Context. The CARMENES instrument, installed at the 3.5 m telescope of the Calar Alto
Observatory in Almería, Spain, was conceived to deliver high-accuracy radial velocity (RV) …

Theories of planet formation predict that low-mass stars should rarely host exoplanets with
masses exceeding that of Neptune. We used radial velocity observations to detect a …

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 …

Cold Jovian planets play an important role in sculpting the dynamical environment in which
inner terrestrial planets form. The core accretion model predicts that giant planets cannot …

Context. A challenge with radial-velocity (RV) data is disentangling the origin of signals
either due to a planetary companion or to stellar activity. In fact, the existence of a planetary …

We present the discovery of TOI-5205b, a transiting Jovian planet orbiting a solar metallicity
M4V star, which was discovered using Transiting Exoplanet Survey Satellite photometry and …

We propose a pebble-driven core accretion scenario to explain the formation of giant
planets around the late-M dwarfs of M★= 0.1–0.2 M⊙. In order to explore the optimal disk …

We report the discovery and characterization of two small transiting planets orbiting the
bright M3. 0V star TOI-1468 (LSPM J0106+ 1913), whose transit signals were detected in …

One of the main scientific goals of the TESS mission is the discovery of transiting small
planets around the closest and brightest stars in the sky. Here, using data from the …

Aims. Knowledge of rotation periods (P rot) is important for understanding the magnetic
activity and angular momentum evolution of late-type stars, as well as for evaluating radial …