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20002023
most citedBeaming in Gamma-Ray Bursts: Evidence for a Standard Energy Reservoir

1.2k citations · 27.5k across the 268 of their papers we have counts for

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Showing 2019 · astro-ph.HEShow all

23 papers · 2 filters

astro-ph.HE2019★ 46 cited

Formation and merging of Mass Gap Black Holes in Gravitational Wave Merger Events from Wide Hierarchical Quadruple Systems

Mohammadtaher Safarzadeh, Adrian S. Hamers, Abraham Loeb +1

We investigate secular evolution in hierarchical quadruple systems as a formation channel of mass-gap black holes (with masses of about ) in systems that will even…

astro-ph.HE2019★ 33 cited

AT 2018cow VLBI: No Long-Lived Relativistic Outflow

Michael F. Bietenholz, Raffaella Margutti, Deanne Coppejans +7

We report on VLBI observations of the fast and blue optical transient (FBOT), AT 2018cow. At ~62 Mpc, AT 2018cow is the first relatively nearby FBOT. The nature of AT 2018cow is no…

astro-ph.HE2019★ 32 cited

XMMSL2 J144605.0+685735 : a slow tidal disruption event

R. D. Saxton, A. M. Read, S. Komossa +6

Aims. We investigate the evolution of X-ray selected tidal disruption events. Methods. New events are found in near-real time data from XMM-Newton slews and are monitored by multi-…

astro-ph.HE2019★ 146 cited

Two years of non-thermal emission from the binary neutron star merger GW170817: rapid fading of the jet afterglow and first constraints on the kilonova fastest ejecta

A. Hajela, R. Margutti, K. D. Alexander +27

We present Chandra and VLA observations of GW170817 at ~521-743 days post merger, and a homogeneous analysis of the entire Chandra data set. We find that the late-time non-thermal…

astro-ph.HE2019★ 102 cited

The Optical Afterglow of GW170817: An Off-axis Structured Jet and Deep Constraints on a Globular Cluster Origin

Wen-fai Fong, P. K. Blanchard, K. D. Alexander +25

We present a revised and complete optical afterglow light curve of the binary neutron star merger GW170817, enabled by deep Hubble Space Telescope (HST) F606W observations at $\app…

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★ 56 cited

A Reverse Shock in GRB 181201A

Tanmoy Laskar, Hendrik van Eerten, Patricia Schady +26

We present comprehensive multiwavelength radio to X-ray observations of GRB 181201A spanning from s to days after the burst, comprising the first joint AL…

astro-ph.HE2019★ 5 cited

The Case for a High-Redshift Origin of GRB100205A

A. A. Chrimes, A. J. Levan, E. R. Stanway +15

The number of long gamma-ray bursts (GRBs) known to have occurred in the distant Universe (z greater than 5) is small (approx 15), however these events provide a powerful way of pr…

astro-ph.HE2019★ 162 cited

Fast Radio Bursts from Magnetars Born in Binary Neutron Star Mergers and Accretion Induced Collapse

Ben Margalit, Edo Berger, Brian D. Metzger

Recently born magnetars are promising candidates for the engines powering fast radio bursts (FRBs). The focus thus far has been placed on millisecond magnetars born in rare core-co…

astro-ph.HE2019★ 15 cited

Measuring the delay time distribution of binary neutron stars. III. Using the individual star formation histories of gravitational wave event host galaxies in the local universe

Mohammadtaher Safarzadeh, Edo Berger, Joel Leja +1

In Paper I (Safarzadeh & Berger 2019) we studied the determination of the delay time distribution (DTD) of binary neutron stars (BNS) through scaling relations between halo/stellar…

astro-ph.HE2019★ 42 cited

Measuring the delay time distribution of binary neutron stars. II. Using the redshift distribution from third-generation gravitational wave detectors network

Mohammadtaher Safarzadeh, Edo Berger, Ken K. -Y. Ng +4

We investigate the ability of current and third-generation gravitational wave (GW) detectors to determine the delay time distribution (DTD) of binary neutron stars (BNS) through a…

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★ 1 cited

Achieving Transformative Understanding of Extreme Stellar Explosions with ELT-enabled Late-time Spectroscopy

D. Milisavljevic, R. Margutti, R. Chornock +35

Supernovae are among the most powerful and influential explosions in the universe. They are also ideal multi-messenger laboratories to study extreme astrophysics. However, many fun…

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★ 64 cited

ALMA Detection of a Linearly Polarized Reverse Shock in GRB 190114C

Tanmoy Laskar, Kate D. Alexander, Ramandeep Gill +11

We present ALMA 97.5 GHz total intensity and linear polarization observations of the mm-band afterglow of GRB 190114C spanning 2.2 to 5.2 hours after the burst. We detect linear po…

astro-ph.HE2019★ 1 cited

GRBs as Probes of the Early Universe with TSO

Nial Tanvir, Jonathan Grindlay, Edo Berger +12

Long gamma-ray bursts (GRBs) are the most luminous known electromagnetic radiation sources in the Universe for the 3 to 300 sec of their prompt flashes (isotropic X/ gamma-ray lumi…

astro-ph.HE2019

Kilonovae: nUV/Optical/IR Counterparts of Neutron Star Binary Mergers with TSO

Brian D. Metzger, Edo Berger, Jonathan Grindlay +12

With the epochal first detection of gravitational waves from a binary neutron star (NS) merger with the GW170817 event, and its direct confirmation that NS-NS mergers are significa…

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★ 3 cited

Multi-Messenger Astronomy with Extremely Large Telescopes

Ryan Chornock, Philip S. Cowperthwaite, Raffaella Margutti +82

The field of time-domain astrophysics has entered the era of Multi-messenger Astronomy (MMA). One key science goal for the next decade (and beyond) will be to characterize gravitat…

astro-ph.HE2019

Multimessenger science opportunities with mHz gravitational waves

John Baker, Zoltán Haiman, Elena Maria Rossi +32

LISA will open the mHz band of gravitational waves (GWs) to the astronomy community. The strong gravity which powers the variety of GW sources in this band is also crucial in a num…

astro-ph.HE2019★ 51 cited

Type Ibn Supernovae May not all Come from Massive Stars

Griffin Hosseinzadeh, Curtis McCully, Ann I. Zabludoff +5

Because core-collapse supernovae are the explosions of massive stars, which have relatively short lifetimes, they occur almost exclusively in galaxies with active star formation. O…

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…