2 code implementations • 13 Aug 2019 • M. Vincenzi, M. Sullivan, R. E. Firth, C. P. Gutiérrez, C. Frohmaier, M. Smith, C. Angus, R. C. Nichol
The design and analysis of time-domain sky surveys requires the ability to simulate accurately realistic populations of core collapse supernova (SN) events.
High Energy Astrophysical Phenomena
