\begin{table}%t2 %\centering \par \caption{\label{tab:abund}Abundances in the atmosphere of \hd\ with the error estimates based on~$n$ measured lines. Abundances derived in our study are compared with those reported by \citet{KRW96} and BNC08. The solar abundances are from \citet{asplund}.} \small \begin{tabular}{lcclrlrc} \hline \hline Ion & \citet{KRW96} & BNC08 &\multicolumn{4}{c}{This paper} &Sun \\ &$\log (El/N_{\rm tot})$ &$\log (El/N_{\rm tot})$ & $\log (El/N_{\rm tot})$ & $n$ & with HFS & $n$ &$\log (El/N_{\rm tot})$\\ \hline \ion{C}{i}&--4.00 & --3.60 &$-$3.92$\pm$0.20 & 14 && &$-$3.65\\ \ion{N}{i}& --4.40:&&$-$4.53$\pm$0.07 & 4 &&&$-$4.26\\ \ion{O}{i}& --3.80 & --3.53 &$-3.58\pm0.22$ & 5 &&&$-$3.38\\ \ion{Na}{i}& --5.90&--6.08 &$-5.91\pm 0.06$ & 2 && &$-$5.87 \\ \ion{Mg}{i} & & --4.52 & $-4.52\pm 0.15$ & 7 &&&$-$4.51 \\ \ion{Mg}{ii}& --4.46:& &$-$4.36: & 1 &&&$-$4.51\\ \ion{Al}{i} && --5.49 & $-$5.52: & 1 &&&$-$5.67\\ \ion{Si}{i} & --4.20 & --4.67 &$-4.51\pm0.20$ & 15& &&$-$4.53\\ \ion{Si}{ii}& & &$-4.20\pm0.15$ &4 && &$-$4.53\\ \ion{S}{i} & & --4.55 &$-5.01\pm0.19$ & 6 & & & $-$4.90\\ \ion{K}{i} & & &$-$7.22: & 1 & & & $-$6.96\\ \ion{Ca}{i} & --5.15 & --5.54 & $-5.29\pm0.16$ & 13 & &&$-$5.73\\ \ion{Ca}{ii} & & & $-5.09 \pm 0.26$ & 5 & & &$-$5.73 \\ \ion{Sc}{ii} & --9.80 & --9.41 &$-9.39\pm0.19$ & 7 & &&$-$8.99\\ \ion{Ti}{i} & --6.87 & --7.34 & $-$7.33$\pm$0.19 & 3 & & &$-$7.14\\ \ion{Ti}{ii} & --6.87 & --7.31 & $-7.23\pm0.17$ & 11 & & &$-$7.14\\ \ion{V}{i} & --7.65 & --7.44 & ~~$-$7.48: & 1 & & &$-$8.04\\ \ion{V}{ii} & & &$-7.41\pm0.24$ & 8 & & &$-$8.04 \\ \ion{Cr}{i} & --5.55 & --5.92 & $-5.70\pm0.21$ & 23 & & &$-$6.40\\ \ion{Cr}{ii} & --5.55 & --5.91 & $-5.46\pm0.35$ & 21 & & &$-$6.40\\ \ion{Mn}{i} & --6.00 & --5.97 & $-6.14\pm0.20$ & 19 &~~$-6.41\pm0.21$ & 14 &$-$6.65\\ \ion{Mn}{ii} & --6.00 & --5.97 & $-5.98\pm0.14$ & 7 &~~$-6.20\pm0.10$ & 7 &$-$6.65\\ \ion{Fe}{i} & --4.50 & --4.71 & $-4.61\pm0.17$ &116 & & &$-$4.59\\ \ion{Fe}{ii} & --4.50 & --4.62 & $-4.39\pm0.17$ & 30 & & &$-$4.59 \\ \ion{Co}{i} & --5.50 & --5.92 & $-5.93\pm0.26$ & 27 &$-6.35\pm0.36$ & 8 &$-$7.12\\ \ion{Co}{ii} & --5.50 & &$-5.63\pm0.31$ & 5 & & &$-$7.12\\ \ion{Ni}{i} & --6.15 & --6.39 & $-6.51\pm0.26$ & 8 & & &$-$5.81\\ \ion{Se}{i} & & & $-$8.40: & 1 & & &$-$8.71 \\ \ion{Sr}{i} & & & $-7.27\pm0.13$ & 5 & & &$-$9.12\\ \ion{Sr}{ii} & --7.25 & &$-8.70\pm0.50$ &2&&&$-$9.12\\ \ion{Y}{i} & &&$-$7.90: & 1 & & &$-$9.83\\ \ion{Y}{ii} & --8.50 & --8.95 &$-8.65\pm0.17$ & 11 & & &$-$9.83\\ \ion{Zr}{ii} & --9.00 & --9.08 &$-9.34\pm0.12$ & 3 & & &$-$9.45\\ \ion{Ba}{ii} &--10.30 &--10.57 & $-10.17\pm0.13$ & 2 & & &$-$9.87\\ \ion{La}{ii} &--10.32:& & $-10.21\pm0.17$ & 4 & &&$-$10.91\\ \ion{Ce}{ii} & --9.40 & --9.72 & $-9.47\pm0.18$ & 11 & & &$-$10.46\\ \ion{Ce}{iii} & & & $-$7.63: & 1 & & &$-$10.46\\ \ion{Pr}{ii} &--10.40 & &$-$10.16: &1 & &&$-$11.33\\ \ion{Pr}{iii} & & & $-8.49\pm0.23$ & 11 & &&$-$11.33\\ \ion{Nd}{ii} & --9.30 & --9.56 & $-9.50\pm0.19$ & 19 & & &$-$10.59\\ \ion{Nd}{iii} & & --8.53 &$-7.83\pm0.26$ & 22 & & &$-$10.59\\ \ion{Sm}{ii} & --9.50 & & $-9.66\pm0.24$ & 21 & &&$-$11.03\\ \ion{Eu}{ii} & --9.40 & --9.94 &$-9.67\pm0.07$ & 5 &$-9.89\pm0.12$& 4 &$-$11.52\\ \ion{Gd}{ii} & --9.45 & & $-9.45\pm0.26$ & 5 & & &$-$10.93\\ \ion{Tb}{ii} & & & $-10.2 \pm 0.3$: &2& &&$-$11.76\\ \ion{Tb}{iii} & & & $-8.36\pm0.28$ & 6 & & &$-$11.76\\ \ion{Dy}{ii} &--10.00 & & $-9.54\pm0.27$ & 4 & & &$-$10.90\\ \ion{Dy}{iii} & & & $-7.28\pm0.33$ & 6 & & &$-$10.90 \\ \ion{Ho}{ii} & & & $-$9.20: &1 &$-10.5\pm0.2$&4 &$-$11.53\\ \ion{Er}{ii} & & &$-9.90\pm0.29$ & 5 &&&$-$11.11\\ \ion{Er}{iii} & & & $-7.71\pm0.11$ & 2 & & &$-$11.11\\ \ion{Tm}{iii} & & & $-$7.85: &1 & & &$-$12.04\\ $\teff$ (K) & $7900\pm200$ & $7420\pm170$ &\multicolumn{4}{c}{$7500\pm130$} & 5777\\ $\logg$ & $4.20\pm0.15$ & $4.09\pm0.08$ &\multicolumn{4}{c}{$4.10\pm0.15$} & 4.44 \\ \vt\ (\kms) & $1.50\pm0.15$ & $1.60\pm0.15$ &\multicolumn{4}{c}{$1.20\pm0.20$} & \\ \hline \end{tabular} \end{table}