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

2017 ◽  
Vol 12 (S333) ◽  
pp. 203-206
Author(s):  
Attila Mészáros

AbstractThe 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.

2008 ◽  
Vol 683 (1) ◽  
pp. L5-L8 ◽  
Author(s):  
Hasan Yüksel ◽  
Matthew D. Kistler ◽  
John F. Beacom ◽  
Andrew M. Hopkins

1998 ◽  
Vol 506 (2) ◽  
pp. L81-L84 ◽  
Author(s):  
Mark Krumholz ◽  
S. E. Thorsett ◽  
Fiona A. Harrison

2009 ◽  
Vol 5 (S265) ◽  
pp. 73-74
Author(s):  
Attila Mészáros ◽  
Jakub Řípa ◽  
David Huja

AbstractThe long gamma-ray bursts are at high redshifts, and they trace the star-formation rate. Hence, they may well serve as milestones in the early Universe.


2012 ◽  
Vol 8 (S292) ◽  
pp. 334-334
Author(s):  
Attila Mészáros ◽  
Zsolt Bagoly ◽  
Lajos G. Balázs ◽  
István Horváth

AbstractIt is remarkable that the long gamma-ray bursts, as objects connected with the supernovae - i.e. with the end of the massive stars, trace the star formation rate. This connection is discussed in this contribution. The presentation is in essence a recapitulation of the article Mészáros A. et al. A&A, 2006, 455, 785.


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