We present a high-precision radial velocity (RV) survey of 719 FGKM stars, which host 164
known exoplanets and 14 newly discovered or revised exoplanets and substellar …

Context. The nearest stars provide a fundamental constraint for our understanding of stellar
physics and the Galaxy. The nearby sample serves as an anchor where all objects can be …

Measured spectral shifts due to intrinsic stellar variability (eg, pulsations, granulation) and
activity (eg, spots, plages) are the largest source of error for extreme-precision radial-velocity …

A complete accounting of nearby objects—from the highest-mass white dwarf progenitors
down to low-mass brown dwarfs—is now possible, thanks to an almost complete set of …

Directly imaging temperate rocky planets orbiting nearby, Sun-like stars with a 6 m class
IR/O/UV space telescope, recently dubbed the Habitable Worlds Observatory, is a high …

We explore the impact of outer stellar companions on the occurrence rate of giant planets
detected with radial velocities. We searched for stellar and planetary companions to a …

Tidal interaction between an exoplanet and its host star is a possible pathway to transfer
angular momentum between the planetary orbit and the stellar spin. In cases where the …

Context. The leading spectrographs used for exoplanets' search and characterization offer
online data reduction softwares (DRS) that yield, as an ancillary result, the full-width at half …

We describe a software package called VPLanet that simulates fundamental aspects of
planetary system evolution over Gyr timescales, with a focus on investigating habitable …

We present a catalog (status 2022 July 1) of triple and higher-order systems identified
containing exoplanets based on data from the literature, including various analyses. We …