Fig. 16.
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Variability of the Kepler star HD 173701 (KIC 8006161) as inferred from (A) p-mode frequency shifts by Salabert et al. (2018), (B) average seismic travel-time shift from our work and (C) photometric variability. The vertical errors bars correspond to ±1 standard deviations. The horizontal error bars represent the observation duration for each measurement (90 days).
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