activity
20122023
most citedA kilonova as the electromagnetic counterpart to a gravitational-wave source

888 citations · 2k across the 32 of their papers we have counts for

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16 papers · 1 filter

astro-ph.SR2023

Time varying Na I D absorption in ILRTs as a probe of circumstellar material

Robert Byrne, Morgan Fraser, Yongzhi Cai +2

Intermediate-Luminosity Red Transients (ILRTs) are a class of observed transient posited to arise from the production of an electron-capture supernova from a super-asymptotic giant…

astro-ph.SR202232 cited

Low luminosity Type II supernovae -- IV. SN 2020cxd and SN 2021aai, at the edges of the sub-luminous supernovae class

G. Valerin, M. L. Pumo, A. Pastorello +20

Photometric and spectroscopic data for two Low Luminosity Type IIP Supernovae (LL SNe IIP) are presented. SN 2020cxd reaches a peak absolute magnitude = -13.90 0.05 m…

astro-ph.SR20219 cited

SN 2021csp -- the explosion of a stripped envelope star within a H and He-poor circumstellar medium

Morgan Fraser, Maximilian D. Stritzinger, Sean J. Brennan +48

We present observations of SN 2021csp, a unique supernova (SN) which displays evidence for interaction with H- and He- poor circumstellar material (CSM) at early times. Using high-…

astro-ph.SR2021

Core-collapse supernova subtypes in luminous infrared galaxies

E. Kankare, A. Efstathiou, R. Kotak +34

We present the discovery and follow-up observations of two CCSNe that occurred in the luminous infrared galaxy (LIRG), NGC3256. The first, SN2018ec, was discovered using the ESO HA…

astro-ph.SR202039 cited

Luminous Red Nova AT 2019zhd, a new merger in M 31

A. Pastorello, M. Fraser, G. Valerin +20

We present the follow-up campaign of the luminous red nova (LRN) AT~2019zhd, the third event of this class observed in M 31. The object was followed by several sky surveys for abou…

astro-ph.SR202014 cited

Revisiting the progenitor of the low-luminosity type II-plateau supernova, SN 2008bk

D. O'Neill, R. Kotak, M. Fraser +3

The availability of updated model atmospheres for red supergiants and improvements in single and binary stellar evolution models, as well as previously unpublished data prompted us…