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20152025
most citedA Kilonova Following a Long-Duration Gamma-Ray Burst at 350 Mpc

356 citations · 2.4k across the 59 of their papers we have counts for

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55 papers · 1 filter

astro-ph.HE2025

GRB 240825A: Early Reverse Shock and Its Physical Implications

Chao Wu, Yun Wang, Hua-Li Li +84

Early multiwavelength observations offer crucial insights into the nature of the relativistic jets responsible for gamma-ray bursts and their interaction with the surrounding mediu…

astro-ph.HE2025★ 1 cited

EP250207b is not a collapsar fast X-ray transient. Is it due to a compact object merger?

P. G. Jonker, A. J. Levan, Xing Liu +41

Fast X-ray Transients (FXTs) are short-lived extra-galactic X-ray sources. Recent progress through multi-wavelength follow-up of Einstein Probe discovered FXTs has shown that sever…

astro-ph.HE2025

The day-long, repeating GRB 250702BDE / EP250702a: A unique extragalactic transient

Andrew J. Levan, Antonio Martin-Carrillo, Tanmoy Laskar +42

Gamma-ray bursts (GRBs) are singular outbursts of high-energy radiation with durations typically lasting from milliseconds to minutes and, in extreme cases, a few hours. They are a…

astro-ph.HE2025

EP240801a/XRF 240801B: An X-ray Flash Detected by the Einstein Probe and Implications of its Multiband Afterglow

Shuai-Qing Jiang, Dong Xu, Agnes P. C. van Hoof +89

We present multiband observations and analysis of EP240801a, a low-energy, extremely soft gamma-ray burst (GRB) discovered on August 1, 2024 by the Einstein Probe (EP) satellite, w…

astro-ph.HE2024★ 9 cited

Multi-Peaked Non-Thermal Light Curves from Magnetar-Powered Gamma-Ray Bursts

Conor M. B. Omand, Nikhil Sarin, Gavin P. Lamb

Binary neutron star mergers and collapsing massive stars can both create millisecond magnetars. Such magnetars are candidate engines to power gamma-ray bursts (GRBs). The non-therm…

astro-ph.HE2024★ 1 cited

The Nature of Optical Afterglows Without Gamma-ray Bursts: Identification of AT2023lcr and Multiwavelength Modeling

Maggie L. Li, Anna Y. Q. Ho, Geoffrey Ryan +29

In the past few years, the improved sensitivity and cadence of wide-field optical surveys have enabled the discovery of several afterglows without associated detected gamma-ray bur…

astro-ph.HE2024★ 3 cited

Distinguishing radiation mechanisms and particle populations in blazar jets through long-term multi-band monitoring with RINGO3 and Fermi

Callum McCall, Helen Jermak, Iain A. Steele +6

We present the results of seven years of multicolour photometric monitoring of a sample of 31 -ray bright blazars using the RINGO3 polarimeter on the Liverpool Telescope from 20…

astro-ph.HE2024★ 3 cited

The Luminous, Slow-Rising Orphan Afterglow AT2019pim as a Candidate Moderately Relativistic Outflow

Daniel A. Perley, Anna Y. Q. Ho, Michael Fausnaugh +34

Classical gamma-ray bursts (GRBs) have two distinct emission episodes: prompt emission from ultrarelativistic ejecta and afterglow from shocked circumstellar material. While both c…

astro-ph.HE2023

A Hubble Space Telescope Search for r-Process Nucleosynthesis in Gamma-ray Burst Supernovae

J. C. Rastinejad, W. Fong, A. J. Levan +23

The existence of a secondary (in addition to compact object mergers) source of heavy element (-process) nucleosynthesis, the core-collapse of rapidly-rotating and highly-magneti…

astro-ph.HE2023

Rapid Generation of Kilonova Light Curves Using Conditional Variational Autoencoder

Surojit Saha, Michael J. Williams, Laurence Datrier +8

The discovery of the optical counterpart, along with the gravitational waves from GW170817, of the first binary neutron star merger, opened up a new era for multi-messenger astroph…

astro-ph.HE2023★ 55 cited

Redback: A Bayesian inference software package for electromagnetic transients

Nikhil Sarin, Moritz Hübner, Conor M. B. Omand +8

Fulfilling the rich promise of rapid advances in time-domain astronomy is only possible through confronting our observations with physical models and extracting the parameters that…

astro-ph.HE2023★ 230 cited

JWST detection of heavy neutron capture elements in a compact object merger

A. Levan, B. P. Gompertz, O. S. Salafia +80

The mergers of binary compact objects such as neutron stars and black holes are of central interest to several areas of astrophysics, including as the progenitors of gamma-ray burs…

astro-ph.HE2023★ 13 cited

GRB 201015A and the nature of low-luminosity soft gamma-ray bursts

M. Patel, B. P. Gompertz, P. T. O'Brien +20

GRB 201015A is a peculiarly low luminosity, spectrally soft gamma-ray burst (GRB), with s (time interval of detection of 90\% of photons from the GRB), a…

astro-ph.HE2023★ 1 cited

Unpacking merger jets: a Bayesian analysis of GW170817, GW190425 and electromagnetic observations of short gamma-ray bursts

Fergus Hayes, Ik Siong Heng, Gavin Lamb +3

We present a novel fully Bayesian analysis to constrain short gamma-ray burst jet structures associated with cocoon, wide-angle and simple top-hat jet models, as well as the binary…

astro-ph.HE2023★ 2 cited

A long-duration gamma-ray burst of dynamical origin from the nucleus of an ancient galaxy

Andrew J. Levan, Daniele B. Malesani, Benjamin P. Gompertz +29

The majority of long duration ( s) gamma-ray bursts (GRBs) are believed to arise from the collapse of massive stars \cite{Hjorth+03}, with a small proportion created from the m…

astro-ph.HE2023★ 47 cited

The first JWST spectrum of a GRB afterglow: No bright supernova in observations of the brightest GRB of all time, GRB 221009A

A. J. Levan, G. P. Lamb, B. Schneider +57

We present JWST and Hubble Space Telescope (HST) observations of the afterglow of GRB 221009A, the brightest gamma-ray burst (GRB) ever observed. This includes the first mid-IR spe…

astro-ph.HE2023★ 12 cited

The brightest GRB ever detected: GRB 221009A as a highly luminous event at z = 0.151

D. B. Malesani, A. J. Levan, L. Izzo +39

Context: The extreme luminosity of gamma-ray bursts (GRBs) makes them powerful beacons for studies of the distant Universe. The most luminous bursts are typically detected at moder…

astro-ph.HE2022★ 106 cited

The case for a minute-long merger-driven gamma-ray burst from fast-cooling synchrotron emission

B. P. Gompertz, M. E. Ravasio, M. Nicholl +12

For decades, gamma-ray bursts (GRBs) have been broadly divided into `long'- and `short'-duration bursts, lasting more or less than 2s, respectively. However, this dichotomy does no…

astro-ph.HE2022★ 356 cited

A Kilonova Following a Long-Duration Gamma-Ray Burst at 350 Mpc

J. C. Rastinejad, B. P. Gompertz, A. J. Levan +32

Here, we report the discovery of a kilonova associated with the nearby (350 Mpc) minute-duration GRB 211211A. In tandem with deep optical limits that rule out the presence of an ac…

astro-ph.HE2022★ 21 cited

A blast from the infant Universe: the very high-z GRB 210905A

A. Rossi, D. D. Frederiks, D. A. Kann +52

We present a detailed follow-up of the very energetic GRB 210905A at a high redshift of z = 6.312 and its luminous X-ray and optical afterglow. We obtained a photometric and spectr…

astro-ph.HE2022★ 1 cited

Inhomogeneous Jets from Neutron Star Mergers: One Jet to Rule them all

Gavin P Lamb, Lorenzo Nativi, Stephan Rosswog +4

Using the resultant profiles from 3D hydrodynamic simulations of relativistic jets interacting with neutron star merger wind ejecta, we show how the inhomogeneity of energy and vel…

astro-ph.HE2021★ 24 cited

The supernova of the MAGIC GRB190114C

A. Melandri, L. Izzo, E. Pian +42

We observed GRB190114C (redshift z = 0.4245), the first GRB ever detected at TeV energies, at optical and near-infrared wavelengths with several ground-based telescopes and the Hub…

astro-ph.HE2021★ 52 cited

Target of Opportunity Observations of Gravitational Wave Events with Vera C. Rubin Observatory

Igor Andreoni, Raffaella Margutti, Om Sharan Salafia +52

The discovery of the electromagnetic counterpart to the binary neutron star merger GW170817 has opened the era of gravitational-wave multi-messenger astronomy. Rapid identification…

astro-ph.HE2021

Are Interactions with Neutron Star Merger Winds Shaping the Jets?

Lorenzo Nativi, Gavin P. Lamb, Stephan Rosswog +2

Jets can become collimated as they propagate through dense environments and understanding such interactions is crucial for linking physical models of the environments to observatio…