Fig. 1
Orbital fit at 7.78 days found by HO15 compared to phase-folded visible and NIR RVs. Top panel: orbital fit (black dashed line)obtained with the visible data (FOCES, SARG, and HERMES RVs from HO15, grey dots) and HARPS-N 2015 RVs (green dots). Bottom panel: orbital fit (black dashed line), GIANO/GIANO-B (red dots), IGRINS (light blue dots), and HARPS-N 2017 (black asterisks, two acquired in GIARPS mode) RVs.
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