Gamma-ray Bursts in Wavelet Space

Details Gamma-ray Bursts in Wavelet Space Gamma-ray Bursts in Wavelet Space

2005-08-31

arxiv.org/abs/astro-ph/0508673v1

AIP Conf.Proc.727:94-97,2004

Astronomy and Astrophysics

Astrophysics

GRB: 30 years of Discovery. ed by E.E. Fenimore and M. Galassi

Scientific paper

10.1063/1.1810809

The gamma-ray burst's lightcurves have been analyzed using a special wavelet transformation. The applied wavelet base is based on a typical Fast Rise-Exponential Decay (FRED) pulse. The shape of the wavelet coefficients' total distribution is determined on the observational frequency grid. Our analysis indicates that the pulses in the long bursts' high energy channel lightcurves are more FRED-like than the lower ones, independently from the actual physical time-scale.

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