Table 2: Absorption lines in NGC 7469.
Feature Comp $\lambda_{{\rm vac}}$ $W^{{\rm a}}_\lambda$ $N_{{\rm ion}}$ $\Delta v^{{\rm b}}$ FWHM $f_{\rm c}$
  # (Å) (Å) $\rm ( 10^{12}~cm^{-2} )$ ( $\rm km~s^{-1}$) ( $\rm km~s^{-1}$)  
Ly$\beta $ 2a 1025.72 <0.05 $\phantom{00}1.5 \pm 3.4$ $-2016 \pm 12$ $29 \pm 1$ $0.93 \pm 0.03$
Ly$\beta $ 2a 1025.72   $\phantom{00}3.2 \pm 7.3$ $-1975 \pm 4$ $29 \pm 1$ $0.93 \pm 0.03$
Ly$\beta $ 2a 1025.72   $\phantom{0}12.9 \pm 29.5$ $-1898 \pm 1$ $29 \pm 1$ $0.93 \pm 0.03$
Ly$\beta $ 2a 1025.72   $\phantom{00}4.0 \pm 9.1$ $-1840 \pm 3$ $29 \pm 1$ $0.93 \pm 0.03$
Ly$\beta $ 1a 1025.72 <0.03 $\phantom{00}8.2 \pm 4.3$ $\phantom{0}$ $-627 \pm 5$ $25 \pm 2$ $0.53 \pm 0.05$
Ly$\beta $ 1b 1025.72   $\phantom{0}53.2 \pm 28.1$ $\phantom{0}$ $-569 \pm 4$ $25 \pm 2$ $0.53 \pm 0.05$
Ly$\beta $ 1c 1025.72   $\phantom{0}15.3 \pm 8.1$ $\phantom{0}$ $-506 \pm \phantom{0}3$ $25 \pm 2$ $0.53 \pm 0.05$
Ly$\beta $ 1d 1025.72   $\phantom{00}3.9 \pm 2.1$ $\phantom{0}$ $-431 \pm 5$ $25 \pm 2$ $0.53 \pm 0.05$
OVI 2a 1031.93 $0.48 \pm 0.02$ $\phantom{0}36.1 \pm 16.2$ $-2015 \pm 12$ $29 \pm 1$ $0.93 \pm 0.03$
OVI 2b 1031.93   $121.2 \pm 16.3$ $-1973 \pm 4$ $29 \pm 1$ $0.93 \pm 0.03$
OVI 2c 1031.93   $494.0 \pm 51.4$ $-1898 \pm 1$ $29 \pm 1$ $0.93 \pm 0.03$
OVI 2d 1031.93   $154.4 \pm 16.9$ $-1838 \pm \phantom{0}3$ $29 \pm 1$ $0.93 \pm 0.03$
OVI 1a 1031.93 $0.23 \pm 0.02$ $\phantom{0}76.1 \pm 25.3$ $\phantom{0}$ $-626 \pm 5$ $25 \pm 2$ $0.53 \pm 0.05$
OVI 1b 1031.93   $494.7^{+1.5\times10^6}_{-167.2}$ $\phantom{0}$ $-569 \pm 4$ $25 \pm 2$ $0.53 \pm 0.05$
OVI 1c 1031.93   $142.3 \pm 28.2$ $\phantom{0}$ $-506 \pm 3$ $25 \pm 2$ $0.53 \pm 0.05$
OVI 1d 1031.93   $\phantom{0}58.7 \pm 15.0$ $\phantom{0}$ $-432 \pm 5$ $25 \pm 2$ $0.53 \pm 0.05$
$^{\rm a}$ 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. (1991).

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