activity
20092024
most citedFermi Observations of GRB 090902B: A Distinct Spectral Component in the Prompt and Delayed Emission

448 citations · 4.7k across the 60 of their papers we have counts for

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Showing 2018Show all

5 papers · 1 filter

astro-ph.HE2018★ 44 cited

A Fermi Gamma-ray Burst Monitor Search for Electromagnetic Signals Coincident with Gravitational-Wave Candidates in Advanced LIGO's First Observing Run

ray Burst Monitor Team, The LIGO Scientific Collaboration, the Virgo Collaboration +1160

We present a search for prompt gamma-ray counterparts to compact binary coalescence gravitational wave (GW) candidates from Advanced LIGO's first observing run (O1). As demonstrate…

astro-ph.HE2018★ 38 cited

Fermi GBM Observations of GRB 150101B: A Second Nearby Event with a Short Hard Spike and a Soft Tail

E. Burns, P. Veres, V. Connaughton +19

In light of the joint multimessenger detection of a binary neutron star merger as the gamma-ray burst GRB 170817A and in gravitational waves as GW170817, we reanalyze the Fermi Gam…

astro-ph.IM2018★ 2 cited

STROBE-X: A probe-class mission for X-ray spectroscopy and timing on timescales from microseconds to years

Paul S. Ray, Zaven Arzoumanian, Søren Brandt +30

We describe the Spectroscopic Time-Resolving Observatory for Broadband Energy X-rays (STROBE-X), a probe-class mission concept that will provide an unprecedented view of the X-ray…

astro-ph.HE2018★ 38 cited

Analysis of Sub-threshold Short Gamma-ray Bursts in Fermi GBM Data

D. Kocevski, E. Burns, A. Goldstein +11

The Fermi Gamma-ray Burst Monitor (GBM) is currently the most prolific detector of Gamma-Ray Bursts (GRBs). Recently the detection rate of short GRBs (SGRBs) has been dramatically…

astro-ph.HE2018★ 19 cited

Gamma-ray burst models in light of the GRB 170817A - GW170817 connection

P. Veres, P. Mészáros, A. Goldstein +8

For the first time, a short gamma-ray burst (GRB) was unambiguously associated with a gravitational wave (GW) observation from a binary neutron star (NS) merger. This allows us to…