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20152025
most citedThe environment of the binary neutron star merger GW170817

171 citations · 519 across the 11 of their papers we have counts for

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13 papers · 1 filter

astro-ph.HE2025

The 157-month Swift-BAT All-Sky Hard X-Ray Survey

Amy Y. Lien, Hans Krimm, Craig Markwardt +12

The Burst Alert Telescope (BAT) onboard the Neil Gehrels Swift observatory has been serving as a survey instrument for the hard X-ray sky, and has detected thousands of X-ray sourc…

astro-ph.HE2025

Constraints on diffuse X-ray Emission from the TeV halo Candidate HESS J1813-126

David Guevel, Kim L Page, Kaya Mori +2

Extended regions of very high energy -ray emission associated with middle-aged pulsars have been found by -ray observatories. These regions, called TeV halos or pulsar halos,…

astro-ph.HE2025

BatAnalysis -- A Comprehensive Python Pipeline for Swift BAT Time-Tagged Event Data Analysis

Tyler Parsotan, David M. Palmer, Samuele Ronchini +7

The Swift Burst Alert Telescope (BAT) is a coded aperture gamma-ray instrument with a large field of view that was designed to detect and localize transient events. When a transien…

astro-ph.HE2024

An Optically Led Search for Kilonovae to z0.3 with the Kilonova and Transients Program (KNTraP)

Natasha Van Bemmel, Jielai Zhang, Jeff Cooke +15

Compact binary mergers detectable in gravitational waves can be accompanied by a kilonova, an electromagnetic transient powered by radioactive decay of newly synthesised r-process…

astro-ph.HE2024

Explaining Non-Merger Gamma-Ray Bursts and Broad-Lined Supernovae with Close Binary Progenitors with Black Hole Central Engine

Christopher L. Fryer, Eric Burns, Anna Y. Q. Ho +5

For over 25 years, the origin of long-duration gamma-ray bursts (lGRBs) has been linked to the collapse of rotating massive stars. However, we have yet to pinpoint the stellar prog…

astro-ph.HE2024

GRB220831A: a hostless, intermediate Gamma-ray burst with an unusual optical afterglow

James Freeburn, Brendan O'Connor, Jeff Cooke +20

GRB220831A is a gamma-ray burst (GRB) with a duration and spectral peak energy that places it at the interface between the distribution of long-soft and short-hard GRBs. In thi…