\begin{table}%t1
   \caption{Visual and absolute magnitudes, $B-V$ color, Hipparcos 
              parallaxes, stellar masses (derived iterativey during the
              abundance analysis using the spectroscopic
              temperatures and abundances) and projected binary separation 
              for program stars. As discussed in the text, the formal errors
              on magnitudes and colors are likely underestimated.}
     \label{t:mag}
%\centering
\par
       \begin{tabular}{lccccccccccc}
         \hline
         \hline
         Object      &  $V_{A}$ &  $V_{B}$   & $(B-V)_{A}$ & $(B-V)_{B}$  & $\pi$  & $M_{V(A)}$  & $M_{V(B)}$ & $M_{A}$ & $M_{B}$ & $\rho$ & $\rho$ \\
         &  &  & &  & mas  &  &  & $M_{\odot}$ & $M_{\odot}$ & $''$ & AU \\
         \hline
HD~8009    & $8.819\pm0.007$ & $9.724\pm0.017$ & $0.64\pm0.03$ & $0.82\pm0.07$ & 15.43 $\pm$ 2.02 & 4.61 $\pm$ 0.29 & 5.52 $\pm$ 0.29 & 0.95 & 0.85 & 4.7 & 326 \\
HD~8071    & $7.312\pm0.003$ & $7.573\pm0.004$ & $0.58\pm0.01$ & $0.60\pm0.01$ & 19.67 $\pm$ 1.58 & 3.73 $\pm$ 0.17 & 3.99 $\pm$ 0.17 & 1.25 & 1.22 & 2.2 & 115 \\
HD~9911    & $9.428\pm0.008$ & $9.448\pm0.008$ & $0.90\pm0.04$ & $0.89\pm0.04$ & 20.40 $\pm$ 3.32 & 5.74 $\pm$ 0.36 & 5.76 $\pm$ 0.36 & 0.85 & 0.85 & 3.9 & 213 \\
HD 13357   & $8.180\pm0.006$ & $8.647\pm0.010$ & $0.67\pm0.03$ & $0.73\pm0.05$ & 20.41 $\pm$ 1.75 & 4.67 $\pm$ 0.19 & 5.14 $\pm$ 0.19 & 0.98 & 0.93 & 5.9 & 297 \\
HD~17159   & $8.775\pm0.007$ & $8.923\pm0.007$ & $0.54\pm0.03$ & $0.53\pm0.03$ & 14.65 $\pm$ 2.24 & 4.40 $\pm$ 0.33 & 4.55 $\pm$ 0.33 & 1.15 & 1.12 & 2.7 & 203 \\
HD~19440   & $7.874\pm0.004$ & $8.574\pm0.007$ & $0.47\pm0.01$ & $0.53\pm0.02$ & 12.55 $\pm$ 1.39 & 3.27 $\pm$ 0.24 & 3.96 $\pm$ 0.24 & 1.25 & 1.14 & 6.0 & 501 \\
HD 30101   & $8.782\pm0.009$ & $8.848\pm0.009$ & $0.82\pm0.04$ & $0.91\pm0.03$ & 23.43 $\pm$ 2.55 & 5.53 $\pm$ 0.24 & 5.66 $\pm$ 0.24 & 0.84 & 0.83 & 4.6 & 205 \\
HD 33334   & $8.023\pm0.004$ & $8.857\pm0.009$ & $0.70\pm0.03$ & $0.80\pm0.07$ & 21.39 $\pm$ 2.18 & 4.59 $\pm$ 0.22 & 5.42 $\pm$ 0.22 & 1.00 & 0.89 & 4.7 & 229 \\
HD~66491   & $9.253\pm0.009$ & $9.312\pm0.009$ & $0.75\pm0.05$ & $0.67\pm0.05$ & 15.11 $\pm$ 2.71 & 4.85 $\pm$ 0.39 & 4.91 $\pm$ 0.39 & 0.96 & 0.96 & 5.1 & 387 \\
BD+23 1978 & $9.395\pm0.010$ & $9.530\pm0.011$ & $0.80\pm0.06$ & $0.75\pm0.05$ & 24.04 $\pm$ 2.97 & 6.17 $\pm$ 0.27 & 6.31 $\pm$ 0.27 & 0.84 & 0.84 & 2.6 & 115 \\ 
HD 106515  & $7.960\pm0.005$ & $8.234\pm0.007$ & $0.79\pm0.02$ & $0.83\pm0.03$ & 27.50 $\pm$ 1.54 & 5.13 $\pm$ 0.12 & 5.41 $\pm$ 0.12 & 0.93 & 0.89 & 7.0 & 257 \\
HD 108574/5& $7.418\pm0.005$ & $7.972\pm0.007$ & $0.56\pm0.01$ & $0.67\pm0.02$ & 25.06 $\pm$ 1.81 & 4.37 $\pm$ 0.16 & 4.93 $\pm$ 0.16 & 1.22 & 1.11 & 9.8 & 399 \\
HD 123963  & $8.758\pm0.006$ & $9.511\pm0.010$ & $0.60\pm0.03$ & $0.54\pm0.04$ & 13.81 $\pm$ 1.74 & 4.33 $\pm$ 0.28 & 5.08 $\pm$ 0.28 & 1.08 & 0.96 & 2.6 & 200 \\
HD 132563  & $8.966\pm0.007$ & $9.472\pm0.010$ & $0.54\pm0.03$ & $0.57\pm0.05$ & 10.15 $\pm$ 2.01 & 3.62 $\pm$ 0.44 & 4.13 $\pm$ 0.44 & 1.13 & 1.06 & 4.2 & 491 \\
HD 132844  & $9.022\pm0.006$ & $9.114\pm0.007$ & $0.55\pm0.05$ & $0.63\pm0.05$ & 16.57 $\pm$ 2.05 & 4.99 $\pm$ 0.27 & 5.08 $\pm$ 0.27 & 1.01 & 0.99 & 3.0 & 192 \\
HD 135101  & $6.656\pm0.006$ & $7.500\pm0.009$ & $0.69\pm0.01$ & $0.75\pm0.02$ & 34.18 $\pm$ 1.78 & 4.30 $\pm$ 0.11 & 5.15 $\pm$ 0.11 & 0.97 & 0.95 & 23.5 & 694 \\
HD 190042  & $8.755\pm0.009$ & $8.778\pm0.006$ & $0.73\pm0.03$ & $0.80\pm0.04$ & 16.52 $\pm$ 1.64 & 4.76 $\pm$ 0.22 & 4.79 $\pm$ 0.22 & 0.96 & 0.94 & 4.2 & 264  \\ 
HD 200466  & $8.399\pm0.005$ & $8.528\pm0.006$ & $0.71\pm0.02$ & $0.79\pm0.03$ & 22.83 $\pm$ 1.75 & 5.14 $\pm$ 0.17 & 5.28 $\pm$ 0.17 & 0.99 & 0.97 & 4.7 & 210 \\ 
HIP 104687 & $8.144\pm0.006$ & $8.189\pm0.006$ & $0.64\pm0.06$ & $0.71\pm0.06$ & 20.87 $\pm$ 1.99 & 4.67 $\pm$ 0.21 & 4.72 $\pm$ 0.21 & 1.09 & 1.08 & 4.0 & 198 \\
HD 213013  & $8.982\pm0.008$ & $9.612\pm0.013$ & $0.81\pm0.04$ & $0.93\pm0.08$ & 21.59 $\pm$ 2.01 & 5.58 $\pm$ 0.20 & 6.21 $\pm$ 0.20 & 0.93 & 0.84 & 5.5 & 263 \\
HD 215812  & $7.275\pm0.005$ & $7.576\pm0.006$ & $0.64\pm0.02$ & $0.70\pm0.02$ & 31.94 $\pm$ 1.66 & 4.78 $\pm$ 0.11 & 5.08 $\pm$ 0.11 & 0.95 & 0.92 & 2.2 &  70 \\
HD 216122  & $8.062\pm0.011$ & $8.186\pm0.013$ & $0.58\pm0.02$ & $0.58\pm0.03$ & 13.11 $\pm$ 2.36 & 3.35 $\pm$ 0.40 & 3.47 $\pm$ 0.40 & 1.23 & 1.22 & 5.3 & 464 \\
HD 219542  & $8.174\pm0.006$ & $8.547\pm0.008$ & $0.64\pm0.03$ & $0.71\pm0.04$ & 18.30 $\pm$ 1.97 & 4.39 $\pm$ 0.23 & 4.78 $\pm$ 0.23 & 1.08 & 1.05 & 5.3 & 303 \\
         \hline
      \end{tabular}
\end{table}