Population studies of exoplanets are key to unlocking their statistical properties. So far, the
inferred properties have been mostly limited to planetary, orbital, and stellar parameters …

I calculate the physical properties of 32 transiting extrasolar planet and brown-dwarf systems
from existing photometric observations and measured spectroscopic parameters. The …

We study tidal dissipation in stars with masses in the range 0.1–1.6 M⊙ throughout their
evolution, including turbulent effective viscosity acting on equilibrium tides and inertial …

In this paper we search for distant massive companions to known transiting gas giant
planets that may have influenced the dynamical evolution of these systems. We present new …

We highlight the importance of gaseous TiO and VO opacity on the highly irradiated close-in
giant planets. The day-side atmospheres of these planets naturally fall into two classes that …

Planet formation is generally described in terms of a system containing the host star and a
protoplanetary disk,–, of which the internal properties (for example, mass and metallicity) …

We present refined values for the physical parameters of transiting exoplanets, based on a
self-consistent and uniform analysis of transit light curves and the observable properties of …

We estimate the strength of the bandpass-integrated thermal emission from the extrasolar
planet HD 209458b at 3.6, 4.5, 5.8, and 8.0 μm using the Infrared Array Camera (IRAC) on …

I present a homogeneous analysis of the transit light curves of 14 well-observed transiting
extrasolar planets. The light curves are modelled using jktebop, random errors are …

We carried out a systematic study of full-orbit phase curves for known transiting systems in
the northern ecliptic sky that were observed during Year 2 of the TESS primary mission. We …