Published February 22, 2022 | Version v1
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Supplementary data for: "Progenitor properties of type II supernovae: fitting to hydrodynamical models using Markov chain Monte Carlo methods"

Authors/Creators

  • 1. Instituto de Astrofísica de La Plata, Argentina
  • 2. European Southern Observatory, Santiago, Chile
  • 3. CENTRA, Lisboa, Portugal
  • 4. Centre for Mathematical Modelling, Santiago, Chile

Description

This entry contains a grid of bolometric light curve and photospheric velocity models applied to stellar evolution progenitors. A full description of the models can be found in Martinez et al. 2020, A&A, 642, A143.

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md5:a6a4aa16a8e2a82eb74898fafff40dba
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