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20192021
most citedSN 2013ai: a link between hydrogen-rich and hydrogen-poor core-collapse supernovae

9 citations · 9 across the 1 of their papers we have counts for

collaborators

5 papers

astro-ph.HE20219 cited

SN 2013ai: a link between hydrogen-rich and hydrogen-poor core-collapse supernovae

S. Davis, P. J. Pessi, M. Fraser +33

We present a study of optical and near-infrared (NIR) spectra along with the light curves of SN 2013ai. These data range from discovery until 380 days after explosion. SN 2013ai is…

astro-ph.SR2020

Progenitor properties of type II supernovae: fitting to hydrodynamical models using Markov chain Monte Carlo methods

L. Martinez, M. C. Bersten, J. P. Anderson +3

The progenitor and explosion properties of type II supernovae (SNe II) are fundamental to understand the evolution of massive stars. Special interest has been given to the range of…

hep-ph2020

DES16C3cje: A low-luminosity, long-lived supernova

C. P. Gutiérrez, M. Sullivan, L. Martinez +89

We present DES16C3cje, a low-luminosity, long-lived type II supernova (SN II) at redshift 0.0618, detected by the Dark Energy Survey (DES). DES16C3cje is a unique SN. The spectra a…

astro-ph.SR2019

Mass discrepancy analysis for a select sample of Type II-Plateau supernovae

Laureano Martinez, Melina C. Bersten

The detailed study of supernovae (SNe) and their progenitors allows to better understand the evolution of massive stars and how these end their lives. Despite its importance, the r…

astro-ph.HE2019

Comparison of the optical light curves of hydrogen-rich and hydrogen-poor type II supernovae

P. J. Pessi, G. Folatelli, J. P. Anderson +12

Type II supernovae (SNe II) show strong hydrogen features in their spectra throughout their whole evolution while type IIb supernovae (SNe IIb) spectra evolve from dominant hydroge…