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.

Autocorrelation analysis of GRBM--Beppo-SAX burst data

FRONTERA, Filippo;GUIDORZI, Cristiano;MONTANARI, Enrico;
2005

Abstract

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.
2005
Borgonovo, L; Frontera, Filippo; Guidorzi, Cristiano; Montanari, Enrico; Soffitta, P.
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11392/494484
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