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20192025
most citedType II supernovae from the Carnegie Supernova Project-I. II. Physical parameter distributions from hydrodynamical modelling

71 citations · 304 across the 15 of their papers we have counts for

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astro-ph.SR2025★ 5 cited

Two Decades of Dust Evolution in SN 2005af through JWST, Spitzer, and Chemical Modeling

Arkaprabha Sarangi, Szanna Zsiros, Tamas Szalai +20

The evolution of dust in core-collapse supernovae (SNe), in general, is poorly constrained owing to a lack of infrared observations after a few years from explosion. Most theories…

astro-ph.SR2023

Circumstellar interaction models for the early bolometric light curve of SN 2023ixf

L. Martinez, M. C. Bersten, G. Folatelli +2

SNe II show growing evidence of interaction with CSM surrounding their progenitor stars as a consequence of enhanced mass loss during the last years of the progenitor's life. We pr…

astro-ph.SR2023

The progenitor of SN 2023ixf from hydrodynamical modelling

M. C. Bersten, M. Orellana, G. Folatelli +5

Context: Supernova (SN) 2023ixf is among the most nearby Type II SNe in the last decades. As such, there is a wealth of observational data of both the event itself and of the assoc…

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…