activity
20182026
most citedPhotochemically-produced SO in the atmosphere of WASP-39b

262 citations · 1.2k across the 64 of their papers we have counts for

collaborators
Showing 2023Show all

10 papers · 1 filter

astro-ph.EP2023★ 1 cited

Spatially resolving the volatile sulfur abundance in the HD 100546 protoplanetary disk

Luke Keyte, Mihkel Kama, Ko-Ju Chuang +5

Volatile elements play a crucial role in the formation of planetary systems. Their abundance and distribution in protoplanetary disks provide vital insights into the connection bet…

astro-ph.EP2023★ 5 cited

The distribution of impactor core material during large impacts on Earth-like planets

Jonathan P. Itcovitz, Auriol S. P. Rae, Thomas M. Davison +2

Large impacts onto young rocky planets may transform their compositions, creating highly reducing conditions at their surfaces and reintroducing highly siderophile metals to their…

astro-ph.EP2023

Atmospheres as a Window to Rocky Exoplanet Surfaces

Xander Byrne, Oliver Shorttle, Sean Jordan +1

As the characterization of exoplanet atmospheres proceeds, providing insights into atmospheric chemistry and composition, a key question is how much deeper into the planet we might…

astro-ph.EP2023

Phanerozoic biological reworking of the continental carbonate rock reservoir

Craig R. Walton, Oliver Shorttle

Understanding the co-evolution of complex life with Earth's geology is an enduring challenge. The rock record evidences remarkable correlations between changes in biology and the w…

astro-ph.EP2023★ 6 cited

Post-main sequence thermal evolution of planetesimals

Yuqi Li, Amy Bonsor, Oliver Shorttle

White dwarfs that have accreted planetary materials provide a powerful tool to probe the interiors and formation of exoplanets. In particular, the high Fe/Si ratio of some white dw…

astro-ph.EP2023★ 22 cited

A mineralogical reason why all exoplanets cannot be equally oxidising

Claire Marie Guimond, Oliver Shorttle, Sean Jordan +1

From core to atmosphere, the oxidation states of elements in a planet shape its character. Oxygen fugacity (fO) is one parameter indicating these likely oxidation states. The o…

astro-ph.EP2023★ 17 cited

Prebiosignature Molecules Can Be Detected in Temperate Exoplanet Atmospheres with JWST

Alastair Claringbold, Paul Rimmer, Sarah Rugheimer +1

The search for biosignatures on exoplanets connects the fields of biology and biochemistry to astronomical observation, with the hope that we might detect evidence of active biolog…

physics.ao-ph2023★ 7 cited

Avoiding methane emission rate underestimates when using the divergence method

Clayton Roberts, Rutger IJzermans, David Randell +5

Methane is a powerful greenhouse gas, and a primary target for mitigating climate change in the short-term future due to its relatively short atmospheric lifetime and greater abili…

astro-ph.EP2023★ 20 cited

Large Interferometer For Exoplanets (LIFE): IX. Assessing the Impact of Clouds on Atmospheric Retrievals at Mid-Infrared Wavelengths with a Venus-Twin Exoplanet

B. S. Konrad, E. Alei, S. P. Quanz +10

The Large Interferometer For Exoplanets (LIFE) initiative aims to develop a space based mid-infrared (MIR) nulling interferometer to measure the thermal emission spectra of tempera…

astro-ph.EP2023★ 1 cited

Azimuthal C/O Variations in a Planet-Forming Disk

Luke Keyte, Mihkel Kama, Alice S. Booth +8

The elemental carbon-to-oxygen ratio (C/O) in the atmosphere of a giant planet is a promising diagnostic of that planet's formation history in a protoplanetary disk. Alongside effo…