Anatomy of rocky planets formed by rapid pebble accretion I. How icy pebbles determine the core fraction and FeO contents

Constraining planetary mass-loss rates by simulating Parker wind profiles with Cloudy (Corrigendum)

The K2 and TESS Synergy. II. Revisiting 26 Systems in the TESS Primary Mission

Magnetic activity variability from Hα line intensive monitoring of two F-type stars with a hot Jupiter, τ Bootis A and υ Andromedae A

The origin of free-floating planets

Assessing the spin-orbit obliquity of low-mass planets in the breaking the chain formation model: A story of misalignment

Hot Exoplanet Atmospheres Resolved with Transit Spectroscopy (HEARTS) VIII. Nondetection of sodium in the atmosphere of the aligned planet KELT-10b

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