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Table A.1

H-like, He-like, and Fe absorption lines at φorb ~ 0.75, φorb ~ 0.05, and ~0.2 (ObsID 3815, 8525, and 9847).

ObsID 3815 ObsID 8525 ObsID 9847
φorb ~ 0.75 φorb ~ 0.05 φorb ~ 0.2

Column Velocity Thermal Column Velocity Thermal Column Velocity Thermal
density shift broadening density shift broadening density shift broadening
N i Δv ξ N i Δv ξ N i Δv ξ
[1016cm-2] [km s-1] [km s-1] [1016cm-2] [km s-1] [km s-1] [1016cm-2] [km s-1] [km s-1]

H-like lines

Ne x 240 ± 50 −360 ± 40
Na xi
Mg xii 3.24 ± 0.15 −80 ± 70 −200 ± 90
Al xiii 130 ± 100 7.9 0.0 ± 104 3 × 104 8.2 8540
Si xiv 420 ± 50 −90 ± 50 517
S xvi 3.4 ± 0.5 220 ± 170 −100 ± 400 2.8
Ar xviii 5 ± 4 26 (0.1 ± 1.0) × 104 1875
Ca xx 2586 60 104 6800

He-like lines

Ne ix 0.89 ± 0.13
Na x 0.99 ± 0.09 −300 ± 100 130 220 ± 60
Mg xi 0.68 ± 0.08
Al xii
Si xiii 90
S xv 310 ± 150 4.2 ± 1.5 300 ± 400 900 ± 600 37
Ar xvii 0.5
Ca xix 8 104

Fe lines

Fe xvii
Fe xviii 1.47 ± 0.16
Fe xix 225.2 ± 0.2
Fe xx 60 ± 40
Fe xxi 240 ± 50 1.6 ± 0.4
Fe xxii 182 ± 10 21 ± 3
Fe xxiii 34 864 1.6 × 10-3 (0.0 ± 1.0) × 104 1.27 × 104
Fe xxiv 250 ± 50 4.5 ± 1.0 10 ± 60

Notes.

(†)

Unconstrained parameter. The calculation has reached one or both limits of the range set for this parameter. Note that primarily affected line series are those consisting of weak or possibly blended lines of Al, Ar, Ca, or Fe.

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