\begin{table}%t1
%\centering
\par
\caption{Atmospheric abundances in the Cr-type star HD~204411 with the error
estimates based on $n$ measured lines.\label{Abund}}	
\begin{footnotesize}
\begin{tabular}{llrlcc}
\noalign{\smallskip}
\hline\hline
Ion &\multicolumn{2}{c}{8400g35} &8700g34  &CA& $\sun$ \\
    &$\log (N/N_{\rm tot})$ & $n$ &$\log (N/N_{\rm tot})$ & $\log (N/N_{\rm tot})$ & $\log (N/N_{\rm tot})$ \\
\hline
\ion{C}{i}   & ~$-$$4.37\pm0.17$ &  5 &~$-$$4.19\pm0.17$ &     & ~~$-$3.45~ \\
\ion{N}{i}   & ~$-$$3.93\pm0.37$ &  3 &~$-$$3.94\pm0.37$ &     & ~~$-$4.11~ \\
\ion{O}{i}   & ~$-$$4.03\pm0.33$ &  4 &~$-$$4.05\pm0.33$ &     & ~~$-$3.30~ \\
\ion{Na}{i}   & ~$-$$5.28\pm0.20$ &  4 &~$-$$5.01\pm0.24$ &     & ~~$-$5.71~ \\
\ion{Mg}{i}   & ~$-$$4.34\pm0.22$ &  6 &~$-$$4.07\pm0.21$ & ~$-$4.8 & ~~$-$4.50~ \\
\ion{Mg}{ii}  & ~$-$$4.62\pm0.55$ &  3 &~$-$$4.67\pm0.63$ & ~$-$4.8 & ~~$-$4.50~ \\
\ion{Al}{ii}  & ~$-$5.85          &  1 &~$-$ 5.85        	  &	    & ~~$-$5.57~ \\
\ion{Si}{i}   & ~$-$$4.13\pm0.11$ &  7 &~$-$$3.90\pm0.11$ & ~$-$4.4 & ~~$-$4.50~ \\
\ion{Si}{ii}  & ~$-$$4.11\pm0.07$ &  2 &~$-$$4.23\pm0.07$ & ~$-$4.5 & ~~$-$4.50~ \\
\ion{S}{i}   & ~$-$$5.17\pm0.46$ &  3 &~$-$$4.94\pm0.46$ &     & ~~$-$4.71~ \\
\ion{Ca}{i}   & ~$-$$5.17\pm0.02$ &  5 &~$-$$4.80\pm0.04$ & ~$-$5.2 & ~~$-$5.68~ \\
\ion{Ca}{ii}  & ~$-$$4.67\pm0.17$ &  5 &~$-$$4.55\pm0.17$ & ~$-$5.2 & ~~$-$5.68~ \\
\ion{Sc}{ii}  & ~$-$9.52          &  1 &~$-$ 9.36        	  & ~$-$9.6 & ~~$-$8.87~ \\
\ion{Ti}{i}   & ~$-$$6.46\pm0.09$ & 13 &~$-$$6.15\pm0.09$ & ~$-$6.5 & ~~$-$7.02~ \\
\ion{Ti}{ii}  & ~$-$$6.49\pm0.16$ & 16 &~$-$$6.36\pm0.16$ & ~$-$6.5 & ~~$-$7.02~ \\
\multicolumn{5}{l}{\ion{V}{i}}  \\
\ion{Cr}{i}   & ~$-$$4.85\pm0.16$ & 52 &~$-$$4.58\pm0.15$ & ~$-$5.0 & ~~$-$6.37~ \\
\ion{Cr}{ii}  & ~$-$$4.70\pm0.21$ & 48 &~$-$$4.65\pm0.21$ & ~$-$5.0 & ~~$-$6.37~ \\
\ion{Mn}{i}   & ~$-$$5.96\pm0.11$ &  9 &~$-$$5.68\pm0.12$ & ~$-$6.0 & ~~$-$6.65~ \\
\ion{Mn}{ii}  & ~$-$$5.66\pm0.38$ & 14 &~$-$$5.63\pm0.40$ & ~$-$6.0 & ~~$-$6.65~ \\
\ion{Fe}{i}   & ~$-$$3.76\pm0.22$ &100 &~$-$$3.48\pm0.21$ & ~$-$4.0 & ~~$-$4.54~ \\
\ion{Fe}{ii}  & ~$-$$3.52\pm0.33$ & 83 &~$-$$3.53\pm0.26$ & ~$-$4.0 & ~~$-$4.54~ \\
\ion{Co}{i}   & ~$-$$6.19\pm0.28$ &  3 &~$-$$5.90\pm0.30$ & ~$-$6.5 & ~~$-$7.12~ \\
\ion{Co}{ii}  & ~$-$6.50          &  1 &~$-$6.50	  & ~$-$6.5 & ~~$-$7.12~ \\
\ion{Ni}{i}   & ~$-$$5.68\pm0.22$ & 28 &~$-$$5.41\pm0.22$ & ~$-$5.7 & ~~$-$5.79~ \\
\ion{Ni}{ii}  & ~$-$$5.31\pm0.12$ &  2 &~$-$$5.31\pm0.14$ & ~$-$5.7 & ~~$-$5.79~ \\
\ion{Zn}{i}   & ~$-$$7.74\pm0.04$ &  2 &~$-$$7.46\pm0.04$ &     & ~~$-$7.44~ \\
\ion{Sr}{ii}  & ~$-$ 8.5          &  2 &~$-$8.0	  & ~$-$8.5 & ~~$-$9.07~ \\
\ion{Y}{ii}  & ~$-$$9.95\pm0.28$ &  5 &~$-$$9.74\pm0.29$ & ~$-$9.9 & ~~$-$9.80~ \\
\ion{Zr}{ii}  & ~$-$ 8.66         &  1 &~$-$ 8.52	  & ~$-$9.0 & ~~$-$9.44~ \\
\ion{Ba}{ii}  & ~$-$$9.02\pm0.28$ &  3 &~$-$$8.60\pm0.31$ & ~$-$8.9 & ~~$-$9.83~ \\
\ion{Ce}{ii}  & $-$10.26          &  1 &~$-$9.97	  &	    & ~$-$10.46~ \\
\ion{Pr}{ii}  & $<$$-$10.5          &  1 &$<$$-$10.5          & ~$-$9.5 & ~$-$11.33~ \\
\ion{Pr}{iii} & $<$$-$10.5          &  1 &$<$$-$10.2	  &	    & ~$-$11.33~ \\
\ion{Nd}{ii}  & ~$-$$9.48\pm0.27$ &  3 &~$-$$9.12\pm0.28$ & ~$-$9.5 & ~$-$10.54~ \\
\ion{Nd}{iii} & $-$$10.05\pm0.10$ &  2 &~$-$$9.95\pm0.14$ &     & ~$-$10.54~ \\
\ion{Eu}{ii}  & $-$10.95          &  1 &$-$10.67	  & $-$11.0 & ~$-$11.53~ \\
\hline
  \teff &\multicolumn{2}{c}{8400}   & 8700  &    8500 &   5777    \\
  \lgg  &\multicolumn{2}{c}{3.50}   &  3.40 &    3.30 &   4.44    \\
\hline
\end{tabular}
\end{footnotesize}
\end{table}