\begin{table}%t10
\caption {\label{sun}Solar abundance values. }                  
%\centering
\par
\begin{tabular}{l c c c c c}     
\hline\hline 
\noalign{\smallskip}      
Element & [X/H]$_{\rm derived}$ & log$\epsilon_{\rm GS96}$ & log$\epsilon_{\rm A05}$ \\
%        & & & \\
\hline      
Al      & --0.34~$\pm$~N.A.($\pm$0.05) & 6.47~$\pm$~0.07 & 6.37~$\pm$~0.07 \\
Ba      &  +0.34~$\pm$~0.02($\pm$0~.06) & 2.13~$\pm$~0.05 & 2.17~$\pm$~0.07 \\
Ca	& --0.09~$\pm$~0.03($\pm$0.03) & 6.36~$\pm$~0.02 & 6.31~$\pm$~0.04 \\
Co	&  +0.05~$\pm$~0.02($\pm$0.06) & 4.92~$\pm$~0.04 & 4.92~$\pm$~0.08 \\
Cr	&  +0.02~$\pm$~0.05($\pm$0.06) & 5.67~$\pm$0~.03 & 5.64~$\pm$~0.10 \\
FeI     &  +0.01~$\pm$~0.01($\pm$0.10) & 7.50~$\pm$~0.04 & 7.45~$\pm$~0.05 \\
FeII    & --0.03~$\pm$~0.02($\pm$0.10) & 7.50~$\pm$~0.04 & 7.45~$\pm$~0.05 \\
La      &   --                      & 1.17~$\pm$~0.07 & 1.13~$\pm$~0.05 \\
Mg	&   --                      & 7.58~$\pm$~0.05 & 7.53~$\pm$~0.09 \\
Na      & --0.10~$\pm$~0.01($\pm$0.04) & 6.33~$\pm$~0.03 & 6.17~$\pm$~0.04 \\
Nd      &   --                      & 1.42~$\pm$~0.06 & 1.45~$\pm$~0.05 \\
Ni	&  +0.01~$\pm$~0.01($\pm$0.03) & 6.25~$\pm$~0.01 & 6.23~$\pm$~0.04 \\     
O       &  --0.01~$\pm$~0.07($\pm$0.08) & 8.87$\pm$0.07 & 8.66~$\pm$~0.05 \\
Sc	&  +0.06~$\pm$~0.02($\pm$0.08) & 3.17~$\pm$~0.10 & 3.05~$\pm$~0.08 \\
Si	& --0.08~$\pm$~0.01($\pm$0.07) & 7.55~$\pm$~0.05 & 7.51~$\pm$~0.04 \\
Ti	&  +0.03~$\pm$~0.05($\pm$0.06) & 5.02~$\pm$~0.06 & 4.90~$\pm$~0.06 \\
V 	& --0.14~$\pm$~0.02($\pm$0.14) & 4.00~$\pm$~0.02 & 4.00~$\pm$~0.02 \\
Y       &   --                      & 2.24~$\pm$~0.03 & 2.21~$\pm$~0.02 \\
\hline             	  
\end{tabular}
\tablefoot {The second column shows our derived solar
abundance (Sect.~\ref{sec-sun}) with its uncertainty (Sect.~\ref{sec-err1}).
The uncertainty listed for [O/H] is derived  from the spectral synthesis fit.
The last two columns report our adopted solar abundances \citep{gre96} and the
values by \citet{asp05}, as a reference.}	   
\end{table}