Autor(es):Mostrar menos -

Aab, A. ^[1] ; Abreu, P. ^{[2, 3]} ; Aglietta, M. ^{[4, 5]} ; Albuquerque, I. F. M. ^[6] ; Albury, J. M. ^[7] ; Allekotte, I. ^{[8, 9]} ; Almela, A. ^{[10, 11]} ; Alvarez Castillo, J. ^[12] ; Alvarez-Muniz, J. ^[13] ; Anastasi, G. A. ^{[14, 15]} ; Anchordoqui, L. ^[16] ; Andrada, B. ^[10] ; Andringa, S. ^{[2, 3]} ; Aramo, C. ^[17] ; Asorey, H. ^{[18, 8, 9]} ; Assis, P. ^{[2, 3]} ; Avila, G. ^{[19, 20]} ; Badescu, A. M. ^[21] ; Balaceanu, A. ^[22] ; Barbato, F. ^{[17, 23]} ; Barreira Luz, R. J. ^{[2, 3]} ; Baur, S. ^[24] ; Becker, K. H. ^[25] ; Bellido, J. A. ^[7] ; Berat, C. ^[26] ; Bertaina, M. E. ^{[4, 27]} ; Bertou, X. ^{[8, 9]} ; Biermann, P. L. ^[28] ; Biteau, J. ^[29] ; Blaess, S. G. ^[7] ; Blanco, A. ^{[2, 3]} ; Blazek, J. ^[30] ; Bleve, C. ^{[31, 32]} ; Bohacova, M. ^[30] ; Bonifazi, C. ^[33] ; Borodai, N. ^[34] ; Botti, A. M. ^{[10, 24]} ; Brack, J. ^[35] ; Bretz, T. ^[36] ; Bridgeman, A. ^[37] ; Briechle, F. L. ^[36] ; Buchholz, P. ^[38] ; Bueno, A. ^{[39, 40]} ; Buitink, S. ^[41] ; Buscemi, M. ^{[42, 43]} ; Caballero-Mora, K. S. ^[44] ; Caccianiga, L. ^[45] ; Calcagni, L. ^{[46, 47]} ; Cancio, A. ^{[10, 11]} ; Canfora, F. ^{[1, 48]} ; Carceller, J. M. ^{[39, 40]} ; Caruso, R. ^{[42, 43]} ; Castellina, A. ^{[4, 5]} ; Catalani, F. ^[49] ; Cataldi, G. ^[32] ; Cazon, L. ^{[2, 3]} ; Chinellato, J. A. ^[50] ; Chudoba, J. ^[30] ; Chytka, L. ^[51] ; Clay, R. W. ^[7] ; Cobos Cerutti, A. C. ^{[52, 53]} ; Colalillo, R. ^{[17, 23]} ; Coleman, A. ^[54] ; Coluccia, M. R. ^{[31, 32]} ; Conceicao, R. ^{[2, 3]} ; Consolati, G. ^{[55, 56]} ; Contreras, F. ^{[19, 20]} ; Cooper, M. J. ^[7] ; Coutu, S. ^[54] ; Covault, C. E. ^[57] ; Daniel, B. ^[50] ; Dasso, S. ^{[58, 59, 60, 61]} ; Daumiller, K. ^[24] ; Dawson, B. R. ^[7] ; Day, J. A. ^[7] ; de Almeida, R. M. ^[62] ; de Jong, S. J. ^{[1, 48]} ; De Mauro, G. ^{[1, 48]} ; de Mello Neto, J. R. T. ^{[33, 63]} ; De Mitri, I. ^{[14, 15]} ; de Oliveira, J. ^[62] ; de Souza, V. ^[64] ; Debatin, J. ^[37] ; Deligny, O. ^[29] ; Dhital, N. ^[34] ; Diaz Castro, M. L. ^[50] ; Diogo, F. ^{[2, 3]} ; Dobrigkeit, C. ^[50] ; D'Olivo, J. C. ^[12] ; Dorosti, Q. ^[38] ; dos Anjos, R. C. ^[65] ; Dova, M. T. ^{[46, 47]} ; Dundovic, A. ^[66] ; Ebr, J. ^[30] ; Engel, R. ^[24] ; Erdmann, M. ^[36] ; Escobar, C. O. ^[67] ; Etchegoyen, A. ^{[10, 11]} ; Falcke, H. ^{[1, 48, 68]} ; Farmer, J. ^[69] ; Farrar, G. ^[70] ; Fauth, A. C. ^[50] ; Fazzini, N. ^[67] ; Feldbusch, F. ^[71] ; Fenu, F. ^{[4, 27]} ; Ferreyro, L. P. ^[10] ; Figueira, J. M. ^[10] ; Filipcic, A. ^{[72, 73]} ; Freire, M. M. ^{[74, 75]} ; Fujii, T. ^{[69, 76]} ; Fuster, A. ^{[10, 11]} ; Garcia, B. ^{[52, 53]} ; Gemmeke, H. ^[71] ; Gherghel-Lascu, A. ^[22] ; Ghia, P. L. ^[29] ; Giaccari, U. ^{[77, 33]} ; Giammarchi, M. ^[55] ; Giller, M. ^[78] ; Glas, D. ^[79] ; Glombitza, J. ^[36] ; Golup, G. ^{[8, 9]} ; Gomez Berisso, M. ^{[8, 9]} ; Gomez Vitale, P. F. ^{[19, 20]} ; Gonzalez, N. ^[10] ; Goos, I. ^{[24, 8, 9]} ; Gora, D. ^[34] ; Gorgi, A. ^{[4, 5]} ; Gottowik, M. ^[25] ; Grubb, T. D. ^[7] ; Guarino, F. ^{[17, 23]} ; Guedes, G. P. ^[80] ; Guido, E. ^{[4, 27]} ; Halliday, R. ^[57] ; Hampel, M. R. ^[10] ; Hansen, P. ^{[46, 47]} ; Harari, D. ^{[8, 9]} ; Harrison, T. A. ^[7] ; Harvey, V. M. ^[7] ; Haungs, A. ^[24] ; Hebbeker, T. ^[36] ; Heck, D. ^[24] ; Heimann, P. ^[38] ; Hill, G. C. ^[7] ; Hojvat, C. ^[67] ; Holt, E. M. ^{[10, 37]} ; Homola, P. ^[34] ; Horandel, J. R. ^{[1, 48]} ; Horvath, P. ^[51] ; Hrabovsky, M. ^[51] ; Huege, T. ^{[24, 41]} ; Hulsman, J. ^{[10, 24]} ; Insolia, A. ^{[42, 43]} ; Isar, P. G. ^[81] ; Jandt, I. ^[25] ; Johnsen, J. A. ^[82] ; Josebachuili, M. ^[10] ; Jurysek, J. ^[30] ; Kaeaepae, A. ^[25] ; Kampert, K. H. ^[25] ; Keilhauer, B. ^[24] ; Kemmerich, N. ^[6] ; Kemp, J. ^[36] ; Klages, H. O. ^[24] ; Kleifges, M. ^[71] ; Kleinfeller, J. ^[19] ; Krause, R. ^[36] ; Kuempel, D. ^[25] ; Mezek, G. Kukec ^[73] ; Awad, A. Kuotb ^[37] ; Lago, B. L. ^[83] ; LaHurd, D. ^[57] ; Lang, R. G. ^[64] ; Legumina, R. ^[78] ; Leigui de Oliveira, M. A. ^[84] ; Lenok, V. ^[24] ; Letessier-Selvon, A. ^{[85, 86]} ; Lhenry-Yvon, I. ^[29] ; Lo Presti, D. ^{[42, 43]} ; Lopes, L. ^{[2, 3]} ; Lopez, R. ^[87] ; Lopez Casado, A. ^[13] ; Lorek, R. ^[57] ; Luce, Q. ^[29] ; Lucero, A. ^[10] ; Malacari, M. ^[69] ; Mallamaci, M. ^{[45, 55]} ; Mancarella, G. ^{[31, 32]} ; Mandat, D. ^[30] ; Mantsch, P. ^[67] ; Mariazzi, A. G. ^{[46, 47]} ; Maris, I. C. ^[88] ; Marsella, G. ^{[31, 32]} ; Martello, D. ^{[31, 32]} ; Martinez, H. ^[89] ; Martinez Bravo, O. ^[87] ; Mathes, H. J. ^[24] ; Mathys, S. ^[25] ; Matthews, J. ^[90] ; Matthiae, G. ^{[91, 92]} ; Mayotte, E. ^[25] ; Mazur, P. O. ^[67] ; Medina-Tanco, G. ^[12] ; Melo, D. ^[10] ; Menshikov, A. ^[71] ; Merenda, K. -D. ^[82] ; Michal, S. ^[51] ; Micheletti, M. I. ^{[74, 75]} ; Middendorf, L. ^[36] ; Miramonti, L. ^{[45, 55]} ; Mitrica, B. ^[22] ; Mockler, D. ^[37] ; Mollerach, S. ^{[8, 9]} ; Montanet, F. ^[26] ; Morello, C. ^{[4, 5]} ; Morlino, G. ^{[14, 15]} ; Mostafa, M. ^[54] ; Mueller, A. L. ^{[10, 24]} ; Muller, M. A. ^{[50, 93]} ; Mueller, S. ^{[10, 37]} ; Mussa, R. ^[4] ; Nellen, L. ^[12] ; Nguyen, P. H. ^[7] ; Niculescu-Oglinzanu, M. ^[22] ; Niechciol, M. ^[38] ; Nitz, D. ^{[94, 95]} ; Nosek, D. ^[96] ; Novotny, V. ^[96] ; Nozka, L. ^[51] ; Nucita, A. ^{[31, 32]} ; Nunez, L. A. ^[18] ; Olinto, A. ^[69] ; Palatka, M. ^[30] ; Pallotta, J. ^{[97, 98]} ; Papenbreer, P. ^[25] ; Parente, G. ^[13] ; Parra, A. ^[87] ; Pech, M. ^[30] ; Pedreira, F. ^[13] ; Pekala, J. ^[34] ; Pelayo, R. ^[99] ; Pena-Rodriguez, J. ^[18] ; Pereira, L. A. S. ^[50] ; Perlin, M. ^[10] ; Perrone, L. ^{[31, 32]} ; Peters, C. ^[36] ; Petrera, S. ^{[14, 15]} ; Phuntsok, J. ^[54] ; Pierog, T. ^[24] ; Pimenta, M. ^{[2, 3]} ; Pirronello, V. ^{[42, 43]} ; Platino, M. ^[10] ; Poh, J. ^[69] ; Pont, B. ^[1] ; Porowski, C. ^[34] ; Prado, R. R. ^[64] ; Privitera, P. ^[69] ; Prouza, M. ^[30] ; Puyleart, A. ^[94] ; Querchfeld, S. ^[25] ; Quinn, S. ^[57] ; Ramos-Pollan, R. ^[18] ; Rautenberg, J. ^[25] ; Ravignani, D. ^[10] ; Reininghaus, M. ^[24] ; Ridky, J. ^[30] ; Riehn, F. ^{[2, 3]} ; Risse, M. ^[38] ; Ristori, P. ^{[97, 98]} ; Rizi, V. ^{[14, 100]} ; Rodrigues de Carvalho, W. ^[6] ; Rodriguez Rojo, J. ^[19] ; Roncoroni, M. J. ^[10] ; Roth, M. ^[24] ; Roulet, E. ^{[8, 9]} ; Rovero, A. C. ^[58] ; Ruehl, P. ^[38] ; Saffi, S. J. ^[7] ; Saftoiu, A. ^[22] ; Salamida, F. ^{[14, 100]} ; Salazar, H. ^[87] ; Saleh, A. ^[73] ; Salina, G. ^[91] ; Sanchez, F. ^[10] ; Santos, E. M. ^[6] ; Santos, E. ^[30] ; Sarazin, F. ^[82] ; Sarmento, R. ^{[2, 3]} ; Sarmiento-Cano, C. ^[10] ; Sato, R. ^[19] ; Savina, P. ^{[31, 32]} ; Schauer, M. ^[25] ; Scherini, V. ^[32] ; Schieler, H. ^[24] ; Schimassek, M. ^[37] ; Schimp, M. ^[25] ; Schmidt, D. ^[37] ; Scholten, O. ^{[101, 41]} ; Schovanek, P. ^[30] ; Schroeder, F. G. ^[37] ; Schroeder, S. ^[25] ; Schumacher, J. ^[36] ; Sciutto, S. J. ^{[46, 47]} ; Shellard, R. C. ^[77] ; Sigl, G. ^[66] ; Silli, G. ^{[10, 24]} ; Sima, O. ^{[22, 102]} ; Smida, R. ^[36] ; Snow, G. R. ^[103] ; Sommers, P. ^[54] ; Soriano, J. F. ^[16] ; Souchard, J. ^[26] ; Squartini, R. ^[19] ; Stanca, D. ^[22] ; Stanic, S. ^[73] ; Stasielak, J. ^[34] ; Stassi, P. ^[26] ; Stolpovskiy, M. ^[26] ; Streich, A. ^[37] ; Suarez, F. ^{[10, 11]} ; Suarez-Duran, M. ^[18] ; Sudholz, T. ^[7] ; Suomijarvi, T. ^[29] ; Supanitsky, A. D. ^[10] ; Supik, J. ^[51] ; Szadkowski, Z. ^[79] ; Taboada, A. ^[24] ; Taborda, O. A. ^{[8, 9]} ; Tapia, A. ^[104] ; Timmermans, C. ^{[1, 48]} ; Todero Peixoto, C. J. ^[49] ; Tome, B. ^{[2, 3]} ; Torralba Elipe, G. ^[13] ; Travnicek, P. ^[30] ; Trini, M. ^[73] ; Tueros, M. ^{[46, 47]} ; Ulrich, R. ^[24] ; Unger, M. ^[24] ; Urban, M. ^[36] ; Valdes Galicia, J. F. ^[12] ; Valino, I. ^[13] ; Valore, L. ^{[17, 23]} ; van Bodegom, P. ^[7] ; van den Berg, A. M. ^[101] ; van Vliet, A. ^[1] ; Varela, E. ^[87] ; Vargas Cardenas, B. ^[12] ; Vazquez, R. A. ^[13] ; Veberic, D. ^[24] ; Ventura, C. ^[63] ; Vergara Quispe, I. D. ^{[46, 47]} ; Verzi, V. ^[91] ; Vicha, J. ^[30] ; Villasenor, L. ^[87] ; Vorobiov, S. ^[73] ; Wahlberg, H. ^{[46, 47]} ; Wainberg, O. ^{[10, 11]} ; Watson, A. A. ^[105] ; Weber, M. ^[71] ; Weindl, A. ^[24] ; Wiedenski, M. ^[79] ; Wiencke, L. ^[82] ; Wilczynski, H. ^[34] ; Wirtz, M. ^[36] ; Wittkowski, D. ^[25] ; Wundheiler, B. ^[10] ; Yang, L. ^[73] ; Yushkov, A. ^[30] ; Zas, E. ^[13] ; Zavrtanik, D. ^{[72, 73]} ; Zavrtanik, M. ^{[72, 73]} ; Zehrer, L. ^[73] ; Zepeda, A. ^[89] ; Zimmermann, B. ^[71] ; Ziolkowski, M. ^[38] ; Zong, Z. ^[29] ; Zuccarello, F. ^{[42, 43]} ; Collaboration, Pierre Auger

Afiliação do(s) autor(es):Mostrar menos -

^[1] Radboud Univ Nijmegen, IMAPP, Nijmegen - Netherlands

^[2] Univ Lisbon, Lab Instrumentacao & Fis Expt Particulas LIP, Lisbon - Portugal

^[3] Univ Lisbon, IST, Lisbon - Portugal

^[4] Ist Nazl Fis Nucl, Sez Torino, Turin - Italy

^[5] Osservatorio Astrofis Torino INAF, Turin - Italy

^[6] Univ Sao Paulo, Inst Fis, Sao Paulo, SP - Brazil

^[7] Univ Adelaide, Adelaide, SA - Australia

^[8] CNEA, UNCuyo, CONICET, Ctr Atom Bariloche, San Carlos De Bariloche, Rio Negro - Argentina

^[9] CNEA, UNCuyo, CONICET, Inst Balseiro, San Carlos De Bariloche, Rio Negro - Argentina

^[10] UNSAM, CONICET, CNEA, Inst Tecnol Detecc & Astroparticulas, Buenos Aires, DF - Argentina

^[11] Univ Tecnol Nacl, Fac Reg Buenos Aires, Buenos Aires, DF - Argentina

^[12] Univ Nacl Autonoma Mexico, Mexico City, DF - Mexico

^[13] Univ Santiago de Compostela, IGFAE, Santiago De Compostela - Spain

^[14] Ist Nazl Fis Nucl, Lab Nazl Gran Sasso, Assergi, Laquila - Italy

^[15] Gran Sasso Sci Inst, Laquila - Italy

^[16] CUNY, Dept Phys & Astron, Lehman Coll, Bronx, NY 10468 - USA

^[17] Ist Nazl Fis Nucl, Sez Napoli, Naples - Italy

^[18] Univ Ind Santander, Bucaramanga - Colombia

^[19] Observ Pierre Auger, Malargue - Argentina

^[20] Comis Nacl Energia Atom, Malargue - Argentina

^[21] Univ Politehn Bucuresti, Bucharest - Romania

^[22] Horia Hulubei Natl Inst Phys & Nucl Engn, Bucharest - Romania

^[23] Univ Napoli Federico II, Dipartimento Fis Ettore Pancini, Naples - Italy

^[24] Karlsruhe Inst Technol, Inst Kernphys, Karlsruhe - Germany

^[25] Berg Univ Wuppertal, Dept Phys, Wuppertal - Germany

^[26] Univ Grenoble Alpes, CNRS, Grenoble Inst Engn, LPSC IN2P3, F-38000 Grenoble - France

^[27] Univ Torino, Dipartimento Fis, Turin - Italy

^[28] Max Planck Inst Radioastron, Bonn - Germany

^[29] Univ Paris Sud, Univ Paris Saclay, IPNO, CNRS IN2P3, Orsay - France

^[30] Czech Acad Sci, Inst Phys, Prague - Czech Republic

^[31] Univ Salento, Dipartimento Matemat & Fis E De Giorgi, Lecce - Italy

^[32] Ist Nazl Fis Nucl, Sez Lecce, Lecce - Italy

^[33] Univ Fed Rio de Janeiro, Inst Fis, Rio De Janeiro, RJ - Brazil

^[34] Inst Nucl Phys PAN, Krakow - Poland

^[35] Colorado State Univ, Ft Collins, CO 80523 - USA

^[36] Rhein Westfal TH Aachen, Phys Inst A 3, Aachen - Germany

^[37] Karlsruhe Inst Technol, Inst Expt Particle Phys ETP, Karlsruhe - Germany

^[38] Univ Siegen, Fachbereich Phys Expt Teilchenphys 7, Siegen - Germany

^[39] Univ Granada, Granada - Spain

^[40] CAFPE, Granada - Spain

^[41] Vrije Univ Brussels, Brussels - Belgium

^[42] Ist Nazl Fis Nucl, Sez Catania, Catania - Italy

^[43] Univ Catania, Dipartimento Fis & Astron, Catania - Italy

^[44] Univ Autonoma Chiapas, Tuxtla Gutierrez, Chiapas - Mexico

^[45] Univ Milan, Dipartimento Fis, Milan - Italy

^[46] Consejo Nacl Invest Cient & Tecn, La Plata - Argentina

^[47] Univ Nacl La Plata, IFLP, La Plata - Argentina

^[48] Nikhef, Sci Pk, Amsterdam - Netherlands

^[49] Univ Sao Paulo, Escola Engn Lorena, Lorena, SP - Brazil

^[50] Univ Estadual Campinas, IFGW, Campinas, SP - Brazil

^[51] Palacky Univ, RCPTM, Olomouc - Czech Republic

^[52] UNSAM, CONICET, CNEA, Inst Tecnol Detecc & Astroparticulas, Mendoza - Argentina

^[53] Univ Tecnol Nacl, CONICET, CNEA, Fac Reg Mendoza, Mendoza - Argentina

^[54] Penn State Univ, University Pk, PA 16801 - USA

^[55] Ist Nazl Fis Nucl, Sez Milano, Milan - Italy

^[56] Politecn Milan, Dipartimento Sci & Tecnol Aerospaziali, Milan - Italy

^[57] Case Western Reserve Univ, Cleveland, OH 44106 - USA

^[58] CONICET UBA, IAFE, Buenos Aires, DF - Argentina

^[59] Consejo Nacl Invest Cient & Tecn, Buenos Aires, DF - Argentina

^[60] Univ Buenos Aires, FCEyN, Dept Fis, Buenos Aires, DF - Argentina

^[61] Univ Buenos Aires, Dept Ciencias Atmosfera & Oceanos, Buenos Aires, DF - Argentina

^[62] Univ Fed Fluminense, EEIMVR, Volta Redonda, RJ - Brazil

^[63] Univ Fed Rio de Janeiro, Observ Valongo, Rio de Janeiro, RJ - Brazil

^[64] Univ Sao Paulo, Inst Fis Sao Carlos, Sao Carlos, SP - Brazil

^[65] Univ Fed Parana, Setor Palotina, Palotina - Brazil

^[66] Univ Hamburg, Inst Theoret Phys 2, Hamburg - Germany

^[67] Fermilab Natl Accelerator Lab, Batavia, IL 60510 - USA

^[68] Stichting Astron Onderzoek Nederland ASTRON, Dwingeloo - Netherlands

^[69] Univ Chicago, Enrico Fermi Inst, 5640 S Ellis Ave, Chicago, IL 60637 - USA

^[70] NYU, 550 1St Ave, New York, NY 10003 - USA

^[71] Karlsruhe Inst Technol, Inst Prozessdatenverarbeitung & Elekt, Karlsruhe - Germany

^[72] J Stefan Inst, Expt Particle Phys Dept, Ljubljana - Slovenia

^[73] Univ Nova Gorica, CAC, Nova Gorica - Slovenia

^[74] UNR, CONICET, Inst Fis Rosario IFIR, Rosario - Argentina

^[75] UNR, Fac Ciencias Bioquim & Farmaceut, Rosario - Argentina

^[76] Univ Tokyo, Inst Cosm Ray Res, Tokyo - Japan

^[77] Ctr Brasileiro Pesquisas Fis, Rio De Janeiro, RJ - Brazil

^[78] Univ Lodz, Fac Astrophys, Lodz - Poland

^[79] Univ Lodz, Fac High Energy Astrophys, Lodz - Poland

^[80] Univ Estadual Feira de Santana, Feira De Santana - Brazil

^[81] Inst Space Sci, Bucharest - Romania

^[82] Colorado Sch Mines, Golden, CO 80401 - USA

^[83] Ctr Fed Educ Tecnol Celso Suckow da Fonseca, Nova Friburgo - Brazil

^[84] Univ Fed ABC, Santo Andre, SP - Brazil

^[85] Univ Paris 06, LPNHE, Paris - France

^[86] Univ Paris 07, CNRS IN2P3, Paris - France

^[87] Benemerita Univ Autonoma Puebla, Puebla - Mexico

^[88] Univ Libre Bruxelles, Brussels - Belgium

^[89] Ctr Invest & Estudios Avanzados IPN, CINVESTAV, Mexico City, DF - Mexico

^[90] Louisiana State Univ, Baton Rouge, LA 70803 - USA

^[91] Ist Nazl Fis Nucl, Sez Roma Tor Vergata, Rome - Italy

^[92] Univ Roma Tor Vergata, Dipartimento Fis, Rome - Italy

^[93] Univ Fed Alfenas, Pocos De Caldas - Brazil

^[94] Michigan Technol Univ, Houghton, MI 49931 - USA

^[95] Karlsruhe Inst Technol, Karlsruhe - Germany

^[96] Charles Univ Prague, Inst Particle & Nucl Phys, Fac Math & Phys, Prague - Czech Republic

^[97] Consejo Nacl Invest Cient & Tecn, Villa Martelli - Argentina

^[98] CITEDEF, Ctr Invest Laseres & Aplicac, Villa Martelli - Argentina

^[99] IPN, UPIITA, Mexico City, DF - Mexico

^[100] Univ Aquila, Dipartimento Sci Fis & Chim, Laquila - Italy

^[101] Univ Groningen, KVI Ctr Adv Radiat Technol, Groningen - Netherlands

^[102] Univ Bucharest, Phys Dept, Bucharest - Romania

^[103] Univ Nebraska, Lincoln, NE 68588 - USA

^[104] Univ Medellin, Medellin - Colombia

^[105] Univ Leeds, Sch Phys & Astron, Leeds, W Yorkshire - England

• Tipo de documento: Artigo Científico
• Fonte: ASTROPHYSICAL JOURNAL; v. 868, n. 1 NOV 20 2018.
• Citações Web of Science: 14

Resumo

We present a detailed study of the large-scale anisotropies of cosmic rays with energies above 4 EeV measured using the Pierre Auger Observatory. For the energy bins {[}4, 8] EeV and E >= 8 EeV, the most significant signal is a dipolar modulation in R.A. at energies above 8 EeV, as previously reported. In this paper we further scrutinize the highest-energy bin by splitting it into three energy ranges. We find that the amplitude of the dipole increases with energy above 4 EeV. The growth can be fitted with a power law with index beta = 0.79 +/- 0.19. The directions of the dipoles are consistent with an extragalactic origin of these anisotropies at all the energies considered. Additionally, we have estimated the quadrupolar components of the anisotropy: they are not statistically significant. We discuss the results in the context of the predictions from different models for the distribution of ultrahigh-energy sources and cosmic magnetic fields. (AU)

• Processo FAPESP: 99/05404-3 - Observatório Pierre Auger
• Beneficiário: Carlos Ourivio Escobar
• Modalidade de apoio: Auxílio à Pesquisa - Temático
• Processo FAPESP: 10/07359-6 - Estudo dos raios cósmicos de mais altas energias com o Observatório Pierre Auger
• Beneficiário: Carola Dobrigkeit Chinellato
• Modalidade de apoio: Auxílio à Pesquisa - Temático