\begin{table}%t2
\caption{\label{tab:onlinebensby}Equivalent widths and elemental abundances based on method~1$^{a}$.} 
\par
\small%\centerline
 {
{
\begin{tabular}{rlccc|ccc|ccc|ccc|ccc|ccc}
\hline\hline
        &
        &
        &
        &
        &
\multicolumn{3}{c|}{Sun}        &
\multicolumn{3}{c|}{OGLE-2008-BLG-209S}  &
\multicolumn{3}{c|}{OGLE-2006-BLG-265S}  &
\multicolumn{3}{c|}{MOA-2006-BLG-099S}  &
\multicolumn{3}{c}{OGLE-2007-BLG-349S}  \\
\multicolumn{2}{c}{element}     &
wavelength &
$\log gf$        &
$\chi_{\rm l}$    &
$W_{\rm \lambda,\odot}$ &
$\log \epsilon (X)_{\odot}$ &
flag    &
$W_{\rm \lambda}$ & 
$\log \epsilon (X)$ &
[$X$/H] &
$W_{\rm \lambda}$ & 
$\log \epsilon (X)$ &
[$X$/H] &
$W_{\rm \lambda}$ & 
$\log \epsilon (X)$ &
[$X$/H] &
$W_{\rm \lambda}$ &
$\log \epsilon (X)$ &
[$X$/H]         \\
\hline
 Al & 1 & 5557.063  & --2.21 & 3.14 &  10.4 & 6.44 & -- &  17.1 & 6.45 &  0.01 &  39.9 & 7.04 &  0.60 &  29.4 & 7.00 &  0.56 &  37.9 & 6.89 &  0.45   \\
 Al & 1 & 6696.023  & --1.62 & 3.14 &  44.9 & 6.62 & -- &  47.9 & 6.45 & -0.17 &  87.8 & 7.09 &  0.47 &  58.8 & 6.84 &  0.23 &  89.5 & 7.03 &  0.41   \\
\vdots &
\vdots &
\vdots &
\vdots &
\vdots &
\vdots &
\vdots &
\vdots &
\vdots &
\vdots &
\vdots &
\vdots &
\vdots &
\vdots &
\vdots &
\vdots &
\vdots &
\vdots &
\vdots &
\vdots \\
\hline
\end{tabular}}}
\medskip
$^{a}$ For each line we give the $\log gf$ value, lower excitation potential~($\chi_{\rm l}$), measured equivalent widths~($W_{\rm \lambda}$), derived absolute abundance~($\log \epsilon (X)$), abundance normalised to the Sun (on a line-by-line basis) ([$X$/H]). The ``flag'' for the Sun indicates that a line has not been measured in the solar spectrum and that the abundance given (and used in the normalisation) for that line is the average abundance based on all the other lines, that could be measured in the solar spectrum, of the same species. The full table is only available in electronic form at the CDS.
\end{table}