activity
20132026
most citedThe Electromagnetic Counterpart of the Binary Neutron Star Merger LIGO/VIRGO GW170817. II. UV, Optical, and Near-IR Light Curves and Comparison to Kilonova Models

1k citations · 11.7k across the 197 of their papers we have counts for

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Showing 2019Show all

12 papers · 1 filter

astro-ph.HE2019★ 18 cited

SN 2016gsd: An unusually luminous and linear type II supernova with high velocities

T. M. Reynolds, M. Fraser, S. Mattila +27

We present observations of the unusually luminous Type II supernova (SN) 2016gsd. With a peak absolute magnitude of V = 19.95 0.08, this object is one of the brightest Typ…

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★ 62 cited

A Galaxy-Targeted Search for the Optical Counterpart of the Candidate NS-BH Merger S190814bv with Magellan

S. Gomez, G. Hosseinzadeh, P. S. Cowperthwaite +13

On 2019 August 14 the Laser Interferometer Gravitational Wave Observatory (LIGO) and the Virgo gravitational wave interferometer announced the detection of a binary merger, S190814…

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.HE2019★ 97 cited

Follow-up of the Neutron Star Bearing Gravitational Wave Candidate Events S190425z and S190426c with MMT and SOAR

G. Hosseinzadeh, P. S. Cowperthwaite, S. Gomez +23

On 2019 April 25.346 and 26.640 UT the LIGO and Virgo gravitational wave (GW) observatories announced the detection of the first candidate events in Observing Run 3 that contain at…

astro-ph.HE2019★ 37 cited

SN 2016iet: The Pulsational or Pair Instability Explosion of a Low Metallicity Massive CO Core Embedded in a Dense Hydrogen-Poor Circumstellar Medium

Sebastian Gomez, Edo Berger, Matt Nicholl +7

We present optical photometry and spectroscopy of SN 2016iet, an unprecedented Type I supernova (SN) at with no obvious analog in the existing literature. The peculiar l…

astro-ph.HE2019★ 72 cited

The tidal disruption event AT2017eqx: spectroscopic evolution from hydrogen rich to poor suggests an atmosphere and outflow

M. Nicholl, P. K. Blanchard, E. Berger +24

We present and analyse a new tidal disruption event (TDE), AT2017eqx at redshift z=0.1089, discovered by Pan-STARRS and ATLAS. The position of the transient is consistent with the…

astro-ph.HE2019★ 2 cited

Radio Time-Domain Signatures of Magnetar Birth

Casey J. Law, Ben Margalit, Nipuni T. Palliyaguru +10

The last decade has seen the rapid, concurrent development of new classes of energetic astrophysical transients, including Fast Radio Bursts, Superluminous Supernovae, and ultralon…

astro-ph.HE2019

Gravity and Light: Combining Gravitational Wave and Electromagnetic Observations in the 2020s

R. J. Foley, K. D. Alexander, I. Andreoni +110

As of today, we have directly detected exactly one source in both gravitational waves (GWs) and electromagnetic (EM) radiation, the binary neutron star merger GW170817, its associa…

astro-ph.HE2019★ 123 cited

The spectral evolution of AT 2018dyb and the presence of metal lines in tidal disruption events

Giorgos Leloudas, Lixin Dai, Iair Arcavi +29

We present light curves and spectra of the tidal disruption event (TDE) ASASSN-18pg / AT 2018dyb spanning a period of one year. The event shows a plethora of strong emission lines,…

astro-ph.HE2019★ 65 cited

A Radio Source Coincident with the Superluminous Supernova PTF10hgi: Evidence for a Central Engine and an Analogue of the Repeating FRB121102?

T. Eftekhari, E. Berger, B. Margalit +9

We present the detection of an unresolved radio source coincident with the position of the Type I superluminous supernova (SLSN) PTF10hgi () about 7.5 years post-explosion…