activity
20162025
most citedHO abundances and cloud properties in ten hot giant exoplanets

216 citations · 2.3k across the 38 of their papers we have counts for

collaborators
Showing 2025Show all

5 papers · 1 filter

astro-ph.IM2025

Direct imaging characterization of cool gaseous planets

Michiel Min, Jo Barstow, Laura C. Mayorga +19

Cool gas giant exoplanets, particularly those with properties similar to those of Jupiter and Saturn, remain poorly characterized due to current observational limitations. This whi…

astro-ph.EP2025

Astroclimes -- measuring the abundance of CO and CH in the Earth's atmosphere using astronomical observations

Marcelo Aron Fetzner Keniger, David Armstrong, Matteo Brogi +2

Monitoring the abundance of greenhouse gases (GHGs) such as carbon dioxide (CO) and methane (CH) is necessary to quantify their impact on global warming and climate change.…

astro-ph.EP2025

The Roasting Marshmallows Program with IGRINS on Gemini South III: Seeing deeper into the metal depleted atmosphere of a gas-giant on the cusp of the hot to ultra-hot Jupiter transition

Vatsal Panwar, Matteo Brogi, Krishna Kanumalla +17

Ultra-hot Jupiters are a class of gas-giant exoplanets that show a peculiar combination of thermochemical properties in the form of molecular dissociation, atomic ionization, and i…

astro-ph.EP2025★ 13 cited

Tracing the formation and migration history: molecular signatures in the atmosphere of misaligned hot Jupiter WASP-94Ab using JWST NIRSpec/G395H

Eva-Maria Ahrer, Siddharth Gandhi, Lili Alderson +12

The discovery of hot Jupiters that orbit very close to their host stars has long challenged traditional models of planetary formation and migration. Characterising their atmospheri…

astro-ph.EP2025

Detectability of oxygen fugacity regimes in the magma ocean world 55 Cancri e at high spectral resolution

Spandan Dash, Matteo Brogi, Fabian Lukas Seidler +5

Ultra-short Period exoplanets (USPs) like 55 Cnc e, hosting dayside magma oceans, present unique opportunities to study surface-atmosphere interactions. The composition of a vapori…