Table 1: Emission lines in NGC 7469.
Line $\rm\lambda_{vac}$ Flux$^{\rm a}$ Velocity$^{\rm b}$ FWHM
  (Å)   $\rm ( km~s^{-1} )$ $\rm ( km~s^{-1} )$
C III 977.02 $\phantom{0}9.5 \pm 2.1$ $\phantom{-}271 \pm 160$ $1599 \pm 210$
N III 991.58 $\phantom{0}5.3 \pm 1.3$ $\phantom{-0}95 \pm 158$ $1599 \pm 210$
Unknown 1014.86 $\phantom{0}6.5 \pm 1.1$ $\phantom{-00}0 \pm 160$ $1939 \pm 518$
O VI broad 1031.93 $85.8 \pm 4.3$ $\phantom{-}323 \pm \phantom{0}37$ $4901 \pm 146$
O VI broad 1037.62 $42.9 \pm 2.2$ $\phantom{-}323 \pm \phantom{0}37$ $4901 \pm 146$
O VI narrow 1031.93 $23.5 \pm 2.9$ $-163 \pm \phantom{0}55$ $1061 \pm \phantom{0}82$
O VI narrow 1037.62 $11.8 \pm 1.5$ $-163 \pm \phantom{0}55$ $1061 \pm \phantom{0}82$
S IV 1062.66 $15.5 \pm 1.3$ $\phantom{-}194 \pm 142$ $7637 \pm 251$
S IV 1072.97 $15.5 \pm 1.3$ $\phantom{-}194 \pm 142$ $7637 \pm 251$
He  II 1085.15 $\phantom{0}3.2 \pm 0.3$ $\phantom{0}$ $-47 \pm 161$ $2575 \pm 210$
$^{\rm a}$ Observed flux in units of $\rm 10^{-14}~erg~cm^{-2}~s^{-1}$.
$^{\rm b}$ Velocity is relative to a systemic redshift of $cz = 4916~\rm km~s^{-1}$ de Vaucouleurs et al. (1991).

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