Statistical differences between swift gamma-ray burst classes based on γ- And x-ray observations

Dorottya Szécsi, Lajos G. Balázs, Zsolt Bagoly, István Horváth, Attila Mészáros, Péter Veres

Research output: Conference contribution

Abstract

There are number of evidences that the gamma-ray bursts (GRBs) have a third group beside the short and long ones: The intermediate group. Although at this time, no reasonable physical explanation is known for them. We use discriminant analysis to confirm the former classification and give some further physical properties for the intermediate GRBs.

Original languageEnglish
Title of host publicationStatistical Challenges in Modern Astronomy V
PublisherSpringer Science and Business Media, LLC
Pages547-549
Number of pages3
ISBN (Print)9781461435198
DOIs
Publication statusPublished - 2012
Event5th Statistical Challenges in Modern Astronomy Symposium, SCMA 2011 - University Park, PA, United States
Duration: jún. 13 2011jún. 15 2011

Publication series

NameLecture Notes in Statistics
Volume209
ISSN (Print)0930-0325
ISSN (Electronic)2197-7186

Other

Other5th Statistical Challenges in Modern Astronomy Symposium, SCMA 2011
CountryUnited States
CityUniversity Park, PA
Period6/13/116/15/11

ASJC Scopus subject areas

  • Statistics and Probability
  • Statistics, Probability and Uncertainty

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    Szécsi, D., Balázs, L. G., Bagoly, Z., Horváth, I., Mészáros, A., & Veres, P. (2012). Statistical differences between swift gamma-ray burst classes based on γ- And x-ray observations. In Statistical Challenges in Modern Astronomy V (pp. 547-549). (Lecture Notes in Statistics; Vol. 209). Springer Science and Business Media, LLC. https://doi.org/10.1007/978-1-4614-3520-4_65