Planets intermediate in size between the Earth and Neptune, and orbiting closer to their host
stars than Mercury does the Sun, are the most common type of planet revealed by exoplanet …

In the past few years, significant advances have been made in understanding the
distributions of exoplanet populations and the architecture of planetary systems. We review …

We used high-precision radial velocity measurements of FGKM stars to determine the
occurrence of giant planets as a function of orbital separation spanning 0.03–30 au. Giant …

Rings are the most frequently revealed substructure in Atacama Large Millimeter/
submillimeter Array (ALMA) dust observations of protoplanetary disks, but their origin is still …

The radii and orbital periods of 4,000+ confirmed/candidate exoplanets have been precisely
measured by the Kepler mission. The radii show a bimodal distribution, with two peaks …

The orbital distribution of giant planets is crucial for understanding how terrestrial planets
form and predicting yields of exoplanet surveys. Here, we derive giant planets occurrence …

Context. Recent years have seen building evidence that planet formation starts early, in the
first~ 0.5 Myr. Studying the dust masses available in young disks enables us to understand …

Our understanding of planet formation has been rapidly evolving in recent years. The
classical planet formation theory, developed when the only known planetary system was our …

The Kepler survey provides a statistical census of planetary systems out to the habitable
zone. Because most planets are non-transiting, orbital architectures are best estimated …

The nature and origin of free-floating planets (FFPs) are still largely unconstrained because
of a lack of large homogeneous samples to enable a statistical analysis of their properties …