Fig. A.3.
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Evolution of R and z with time for the orbit integrations of the three selected stars: A, B, and C. Each star’s R(t) is shown over a period of 4 Gyr, with t = 0 Gyr set to the first maximum such that the three stars are in phase. The z(t) is shown over the same time period for the corresponding star. Grey dash-dot and dotted lines correspond to the periods according to the frequencies derived by SuperFreq and NAFF, respectively.
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