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gptkbp:instanceOf
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cosmic ray observatory
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gptkbp:affiliation
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gptkb:International_Union_of_Pure_and_Applied_Physics
gptkb:International_Cosmic_Ray_Conference
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gptkbp:collaboratesWith
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over 500 scientists
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gptkbp:country
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gptkb:Argentina
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gptkbp:elevation
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1400 meters
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gptkbp:established
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2000
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gptkbp:fundedBy
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gptkb:treaty
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https://www.w3.org/2000/01/rdf-schema#label
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Pierre Auger Observatory
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gptkbp:location
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gptkb:Malargüe,_Mendoza_Province,_Argentina
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gptkbp:namedAfter
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gptkb:Pierre_Auger
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gptkbp:notableFinds
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anisotropy in arrival directions of cosmic rays
evidence for extragalactic origin of ultra-high-energy cosmic rays
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gptkbp:numberOfFluorescenceTelescopes
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27
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gptkbp:numberOfSurfaceDetectors
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1600
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gptkbp:operatedBy
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gptkb:Pierre_Auger_Collaboration
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gptkbp:purpose
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study ultra-high-energy cosmic rays
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gptkbp:releaseDate
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public data available
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gptkbp:researchArea
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astroparticle physics
cosmic ray physics
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gptkbp:sensorType
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fluorescence telescope
water Cherenkov detector
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gptkbp:servesArea
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3000 square kilometers
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gptkbp:troopContributingCountries
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over 17 countries
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gptkbp:website
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https://www.auger.org/
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gptkbp:bfsParent
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gptkb:NA61/SHINE
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gptkbp:bfsLayer
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4
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