Stellar obliquities in exoplanetary systems
The rotation of a star and the revolutions of its planets are not necessarily aligned. This
article reviews the measurement techniques, key findings, and theoretical interpretations …
article reviews the measurement techniques, key findings, and theoretical interpretations …
Origins of hot Jupiters
RI Dawson, JA Johnson - Annual Review of Astronomy and …, 2018 - annualreviews.org
Hot Jupiters were the first exoplanets to be discovered around main sequence stars and
astonished us with their close-in orbits. They are a prime example of how exoplanets have …
astonished us with their close-in orbits. They are a prime example of how exoplanets have …
Five carbon-and nitrogen-bearing species in a hot giant planet's atmosphere
P Giacobbe, M Brogi, S Gandhi, PE Cubillos… - Nature, 2021 - nature.com
The atmospheres of gaseous giant exoplanets orbiting close to their parent stars (hot
Jupiters) have been probed for nearly two decades,. They allow us to investigate the …
Jupiters) have been probed for nearly two decades,. They allow us to investigate the …
A broadband thermal emission spectrum of the ultra-hot Jupiter WASP-18b
Close-in giant exoplanets with temperatures greater than 2,000 K ('ultra-hot Jupiters') have
been the subject of extensive efforts to determine their atmospheric properties using thermal …
been the subject of extensive efforts to determine their atmospheric properties using thermal …
TESS transit timing of hundreds of hot Jupiters
We provide a database of transit times and updated ephemerides for 382 planets based on
data from the NASA Transiting Exoplanet Survey Satellite (TESS) and previously reported …
data from the NASA Transiting Exoplanet Survey Satellite (TESS) and previously reported …
The orbit of WASP-12b is decaying
WASP-12b is a transiting hot Jupiter on a 1.09 day orbit around a late-F star. Since the
planet's discovery in 2008, the time interval between transits has been decreasing by 29±2 …
planet's discovery in 2008, the time interval between transits has been decreasing by 29±2 …
Empirical limb-darkening coefficients and transit parameters of known exoplanets from TESS
Although the main goal of the Transiting Exoplanet Survey Satellite (TESS) is to search for
new transiting exoplanets, its data can also be used to study already-known systems in …
new transiting exoplanets, its data can also be used to study already-known systems in …
A preponderance of perpendicular planets
Abstract Observing the Rossiter–McLaughlin effect during a planetary transit allows the
determination of the angle λ between the sky projections of the star's spin axis and the …
determination of the angle λ between the sky projections of the star's spin axis and the …
A Combined Ground-based and JWST Atmospheric Retrieval Analysis: Both IGRINS and NIRSpec Agree that the Atmosphere of WASP-77A b Is Metal-poor
Ground-based high-resolution and space-based low-resolution spectroscopy are the two
main avenues through which transiting exoplanet atmospheres are studied. Both methods …
main avenues through which transiting exoplanet atmospheres are studied. Both methods …
DREAM-III. A helium survey in exoplanets on the edge of the hot Neptune desert with GIANO-B at TNG
G Guilluy, V Bourrier, Y Jaziri, W Dethier… - Astronomy & …, 2023 - aanda.org
Context. The population of close-in exoplanets features a desert of hot Neptunes whose
origin remains uncertain. These planets may have lost their atmosphere, eroding into mini …
origin remains uncertain. These planets may have lost their atmosphere, eroding into mini …