Table A.2
Parameters for spectral line features for ObsID 11044.
| P Cygni profiles | ||||||||||||
| Absorption | Emission | |||||||||||
|
|
||||||||||||
| Reference | Obs. | Thermal | Velocity | Column | Obs. | Norm | Thermal | Velocity | ||||
| wavelength | wavel. | Norm | broadening | FWHM | shift | density | wavel. | broadening | FWHM | shift | ||
| Line | λ theory | λ obs | A | v therm | Γ | Δv | N i | λ obs | A | v therm | Γ | Δv |
| (Å) | (Å) | (10-3 ph s-1 cm2) | (km s-1) | (keV) | (km s-1) | (1016 cm-2) | (Å) | (10-3 ph s-1 cm2) | (km s-1) | (keV) | (km s-1) | |
|
|
||||||||||||
| Si xiv Lyα | 6.1805 | 6.166(2) | −0.12 ± 0.05 |
|
– | −700 ± 100 | 0.9(3) | 6.181(3) | 0.21 ± 0.06 |
|
– | 20 ± 150 |
| Mg xii Lyα | 8.4192 | 8.402(4) | −0.13 ± 0.07 | ≤ 200 | ≤ 0.010 | −610 ± 140 | 0.7(2) | 8.419(3) |
|
|
– | −10 ± 110 |
| Ne x Lyα | 12.1317 | 12.115(3) |
|
|
≤ 0.012 | −410 ± 70 | 3.0(4) | 12.128(2) |
|
≤ 269 |
|
−90 ± 50 |
| Ne x Lyβ | 10.2327 | 10.231(2) |
|
|
|
−50 ± 60 | 74(2) | 10.237(2) |
|
≤ 1082 |
|
130 ± 60 |
| Ne x Lyδ | 9.4794 | 9.464(1) |
|
|
≤ 0.05 | −490 ± 30 | 83(19) | 9.500(6) |
|
≤ 821 | ≤ 0.05 | 650 ± 190 |
| Mg xi triplet | ||||||||||||
|
|
||||||||||||
| Mg xi r | 9.1687 | 9.14(1) | −0.3 ± 0.1 | ≤ 200 |
|
−940 ± 330 | 0.9(4) | 9.168(2) |
|
280 ± 100 | ≤ 0.008 | −20 ± 70 |
| Mg xi i | 9.2312 | 9.228(5) |
|
≤ 700 | ≤ 0.026 | −100 ± 160 | ||||||
| Mg xi f | 9.3143 | 9.308(7) |
|
≤ 810 | ≤ 0.025 | −200 ± 230 | ||||||
| Emission lines | ||||||||||||
|
|
||||||||||||
| Fe Kα | 1.9373 | 1.937(3) | 1.0 ± 0.4 | ≤ 950 | ≤ 0.5 | −50 ± 450 | ||||||
| Fe xxv | 1.8504 | 1.862(6) | 0.22 ± 0.2 | ≤ 970 | ≤ 0.5 | 1880 ± 970 | ||||||
| Si xiii He f | 6.7403 | 6.741(1) | 0.28 ± 0.07 | ≤ 240 | ≤ 0.017 | 30 ± 40 | ||||||
| Ne ix He i | 13.55 | 13.55(2) | 0.28 ± 0.12 | 600 ± 400 | – | 0 ± 440 | ||||||
| Absorption lines | ||||||||||||
|
|
||||||||||||
| Si xii (Li) | 6.7176 | 6.705(1) | −0.13 ± 0.04 |
|
– | −670 ± 50 | 0.6(2) | |||||
| Fe xxi | 12.2840 | 12.265(7) | −0.15 ± 0.06 |
|
– | −460 ± 170 | – | |||||
Notes. All lines, including the emission and absorption line portion of the P Cygni line profiles, are modeled with Voigt profiles. Number in brackets corresponds to the uncertainty in units of the last digit. Equivalent width and column density are not calculated for emission lines.
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