Curtis McCully, David Sand, Melissa L. Graham, Andy Howell, Griffin Hosseinzadeh, Anders Jerkstrand, Iair Arcavi
Abstract
We have intensively followed a sample of SNe type II during their photospheric phase. A single nebular spectra will allow us to complete our analysis with the following results: we will constrain the progenitor mass, estimate the nucleosynthesis yields of e.g., oxygen via detailed spectral modeling, measure the nebular ejecta velocities and line profiles to probe any asymmetries in the explosion mechanism and study circumstellar interaction.
Publications using this program's data
[data][ADS] The diversity of Type II supernova versus the similarity in their progenitors
[data][ADS] Optical and Ultraviolet Observations of the Very Young Type IIP SN 2014cx in NGC 337