Fig. 4
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Comparison of our orbital solution to the Putkuri et al. (2023) one for our data around periastron. The phases on the left panel are calculated with our ephemeris, the ones on the right panel with the Putkuri et al. (2023) one. The symbols show our observed radial velocities (combined data), on both panels. The colour coding is as in Fig. 3. The solid lines indicate the orbital solutions for the respective components.
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