A versatile multifluid HD/MHD code that runs on clusters of CPUs or GPUs, with special emphasis on protoplanetary disks.
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Updated
Sep 11, 2026 - C
A versatile multifluid HD/MHD code that runs on clusters of CPUs or GPUs, with special emphasis on protoplanetary disks.
Generate and manipulate semi-analytic models of planet wakes
Visualization library and CLI for protoplanetary disks simulations
A python package for processing and analyzing protostars/protoplanetary disks in FITS images.
DBNets is a ML-based tool for inferring the mass of putative gap-opening planets in protoplanetary discs. For more details read our paper at this link: https://doi.org/10.1051/0004-6361/202348421.
Interactive offline all-sky atlas of published images of circumstellar disks, directly imaged companions, and coronagraphic quasar hosts — 970+ systems, 4600+ image records, every image cited to its paper
Modeling Protoplanetary dust disk in the presence of a Giant Planet
Inferring the minimum-mass extrasolar nebula (MMEN) from SysSim
A framework to model stellar irradiated disks with frequency-dependent absorption and scattering opacities in Athena++ (Baronett, Jiang et al., in revision)
GPU-accelerated model for dust evolution in protoplanetary disks, with Lagrangian particle and Eulerian fluid solvers for NVIDIA and AMD GPUs
GitHub repository for my protoplanetary disk research at the University of Florida. This code utilizes FARGO3D and Zeus-2D code
A Python module for 2D and 3D pebble accretion in protoplanetary disks from TriPoDPy, based on Ormel (2017) and Drążkowska et al. (2023).
Production input and output files, data analysis and plotting notebooks, and high-performance-computing-related resources related to Baronett et al. (2024)
PLANAR: bias-aware unsupervised morphology discovery for protoplanetary disk observations (EXXA pipeline).
Editable and reproducible Quarto-based catalog of protoplanetary disks with educational astronomy and data science activities.
Search for substructures in protoplanetary disk with ALMA DSHARP data
Public FARGO3D with dust diffusion, beta cooling and the planet–disk setups of Yu, Li & Lee (2026).
Impact of different temperature profiles and disc-to-star mass ratios on the disk's surface density profile when it reaches equilibrium
Figure and source code for the Streaming Instability Code Comparison Project
Generate temperature-dependent dust opacities for RADMC-3D using Optool
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