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

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Showing 2020Show all

7 papers · 1 filter

astro-ph.SR2020★ 26 cited

Low luminosity Type II supernovae III. SN 2018hwm, a faint event with an unusually long plateau

A. Reguitti, M. L. Pumo, P. A. Mazzali +9

In this work, we present photometric and spectroscopic data of the low-luminosity Type IIP supernova (SN) 2018hwm. The object shows a faint ( mag) and very long (130…

astro-ph.HE2020★ 5 cited

The First Data Release of CNIa0.02 -- A Complete Nearby (Redshift <0.02) Sample of Type Ia Supernova Light Curves

Ping Chen, Subo Dong, C. S. Kochanek +41

The CNIa0.02 project aims to collect a complete, nearby sample of Type Ia supernovae (SNe Ia) light curves, and the SNe are volume-limited with host-galaxy redshifts z_host < 0.02.…

astro-ph.HE2020★ 29 cited

SN 2018gjx reveals that some SNe Ibn are SNe IIb exploding in dense circumstellar material

S. J. Prentice, K. Maguire, I. Boian +27

We present the data and analysis of SN 2018gjx, an unusual low-luminosity transient with three distinct spectroscopic phases. Phase I shows a hot blue spectrum with signatures of i…

astro-ph.HE2020★ 9 cited

PTF11rka: an interacting supernova at the crossroads of stripped-envelope and H-poor super-luminous stellar core collapses

Elena Pian, Paolo A. Mazzali, Takashi J. Moriya +17

The hydrogen-poor supernova PTF11rka (z = 0.0744), reported by the Palomar Transient Factory, was observed with various telescopes starting a few days after the estimated explosion…

astro-ph.HE2020★ 50 cited

The Spectacular Ultraviolet Flash From the Peculiar Type Ia Supernova 2019yvq

A. A. Miller, M. R. Magee, A. Polin +42

Early observations of Type Ia supernovae (SNeIa) provide essential clues for understanding the progenitor system that gave rise to the terminal thermonuclear explosion. We pres…

astro-ph.HE2020★ 17 cited

The intermediate nebular phase of SN 2014J: onset of clumping as the source of recombination

P. A. Mazzali, I. Bikmaev, R. Sunyaev +6

At the age of about 1 year, the spectra of most Type Ia supernovae are dominated by strong forbidden nebular emission lines of FeII and FeIII. Later observations (at about 2 years)…