Exoplanetary science is on the verge of an unprecedented revolution. The thousands of
exoplanets discovered over the past decade have most recently been supplemented by …

Characterizing the atmospheres of extrasolar planets is the new frontier in exoplanetary
science. The last two decades of exoplanet discoveries have revealed that exoplanets are …

Clouds are prevalent in many of the exoplanet atmospheres that have been observed to
date. For transiting exoplanets, we know if clouds are present because they mute spectral …

High-resolution spectroscopy (R≥ 25,000) has recently emerged as one of the leading
methods for detecting atomic and molecular species in the atmospheres of exoplanets …

We present here the analysis of 30 gaseous extrasolar planets, with temperatures between
600 and 2400 K and radii between 0.35 and 1.9 R Jup. The quality of the HST/WFC3 …

Transmission spectroscopy of exoplanets has the potential to provide precise
measurements of atmospheric chemical abundances, in particular of hot Jupiters whose …

Thousands of transiting exoplanets have been discovered, but spectral analysis of their
atmospheres has so far been dominated by a small number of exoplanets and data …

We present a consistent optimal estimation retrieval analysis of 10 hot Jupiter exoplanets,
each with transmission spectral data spanning the visible to near-infrared wavelength range …

This article summarizes a workshop held on March, 2014, on the potential of the James
Webb Space Telescope (JWST) to revolutionize our knowledge of the physical properties of …

We report near-infrared spectroscopy of the gas giant planet HD 189733b in transit. We
used the Hubble Space Telescope Wide Field Camera 3 (HST WFC3) with its G141 grism …