\begin{table}%t1
\caption{\label{tab:bkpeg_std}Photometric data for \BK\ and the comparison stars.}
%\begin{minipage}{\textwidth}
%%\begin{center}
\par
%\centerline
{\begin{tabular}{lllrrrrrrrrrrrr} \hline
\hline\noalign{\smallskip}
Object&Sp. Type&Ref.   &$V$&$\sigma$&$b-y$&$\sigma$&$m_1$&$\sigma$&$c_1$ &$\sigma$&$N$($uvby$)&$\beta$&$\sigma$&$N$($\beta$)\\
\noalign{\smallskip}
\hline
\noalign{\smallskip}
%jvc090608 mean uvby corrected via meanuvby_plot.pro
 BK~Peg  & F8\tablefootmark{a}        & C10    & 9.982  & 7& 0.362 & 6& 0.143 &12& 0.456 &12&176 & 2.639   & 7 & 9\\    
          &                           & C10    &10.463  & 4& 0.369 & 7& 0.136 &11& 0.477 & 4&  6 &         &   &  \\    
%
\hline
%HD222249 & F5~IV      &        & 7.146  & 6& 0.309 & 4& 0.177 & 9& 0.503 & 8&119 & 2.645   & 3 & 8\\ % all
 HD 222249 & F5~IV\tablefootmark{b} & C10    & 7.146  & 6& 0.309 & 4& 0.177 & 8& 0.503 & 8&118 & 2.645   & 3 & 8\\ %excl dev
          &            & O83    & 7.139  & 5& 0.317 & 3& 0.158 & 4& 0.503 & 4&  1 &         &   &  \\
          &            & O94    & 7.151  & 9& 0.317 & 3& 0.161 & 3& 0.507 & 2&  3 & 2.645   & 8 & 3\\
          &            & P69    & 7.010  &  & 0.303 &  & 0.190 &  & 0.487 &  &  2 &         &   &  \\
%         &            & P69    & 7.01   &  & 0.303 &  & 0.190 &  & 0.487 &  &  2 &         &   &  \\
%n2000                 &          7.148       0.317      0.160      0.506       4   2.645         3
%bq_prcats                                                                          2.645     8   3
%osnbeta_bprcats                                                                    2.648     5   1  not included
%
\hline
%HD222391 & G0~III     &        & 7.567  & 6& 0.362 & 6& 0.185 &11& 0.424 & 9&137 & 2.617   & 4 & 8\\
 HD 222391 & G0~III\tablefootmark{c} & C10    & 7.566  & 6& 0.362 & 6& 0.185 &11& 0.424 & 8&134 & 2.617   & 4 & 8\\
          &            & O83    & 7.559  & 5& 0.371 & 3& 0.170 & 4& 0.420 & 5&  1 &         &   &  \\
          &            & O94    &        &  & 0.372 & 3& 0.167 & 4& 0.427 & 6&  1 & 2.620   &  6& 2\\
%         &            & O94    & 7.564  &  & 0.372 & 3& 0.167 & 4& 0.427 & 6&  1 & 2.620   &  6& 2\\
%n2000                 &          7.559       0.371      0.168      0.423       2   2.624         1
%bq_prcats                                                                          2.624     6   1  included
%osnbeta_bprcats                                                                    2.616     5   1  included
%
\hline
%HD223323 & F2~IV-V    &        & 7.084  & 6& 0.290 & 5& 0.138 &10& 0.414 & 9&189 & 2.636   & 7 &13\\
 HD 223323 & F2~IV-V\tablefootmark{d} & C10    & 7.084  & 6& 0.290 & 5& 0.138 &10& 0.414 & 9&189 & 2.636   & 7 &13\\
          &            & J96    & 7.076  & 4& 0.302 & 1& 0.123 & 1& 0.407 & 1&  9 & 2.640   &   &  \\
          &            & J96    & 7.094  & 2& 0.300 & 0& 0.128 & 5& 0.409 & 4&  2 &         &   &  \\
          &            & J96    & 7.089  & 1& 0.299 & 0& 0.120 & 0& 0.406 & 1&  2 &         &   &  \\
          &            & O83    & 7.080  & 6& 0.296 & 5& 0.124 & 5& 0.412 & 4&  4 & 2.643   & 5 & 4\\
%n2000                 &          7.080       0.296      0.124      0.412       4   2.643         4
\hline
\end{tabular}}
%\medskip
  \tablebib{\tablefoottext{a}{Popper (\cite{dmp83})}; \tablefoottext{b}{Harlan \& Taylor (\cite{ht70});}  \tablefoottext{c}{Heard (\cite{h56});} \tablefoottext{d}{Harlan (\cite{h69}).}}\vspace*{-2mm}
\tablefoot{C10 = This paper. J96 = Jordi et al. (\cite{jordi96}).  
O83  = Olsen (\cite{olsen83}).  O94  = Olsen (\cite{olsen94}). 
P69  = Perry  (\cite{perry69}). 
For \BK, the $uvby\beta$ information by C10 is the mean value outside eclipses
(first line) and during the central part of secondary eclipse (second line), 
where 98\% ($y$) of the light of the secondary component is eclipsed. 
N is the total number of observations used to form the mean values, and
$\sigma$ is the rms error (per observation) in mmag.}
%\end{minipage}
\end{table}