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
- DOI
- 10.1063/1.3621778;
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