Aims. We determine the radii and masses of 293 nearby, bright M dwarfs of the CARMENES
survey. This is the first time that such a large and homogeneous high-resolution (R> 80 000) …

The detection of transiting exoplanets in time-series photometry requires the removal or
modeling of instrumental and stellar noise. While instrumental systematics can be reduced …

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 …

We present a velocimetric and spectropolarimetric analysis of 27 observations of the 22-Myr
M1 star AU Microscopii (AU Mic) collected with the high-resolution YJHK (0.98–2.35 μm) …

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 …

Abstract Since 2014, NASA's K2 mission has observed large portions of the ecliptic plane in
search of transiting planets and has detected hundreds of planet candidates. With …

In stellar astrophysics, the technique of population synthesis has been successfully used for
several decades. For planets, it is in contrast still a young method which only became …

We present a spectroscopic analysis of a 1-yr intensive monitoring campaign of the 22-Myr
old planet-hosting M dwarf AU Mic using the HARPS spectrograph. In a companion paper …

The system of two transiting Neptune-sized planets around the bright, young M-dwarf AU
Mic provides a unique opportunity to test models of planet formation, early evolution, and …

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 …