\begin{table}%t2
\caption{Atmospheric abundances in the Ap star HD~133792 with the error
estimates based on~$n$ measured lines. Abundances in the solar atmosphere and in the evolved Ap~star HD~204411 are given for \mbox{comparison}.}
\label{Abund}
%\centering
\small
\begin{tabular}{l|lr|l|c}
\hline
\hline
Ion &\multicolumn{2}{c|}{\hd} & HD~204411  & Sun \\                                  
    &$\log~ (N/N_{\rm tot})$ & $n$ &$\log~ (N/N_{\rm tot})$ & $\log~ (N/N_{\rm tot})$ \\       
\hline
\ion{Be}{ii}  &  $-$11.80:         &  2 &         & ~$-$10.66~ \\                                  
\ion{C}{i}    & $-$4.68 $\pm$ 0.07 &  2 & ~$-$4.37& ~~$-$3.65~ \\
\ion{N}{i}    & $-$5.16 $\pm$ 0.08 &  2 & ~$-$3.93& ~~$-$4.26~ \\			
\ion{O}{i}    & $-$4.23 $\pm$ 0.42 &  5 & ~$-$4.03& $-$3.38~ \\			
\ion{Na}{i}   & $-$5.35 $\pm$ 0.22 &  2 & ~$-$5.28& ~~$-$5.87~ \\			
\ion{Mg}{i}   & $-$3.91 $\pm$ 0.02 &  5 & ~$-$4.34& ~~$-$4.51~ \\	
\ion{Mg}{ii}  & $-$4.18 $\pm$ 0.68 &  2 & ~$-$4.62& ~~$-$4.51~ \\			
\ion{Al}{ii}  & $-$6.03:	   &  1 & ~$-$5.85& ~~$-$5.67~ \\			
\ion{Si}{i}   & $-$3.69 $\pm$ 0.21 &  3 & ~$-$4.13& ~~$-$4.53~ \\			
\ion{Si}{ii}  & $-$5.09 $\pm$ 0.50 &  5 & ~$-$4.11& ~~$-$4.53~ \\			
\ion{Ca}{i}   & $-$5.31 $\pm$ 0.20 &  2 & ~$-$5.17& ~~$-$5.73~ \\			
\ion{Ca}{ii}  & $-$7.36 $\pm$ 0.83 &  3 & ~$-$4.67& ~~$-$5.73~ \\			
\ion{Sc}{ii}  & $-$9.50 $\pm$ 0.38 &  2 & ~$-$9.52& ~~$-$8.99~ \\			
\ion{Ti}{ii}  & $-$6.88 $\pm$ 0.18 & 50 & ~$-$6.49& ~~$-$7.14~ \\			
\ion{V}{ii}   & $-$8.14 $\pm$ 0.17 &  8 &         & ~~$-$8.04~ \\			
\ion{Cr}{i}   & $-$3.79 $\pm$ 0.20 &131 & ~$-$4.85& ~~$-$6.40~ \\			
\ion{Cr}{ii}  & $-$3.75 $\pm$ 0.22 &320 & ~$-$4.70& ~~$-$6.40~ \\			
\ion{Mn}{i}   & $-$5.55 $\pm$ 0.17 & 13 & ~$-$5.96& ~~$-$6.65~ \\			
\ion{Mn}{ii}  & $-$5.39 $\pm$ 0.10 &  9 & ~$-$5.66& ~~$-$6.65~ \\			
\ion{Fe}{i}   & $-$3.31 $\pm$ 0.20 &247 & ~$-$3.76& ~~$-$4.59~ \\			
\ion{Fe}{ii}  & $-$3.18 $\pm$ 0.25 &347 & ~$-$3.52& ~~$-$4.59~ \\			
\ion{Co}{i}   & $-$6.49 $\pm$ 0.16 &  6 & ~$-$6.19& ~~$-$7.12~ \\			
\ion{Co}{ii}  & $-$5.99 $\pm$ 0.79 &  6 & ~$-$6.50& ~~$-$7.12~ \\			
\ion{Ni}{i}   & $-$6.05 $\pm$ 0.25 & 15 & ~$-$5.68& ~~$-$5.81~ \\			
\ion{Ni}{ii}  & $-$5.96 $\pm$ 0.11 &  2 & ~$-$5.31& ~~$-$5.81~ \\			
\ion{Sr}{i}   & $-$5.71 $\pm$ 0.37 &  8 & ~$-$7.74& ~~$-$9.12~ \\			
\ion{Sr}{ii}  & $-$6.36 $\pm$ 0.09 &  3 & ~$-$8.5 & ~~$-$9.12~ \\			
\ion{Y}{ii}   & $-$9.12 $\pm$ 0.46 &  6 & ~$-$9.95& ~~$-$9.83~ \\			
\ion{Zr}{ii}  & $-$9.47 $\pm$ 0.10 &  7 & ~$-$8.66& ~~$-$9.45~ \\			
\ion{Ru}{ii}  & $-$8.82:	   &  1 &	   & ~$-$10.20~ \\			
\ion{Pd}{i }  & $-$7.33 $\pm$ 0.10 &  2 &	   & ~$-$10.35~ \\			
\ion{Ba}{ii}  & $-$8.73 $\pm$ 0.16 &  4 & ~$-$9.02& ~~$-$9.87~ \\			
\ion{La}{iii} & $\le$$-$9.6	   &  2 &	   & ~$-$10.46~ \\			
\ion{Ce}{ii}  & $-$9.07:	   &  1 & $-$10.26& ~$-$10.46~ \\			
\ion{Ce}{iii} & $-$8.41 $\pm$ 0.07 &  3 &	  & ~$-$10.46~ \\			
\ion{Pr}{iii} & $-$9.51 $\pm$ 0.17 &  3 & $<$$-$10.5& ~$-$11.33~ \\			
\ion{Nd}{ii}  & $-$9.08 $\pm$ 0.43 &  3 & ~$-$9.48& ~$-$10.59~ \\			
\ion{Nd}{iii} & $-$9.10 $\pm$ 0.01 &  2 & $-$10.05& ~$-$10.59~ \\			
\ion{Sm}{ii}  & $\le$$-$10.4         &  1 &         & ~$-$11.03~ \\                            
\ion{Eu}{ii}  & $-$9.80 $\pm$ 0.20   &  4 & $-$10.95& ~$-$11.52~ \\                             
\ion{Gd}{ii}  & $-$9.60 $\pm$ 0.04 &  2 &         & ~$-$10.92~ \\                             
\ion{Dy}{ii}  & $-$10.02 $\pm$ 0.38  &  3 &         & ~$-$10.90~ \\			
\ion{Er}{ii}  & $\le$$-$9.4        &  1 &         & ~$-$11.11~ \\			
\hline						
\te     &\multicolumn{2}{c|}{9400~K}   & 8400~K      & 5777~K  \\			
\lgg    &\multicolumn{2}{c|}{3.70~~~~~}& 3.50        & 4.44~~~~\\			
\bs     &\multicolumn{2}{c|}{1.1~kG}   &$\le$0.7~kG  & 	       \\			
\hline						
\end{tabular}
\end{table}