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Cited article:

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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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The Evolution of Disk Winds from a Combined Study of Optical and Infrared Forbidden Lines

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Unified Simulations of Planetary Formation and Atmospheric Evolution: Effects of Pebble Accretion, Giant Impacts, and Stellar Irradiation on Super-Earth Formation

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The Astrophysical Journal 892 (2) 124 (2020)
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Breaking Resonant Chains: Destabilization of Resonant Planets Due to Long-term Mass Evolution

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Near mean motion resonance of terrestrial planet pair induced by giant planet: application to Kepler-68 system

Jianghui Ji, Su Wang and Mengrui Pan
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Sub-Neptune formation: the view from resonant planets

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Most super-Earths formed by dry pebble accretion are less massive than 5 Earth masses

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Close-in Super-Earths: The first and the last stages of planet formation in an MRI-accreting disc

Marija R Jankovic, James E Owen and Subhanjoy Mohanty
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Time-dependent evolution of the protoplanetary discs with magnetic winds

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Monthly Notices of the Royal Astronomical Society 488 (4) 4623 (2019)
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Formation of planetary systems by pebble accretion and migration

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Astronomy & Astrophysics 627 A83 (2019)
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Formation of the terrestrial planets in the solar system around 1 au via radial concentration of planetesimals

Masahiro Ogihara, Eiichiro Kokubo, Takeru K. Suzuki and Alessandro Morbidelli
Astronomy & Astrophysics 612 L5 (2018)
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A balanced budget view on forming giant planets by pebble accretion

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