Fig. 1.
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Orbital solutions for HD 164 438 obtained only with MONOS data. Upper panel: new orbital solution for HD 164 438 obtained from our RV measurements of the He I λ5876 line using a Gaussian fit. The orbital solution was obtained using the SBOP code. Lower panel: orbital solution using our x-corr RV measurements. The RVs determined by Mayer et al. (2017) (red circle) are shifted by 6.5 km s−1 to bring them to our velocity rest frame. MONOS RVs are shown with the navy square symbols. The dotted blue line shows the γ of the system.
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