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 …

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 …

We present a new generation of substellar atmosphere and evolution models, appropriate
for application to studies of L-, T-, and Y-type brown dwarfs and self-luminous extrasolar …

The abundances of main carbon-and oxygen-bearing gases in the atmospheres of giant
exoplanets provide insights into atmospheric chemistry and planet formation processes …

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 …

High-resolution Doppler-resolved spectroscopy has opened up a new window into the
atmospheres of both transiting and non-transiting exoplanets. Here, we present VLT/UVES …

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

We present thermal phase curve measurements for the hot Jupiter WASP-103b observed
with Hubble/WFC3 and Spitzer/IRAC. The phase curves have large amplitudes and …

Ultrahot Jupiters are gas giants that orbit so close to their host star that they are tidally
locked, causing a permanent hot dayside and a cooler nightside. Signatures of their …

The magnetosphere of an exoplanet has yet to be unambiguously detected. Investigations of
star–planet interaction and neutral atomic hydrogen absorption during transit to detect …