Fig. A.3

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Spectral profile around the Hα line of HIP 95176. The spectra have been corrected from the Doppler shift of the F component, which produces the lines at rest in the chosen frame (seen as dark vertical features). The Hα line thus moves with the B companion. All spectra have been re-ordered according to their orbital phase, and interpolations between them have been performed to smooth the features. Phase 0 was set arbitrarily at JD 2455639.78, and roughly corresponds to quadrature, with the B star coming towards the observer. The color map has been normalized to unity at the continuum.
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