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19962020
most citedThe Fermi Gamma-Ray Burst Monitor

1.6k citations · 7.8k across the 89 of their papers we have counts for

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Showing 2014Show all

9 papers · 1 filter

astro-ph.IM2014★ 131 cited

Localization of Gamma-Ray Bursts using the Fermi Gamma-Ray Burst Monitor

V. Connaughton, M. S. Briggs, A. Goldstein +25

The Fermi Gamma-ray Burst Monitor (GBM) has detected over 1400 Gamma-Ray Bursts (GRBs) since it began science operations in July, 2008. We use a subset of over 300 GRBs localized b…

astro-ph.HE2014★ 28 cited

Swift and Fermi observations of X-ray flares: the case of Late Internal Shock

E. Troja, L. Piro, V. Vasileiou +5

Simultaneous Swift and Fermi observations of gamma-ray bursts (GRBs) offer a unique broadband view of their afterglow emission, spanning more than ten decades in energy. We present…

astro-ph.HE2014★ 31 cited

Synchrotron Cooling in Energetic Gamma-Ray Bursts Observed by the Fermi Gamma-Ray Burst Monitor

Hoi-Fung Yu, Jochen Greiner, Hendrik van Eerten +15

We study the time-resolved spectra of eight GRBs observed by Fermi GBM in its first five years of mission, with 1 keV - 1 MeV fluence erg cm and signal-…

astro-ph.HE2014★ 84 cited

High-energy electromagnetic offline follow-up of LIGO-Virgo gravitational-wave binary coalescence candidate events

Lindy Blackburn, Michael S. Briggs, Jordan Camp +5

We present two different search methods for electromagnetic counterparts to gravitational-wave (GW) events from ground-based detectors using archival NASA high-energy data from the…

astro-ph.HE2014★ 32 cited

An Observed Correlation Between Thermal and Non-Thermal Emission in Gamma-Ray Bursts

J. Michael Burgess, Robert D. Preece, Felix Ryde +22

Recent observations by the Gamma-ray Space Telescope have confirmed the existence of thermal and non-thermal components in the prompt photon spectra of some Gamma-ray burst…

astro-ph.HE2014★ 33 cited

Cherenkov Telescope Array is Well Suited to Follow Up Gravitational Wave Transients

Imre Bartos, Peter Veres, Daniel Nieto +8

The first gravitational-wave (GW) observations will greatly benefit from the detection of coincident electromagnetic counterparts. Electromagnetic follow-ups will nevertheless be c…