Small, cool and sulfurous exoplanet may help write recipe for planetary formation

Watery planets orbiting dead stars may be good candidates for studying life—if they can survive long enough

NGTS-30b/TOI-4862b: An ~1 Gyr old 98-day transiting warm Jupiter

Fundamental effective temperature measurements for eclipsing binary stars – V. The circumbinary planet system EBLM J0608−59

Buoyancy torques prevent low-mass planets from stalling in low-turbulence radiative disks

The CUISINES Framework for Conducting Exoplanet Model Intercomparison Projects, Version 1.0

High-resolution transmission spectroscopy of warm Jupiters: An ESPRESSO sample with predictions for ANDES

Constraints on the formation history and composition of Kepler planets from their distribution of orbital period ratios

A formation pathway for terrestrial planets with moderate water content involving atmospheric-volatile recycling

Probing atmospheric escape through metastable He I triplet lines in 15 exoplanets observed with SPIRou

Different Planetary Eccentricity-Period (PEP) Distributions of Small- and Giant-Planets

More Likely Than You Think: Inclination-Driving Secular Resonances are Common in Known Exoplanet Systems

What no one has seen before: gravitational waveforms from warp drive collapse

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