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Table 6

The ten strongest modelled lines around the 16 Å blend, using the fitted model to the sources.

Ion Wavelength Emission
Å  × 1047      photons   s-1

NGC 5044
Fe xix 15.358 11.7
Fe xix 15.364 16.1
Fe xviii 15.831 24.3
Fe xviii 16.165 26.1
Fe xix 16.282 26.4
Fe xviii 15.628 38.9
Fe xviii 16.002 41.0
O viii 16.003 62.1
Fe xix 16.106 87.2
Fe xviii 16.078 120.9

NGC 5813
Fe xix 16.282 7.7
Fe xviii 15,874 7.9
Fe xvii 15.456 9.9
Fe xviii 15.831 16.9
Fe xviii 16.165 17.3
O viii 16.003 18.0
Fe xix 16.106 25.3
Fe xviii 15.628 26.9
Fe xviii 16.002 28.6
Fe xviii 16.078 84.3

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