MoCafe (Monte Carlo radiative transfer)
  • MoCafe is a 3D continuum radiative transfer (RT) code based on the Monte Carlo algorithm. The code is written in modern fortran and runs in parallel using MPI. MPI-3 is used to use the shared-memory in each host (node).
Published Simulation Data
- Attenuation Curves in Clumpy, Galactic Environments
- MoCafe/Galaxy
  • The MoCafe/Galaxy code has been developed to simulate dusty galaxies.
  • Versions that calculate the infrared emission and polarization are also available.
  • More complete description will be published.
- MCMC Fitting of Galaxy Images
  • A Markov Chain Monte Carlo code to fit the optical/FUV observational images of spiral galaxies was developed and is being tested.