Number of the records: 1  

Recent highlights from the Pierre Auger Observatory

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    SYSNO ASEP0521558
    Document TypeC - Proceedings Paper (int. conf.)
    R&D Document TypeConference Paper
    TitleRecent highlights from the Pierre Auger Observatory
    Author(s) Boháčová, Martina (FZU-D) RID, ORCID
    Number of authors1
    Article number199
    Source TitleProceedings, 53rd Rencontres de Moriond on Electroweak Interactions and Unified Theories. - Paris : ARISF / LPNHE, 2018 ; Auge E. ; Dumarchez J. ; Tran Thanh Van J. - ISBN 9791096879076
    Pagess. 1-8
    Number of pages6 s.
    Publication formOnline - E
    ActionRencontres de Moriond on Electroweak Interactions and Unified Theories /53./ (Moriond EW 2018)
    Event date10.03.2018 - 17.03.2018
    VEvent locationLa Thuile
    CountryIT - Italy
    Event typeWRD
    Languageeng - English
    CountryFR - France
    Keywordscosmic rays ; air showers ; mass composition ; anizotropy searches
    Subject RIVBF - Elementary Particles and High Energy Physics
    OECD categoryParticles and field physics
    R&D ProjectsLTT18004 GA MŠMT - Ministry of Education, Youth and Sports (MEYS)
    LM2015038 GA MŠMT - Ministry of Education, Youth and Sports (MEYS)
    EF16_013/0001402 GA MŠMT - Ministry of Education, Youth and Sports (MEYS)
    Institutional supportFZU-D - RVO:68378271
    AnnotationUltrahigh-energy cosmic rays are the most energetic particles observed, reachingorders of magnitude above the LHC energy range. The Pierre Auger Observatory,located in Mendoza province, Argentina, is the largest ultrahigh-energy cosmicray observatory in the world. Since the start of operation in 2004, theObservatory has reached unprecedented exposure and the high-quality data setspans three orders of magnitude in energy, yielding a plethora of scientificfindings. A selection of recently published results on the large andintermediate scale anisotropies in ultrahigh-energy cosmic ray arrivaldirections and search for neutrinos correlated with GW170817 is being presentedin this contribution. Implications for the future operation and motivations forthe Observatory upgrade are also briefly outlined.


    WorkplaceInstitute of Physics
    ContactKristina Potocká, potocka@fzu.cz, Tel.: 220 318 579
    Year of Publishing2020
Number of the records: 1  

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