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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 James Webb space telescope mission
JP Gardner, JC Mather, R Abbott, JS Abell… - Publications of the …, 2023 - iopscience.iop.org
We summarize the history, concept, scientific program, and technical performance of the
James Webb Space Telescope (JWST, Webb; Gardner et al. 2006). This paper points to and …
James Webb Space Telescope (JWST, Webb; Gardner et al. 2006). This paper points to and …
SO2, silicate clouds, but no CH4 detected in a warm Neptune
WASP-107b is a warm (approximately 740 K) transiting planet with a Neptune-like mass of
roughly 30.5 M⊕ and Jupiter-like radius of about 0.94 RJ (refs.,), whose extended …
roughly 30.5 M⊕ and Jupiter-like radius of about 0.94 RJ (refs.,), whose extended …
Dynamics and clouds in planetary atmospheres from telescopic observations
This review presents an insight into our current knowledge of the atmospheres of the planets
Venus, Mars, Jupiter, Saturn, Uranus and Neptune, the satellite Titan, and those of …
Venus, Mars, Jupiter, Saturn, Uranus and Neptune, the satellite Titan, and those of …
Sulfur dioxide in the mid-infrared transmission spectrum of WASP-39b
The recent inference of sulfur dioxide (SO2) in the atmosphere of the hot (approximately
1,100 K), Saturn-mass exoplanet WASP-39b from near-infrared JWST observations …
1,100 K), Saturn-mass exoplanet WASP-39b from near-infrared JWST observations …
[HTML][HTML] JWST-TST DREAMS: quartz clouds in the atmosphere of WASP-17b
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 …
date. For transiting exoplanets, we know if clouds are present because they mute spectral …
The Sonora substellar atmosphere models. IV. Elf Owl: atmospheric mixing and chemical disequilibrium with varying metallicity and C/O ratios
Disequilibrium chemistry due to vertical mixing in the atmospheres of many brown dwarfs
and giant exoplanets is well established. Atmosphere models for these objects typically …
and giant exoplanets is well established. Atmosphere models for these objects typically …
β Pictoris b through the eyes of the upgraded CRIRES+-Atmospheric composition, spin rotation, and radial velocity
Context. High-resolution spectrographs fed by adaptive optics (AO) provide a unique
opportunity to characterize directly imaged exoplanets. Observations with such instruments …
opportunity to characterize directly imaged exoplanets. Observations with such instruments …
The JWST Early Release Science Program for direct observations of exoplanetary systems I: High-contrast imaging of the exoplanet HIP 65426 b from 2 to 16 μm
Abstract We present JWST Early Release Science coronagraphic observations of the super-
Jupiter exoplanet, HIP 65426b, with the Near-Infrared Camera (NIRCam) from 2 to 5 μm …
Jupiter exoplanet, HIP 65426b, with the Near-Infrared Camera (NIRCam) from 2 to 5 μm …
JWST Measurements of 13C, 18O, and 17O in the Atmosphere of Super-Jupiter VHS 1256 b
S Gandhi, S de Regt, I Snellen, Y Zhang… - The Astrophysical …, 2023 - iopscience.iop.org
Isotope ratios have recently been measured in the atmospheres of directly imaged and
transiting exoplanets from ground-based observations. The arrival of JWST allows us to …
transiting exoplanets from ground-based observations. The arrival of JWST allows us to …