We provide a brief review of many aspects of the planetary physics of hot Jupiters. Our aim is
to cover most of the major areas of current study while providing the reader with additional …

Groundbased and spacecraft telescopic observations, combined with an intensive modeling
effort, have greatly enhanced our understanding of hot giant planets and brown dwarfs over …

We carried out a Bayesian homogeneous determination of the orbital parameters of 231
transiting giant planets (TGPs) that are alone or have distant companions; we employed …

Extremely irradiated hot Jupiters, exoplanets reaching dayside temperatures> 2000 K,
stretch our understanding of planetary atmospheres and the models we use to interpret …

Observations of exoplanet atmospheres have shown that aerosols, like in the solar system,
are common across a variety of temperatures and planet types. The formation and …

We report high-resolution spectroscopic detection of TiO molecular signature in the day-side
spectra of WASP-33b, the second hottest known hot Jupiter. We used the High Dispersion …

ABSTRACT HAT-P-20b is a giant metal-rich exoplanet orbiting a metal-rich star. We analyze
two secondary eclipses of the planet in each of the 3.6 and 4.5 μm bands of Warm Spitzer …

Recent observations of ultra-hot Jupiters with dayside temperatures in excess of 2500 K
have found evidence for new physical processes at play in their atmospheres. In this work …

The full-phase infrared light curves of low-eccentricity hot Jupiters show a trend of increasing
dayside-to-nightside brightness temperature difference with increasing equilibrium …

Transport-induced quenching, ie the homogenization of chemical abundances by
atmospheric advection, is thought to occur in the atmospheres of hot gas giant exoplanets …