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Update on the correlation of the highest energy cosmic rays with nearby extragalactic matter

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Autor(es):
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Abreu, P. [1, 2] ; Aglietta, M. [3, 4] ; Ahn, E. J. [5] ; Allard, D. [6] ; Allekotte, I. [7, 8] ; Allen, J. [9] ; Alvarez Castillo, J. [10] ; Alvarez-Muniz, J. [11] ; Ambrosio, M. [12, 13] ; Aminaei, A. [14] ; Anchordoqui, L. [15] ; Andringa, S. [1, 2] ; Anticlc, T. [16] ; Anzalone, A. [17] ; Aramo, C. [12, 13] ; Arganda, E. [18] ; Arisaka, K. [19] ; Arqueros, F. [18] ; Asorey, H. [7, 8] ; Assis, P. [1, 2] ; Aublin, J. [20] ; Ave, M. [21, 22] ; Avenier, M. [23] ; Avila, G. [24, 25] ; Baecker, T. [26] ; Badagnani, D. [27, 28] ; Balzer, M. [29] ; Barber, K. B. [30] ; Barbosa, A. F. [31] ; Bardenet, R. [32] ; Barroso, S. L. C. [33] ; Baughman, B. [34] ; Beatty, J. J. [34] ; Becker, B. R. [35] ; Becker, K. H. [36] ; Belletoile, A. [23] ; Bellido, J. A. [30] ; Berat, C. [23] ; Bergmann, T. [29] ; Bertou, X. [7, 8] ; Biermann, P. L. [37] ; Billoir, P. [20] ; Blanco, F. [18] ; Blanco, M. [38] ; Bleve, C. [36, 39, 40] ; Bluemer, H. [22, 41] ; Bohacoca, M. [21, 42] ; Boncioli, D. [43, 44] ; Bonifazi, C. [45, 20] ; Bonino, R. [3, 4] ; Borodai, N. [46] ; Brack, J. [47] ; Brogueira, P. [1, 2] ; Brown, W. C. [48] ; Bruijn, R. [49] ; Buchholz, P. [26] ; Bueno, A. [11] ; Burton, R. E. [50] ; Busca, N. G. [6] ; Caballero-Mora, K. S. [41] ; Caramete, L. [37] ; Caruso, R. [51, 52] ; Castellina, A. [3, 4] ; Catalano, O. [17] ; Cataldi, G. [39, 40] ; Cazon, L. [1, 2] ; Cester, R. [53, 3] ; Chauvin, J. [23] ; Chiavassa, A. [3, 4] ; Chinellato, J. A. [54] ; Chou, A. [5, 9] ; Chudoba, J. [42] ; Clay, R. W. [30] ; Colombo, E. [55] ; Coluccia, M. R. [39, 40] ; Conceicao, R. [1, 2] ; Contreras, F. [25] ; Cook, H. [49] ; Cooper, M. J. [30] ; Coppens, J. [14, 56] ; Cordier, A. [32] ; Cotti, U. [57] ; Coutu, S. [58] ; Covault, C. E. [50] ; Creusot, A. [59] ; Criss, A. [58] ; Cronin, J. [21] ; Curutiu, A. [37] ; Dagoret-Campagne, S. [32] ; Dallier, R. [60] ; Dasso, S. [61, 62, 63] ; Daumiller, K. [22] ; Dawson, B. R. [30] ; de Almeida, R. M. [54, 45] ; De Domenico, M. [51, 52] ; De Donato, C. [10, 23] ; de Jong, S. J. [14] ; De La Vega, G. [64] ; de Mello Junior, W. J. M. [54] ; de Mello Neto, J. R. T. [45] ; De Mitri, I. [39, 40] ; de Souza, V. [65] ; de Vries, K. D. [66] ; Decerprit, G. [6] ; Del Peral, L. [38] ; Deligny, O. [67] ; Della Selva, A. [12, 13] ; Dembinski, H. [22] ; Denkiewicz, A. [55] ; Di Giulio, C. [43, 44] ; Diaz, J. C. [68] ; Castro, M. L. Diaz [69] ; Diep, P. N. [70] ; Dobrigkeit, C. [54] ; D'Olivo, J. C. [10] ; Dong, P. N. [70, 67] ; Dorofeev, A. [47] ; dos Anjos, J. C. [31] ; Dova, M. T. [27, 28] ; D'Urso, D. [12, 13] ; Dutan, I. [37] ; Ebr, J. [42] ; Engel, R. [22] ; Erdmann, M. [71] ; Escobar, C. O. [54] ; Etchegoyen, A. [55] ; San Luis, P. Facal [21] ; Falcke, H. [14, 72] ; Farrar, G. [9] ; Fauth, A. C. [54] ; Fazzini, N. [5] ; Ferguson, A. P. [50] ; Ferrero, A. [55] ; Fick, B. [68] ; Filevich, A. [55] ; Filipcic, A. [59, 73] ; Fleck, I. [26] ; Fliescher, S. [71] ; Fracchiolla, C. E. [47] ; Fraenkel, E. D. [66] ; Froehlich, U. [26] ; Fuchs, B. [31] ; Fulgione, W. [3, 4] ; Gamarra, R. F. [55] ; Gambetta, S. [74, 75] ; Garcia, B. [64] ; Garcia Gamez, D. [76, 77] ; Garcia-Pinto, D. [18] ; Garrido, X. [22] ; Gascon, A. [76, 77] ; Gelmini, G. [19] ; Gemmeke, H. [29] ; Gesterling, K. [35] ; Ghia, P. L. [3, 4, 67] ; Giaccari, U. [39, 40] ; Giller, M. [78] ; Glass, H. [5] ; Gold, M. S. [35] ; Golup, G. [7, 8] ; Gomez Albarracin, F. [27, 28] ; Gomez Berisso, M. [7, 8] ; Goncalves, P. [1, 2] ; Gonzalez, D. [41] ; Gonzalez, J. G. [41] ; Gookin, B. [47] ; Gora, D. [46, 41] ; Gorgi, A. [3, 4] ; Gouffon, P. [65] ; Gozzini, S. R. [49] ; Grashorn, E. [34] ; Grebe, S. [14] ; Grigat, M. [71] ; Grillo, A. F. [79] ; Guardincerri, Y. [61, 62] ; Guarino, F. [12, 13] ; Guedes, G. P. [80] ; Hague, J. D. [35] ; Hansen, P. [27, 28] ; Harari, D. [7, 8] ; Harmsma, S. [56, 66] ; Harton, J. L. [47] ; Haungs, A. [22] ; Hebbeker, T. [71] ; Heck, D. [22] ; Herve, A. E. [30] ; Hojvat, C. [5] ; Holmes, V. C. [30] ; Homola, P. [46] ; Hoeandel, J. R. [14] ; Horneffer, A. [14] ; Hrabovsky, M. [42, 81] ; Huege, T. [22] ; Insolia, A. [51, 52] ; Ionita, F. [21] ; Italiano, A. [51, 52] ; Jiraskova, S. [14] ; Kadija, K. [16] ; Kaducak, M. [5] ; Kampert, K. H. [36] ; Karhan, P. [82] ; Karova, T. [42] ; Kasper, P. [5] ; Kegl, B. [32] ; Keilhauer, B. [22] ; Keivani, A. [83] ; Kelley, J. L. [14] ; Kemp, E. [54] ; Kieckhafer, R. M. [68] ; Klages, H. O. [22] ; Kleifges, M. [29] ; Kleinfeller, J. [22] ; Knapp, J. [49] ; Koang, D-H. [23] ; Kotera, K. [21] ; Krohm, N. [36] ; Kroemer, O. [29] ; Kruppke-Hansen, D. [36] ; Kuehn, F. [5] ; Kuempel, D. [36] ; Kulbartz, J. K. [84] ; Kunka, N. [29] ; La Rosa, G. [17] ; Lachaud, C. [6] ; Lautridou, P. [60] ; Leao, M. S. A. B. [85] ; Lebrun, D. [23] ; Lebrun, P. [5] ; de Oliveira, M. A. Leigui [85] ; Lemiere, A. [67] ; Letessier-Selvon, A. [20] ; Lhenry-Yvon, I. [67] ; Link, K. [41] ; Lopez, R. [86] ; Lopez Agueera, A. [11] ; Louedec, K. [32] ; Lozano Bahilo, J. [76, 77] ; Lucero, A. [3, 4, 55] ; Ludwig, M. [41] ; Lyberis, H. [67] ; Maccarone, M. C. [17] ; Macolino, C. [87, 20, 88] ; Maldera, S. [3, 4] ; Mandat, D. [42] ; Mantsch, P. [5] ; Mariazzi, A. G. [27, 28] ; Marin, V. [60] ; Maris, I. C. [20] ; Marquez Falcon, H. R. [57] ; Marsella, G. [39, 89] ; Martello, D. [39, 40] ; Martin, L. [60] ; Martinez Bravo, O. [86] ; Mathes, H. J. [22] ; Matthews, J. [83, 90] ; Matthews, J. A. J. [35] ; Matthiae, G. [43, 44] ; Maurizio, D. [53, 3] ; Mazur, P. O. [5] ; McEwen, M. [38] ; Medina-Tanco, G. [10] ; Melissas, M. [41] ; Melo, D. [53, 3] ; Menichetti, E. [53, 3] ; Menshikov, A. [29] ; Meurer, C. [71] ; Micanovic, S. [16] ; Micheletti, M. I. [55] ; Miller, W. [35] ; Miramonti, L. [91, 92] ; Mollerach, S. [7, 8] ; Monasor, M. [21] ; Ragaigne, D. Monnier [32] ; Montanet, F. [23] ; Morales, B. [10] ; Morello, C. [3, 4] ; Moreno, E. [86] ; Moreno, J. C. [27, 28] ; Morris, C. [34] ; Mostafa, M. [47] ; Mueller, S. [22] ; Muller, M. A. [54] ; Muenchmeyer, M. [20] ; Mussa, R. [53, 3] ; Navarra, G. [3, 4] ; Navarro, J. L. [76, 77] ; Navas, S. [76, 77] ; Necesal, P. [42] ; Nellen, L. [10] ; Nhung, P. T. [70] ; Nierstenhoefer, N. [36] ; Nitz, D. [68] ; Nosek, D. [82] ; Nozka, L. [42] ; Nyklicek, M. [42] ; Oehlschlager, J. [22] ; Olinto, A. [21] ; Oliva, P. [36] ; Olmos-Gilbaja, V. M. [11] ; Ortiz, M. [18] ; Pacheco, N. [38] ; Selmi-Dei, D. Pakk [54] ; Palatka, M. [42] ; Pallotta, J. ; Palmieri, N. [41] ; Parente, G. [11] ; Parizot, E. [6] ; Parra, A. [11] ; Parrisius, J. [41] ; Parsons, R. D. [49] ; Pastor, S. [93] ; Paul, T. [94] ; Pavlidou, V. [21] ; Payet, K. [23] ; Pech, M. [42] ; Pekala, J. [46] ; Pelayo, R. [11] ; Pepe, I. M. [95] ; Perrone, L. [39, 89] ; Pesce, R. [74, 75] ; Petermann, E. [96] ; Petrera, S. [87, 88] ; Petrinca, P. [43, 44] ; Petrolini, A. [74, 75] ; Petrov, Y. [47] ; Petrovic, J. [56] ; Pfendner, C. [97] ; Phan, N. [35] ; Piegaia, R. [61, 62] ; Pierog, T. [22] ; Pimenta, M. [1, 2] ; Pirronell, V. [51, 52] ; Platino, M. [55] ; Ponce, V. H. [7, 8] ; Pontz, M. [26] ; Privitera, P. [21] ; Prouza, M. [42] ; Quel, E. J. [62] ; Rautenberg, J. [36] ; Ravel, O. [60] ; Ravignani, D. [55] ; Revenu, B. [60] ; Ridky, J. [42] ; Riggi, S. [51, 52] ; Risse, M. [26] ; Ristori, P. [62] ; Rivera, H. [91, 92] ; Riviere, C. [23] ; Rizi, V. [87, 88] ; Robledo, C. [86] ; Rodriguez, G. [11] ; Rodriguez Martino, J. [51, 52, 25] ; Rodriguez Rojo, J. [25] ; Rodriguez-Cabo, I. [11] ; Rodriguez-Frias, M. D. [38] ; Ros, G. [38] ; Rosado, J. [18] ; Rossler, T. [81] ; Roth, M. [22] ; Rouille-d'Orfeuil, B. [21] ; Roulet, E. [7, 8] ; Rovero, A. C. [63] ; Salamida, F. [22, 87, 88] ; Salazar, H. [86] ; Salina, G. [43, 44] ; Sanchez, F. [55] ; Santander, M. [25] ; Santo, C. E. [1, 2] ; Santos, E. [1, 2] ; Santos, E. M. [45] ; Sarazin, F. [98] ; Sarkar, S. [99] ; Sato, R. [25] ; Scharf, N. [71] ; Scherini, V. [91, 92] ; Schieler, H. [22] ; Schiffer, P. [71] ; Schmidt, A. [29] ; Schmidt, F. [21] ; Schmidt, T. [41] ; Scholten, O. [66] ; Schoorlemmer, H. [14] ; Schovancova, J. [42] ; Schovanek, P. [42] ; Schroeder, F. [22] ; Schulte, S. [71] ; Schuessler, F. [22] ; Schuster, D. [98] ; Sciutto, S. J. [27, 28] ; Scuderi, M. [51, 52] ; Segreto, A. [17] ; Settimo, M. [39, 40] ; Shadkam, A. [83] ; Shellard, R. C. [31] ; Sidelnik, I. [55] ; Sigl, G. [84] ; Smialkowski, A. [78] ; Smida, R. [42, 22] ; Snow, G. R. [96] ; Sommers, P. [58] ; Sorokin, J. [30] ; Spinka, H. [100, 5] ; Squartini, R. [25] ; Stapleton, J. [34] ; Stasielak, J. [46] ; Stephan, M. [71] ; Strazzeri, E. [17] ; Stutz, A. [23] ; Suarez, F. [55] ; Suomijaervi, T. [67] ; Supanitsky, A. D. [10] ; Susa, T. [16] ; Sutherland, M. S. [34] ; Swain, J. [94] ; Szadkowski, Z. [36, 78] ; Tamashiro, A. [63] ; Tapia, A. [55] ; Tarutina, T. [27, 28] ; Tascau, O. [36] ; Tcaciuc, R. [26] ; Tcherniakhovski, D. [29] ; Tegolo, D. [51, 52] ; Thao, N. T. [70] ; Thomas, D. [47] ; Tiffenberg, J. [61, 62] ; Timmermans, C. [14, 56] ; Tiwari, D. K. [57] ; Tkaczyk, W. [78] ; Peixoto, C. J. Todero [85] ; Tome, B. [1, 2] ; Tonachini, A. [53, 3] ; Travnicek, P. [42] ; Tridapalli, D. B. [65] ; Tristram, G. [6] ; Trovato, E. [51, 52] ; Tueros, M. [27, 28] ; Ulrich, R. [58, 22] ; Unger, M. [22] ; Urban, M. [32] ; Valdes Galicia, J. F. [10] ; Valino, I. [22] ; Valore, L. [12, 13] ; van den Berg, A. M. [66] ; Vargas Cardenas, B. [10] ; Vazquez, J. R. [18] ; Vazquez, R. A. [11] ; Veberic, D. [59] ; Venters, T. [21] ; Verzi, V. [43, 44] ; Videla, M. [64] ; Villasenor, L. [57] ; Wahlberg, H. [27, 28] ; Wahrlich, P. [30] ; Wainberg, O. [55] ; Warner, D. [47] ; Watson, A. A. [49] ; Weidenhaupt, K. [71] ; Weindl, A. [22] ; Whelan, B. J. [30] ; Wieczorek, G. [78] ; Wiencke, L. [98] ; Wilczynska, B. [46] ; Wilczynski, H. [46] ; Will, M. [22] ; Williams, C. [21] ; Winchen, T. [71] ; Winders, L. [15] ; Winnick, M. G. [30] ; Wommer, M. [22] ; Wundheiler, B. [55] ; Yamamoto, T. [21] ; Younk, P. [47] ; Yuan, G. [83] ; Yushkov, A. [12, 13] ; Zamorano, B. [76, 77] ; Zas, E. [11] ; Zavrtanik, D. [59, 73] ; Zavrtanik, M. [59, 73] ; Zaw, I. [9] ; Zepeda, A. [101] ; Ziolkowski, M. [26] ; Collaboration, Pierre Auger
Número total de Autores: 481
Afiliação do(s) autor(es):
Mostrar menos -
[1] LIP, P-1000 Lisbon - Portugal
[2] Inst Super Tecn, Lisbon - Portugal
[3] Sezione Ist Nazl Fis Nucl, Turin - Italy
[4] Univ Turin, Ist Fis Spazio Interplanetario INAF, Turin - Italy
[5] Fermilab Natl Accelerator Lab, Batavia, IL - USA
[6] Univ Paris 11, APC, CNRS IN2P3, Orsay - France
[7] Ctr Atom Bariloche, San Carlos De Bariloche, Rio Negro - Argentina
[8] Inst Balseiro CNEA UNCuyo CONICET, San Carlos De Bariloche, Rio Negro - Argentina
[9] NYU, New York, NY - USA
[10] Univ Nacl Autonoma Mexico, Mexico City 04510, DF - Mexico
[11] Univ Santiago de Compostela, Santiago De Compostela - Spain
[12] Sezione Ist Nazl Fis Nucl, Naples - Italy
[13] Univ Naples Federico 2, Naples - Italy
[14] Radboud Univ Nijmegen, IMAPP, NL-6525 ED Nijmegen - Netherlands
[15] Univ Wisconsin, Milwaukee, WI 53201 - USA
[16] Rudjer Boskovic Inst, Zagreb 10000 - Croatia
[17] Ist Astrofis Spaziale & Fis Cosm Palermo INAF, Palermo - Italy
[18] Univ Complutense Madrid, Madrid - Spain
[19] Univ Calif Los Angeles, Los Angeles, CA - USA
[20] Univ Paris 06, LPNHE, CNRS IN2P3, Paris - France
[21] Univ Chicago, Enrico Fermi Inst, Chicago, IL 60637 - USA
[22] Karlsruhe Inst Technol, Inst Kernphys, Karlsruhe - Germany
[23] Univ Grenoble 1, LPSC, CNRS IN2P3, Grenoble - France
[24] Comis Nacl Energia Atom, Malargue - Argentina
[25] Pierre Auger So Observ, Malargue - Argentina
[26] Univ Siegen, Siegen - Germany
[27] Consejo Nacl Invest Cient & Tecn, La Plata, Buenos Aires - Argentina
[28] Univ Nacl La Plata, IFLP, La Plata, Buenos Aires - Argentina
[29] Karlsruhe Inst Technol, Inst Prozessdatenverarbeitung & Elekt, Karlsruhe - Germany
[30] Univ Adelaide, Adelaide, SA - Australia
[31] Ctr Brasileiro Pesquisas Fis, Rio De Janeiro - Brazil
[32] Univ Paris 11, LAL, CNRS IN2P3, Orsay - France
[33] Univ Estadual Sudoeste Bahia, Vitoria Da Conquista, BA - Brazil
[34] Ohio State Univ, Columbus, OH 43210 - USA
[35] Univ New Mexico, Albuquerque, NM 87131 - USA
[36] Berg Univ Wuppertal, Wuppertal - Germany
[37] Max Planck Inst Radioastron, D-5300 Bonn - Germany
[38] Univ Alcala De Henares, Alcala De Henares, Madrid - Spain
[39] Sezione Ist Nazl Fis Nucl, Lecce - Italy
[40] Univ Salento, Dipartimento Fis, Lecce - Italy
[41] Karlsruhe Inst Technol, Inst Expt Kernphys, Karlsruhe - Germany
[42] Acad Sci Czech Republic, Inst Phys, Prague - Czech Republic
[43] Sezione Ist Nazl Fis Nucl, Rome - Italy
[44] Univ Roma II Tor Vergata, Rome - Italy
[45] Univ Fed Rio de Janeiro, Inst Fis, Rio De Janeiro - Brazil
[46] Inst Nucl Phys PAN, Krakow - Poland
[47] Colorado State Univ, Ft Collins, CO 80523 - USA
[48] Colorado State Univ, Pueblo, CO - USA
[49] Univ Leeds, Sch Phys & Astron, Leeds LS2 9JT, W Yorkshire - England
[50] Case Western Reserve Univ, Cleveland, OH 44106 - USA
[51] Univ Catania, Catania - Italy
[52] Sezione Ist Nazl Fis Nucl, Catania - Italy
[53] Univ Turin, Turin - Italy
[54] Univ Estadual Campinas, IFGW, Campinas, SP - Brazil
[55] Ctr Atom Constituyentes Comis Nacl Energia Atom C, Buenos Aires, DF - Argentina
[56] Nikhef, Amsterdam - Netherlands
[57] Univ Michoacana, Morelia, Michoacan - Mexico
[58] Penn State Univ, University Pk, PA 16802 - USA
[59] Univ Nova Gorica, Lab Astroparticle Phys, Nova Gorica - Slovenia
[60] CNRS IN2P3, SUBATECH, Nantes - France
[61] Univ Buenos Aires, FCEyN, Dept Fis, RA-1053 Buenos Aires, DF - Argentina
[62] Consejo Nacl Invest Cient & Tecn, RA-1033 Buenos Aires, DF - Argentina
[63] Inst Astron & Fis Espacio CONICET UBA, Buenos Aires, DF - Argentina
[64] Natl Technol Univ, Fac Mendoza CONICET CNEA, Mendoza - Argentina
[65] Univ Sao Paulo, Inst Fis, Sao Carlos, SP - Brazil
[66] Univ Groningen, Kernfys Versneller Inst, Groningen - Netherlands
[67] Univ Paris 11, Inst Phys Nucl Orsay, CNRS IN2P3, Orsay - France
[68] Michigan Technol Univ, Houghton, MI 49931 - USA
[69] Pontificia Univ Catolica Rio de Janeiro, Rio De Janeiro - Brazil
[70] Inst Nucl Sci & Technol, Hanoi - Vietnam
[71] Rhein Westfal TH Aachen, Phys Inst A 3, Aachen - Germany
[72] ASTRON, Dwingeloo - Netherlands
[73] J Stefan Inst, Ljubljana - Slovenia
[74] Univ Genoa, Dipartimento Fis, Genoa - Italy
[75] Ist Nazl Fis Nucl, I-16146 Genoa - Italy
[76] Univ Granada, Granada - Spain
[77] CAFPE, Granada - Spain
[78] Univ Lodz, PL-90131 Lodz - Poland
[79] INFN, Lab Nazl Gran Sasso, Laquila - Italy
[80] Univ Estadual Feira de Santana, Feira De Santana - Brazil
[81] Palacky Univ, CR-77147 Olomouc - Czech Republic
[82] Charles Univ Prague, Fac Math & Phys, Inst Particle & Nucl Phys, Prague - Czech Republic
[83] Louisiana State Univ, Baton Rouge, LA 70803 - USA
[84] Univ Hamburg, Hamburg - Germany
[85] Univ Fed ABC, Santo Andre, SP - Brazil
[86] Benemerita Univ Autonoma Puebla, Puebla - Mexico
[87] Univ Aquila, I-67100 Laquila - Italy
[88] INFN, Laquila - Italy
[89] Univ Salento, Dipartimento Ingn Innovaz, Lecce - Italy
[90] Southern Univ, Baton Rouge, LA - USA
[91] Univ Milan, Milan - Italy
[92] Sezione Ist Nazl Fis Nucl, Milan - Italy
[93] Univ Valencia, CSIC, Inst Fis Corpuscular, Valencia - Spain
[94] Northeastern Univ, Boston, MA 02115 - USA
[95] Univ Fed Bahia, Salvador, BA - Brazil
[96] Univ Nebraska, Lincoln, NE - USA
[97] Univ Wisconsin, Madison, WI - USA
[98] Colorado Sch Mines, Golden, CO 80401 - USA
[99] Univ Oxford, Rudolf Peierls Ctr Theoret Phys, Oxford - England
[100] Argonne Natl Lab, Argonne, IL 60439 - USA
[101] Ctr Invest & Estudios Avanzados IPN CINVESTAV, Mexico City, DF - Mexico
Número total de Afiliações: 101
Tipo de documento: Artigo Científico
Fonte: Astroparticle Physics; v. 34, n. 5, p. 314-326, DEC 2010.
Citações Web of Science: 226
Resumo

Data collected by the Pierre Auger Observatory through 31 August 2007 showed evidence for anisotropy in the arrival directions of cosmic rays above the Greisen-Zatsepin-Kuz'min energy threshold, 6 x 10(19) eV. The anisotropy was measured by the fraction of arrival directions that are less than 3.1 degrees from the position of an active galactic nucleus within 75 Mpc (using the Veron-Cetty and Veron 12th catalog). An updated measurement of this fraction is reported here using the arrival directions of cosmic rays recorded above the same energy threshold through 31 December 2009. The number of arrival directions has increased from 27 to 69, allowing a more precise measurement. The correlating fraction is (38(-6)(+7))%, compared with 21% expected for isotropic cosmic rays. This is down from the early estimate of (69-(+11)(13))%. The enlarged set of arrival directions is examined also in relation to other populations of nearby extragalactic objects: galaxies in the 2 Microns All Sky Survey and active galactic nuclei detected in hard X-rays by the Swift Burst Alert Telescope. A celestial region around the position of the radiogalaxy Cen A has the largest excess of arrival directions relative to isotropic expectations. The 2-point autocorrelation function is shown for the enlarged set of arrival directions and compared to the isotropic expectation. (C) 2010 Elsevier B.V. All rights reserved. (AU)