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20182026
most citedType II supernovae from the Carnegie Supernova Project-I. II. Physical parameter distributions from hydrodynamical modelling

71 citations · 597 across the 55 of their papers we have counts for

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astro-ph.SR2026

SN 2024afyu interpreted as a Pair Instability Supernova

P. J. Pessi, S. Barmentloo, Ł. Wyrzykowski +63

Pair-instability supernovae (PISNe) are the predicted explosions of very massive stars triggered by electron-positron pair production. Numerous transients have been proposed as PIS…

astro-ph.SR2026

Light-Curve and Spectral Properties of Type II Supernovae from the ATLAS survey

K. Ertini, J. P. Anderson, G. Folatelli +22

Type II supernovae (SNe II) are the most common terminal stellar explosions in the Universe. With SNe now being detected within days after explosion, there is growing evidence that…

astro-ph.SR2024★ 10 cited

SN 2020pvb: a Type IIn-P supernova with a precursor outburst

Nancy Elias-Rosa, Seán J. Brennan, Stefano Benetti +37

We present photometric and spectroscopic data sets for SN 2020pvb, a Type IIn-P supernova (SN) similar to SNe 1994W, 2005cl, 2009kn and 2011ht, with a precursor outburst detected (…

astro-ph.SR2022★ 38 cited

Type II supernovae from the Carnegie Supernova Project-I. III. Understanding SN II diversity through correlations between physical and observed properties

L. Martinez, J. P. Anderson, M. C. Bersten +17

SNe II show great photometric and spectroscopic diversity which is attributed to the varied physical characteristics of their progenitor and explosion properties. In this study, th…

astro-ph.SR2021★ 37 cited

Type II supernovae from the Carnegie Supernova Project-I. I. Bolometric light curves of 74 SNe II using uBgVriYJH photometry

L. Martinez, M. C. Bersten, J. P. Anderson +18

The present study is the first of a series of three papers where we characterise the type II supernovae (SNe~II) from the Carnegie Supernova Project-I to understand their diversity…

astro-ph.SR2021★ 71 cited

Type II supernovae from the Carnegie Supernova Project-I. II. Physical parameter distributions from hydrodynamical modelling

L. Martinez, M. C. Bersten, J. P. Anderson +18

Linking supernovae to their progenitors is a powerful method for furthering our understanding of the physical origin of their observed differences, while at the same time testing s…