A quarter century of spectroscopic monitoring of the nearby M dwarf Gl 514 - A super-Earth on an eccentric orbit moving in and out of the habitable zone

Open Access

Fig. C.2

Phase-folded RVs of HARPS_terra and CARMENES-VIS showing the spectroscopic orbit of Gl 514 b for the circular case. The blue solid line is the best-fit solution using a QPC kernel to model the activity. The error bars include the uncorrelated jitter terms added in quadrature to the formal RV uncertainties. Cyan dots correspond to RV data averaged over 15 phase bins.

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