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A benchmark companion at the hydrogen-burning limit imaged in the core cluster of the Fornax-Horologium association
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Hidden under a warm blanket: If planets existed in protostellar disks, they would hardly produce observable substructures
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A precise metallicity and carbon-to-oxygen ratio for a warm giant exoplanet from its panchromatic JWST emission spectrum
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Metallicity Regulates Planet Formation across All Masses
Locked in ice: how pebble drift and volatile entrapment can significantly impact carbon and oxygen ratios in evolving protoplanetary discs
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Searching for Giant Exoplanets around M-dwarf Stars (GEMS) I: Survey Motivation
Shubham Kanodia, Caleb I. Cañas, Suvrath Mahadevan, Eric B. Ford, Ravit Helled, Dana E. Anderson, Alan Boss, William D. Cochran, Megan Delamer, Te Han, Jessica E. Libby-Roberts, Andrea S. J. Lin, Simon Müller, Paul Robertson, Gumundur Stefánsson and Johanna Teske The Astronomical Journal 167(4) 161 (2024) https://doi.org/10.3847/1538-3881/ad27cb
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Population synthesis models indicate a need for early and ubiquitous disk substructures
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Which stars can form planets: Planetesimal formation at low metallicities
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How external photoevaporation changes the chemical composition of the inner disc
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Mind the gap: Distinguishing disc substructures and their impact on the inner disc composition
A fading radius valley towards M dwarfs, a persistent density valley across stellar types
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A Recipe for Eccentricity and Inclination Damping for Partial-gap Opening Planets in 3D Disks