\begin{table}%t7
\caption{Abundance uncertainties linked to stellar parameters.
Case of the "warm" star CS~22948--066.}
\label{errTemp2}
%\centering
\par
\begin{tabular}{lrrrr}
\hline  \hline
\multicolumn {2}{l}{CS~22948--066}\\
\multicolumn {5}{c}{A: $T_{{\rm eff}}=$ 5100 K, log $g$ = 1.8 dex, \vt~= 2.0 
km s$^{-1}$}\\
\multicolumn {5}{c}{B: $T_{{\rm eff}}=$ 5100 K, log $g$ = 1.7 dex, \vt~= 2.0 
km s$^{-1}$}\\
\multicolumn {5}{c}{C: $T_{{\rm eff}}=$ 5100 K, log $g$ = 1.8 dex, \vt~= 1.8 
km s$^{-1}$}\\
\multicolumn {5}{c}{D: $T_{{\rm eff}}=$ 5000 K, log $g$ = 1.8 dex, \vt~= 2.0 
km s$^{-1}$}\\
\multicolumn {5}{c}{E: $T_{{\rm eff}}=$ 5000 K, log $g$ = 1.5 dex, \vt~= 2.0 
km s$^{-1}$}\\
\hline
El.   & $\Delta_{B-A} $ & $\Delta_{C-A} $& $\Delta_{D-A} $& 
$\Delta_{E-A} $\\
\hline
[Fe/H]      &$-$0.02 & 0.02 &$-$0.05 &$-$0.11\\
$[$O I/Fe]  &$-$0.01 &$-$0.02 &$-$0.02 &$-$0.05\\
$[$Na I/Fe] & 0.03 & 0.08 &$-$0.04 & 0.05\\
$[$Mg I/Fe] & 0.04 & 0.06 &$-$0.01 & 0.10\\
$[$Al I/Fe] & 0.03 & 0.05 &$-$0.04 & 0.04\\
$[$Si I/Fe] & 0.03 & 0.05 &$-$0.05 & 0.04\\
$[$K I/Fe]  & 0.02 &$-$0.02 &$-$0.03 & 0.05\\
$[$Ca I/Fe] & 0.02 &$-$0.01 &$-$0.02 & 0.05\\
$[$Sc II/Fe]&$-$0.01 & 0.02 & 0.00 &$-$0.03\\
$[$Ti I/Fe] & 0.02 &$-$0.02 &$-$0.07 &$-$0.01\\
$[$Ti II/Fe]&$-$0.01 & 0.03 & 0.00 &$-$0.03\\
$[$Cr I/Fe] & 0.03 & 0.03 &$-$0.06 & 0.02\\
$[$Mn I/Fe] & 0.03 & 0.05 &$-$0.06 & 0.02\\
$[$Fe I/Fe] & 0.02 & 0.03 &$-$0.06 & 0.02\\
$[$Fe II/Fe]&$-$0.02 &$-$0.02 & 0.06 &$-$0.01\\
$[$Co I/Fe] & 0.03 & 0.02 &$-$0.07 & 0.01\\
$[$Ni I/Fe] & 0.02 & 0.10 &$-$0.07 & 0.01\\
$[$Zn I/Fe] & 0.01 &$-$0.02 & 0.00 & 0.03\\
$[$O I/Mg I]&$-$0.05 &$-$0.08 &$-$0.01 &$-$0.15\\
$[$O/Mg]$^*$&$-$0.01 &$-$0.03 &$-$0.13 &$-$0.12\\
\hline
\multicolumn{5}{l}{Note: [O/Mg]$^*$ = [O~I/Fe~II]-[Mg~I/Fe~I].}
\end{tabular}
\end{table}