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A template for describing intrinsic GRB pulse shapes

Publication ,  Journal Article
Hakkila, J; Loredo, TJ; Wolpert, RL; Broadbent, ME; Preece, RD
Published in: eConf C1304143
August 27, 2013

A preliminary study of a set of well-isolated pulses in GRB light curves indicates that simple pulse models, with smooth and monotonic pulse rise and decay regions, are inadequate. Examining the residuals of fits of pulses to such models suggests the following patterns of departure from the smooth pulse model of Norris et al. (2005): A Precursor Shelf occurs prior to or concurrent with the exponential Rapid Rise. The pulse reaches maximum intensity at the Peak Plateau, then undergoes a Rapid Decay. The decay changes into an Extended Tail. Pulses are almost universally characterized by hard-to-soft evolution, arguing that the new pulse features reflect a single physical phenomenon, rather than artifacts of pulse overlap.

Duke Scholars

Published In

eConf C1304143

Publication Date

August 27, 2013

Volume

24

Start / End Page

2013
 

Citation

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Hakkila, J., Loredo, T. J., Wolpert, R. L., Broadbent, M. E., & Preece, R. D. (2013). A template for describing intrinsic GRB pulse shapes. EConf C1304143, 24, 2013.
Hakkila, Jon, Thomas J. Loredo, Robert L. Wolpert, Mary E. Broadbent, and Robert D. Preece. “A template for describing intrinsic GRB pulse shapes.” EConf C1304143 24 (August 27, 2013): 2013.
Hakkila J, Loredo TJ, Wolpert RL, Broadbent ME, Preece RD. A template for describing intrinsic GRB pulse shapes. eConf C1304143. 2013 Aug 27;24:2013.
Hakkila, Jon, et al. “A template for describing intrinsic GRB pulse shapes.” EConf C1304143, vol. 24, Aug. 2013, p. 2013.
Hakkila J, Loredo TJ, Wolpert RL, Broadbent ME, Preece RD. A template for describing intrinsic GRB pulse shapes. eConf C1304143. 2013 Aug 27;24:2013.

Published In

eConf C1304143

Publication Date

August 27, 2013

Volume

24

Start / End Page

2013