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Cited article:

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Radial distribution of giant exoplanets at Solar System scales

A.-M. Lagrange, F. Philipot, P. Rubini, N. Meunier, F. Kiefer, P. Kervella, P. Delorme and H. Beust
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N-body simulation of planetary formation through pebble accretion in a radially structured protoplanetary disk

Tenri Jinno, Takayuki R Saitoh, Yota Ishigaki and Junichiro Makino
Publications of the Astronomical Society of Japan 75 (5) 951 (2023)
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Early Water Delivery to Terrestrial Planet Regions during the Stages of Jupiter’s Formation and Migration in the Grand Tack Model

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Combined effects of disc winds and turbulence-driven accretion on planet populations

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How the planetary eccentricity influences the pebble isolation mass

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A New Third Planet and the Dynamical Architecture of the HD 33142 Planetary System*

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Flux-limited Diffusion Approximation Models of Giant Planet Formation by Disk Instability. II. Quadrupled Spatial Resolution

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