Table 2: Results of double-Gaussian fits to the He I $\lambda {6678}$ P Cyg profiles: 3 degrees of freedom. In this set of fits, the Gaussian widths are kept fixed to the mean widths of the absorption and emission components, and the continuum flux for each profile is kept fixed at the continuum for each spectrum. In addition, the height of the emission component is kept fixed at the height of the emission component in the summed spectrum. The absorption components' height and the line components' velocities (with respect to the cluster velocity) are allowed to vary.
Orbital $V_{_{\rm Emission}}$ $V_{_{\rm Absorption}}$ $h_{_{\rm Absorption}}$ $\chi^2$
Phase (km s-1) (km s-1) ( ${\rm erg~cm}^{-2}~{\rm s}^{-1}~{\rm\AA}^{-1}$)  
0.721 $ -41.9 \pm 23.8$ $-4.5 \pm 5.4 $ $-1.22 \pm0.01 $ 1.649
0.732 $-9.9 \pm 44.4$ $ 7.0 \pm10.2 $ $-1.25 \pm0.02 $ 0.941
0.742 $-16.0 \pm 27.2$ $ 7.5 \pm 6.4 $ $-1.22 \pm0.01 $ 1.287
0.816 $36.3 \pm 20.4$ $10.7 \pm 5.6 $ $-1.09 \pm0.01 $ 2.909
0.833 $33.2 \pm 23.2$ $19.5 \pm 6.4 $ $-1.09 \pm0.01 $ 0.654
0.848 $59.7 \pm 37.4$ $25.4 \pm 10.2 $ $-1.06 \pm0.02 $ 0.796
0.910 1 $11.2 \pm 21.0$ $43.4 \pm 6.8 $ $-0.80 \pm0.02 $ 1.381
0.927 $86.5 \pm 27.6$ $40.6 \pm 10.2 $ $-0.77 \pm0.02 $ 0.906
0.942 $89.6 \pm 26.2$ $46.6 \pm 10.0 $ $-0.75 \pm0.02 $ 1.024
1.004 $66.6 \pm 25.0$ $20.6 \pm 11.8 $ $-0.62 \pm0.02 $ 0.761
1.020 $74.8 \pm 23.8$ $21.5 \pm 10.2 $ $-0.66 \pm0.02 $ 0.980
1.035 $89.0 \pm 19.4$ $20.0 \pm 7.8 $ $-0.66 \pm0.02 $ 1.435
1.098 $47.7 \pm 27.2$ $-2.0 \pm 8.0 $ $-0.95 \pm0.02 $ 1.131
1.114 $94.8 \pm 23.8$ $12.5 \pm 6.2 $ $-0.92 \pm0.02 $ 1.149
1.130 $60.9 \pm 26.2$ $ 6.1 \pm 6.8 $ $-1.04 \pm0.02 $ 1.126


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