6533b85dfe1ef96bd12be9b8
RESEARCH PRODUCT
Correlation of the highest-energy cosmic rays with nearby extragalactic objects.
J. AbrahamP. AbreuM. AgliettaC. AguirreD. AllardI. AllekotteJ. AllenP. AllisonJ. Alvarez MunizM. AmbrosioL. AnchordoquiS. AndringaA. AnzaloneC. AramoS. Argiro'K. ArisakaE. ArmengaudF. ArneodoF. ArqueroT. AschH. AsoreyP. AssisB. S. AtulugamaJ. AublinM. AveG. AvilaT. BackerD. BadagnaniA. F. BarbosaD. BarnhillS. L. C. BarrosoP. BauleoJ. J. BeattyT. BeauB. R. BeckerK. H. BeckerJ. A. BellidoS. BenzviC. BeratT. BergmannX. BertouP. L. BiermannP. BilloirO. Blanch BigasF. BlancoP. BlasiC. BleveH. BlumerM. BohacovaC. BonifaziR. BoninoM. BoratavJ. BrackP. BrogueiraW. C. BrownP. BuchholzA. BuenoR. E. BurtonN. G. BuscaK. S. Caballero MoraB. CaiD. V. CaminL. CarameteR. CarusoW. CarvalhoA. CastellinaO. CatalanoG. CataldiL. CazonR. CesterJ. ChauvinA. ChiavassaJ. A. ChinellatoA. ChouJ. ChyeP. D. J. ClarkR. W. ClayE. ColomboR. ConceicaoB. ConnollyF. ContrerasJ. CoppensA. CordierU. CottiS. CoutuC. E. CovaultA. CreusotA. CrissJ. CroninA. CurutiuS. Dagoret CampagneK. DaumillerB. R. DawsonR. M. 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HorandelA. HornefferM. HorvatM. HrabovskyT. HuegeM. HussainM. IarloriA. InsoliaF. IonitaA. ItalianoM. KaducakK. H. KampertT. KarovaB. KeglB. KeilhauerE. KempR. M. KieckhaferH. O. KlagesM. KleifgesJ. KleinfellerR. KnapikJ. KnappD. H. KoangA. KriegerO. KromerD. KuempelN. KunkaA. KusenkoG. La RosaC. LachaudB. L. LagoD. LebrunP. LebrunJ. LeeM. A. Leigui De OliveiraA. Letessier SelvonM. LeutholdI. Lhenry YvonR. LopezA. Lopez AgueraJ. Lozano BahiloR. Luna GarciaM. C. MaccaroneC. MacolinoS. MalderaM. E. MancenidoD. MandatP. MantschA. G. MariazziI. C. MarisH. R. Marquez FalconJ. MartinezO. Martinez BravoH. J. MathesJ. MatthewsJ. A. J. MatthewsG. MatthiaeD. MaurizioP. O. MazurT. MccauleyM. McewenR. R. McneilM. C. MedinaG. Medina TancoA. MeliD. MeloE. MenichettiA. MenschikovC.h.r. MeurerR. MeyhandanM. I. MichelettiG. MieleW. MillerS. MollerachM. MonasorD. Monnier RagaigneF. MontanetB. MoralesC. MorelloJ. C. MorenoC. MorrisM. MostafaM. A. MullerR. MussaG. NavarraJ. L. NavarroS. NavasP. NecesalL. NellenC. Newman HolmesD. NewtonN. T. ThaoN. NierstenhoeferD. NitzD. NosekL. NozkaJ. OehlschlagerT. OhnukiA. OlintoV. M. Olmos GilbajaM. OrtizF. OrtolaniS. OstapchenkoL. OteroN. PachecoD. Pakk Selmi DeiM. PalatkaJ. PallottaG. ParenteE. ParizotS. ParlatiS. PastorM. PatelT. PaulV. PavlidouK. PayetM. PechJ. PekalaR. PelayoI. M. PepeS. PetreraP. PetrincaY. PetrovP. N. DiepP. N. DongP. T. NhungA. PichelR. PiegaiaT. PierogM. PimentaT. PintoV. PirronelloO. PisantiM. PlatinoJ. PochonP. PriviteraM. ProuzaE. J. QuelJ. RautenbergA. RedondoS. ReucroftB. RevenuF. A. S. RezendeJ. RidkyS. RiggiM. RisseC. RiviereV. RiziM. RobertsC. RobledoG. RodriguezM. D. Rodriguez FriasJ. RodriguezmartinoJ. Rodriguez RojoI. Rodriguez CaboG. RosJ. RosadoM. RothC. RoucelleB. Rouille' D’orfeuilE. RouletA. C. RoveroF. SalamidaH. SalazarG. SalinaF. SanchezM. SantanderC. E. SantoE. M. SantosF. SarazinS. SarkarR. SatoV. ScheriniH. SchielerA. SchmidtF. SchmidtT. SchmidtO. ScholtenP. SchovanekF. SchusslerS. J. SciuttoM. ScuderiA. SegretoD. SemikozM. SettimoR. C. ShellardI. SidelnikB. B. SiffertG. SiglN. Smetniansky De GrandeA. SmialkowskiR. SmidaA. G. K. SmithB. E. SmithG. R. SnowP. SokolskyP. SommersJ. SorokinH. SpinkaR. SquartiniE. StrazzeriA. StutzF. SuarezT. SuomijarviA. D. SupanitskyM. S. SutherlandJ. SwaincZ. SzadkowskiJ. TakahashiA. TamashiroA. TamburroO. TascauR. TcaciucD. ThomasR. TiconJ. TiffenbergC. TimmermansW. TkaczykC. J. Todero PeixotoB. Tome'A. TonachiniI. TorresD. TorresiP. TravnicekA. TripathiG. TristramD. TscherniakhovskiM. TuerosV. TunnicliffeR. UlrichM. UngerM. UrbanaJ. F. Valdes GaliciaI. ValinoL. ValoreA. M. Van Den BergV. Van ElewyckR. A. VazquezD. VebericA. VeigaA. VelardeT. VenterscV. VerziM. VidelL. VillasenorS. VorobiovL. VoyvodicH. WahlberO. WainberP. WalkerD. WarnerA. A. WatsonS. WesterhoffG. WieczorekL. WienckeB. WilczynskaH. WilczynskiC. WilemanM. G. WinnickH. WuaB. WundheilerT. YamamotoP. YounkE. ZasbD. ZavrtanikM. ZavrtanikA. ZechA. ZepedaM. ZiolkowskiPaolo BernardiniIvan De MitriGiovanni MancarellaDaniele MartelloLorenzo Perronesubject
Active galactic nucleus[SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]AstronomyAstrophysics::High Energy Astrophysical Phenomenaparticle source [cosmic radiation]Cosmic background radiationFOS: Physical sciencesFluxOsservatorio Pierre AugerCosmic rayanisotropyAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics01 natural sciences[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]Raggi cosmici0103 physical sciencesUltra-high-energy cosmic ray010303 astronomy & astrophysicsBackground radiationNuclei galattivi attiviPhysicsPierre Auger ObservatorySPECTRUMMultidisciplinary[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]010308 nuclear & particles physicsMedicine (all); MultidisciplinaryMedicine (all)Settore FIS/01 - Fisica SperimentaleAstrophysics (astro-ph)angular dependence [cosmic radiation]Astrophysics::Instrumentation and Methods for AstrophysicsFísicaEnergia ultra altaExperimental High Energy Physicsddc:500Energy (signal processing)experimental resultsdescription
Using data collected at the Pierre Auger Observatory during the past 3.7 years, we demonstrated a correlation between the arrival directions of cosmic rays with energy above ~ 6x10^{19} electron volts and the positions of active galactic nuclei (AGN) lying within ~ 75 megaparsecs. We rejected the hypothesis of an isotropic distribution of these cosmic rays with at least a 99% confidence level from a prescribed a priori test. The correlation we observed is compatible with the hypothesis that the highest energy particles originate from nearby extragalactic sources whose flux has not been substantially reduced by interaction with the cosmic background radiation. AGN or objects having a similar spatial distribution are possible sources.
year | journal | country | edition | language |
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2007-11-09 |