Gl514 RVs and activity diagnostics

We found strong evidence that Gl~514 hosts a super-Earth on a likely eccentric orbit, residing in the conservative habitable zone for nearly 34% of its orbital period. The planet Gl 514 b has minimum mass m_b_sini_b_=5.2+/-0.9M_{sun}_, orbital period P_b_=140.43+/-0.41 days, and eccentricity e_b_=0.45^+0.15^_-0.14_. No evidence for transits is found in the TESS light curve.

There is no evidence for a longer period companion in the radial velocities and, based on astrometry, we can rule out a ~0.2M_{Jup}_ planet at a distance of ~3-10au, and massive giant planets/brown dwarfs out to several tens of au. We discuss the possible presence of a second low-mass companion at a shorter distance from the host than Gl 514 b. Gl 514 b represents an interesting science case to study the habitability of planets on eccentric orbits.

We advocate for additional spectroscopic follow-up to get more accurate and precise planetary parameters. Further follow-up is also needed to investigate sub m/s and shorter period signals.