Code ComparisonΒΆ
Several groups have started a comparison of their supernova radiative transfer codes to understand systematics uncertainties and different strategies. The first meeting is summarized here.
The description of file formats used can be found here https://docs.google.com/document/d/1YQky4yq45z-KGbKG1MhLRivSP6RmEjte7nN-UZ0H-3M/edit?usp=sharing.
For our code comparison, we will calculate spectra at 5, 10, 15, 20 days post-explosion.