arXiv Analytics

Sign in

arXiv:0905.4821 [astro-ph.HE]AbstractReferencesReviewsResources

A comparison of the gamma-ray bursts detected by BATSE and Swift

D. Huja, A. Meszaros, J. Ripa

Published 2009-05-29Version 1

The durations of 388 gamma-ray bursts, detected by the Swift satellite, are studied statistically in order to search for their subgroups. Then the results are compared with the results obtained earlier from the BATSE database. The standard chi^2 test is used. Similarly to the BATSE database, the short and long subgroups are well detected also in the Swift data. Also the intermediate subgroup is seen in the Swift database. The whole sample of 388 GRBs gives a support for three subgroups.

Comments: 9 pages, 3 figures, accepted for publication in Astronomy and Astrophysics
Journal: Astronomy and Astrophysics, 504 (2009) 67-71
Categories: astro-ph.HE, astro-ph.CO
Related articles: Most relevant | Search more
arXiv:1001.2455 [astro-ph.HE] (Published 2010-01-14)
On the Intermediate Subgroup of the Gamma-Ray Bursts in the Swift Database
arXiv:1004.3420 [astro-ph.HE] (Published 2010-04-20)
A Search for the Intermediate Subgroup of Gamma-Ray Bursts in the Swift Dataset
arXiv:1003.2582 [astro-ph.HE] (Published 2010-03-12)
Observations, theory and implications of thermal emission from gamma-ray bursts