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Exoplanet statistics and theoretical implications
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 …
distributions of exoplanet populations and the architecture of planetary systems. We review …
Density, not radius, separates rocky and water-rich small planets orbiting M dwarf stars
Exoplanets smaller than Neptune are common around red dwarf stars (M dwarfs), with those
that transit their host star constituting the bulk of known temperate worlds amenable for …
that transit their host star constituting the bulk of known temperate worlds amenable for …
Water in the terrestrial planet-forming zone of the PDS 70 disk
Terrestrial and sub-Neptune planets are expected to form in the inner (less than 10 au)
regions of protoplanetary disks. Water plays a key role in their formation,–, although it is yet …
regions of protoplanetary disks. Water plays a key role in their formation,–, although it is yet …
Architectures of compact multi-planet systems: diversity and uniformity
One of the most important developments in exoplanet science in the past decade is the
discovery of multi-planet systems with sub-Neptune-sized planets interior to 1~ AU. This …
discovery of multi-planet systems with sub-Neptune-sized planets interior to 1~ AU. This …
Planet formation theory in the era of ALMA and Kepler: from pebbles to exoplanets
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 …
classical planet formation theory, developed when the only known planetary system was our …
Hints for a turnover at the snow line in the giant planet occurrence rate
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 …
form and predicting yields of exoplanet surveys. Here, we derive giant planets occurrence …
The nature of the radius valley-Hints from formation and evolution models
The existence of a radius valley in the Kepler size distribution stands as one of the most
important observational constraints to understand the origin and composition of exoplanets …
important observational constraints to understand the origin and composition of exoplanets …
Occurrence rates of planets orbiting FGK stars: Combining Kepler DR25, Gaia DR2, and Bayesian inference
We characterize the occurrence rate of planets, ranging in size from 0.5 to 16 R⊕, orbiting
FGK stars with orbital periods from 0.5 to 500 days. Our analysis is based on results from …
FGK stars with orbital periods from 0.5 to 500 days. Our analysis is based on results from …
The New Generation Planetary Population Synthesis (NGPPS)-I. Bern global model of planet formation and evolution, model tests, and emerging planetary systems
Context. The explosion of observational data on exoplanets gives many constraints on
theoretical models of planet formation and evolution. Observational data probe very large …
theoretical models of planet formation and evolution. Observational data probe very large …
A fading radius valley towards M dwarfs, a persistent density valley across stellar types
The radius valley separating super-Earths from mini-Neptunes is a fundamental benchmark
for theories of planet formation and evolution. Observations show that the location of the …
for theories of planet formation and evolution. Observations show that the location of the …