\begin{table}%t4           
\caption[] {\label{tab:24133_phel}Adopted photometric elements for V1130~Tau.
}
\centerline {\begin{tabular}{ll}             
\hline\hline             
\noalign{\smallskip}             
$i$              & $73{\fdg}82 \pm 0{\fdg}20$\\
$r_{\rm p}$            & $0.2952 \pm 0.0018$\\      
$r_{\rm p}\rm (pole)$      &  0.2862\\
$r_{\rm p}\rm (point)$     &  0.3125\\
$r_{\rm p}\rm (side)$      &  0.2935\\
$r_{\rm p}\rm (back)$      &  0.3048\\
$r_{\rm s}$            & $0.3535 \pm 0.0021$\\ 
$r_{\rm s}\rm (pole)$      &  0.3369\\
$r_{\rm s}\rm (point)$     &  0.3965\\
$r_{\rm s}\rm (side)$      &  0.3506\\
$r_{\rm s}\rm (back)$      &  0.3717\\
\noalign{\smallskip}             
\end{tabular}  }           
\centerline {\begin{tabular}{lrrrr}             
\noalign{\smallskip}             
          & $y$    & $b$    & $v$   & $u$\\           
\noalign{\smallskip}
$L_{\rm s}/L_{\rm p}$ &  1.443  &  1.437  &   1.432  &   1.434\vspace{-0.8mm}\\
          &$\pm  $23&$\pm  $23&$\pm   $23 &$\pm  $23\\ 
\noalign{\smallskip}             
\hline             
\end{tabular}             }

\tablefoot {The individual luminosity ratios are based on the mean stellar and 
orbital parameters.}
\end{table}