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Table 6

Sine function parameters describing the orbital modulation of the Doppler shifts.

K W v 0 Δφ χ2/ d.o.f.
[km s-1] [km s-1]

all lines included in Fig. 9:
276 ± 11 40 ± 14 0.073 ± 0.002 428.28 / 34 12.59
242 ± 10 −7 0 539.01/36 14.97
266 ± 10 7 0.070 ± 0.002 433.93 / 35 12.39
297 ± 11 −84 ± 8 0 442.79/35 12.65

fit to Ne x, Mg xii, and Si xiv:
8 ± 36 0.072 ± 0.004 30.87 / 9 3.43
271 ± 19 −7 0 63.45/11 5.77
286 ± 20 7 0.072 ± 0.002 30.9 / 10 3.09
313 ± 24 −62 ± 18 0 39.07/10 3.91

fit to Ne x:
276 ± 37 83 ± 48 0.076 ± 0.006 1.72 / 1 1.72
236 ± 33 −7 0 41.24/3 13.75
267 ± 34 −7 0.067 ± 0.003 8.49/2 4.24
285 ± 36 106 ± 26 0 2.67 / 2 1.33

fit to Mg xii:
88 ± 91 0.07 ± 0.01 0.48 / 1 0.48
309 ± 30 −7 0 7.67/3 2.56
318 ± 32 7 0.075 ± 0.003 3.46 / 2 1.73
334 ± 47 −33 ± 38 0 6.39/2 3.19

fit to Si xiv:
80 ± 89 0.063 ± 0.013 0.69 / 1 0.69
256 ± 38 −7 0 6.79/3 2.26
262 ± 38 7 0.075 ± 0.004 3.31 / 2 1.65
275 ± 48 −30 ± 37 0 5.74/2 2.87

Notes. The fits are to a model of the form v(φ) = v0 + KW·sin [ 2π(φ − Δφ) ]. Parameters without uncertainties were held fixed in the fit. KW – amplitude of the sine curve; v0 – offset of the sine curve, Δφ – phase shift: v0 = −7 km s-1 and Δφ = 0 are fixed to the orbital motion of the black hole. Best fits are printed in bold.

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