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- W2018753375 abstract "We study a sample of bright, long Burst and Transient Source Experiment (BATSE) gamma-ray burst (GRB) light curves in the 200 s before the detection of the GRB prompt emission. We find that in a sizable fraction of cases (∼20 per cent) there is evidence of emission above the background coming from the same direction as the GRB. This emission is characterized by a softer spectrum with respect to the main spectrum and contains a small fraction (0.1–1 per cent) of the total event counts. The precursors have typical delays of several tens of seconds extending (in few cases) up to 200 s (the limit of the investigated period). Their spectra are typically non-thermal power-law spectra, aside from a few cases. Such long delays and the non-thermal origin of their spectra are hard to reconcile with any model for the progenitor." @default.
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- W2018753375 date "2005-02-01" @default.
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- W2018753375 title "Precursor activity in bright, long BATSE gamma-ray bursts" @default.
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- W2018753375 doi "https://doi.org/10.1111/j.1365-2966.2005.08687.x" @default.
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