Published June 21, 2021 | Version v1
Dataset Open

Probabilistic Reconstruction of Type Ia Supernova SN 2002bo

  • 1. Department of Physics and Astronomy, Michigan State University, East Lansing, MI 48824, USA
  • 2. Department of Physics, New York University, New York, NY, 10003, USA
  • 3. Max-Planck-Institut fur Astrophysik, Karl-Schwarzschild-Str. 1, 85748 Garching, Germany
  • 4. Max-Planck-Institut fur extraterrestrische Physik, Giessenbachstrasse 1, 85748 Garching bei Munchen, Germany
  • 5. Leibniz Supercomputing Centre, Boltzmannstr. 1, 85748 Garching bei Munchen, Germany
  • 6. Astrophysics Research Centre, School of Mathematics and Physics, Queen's University Belfast, BT7 1NN, UK
  • 7. GSI Helmholtzzentrum f\"ur Schwerionenforschung, Planckstrass e 1, 64291 Darmstadt, Germany
  • 8. Machine Learning Research Lab, Volkswagen AG, Munich, Germany



  • The TARDIS configuration YAML file used as a template for the training spectra.
  • HDF5 file of posterior samples of model parameters and their associated weights from the nested sampler.


  • Input grid of model parameters and corresponding spectra produced by TARDIS used to generate the training grid of the emulator.


For further questions, please contact John O'Brien at


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