Highlights from the Pierre Auger Observatory

Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68378271%3A_____%2F19%3A00521546" target="_blank" >RIV/68378271:_____/19:00521546 - isvavai.cz</a>
Result on the web
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DOI - Digital Object Identifier
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Result language
angličtina
Original language name
Highlights from the Pierre Auger Observatory
Original language description
The Pierre Auger Observatory, the largest cosmic ray detector in the world, was built to study the cosmic rays with ????>10^17 eV with unprecedented statistics. Recently it has determined, with a 5.2???? significance, that the arrival directions of cosmic rays with energies above 8EeV are anisotropic and can be described by a dipole whose direction favors an extragalactic origin of Ultra-High Energy Cosmic Rays. At an intermediate angular scale, the two largest departures from isotropy for the arrival directions of events with ????>39EeV and ????>60EeV are best described by a correlation with two nearby populations of extragalactic gamma-ray sources, namely starburst galaxies and AGNs. In the multi-messenger astronomy era, Auger is actively participating in neutrino searches in coincidence with gravitational wave events.nn
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)

Publication year
2019
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Article name in the collection
Proceedings of Science. 36th International Cosmic Ray Conference ICRC2019
ISBN
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ISSN
1824-8039
e-ISSN
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Number of pages
23
Pages from-to
1-23
Publisher name
Proceedings of Science
Place of publication
Trieste
Event location
Madison
Event date
Jul 24, 2019
Type of event by nationality
WRD - Celosvětová akce
UT code for WoS article
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