Published August 19, 2011 | Version v1
Journal article

Observational differences between Swift GRB classes

  • 1. Konkoly Observatory, Budapest (Hungary)
  • 2. Bolyai Military University, Budapest (Hungary)
  • 3. Eoetvoes University, Budapest (Hungary)

Description

There are accumulating evidences that GRBs have an intermediate group, beside the short and long classes. Based on the observational data available in the Swift table we compared the observational γ and X ray properties of GRBs making use the discriminant analysis of the multivariate mathematical statistics. The analysis resulted in two canonical discriminating functions giving the maximum separation between the groups. The first discriminating function is dominated by the γ and X-ray fluence while the second one is almost identical with the photon index.

Additional details

Identifiers

Publishing Information

Journal Title
AIP Conference Proceedings
Journal Volume
1358
Journal Issue
1
Journal Page Range
p. 231-234
ISSN
0094-243X
CODEN
APCPCS

Conference

Title
Gamma ray bursts 2010 conference
Dates
1-4 Nov 2010
Place
Annapolis, MD (United States)

INIS

Country of Publication
United States
Country of Input or Organization
International Atomic Energy Agency (IAEA)
INIS RN
43083671
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Resource subtype / Literary indicator
Conference
Descriptors DEI
ASTROPHYSICS; COSMIC PHOTONS; GAMMA ASTRONOMY; GAMMA RADIATION; MULTIVARIATE ANALYSIS; X RADIATION
Descriptors DEC
ASTRONOMY; BOSONS; COSMIC RADIATION; ELECTROMAGNETIC RADIATION; ELEMENTARY PARTICLES; IONIZING RADIATIONS; MASSLESS PARTICLES; MATHEMATICS; PHOTONS; PHYSICS; RADIATIONS; STATISTICS

Optional Information

Notes
(c) 2011 American Institute of Physics