SIMBAD references

2001MNRAS.328..283B - Mon. Not. R. Astron. Soc., 328, 283-290 (2001/November-3)

Reclassification of gamma-ray bursts.

BALASTEGUI A., RUIZ-LAPUENTE P. and CANAL R.

Abstract (from CDS):

We have applied two different automatic classifier algorithms to the BATSE Current GRB Catalog data and we obtain three different classes of gamma-ray bursts (GRBs). Our results confirm the existence of a third, intermediate class of GRBs, with mean duration ∼ 25-50 s, as deduced from a cluster analysis and from a neural network algorithm. Our analyses imply longer durations than those found by Mukherjee et al. and Horváth, whose intermediate class had durations 2-10 s. From the neural network analysis no difference in hardness between the two longest classes is found, and from both methods we find that the intermediate-duration class constitutes the most homogeneous sample of GRBs in its space distribution, while the longest-duration class constitutes the most inhomogeneous one with <V/V_max>∼0.1, being thus the deepest population of GRBs with z_max∼10. The trend previously found in long bursts, of spatial inhomogeneity increasing with hardness, only holds for this new longest-duration class.

Abstract Copyright: The Royal Astronomical Society

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

Simbad objects: 2

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