activity
20012022
most citedThe Fermi Gamma-Ray Burst Monitor

1.6k citations · 9.9k across the 74 of their papers we have counts for

collaborators
Showing 2014Show all

8 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★ 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★ 33 cited

GROND coverage of the main peak of Gamma-Ray Burst 130925A

J. Greiner, H. -F. Yu, T. Krühler +23

Prompt or early optical emission in gamma-ray bursts is notoriously difficult to measure, and observations of the dozen cases show a large variety of properties. Yet, such early em…

astro-ph.HE2014★ 67 cited

Quasi-Periodic Oscillations in Short Recurring Bursts of the Soft-Gamma Repeater J1550-5418

Daniela Huppenkothen, Caroline D'Angelo, Anna L. Watts +11

The discovery of quasi-periodic oscillations (QPOs) in magnetar giant flares has opened up prospects for neutron star asteroseismology. The scarcity of giant flares makes a search…

astro-ph.HE2014★ 39 cited

Time resolved spectroscopy of SGR J1550-5418 bursts detected with Fermi/GBM

G. Younes, C. Kouveliotou, A. J. van der Horst +18

We report on time-resolved spectroscopy of the 63 brightest bursts of SGR J1550-5418, detected with Fermi/Gamma-ray Burst Monitor during its 2008-2009 intense bursting episode. We…

astro-ph.HE2014★ 53 cited

A Missing-Link in the Supernova-GRB Connection: The Case of SN 2012ap

Sayan Chakraborti, Alicia Soderberg, Laura Chomiuk +50

Gamma Ray Bursts (GRBs) are characterized by ultra-relativistic outflows, while supernovae are generally characterized by non-relativistic ejecta. GRB afterglows decelerate rapidly…