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. One of the long-term goals of exoplanet science is the atmospheric characterization
of dozens of small exoplanets in order to understand their diversity and search for habitable …

Over the past three decades, we have witnessed one of the great revolutions in our
understanding of the cosmos—the dawn of the Exoplanet Era. Where once we knew of just …

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 present exoplanet occurrence rates estimated with approximate Bayesian computation
for planets with radii between 0.5 and 16 R⊕ and orbital periods between 0.78 and 400 …

The Planetary Camera and Spectrograph (PCS) for the Extremely Large Telescope (ELT)
will be dedicated to detecting and characterising nearby exoplanets with sizes from sub …

The search for habitable planets has revealed many planets that can vary greatly from an
Earth analog environment. These include highly eccentric orbits, giant planets, different bulk …

The discovery and characterization of Earth-sized planets that are in, or near, a tidally locked
state are of crucial importance to understanding terrestrial planet evolution. For this purpose …

We present the occurrence rates for rocky planets in the habitable zones (HZs) of main-
sequence dwarf stars based on the Kepler DR25 planet candidate catalog and Gaia-based …

The expected yield of potentially Earth-like planets is a useful metric for designing future
exoplanet-imaging missions. Recent yield studies of direct-imaging missions have focused …