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

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).

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.

Search for substructures in protoplanetary disk with ALMA DSHARP data

Turbulent convection in a vertical column of PPD

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

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