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Treatment of overlapping gaseous absorption with the correlated-k method in hot Jupiter and brown dwarf atmosphere models

Astronomy and astrophysics (Berlin), 2017-02, Vol.598, p.A97

2017

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The UK Met Office global circulation model with a sophisticated radiation scheme applied to the hot Jupiter HD 209458b

Astronomy and astrophysics (Berlin), 2016-11, Vol.595, p.A36

2016

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Implications of three-dimensional chemical transport in hot Jupiter atmospheres: Results from a consistently coupled chemistry-radiation-hydrodynamics model

Astronomy and astrophysics (Berlin), 2020-04, Vol.636, p.A68

2020

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Confirmation of water emission in the dayside spectrum of the ultrahot Jupiter WASP-121b

Monthly notices of the Royal Astronomical Society, 2020-08, Vol.496 (2), p.1638-1644

2020

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Atmospheric Convection Plays a Key Role in the Climate of Tidally Locked Terrestrial Exoplanets: Insights from High-resolution Simulations

The Astrophysical journal, 2020-05, Vol.894 (2), p.84

2020

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The 3D Thermal, Dynamical, and Chemical Structure of the Atmosphere of HD 189733b: Implications of Wind-driven Chemistry for the Emission Phase Curve

The Astrophysical journal, 2018-12, Vol.869 (1), p.28

2018

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Accuracy tests of radiation schemes used in hot Jupiter global circulation models

Astronomy and astrophysics (Berlin), 2014-04, Vol.564, p.np-np

2014

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Results from a set of three-dimensional numerical experiments of a hot Jupiter atmosphere

Astronomy and astrophysics (Berlin), 2017-08, Vol.604, p.A79

2017

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Fully scalable forward model grid of exoplanet transmission spectra

Monthly notices of the Royal Astronomical Society, 2019-02, Vol.482 (4), p.4503-4513

2019

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Exploring the climate of Proxima B with the Met Office Unified Model

Astronomy and astrophysics (Berlin), 2017-05, Vol.601, p.A120

2017

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Observability of signatures of transport-induced chemistry in clear atmospheres of hot gas giant exoplanets

Monthly notices of the Royal Astronomical Society, 2023-02, Vol.519 (2), p.3129-3153

2023

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Mineral dust increases the habitability of terrestrial planets but confounds biomarker detection

Nature communications, 2020-06, Vol.11 (1), p.2731-2731, Article 2731

2020

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Stratospheric dayside-to-nightside circulation drives the 3D ozone distribution on synchronously rotating rocky exoplanets

Monthly notices of the Royal Astronomical Society, 2023-11, Vol.526 (1), p.263-278

2023

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The carbon-to-oxygen ratio: implications for the spectra of hydrogen-dominated exoplanet atmospheres

Monthly notices of the Royal Astronomical Society, 2019-06, Vol.486 (1), p.1123-1137

2019

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TRAPPIST-1 Habitable Atmosphere Intercomparison (THAI): motivations and protocol version 1.0

Geoscientific Model Development, 2020-02, Vol.13 (2), p.707-716

2020

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The Impact of the Explicit Representation of Convection on the Climate of a Tidally Locked Planet in Global Stretched-mesh Simulations

The Astrophysical journal, 2024-07, Vol.970 (1), p.7

2024

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The Influence of a Substellar Continent on the Climate of a Tidally Locked Exoplanet

The Astrophysical journal, 2018-02, Vol.854 (2), p.171

2018

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Solar-to-supersolar sodium and oxygen absolute abundances for a ‘hot Saturn’ orbiting a metal-rich star

Monthly notices of the Royal Astronomical Society, 2022-08, Vol.515 (2), p.3037-3058

2022

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Lightning-induced chemistry on tidally-locked Earth-like exoplanets

Monthly notices of the Royal Astronomical Society, 2022-10, Vol.517 (2), p.2383-2402

2022

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The unified model, a fully-compressible, non-hydrostatic, deep atmosphere global circulation model, applied to hot Jupiters: ENDGame for a HD 209458b test case

Astronomy and astrophysics (Berlin), 2014-01, Vol.561, p.np-np

2014

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A JWST NIRSpec Phase Curve for WASP-121b: Dayside Emission Strongest Eastward of the Substellar Point and Nightside Conditions Conducive to Cloud Formation

Astrophysical journal. Letters, 2023-02, Vol.943 (2), p.L17

2023

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Shallow-water modelling of the atmospheric circulation regimes of brown dwarfs and their observable features

Monthly notices of the Royal Astronomical Society, 2023-08, Vol.525 (1), p.150-163

2023

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Longitudinally Asymmetric Stratospheric Oscillation on a Tidally Locked Exoplanet

The Astrophysical journal, 2022-05, Vol.930 (2), p.152

2022

Volltextzugriff (PDF)

Ground-based transmission spectroscopy with FORS2: A featureless optical transmission spectrum and detection of H2O for the ultra-hot Jupiter WASP-103b

Monthly notices of the Royal Astronomical Society, 2020-10, Vol.497 (4), p.5155-5170

2020

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Implications of different stellar spectra for the climate of tidally locked Earth-like exoplanets

Astronomy and astrophysics (Berlin), 2020-07, Vol.639, p.A99

2020

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Treatment of overlapping gaseous absorption with the correlated-k method in hot Jupiter and brown dwarf atmosphere models

The UK Met Office global circulation model with a sophisticated radiation scheme applied to the hot Jupiter HD 209458b

Implications of three-dimensional chemical transport in hot Jupiter atmospheres: Results from a consistently coupled chemistry-radiation-hydrodynamics model

Confirmation of water emission in the dayside spectrum of the ultrahot Jupiter WASP-121b

Atmospheric Convection Plays a Key Role in the Climate of Tidally Locked Terrestrial Exoplanets: Insights from High-resolution Simulations

The 3D Thermal, Dynamical, and Chemical Structure of the Atmosphere of HD 189733b: Implications of Wind-driven Chemistry for the Emission Phase Curve

Accuracy tests of radiation schemes used in hot Jupiter global circulation models

Results from a set of three-dimensional numerical experiments of a hot Jupiter atmosphere

Fully scalable forward model grid of exoplanet transmission spectra

Exploring the climate of Proxima B with the Met Office Unified Model

Observability of signatures of transport-induced chemistry in clear atmospheres of hot gas giant exoplanets

Mineral dust increases the habitability of terrestrial planets but confounds biomarker detection

Stratospheric dayside-to-nightside circulation drives the 3D ozone distribution on synchronously rotating rocky exoplanets

The carbon-to-oxygen ratio: implications for the spectra of hydrogen-dominated exoplanet atmospheres

TRAPPIST-1 Habitable Atmosphere Intercomparison (THAI): motivations and protocol version 1.0

The Impact of the Explicit Representation of Convection on the Climate of a Tidally Locked Planet in Global Stretched-mesh Simulations

The Influence of a Substellar Continent on the Climate of a Tidally Locked Exoplanet

Solar-to-supersolar sodium and oxygen absolute abundances for a ‘hot Saturn’ orbiting a metal-rich star

Lightning-induced chemistry on tidally-locked Earth-like exoplanets

The unified model, a fully-compressible, non-hydrostatic, deep atmosphere global circulation model, applied to hot Jupiters: ENDGame for a HD 209458b test case

A JWST NIRSpec Phase Curve for WASP-121b: Dayside Emission Strongest Eastward of the Substellar Point and Nightside Conditions Conducive to Cloud Formation

Shallow-water modelling of the atmospheric circulation regimes of brown dwarfs and their observable features

Longitudinally Asymmetric Stratospheric Oscillation on a Tidally Locked Exoplanet

Ground-based transmission spectroscopy with FORS2: A featureless optical transmission spectrum and detection of H2O for the ultra-hot Jupiter WASP-103b

Implications of different stellar spectra for the climate of tidally locked Earth-like exoplanets

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