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Spatial distribution of GRBs and large scale structure of the Universe

Published online by Cambridge University Press:  17 August 2016

Zsolt Bagoly ,
István I. Rácz ,
Lajos G. Balázs ,
L. Viktor Tóth  and
István Horváth
Zsolt Bagoly
Affiliation:
Eötvös University, Budapest, email: zsolt.bagoly@ttk.elte.hu
István I. Rácz
Affiliation:
Eötvös University, Budapest, email: zsolt.bagoly@ttk.elte.hu Konkoly Observatory of the Hungarian Academy of Sciences, Budapest
Lajos G. Balázs
Affiliation:
Eötvös University, Budapest, email: zsolt.bagoly@ttk.elte.hu Konkoly Observatory of the Hungarian Academy of Sciences, Budapest
L. Viktor Tóth
Affiliation:
Eötvös University, Budapest, email: zsolt.bagoly@ttk.elte.hu
István Horváth
Affiliation:
National University of Public Service, Budapest
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Abstract

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We studied the space distribution of the starburst galaxies from Millennium XXL database at z = 0.82. We examined the starburst distribution in the classical Millennium I (De Lucia et al. (2006)) using a semi-analytical model for the genesis of the galaxies. We simulated a starburst galaxies sample with Markov Chain Monte Carlo method. The connection between the large scale structures homogenous and starburst groups distribution (Kofman and Shandarin 1998), Suhhonenko et al. (2011), Liivamägi et al. (2012), Park et al. (2012), Horvath et al. (2014), Horvath et al. (2015)) on a defined scale were checked too.

Keywords

methods: data analysismethods: numericalmethods: n-body simulationsgalaxies: structurecosmology: observationsgamma rays: observations
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. 3 - 4
Copyright
Copyright © International Astronomical Union 2016 

References

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