Wavelet Analysis of the BATSE 64ms GRB Lightcurves

Details Wavelet Analysis of the BATSE 64ms GRB Lightcurves Wavelet Analysis of the BATSE 64ms GRB Lightcurves

Jun 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004aspc..312...51b&link_type=abstract

Third Rome Workshop on Gamma-Ray Bursts in the Afterglow Era ASP Conference Series, Volume 312, Proceedings of the conference he

Astronomy and Astrophysics

Astronomy

Scientific paper

A special wavelet transformation with a base function based on a Fast Rise-Exponential Decay (FRED) pulse is developed. Using BATSE 64ms total count data about half of the long (T50 ≥ 2s) bursts' lightcurves could be compressed with a ratio of 1:10 or better. The wavelet compression ratios show that >320 keV lightcurves compress better than the lower energy counterparts which indicates that they are more FRED-like than the lower energy ones.

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