Redshift distribution of gamma-ray bursts and star formation rate
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216208%3A11320%2F06%3A00206023" target="_blank" >RIV/00216208:11320/06:00206023 - isvavai.cz</a>
Result on the web
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DOI - Digital Object Identifier
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Alternative languages
Result language
angličtina
Original language name
Redshift distribution of gamma-ray bursts and star formation rate
Original language description
The redshift distribution of gamma-ray bursts from the BATSE Catalog is compared with the star formation rate. A method independent of the models of the gamma-ray bursts is used. The short and the long subgroups are studied separately. The distribution of the long bursts may be proportional to the star formation rate. For the short bursts this can also happen, but the proportionality is less evident.
Czech name
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Czech description
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Classification
Type
J<sub>x</sub> - Unclassified - Peer-reviewed scientific article (Jimp, Jsc and Jost)
CEP classification
BN - Astronomy and celestial mechanics, astrophysics
OECD FORD branch
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Result continuities
Project
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Continuities
S - Specificky vyzkum na vysokych skolach
Others
Publication year
2006
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Data specific for result type
Name of the periodical
Astronomy and Astrophysics
ISSN
0004-6361
e-ISSN
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Volume of the periodical
455
Issue of the periodical within the volume
3
Country of publishing house
DE - GERMANY
Number of pages
6
Pages from-to
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UT code for WoS article
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EID of the result in the Scopus database
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