Fig. 7.
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Radial velocity measurements as a function of the orbital phase with the fit from Fig. 5 scaled according to Eq. (3) and vertically shifted by 0.23 km s−1. The red dashed-dotted line corresponds to a linear fit to the RV values (except the one from Lunt 1918). The horizontal error bars reflect the time range during which the RV is obtained.
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