Context. A new class of exoplanets has emerged: the ultra hot Jupiters, the hottest close-in
gas giants. The majority of them have weaker-than-expected spectral features in the 1.1− 1.7 …

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 …

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 …

We present a comprehensive analysis of the Hubble Space Telescope observations of the
atmosphere of WASP-121 b, an ultra-hot Jupiter. After reducing the transit, eclipse, and …

We investigate the use of deep convolutional neural networks (deep CNNs) for automatic
visual detection of galaxy mergers. Moreover, we investigate the use of transfer learning in …

Ultrahot Jupiters represent an exciting avenue for testing extreme physics and observing
atmospheric circulation regimes not found in our solar system. Their high temperatures …

We present the analysis of a full-orbit, spectroscopic phase curve of the ultra hot Jupiter
(UHJ) WASP-18b, obtained with the Wide Field Camera 3 aboard the Hubble Space …

Most planets currently amenable to transit spectroscopy are close enough to their host stars
to exhibit a relatively strong day to night temperature gradient. For hot planets this leads to a …

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 …

We report 78 secondary eclipse depths for a sample of 36 transiting hot Jupiters observed at
3.6 and 4.5 μm using the Spitzer Space Telescope. Our eclipse results for 27 of these …