Synergies between CTA and VLBI
The result's identifiers
Result code in 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>
Result on the web
<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>
Alternative languages
Result language
angličtina
Original language name
Synergies between CTA and VLBI
Original language description
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
Czech name
—
Czech description
—
Classification
Type
D - Article in proceedings
CEP classification
—
OECD FORD branch
10303 - Particles and field physics
Result continuities
Project
—
Continuities
—
Others
Publication year
2019
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Data specific for result type
Article name in the collection
Proceedings of Science
ISBN
—
ISSN
1824-8039
e-ISSN
—
Number of pages
11
Pages from-to
1-11
Publisher name
Sissa Medilab srl
Place of publication
Trieste
Event location
Granada
Event date
Oct 8, 2019
Type of event by nationality
WRD - Celosvětová akce
UT code for WoS article
—