Black Hole Group at IAG USP
Astrophysics research group. Research topics: black hole physics, high energy astrophysics, high-perfomance computing
Universidade de São Paulo
Pinned Repositories
AGNNES
Python (Tensorflow) code for performing Low-Luminosity AGN SED fitting.
bibtex-refs
BibTeX references
DL_BH_fluids
The architecture used in the Black Hole Weather Forecasting with Deep Learning
fermipy-tutorial
Fermi-LAT analysis lesson with FermiPy
gpumonty
Computes spectral energy distributions from radiatively inefficient accretion flows around black holes. GPU-accelerated, CUDA (alpha, unstable)
grmonty
grmonty: relativistic Monte Carlo code
harmpi
3D massively parallel general relativictic MHD code HARMPI
pluto
PLUTO: A Numerical Code for Computational Astrophysics
pyPLUTO
Black Hole Group at IAG USP's Repositories
black-hole-group/grmonty
grmonty: relativistic Monte Carlo code
black-hole-group/fermipy-tutorial
Fermi-LAT analysis lesson with FermiPy
black-hole-group/pluto
PLUTO: A Numerical Code for Computational Astrophysics
black-hole-group/AGNNES
Python (Tensorflow) code for performing Low-Luminosity AGN SED fitting.
black-hole-group/DL_BH_fluids
The architecture used in the Black Hole Weather Forecasting with Deep Learning
black-hole-group/pyPLUTO
black-hole-group/bibtex-refs
BibTeX references
black-hole-group/gpumonty
Computes spectral energy distributions from radiatively inefficient accretion flows around black holes. GPU-accelerated, CUDA (alpha, unstable)
black-hole-group/harmpi
3D massively parallel general relativictic MHD code HARMPI