\begin{table}%t1
\caption{\label{tab:ewori_std}Photometric data for \EW\ and the comparison stars.}
%\centering
\small
\begin{tabular}{lllrrrrrrrrrrrr} 
\hline
\hline\noalign{\smallskip}
Object&Sp. type&Ref.     &$V$&$\sigma$&$b-y$&$\sigma$&$m_1$&$\sigma$&$c_1$ &$\sigma$&$N$($\it uvby$)&$\beta$&$\sigma$&$N$($\beta$)\\
\hline
 EW~Ori  & G0~V\tablefootmark{a}       & C10    & 9.902  & 7& 0.390 & 5& 0.186 & 8& 0.364 &10&324 & 2.613   & 8 &25\\    
          &            & C10    &10.510  & 7& 0.379 & 5& 0.181 & 4& 0.369 & 4&  4 &         &   &  \\  
          &            & HH75   & 9.905  & 7& 0.387 & 5& 0.201 & 1& 0.350 &10&  2 &         &   &  \\
          &            & L02    & 9.924  &  & 0.407 &  & 0.175 &  & 0.353 &  &  1 & 2.629   &   & 1\\
\hline\noalign{\smallskip}
 HD 34658  & F3~III/IV\tablefootmark{b}   & C10    & 5.334  & 5& 0.258 & 3& 0.196 & 5& 0.668 & 6&180 & 2.691   & 4 &15\\ 
          &            & SP65   &        &  & 0.268 &  & 0.177 &  & 0.682 &  &  2 &         &   &  \\
          &            & C66    &        &  &       &  &       &  &       &  &    & 2.685   &   & 7\\
          &            & GO7677 & 5.334  & 2& 0.260 & 2& 0.189 & 3& 0.671 & 5&  4 & 2.685   & 6 & 3\\
          &            & AF90   & 5.326  &12& 0.263 &20& 0.184 &18& 0.659 &23&  2 & 2.676   & 3 & 2\\
\hline\noalign{\smallskip}
 HD 34745  & F7~V\tablefootmark{b}       & C10    & 6.999  & 6& 0.343 & 4& 0.171 & 7& 0.363 & 8&236 & 2.618   & 8 &17\\
          &            & O83    & 6.998  & 6& 0.351 & 1& 0.168 & 5& 0.360 & 1&  2 &         &   &  \\
          &            & O94    & 7.008  & 4& 0.350 & 3& 0.157 & 4& 0.367 & 5&  1 & 2.614   & 6 & 1\\   
\hline\noalign{\smallskip}
 HD 35638  & F5~V\tablefootmark{b}       & C10    & 7.645  & 6& 0.290 & 4& 0.164 & 7& 0.420 & 8&172 & 2.651   & 8 &16\\
          &            & O83    & 7.648  & 5& 0.297 & 3& 0.158 & 2& 0.417 & 1&  2 &         &   &  \\
          &            & O94    & 7.653  & 5& 0.295 & 3& 0.151 & 4& 0.430 & 6&  1 & 2.648   & 6 & 1\\  
\hline
\end{tabular}
\tablefoot {For EW~Ori, the ${\it uvby}\beta$ information by C10 (first line), HH75, and L02 is 
the mean value outside eclipses. For C10 (second line) indices during the total part of secondary eclipse are included. \\
$N$ is the total number of observations used to form the mean values, and~$\sigma$ is the rms error (per observation) in~mmag. \\
\tablefoottext{a}{Popper et~al. (\cite{plft86}); spectral type of the primary component;} 
\tablefoottext{b}{Houk \& Swift (\cite{houk99}).}}
\vspace*{-3mm}
\tablebib {AF90 = Arellano Ferro et~al. (\cite{af90}), C10~= this paper, C66~= Crawford et~al. (\cite{c66}), GO7677~= Gr{\o}nbech \& Olsen (\cite{go76}, \cite{go77}) (revised catalogue),
HH75~= Hilditch \& Hill (\cite{hh75}), L02~= Lacy (\cite{l02}), O83~= Olsen (\cite{olsen83}),    
O94~= $\it uvby$: Olsen (\cite{olsen94}), $\beta$: Olsen (unpublished), SP65~= Str\"omgren \& Perry (\cite{sp2}).}
\vspace*{3mm}
\end{table}