0.8mm}\\  
                     &  $\pm50$   &   $\pm68$  &   $\pm46$  &   $\pm97$\\                
%c                      0.7461        0.7595       0.7456       0.7482
%sqrt                   0.7379
%log                    0.7380
$r_{\rm p} + r_{\rm s}$          &  0.1898    &   0.1915   &   0.1900   &  0.1913\vspace{-0.8mm}\\  
                     &  $\pm 5$   &   $\pm 5$  &   $\pm 4$  &  $\pm 7$ \\               
%$r_p + r_s$          &  0.18983   &   0.19147  &   0.19000  &  0.19130\vspace{-0.8mm}\\  
%                     &  $\pm 46$  &   $\pm 51$ &   $\pm 44$ &  $\pm 74$ \\               
%c                      0.19130       0.19312      0.19120     0.19292            
%sqrt                   0.19005
%log                    0.19004                                   
$u_{\rm p} = u_{\rm s}$          &  0.55      &   0.64     &   0.72     &  0.70\\                   
%c                      0.64          0.73         0.79        0.79
%
$y_{\rm p} = y_{\rm s}$          &  1.09      &   1.24     &   1.42     &  1.68\\
%
$J_{\rm s}/J_{\rm p}$            &  1.0444    &    1.0447  &   1.0569   &  1.1016\vspace{-0.8mm}\\
                     &  $\pm31$   &    $\pm37$ &   $\pm34$  &  $\pm60$\\
%c                      1.0456         1.0437      1.0567      1.1007
%sqrt                   1.0446
%log                    1.0444
%
$L_{\rm s}/L_{\rm p}$            &  0.5670    &    0.5817  &   0.5756   &  0.5990 \\
%c                      0.5804         0.6002      0.5852      0.6133
%sqrt                   0.5670
%log                    0.5671
%
$\sigma$ ~ (mmag.)  &  4.8       &    5.2     &   4.7      &  7.9   \\      
\hline
\end{tabular}            
}         
\tablefoot{Linear limb darkening coefficients by Van Hamme (\cite{vh93}) were adopted, a mass ratio of 0.89 was assumed, and phase shift and  mag. 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}