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Table 3:

The observed line photon fluxes.
ion     $\lambda_0$     $\lambda_{\rm obs}$ ${\it FWHM}$Observed flux
      [Å]    [Å][Å] 
XV    5.064    5.061(.035)  --  16.6(11.8)
Si  XIV    6.182    6.200(.018)  --   3.9(  2.3)
Si  XIII    6.648    6.656(.023)  --   3.4(  2.2)
Si  XIII    6.688    6.698(.041)  --   2.4(  2.2)
Si  XIII    6.740    6.766(.027)  --   2.7(  2.2)
Mg  XII    8.423    8.474(  --)  --   4.2(  --)
Mg  XI    9.169    9.168(.014)  --   6.4(  3.4)
Mg  XI    9.315    9.318(.018)  --   12.0(  6.2)
Ne  X    9.708    9.689(.032)  --   7.6(  4.8)
Ne  X  10.239  10.225(.011)  --   11.5(  4.5)
Ne  IX  10.765  10.759(.012)  --   7.7(  3.7)
Ne  IX  11.001  10.994(.008)  --   12.6(  4.2)
Ne  IX  11.544  11.543(.006)  --   22.0(  4.8)
Ne  X  12.134  12.135(.003)  0.017(.014)   89.6(  7.8)
Ne  IX  13.447  13.452(.002)  0.024(.007)  215.0(11.0)
Ne  IX  13.553  13.555(.002)   $\mathrel{\hbox{\rlap{\hbox{\lower4pt\hbox{$\sim$ }}}\hbox{$<$ }}}$0.020  129.0(  9.0)
Ne  IX  13.700  13.699(.003)  0.041(.011)  81.2(  7.7)
Ni  XIX  14.040  14.058(.028)   $\mathrel{\hbox{\rlap{\hbox{\lower4pt\hbox{$\sim$ }}}\hbox{$<$ }}}$0.093   5.6(  4.4)
Ni  XVIII  14.081   
Ni  XVIII  14.370  14.381(.033)   $\mathrel{\hbox{\rlap{\hbox{\lower4pt\hbox{$\sim$ }}}\hbox{$<$ }}}$0.120  10.2(  6.6)
VIII  14.821  14.824(.014)  --   6.9(  2.8)
Fe  XVII  15.013  15.031(.008)  0.070(.022)  35.9(  6.5)
VIII  15.176  15.174(.020)   fix   9.0(  4.1)
Fe  XVII  15.260  15.258(.008)   $\mathrel{\hbox{\rlap{\hbox{\lower4pt\hbox{$\sim$ }}}\hbox{$<$ }}}$0.056   17.4(  5.1)
VIII  16.006  16.010(.006)   $\mathrel{\hbox{\rlap{\hbox{\lower4pt\hbox{$\sim$ }}}\hbox{$<$ }}}$0.053   29.7(  5.4)
Fe  XVII  16.775  16.790(.006)   $\mathrel{\hbox{\rlap{\hbox{\lower4pt\hbox{$\sim$ }}}\hbox{$<$ }}}$0.041   20.4(  4.6)
Fe  XVII  17.051  17.056(.060)  fix at 0   22.9(12.6)
Fe  XVII  17.100  17.098(.039)  fix at 0   15.1(10.3)
VII  18.627  18.634(.018)  0.066(.060)  17.5(  6.7)
VIII  18.969  18.972(.002)  0.027(.006)  229.0(12.0)
VII  20.910  20.917(.019)  0.069   20.7(  8.6)
VII  21.602  21.610(.003)   $\mathrel{\hbox{\rlap{\hbox{\lower4pt\hbox{$\sim$ }}}\hbox{$<$ }}}$0.043  119.0(12.0)
VII  21.804  21.807(.003)  0.030(.011)  103.0(11.0)
VII  22.101  22.105(.015)  0.035   15.3(  6.3)
VII  24.781  24.794(.005)  0.046(.018)   81.2(11.3)
VI  28.787  28.799(fix)  0.138(.103)   31.2(12.0)
VI  29.084  29.096(fix)    $\mathrel{\hbox{\rlap{\hbox{\lower4pt\hbox{$\sim$ }}}\hbox{$<$ }}}$0.146   27.1(10.0)
VI  29.536  29.548(fix)  --   6.0(  6.3)
VI  33.736  33.743(.005)  --   59.3(11.0)
Notes: Statistical 1$\sigma$ errors are in parentheses. $\lambda_0$ is the theoretical wavelength from Kelly (1987).
$\lambda_{\rm obs}$ is the observed wavelength. The flux is in units 10-6 photons cm-2 s-1.

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