The masses and radii of exoplanets are fundamental quantities needed for their
characterisation. Studying the different populations of exoplanets is important for …

Context. The High Accuracy Radial velocity Planet Searcher (HARPS) spectrograph has
been mounted since 2003 at the ESO 3.6 m telescope in La Silla and provides state-of-the …

Young exoplanets are snapshots of the planetary evolution process. Planets that orbit stars
in young associations are particularly important because the age of the planetary system is …

Mature super-Earths and sub-Neptunes are predicted to be≃ Jovian radius when younger
than 10 Myr. Thus, we expect to find 5–15 R⊕ planets around young stars even if their older …

We present the discovery of a transiting hot Jupiter orbiting HIP 67522 (T eff∼ 5650 K; M*∼
1.2M⊙) in the 10–20 Myr old Sco-Cen OB association. We identified the transits in the TESS …

Exoplanets can evolve significantly between birth and maturity, as their atmospheres, orbits,
and structures are shaped by their environment. Young planets (< 1 Gyr) offer an opportunity …

Young exoplanets can offer insight into the evolution of planetary atmospheres,
compositions, and architectures. We present the discovery of the young planetary system …

The ExoClock project is an inclusive, integrated, and interactive platform that was developed
to monitor the ephemerides of the Ariel targets to increase the mission efficiency. The project …

We introduce the public version of the BAyesian STellar Algorithm (BASTA), an open-source
code written in Python to determine stellar properties based on a set of astrophysical …

The detection and characterization of young planetary systems offer a direct path to study
the processes that shape planet evolution. We report on the discovery of a sub-Neptune …