A physically-based flux characteristic for gamma-ray bursts is proposed that consists of the photon flux in a particular energy range positioned at the peak of the energy spectrum accumulated during the sum of emission time intervals. LogN-LogF distributions are investigated using these fluxes for bright BATSE bursts with peak fluxes on the 64 ms time scale larger than 2 ph/cm2⋅s.
Topics
Gamma ray bursts
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© 2000 American Institute of Physics.
2000
American Institute of Physics
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