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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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Showing 2021Show all

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astro-ph.CO2021★ 7 cited

Carnegie Supernova Project: kinky -band light-curves of Type Ia supernovae

P. J. Pessi, E. Y. Hsiao, G. Folatelli +19

We present detailed investigation of a specific -band light-curve feature in Type Ia supernovae (SNe Ia) using the rapid cadence and high signal-to-noise ratio light-curves obta…

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…

astro-ph.HE2021★ 9 cited

Transitional events in the spectrophotometric regime between stripped envelope and superluminous supernovae

S. J. Prentice, C. Inserra, S. Schulze +24

The division between stripped-envelope supernovae (SE-SNe) and superluminous supernovae (SLSNe) is not well defined in either photometric or spectroscopic space. While a sharp lumi…

astro-ph.HE2021★ 10 cited

SN 2018bsz: significant dust formation in a nearby superluminous supernova

T. -W. Chen, S. J. Brennan, R. Wesson +41

We investigate the thermal emission and the extinction from dust associated with the nearby (z = 0.0267) superluminous supernova (SLSN) 2018bsz. Our dataset combines daily-cadence,…

astro-ph.HE2021★ 9 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…