\begin{table}%t11
\caption {
Our BS candidates in M 67, and their photometry.
First column is our identification number (Table~3),
second column that from BDA, and third that from \cite{Sanders77}.
Last column gives the astrometric membership 
(void values
for stars without astrometric membership determination). 
}
{\scriptsize
%{\footnotesize
%\begin{center}
\par
\begin{tabular}{ccccccccc}
\hline
 ID$_{\rm 3}$  & ID$_{\rm BDA}$ & ID$_{\rm S}$ & $b-y$ & $V$ & $m_1$ & $c_1$ & $H_{\beta}$ & M/NM  \\ 
\hline
 559&  16& 751& 0.330$\pm$0.001& 12.700$\pm$0.003& 0.172$\pm$0.002& 0.464$\pm$  0.004& 2.914$\pm$0.029&M\\
 761&  55& 752& 0.181$\pm$0.001& 11.310$\pm$0.003& 0.230$\pm$0.002& 0.841$\pm$  0.004& 2.735$\pm$0.006&M\\
 883&  81& 977& 0.344$\pm$0.004& 10.032$\pm$0.003& 0.016$\pm$0.005& 0.003$\pm$  0.026& 2.706$\pm$0.005& \\
 947 & 95&1005& 0.319$\pm$0.001& 12.673$\pm$0.003& 0.191$\pm$0.002& 0.450$\pm$  0.003& 2.637$\pm$0.006& M\\
1033& 124& 997& 0.292$\pm$0.001& 12.143$\pm$0.003& 0.172$\pm$0.002& 0.536$\pm$  0.004& 2.646$\pm$0.005& M\\
1042& 130&2204& 0.295$\pm$0.001& 12.898$\pm$0.003& 0.168$\pm$0.002& 0.496$\pm$  0.004& 2.671$\pm$0.004& M\\
1046& 131&1082& 0.266$\pm$0.003& 11.260$\pm$0.003& 0.120$\pm$0.006& 0.731$\pm$  0.008& 2.704$\pm$0.007& M\\
1050& 134& 984& 0.367$\pm$0.001& 12.259$\pm$0.003& 0.180$\pm$0.002& 0.409$\pm$  0.004& 2.626$\pm$0.000& M\\
1060& 136&1072& 0.418$\pm$0.001& 11.279$\pm$0.003& 0.160$\pm$0.002& 0.452$\pm$  0.004& 2.629$\pm$0.007& M\\
1140& 153& 968& 0.064$\pm$0.001& 11.267$\pm$0.003& 0.209$\pm$0.002& 0.987$\pm$  0.004& 2.803$\pm$0.008& M\\
1154& 156&1066& 0.059$\pm$0.001& 10.948$\pm$0.003& 0.203$\pm$0.003& 0.997$\pm$  0.004& 2.847$\pm$0.003& M\\
1176& 161&1036& 0.327$\pm$0.004& 12.760$\pm$0.004& 0.159$\pm$0.005& 0.380$\pm$  0.008& 2.660$\pm$0.006& M\\
1272& 184&1280& 0.165$\pm$0.001& 12.223$\pm$0.003& 0.174$\pm$0.002& 0.820$\pm$  0.004& 2.779$\pm$0.011& M\\
1274& 185&1263& 0.126$\pm$0.001& 11.062$\pm$0.003& 0.218$\pm$0.002& 0.949$\pm$  0.004& 2.639$\pm$0.012& M\\
1300& 190&1284& 0.166$\pm$0.002& 10.912$\pm$0.003& 0.173$\pm$0.003& 0.908$\pm$  0.004& 2.776$\pm$0.003& M\\
1351& 207&1195& 0.264$\pm$0.001& 12.301$\pm$0.003& 0.143$\pm$0.003& 0.551$\pm$  0.004&  & M\\
1370& 210&1273& 0.375$\pm$0.001& 12.220$\pm$0.003& 0.160$\pm$0.002& 0.403$\pm$  0.003& 2.641$\pm$0.011& M\\
1649& 282&1440& 0.349$\pm$0.005& 13.441$\pm$0.005& 0.112$\pm$0.007& 0.442$\pm$  0.007& & M\\
1087&4006&1031& 0.306$\pm$0.001& 13.277$\pm$0.003& 0.171$\pm$0.002& 0.428$\pm$  0.003& 2.648$\pm$0.008& M\\
1181&9226&2226& 0.294$\pm$0.004& 12.596$\pm$0.004& 0.139$\pm$0.005& 0.517$\pm$  0.006&  &  \\
1529& 261&1466& 0.146$\pm$0.002& 10.577$\pm$0.003& 0.275$\pm$0.003& 0.796$\pm$  0.004&  & M\\
 261&7489& 489& 0.321$\pm$0.002& 12.903$\pm$0.003& 0.187$\pm$0.003& 0.478$\pm$  0.004&  & M\\
 659&  30& 792& 0.403$\pm$0.002& 11.993$\pm$0.003& 0.132$\pm$0.003& 0.485$\pm$  0.004& 2.732$\pm$0.014& M\\
\hline
\end{tabular}
\label{BlueS67} 
}
\end{table}