\begin{table}%t2
\caption{\label{AbundanceDeviation}Primary abundances with respect to
solar values$^*$.}
\small%\centerline
{
\begin{tabular}{lcccccc}
\hline
\hline
                                  & \element[][]{H} &\element[][]{He}  & \element[][]{C} & \element[][]{N} & \element[][]{O} & \element[][]{Si}$_{{\rm (LTE)}}$ \\
\hline
Figure~\ref{UUSgeSixplotPrim}     & $12.00$         & $10.53$          & $8.19$          & $8.98$          & $8.56$          & $7.81$ \\
$75~000$~K                       & $(fix)$         & $-0.4$           & $-0.2$          & $+1.2$          & $-0.1$          & $\le$$ +0.3$ \\
\hline
Figure~\ref{UUSgeSixplotPrim85}   & $12.00$         & $10.73$          & $8.19$          & $9.28$          & $8.56$          & $7.81$ \\
$85~000$~K                       & $(fix)$         & $-0.2$           & $-0.2$          & $+1.5$          & $-0.1$          & $\le $$+0.3$ \\
\hline
Figure~\ref{UUSgeSixplotPrimLogg} & $12.00$         & $10.43$          & $8.19$          & $9.38$          & $8.56$          & $7.81$ \\
$85~000$~K$^{**}$                & $(fix)$         & $-0.5$           & $-0.2$          & $+1.6$          & $-0.1$          & $\le$$ +0.3$ \\
\hline
\end{tabular}}
\smallskip 
 $^*$ Based on \cite{2005Asplund}.\\
 $^{**}$ Reduced $\log g_{{\rm p}} = 4.5$ to match \ion{He}{ii}
$\lambda 4686$. 
\end{table}