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

We present a novel, model-independent framework for studying the architecture of an
exoplanetary system at the system level. This framework allows us to characterise, quantify …

We report the discovery and characterization of a pair of sub-Neptunes transiting the bright K-
dwarf TOI-1064 (TIC 79748331), initially detected in the Transiting Exoplanet Survey …

Neptune-sized planets exhibit a wide range of compositions and densities, depending on
factors related to their formation and evolution history, such as the distance from their host …

Context. The GAPS collaboration is carrying out a spectroscopic and photometric follow-up
of a sample of young stars with planets (age≲ 600 Myr) to characterise planetary systems at …

We investigate starspot distributions consistent with space-based photometry of F, G, and K
stars in six stellar associations ranging in age from 10 Myr to 4 Gyr. We show that a simple …

The study of stellar flares has increased with new observations from CoRoT, Kepler, and
TESS satellites, revealing the broad-band visible emission from these events. Typically …

While the solar system contains no planets between the sizes of Uranus and Saturn, our
current exoplanet census includes several dozen such planets with well-measured masses …

Context. Although the number of exoplanets reported in the literature exceeds 5000 so far,
only a few dozen of them are young planets (≤ 900 Myr). However, a complete …

Context. Planetary atmospheric evolution modelling is a prime tool for understanding the
observed exoplanet population and constraining formation and migration mechanisms, but it …