\begin{table}%t3
\caption[] {\label{tab:stdphot_publ}
Published $uvby\beta$ photometry for the eclipsing binaries and the comparison stars.
$N$ is the total number of observations used to form the mean values, and
$\sigma$ is the rms error (per observation) in  mmag.
%
References are:
GO76   = Gr{\o}nbech \& Olsen  (\cite{go76}),    
GO77   = Gr{\o}nbech \& Olsen  (\cite{go77}),    
HM80   = Heck \& Manfroid (\cite{hm80}),         
K98    = Kaltcheva (\cite{ntk98}),               
KOC00  = Kaltcheva et al. (\cite{koc00}),        
K78    = Kilkenny (\cite{k78}),                  
K81    = Kilkenny (\cite{k81}),                  
K92    = Knude (\cite{k92}),                     
LPLM90 = Landolt et al. (\cite{lplm90}),         
S85    = Shobbrook (\cite{s85}),                 
SHL92  = Slawson et al. (\cite{shl92}),          
%SL94   = Shobbrook \& Lyng{\aa} (\cite{sl94}),  
%BCM92  = Balona et al. (\cite{bcm92}),          
TAT95  = Twarog \& Anthony-Twarog (\cite{tt95}), 
WK83   = Wolf \& Kern (\cite{wk83}).             
}
\begin{tabular}{llllrrrrrrrrrrr} \hline
\hline
Object&Ref.      &Sp. type&$V$&$\sigma$&$b-y$&$\sigma$&$m_1$&$\sigma$&$c_1$ &$\sigma$&$N$($uvby$)&$\beta$&$\sigma$&$N$($\beta$)\\
\hline
%spectral types: from Simbad
DW\,Car  & --         &B1V+B1V  &        &  &        &  &       &  &       &  &    &         &   &  \\              
HD~93191 & --          &A0       &        &  &        &  &       &  &       &  &    &         &   &  \\
HD~92072 &K98         &B5V      &  7.119 &  &$-0.030$&  &  0.085&  &  0.433&  &    &   2.715 &   &  \\
        &LPLM90      &         &  7.068 &12&$-0.046$& 4&  0.115& 8&  0.423& 8&  17&   2.702 &  8&15\\
HD92288 &KOC00       &B6V      &  7.893 &17&$-0.012$& 3&  0.102& 1&  0.500& 4&   2&   2.705 &  1& 2\\
        &LPLM90      &         &  7.904 & 5&$-0.022$& 2&  0.099& 7&  0.525&12&   3&   2.708 &  4& 3\\
\hline
BF\,Cen  &WK83       &B8       &  8.54  &  &  0.054 &  &  0.029&  &  0.172&  &   1&   2.609 &   & 1\\
        &S85         &         &  8.62  &  &  0.058 &  &  0.010&  &  0.150&  &   4&   2.619 &   & 3\\ %is 3(Pl.1)
HD~100942&KOC00       &B8/B9V   &  7.762 & 2&  0.011 & 3&  0.138& 5&  0.698&11&   3&   2.800 &  7& 1\\
HD~101466&KOC00       &A0IV     &  7.318 & 3&  0.034 & 8&  0.143& 8&  1.052& 0&   2&   2.858 &  7& 1\\
        &SHL92       &         &  7.35  &  &        &  &       &  &       &  &   2&         &   &  \\
\hline
AC\,Vel  &WK83       &B3IV     &  8.88  &  &  0.155 &  & --0.013&  &  0.331&  &   1&   2.629 &   & 1\\
%HD93943 &GOS76       &B9.5IV-V &  5.964 & 8&  0.020 & 7&  0.123&10&  1.023& 1&   2&         &   &  \\
HD~93943 &GO76,77     &B9.5IV-V &  5.865 & 8&  0.018 & 7&  0.122&10&  1.029& 1&   2&   2.848 &  5& 3\\
%      &SL94         &         &        &  &        &  &       &  &       &  &    &         &   &  \\  %I can't find it in LSSMW
%        &BCM92?     &         &        &  &        &  &       &  &       &  &    &         &   &  \\ no info
HD~92757 & --          &B9.5V    &        &  &        &  &       &  &       &  &    &         &   &  \\
HD~92155 &HM80        &B3V      & 6.432  & 4&$-0.069$& 2&  0.096& 6&  0.356& 6&   6&   2.654 &  4& 5\\
\hline
NSV5783 &K92         &B5V      &  8.674 &  &  0.029 &  &  0.060&  &  0.428&  &    &   2.714 &   &  \\
        &K81         &         &        &  &        &  &       &  &       &  &    &   2.696 &   & 2\\ %=HD109724
        &K78         &         &  8.69  &  &  0.023 &  &  0.075&  &  0.410&  &   3&         &   &  \\
%HD108925&GO76       &A3V      &  6.447 &  &  0.088 &  &  0.154&  &  1.167&  &   2&         &   &  \\
HD~108925&GO76, 77     &A3V      &  6.448 &8 &  0.087 & 8&  0.153& 4&  1.172& 3&   2&   2.853 &  9& 3\\
        &TAT95       &         &  6.452 &2 &  0.081 & 4&   --   &  &    --  &  &   4&         &   &  \\
        &SHL92       &         &  6.44  &  &        &  &       &  &       &  &   1&         &   &  \\
HD~109808&SHL92       &A1/A2V   &  6.934 &  &        &  &       &  &       &  &    &         &   &  \\
\hline
\end{tabular}
\end{table}