On the properties of the RHESSI intermediate-duration gamma-ray bursts

Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216208%3A11320%2F11%3A10105126" target="_blank" >RIV/00216208:11320/11:10105126 - isvavai.cz</a>
Result on the web
<a href="http://dx.doi.org/10.1063/1.3621782" target="_blank" >http://dx.doi.org/10.1063/1.3621782</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1063/1.3621782" target="_blank" >10.1063/1.3621782</a>

Result language
angličtina
Original language name
On the properties of the RHESSI intermediate-duration gamma-ray bursts
Original language description
The intermediate-duration gamma-ray bursts (GRBs) identified in the data of the RHESSI satellite are investigated with respect to their spectral lags, peak count rates, redshifts, supernova observations, and star formation rates of their host galaxies. Standard statistical tests like Kolmogorov-Smirnov and Student t-test are used. It is discussed whether these bursts belong to the group of so-called short or long GRBs, or if they significantly differ from both groups
Czech name
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Czech description
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Project
Result was created during the realization of more than one project. More information in the Projects tab.
Continuities
P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)<br>Z - Vyzkumny zamer (s odkazem do CEZ)<br>S - Specificky vyzkum na vysokych skolach

Publication year
2011
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

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