Area of research
Astronomy and Astrophysics · Instrumentation
Research interest
Research interests include Physics, Exoplanet, Planet, Astrophysics, Hot Jupiter, and Atmosphere (unit).
BOWIE-ALIGN: <i>JWST</i> reveals hints of planetesimal accretion and complex sulphur chemistry in the atmosphere of the misaligned hot Jupiter WASP-15b
Nightside clouds and disequilibrium chemistry on the hot Jupiter WASP-43b
A benchmark JWST near-infrared spectrum for the exoplanet WASP-39 b
Inhomogeneous terminators on the exoplanet WASP-39 b
BOWIE-ALIGN: how formation and migration histories of giant planets impact atmospheric compositions
BOWIE-ALIGN: A <i>JWST</i> comparative survey of aligned versus misaligned hot Jupiters to test the dependence of atmospheric composition on migration history
Early Release Science of the exoplanet WASP-39b with JWST NIRSpec PRISM
Early Release Science of the exoplanet WASP-39b with JWST NIRSpec G395H
Early Release Science of the exoplanet WASP-39b with JWST NIRCam
A JWST NIRSpec Phase Curve for WASP-121b: Dayside Emission Strongest Eastward of the Substellar Point and Nightside Conditions Conducive to Cloud Formation
Diurnal variations in the stratosphere of the ultrahot giant exoplanet WASP-121b
Transmission spectroscopy with VLT FORS2: a featureless spectrum for the low-density transiting exoplanet WASP-88b
Confirmation of water emission in the dayside spectrum of the ultrahot Jupiter WASP-121b
A library of self-consistent simulated exoplanet atmospheres
Idealised simulations of the deep atmosphere of hot Jupiters
The Limits of the Primitive Equations of Dynamics for Warm, Slowly Rotating Small Neptunes and Super Earths
The carbon-to-oxygen ratio: implications for the spectra of hydrogen-dominated exoplanet atmospheres
Acceleration of superrotation in simulated hot Jupiter atmospheres
An absolute sodium abundance for a cloud-free ‘hot Saturn’ exoplanet
The 3D Thermal, Dynamical, and Chemical Structure of the Atmosphere of HD 189733b: Implications of Wind-driven Chemistry for the Emission Phase Curve
Advection of Potential Temperature in the Atmosphere of Irradiated Exoplanets: A Robust Mechanism to Explain Radius Inflation
Results from a set of three-dimensional numerical experiments of a hot Jupiter atmosphere
Treatment of overlapping gaseous absorption with the correlated-<i>k</i>method in hot Jupiter and brown dwarf atmosphere models