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Anomalies in the GRBs' distribution

Published online by Cambridge University Press:  17 August 2016

Zsolt Bagoly ,
István Horváth ,
Jon Hakkila  and
L. Viktor Tóth
Zsolt Bagoly
Affiliation:
Eötvös University, Budapest, email: zsolt.bagoly@ttk.elte.hu
István Horváth
Affiliation:
National University of Public Service, Budapest
Jon Hakkila
Affiliation:
College of Charleston, Charleston, SC
L. Viktor Tóth
Affiliation:
Eötvös University, Budapest, email: zsolt.bagoly@ttk.elte.hu
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Abstract

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Gamma-ray bursts are the most luminous objects known: they outshine their host galaxies making them ideal candidates for probing large-scale structure. Earlier it has been found that the angular distribution of different groups of GRBs (long, intermediate and short) show deviation from the full randomness at different levels (e.g. Vavrek et al. (2008)).

In the current sample there are more than 361 GRBs with position and redshift: the large scale homogeneous and isotropic distribution were checked with nearest-neighbour tests and with the two-point correlation function.

Keywords

methods: data analysisgalaxies: high-redshiftgamma rays: burstscosmology: observations(cosmology:) large-scale structure of universe
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 11 , Symposium S319: Galaxies at High Redshift and Their Evolution Over Cosmic Time , August 2015 , pp. 2
Copyright
Copyright © International Astronomical Union 2016 

References

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