activity
20162023
most citedA kilonova as the electromagnetic counterpart to a gravitational-wave source

888 citations · 1.5k across the 16 of their papers we have counts for

collaborators

29 papers

astro-ph.HE2023

Detailed spectrophotometric analysis of the superluminous and fast evolving SN 2019neq

Achille Fiore, Stefano Benetti, Leonardo Tartaglia +24

SN 2019neq was a very fast evolving superluminous supernova. At a redshift z=0.1059, its peak absolute magnitude was -21.5+/-0.2 mag in g band. In this work, we present data and an…

astro-ph.HE2022

SN 2020acat: A purr-fect example of a fast rising Type IIb Supernova

K. Medler, P. A. Mazzali, J. Teffs +31

The Ultra-Violet (UV) and Near Infrared (NIR) photometric and optical spectroscopic observations of SN 2020acat covering days after explosion are presented here. U…

astro-ph.HE20212 cited

How low can you go? SN 2018zd as a low-mass Fe core-collapse supernova

E. Callis, M. Fraser, A. Pastorello +38

We present spectroscopy and photometry of SN 2018zd, a Type IIP core-collapse supernova with signatures of interaction with circumstantial material in its earliest spectra. High io…

astro-ph.HE20212 cited

Intermediate-luminosity red transients: Spectrophotometric properties and connection to electron-capture supernova explosions

Y. -Z. Cai, A. Pastorello, M. Fraser +56

We present the spectroscopic and photometric study of five intermediate-luminosity red transients (ILRTs), namely AT 2010dn, AT 2012jc, AT 2013la, AT 2013lb, and AT 2018aes. They s…

astro-ph.HE202131 cited

The double-peaked type Ic Supernova 2019cad: another SN 2005bf-like object

C. P. Gutiérrez, M. C. Bersten, M. Orellana +23

We present the photometric and spectroscopic evolution of supernova (SN) 2019cad during the first days from explosion. Based on the light curve morphology, we find that S…

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…