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Table A.1

List of lines of interest

Ion ID Wavelength (Å) EX CEX RR CRR DR CDR ICapella (ph m−2 s−1) UCapella IHR1099 (ph m−2 s−1) UHR1099
Fe XVI 1 40.1517 0.543 0.008 0.041 0.016 0.000 0.385 0.8458 0.0448 0.2479 0.1462
Fe XVI 2 39.8258 0.608 0.002 0.045 0.018 0.000 0.319 0.4057 0.1374 0.1163 0.4795
Fe XVI 3 15.2008 0.000 0.000 0.000 0.000 0.934 0.066 0.4529 0.9431 0.0616 0.5325
Fe XVI 4 15.2442 0.365 0.002 0.000 0.000 0.607 0.025 0.7161 0.0719 0.0962 0.1186
Fe XVI 3 15.2109 0.965 0.002 0.000 0.000 0.021 0.012 1.2664 0.9431 0.1756 0.5325
Fe XVI 3 15.2140 0.000 0.000 0.000 0.000 0.973 0.027 0.3508 0.9431 0.0456 0.5325
Fe XVI 5 36.7478 0.633 0.007 0.073 0.030 0.000 0.248 0.3032 21.4497 0.0741 12.7918
Fe XVI 4 15.2597 0.000 0.000 0.000 0.000 0.935 0.064 0.2516 0.0719 0.0329 0.1186
Fe XVI 6 15.0960 0.182 0.001 0.000 0.000 0.760 0.056 0.3394 0.8149 0.0452 0.2251
Fe XVI 7 15.3150 0.000 0.000 0.000 0.000 0.957 0.043 0.2498 1.4674 0.0335 0.2118
Fe XVI 6 15.0794 0.000 0.000 0.000 0.000 0.990 0.010 0.3070 0.8149 0.0457 0.2251
Fe XVI 6 15.0752 0.000 0.000 0.000 0.000 0.997 0.003 0.3107 0.8149 0.0463 0.2251
Fe XVI 8 35.1134 0.000 0.007 0.100 0.021 0.000 0.860 0.3103 2.1108 0.0709 11.3896
Fe XVI 9 15.0260 0.000 0.000 0.000 0.000 0.995 0.005 0.3035 0.1278 0.0454 0.0230
Fe XVI 6 15.0916 0.000 0.000 0.000 0.000 0.991 0.009 0.2497 0.8149 0.0371 0.2251
Fe XVI 9 15.0472 0.000 0.000 0.000 0.000 0.997 0.003 0.2931 0.1278 0.0446 0.0230
Fe XVI 9 15.0309 0.000 0.000 0.000 0.000 0.999 0.001 0.2940 0.1278 0.0448 0.0230
Fe XVI 5 36.8018 0.662 0.022 0.071 0.021 0.000 0.216 0.1502 21.4497 0.0365 12.7918
Fe XVI 1 40.2348 0.000 0.026 0.082 0.025 0.000 0.861 0.1891 0.0448 0.0622 0.1462
Fe XVI 9 15.0471 0.000 0.000 0.000 0.000 0.999 0.001 0.2363 0.1278 0.0360 0.0230

  1. Full data table can be found at the CDS.

  2. ID: line ID (see Figs. A.1 and A.2)

  3. EX/CEX/RR/CRR/DR/CDR: contributions of upper level population from direct excitation, excitation followed by cascades, radiative recombination, radiative recombination followed by cascades, dielectronic recombination, dielectronic recombination followed by cascades

  4. Icapella, IHr 1099 line fluxes from the best-fit models (model 1)

  5. UCapella, UHr 1099 fractional systematic uncertainties of the lines from the Gaussian fits (model 2)

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