Testing the Gamma-ray Burst Pulse Start Conjecture

We test the hypothesis that prompt gamma-ray burst (GRB) pulse emission starts simultaneously at all energies (the Pulse Start Conjecture). Our analysis, using a sample of BATSE bursts observed with four-channel, 64 ms data and performed using a pulse-fit model, generally supports this hypothesis fo...

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Veröffentlicht in:The Astrophysical journal 2009-11, Vol.705 (1), p.372-385
Hauptverfasser: Hakkila, Jon, Nemiroff, Robert J
Format: Artikel
Sprache:eng
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Zusammenfassung:We test the hypothesis that prompt gamma-ray burst (GRB) pulse emission starts simultaneously at all energies (the Pulse Start Conjecture). Our analysis, using a sample of BATSE bursts observed with four-channel, 64 ms data and performed using a pulse-fit model, generally supports this hypothesis for the Long GRB class, although a few discrepant pulses belong to bursts observed during times characterized by low signal-to-noise ratio, hidden pulses, and/or significant pulse overlap. The typical uncertainty in making this statement is
ISSN:0004-637X
1538-4357
DOI:10.1088/0004-637X/705/1/372