The average spectral density contours of BATSE GRBs over the time/energy domain

Details The average spectral density contours of BATSE GRBs over the time/energy domain The average spectral density contours of BATSE GRBs over the time/energy domain

May 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998aipc..428..364a&link_type=abstract

Fourth Huntsville gamma-ray burst symposium. AIP Conference Proceedings, Volume 428, pp. 364-368 (1998).

Computer Science

Gamma-Ray Sources, Gamma-Ray Bursts, Gamma-Ray, Spectroscopy And Spectrophotometry

Scientific paper

Statistical studies of the spectral evolution of cosmic gamma-ray bursts are performed, based on the procedure of peak aligned averaging. Using BATSE data with 16 energy channels measured on the 2048 ms time scale, two-dimensional surfaces representing the average spectral density evolution are created for three intensity groups of bursts. The basic signatures of spectral density evolution are found for the group of brightest events. Comparisons are performed among the basic properties of the average spectral density evolution of three intensity groups of bright, medium and dim bursts.

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