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- 2017
- The role of pebble fragmentation in planetesimal formation II. Numerical simulations
- Initial mass function of planetesimals formed by the streaming instability
- Concentrating small particles in protoplanetary disks through the streaming instability
- Breaking the chains : Hot super-Earth systems from migration and disruption of compact resonant chains
- Radially resolved simulations of collapsing pebble clouds in protoplanetary discs
- The unstable fate of the planet orbiting the A star in the HD 131399 triple stellar system
- 2016
- Dark matter cores all the way down
- Spontaneous concentrations of solids through two-way drag forces between gas and sedimenting particles
- THE AGORA HIGH-RESOLUTION GALAXY SIMULATIONS COMPARISON PROJECT. II. ISOLATED DISK TEST
- Full-lifetime simulations of multiple unequal-mass planets across all phases of stellar evolution