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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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35 papers · 1 filter

astro-ph.HE2023★ 20 cited

SN2017egm: A Helium-rich Superluminous Supernova with Multiple Bumps in the Light Curves

Jiazheng Zhu, Ning Jiang, Subo Dong +28

When discovered, SN~2017egm was the closest (redshift ) hydrogen-poor superluminous supernova (SLSN-I) and a rare case that exploded in a massive and metal-rich galaxy. Thu…

astro-ph.HE2022★ 20 cited

Oxygen and calcium nebular emission line relationships in core-collapse supernovae and Ca-rich transients

Simon Prentice, Kate Maguire, Louis Siebenaler +1

This work examines the relationships between the properties (flux ratios, full width at half-maximum velocities) of the [O I] 6300, 6364, [Ca II] 7291, 7323, and the Ca II…

astro-ph.HE2021

A Linear Relation Between the Color Stretch and the Rising Color Slope of Type Ia Supernovae

Ping Chen, Subo Dong, Chris Ashall +34

Using data from the Complete Nearby () sample of Type Ia Supernovae (CNIa0.02), we discover a linear relation between two parameters derived from the color cur…

astro-ph.HE2021★ 28 cited

Less than 1% of Core-Collapse Supernovae in the local universe occur in elliptical galaxies

I. Irani, S. J. Prentice, S. Schulze +39

We present observations of three Core-collapse supernovae (CCSNe) in elliptical hosts, detected by the Zwicky Transient Facility Bright Transient Survey (BTS). SN 2019ape is a SN I…

astro-ph.HE2021★ 9 cited

Transitional events in the spectrophotometric regime between stripped envelope and superluminous supernovae

S. J. Prentice, C. Inserra, S. Schulze +24

The division between stripped-envelope supernovae (SE-SNe) and superluminous supernovae (SLSNe) is not well defined in either photometric or spectroscopic space. While a sharp lumi…

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★ 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…

astro-ph.HE2021★ 12 cited

Observations and Spectral Modelling of the Narrow-Lined Type Ic SN 2017ein

Jacob Teffs, Simon J. Prentice, Paolo Mazzali +1

SN 2017ein is a narrow-lined Type Ic SN that was found to share a location with a point-like source in the face on spiral galaxy NGC 3938 in pre-supernova images, making SN 2017ein…

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)…

astro-ph.HE2019★ 23 cited

LSQ13ddu: A rapidly-evolving stripped-envelope supernova with early circumstellar interaction signatures

Peter Clark, Kate Maguire, Cosimo Inserra +30

This paper describes the rapidly evolving and unusual supernova LSQ13ddu, discovered by the La Silla-QUEST survey. LSQ13ddu displayed a rapid rise of just 4.80.9 d to reach a…

astro-ph.HE2019★ 55 cited

Determining the Ni distribution of type Ia supernovae from observations within days of explosion

M. R. Magee, K. Maguire, R. Kotak +4

Recent studies have shown how the distribution of Ni within the ejecta of type Ia supernovae can have profound consequences on the observed light curves. Observations at ear…

astro-ph.HE2019★ 52 cited

The transitional gap transient AT 2018hso: new insights on the luminous red nova phenomenon

Y-Z. Cai, A. Pastorello, M. Fraser +20

Aims: AT 2018hso is a new transient showing transitional properties between those of LRNe and the class of intermediate luminosity red transients (ILRTs) similar to SN 2008S. Throu…

astro-ph.HE2019★ 26 cited

The rise and fall of an extraordinary Ca-rich transient -- The discovery of ATLAS19dqr/SN 2019bkc

S. J. Prentice, K. Maguire, A. Flörs +25

This work presents the observations and analysis of ATLAS19dqr/SN 2019bkc, an extraordinary rapidly evolving transient event located in an isolated environment, tens of kiloparsecs…

astro-ph.HE2019★ 37 cited

SN2018kzr: a rapidly declining transient from the destruction of a white dwarf

Owen R. McBrien, Stephen J. Smartt, Ting-Wan Chen +31

We present SN2018kzr, the fastest declining supernova-like transient, second only to the kilonova, AT2017gfo. SN2018kzr is characterized by a peak magnitude of , peak…

astro-ph.HE2019★ 53 cited

SN 2017gmr: An energetic Type II-P supernova with asymmetries

Jennifer E. Andrews, D. J. Sand, S. Valenti +77

We present high-cadence ultraviolet (UV), optical, and near-infrared (NIR) data on the luminous Type II-P supernova SN 2017gmr from hours after discovery through the first 180 days…

astro-ph.HE2018★ 144 cited

Investigating the properties of stripped-envelope supernovae, what are the implications for their progenitors?

S. J. Prentice, C. Ashall, P. A. James +41

We present observations and analysis of 18 stripped-envelope supernovae observed during 2013 -- 2018. This sample consists of 5 H/He-rich SNe, 6 H-poor/He-rich SNe, 3 narrow lined…

astro-ph.HE2018★ 236 cited

The Cow: discovery of a luminous, hot and rapidly evolving transient

S. J. Prentice, K. Maguire, S. J. Smartt +27

We present the ATLAS discovery and initial analysis of the first 18 days of the unusual transient event, ATLAS18qqn/AT2018cow. It is characterized by a high peak luminosity (…

astro-ph.HE2018★ 50 cited

A nearby superluminous supernova with a long pre-maximum 'plateau' and strong CII features

J. P. Anderson, P. J. Pessi, L. Dessart +63

Super-luminous supernovae (SLSNe) are rare events defined as being significantly more luminous than normal terminal stellar explosions. The source of the extra powering needed to a…

astro-ph.HE2017★ 126 cited

The early detection and follow-up of the highly obscured Type II supernova 2016ija/DLT16am

L. Tartaglia, D. J. Sand, S. Valenti +45

We present our analysis of the Type II supernova DLT16am (SN~2016ija). The object was discovered during the ongoing (DLT40) one day cadence supernova search a…

astro-ph.HE2017★ 888 cited

A kilonova as the electromagnetic counterpart to a gravitational-wave source

S. J. Smartt, T. -W. Chen, A. Jerkstrand +118

Gravitational waves were discovered with the detection of binary black hole mergers and they should also be detectable from lower mass neutron star mergers. These are predicted to…