2022MNRAS.517.5770Z


Query : 2022MNRAS.517.5770Z

2022MNRAS.517.5770Z - Mon. Not. R. Astron. Soc., 517, 5770-5779 (2022/December-3)

Distribution of gamma-ray bursts on the T90-HR plane and their classification revisited.

ZHANG L., LUO J.-J., HUANG Y.-F., GONG Y.-J. and WU S.

Abstract (from CDS):

Using four mixed bivariate distributions (Normal distribution, Skew-Normal distribution, Student distribution, Skew-Student distribution) and bootstrap re-sampling analysis. We analyse the samples of CGRO/BATSE, Swift/BAT, and Fermi/GBM gamma-ray bursts in detail on the T90-HR (Hardness Ratio) plane. The Bayesian information criterion is used to judge the goodness of fit for each sample, comprehensively. It is found that all the three samples show a symmetric (either Normal or Student) distribution. It is also found that the existence of three classes of gamma-ray bursts is preferred by the three samples, but the strength of this preference varies with the sample size: when the sample size of the data set is larger, the preference of three classes scheme becomes weaker. Therefore, the appearance of an intermediate class may be caused by a small sample size and the possibility that there are only two classes of gamma-ray bursts still cannot be expelled yet. A further bootstrap re-sampling analysis also confirms this result.

Abstract Copyright: © 2022 The Author(s) Published by Oxford University Press on behalf of Royal Astronomical Society

Journal keyword(s): methods: data analysis - methods: statistical - gamma-ray bursts

Simbad objects: 4

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Number of rows : 4
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 GRB 220101A gB 00 05 24.89 +31 46 07.7           ~ 85 0
2 GRB 220325A gB 17 57 57.00 -07 02 09.3           ~ 15 0
3 PSR J1808-2024 Psr 18 08 39.32 -20 24 40.1           ~ 1316 2
4 GRB 211225B gB ~ ~           ~ 6 0

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