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Unified Simulations of Planetary Formation and Atmospheric Evolution. II. Rapid Disk Clearing by Photoevaporation Yields Low-mass Super-Earth Atmospheres

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Dust Pileup at the Dead-zone Inner Edge and Implications for the Disk Shadow

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Constraining the Formation of the Four Terrestrial Planets in the Solar System

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Formation of Giant Planet Satellites

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Subsolar Al/Si and Mg/Si ratios of non-carbonaceous chondrites reveal planetesimal formation during early condensation in the protoplanetary disk

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Formation of planetary systems by pebble accretion and migration

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Formation of close-in super-Earths in evolving protoplanetary disks due to disk winds

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