Highlights from the Pierre Auger Observatory

Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68378271%3A_____%2F17%3A00522168" target="_blank" >RIV/68378271:_____/17:00522168 - isvavai.cz</a>
Result on the web
<a href="https://www.sciencedirect.com/science/article/pii/S2405601417303966?via%3Dihub" target="_blank" >https://www.sciencedirect.com/science/article/pii/S2405601417303966?via%3Dihub</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1016/j.nuclphysbps.2017.06.017" target="_blank" >10.1016/j.nuclphysbps.2017.06.017</a>

Result language
angličtina
Original language name
Highlights from the Pierre Auger Observatory
Original language description
The Pierre Auger Observatory, based in Mendoza province, Argentina represents the largest ultrahigh-energy cosmic ray observatory ever built. After twelve years of operation the exposure reached almost 60 000 km2 sr yr and the unprecedented quality data set spans three orders of magnitude in energy. The status and performance of the detectors and their enhancements are described. The rich harvest of the results obtained so far is presented including the energy spectrum, searches for anisotropy, measurement of the position of shower maximum and their interpretation in terms of mass composition as well as limits on photons and neutrinos in the primary flux. Implications of the results on future operation and motivations for the upgrade of the Observatory are also discussed.
Czech name
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Czech description
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Project
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Continuities
I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Publication year
2017
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

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