The feasibility of independent observations and detections of GRBs in X rays
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F11%3A00373099" target="_blank" >RIV/67985815:_____/11:00373099 - 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
The feasibility of independent observations and detections of GRBs in X rays
Original language description
According to the observational statistics a large majority of all GRBs exhibit X ray emission. In addition, a dedicated separate group of GRB, the XRFs, exists which emission dominates in the X ray spectral range. And the third group of GRB related objects (yet hypothetical) are the group of off-axis observed GRBs (orphan afterglows). These facts justify the consideration of an independent experiment for monitoring, detection and analyses of GRBs and others fast X ray transients in X rays. We will present and discuss such experiment based on wide-field X ray telescopes of Lobster Eye type. The wide field and fine sensitivity of Lobster Eye X ray All Sky Monitor make such instruments important tools in study of GRBs and related objects.
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
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Continuities
Z - Vyzkumny zamer (s odkazem do CEZ)
Others
Publication year
2011
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 2010
ISBN
978-0-7354-0916-3
ISSN
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e-ISSN
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Number of pages
4
Pages from-to
423-426
Publisher name
American Institute of Physics
Place of publication
Melville
Event location
Annapolis
Event date
Nov 1, 2010
Type of event by nationality
WRD - Celosvětová akce
UT code for WoS article
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