activity
20182025
most citedPhotochemically-produced SO in the atmosphere of WASP-39b

262 citations · 361 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph.EP2025

The Impact of Different Haze Types on the Atmosphere and Observations of Hot Jupiters: 3D Simulations of HD 189733b, HD209458b and WASP-39b

Mei Ting Mak, Denis Sergeev, Nathan Mayne +6

We present the results from the simulations of the atmospheres of hot-Jupiters HD189733b, HD209458b and WASP-39b, assuming the presence of three different types of haze. Using a 3D…

astro-ph.EP2025★ 7 cited

Cloudy mornings and clear evenings on a gas giant exoplanet

Sagnick Mukherjee, David K. Sing, Guangwei Fu +25

The spectra of exoplanet atmospheres are affected by aerosols (clouds and hazes) of uncertain origin. Proposed aerosol formation mechanisms include gas condensation or photochemica…

astro-ph.EP2024

Biosignatures from pre-oxygen photosynthesising life on TRAPPIST-1e

Jake K. Eager-Nash, Stuart J. Daines, James W. McDermott +13

In order to assess observational evidence for potential atmospheric biosignatures on exoplanets, it will be essential to test whether spectral fingerprints from multiple gases can…

astro-ph.EP2024★ 10 cited

3D simulations of TRAPPIST-1e with varying CO2, CH4 and haze profiles

Mei Ting Mak, Denis Sergeev, Nathan Mayne +6

Using a 3D General Circulation Model, the Unified Model, we present results from simulations of a tidally-locked TRAPPIST-1e with varying carbon dioxide CO2 and methane CH4 gas con…

astro-ph.EP2023★ 13 cited

3D simulations of the Archean Earth including photochemical haze profiles

M. T. Mak, N. J. Mayne, D. E. Sergeev +5

We present results from 3D simulations of the Archean Earth including a prescribed (non-interactive) spherical haze generated through a 1D photochemical model. Our simulations sugg…

astro-ph.EP2022★ 262 cited

Photochemically-produced SO in the atmosphere of WASP-39b

Shang-Min Tsai, Elspeth K. H. Lee, Diana Powell +82

Photochemistry is a fundamental process of planetary atmospheres that regulates the atmospheric composition and stability. However, no unambiguous photochemical products have been…

astro-ph.EP2018★ 69 cited

Observable signatures of wind--driven chemistry with a fully consistent three dimensional radiative hydrodynamics model of HD 209458b

Benjamin Drummond, N. J. Mayne, James Manners +8

We present a study of the effect of wind-driven advection on the chemical composition of hot Jupiter atmospheres using a fully-consistent 3D hydrodynamics, chemistry and radiative…