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Fig. 14
Gl 393. Panel a: GP fit (black solid line) and 1-sigma uncertainties (grey area) to theRV data of HIRES (green points), HARPS (blue points) and CARMENES VIS channel (red squares). Panel b: activity subtracted RVs, phase-folded to the 7.03 d period. The Keplerian model (black solid line) is overplotted.
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