activity
20072026
most citedHighly inclined and eccentric massive planets I: Planet-disc interactions

115 citations · 709 across the 37 of their papers we have counts for

collaborators

37 papers

astro-ph.SR2026

Southern Massive Stars at High Angular Resolution (SMaSH+): Properties of hierarchical massive triples

E. Bordier, H. Sana, A. J. Frost +9

While massive stars are frequently found in triple architectures, the lack of observed parameter distributions has long remained a bottleneck for statistical models of their evolut…

nlin.CD2024★ 5 cited

Improved detection of chaos with Lagrangian descriptors using differential algebra

Alexandru Căliman, Jérôme Daquin, Anne-Sophie Libert

Lagrangian descriptors (LDs) based on the arc length of orbits previously demonstrated their utility in delineating structures governing the dynamics. Recently, a chaos indicator b…

astro-ph.EP2024★ 7 cited

Drifts of the sub-stellar points of the TRAPPIST-1 planets

Revol Alexandre, Émeline Bolmont, Mariana Sastre +4

Accurate modeling of tidal interactions is crucial for interpreting recent JWST observations of the thermal emissions of TRAPPIST-1~b and c and for characterizing the surface condi…

astro-ph.IM2024★ 13 cited

The PLATO Mission

Heike Rauer, Conny Aerts, Juan Cabrera +842

PLATO (PLAnetary Transits and Oscillations of stars) is ESA's M3 mission designed to detect and characterise extrasolar planets and perform asteroseismic monitoring of a large numb…

astro-ph.EP2023★ 36 cited

A roadmap for the atmospheric characterization of terrestrial exoplanets with JWST

TRAPPIST-1 JWST Community Initiative, :, Julien de Wit +80

Ultra-cool dwarf stars are abundant, long-lived, and uniquely suited to enable the atmospheric study of transiting terrestrial companions with JWST. Amongst them, the most prominen…

astro-ph.EP2023★ 10 cited

Tidal interactions shape period ratios in planetary systems with three-body resonant chains

Carolina Charalambous, Jean Teyssandier, Anne-Sophie Libert

These last years several Systems with Tightly packed Inner Planets in the super-Earth mass regime have been discovered harboring chains of resonances. It is generally believed that…

astro-ph.EP2022★ 5 cited

Resonance capture and long-term evolution of planets in binary star systems

Arnaud Roisin, Nikita Doukhanin, Jean Teyssandier +1

The aim of this work is to study the impact of a binary companion on the evolution of two-planet systems during both the type-II migration phase and their long-term evolution after…

astro-ph.EP2022★ 23 cited

Proximity of exoplanets to first-order mean-motion resonances

Carolina Charalambous, Jean Teyssandier, Anne-Sophie Libert

Planetary formation theories and, more specifically, migration models predict that planets can be captured in mean-motion resonances (MMRs) during the disc phase. The distribution…

astro-ph.EP2021★ 20 cited

TRAPPIST-1: Dynamical analysis of the transit-timing variations and origin of the resonant chain

Jean Teyssandier, Anne-Sophie Libert, Eric Agol

We analyze solutions drawn from the recently published posterior distribution of the TRAPPIST-1 system, which consists of seven Earth-size planets appearing to be in a resonant cha…

astro-ph.EP2021★ 4 cited

Bridges and gaps at low-eccentricity first-order resonances

Kyriaki I. Antoniadou, Anne-Sophie Libert

Previous works on the divergence of first-order mean-motion resonances (MMRs) have studied in detail the extent of the pericentric and apocentric libration zones of adjacent first-…

astro-ph.EP2021★ 2 cited

Planetary migration in precessing disks for S-type wide binaries

Arnaud Roisin, Jean Teyssandier, Anne-Sophie Libert

The discovery of numerous circumprimary planets in the last few years has brought to the fore the question of planet formation in binary systems. The significant dynamical influenc…

astro-ph.EP2021

Inclination-type resonance in two-planet systems

Sotiris Sotiriadis, Anne-Sophie Libert

We investigate the inclination-growth mechanisms for two-planet systems during the late protoplanetary disc phase. In previous works, much attention has been directed to the inclin…

astro-ph.EP2020★ 2 cited

Evolution of a migrating giant planet in the presence of an inclined binary companion

Arnaud Roisin, Anne-Sophie Libert

Aims. There are a growing number of giant planets discovered moving around one stellar component of a binary star, most of which have very diverse eccentricity. These discoveries r…

astro-ph.EP2020★ 13 cited

Transit-Timing Variation Signature of Planet Migration: The Case of K2-24

Jean Teyssandier, Anne-Sophie Libert

The convergent migration of two planets in a gaseous disc can lead to capture in mean motion resonance (MMR). In addition, pairs of planets in or near MMRs are known to produce str…

astro-ph.EP2020★ 8 cited

Exploiting periodic orbits as dynamical clues for Kepler and K2 systems

Kyriaki I. Antoniadou, Anne-Sophie Libert

Many extrasolar systems possessing planets in mean-motion resonance or resonant chain have been discovered to date. The transit method coupled with transit timing variation analysi…

astro-ph.EP2019★ 17 cited

Resonant Laplace-Lagrange theory for extrasolar systems in mean-motion resonance

Marco Sansottera, Anne-Sophie Libert

Extrasolar systems with planets on eccentric orbits close to or in mean-motion resonances are common. The classical low-order resonant Hamiltonian expansion is unfit to describe th…

astro-ph.EP2019★ 13 cited

On the 3D secular dynamics of radial-velocity-detected planetary systems

Mara Volpi, Arnaud Roisin, Anne-Sophie Libert

Aims. To date, more than 600 multi-planetary systems have been discovered. Due to the limitations of the detection methods, our knowledge of the systems is usually far from complet…

astro-ph.EP2018★ 15 cited

Spatial resonant periodic orbits in the restricted three-body problem

K. I. Antoniadou, A. -S. Libert

The quest of exo-Earths has become a prominent field. In this work, we study the stability of non-coplanar planetary configurations consisting of an inclined inner terrestrial plan…

astro-ph.EP2018★ 21 cited

Dynamical evolution of triple-star systems by Lidov-Kozai cycles and tidal friction

Manon Bataille, Anne-Sophie Libert, Alexandre C. M. Correia

Many triple-star systems have an inner pair with an orbital period of a few days only. A common mechanism to explain the short-period pile-up present in the observations is the mig…

astro-ph.EP2018★ 20 cited

Origin and continuation of 3/2, 5/2, 3/1, 4/1 and 5/1 resonant periodic orbits in the circular and elliptic restricted three-body problem

Kyriaki I. Antoniadou, Anne-Sophie Libert

We consider a planetary system consisting of two primaries, namely a star and a giant planet, and a massless secondary, say a terrestrial planet or an asteroid, which moves under t…

astro-ph.EP2018★ 13 cited

Puzzling out the coexistence of terrestrial planets and giant exoplanets. The 2/1 resonant periodic orbits

Kyriaki I. Antoniadou, Anne-Sophie Libert

Hundreds of giant planets have been discovered so far and the quest of exo-Earths in giant planet systems has become intriguing. In this work, we aim to address the question of the…

astro-ph.EP2018★ 8 cited

Influence of periodic orbits on the formation of giant planetary systems

Anne-Sophie Libert, Sotiris Sotiriadis, Kyriaki I. Antoniadou

The late-stage formation of giant planetary systems is rich in interesting dynamical mechanisms. Previous simulations of three giant planets initially on quasi-circular and quasi-c…

astro-ph.EP2018★ 2 cited

Formation of terrestrial planets in eccentric and inclined giant planet systems

Sotiris Sotiriadis, Anne-Sophie Libert, Sean N. Raymond

Evidence of mutually inclined planetary orbits has been reported for giant planets these last years. Here we aim to study the impact of eccentric and inclined massive giant planets…

astro-ph.EP2017★ 35 cited

The language of exoplanet ranking metrics needs to change

Elizabeth Tasker, Joshua Tan, Kevin Heng +14

We have found many Earth-sized worlds but we have no way of determining if their surfaces are Earth-like. This makes it impossible to quantitatively compare habitability, and prete…