Generate and manipulate semi-analytic models of planet wakes

A versatile multifluid HD/MHD code that runs on clusters of CPUs or GPUs, with special emphasis on protoplanetary disks.

A python package for processing and analyzing protostars/protoplanetary disks in FITS images.

Modeling Protoplanetary dust disk in the presence of a Giant Planet

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.

Inferring the minimum-mass extrasolar nebula (MMEN) from SysSim

Production input and output files, data analysis and plotting notebooks, and high-performance-computing-related resources related to Baronett, et al. (2024).

Search for substructures in protoplanetary disk with ALMA DSHARP data

GitHub repository for my protoplanetary disk research at the University of Florida. This code utilizes FARGO3D and Zeus-2D code

Figure and source code for the Streaming Instability Code Comparison Project.

Impact of different temperature profiles and disc-to-star mass ratios on the disk's surface density profile when it reaches equilibrium

Turbulent convection in a vertical column of PPD

Generative_Image_Rotation: Using Pix2Pix cGAN to transform randomly oriented Protoplanetary Disk images into standardized face-on views for astronomical research.