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. 14

Posterior distributions for the conjuction times T_conj,b of Gl 514 b that are close to TESS Sectors 23 (March-April 2020) and 50 (March-April 2022). The posteriors are derived from that obtained for our best-fit QPC model. The vertical lines mark the time-span of TESS observations.

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