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

Kód výsledku v IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216208%3A11320%2F18%3A10388124" target="_blank" >RIV/00216208:11320/18:10388124 - isvavai.cz</a>
Výsledek na webu
<a href="https://doi.org/10.1017/S1743921317011218" target="_blank" >https://doi.org/10.1017/S1743921317011218</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1017/S1743921317011218" target="_blank" >10.1017/S1743921317011218</a>

Jazyk výsledku
angličtina
Název v původním jazyce
Spatial distribution of the gamma-ray bursts at very high redshift
Popis výsledku v původním jazyce
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.
Název v anglickém jazyce
Spatial distribution of the gamma-ray bursts at very high redshift
Popis výsledku anglicky
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.

Projekt
—
Návaznosti
I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Rok uplatnění
2018
Kód důvěrnosti údajů
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

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