\begin{table}%t5
\caption{\label{tab:teff}
%Effective temperatures (K) for the `average' component of \BK.
Effective temperatures (K) for the combined light of \BK.}
%\centerline
{\begin{tabular}{ccccccccccc} \hline
\hline\noalign{\smallskip}
 $A_{\rm V}$& [Fe/H] & $(b-y)_0$ &$c_0$&$(V-J)_0$&$(V-H)_0$&$(V-K_{\rm s})_0$& A96 & H07 &RM05 & M06  \\
\noalign{\smallskip}
\hline
\noalign{\smallskip}
%0.188&$-0.10$ &0.405&0.320&1.208&1.458&1.564 & 6280 & 6270 &6270/6255/6130/6265 &  6290 \\
 0.188&$-0.12$ &0.405&0.320&1.208&1.458&1.564 & 6280 & 6270 &6270/6255/6130/6265 &  6290 \\
%         .064    .20                                    150    120        145  110  110
\noalign{\smallskip}            
\hline
\end{tabular}           }
   \tablefoot{$A_{\rm V}$ is the adopted visual interstellar absorption. The $V_0$ magnitude and the $(b-y)_0$ and $c_0$ indices are based on the  out-of-eclipse $uvby$ standard indices from Table~\ref{tab:bkpeg_std}. The 2MASS observations ($J,H,K_{\rm s}$) were obtained at phase 0.879. The results from A96 are based on their $uvby$ calibration, those from RM05 on their $uvby$, $(V-J)$, $(V-H)$, and $(V-K_{\rm s})$ calibrations (in that order); the calibration by M06 is for $(V-K_{\rm s})$.}
   \vspace*{-2mm}
\tablebib{A96 = Alonso et al. (\cite{alonso96}). H07 = Holmberg et al. (\cite{holmberg07}).
RM05 = Ram\'\i rez \& Mel\'endez (\cite{rm05}). M06 = Masana et al. (\cite{masana06}).}
\end{table}