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Spatial distribution of the gamma-ray bursts at very high redshift

Published online by Cambridge University Press:  08 May 2018

Attila Mészáros Open the ORCID record for Attila Mészáros [Opens in a new window]
Attila Mészáros*
Affiliation:
Charles University, Faculty of Mathematics and Physics, Astronomical Institute, V Holešovičkách 2, Prague 8, Czech Republic, email:[email protected]
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Abstract

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The author - with his collaborators - already in years 1995-96 have shown - purely from the analyses of the observations - that the gamma-ray bursts (GRBs) can be till redshift 20. Since that time several other statistical studies of the spatial distribution of GRBs were provided. Remarkable conclusions concerning the star-formation rate and the validity of the cosmological principle were obtained about the regions of the cosmic dawn. In this contribution these efforts are surveyed.

Keywords

Cosmology: large-scale structure of the UniverseobservationsmiscellaneousStars: gamma-ray bursts
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 12 , Symposium S333: Peering towards Cosmic Dawn , October 2017 , pp. 203 - 206
Copyright
Copyright © International Astronomical Union 2018 

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