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Gamma-Ray Burst Energetics in the Swift Era

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Daniel Kocevski1 and Nathaniel Butler1

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[1]

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The Afterglows of Swift-era Gamma-Ray Bursts. II. Type I GRB versus Type II GRB Optical Afterglows

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Afterglow Observations of Fermi Large Area Telescope Gamma-ray Bursts and the Emerging Class of Hyper-energetic Events

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The Afterglows of Swift-era Gamma-ray Bursts. I. Comparing pre-Swift and Swift-era Long/Soft (Type II) GRB Optical Afterglows

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A New Class of Gamma-ray Bursts from Stellar Disruptions by Intermediate-mass Black Holes

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The Collimation and Energetics of the Brightest Swift Gamma-ray Bursts

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The Cosmic Rate, Luminosity Function, and Intrinsic Correlations of Long Gamma-Ray Bursts

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Discerning the Physical Origins of Cosmological Gamma-ray Bursts Based on Multiple Observational Criteria: The Cases of z = 6.7 GRB 080913, z = 8.2 GRB 090423, and Some Short/Hard GRBs

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[9]

A New Paradigm for Gamma-ray Bursts: Long-term Accretion Rate Modulation by an External Accretion Disk

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Prompt High-Energy Emission from Proton-Dominated Gamma-Ray Bursts

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Jet Breaks and Energetics of Swift Gamma-Ray Burst X-Ray Afterglows

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[12]

Generalized Tests for Selection Effects in Gamma-Ray Burst High-Energy Correlations

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[13]

Revealing the High-Redshift Star Formation Rate with Gamma-Ray Bursts

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Observations of the Prompt Gamma-Ray Emission of GRB 070125

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A Comprehensive Study of GRB 070125, A Most Energetic Gamma-Ray Burst

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The Rapid Decline of the Prompt Emission in Gamma-Ray Bursts

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[17]

Jet Breaks and Missing Breaks in the X-Ray Afterglow of Gamma-Ray Bursts

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