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most citedFermi Large Area Telescope Second Source Catalog

1.3k citations · 19.5k across the 113 of their papers we have counts for

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astro-ph2006★ 53 cited

Extreme Properties Of GRB061007: A Highly Energetic OR Highly Collimated Burst?

P. Schady, M. De Pasquale, J. Cummings +20

%auto-ignore This paper has been withdrawn by the authors due to dublicate submission. To download the paper please go to astro-ph/0611081

astro-ph2006★ 3 cited

Extreme Properties Of GRB061007: A Highly Energetic Or A Highly Collimated Burst?

P. Schady, M. De Pasquale, M. J. Page +20

GRB061007 is the brightest gamma-ray burst (GRB) to be detected by Swift and is accompanied by an exceptionally luminous afterglow that had a V-band magnitude <11.1 at 80s after th…

astro-ph2006★ 68 cited

Temporal Profiles and Spectral Lags of XRF 060218

En-Wei Liang, Bin-Bin Zhang, Mike Stamatikos +5

The spectral and temporal properties of the non-thermal emission ofthe nearby XRF 060218 in 0.3-150 keV band are studied. We show that both the spectral energy distribution and the…

astro-ph2006★ 556 cited

Swift detects a remarkable gamma-ray burst, GRB 060614, that introduces a new classification scheme

N. Gehrels, J. P. Norris, V. Mangano +19

Gamma ray bursts (GRBs) are known to come in two duration classes, separated at ~2 s. Long bursts originate from star forming regions in galaxies, have accompanying supernovae (SNe…

astro-ph2006★ 2 cited

An Algorithm for Detecting Quantum-Gravity Photon Dispersion in Gamma-Ray Bursts: DISCAN

Jeffrey D. Scargle, Jay P. Norris, Jerry T. Bonnell

DisCan is a new algorithm implementing photon dispersion cancellation in order to measure energy-dependent delays in variable sources. This method finds the amount of reversed disp…

astro-ph2006

GRB 050717: A Long, Short-Lag, High Peak Energy Burst Observed by Swift and Konus

H. A. Krimm, C. Hurkett, V. Pal'shin +10

The long burst GRB 050717 was observed simultaneously by the Burst Alert Telescope (BAT) on Swift and the Konus instrument on Wind. Significant hard to soft spectral evolution was…