\begin{table}%T4 
\par
\caption{\label{tab:abundances}Measured equivalent widths and calculated elemental abundances for each star\tablefootmark{\dag}$\!$.                                 } 
\small%\centering
\par
\begin{tabular}{lccrccrcrcrcrcrcrcrcrc}
\hline\hline
\noalign{\smallskip} 
        &        &
        &\multicolumn{3}{c}{Sun}               &
\multicolumn{2}{c}{ob09076}  &
\multicolumn{2}{c}{mb09493}  &
\multicolumn{2}{c}{mb09133}  &
\multicolumn{2}{c}{mb09475}  &
\multicolumn{2}{c}{mb99022}  &
\multicolumn{2}{c}{mb09489}  &
\multicolumn{2}{c}{mb09456}  &
\multicolumn{2}{c}{mb09259}  \\
El.    &
$\lambda$ &
$\chi_{\rm l}$    &
$W_{\rm \lambda}$ &
$X$ &
flg    &
$W_{\rm \lambda}$ &
$X$ &
$W_{\rm \lambda}$ &
$X$ &
$W_{\rm \lambda}$ &
$X$ &
$W_{\rm \lambda}$ &
$X$ &
$W_{\rm \lambda}$ &
$X$ &
$W_{\rm \lambda}$ &
$X$ &
$W_{\rm \lambda}$ &
$X$ &
$W_{\rm \lambda}$ &
$X$ \\
\hline
\ion{Al}{i } & 6696.023 & 3.14 &  38.3 & 6.51 &      0 &   --  &  --  &  20.6 & 5.99 &  20.4 & 6.06 &   --  &  --  &  28.6 & 6.30 &  37.5 & 6.45 &  47.7 & 6.64 &   --  &  --   \\
\ion{Al}{i } & 6698.673 & 3.14 &  20.7 & 6.47 &      0 &   --  &  --  &  12.3 & 6.04 &   7.5 & 5.88 &   --  &  --  &  17.3 & 6.32 &  20.3 & 6.39 &  33.6 & 6.70 &   --  &  --   \\
\vdots &
\vdots &
\vdots &
\vdots &
\vdots &
\vdots &
\vdots &
\vdots &
\vdots &
\vdots &
\vdots &
\vdots &
\vdots &
\vdots &
\vdots &
\vdots &
\vdots &
\vdots &
\vdots &
\vdots \\
\hline
\end{tabular}
\tablefoot{\tablefoottext{\dagger}{For each spectral line we give the lower excitation potential ($\chi_{\rm l}$), measured equivalent widths ($W_{\rm \lambda}$),
derived absolute abundance ($X \equiv \log \epsilon (X)$). We have only included the stars that are new to this work.
The table is only available in  electronic
form at the CDS.}}
\end{table}