Gamma-ray Bursts in Wavelet Space
arXiv:astro-ph/0508673 · doi:10.1063/1.1810809
Abstract
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.
GRB: 30 years of Discovery. ed by E.E. Fenimore and M. Galassi