Context. The Gaia DR3 catalogue contains, for the first time, about 800 000 solutions with
either orbital elements or trend parameters for astrometric, spectroscopic, and eclipsing …

Context. The astrometric discovery of sub-stellar mass companions orbiting stars is
exceedingly hard due to the required sub-milliarcsecond precision, limiting the application of …

Here we present juliet, a versatile tool for the analysis of transits, radial velocities, or both.
juliet is built over many available tools for the modelling of transits, radial velocities, and …

We carried out a Bayesian homogeneous determination of the orbital parameters of 231
transiting giant planets (TGPs) that are alone or have distant companions; we employed …

We report on the masses, sizes, and orbits of the planets orbiting 22 Kepler stars. There are
49 planet candidates around these stars, including 42 detected through transits and 7 …

With the maturation of near-infrared high-resolution spectroscopy, especially when used for
precision radial velocity, data reduction has faced unprecedented challenges in terms of …

ABSTRACT HIP 9618 (HD 12572, TOI-1471, TIC 306263608) is a bright (G= 9.0 mag) solar
analogue. TESS photometry revealed the star to have two candidate planets with radii of …

Photospheric stellar activity (ie dark spots or bright plages) might be an important source of
noise and confusion in stellar radial-velocity (RV) measurements. Radial-velocimetry planet …

The distribution of close-in exoplanets is shaped by a complex interplay between
atmospheric and dynamical processes. The Desert-Rim Exoplanets Atmosphere and …

While giant extrasolar planets have been studied for more than two decades now, there are
still some open questions as to their dominant formation and migration processes, as well as …