\begin{table}%t16
%\centering
\par
\caption{Sample stars with published $^6$Li detection. 
The data are from Smith et~al. (\cite{Smith98}, sln98), Cayrel et~al. (\cite{Cayrel99}a, c99) and
Nissen et~al. (\cite{Nissen00}, n00). Columns 2 and 3 give the \teff(2) and [Fe/H]
values that we attributed to the stars while Cols.~4 and~5 display the
values quoted in the original papers. For completeness, we note that a
re-analysis by Asplund et~al. (\cite{Asplund05}) of HIP 8572 and HIP 96115 from very
high resolution and {\it S/N} UVES (Dekker et~al. 1999) spectra finds a slightly
less than 2$\sigma$ detection for HIP 8572 and no $^6$Li detection for HIP
96115.\label{tab16}}
\footnotesize {
{
\begin{tabular}{cccccccc}
\noalign{\smallskip}
\hline
\hline
\noalign{\smallskip}
 HIP   & \teff & [Fe/H] & \teff    & [Fe/H]   & Li      & $^6$Li/$^7$Li & Ref \\
       & (2)   &        & lit & lit & NLTE    &               &     \\
\noalign{\smallskip}
\hline
8572   & 6287 & --2.51 & 6295 & --2.15 & 2.236 & $0.02\pm0.01$ & n00 \\
48152  & 6377 & --2.28 & 6300 & --2.30 & 2.249 & $0.05\pm0.02$ & c99 \\
       &      &       & 6300 & --2.25 &       & $0.06\pm0.02$ & n00 \\
96115  & 6322 & --2.42 & 6280 & --2.60 & 2.223 & $0.05\pm0.03$ & sln98 \\
\hline
\end{tabular}
}
}
\end{table}