\begin{table}%t2
\caption{Absorption lines in NGC~7469.\label{tbl-alines}}
%\centerline
{
\begin{tabular}{lccccccc}
\hline
\hline
Feature & Comp & $\lambda_{{\rm vac}}$ & $W^{{\rm a}}_\lambda$ &
$N_{{\rm ion}}$ & $\Delta v^{{\rm b}}$ & $FWHM$ & $f_{\rm c}$ \\
     & \#    & (\AA)  & (\AA) & $\rm ( 10^{12}~cm^{-2} )$ &
($\rm km~s^{-1}$) & ($\rm km~s^{-1}$) &  \\
\hline
Ly$\beta$ & 2a & 1025.72 & $<$0.05 & $\phantom{00}1.5 \pm 
%\phantom{00}
3.4$ & $-2016
\pm 12$ & $29 \pm 1$ & $0.93 \pm 0.03$ \\
Ly$\beta$ & 2a & 1025.72 &  & $\phantom{00}3.2 \pm 
%\phantom{00}
7.3$ & $-1975
\pm 
%\phantom{0}
4$ & $29 \pm 1$ & $0.93 \pm 0.03$ \\
Ly$\beta$ & 2a & 1025.72 &  & $\phantom{0}12.9 \pm 
%\phantom{0}
29.5$ & $-1898
\pm 
%\phantom{0}
1$ & $29 \pm 1$ & $0.93 \pm 0.03$ \\
Ly$\beta$ & 2a & 1025.72 &  & $\phantom{00}4.0 \pm 
%\phantom{00}
9.1$ & $-1840
\pm 
%\phantom{0}
3$ & $29 \pm 1$ & $0.93 \pm 0.03$ \\
Ly$\beta$ & 1a & 1025.72 & $<$0.03 & $\phantom{00}8.2 \pm 
%\phantom{00}
4.3$ &
$\phantom{0}$$-627 \pm 
%\phantom{0}
5$ & $25 \pm 2$ & $0.53 \pm 0.05$ \\
Ly$\beta$ & 1b & 1025.72 &  & $\phantom{0}53.2 \pm 
%\phantom{0}
28.1$ &
$\phantom{0}$$-569 \pm 
%\phantom{0}
4$ & $25 \pm 2$ & $0.53 \pm 0.05$ \\
Ly$\beta$ & 1c & 1025.72 &  & $\phantom{0}15.3 \pm 
%\phantom{00}
8.1$ &
$\phantom{0}$$-506 \pm \phantom{0}3$ & $25 \pm 2$ & $0.53 \pm 0.05$ \\
Ly$\beta$ & 1d & 1025.72 &  & 
$\phantom{00}3.9 \pm 
%\phantom{00}
2.1$ &
$\phantom{0}$$-431 \pm 
%\phantom{0}
5$ & $25 \pm 2$ & $0.53 \pm 0.05$ \\
OVI     & 2a & 1031.93 & $0.48 \pm 0.02$ & $\phantom{0}36.1 \pm 
%\phantom{0}
16.2$ & $-2015
\pm 12$ & $29 \pm 1$ & $0.93 \pm 0.03$ \\
OVI     & 2b & 1031.93 &  & $121.2 \pm 
%\phantom{0}
16.3$ & $-1973 \pm
%\phantom{0}
4$ & $29 \pm 1$ & $0.93 \pm 0.03$ \\
OVI     & 2c & 1031.93 &  & $494.0 \pm 
%\phantom{0}
51.4$ & $-1898 \pm
%\phantom{0}
1$ & $29 \pm 1$ & $0.93 \pm 0.03$ \\
OVI     & 2d & 1031.93 &  & $154.4 \pm 
%\phantom{0}
16.9$ & $-1838 \pm
\phantom{0}3$ & $29 \pm 1$ & $0.93 \pm 0.03$ \\
OVI     & 1a & 1031.93 & $0.23 \pm 0.02$ & $\phantom{0}76.1 \pm 
%\phantom{0}
25.3$ &
$\phantom{0}$$-626 \pm 
%\phantom{0}
5$ & $25 \pm 2$ & $0.53 \pm 0.05$ \\
OVI     & 1b & 1031.93 &  & $494.7^{+1.5\times10^6}_{-167.2}$ &
$\phantom{0}$$-569 \pm 
%\phantom{0}
4$ & $25 \pm 2$ & $0.53 \pm 0.05$ \\
OVI     & 1c & 1031.93 &  & $142.3 \pm 
%\phantom{0}
28.2$ & $\phantom{0}$$-506
\pm 
%\phantom{0}
3$ & $25 \pm 2$ & $0.53 \pm 0.05$ \\
OVI     & 1d & 1031.93 &  & $\phantom{0}58.7 \pm 
%\phantom{0}
15.0$ &
$\phantom{0}$$-432 \pm 
%\phantom{0}
5$ & $25 \pm 2$ & $0.53 \pm 0.05$ \\
\hline
\end{tabular}}
\medskip
$^{{\rm a}}$ Equivalent widths are integrated over all components of each spectral feature.
Upper limits are $2 \sigma$.  \\
$^{{\rm b}}$ Velocity is relative to a systemic redshift of
$cz = 4916~\rm km~s^{-1}$ de~Vaucouleurs et~al. (\cite{RC3}).
\end{table}