Fig. 4
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Top panel: ASAS-SN photometric time series of GJ 1018. The magenta, gray, and blue vertical lines correspond to the TESS, HARPS, and ESPRESSO observing windows, respectively. Left panels: GLS periodograms of the ASAS-SN photometry corrected for the long-term trend. The vertical blue solid line indicates the median rotation modulation period obtained by the GLS, and the vertical blue dashed line indicate its second harmonic. The horizontal dotted lines indicate the 10 (orange), 1 (blue), and 0.1% (green) FAP levels. Right panels: phase-folded light curves to the maximum power period obtained by the GLS periodogram. The gray data points correspond to a 5-day binning.
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