\begin{table}%t4 \caption{\label{lineflux}Measured line fluxes for HD~163296 with $1\sigma$ errors.} \small%\centerline { \begin{tabular}{llrrrrrr} \hline \hline Line ID &$\lambda$ (theory)& \multicolumn{2}{c}{RGS1} & \multicolumn{2}{c}{RGS2} & Flux & unabs. intensity \\ & [\AA] & $\lambda$ (fit)[\AA]& [counts] &$\lambda$ (fit) [\AA]&[counts] & [$10^{-6}$~cts~cm$^{-2}$~s$^{-1}$]& [$10^{27}$~erg~s$^{-1}$] \\ \hline \ion{Ne}{x} Ly~$\alpha$ &12.14 & n.a. & n.a. &$12.14\pm0.01$ &$ 38\pm 9$ &$5.1 \pm1.2 $&$ 17.7 \pm 6.2 $\\ \ion{Ne}{ix} $r^a$ &13.46 & n.a. & n.a. &$13.45\pm0.01$ &$32 \pm 9 $ &$ 4.4\pm1.2 $&$ 14.5 \pm 5.7 $\\ \ion{Ne}{ix} $i^a$ &13.56 & n.a. & n.a. &$13.55\pm0.01$ &$21\pm 9 $ &$ 2.9\pm1.2 $&$ 9.6 \pm 4.8 $\\ \ion{Ne}{ix} $f$ &13.70 & n.a. & n.a. &$13.69\pm0.01$ &$22 \pm 8 $ &$ 3.0\pm1.1 $&$ 9.9 \pm 4.6 $\\ \ion{O}{viii} Ly~$\alpha$&18.97 &$18.98\pm0.01$ & $74 \pm 10 $ &$18.98\pm0.01$ &$117\pm13$ &$18.7\pm2.2 $&$ 54.6 \pm 20.4 $\\ \ion{O}{vii} $r$ &21.6 &$21.57\pm0.01$ & $42.7 \pm 7.8$ & n.a. & n.a. &$14.6\pm 2.7$&$ 45.2 \pm 21.5 $\\ \ion{O}{vii} $i$ &21.8 &$21.77\pm0.01$ & $ 7.8\pm 4.4$ & n.a. & n.a. &$ 3.2\pm1.8 $&$ 10.0 \pm 7.2 $\\ \ion{O}{vii} $f$ &22.1 &$22.07\pm0.01$ & $46.2 \pm 8.1$ & n.a. & n.a. &$14.6\pm2.6 $&$ 46.0 \pm 22.6 $\\ \ion{N}{vii} Ly~$\alpha$ &24.78 & n.a. & n.a.$^b $ &$24.78\pm0.01$ &$14\pm 6$ &$3.3\pm 1.4 $&$ 8.0 \pm 4.6 $\\ \ion{C}{vi} Ly~$\alpha$ &33.70 & n.a. & n.a. &$33.70\pm0.01$ &$ 50\pm 9$ &$20 \pm3.6$&$ 73.0 \pm 56.6 $\\ \ion{Fe}{xvii} &15.01 &$15.01\pm0.01$ & $50 \pm 9 $ &$15.03\pm0.01$ &$101\pm13$ &$11.5\pm1.7 $&$ 35.5 \pm 11.6 $\\ \ion{Fe}{xvii} &15.26 & n.a. & n.a.$^b $ &$15.28\pm0.01$ &$68\pm11$ &$ 8.7\pm1.4 $&$ 26.8 \pm 9.0 $\\ \ion{Fe}{xvii} &16.78 &$16.79\pm0.01$ & $26 \pm 7 $ &$16.78\pm0.01$ &$59\pm11$ &$6.6 \pm1.3 $&$ 20.0 \pm 7.6 $\\ \ion{Fe}{xvii} &17.05$^d$ & n.a. & n.a. &$17.05\pm0.01^c$&$53\pm14$ &$7.4 \pm1.9 $&$ 22.4 \pm 9.3 $\\ \ion{Fe}{xvii} &17.10$^d$ & n.a. & n.a. &$17.10\pm0.01^c$&$59\pm14$ &$8.2 \pm1.9 $&$ 24.9 \pm 10.0 $\\ \hline \end{tabular}} \medskip $^a$ Line blended (see text); $^b$~region contains empty bins; $^c$~lines are not resolved, but two components are necessary to reproduce the line width, for the fit we fix the difference in~$\lambda$. \end{table}