activity
20192024
most citedEquatorial anti-rotating day side wind flow in WASP-43b elicited by deep wind jets?

79 citations · 318 across the 9 of their papers we have counts for

collaborators

9 papers

astro-ph.EP2024★ 3 cited

From CO- to HO-dominated atmospheres and back -- How mixed outgassing changes the volatile distribution in magma oceans around M dwarf stars

Ludmila Carone, Rory Barnes, Lena Noack +7

We investigate the impact of CO on TRAPPIST-1 e, f and g during the magma ocean stage. These potentially habitable rocky planets are currently the most accessible for astronomi…

astro-ph.EP2024

The effect of lightning on the atmospheric chemistry of exoplanets and potential biosignatures

Patrick Barth, Eva E. Stüeken, Christiane Helling +2

Lightning has been suggested to play a role in triggering the occurrence of bio-ready chemical species. Future missions (PLATO, ARIEL, HWO, LIFE) and ground-based ELTs will investi…

physics.geo-ph2023★ 46 cited

Isotopic constraints on lightning as a source of fixed nitrogen in Earth's early biosphere

Patrick Barth, Eva E. Stüeken, Christiane Helling +4

Bioavailable nitrogen is thought to be a requirement for the origin and sustenance of life. Before the onset of biological nitrogen fixation, abiotic pathways to fix atmospheric N2…

astro-ph.EP2023★ 12 cited

The energetic particle environment of a GJ 436 b-like planet

D. Rodgers-Lee, P. B. Rimmer, A. A. Vidotto +8

A key first step to constrain the impact of energetic particles in exoplanet atmospheres is to detect the chemical signature of ionisation due to stellar energetic particles and Ga…

astro-ph.EP2021★ 43 cited

An upper limit on late accretion and water delivery in the Trappist-1 exoplanet system

Sean N. Raymond, Andre Izidoro, Emeline Bolmont +9

The Trappist-1 system contains seven roughly Earth-sized planets locked in a multi-resonant orbital configuration, which has enabled precise measurements of the planets' masses and…

astro-ph.EP2020★ 27 cited

Coexistence of CH4, CO2 and H2O in exoplanet atmospheres

P. Woitke, O. Herbort, Ch. Helling +4

We propose a classification of exoplanet atmospheres based on their H, C, O, N element abundances below about 600 K. Chemical equilibrium models were run for all combinations of H,…