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20032009
most citedFermi Large Area Telescope Bright Gamma-ray Source List

513 citations · 2.4k across the 13 of their papers we have counts for

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astro-ph2008311 cited

From Shock Breakout to Peak and Beyond: Extensive Panchromatic Observations of the Type Ib Supernova 2008D associated with Swift X-ray Transient 080109

Maryam Modjaz, W. Li, N. Butler +38

We present extensive early photometric (ultraviolet through near-infrared) and spectroscopic (optical and near-infrared) data on supernova (SN) 2008D as well as X-ray data analysis…

astro-ph2008159 cited

Observations of the Naked-Eye GRB 080319B: Implications of Nature's Brightest Explosion

J. S. Bloom, D. A. Perley, W. Li +18

The first gamma-ray burst (GRB) confirmed to be bright enough to be seen with the naked eye, GRB 080319B at redshift z = 0.937, allowed for exquisite follow-up observations across…

astro-ph200888 cited

Generalized Tests for Selection Effects in GRB High-Energy Correlations

Nathaniel R. Butler, Daniel Kocevski, Joshua S. Bloom

Several correlations among parameters derived from modelling the high-energy properties of GRBs have been reported. We show that well-known examples of these have common features i…

astro-ph200769 cited

GRB Energetics in the Swift Era

Daniel Kocevski, Nathaniel Butler

We examine the rest frame energetics of 76 gamma-ray bursts (GRBs) with known redshift that were detected by the Swift spacecraft and monitored by the satellite's X-ray Telescope (…

astro-ph2007283 cited

A Complete Catalog of Swift GRB Spectra and Durations: Demise of a Physical Origin for Pre-Swift High-Energy Correlations

Nathaniel R. Butler, Daniel Kocevski, Joshua S. Bloom +1

We calculate durations and spectral paramaters for 218 Swift bursts detected by the BAT instrument between and including GRBs 041220 and 070509, including 77 events with measured r…

astro-ph200740 cited

X-ray Hardness Variations as an Internal/External Shock Diagnostic

Nathaniel R. Butler, Daniel Kocevski

The early, highly time-variable X-ray emission immediately following GRBs exhibits strong spectral variations that are unlike the temporally smoother emission which dominates after…