Fig. 7
Phase plots for the 1
06495 period calculated using ephemeris 2. Top: all yellow-band photometry O–C residuals prewhitened for the 2.5 d period and its harmonics are shown. Middle: a plot of all the residuals from the orbital solution for the Gaussian-fit He i 6678 Å RVs. Bottom: a plot of the residuals from the orbital solution for the Gaussian fit He i 6678 Å RVs for the subset of Aurelie spectra.
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