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Correlation of the highest-energy cosmic rays with nearby extragalactic objects.

Authors :
Abraham J
Abreu P
Aglietta M
Aguirre C
Allard D
Allekotte I
Allen J
Allison P
Alvarez C
Alvarez-Muñiz J
Ambrosio M
Anchordoqui L
Andringa S
Anzalone A
Aramo C
Argirò S
Arisaka K
Armengaud E
Arneodo F
Arqueros F
Asch T
Asorey H
Assis P
Atulugama BS
Aublin J
Ave M
Avila G
Bäcker T
Badagnani D
Barbosa AF
Barnhill D
Barroso SL
Bauleo P
Beatty J
Beau T
Becker BR
Becker KH
Bellido JA
Benzvi S
Berat C
Bergmann T
Bernardini P
Bertou X
Biermann PL
Billoir P
Blanch-Bigas O
Blanco F
Blasi P
Bleve C
Blümer H
Bohácová M
Bonifazi C
Bonino R
Boratav M
Brack J
Brogueira P
Brown WC
Buchholz P
Bueno A
Busca NG
Caballero-Mora KS
Cai B
Camin DV
Caruso R
Carvalho W
Castellina A
Catalano O
Cataldi G
Cazón-Boado L
Cester R
Chauvin J
Chiavassa A
Chinellato JA
Chou A
Chye J
Clark PD
Clay RW
Colombo E
Conceição R
Connolly B
Contreras F
Coppens J
Cordier A
Cotti U
Coutu S
Covault CE
Creusot A
Cronin J
Dagoret-Campagne S
Daumiller K
Dawson BR
de Almeida RM
De Donato C
de Jong SJ
De La Vega G
de Mello Junior WJ
de Mello Neto JR
De Mitri I
de Souza V
Del Peral L
Deligny O
Selva AD
Fratte CD
Dembinski H
Di Giulio C
Diaz JC
Dobrigkeit C
D'Olivo JC
Dornic D
Dorofeev A
Dos Anjos JC
Dova MT
D'Urso D
Duvernois MA
Engel R
Epele L
Erdmann M
Escobar CO
Etchegoyen A
Facal San Luis P
Falcke H
Farrar G
Fauth AC
Fazzini N
Fernández A
Ferrer F
Ferry S
Fick B
Filevich A
Filipcic A
Fleck I
Fonte R
Fracchiolla CE
Fulgione W
García B
García Gámez D
Garcia-Pinto D
Garrido X
Geenen H
Gelmini G
Gemmeke H
Ghia PL
Giller M
Glass H
Gold MS
Golup G
Albarracin FG
Berisso MG
Herrero RG
Gonçalves P
Gonçalves do Amaral M
Gonzalez D
Gonzalez JG
González M
Góra D
Gorgi A
Gouffon P
Grassi V
Grillo A
Grunfeld C
Guardincerri Y
Guarino F
Guedes GP
Gutiérrez J
Hague JD
Hamilton JC
Hansen P
Harari D
Harmsma S
Harton JL
Haungs A
Hauschildt T
Healy MD
Hebbeker T
Heck D
Hojvat C
Holmes VC
Homola P
Hörandel J
Horneffer A
Horvat M
Hrabovsky M
Huege T
Iarlori M
Insolia A
Ionita F
Italiano A
Kaducak M
Kampert KH
Keilhauer B
Kemp E
Kieckhafer RM
Klages HO
Kleifges M
Kleinfeller J
Knapik R
Knapp J
Koang DH
Kopmann A
Krieger A
Krömer O
Kümpel D
Kunka N
Kusenko A
La Rosa G
Lachaud C
Lago BL
Lebrun D
Lebrun P
Lee J
Leigui de Oliveira MA
Letessier-Selvon A
Leuthold M
Lhenry-Yvon I
López R
Lopez Agüera A
Lozano Bahilo J
Maccarone MC
Macolino C
Maldera S
Malek M
Mancarella G
Manceñido ME
Mandat D
Mantsch P
Mariazzi AG
Maris IC
Martello D
Martínez J
Martínez Bravo O
Mathes HJ
Matthews J
Matthews JA
Matthiae G
Maurizio D
Mazur PO
McCauley T
McEwen M
McNeil RR
Medina MC
Medina-Tanco G
Meli A
Melo D
Menichetti E
Menschikov A
Meurer C
Meyhandan R
Micheletti MI
Miele G
Miller W
Mollerach S
Monasor M
Monnier Ragaigne D
Montanet F
Morales B
Morello C
Moreno E
Moreno JC
Morris C
Mostafá M
Muller MA
Mussa R
Navarra G
Navarro JL
Navas S
Nellen L
Newman-Holmes C
Newton D
Thi TN
Nierstenhöfer N
Nitz D
Nosek D
Nozka L
Oehlschläger J
Ohnuki T
Olinto A
Olmos-Gilbaja VM
Ortiz M
Ostapchenko S
Otero L
Pakk Selmi-Dei D
Palatka M
Pallotta J
Parente G
Parizot E
Parlati S
Pastor S
Patel M
Paul T
Pavlidou V
Payet K
Pech M
Pekala J
Pelayo R
Pepe IM
Perrone L
Petrera S
Petrinca P
Petrov Y
Ngoc D
Ngoc D
Pham Thi TN
Pichel A
Piegaia R
Pierog T
Pimenta M
Pinto T
Pirronello V
Pisanti O
Platino M
Pochon J
Porter TA
Privitera P
Prouza M
Quel EJ
Rautenberg J
Reucroft S
Revenu B
Rezende FA
Rídky J
Riggi S
Risse M
Rivière C
Rizi V
Roberts M
Robledo C
Rodriguez G
Rodríguez Frías D
Rodriguez Martino J
Rodriguez Rojo J
Rodriguez-Cabo I
Ros G
Rosado J
Roth M
Rouillé-d'Orfeuil B
Roulet E
Rovero AC
Salamida F
Salazar H
Salina G
Sánchez F
Santander M
Santo CE
Santos EM
Sarazin F
Sarkar S
Sato R
Scherini V
Schieler H
Schmidt F
Schmidt T
Scholten O
Schovánek P
Schüssler F
Sciutto SJ
Scuderi M
Segreto A
Semikoz D
Settimo M
Shellard RC
Sidelnik I
Siffert BB
Sigl G
De Grande NS
Smialkowski A
Smída R
Smith AG
Smith BE
Snow GR
Sokolsky P
Sommers P
Sorokin J
Spinka H
Squartini R
Strazzeri E
Stutz A
Suarez F
Suomijärvi T
Supanitsky AD
Sutherland MS
Swain J
Szadkowski Z
Takahashi J
Tamashiro A
Tamburro A
Tascau O
Tcaciuc R
Thomas D
Ticona R
Tiffenberg J
Timmermans C
Tkaczyk W
Todero Peixoto CJ
Tomé B
Tonachini A
Torresi D
Travnicek P
Tripathi A
Tristram G
Tscherniakhovski D
Tueros M
Tunnicliffe V
Ulrich R
Unger M
Urban M
Valdés Galicia JF
Valiño I
Valore L
van den Berg AM
van Elewyck V
Vázquez RA
Veberic D
Veiga A
Velarde A
Venters T
Verzi V
Videla M
Villaseñor L
Vorobiov S
Voyvodic L
Wahlberg H
Wainberg O
Waldenmaier T
Walker P
Warner D
Watson AA
Westerhoff S
Wieczorek G
Wiencke L
Wilczynska B
Wilczynski H
Wileman C
Winnick MG
Wu H
Wundheiler B
Xu J
Yamamoto T
Younk P
Zas E
Zavrtanik D
Zavrtanik M
Zech A
Zepeda A
Ziolkowski M
Kégl B
Source :
Science (New York, N.Y.) [Science] 2007 Nov 09; Vol. 318 (5852), pp. 938-43.
Publication Year :
2007

Abstract

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 6 x 10(19) electron volts and the positions of active galactic nuclei (AGN) lying within approximately 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.

Details

Language :
English
ISSN :
1095-9203
Volume :
318
Issue :
5852
Database :
MEDLINE
Journal :
Science (New York, N.Y.)
Publication Type :
Academic Journal
Accession number :
17991855
Full Text :
https://doi.org/10.1126/science.1151124