\begin{table}%t1
 \caption{Photometry and physical parameters for the five stars.\label{tabstars}}
%\centerline
{\begin{tabular}{llllllccc}
\hline\hline
{Number$^a$} & {$V$} & {$(B-V)$}{$_0$} &
{$T$}{$_{\rm eff}$} & {$\log{g}$} & {\boldmath $\xi$} & $\alpha(J2000)$& $ \delta (J2000)$ & ${v_{r}}^b$\\
 & mag & mag & K & cgs & \kms & hms & $^\circ,',''$ & \kms \\
\hline
 \object{1272}     & 16.62 & 1.15 & 4421 & 1.2 & 1.45 &19 17 37.1 & --34 39 11.9 & 158.9 \\
 \object{1282}$^c$ & 16.08 & 1.30 & 4203 & 1.3 & 1.60 &19 17 39.4 & --34 39 06.4 & 158.2 \\
 \object{1515}     & 16.76 & 1.12 & 4468 & 2.0 & 1.45 &19 17 38.2 & --34 39 16.8 & 157.8 \\
 \object{1665}$^d$ & 15.04 & 1.50 & 3945 & 0.8 & 1.60 &19 17 43.2 & --34 39 43.2 & 159.6\\
 \object{1708}$^e$ & 16.08 & 1.28 & 4231 & 1.2 & 1.70 &19 17 43.5 & --34 39 12.4 & 160.6\\
\hline
\end{tabular}}
\smallskip
$^a$ Referred to the catalog of Buonanno et~al. (1995), available via CDS 
 at {\tt http://cdsweb.u-strasbg.fr/cgi-bin/qcat?J/AJ/109/663/}  
$^b$ The presented $v_r$ is the heliocentric value.\\   
$^c$ This is star \object{S34} in \citet{tarantella04}.  \\ 
$^d$ This is star \object{S16} in \citet{tarantella04}.\\ 
$^e$ This is star \object{S35} in \citet{tarantella04}.
\end{table}