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20082026
most citedA kilonova as the electromagnetic counterpart to a gravitational-wave source

888 citations · 9.8k across the 174 of their papers we have counts for

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Showing 2021 · astro-ph.HEShow all

8 papers · 2 filters

astro-ph.HE2021★ 8 cited

Close, bright and boxy: the superluminous SN 2018hti

A. Fiore, S. Benetti, M. Nicholl +37

SN 2018hti was a very nearby (z=0.0614) superluminous supernova with an exceedingly bright absolute magnitude of -21.7 mag in r-band at maximum. The densely sampled pre-maximum lig…

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★ 5 cited

SN 2019hcc: A Type II Supernova Displaying Early O II Lines

Eleonora Parrag, Cosimo Inserra, Steve Schulze +18

We present optical spectroscopy together with ultraviolet, optical and near-infrared photometry of SN 2019hcc, which resides in a host galaxy at redshift 0.044, displaying a sub-so…

astro-ph.HE2021★ 9 cited

SN 2020cpg: an energetic link between type IIb and Ib supernovae

K. Medler, P. A. Mazzali, J. Teffs +18

Stripped-envelope supernovae (SE-SNe) show a wide variety of photometric and spectroscopic properties. This is due to the different potential formation channels and the stripping m…