Spatial distribution of the gamma-ray bursts at very high redshift
The result's identifiers
Result code in 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>
Result on the web
<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>
Alternative languages
Result language
angličtina
Original language name
Spatial distribution of the gamma-ray bursts at very high redshift
Original language description
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.
Czech name
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Czech description
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Classification
Type
D - Article in proceedings
CEP classification
—
OECD FORD branch
10308 - Astronomy (including astrophysics,space science)
Result continuities
Project
—
Continuities
I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace
Others
Publication year
2018
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Data specific for result type
Article name in the collection
PEERING TOWARDS COSMIC DAWN
ISBN
978-1-107-19246-1
ISSN
1743-9213
e-ISSN
1743-9221
Number of pages
4
Pages from-to
203-206
Publisher name
CAMBRIDGE UNIV PRESS
Place of publication
CAMBRIDGE
Event location
Dubrovnik
Event date
Oct 2, 2017
Type of event by nationality
WRD - Celosvětová akce
UT code for WoS article
000455232000041