\begin{table}%t3
\caption[]{\label{tab:24133_wd}
Photometric solutions for V1130~Tau.
}
 {\begin{tabular}{lrrrr} \hline
\hline\noalign{\smallskip}
                     &     $y$    &       $b$  &       $v$  &   $u$\\                   
\noalign{\smallskip}
\hline
\noalign{\smallskip}
$i$ \, (\degr)       &  73.97     &   73.84    &   73.73    &  74.20\vspace{-0.8mm}\\   
                     & $\pm $2    &  $\pm $4   &  $\pm $4   & $\pm $6\\                 
$\Omega_{\rm p}$           &   4.5138   &    4.5079  &    4.4954  &   4.5642\vspace{-0.8mm}\\  
                     &  $\pm $39  &   $\pm $40 &   $\pm $41 &  $\pm $64\\                
$\Omega_{\rm s}$           &   4.0727   &    4.0753  &    4.0775  &   4.0805\vspace{-0.8mm}\\  
                     &  $\pm $25  &   $\pm $29 &   $\pm $30 &  $\pm $45\\                
$r_{\rm p}$                &  0.2956    &   0.2961   &   0.2973   &  0.2911\\
$r_{\rm s}$                &  0.3542    &   0.3539   &   0.3536   &  0.3532\\                
$k$                  &  1.198     &   1.195    &   1.189    &  1.213\\                 
$r_{\rm p} + r_{\rm s}$          &  0.6498    &   0.6500   &   0.6509   &  0.6443\\                
$u_{\rm p} = u_{\rm s}$          &  0.52      &   0.61     &   0.67     &  0.63   \\
$T_{{\rm eff},\rm s}$    &  6638      &   6639     &   6643     &  6628\vspace{-0.8mm}\\
                     &$\pm $4     & $\pm $3    &$\pm  $3    &$\pm $4\\
$L_{\rm s}/L_{\rm p}$            &  1.444     &    1.436   &   1.429    &  1.436  \\
$\sigma$ \, (mmag)  &  4.5       &    4.3     &   4.3      &  6.5   \\
\hline
\end{tabular}            }

\tablefoot {Limb darkening coefficients by van Hamme (\cite{vh93}),
gravity darkening exponents of~0.33, and bolometric albedo
coefficients of~0.5 were adopted, as appropriate for convective envelopes.
$T_{{\rm eff},p}$ was assumed to be 6650~K, see Sect.~\ref{sec:absdim}.
The errors quoted for the free parameters are the {\it formal} standard errors
determined from the iterative least squares solution procedure.}
\end{table}