Vincent Van Eylen

Hot Jupiters with relatives: discovery of additional planets in orbit around WASP-41 and WASP-47

SOPHIE velocimetry ofKeplertransit candidates

The EBLM Project

Investigating hot-Jupiter inflated radii with hierarchical Bayesian modelling

Obliquities of exoplanet host stars

WASP-117b: a 10-day-period Saturn in an eccentric and misaligned orbit

A combined transmission spectrum of the Earth-sized exoplanets TRAPPIST-1 b and c

On the Feasibility of Intense Radial Velocity Surveys for Earth-Twin Discoveries

FRIENDS OF HOT JUPITERS. I. A RADIAL VELOCITY SEARCH FOR MASSIVE, LONG-PERIOD COMPANIONS TO CLOSE-IN GAS GIANT PLANETS

The Fate of Binaries in the Galactic Center: The Mundane and the Exotic

Warm Jupiters Are Less Lonely than Hot Jupiters: Close Neighbors

THE ECCENTRICITY DISTRIBUTION OF SHORT-PERIOD PLANET CANDIDATES DETECTED BY KEPLER IN OCCULTATION

Variability in the super-Earth 55 Cnc e

The Occurrence and Architecture of Exoplanetary Systems

Star–disc–binary interactions in protoplanetary disc systems and primordial spin–orbit misalignments

Peculiar architectures for the WASP-53 and WASP-81 planet-hosting systems

New Low-mass Eclipsing Binary Systems in Praesepe Discovered by K2

Detecting the spin-orbit misalignment of the super-Earth 55 Cancri e

Limb darkening and exoplanets: testing stellar model atmospheres and identifying biases in transit parameters

ROSSITER-MCLAUGHLIN OBSERVATIONS OF 55 Cnc e

A STUDY OF THE SHORTEST-PERIOD PLANETS FOUND WITH KEPLER

Rossiter–McLaughlin models and their effect on estimates of stellar rotation, illustrated using six WASP systems

A-type Stars, the Destroyers of Worlds: The Lives and Deaths of Jupiters in Evolving Stellar Binaries

MASCARA-3b

A puffy polar planet

Asteroseismic inference on the spin-orbit misalignment and stellar parameters of HAT-P-7

WHAT ASTEROSEISMOLOGY CAN DO FOR EXOPLANETS: KEPLER-410A b IS A SMALL NEPTUNE AROUND A BRIGHT STAR, IN AN ECCENTRIC ORBIT CONSISTENT WITH LOW OBLIQUITY

ECCENTRICITY FROM TRANSIT PHOTOMETRY: SMALL PLANETS IN KEPLER MULTI-PLANET SYSTEMS HAVE LOW ECCENTRICITIES

ORBITAL CIRCULARIZATION OF HOT AND COOL KEPLER ECLIPSING BINARIES

Do Close-in Giant Planets Orbiting Evolved Stars Prefer Eccentric Orbits?

ACCURATE PARAMETERS OF THE OLDEST KNOWN ROCKY-EXOPLANET HOSTING SYSTEM: KEPLER-10 REVISITED

Properties of extrasolar planets and their host stars: A case study of HAT‐P‐7