Generate and manipulate semi-analytic models of planet wakes
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Updated
Oct 8, 2024 - Python
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).
GitHub repository for my protoplanetary disk research at the University of Florida. This code utilizes FARGO3D and Zeus-2D code
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.
Project and source files related to the Streaming Instability Code Comparison (SICC) Project led by PFITS+ and the UFOS Project.
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