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

888 citations · 2.7k across the 48 of their papers we have counts for

collaborators
Showing 2021 · astro-ph.HEShow all

6 papers · 2 filters

astro-ph.HE2021★ 2 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.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★ 2 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.HE2021★ 31 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.HE2021

Progenitor, environment, and modelling of the interacting transient, AT 2016jbu (Gaia16cfr)

S. J. Brennan, M. Fraser, J. Johansson +67

We present the bolometric lightcurve, identification and analysis of the progenitor candidate, and preliminary modelling of AT2016jbu (Gaia16cfr). We find a progenitor consistent w…

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…