Autocorrelation analysis of GRBM--Beppo-SAX burst data

Details Autocorrelation analysis of GRBM--Beppo-SAX burst data Autocorrelation analysis of GRBM--Beppo-SAX burst data

May 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005ncimc..28..275b&link_type=abstract

Il Nuovo Cimento C, vol. 28, Issue 3, p.275

Physics

1

Scientific paper

An autocorrelation function (ACF) analysis was performed on 17 gamma-ray bursts with known redshift, using data from the GRBM on board Beppo-SAX. When corrected from the cosmic time dilation effect, the ACFs show a bimodal distribution at about half-maximum, in agreement with a previous study based on BATSE and Konus burst data. Although the results show more dispersion, the separation between the two classes is highly significant.

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