\begin{table}%t3
       \caption{\label{abs_lines}The rest wavelengths ($\lambda_{\rm rest}$), observed wavelengths ($\lambda_{\rm obs}$), equivalent widths ({\it EW}), blueshifts ($v_{\rm blue}$), fluxes, velocity widths ($v_{\rm broad}$, {\it FWHM}) and range of~log~$\xi$ (log~$\xi_{\rm max}$) where the ion is most abundant of absorption (top section) and emission lines (bottom section) in the RGS spectrum of NGC~7469; rms errors are quoted throughout, except for~log~$\xi_{\rm max}$ where the error bars give the range where the ion has a higher relative abundance than adjacent ionisation states. Blueshifts are not given for lines whose equivalent width is consistent with zero. Also listed are rest wavelengths, blueshifts, fluxes, velocity widths and~log~$\xi_{\rm max}$ for the broad and narrow \ion{O}{vi}~emission lines observed by FUSE (Kriss et~al. \cite{kriss2003}).}
          $$
\begin{array}{p{0.9in}p{0.6in}p{0.9in}p{0.7in}p{0.9in}p{0.7in}p{0.7in}p{0.8in}}
 \hline\hline
 \noalign{\smallskip}
Transition & $\lambda_{\rm rest}^{\rm {a}}$ & $\lambda_{\rm obs}^{\rm {b}}$ & $EW^{\rm {c}}$ &$ v_{\rm blue}^{\rm {d}}$ & Flux$^{\rm {e}}$ &$ v_{\rm broad}^{\rm {f}}$ & log $\xi_{\rm max}^{\rm {g}}$ \\
 \noalign{\smallskip}
 \hline
 \noalign{\smallskip}
\ion{O}{viii} Ly$\alpha$ & 18.969 & 18.89 $\pm$ 0.05 & 10 $\pm$ 10    & &               & & 1.8 $\pm$ 0.3 \\
\ion{O}{viii} Ly$\beta$  & 16.006 & 15.98 $\pm$ 0.02 & 20 $\pm$ 10    & $-$600 $\pm$ 500  &               & & 1.8 $\pm$ 0.3 \\
\ion{O}{viii} Ly$\gamma$ & 15.176 & 15.12 $\pm$ 0.05 & 10 $\pm$ 10    & &               & & 1.8 $\pm$ 0.3 \\
\ion{O}{vii} 3$-$1 (r)   & 18.629 & 18.57 $\pm$ 0.04 & 10 $\pm$ 10    & &               & & 1.1 $^{\rm +0.4}_{\rm -0.5}$ \\
\ion{O}{v} Be$\alpha$    & 22.334 & 22.25 $\pm$ 0.04 & 20 $\pm$ 20    & &               & & 0$^{\rm +0.4}_{\rm -0.3}$ \\
\ion{O}{iii} C$\alpha$   & 23.058 & 22.99 $\pm$ 0.04 & 70 $\pm$ 20    & $-$800 $\pm$ 500  &               & & $-$1.8 $\pm$ 0.6 \\
\ion{N}{vii} Ly$\alpha$  & 24.781 & 24.72 $\pm$ 0.04 & 10 $\pm$ 10    & &               & & 1.5 $\pm$ 0.3 \\
\ion{N}{iv} Be$\alpha$   & 29.896 & 29.87 $\pm$ 0.03 & 60 $\pm$ 20    & $-$300 $\pm$ 400  &               & & $-$0.6 $\pm$ 0.5 \\
\ion{C}{vi} Ly$\alpha$   & 33.736 & 33.65 $\pm$ 0.03 & 50 $\pm$ 20    & $-$800 $\pm$ 200  &               & & 1.1 $^{\rm +0.4}_{\rm -0.3}$ \\
\ion{C}{vi} Ly$\gamma$   & 26.990 & 26.90 $\pm$ 0.03 & 20 $\pm$ 10    & $-$1000 $\pm$ 300 &               & & 1.1 $^{\rm +0.4}_{\rm -0.3}$ \\
\ion{Ne}{ix} He$\beta$   & 11.547 & 11.48 $\pm$ 0.02 & 50 $\pm$ 20    & $-$1600 $\pm$ 500 &               & & 1.7 $^{\rm +0.3}_{\rm -0.4}$ \\
\ion{Ne}{vii} Be$\alpha$ & 13.814$^{\rm {h}}$ & 13.79 $\pm$ 0.02   & 40 $\pm$ 10 & $-$500 $\pm$ 500 &  & & 0.5 $\pm$ 0.3 \\
 \noalign{\smallskip}
 \hline
 \noalign{\smallskip}
\ion{O}{viii} Ly$\alpha$ & 18.969 & 18.98 $\pm$ 0.05 & $-$20 $\pm$ 10 & 200 $\pm$ 700     & 1.4 $\pm$ 1.0 & 0$^{\rm +3000}_{\rm -0}$    & 1.8 $\pm$ 0.3\\
\ion{O}{vii} (f)         & 22.101 & 22.07 $\pm$ 0.02 & $-$80 $\pm$ 20 & $-$400 $\pm$ 200  & 6.0 $\pm$ 1.7 & 0$^{\rm +700}_{\rm -0}$     & 1.1 $^{\rm +0.4}_{\rm -0.5}$ \\
\ion{O}{vii} (i)         & 21.807 & 21.80 $\pm$ 0.04 & $-$40 $\pm$ 20 & $-$100 $\pm$ 500  & 2.7 $\pm$ 1.6 & 700$^{\rm +2000}_{\rm -700}$ & 1.1 $^{\rm +0.4}_{\rm -0.5}$ \\
\ion{O}{vi}$^{\rm {i, j}}$ & 1031.93 & & & 323 $\pm$ 37    & 4457 $\pm$ 223 & 4901 $\pm$ 146 & 0.5 $^{\rm +0.1}_{\rm -0.2}$ \\
\ion{O}{vi}$^{\rm {i, j}}$ & 1037.62 & & & 323 $\pm$ 37    & 2241 $\pm$ 115 & 4901 $\pm$ 146 & 0.5 $^{\rm +0.1}_{\rm -0.2}$ \\
\ion{O}{vi}$^{\rm {i, k}}$ & 1031.93 & & & $-$163 $\pm$ 55 & 1221 $\pm$ 151 & 1061 $\pm$ 82 & 0.5 $^{\rm +0.1}_{\rm -0.2}$ \\
\ion{O}{vi}$^{\rm {i, k}}$ & 1037.62 & & & $-$163 $\pm$ 55 & 616 $\pm$ 78   & 1061 $\pm$ 82 & 0.5 $^{\rm +0.1}_{\rm -0.2}$ \\
\ion{C}{vi} Ly$\alpha$  & 33.736 & 33.82 $\pm$ 0.03 & $-$90 $\pm$ 30 &  700 $\pm$ 200    & 3.6 $\pm$ 1.3 & 700$^{\rm +800}_{\rm -700}$ & 1.1 $^{\rm +0.4}_{\rm -0.3}$ \\
 \noalign{\smallskip}
 \hline
 \end{array}
          $$
  \end{table}