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Table 5.

Results of the MCMC accretion disk plus Gaussian model fitting.

Line q σ i e ϕ0 r1 r2 Vel. FWHM Ampl.
(km s−1) (°) (°) (Rg) (Rg) (km s−1) (km s−1)
Hα, –13d 800 ± 400 37 500 ± 6500 0.02 ± 0.01
He II, –13d –170 ± 135 31 000 ± 850 0.13 ± 0.01
Hα, –3d 2.41 ± 0.04 1018 ± 273 85 ± 6 0.96 ± 0.02 256 ± 2 302 ± 13 4095 ± 315 –944 ± 1019 1014 ± 957 0.02 ± 0.01
He II, –3d 2.12 ± 0.05 1570 ± 205 89 ± 1 0.97 ± 0.01 219 ± 2 121 ± 12 2250 ± 375 675 ± 380 1750 ± 650 0.02 ± 0.01
Hα, +10d 2.28 ± 0.04 1270 ± 145 78 ± 5 0.96 ± 0.02 242 ± 2 270 ± 11 1453 ± 74 –494 ± 935 2169 ± 818 0.02 ± 0.01
He II, +10d 2.92 ± 0.06 1330 ± 100 86 ± 3 0.97 ± 0.01 208 ± 1 530 ± 10 2100 ± 90 400 ± 90 2400 ± 110 0.07 ± 0.01

Notes. For completeness we also provide the results of the Gaussian-only model for the first epoch, where the accretion disk model does not provide a good fit.

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