Hot Jupiters: origins, structure, atmospheres
JJ Fortney, RI Dawson… - Journal of Geophysical …, 2021 - Wiley Online Library
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 …
to cover most of the major areas of current study while providing the reader with additional …
Atmospheric dynamics of hot giant planets and brown dwarfs
AP Showman, X Tan, V Parmentier - Space Science Reviews, 2020 - Springer
Groundbased and spacecraft telescopic observations, combined with an intensive modeling
effort, have greatly enhanced our understanding of hot giant planets and brown dwarfs over …
effort, have greatly enhanced our understanding of hot giant planets and brown dwarfs over …
The cloudy shape of hot Jupiter thermal phase curves
V Parmentier, AP Showman… - Monthly Notices of the …, 2021 - academic.oup.com
Hot Jupiters have been predicted to have a strong day/night temperature contrast and a
hotspot shifted eastward of the substellar point. This was confirmed by numerous phase …
hotspot shifted eastward of the substellar point. This was confirmed by numerous phase …
Transiting exoplanet atmospheres in the era of JWST
EMR Kempton, HA Knutson - Reviews in Mineralogy …, 2024 - pubs.geoscienceworld.org
The field of exoplanet atmospheric characterization has recently made considerable
advances with the advent of high-resolution spectroscopy from large ground-based …
advances with the advent of high-resolution spectroscopy from large ground-based …
The atmospheric circulation of ultra-hot Jupiters
X Tan, TD Komacek - The Astrophysical Journal, 2019 - iopscience.iop.org
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 …
have found evidence for new physical processes at play in their atmospheres. In this work …
New mass and radius constraints on the LHS 1140 planets: LHS 1140 b is either a temperate mini-Neptune or a water world
The two-planet transiting system LHS 1140 has been extensively observed since its
discovery in 2017, notably with Spitzer, HST, TESS, and ESPRESSO, placing strong …
discovery in 2017, notably with Spitzer, HST, TESS, and ESPRESSO, placing strong …
Eureka!: an end-to-end pipeline for JWST time-series observations
$\texttt {Eureka!} $ is a data reduction and analysis pipeline for exoplanet time-series
observations, with a particular focus on JWST data. Over the next 1-2 decades, JWST will …
observations, with a particular focus on JWST data. Over the next 1-2 decades, JWST will …
Carbon monoxide emission lines reveal an inverted atmosphere in the ultra hot Jupiter WASP-33 b consistent with an eastward hot spot
L van Sluijs, JL Birkby, J Lothringer… - Monthly Notices of …, 2023 - academic.oup.com
We report the first detection of CO emission at high spectral resolution in the day-side
infrared thermal spectrum of an exoplanet. These emission lines, found in the atmosphere of …
infrared thermal spectrum of an exoplanet. These emission lines, found in the atmosphere of …
Climate of an ultra hot Jupiter-Spectroscopic phase curve of WASP-18b with HST/WFC3
J Arcangeli, JM Désert, V Parmentier… - Astronomy & …, 2019 - aanda.org
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 …
(UHJ) WASP-18b, obtained with the Wide Field Camera 3 aboard the Hubble Space …
Transit signatures of inhomogeneous clouds on hot Jupiters: insights from microphysical cloud modeling
We determine the observability in transmission of inhomogeneous cloud cover on the limbs
of hot Jupiters through post-processing a general circulation model to include cloud …
of hot Jupiters through post-processing a general circulation model to include cloud …