The Galacticus galaxy formation model
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Updated
Jun 10, 2024 - Fortran
The Galacticus galaxy formation model
Datasets for the Galacticus galaxy formation model
MCFOST radiative transfer code
Phantom Smoothed Particle Hydrodynamics and Magnetohydrodynamics code
Pulsar 3D simulation for Masters in Physics for the University of Brasília (UnB)
A python library for analyzing Phantom SPH data using Sarracen.
Castro (Compressible Astrophysics): An adaptive mesh, astrophysical compressible (radiation-, magneto-) hydrodynamics simulation code for massively parallel CPU and GPU architectures.
A framework for hydrodynamics explorations and prototyping
X-PSI: X-ray Pulse Simulation and Inference
Particle-in-cell code for plasma simulation
3D visualization of the stellar neighbourhood
Installation scripts for the Galacticus galaxy formation model
Astronomical simulator of solar system and local stars
Home of the semi-analytical / semi-numerical galaxy evolution and reionization code ASTRAEUS
Physical vector and particle types for Julia
PION (PhotoIonization of Nebulae) is a C++ computational fluid-dynamics package for astrophysics, including MHD, radiative transfer, chemical kinetics and postprocessing routines. It is used mainly for modelling nebulae around massive stars.
Computational Astrophysics AST245: N-Body simulation and other exercises
Code to analyse data outputs from zoom galaxy cluster simulations investigating the effect of different mass and spatial resolutions.
Analyse the orbital evolution of Extreme Mass Ratio Inspirals, according to Einstein's general theory of relativity.
Analysis tools for the Galacticus galaxy formation model written in Python
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