On the feasibility of independent detection of optical afterglows of GRBs.
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F01%3A01010125" target="_blank" >RIV/67985815:_____/01:01010125 - 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
On the feasibility of independent detection of optical afterglows of GRBs.
Original language description
It proves to be feasible that both flaring (OTs) as well as fanding (OAs) optical emission related to GRBs may be detected by optical sky patrols. The rate of OAs ans OTs may be higher than the rate of GRBs due to different beaming.
Czech name
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Czech description
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Classification
Type
D - Article in proceedings
CEP classification
BN - Astronomy and celestial mechanics, astrophysics
OECD FORD branch
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Result continuities
Project
Result was created during the realization of more than one project. More information in the Projects tab.
Continuities
Z - Vyzkumny zamer (s odkazem do CEZ)
Others
Publication year
2001
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Data specific for result type
Article name in the collection
Gamma-ray bursts in the afterglow era.
ISBN
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ISSN
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e-ISSN
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Number of pages
3
Pages from-to
402-404
Publisher name
Springer
Place of publication
Berlin
Event location
Řím [IT]
Event date
Oct 17, 2000
Type of event by nationality
WRD - Celosvětová akce
UT code for WoS article
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