activity
20092022
most citedTransit timing variations in WASP-10b induced by stellar activity?

125 citations · 588 across the 19 of their papers we have counts for

collaborators

19 papers

astro-ph.EP2022★ 50 cited

Detection of the tidal deformation of WASP-103b at with CHEOPS

S. C. C. Barros, B. Akinsanm, G. Boué +5

WASP-103b is the exoplanet with the highest expected deformation signature in its transit light curve and one of the shortest expected spiral-in times. Measuring the tidal deformat…

astro-ph.EP2021★ 3 cited

Ellipsoidal equilibrium figure and Cassini states of rotating planets and satellites deformed by a tidal potential in the spatial case

Hugo A. Folonier, Gwenaël Boué, Sylvio Ferraz-Mello

The equilibrium figure of an inviscid tidally deformed body is the starting point for the construction of many tidal theories such as Darwinian tidal theories or the hydrodynamical…

astro-ph.EP2021★ 34 cited

The large obliquity of Saturn explained by the fast migration of Titan

Melaine Saillenfest, Giacomo Lari, Gwenaël Boué

The obliquity of a planet is the tilt between its equator and its orbital plane. Giant planets are expected to form with near-zero obliquities. After its formation, some dynamical…

astro-ph.EP2021★ 13 cited

Constraining the Earth's Dynamical Ellipticity from Ice Age Dynamics

Mohammad Farhat, Jacques Laskar, Gwenaël Boué

The dynamical ellipticity of a planet expresses the departure of its mass distribution from spherical symmetry. It enters as a parameter in the description of a planet's precession…

astro-ph.EP2020★ 30 cited

Discovery and characterization of the exoplanets WASP-148b and c. A transiting system with two interacting giant planets

G. Hebrard, R. F. Diaz, A. C. M. Correia +39

We present the discovery and characterization of WASP-148, a new extrasolar system that includes at least two giant planets. The host star is a slowly rotating inactive late-G dwar…

astro-ph.EP2019★ 29 cited

Orbital relaxation and excitation of planets tidally interacting with white dwarfs

Dimitri Veras, Michael Efroimsky, Valeri V. Makarov +6

Observational evidence of white dwarf planetary systems is dominated by the remains of exo-asteroids through accreted metals, debris discs, and orbiting planetesimals. However, exo…