Synergies between CTA and VLBI

Kód výsledku v IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68378271%3A_____%2F19%3A00552376" target="_blank" >RIV/68378271:_____/19:00552376 - isvavai.cz</a>
Výsledek na webu
<a href="https://pos.sissa.it/344/047/pdf" target="_blank" >https://pos.sissa.it/344/047/pdf</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.22323/1.344.0047" target="_blank" >10.22323/1.344.0047</a>

Jazyk výsledku
angličtina
Název v původním jazyce
Synergies between CTA and VLBI
Popis výsledku v původním jazyce
Gamma rays are produced by the most powerful and often explosive physical processes in the Universe. Understanding the origin and role of relativistic cosmic particles in galactic and extragalactic objects is among the key issue that will be addressed by the Cherenkov Telescope Array (CTA). With its huge improvement in sensitivity, angular resolution, energy range, and flexibility of operation, CTA will provide a step forward in our understanding of the gamma-ray emission in transients and active galactic nuclei (AGN).n
Název v anglickém jazyce
Synergies between CTA and VLBI
Popis výsledku anglicky
Gamma rays are produced by the most powerful and often explosive physical processes in the Universe. Understanding the origin and role of relativistic cosmic particles in galactic and extragalactic objects is among the key issue that will be addressed by the Cherenkov Telescope Array (CTA). With its huge improvement in sensitivity, angular resolution, energy range, and flexibility of operation, CTA will provide a step forward in our understanding of the gamma-ray emission in transients and active galactic nuclei (AGN).n

Rok uplatnění
2019
Kód důvěrnosti údajů
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

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