Early Release Science of the exoplanet WASP-39b with JWST NIRSpec PRISM
Transmission spectroscopy,–of exoplanets has revealed signatures of water vapour,
aerosols and alkali metals in a few dozen exoplanet atmospheres,. However, these previous …
aerosols and alkali metals in a few dozen exoplanet atmospheres,. However, these previous …
[HTML][HTML] The HITRAN2020 molecular spectroscopic database
IE Gordon, LS Rothman, RJ Hargreaves… - Journal of quantitative …, 2022 - Elsevier
The HITRAN database is a compilation of molecular spectroscopic parameters. It was
established in the early 1970s and is used by various computer codes to predict and …
established in the early 1970s and is used by various computer codes to predict and …
[HTML][HTML] The 2024 release of the ExoMol database: molecular line lists for exoplanet and other hot atmospheres
The ExoMol database (www. exomol. com) provides molecular data for spectroscopic
studies of hot atmospheres. These data are widely used to model atmospheres of …
studies of hot atmospheres. These data are widely used to model atmospheres of …
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 …
Retrieving scattering clouds and disequilibrium chemistry in the atmosphere of HR 8799e
P Mollière, T Stolker, S Lacour, G Otten… - Astronomy & …, 2020 - aanda.org
Context. Clouds are ubiquitous in exoplanet atmospheres and they represent a challenge
for the model interpretation of their spectra. When generating a large number of model …
for the model interpretation of their spectra. When generating a large number of model …
Hot exoplanetary atmospheres in 3D
W Pluriel - Remote Sensing, 2023 - mdpi.com
Hot giant exoplanets are very exotic objects with no equivalent in the Solar System that
allow us to study the behavior of atmospheres under extreme conditions. Their thermal and …
allow us to study the behavior of atmospheres under extreme conditions. Their thermal and …
Detecting exomoons from radial velocity measurements of self-luminous planets: application to observations of HR 7672 B and future prospects
The detection of satellites around extrasolar planets, so called exomoons, remains a largely
unexplored territory. In this work, we study the potential of detecting these elusive objects …
unexplored territory. In this work, we study the potential of detecting these elusive objects …
The 13CO-rich atmosphere of a young accreting super-Jupiter
Y Zhang, IAG Snellen, AJ Bohn, P Mollière, C Ginski… - Nature, 2021 - nature.com
Isotope abundance ratios have an important role in astronomy and planetary sciences,
providing insights into the origin and evolution of the Solar System, interstellar chemistry and …
providing insights into the origin and evolution of the Solar System, interstellar chemistry and …
[HTML][HTML] Atmospheric Rossiter–McLaughlin effect and transmission spectroscopy of WASP-121b with ESPRESSO
F Borsa, R Allart, N Casasayas-Barris… - Astronomy & …, 2021 - aanda.org
Context. Ultra-hot Jupiters are excellent laboratories for the study of exoplanetary
atmospheres. WASP-121b is one of the most studied; many recent analyses of its …
atmospheres. WASP-121b is one of the most studied; many recent analyses of its …
An atomic spectral survey of WASP-76b: resolving chemical gradients and asymmetries
AY Kesseli, IAG Snellen… - The Astronomical …, 2022 - iopscience.iop.org
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 …
locked, causing a permanent hot dayside and a cooler nightside. Signatures of their …