Kwang-Il Seon's Home Page
The first principle is that you must not fool yourself. - Richard Feyman
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
The attenuation curves are available for download here: Download the data (28 MB)
Seon & Draine (2016, ApJ, 833, 201) http://adsabs.harvard.edu/abs/2016ApJ...833..201S
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.
© 2013 Seon, Kwang-Il