activity
20242026
most citedRV-exoplanet eccentricities: Good, Beta, and Best

11 citations · 16 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph.SR2026

RedDots: Magnetic field of the nearby active M dwarf GJ 729, and a search for companions

E. L. Brown, S. V. Jeffers, S. C. Marsden +5

M dwarfs are prime targets for discovering exoplanets, and the nearest M dwarfs to the Sun provide among the best opportunities for follow-up detailed exoplanet characterization. G…

astro-ph.EP2026

RedDots: Multiplanet system around M dwarf GJ 887 in the solar neighborhood

C. Hartogh, S. V. Jeffers, S. Dreizler +7

GJ 887 is a bright M dwarf in the solar neighborhood with two currently reported nontransiting exoplanets with periods of and along with an addition…

astro-ph.EP2025★ 3 cited

The CARMENES search for exoplanets around M dwarfs : Understanding the wavelength dependence of radial velocity measurements

S. V. Jeffers, J. R. Barnes, P. Schöfer +22

Context. Current exoplanet surveys are focused on detecting small exoplanets orbiting in the liquid-water habitable zones of their host stars. Despite the recent significant advanc…

astro-ph.EP2025★ 2 cited

RedDots: Planetary masses in the GJ1061 system from planet-planet interaction

S. Dreizler, S. V. Jeffers, F. Liebing +8

GJ1061 is a very nearby M star hosting three low-mass temperate planets detected from radial velocity variations. The close to 4:2:1 period commensurability of the planets, the ava…

astro-ph.EP2025★ 11 cited

RV-exoplanet eccentricities: Good, Beta, and Best

A. T. Stevenson, C. A. Haswell, J. P. Faria +4

We examine the eccentricity distribution(s) of radial velocity detected exoplanets. Previously, the eccentricity distribution was found to be described well by a Beta distribution…

astro-ph.SR2024

Identifying activity induced RV periodicities and correlations using Central Line Moments

J. R. Barnes, S. V. Jeffers, C. A. Haswell +5

The radial velocity (RV) method of exoplanet detection requires mitigation of nuisance signals arising from stellar activity. Using analytic cool and facular spot models, we explor…

astro-ph.SR2024

The variable magnetic field of V889 Her and the challenge of detecting exoplanets around young Suns using Gaussian process regression

E. L. Brown, S. C. Marsden, S. V. Jeffers +3

Discovering exoplanets orbiting young Suns can provide insight into the formation and early evolution of our own solar system, but the extreme magnetic activity of young stars obfu…