\begin{table}%t5
\caption{\label{tab:err}Abundance changes from changing stellar parameters.}             
%\centering
\small         
\begin{tabular}{lcccc}
\hline\hline       
     & $\delta$({\teff}) & $\delta$({\logg}) & $\delta$([Fe/H]) & $\delta$({\vt}) \\
     & +150~K & +0.3~dex & +0.3~dex & +0.3~{\kms} \\ 
\hline
Fe {\small I}  & 0.19     & $-$0.04 & 0.00    & $-$0.06 \\
Fe {\small II} & 0.02     & 0.08    & 0.00    & $-$0.05 \\
Na {\small I} & 0.03     & $-$0.05 & $-$0.02 & $-$0.09 \\
Mg {\small I}  & $-$0.02  & $-$0.04 & 0.00    & $-$0.01 \\
Ca {\small I}  & $-$0.07  & 0.01    & 0.01    & 0.04 \\
Sc {\small II} & $-$0.12  & 0.12    & 0.00    & 0.04 \\
Ti {\small I}  & 0.00     & 0.00    & 0.01    & 0.04 \\
Ti {\small II} & $-$0.12  & 0.11    & 0.00    & $-$0.01 \\
Cr {\small I}  & 0.01     & $-$0.01 & 0.00    & $-$0.03 \\
Ni {\small I}  & $-$0.05  & 0.02    & 0.01    & 0.06  \\
Ba {\small II} & $-$0.08  & 0.12    & 0.00    & 0.05  \\
\hline
\end{tabular}
\end{table}