Artículos de revistas
Correlation of the highest-energy cosmic rays with nearby extragalactic objects
Registro en:
Science. Amer Assoc Advancement Science, v. 318, n. 5852, n. 938, n. 943, 2007.
0036-8075
WOS:000250788500033
10.1126/science.1151124
Autor
Abraham, J
Abreu, P
Aglietta, M
Aguirre, C
Allard, D
Allekotte, I
Allen, J
Allison, P
Alvarez, C
Alvarez-Muniz, J
Ambrosio, M
Anchordoqui, L
Andringa, S
Anzalone, A
Aramo, C
Argiro, S
Arisaka, K
Armengaud, E
Arneodo, F
Arqueros, F
Asch, T
Asorey, H
Assis, P
Atulugama, BS
Aublin, J
Ave, M
Avila, G
Backer, T
Badagnani, D
Barbosa, AF
Barnhill, D
Barroso, SLC
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
Blumer, H
Bohacova, 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
Cazon-Boado, L
Cester, R
Chauvin, J
Chiavassa, A
Chinellato, JA
Chou, A
Chye, J
Clark, PDJ
Clay, RW
Colombo, E
Conceicao, 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, JM
de Mello, JRT
De Mitri, I
de Souza, V
del Peral, L
Deligny, O
Della Selva, A
Delle Fratte, C
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
San Luis, PF
Falcke, H
Farrar, G
Fauth, AC
Fazzini, N
Fernandez, A
Farrar, G
Fauth, AC
Fazzini, N
Fernandez, A
Ferrer, F
Ferry, S
Fick, B
Filevich, A
Filipcic, A
Fleck, I
Fonte, R
Fracchiolla, CE
Fulgione, W
Garcia, B
Gamez, DG
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
Goncalves, P
do Amaral, MG
Gonzalez, D
Gonzalez, JG
Gonzalez, M
Gora, D
Gorgi, A
Gouffon, P
Grassi, V
Grillo, A
Grunfeld, C
Guardincerri, Y
Guarino, F
Guedes, GP
Gutierrez, 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
Horandel, 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
Kromer, D
Kumpel, 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
Lopez, R
Aguera, AL
Bahilo, JL
Maccarone, MC
Macolino, C
Maldera, S
Malek, M
Mancarella, G
Mancenido, ME
Mandat, D
Mantsch, P
Mariazzi, AG
Maris, IC
Martello, D
Martinez, J
Bravo, OM
Mathes, HJ
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
Ragaigne, DM
Montanet, F
Morales, B
Morello, C
Moreno, E
Moreno, JC
Morris, C
Mostafa, M
Muller, MA
Mussa, R
Navarra, G
Navarro, JL
Navas, S
Nellen, L
Newman-Holmes, C
Newton, D
Thi, TN
Nierstenhofer, N
Nitz, D
Nosek, D
Nozka, L
Oehlschlager, J
Ohnuki, T
Olinto, A
Olmos-Gilbaja, VM
Ortiz, M
Ostapchenko, S
Otero, L
Selmi-Dei, DP
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, DP
Ngoc, DP
Thi, TNP
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, FAS
Ridky, J
Riggi, S
Risse, M
Riviere, C
Rizi, V
Roberts, M
Robledo, C
Rodriguez, G
Frias, D
Martino, JR
Rojo, JR
Rodriguez-Cabo, I
Ros, G
Rosado, J
Roth, M
Rouille-d'Orfeuil, B
Roulet, E
Rovero, AC
Salamida, F
Salazar, H
Salina, G
Sanchez, F
Santander, M
Santo, CE
Santos, EM
Sarazin, F
Sarkar, S
Sato, R
Scherini, V
Schieler, H
Schmidt, F
Schmidt, T
Scholten, O
Schovanek, P
Schussler, F
Sciutto, SJ
Scuderi, M
Segreto, A
Semikoz, D
Settimo, M
Shellard, RC
Sidelnik, I
Siffert, BB
Sigl, G
De Grande, NS
Smialkowski, A
Smida, R
Smith, AGK
Smith, BE
Snow, GR
Sokolsky, P
Sommers, P
Sorokin, J
Spinka, H
Squartini, R
Strazzeri, E
Stutz, A
Suarez, F
Suomijarvi, 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
Peixoto, CJ
Tome, B
Tonachini, A
Torresi, D
Travnicek, P
Tripathi, A
Tristram, G
Tscherniakhovski, D
Tueros, M
Tunnicliffe, V
Ulrich, R
Unger, M
Urban, M
Galicia, JFV
Valino, I
Valore, L
van den Berg, AM
van Elewyck, V
Vazquez, RA
Veberic, D
Veiga, A
Velarde, A
Venters, T
Verzi, V
Videla, M
Villasenor, 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
Institución
Resumen
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 similar to 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. 318 5852 938 943