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Fig. 5.

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Activity-indicators-based analysis of the simulated planet host with random spectral variability. Upper and middle panels: GLS periodogram for the BIS and FWHM data, respectively. The dashed vertical lines mark the expected 7-days planetary frequency. Lower panels: bisector and full-width half maximum data as a function of RVs obtained for the spectra through cross-correlating against a PHOENIX template.

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