activity
20152024
most citedA kilonova as the electromagnetic counterpart to a gravitational-wave source

888 citations · 3.7k across the 47 of their papers we have counts for

collaborators
Showing 2019Show all

8 papers · 1 filter

astro-ph.HE2019★ 23 cited

LSQ13ddu: A rapidly-evolving stripped-envelope supernova with early circumstellar interaction signatures

Peter Clark, Kate Maguire, Cosimo Inserra +30

This paper describes the rapidly evolving and unusual supernova LSQ13ddu, discovered by the La Silla-QUEST survey. LSQ13ddu displayed a rapid rise of just 4.80.9 d to reach a…

astro-ph.HE2019★ 55 cited

Determining the Ni distribution of type Ia supernovae from observations within days of explosion

M. R. Magee, K. Maguire, R. Kotak +4

Recent studies have shown how the distribution of Ni within the ejecta of type Ia supernovae can have profound consequences on the observed light curves. Observations at ear…

astro-ph.HE2019★ 52 cited

The transitional gap transient AT 2018hso: new insights on the luminous red nova phenomenon

Y-Z. Cai, A. Pastorello, M. Fraser +20

Aims: AT 2018hso is a new transient showing transitional properties between those of LRNe and the class of intermediate luminosity red transients (ILRTs) similar to SN 2008S. Throu…

astro-ph.HE2019★ 26 cited

The rise and fall of an extraordinary Ca-rich transient -- The discovery of ATLAS19dqr/SN 2019bkc

S. J. Prentice, K. Maguire, A. Flörs +25

This work presents the observations and analysis of ATLAS19dqr/SN 2019bkc, an extraordinary rapidly evolving transient event located in an isolated environment, tens of kiloparsecs…

astro-ph.HE2019★ 37 cited

SN2018kzr: a rapidly declining transient from the destruction of a white dwarf

Owen R. McBrien, Stephen J. Smartt, Ting-Wan Chen +31

We present SN2018kzr, the fastest declining supernova-like transient, second only to the kilonova, AT2017gfo. SN2018kzr is characterized by a peak magnitude of , peak…

astro-ph.HE2019★ 53 cited

SN 2017gmr: An energetic Type II-P supernova with asymmetries

Jennifer E. Andrews, D. J. Sand, S. Valenti +77

We present high-cadence ultraviolet (UV), optical, and near-infrared (NIR) data on the luminous Type II-P supernova SN 2017gmr from hours after discovery through the first 180 days…