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Article
A UV resonance line echo from a shell around a hydrogen-poor superluminous supernova
Hydrogen-poor superluminous supernovae (SLSN-I) are a class of rare and energetic explosions that have been discovered in untargeted transient surveys in the past decade1,2. The progenitor stars and the physical ...
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Article
Confined dense circumstellar material surrounding a regular type II supernova
With the advent of new wide-field, high-cadence optical transient surveys, our understanding of the diversity of core-collapse supernovae has grown tremendously in the last decade. However, the pre-supernova e...
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Article
Correction: Corrigendum: The superluminous transient ASASSN-15lh as a tidal disruption event from a Kerr black hole
Nature Astronomy 1, 0002 (2016); published 12 December 2016; corrected 22 December 2016. In the version of this Letter originally published the estimated energy radiated by ASASSN-15lh up to 25 May 2016 was in...
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Article
The superluminous transient ASASSN-15lh as a tidal disruption event from a Kerr black hole
When a star passes within the tidal radius of a supermassive black hole, it will be torn apart1. For a star with the mass of the Sun (M⊙) and a non-spinning black hole with a mass <108M⊙, the tidal radius lies ou...
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Chapter and Conference Paper
Gamma-Ray Burst Afterglows as Probes of High-Z Star Formation
Gamma-Ray Bursts (GRBs) are bright and distant explosions, caused by the death of a massive star, making them excellent probes of star formation at all redshifts. One application of GRBs is to perform optical ...