Table 4: Parameters of the emission lines included with the slab and xabs model fits to the RGS spectrum of NGC 7469: line identification, FWHM in km s-1, velocity shift  $v_{\rm shift}$ in km s-1 and line flux F in 10-6 photons cm-2 s-1.
Line FWHM $v_{\rm shift}$ F
C VI Ly$\alpha $ $\rm0^{+2000}_{-0}$ $\rm -70^{+240}_{-470}$ $30 \pm 10$
N VII Ly$\alpha $ $\rm0^{+11000}_{-0}$ $\rm 1100^{+540}_{-270}$ $9 \pm 7$
O VII f $\rm 1200^{+1000}_{-700}$ $\rm -520 \pm 200$ $70 \pm 10$
O VII i $\rm 2500^{+1500}_{-2500}$ $\rm -760^{+980}_{-720}$ $60 \pm 20$
O VII r $\rm 970^{+1800}_{-970}$ $\rm -110^{+1300}_{-670}$ $40 \pm 10$
O VIII Ly$\alpha $ $\rm 640^{+630}_{-640}$ $\rm -520^{+430}_{-230}$ $\rm 80^{+60}_{-30}$
Ne X Ly$\alpha $ $\rm0^{+1000}_{-0}$ $\rm 300^{+440}_{-230}$ $18 \pm 6$
Fe XVIII $\lambda$17.56 Å $\rm0^{+1900}_{-0}$ $-770 \pm 310$ $15 \pm 6$
Fe XVII $\lambda$17.14 Å $\rm0^{+5400}_{-0}$ $\rm 1700^{+740}_{-300}$ $22 \pm 5$

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