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 …
Multiple Clues for Dayside Aerosols and Temperature Gradients in WASP-69 b from a Panchromatic JWST Emission Spectrum
WASP-69 b is a hot, inflated, Saturn-mass planet (0.26 M Jup) with a zero-albedo
equilibrium temperature of 963 K. Here, we report the JWST 2–12 μm emission spectrum of …
equilibrium temperature of 963 K. Here, we report the JWST 2–12 μm emission spectrum of …
[HTML][HTML] Patchy nightside clouds on ultra-hot Jupiters: general circulation model simulations with radiatively active cloud tracers
The atmospheres of ultra-hot Jupiters have been characterized in detail through recent
phase curve and low-and high-resolution emission and transmission spectroscopic …
phase curve and low-and high-resolution emission and transmission spectroscopic …
The Possible Tidal Demise of Kepler's First Planetary System
S Vissapragada, A Chontos… - The Astrophysical …, 2022 - iopscience.iop.org
We present evidence of tidally-driven inspiral in the Kepler-1658 (KOI-4) system, which
consists of a giant planet (1.1RJ, 5.9MJ) orbiting an evolved host star (2.9R⊙, 1.5M⊙) …
consists of a giant planet (1.1RJ, 5.9MJ) orbiting an evolved host star (2.9R⊙, 1.5M⊙) …
The geometric albedo of the hot Jupiter HD 189733b measured with CHEOPS
AF Krenn, M Lendl, JA Patel, L Carone… - Astronomy & …, 2023 - aanda.org
Context. Measurements of the occultation of an exoplanet at visible wavelengths allow us to
determine the reflective properties of a planetary atmosphere. The observed occultation …
determine the reflective properties of a planetary atmosphere. The observed occultation …
Cloudy and cloud-free thermal phase curves with picaso: Applications to wasp-43b
N Robbins-Blanch, T Kataria, NE Batalha… - The Astrophysical …, 2022 - iopscience.iop.org
We present new functionality within PICASO, a state-of-the-art radiative transfer model for
exoplanet and brown dwarf atmospheres, by developing a new pipeline that computes …
exoplanet and brown dwarf atmospheres, by developing a new pipeline that computes …
Modelling the day–night temperature variations of ultra-hot Jupiters: confronting non-grey general circulation models and observations
ABSTRACT Ultra-hot Jupiters (UHJs) are natural laboratories to study extreme physics in
planetary atmospheres and their rich observational data sets are yet to be confronted with …
planetary atmospheres and their rich observational data sets are yet to be confronted with …
Yunma: Enabling spectral retrievals of exoplanetary clouds
In this paper, we present YunMa, an exoplanet cloud simulation and retrieval package,
which enables the study of cloud microphysics and radiative properties in exoplanetary …
which enables the study of cloud microphysics and radiative properties in exoplanetary …
Emergent spectral fluxes of hot Jupiters: an abrupt rise in dayside brightness temperature under strong irradiation
We study the emergent spectral fluxes of transiting hot Jupiters, using secondary eclipses
from Spitzer. To achieve a large and uniform sample, we have reanalyzed all secondary …
from Spitzer. To achieve a large and uniform sample, we have reanalyzed all secondary …
Modeling Atmospheric Lines by the Exoplanet Community (MALBEC) version 1.0: A CUISINES radiative transfer intercomparison project
Radiative transfer (RT) models are critical in the interpretation of exoplanetary spectra, in
simulating exoplanet climates, and when designing the specifications of future flagship …
simulating exoplanet climates, and when designing the specifications of future flagship …