\begin{table}%t3 \caption{\label{lineflux}The observed line photon fluxes.} %\centerline {\begin{tabular}{l@{\ }l@{\ }l@{\ }c@{\ }r@{\ }} \hline \hline ion &~~~~ $\lambda_0$&~~~~ $\lambda_{\rm obs}$&${\it FWHM}$&Observed flux\\ &~~~~ [\AA] &~~~~[\AA] &[\AA]& \\ \hline S~{\sc xv} & ~~~~5.064 &~~~~5.061(.035) &~~--- &~~16.6(11.8)\\ Si~{\sc xiv} & ~~~~6.182 &~~~~6.200(.018) &~~--- &~~ 3.9(~~2.3)\\ Si~{\sc xiii} & ~~~~6.648 &~~~~6.656(.023) &~~--- &~~ 3.4(~~2.2)\\ Si~{\sc xiii} & ~~~~6.688 &~~~~6.698(.041) &~~--- &~~ 2.4(~~2.2)\\ Si~{\sc xiii} & ~~~~6.740 &~~~~6.766(.027) &~~--- &~~ 2.7(~~2.2)\\ Mg~{\sc xii} & ~~~~8.423 &~~~~8.474(~~----)&~~--- &~~ 4.2(~~----)\\ Mg~{\sc xi} & ~~~~9.169 &~~~~9.168(.014) &~~--- &~~ 6.4(~~3.4)\\ Mg~{\sc xi} & ~~~~9.315 &~~~~9.318(.018) &~~--- &~~ 12.0(~~6.2)\\ Ne~{\sc x} & ~~~~9.708 &~~~~9.689(.032) &~~--- &~~ 7.6(~~4.8)\\ Ne~{\sc x} &~~10.239 &~~10.225(.011) &~~--- &~~ 11.5(~~4.5)\\ Ne~{\sc ix} &~~10.765 &~~10.759(.012) &~~--- &~~ 7.7(~~3.7)\\ Ne~{\sc ix} &~~11.001 &~~10.994(.008) &~~--- &~~ 12.6(~~4.2)\\ Ne~{\sc ix} &~~11.544 &~~11.543(.006) &~~--- &~~ 22.0(~~4.8)\\ Ne~{\sc x} &~~12.134 &~~12.135(.003) &~~0.017(.014) &~~ 89.6(~~7.8)\\ Ne~{\sc ix} &~~13.447 &~~13.452(.002) &~~0.024(.007) &~~215.0(11.0)\\ Ne~{\sc ix} &~~13.553 &~~13.555(.002) &~~$\la$0.020 &~~129.0(~~9.0)\\ Ne~{\sc ix} &~~13.700 &~~13.699(.003) &~~0.041(.011) &~~81.2(~~7.7)\\ Ni~{\sc xix} &~~14.040 &~~14.058(.028)&~~$\la$0.093 &~~ 5.6(~~4.4)\\ Ni~{\sc xviii} &~~14.081 & & & \\ Ni~{\sc xviii} &~~14.370 &~~14.381(.033)&~~$\la$0.120 &~~10.2(~~6.6)\\ O~{\sc viii} &~~14.821 &~~14.824(.014) &~~--- &~~ 6.9(~~2.8)\\ Fe~{\sc xvii} &~~15.013 &~~15.031(.008) &~~0.070(.022) &~~35.9(~~6.5)\\ O~{\sc viii} &~~15.176 &~~15.174(.020) &~~ fix &~~ 9.0(~~4.1)\\ Fe~{\sc xvii} &~~15.260 &~~15.258(.008) &~~$\la$0.056 &~~ 17.4(~~5.1)\\ O~{\sc viii} &~~16.006 &~~16.010(.006) &~~$\la$0.053 &~~ 29.7(~~5.4)\\ Fe~{\sc xvii} &~~16.775 &~~16.790(.006) &~~$\la$0.041 &~~ 20.4(~~4.6) \\ Fe~{\sc xvii} &~~17.051 &~~17.056(.060) &~~fix at 0 &~~ 22.9(12.6)\\ Fe~{\sc xvii} &~~17.100 &~~17.098(.039) &~~fix at 0 &~~ 15.1(10.3)\\ O~{\sc vii} &~~18.627 &~~18.634(.018) &~~0.066(.060) &~~17.5(~~6.7)\\ O~{\sc viii} &~~18.969 &~~18.972(.002) &~~0.027(.006) &~~229.0(12.0)\\ N~{\sc vii} &~~20.910 &~~20.917(.019) &~~0.069 &~~ 20.7(~~8.6)\\ O~{\sc vii} &~~21.602 &~~21.610(.003) &~~$\la$0.043 &~~119.0(12.0)\\ O~{\sc vii} &~~21.804 &~~21.807(.003) &~~0.030(.011)&~~103.0(11.0) \\ O~{\sc vii} &~~22.101 &~~22.105(.015) &~~0.035 &~~ 15.3(~~6.3)\\ N~{\sc vii} &~~24.781 &~~24.794(.005) &~~0.046(.018) &~~ 81.2(11.3) \\ N~{\sc vi} &~~28.787 &~~28.799(fix) &~~0.138(.103) ~~& 31.2(12.0) \\ N~{\sc vi} &~~29.084 &~~29.096(fix) &~~~$\la$0.146 &~~ 27.1(10.0) \\ N~{\sc vi} &~~29.536 &~~29.548(fix) &~~--- &~~ 6.0(~~6.3)\\ C~{\sc vi} &~~33.736 &~~33.743(.005) &~~--- &~~ 59.3(11.0) \\ \hline \end{tabular}} \smallskip \par Notes: Statistical 1$\sigma$ errors are in parentheses. $\lambda_0$ is the theoretical wavelength from Kelly (\cite{Kelly1987}). $\lambda_{\rm obs}$ is the observed wavelength. The flux is in units 10$^{-6}$~photons~cm$^{-2}$~s$^{-1}$. \end{table}