At the dawn of the first discovery of exoplanets orbiting Sun-like stars in the mid-1990s, few
believed that observations of exoplanet atmospheres would ever be possible. After the 2002 …

The field of exoplanet atmospheric characterization has recently made considerable
advances with the advent of high-resolution spectroscopy from large ground-based …

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 …

We present new, full-orbit observations of the infrared phase variations of the canonical hot
Jupiter HD 189733b obtained in the 3.6 and 4.5 μm bands using the Spitzer Space …

We present results from an atmospheric circulation study of nine hot Jupiters that compose a
large transmission spectral survey using the Hubble and Spitzer Space Telescopes. These …

If both the day-side and night-side effective temperatures of a planet can be measured, it is
possible to estimate its Bond albedo, 0< AB< 1, as well as its day–night heat redistribution …

We present observations of six transits and six eclipses of the transiting planet system HD
189733 taken with the Spitzer Space Telescope's Infrared Array Camera (IRAC) at 8 μm, as …

We present evidence for a correlation between the observed properties of hot Jupiter
emission spectra and the activity levels of the host stars measured using Ca ii H & K …

We present an optical to near-infrared transmission spectrum of the hot Jupiter HAT-P-1b,
based on Hubble Space Telescope observations, covering the spectral regime from 0.29 to …

A key hypothesis in the field of exoplanet atmospheres is the trend of atmospheric thermal
structure with planetary equilibrium temperature. We explore this trend and report here the …