\begin{table}%tb1
\caption{$V$ and $K_{\rm s}$ magnitudes,  Str\"{o}mgren indices, and
photometric and spectroscopic indices of the strength of the H$\beta$ line.
The derived interstellar reddening of \by\ is given in Col.~10, and the absolute
visual magnitude derived from the Str\"{o}mgren photometry is given in Col.~11. 
Columns~12 and~13 give the absolute visual magnitude and its 1-$\sigma$ error derived from the 
Hipparcos parallax if available with an error less than~30\%.}
\label{tab:B.1}
\small%\centerline
{
\begin{tabular}{lrrccccccrccc}
\noalign{\smallskip}
\hline\hline
\noalign{\smallskip}
  ID   &   $V$ & $K_{\rm s}$ &  $b-y$ & $m_1$  &$c_1$ & $\beta$(phot) & Ref.$^{a}$ & $\beta$(UVES) & $E(b-y)$ & $M_{V}$(phot)
  & $M_{V}$(par) & $\sigma$   \\
\noalign{\smallskip}
\hline
\noalign{\smallskip}
\object{BD~$-13\degr3442$} & 10.288 &  9.018 & 0.308 & 0.050 & 0.385 & 2.622 & 4 &  8.820 &  0.022 &  3.67 &       & \\      
\object{CD~$-30\degr18140$} &  9.949 &  8.655 & 0.323 & 0.047 & 0.344 & 2.606 & 1 &  8.755 &  0.019 &  3.88 &  4.19 &  0.46 \\
\object{CD~$-35\degr14849$} & 10.568 &  9.293 & 0.321 & 0.040 & 0.293 & 2.603 & 1 &  8.751 &  0.011 &  4.47 &       & \\     
\object{CD~$-42\degr14278$} & 10.216 &  8.770 & 0.361 & 0.040 & 0.229 & 2.576 & 1 &  8.587 &  0.015 &  4.94 &       & \\      
\object{G~11-44} & 11.091 &  9.740 & 0.335 & 0.061 & 0.248 & 2.588 & 1 &  8.660 & $-$0.005 &  4.80 &       &  \\      
\object{G~13-09} &  9.998 &  8.739 & 0.311 & 0.048 & 0.373 & 2.609 & 1 &  8.806 &  0.021 &  3.75 &  3.70 &  0.59  \\
\object{G~18-39} & 10.392 &  9.017 & 0.346 & 0.073 & 0.286 & 2.581 & 1 &  8.638 &  0.002 &  4.35 &       &        \\
\object{G~20-08} &  9.948 &  8.498 & 0.356 & 0.047 & 0.251 & 2.574 & 1 &  8.671 &  0.020 &  4.79 &  4.47 &  0.43  \\
\object{G~24-03} & 10.467 &  9.020 & 0.363 & 0.057 & 0.271 & 2.585 & 1 &  8.616 &  0.019 &  4.53 &       &        \\      
\object{G~29-23} & 10.230 &  8.831 & 0.339 & 0.059 & 0.332 & 2.590 & 1 &  8.706 &  0.017 &  3.87 &       &        \\
\object{G~53-41} & 11.022 &  9.595 & 0.356 & 0.083 & 0.271 & 2.589 & 1 &  8.580 & $-$0.003 &  4.54 &     &        \\     
\object{G~64-12} & 11.459 & 10.208 & 0.307 & 0.043 & 0.337 & 2.617 & 4 &  8.860 &  0.020 &  4.37 &       &        \\
\object{G~64-37} & 11.144 &  9.923 & 0.300 & 0.054 & 0.333 & 2.623 & 4 &  8.861 &  0.007 &  4.31 &       &        \\
\object{G~66-30} & 11.028 &  9.789 & 0.305 & 0.072 & 0.358 & 2.634 & 1 &  8.962 &  0.016 &  4.20 &       &        \\
\object{G~126-62} &  9.478 &  8.075 & 0.330 & 0.063 & 0.327 & 2.588 & 1 &  8.739 &  0.012 &  4.00 &  4.06 &  0.37 \\
\object{G~186-26} & 10.829 &  9.590 & 0.306 & 0.041 & 0.339 & 2.608 & 1 &  8.844 &  0.019 &  4.31 &  5.12 &  0.50 \\
\object{HD~106038} & 10.179 &  8.761 & 0.342 & 0.092 & 0.264 & 2.583 & 1 &  8.595 & $-$0.017 &  4.69 &  4.99 &  0.36 \\
\object{HD~108177} &  9.671 &  8.354 & 0.330 & 0.059 & 0.287 & 2.594 & 1 &  8.665 & $-$0.002 &  4.36 &  4.87 &  0.26 \\
\object{HD~110621} &  9.906 &  8.566 & 0.337 & 0.067 & 0.324 & 2.595 & 1 &  8.679 &  0.007 &  3.89 &  4.12 &  0.46   \\
\object{HD~140283} &  7.213 &  5.588 & 0.380 & 0.033 & 0.284 & 2.564 & 1 &  8.434 &  0.013 &  3.83 &  3.36 &  0.12   \\
\object{HD~160617} &  8.733 &  7.311 & 0.347 & 0.051 & 0.331 & 2.584 & 1 &  8.594 &  0.010 &  3.51 &  3.37 &  0.31   \\
\object{HD~179626} &  9.210 &  7.680 & 0.373 & 0.095 & 0.293 & 2.588 & 1 &  8.551 &  0.005 &  4.29 &  3.57 &  0.39   \\
\object{HD~181743} &  9.687 &  8.274 & 0.351 & 0.052 & 0.224 & 2.582 & 1 &  8.567 & $-$0.001 &  4.97 &  4.95 &  0.34 \\
\object{HD~188031} & 10.148 &  8.857 & 0.328 & 0.058 & 0.310 & 2.592 & 1 &  8.730 &  0.009 &  4.19 &       &         \\
\object{HD~193901} &  8.660 &  7.144 & 0.383 & 0.099 & 0.221 & 2.568 & 1 &  8.443 & $-$0.006 &  5.16 &  5.46 &  0.12 \\
\object{HD~194598} &  8.354 &  6.982 & 0.344 & 0.091 & 0.269 & 2.588 & 1 &  8.624 & $-$0.011 &  4.63 &  4.62 &  0.15 \\
\object{HD~215801} & 10.044 &  8.642 & 0.334 & 0.049 & 0.330 & 2.572 & 1 &  8.589 & $-$0.001 &  3.47 &       &         \\
\object{LP~815-43} & 10.912 &  9.650 & 0.304 & 0.048 & 0.382 & 2.623 & 1 &  8.913 &  0.031 &  4.18 &       &         \\
\object{CD~$-24\degr17504$} & 12.124 & 10.807 & 0.322 & 0.043 & 0.283 & 2.609 & 4 &  8.770 &  0.010 &  4.60 &       & \\     
\object{CD~$-71\degr1234$} & 10.44  &  9.114 &       &       &      &       & 5 &  8.790 &  0.019 &  3.67 &       &  \\    
\object{CS~22943-095} & 11.762 & 10.469 & 0.324 & 0.045 & 0.335 & 2.619 & 3 &  8.804 &  0.025 &  4.17 &       &     \\ 
\object{G~04-37} & 11.426 &  9.974 & 0.363 & 0.031 & 0.306 & 2.614 & 4 &  8.759 &  0.053 &  4.43 &       &      \\
\object{G~48-29} & 10.467 &  9.264 & 0.298 & 0.057 & 0.351 & 2.620 & 4 &  8.911 &  0.013 &  4.29 &       &      \\
\object{G~59-27} & 10.892 &  9.560 & 0.321 & 0.058 & 0.301 & 2.595 & 1 &  8.750 &  0.004 &  4.32 &       &      \\
\object{G~126-52} & 10.996 &  9.719 & 0.322 & 0.045 & 0.347 & 2.608 & 2 &  8.846 &  0.031 &  4.20 &       &      \\
\object{G~166-54} & 11.005 &  9.731 & 0.324 & 0.043 & 0.322 & 2.619 & 4 &  8.842 &  0.027 &  4.42 &       &      \\
\object{HD~84937} &  8.332 &  7.062 & 0.303 & 0.056 & 0.354 & 2.613 & 1 &  8.821 &  0.009 &  3.95 &  3.77 &  0.19 \\
\object{HD~338529} &  9.370 &  8.144 & 0.308 & 0.045 & 0.366 & 2.600 & 1 &  8.832 & 0.023 &  3.98 &  3.48 &  0.46 \\
\object{LP~635-14} & 11.362 &  9.997 & 0.347 & 0.026 & 0.366 & 2.611 & 4 &  8.820 & 0.060 &  4.02 &       &      \\
\object{LP~651-4} & 12.053 & 10.842 & 0.321 & 0.023 & 0.340 & 2.615 & 4 &  8.813 &  0.033 &  4.27 &       &      \\
\hline
\end{tabular}}
\smallskip
 $^{a}$  References of $V$, $b-y$, $m_1$, $c_1$ and $\beta$(phot): (1) Schuster \& Nissen (\cite{schuster88});
(2) Schuster et~al. (\cite{schuster93}); (3) Schuster et~al. (\cite{schuster96}); (4) Schuster et~al. (\cite{schuster06});
(5) Ryan (\cite{ryan89}). For all stars, $K_{\rm s}$ has been taken from the 2MASS catalogue (Skrutski et~al.
\cite{skrutskie06}).
\end{table}