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Holt, E.J. Quel, E. Kemp, E. Mayotte, E.M. Santos, E. Roulet, E. Santos, E. Varela, E. Zas, F. Arqueros, F. Barbato, F. Canfora, F. Contreras, F. Diogo, F. Fenu, F. Gat\\'e, F.G. Schr\\\"oder, F. Guarino, F.L. Briechle, F. Montanet, F. Oikonomou, F. Pedreira, F. Riehn, F. Salamida, F. Salesa Greus, F. S\\'anchez, F. Sarazin, F. Strafella, F. Suarez, F. Zuccarello, G.A. Anastasi, G. Avila, G. Cataldi, G.C. Hill, G. Consolati, G. De Mauro, G. Farrar, G. Golup, G. Kukec Mezek, G. Marsella, G. Matthiae, G. Medina-Tanco, G. M\\\"uller, G. Parente, G.P. Guedes, G. Rodriguez Fernandez, G.R. Snow, G. Salina, G. Sigl, G. Silli, G. Torralba Elipe, G. van Aar, G. Varner, H. Asorey, H. Falcke, H. Gemmeke, H.J. Mathes, H. Martinez, H.O. Klages, H. Salazar, H. Schieler, H. Wahlberg, H. Wilczy\\'nski, I. Allekotte, I. Al Samarai, I. Brancus, I.C. Mari\\c{s}, I. De Mitri, I.D. Vergara Quispe, I.F.M. Albuquerque, I. Jandt, I. Katkov, I. Lhenry-Yvon, I. Naranjo, I. Vali\\~no, J.A. Bellido, J.A. 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Boh\\'a\\v{c}ov\\'a, M. Buscemi, M.E. Bertaina, M. Erdmann, M. Erfani, M. Giammarchi, M. Giller, M. G\\'omez Berisso, M. Hrabovsk\\'y, M.I. Micheletti, M.J. Cooper, M. Josebachuili, M.J. Roncoroni, M. Kleifges, M. Lauscher, M.L. D\\'iaz Castro, M. Malacari, M. Mallamaci, M.M. Freire, M. Mostaf\\'a, M. Niculescu-Oglinzanu, M. Niechciol, M. Palatka, M. Pech, M. Perl\\'in, M. Pimenta, M. Platino, M. Plum, M. Prouza, M.R. Coluccia, M.R. Hampel, M. Risse, M. Roth, M. Schauer, M. Schimp, M. Settimo, M. Suarez Dur\\'an, M.T. Dova, M. Trini, M. Unger, M. Urban, M. Weber, M. Wirtz, M. Zavrtanik, M. Ziolkowski, N. Arsene, N. Borodai, N. Fazzini, N. Gonz\\'alez, N. Kemmerich, N. Krohm, N. Kunka, O.A. Taborda, O. Deligny, O. Fratu, O. Kambeitz, O. Mart\\'inez Bravo, O. Scholten, O. Sima, O. Wainberg, P. Abreu, P. Assis, P. Billoir, P. Buchholz, P.F. G\\'omez Vitale, P.G. Isar, P. Gorham, P. Hansen, P. Heimann, P.H. Nguyen, P. Homola, P. Horvath, P.L. Biermann, P.L. Ghia, P. Mantsch, P.O. Mazur, P. Papenbreer, P. Pieroni, P. Privitera, P. Ristori, P. Ruehl, P. Sanchez-Lucas, P. Schov\\'anek, P. Sommers, P. Stassi, P. Travnicek, P. van Bodegom, Q. Dorosti, Q. Luce, R.A. V\\'azquez, R. Caruso, R.C. dos Anjos, R. Colalillo, R. Concei\\c{c}\\~ao, R.C. Shellard, R. Engel, R. Gaior, R.J. Barreira Luz, R. Krause, R. Legumina, R. L\\'opez, R.M. de Almeida, R.M. Kieckhafer, R. Mussa, R. Pelayo, R. Piegaia, R. Ramos-Pollan, R.R. Prado, R. Sarmento, R. Sato, R. Squartini, R. Ulrich, R. \\v{S}m\\'ida, R.W. Clay, S. Andringa, S. Buitink, S. Coutu, S. D'Amico, S. Dasso, S.G. Blaess, S. Jansen, S.J. De Jong, S.J. Saffi, S.J. Sciutto, S. Mathys, S. Michal, S. Mollerach, S. M\\\"uller, S. Petrera, S. Querchfeld, S. Quinn, S. Sonntag, S. Stani\\v{c}, S. Vorobiov, T.A. Harrison, T. Bretz, T.D. Grubb, T. Fujii, T. Hebbeker, The Pierre Auger Collaboration: A. Aab, T. Huege, T. Niggemann, T. Paul, T. Pierog, T. Sudholz, T. Suomij\\\"arvi, U. Giaccari, V. de Souza, V.M. Theodoro, V. Novotny, V. Pirronello, V. Rizi, V. Scherini, V. Verzi, W. Rodrigues de Carvalho, X. Bertou, Z. Szadkowski, Z. Zong","submitted_at":"2017-09-21T13:42:10Z","abstract_excerpt":"Cosmic rays are atomic nuclei arriving from outer space that reach the highest energies observed in nature. Clues to their origin come from studying the distribution of their arrival directions. Using $3 \\times 10^4$ cosmic rays above $8 \\times 10^{18}$ electron volts, recorded with the Pierre Auger Observatory from a total exposure of 76,800 square kilometers steradian year, we report an anisotropy in the arrival directions. 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Morello, C.O. Escobar, C. Peters, C. Porowski, C. Timmermans, C. Ventura, D. Boncioli, D. Garcia-Pinto, D. G{\\l}as, D. Harari, D. Heck, D. Kuempel, D. LaHurd, D. Lo Presti, D. Mandat, D. Martello, D. Melo, D. Mockler, D. Nitz, D. Nosek, D. Ravignani, D. Rogozin, D. Schmidt, D. Stanca, D. Veberi\\v{c}, D. Walz, D. Wittkowski, D. Zavrtanik, E. Holt, E.J. Quel, E. Kemp, E. Mayotte, E.M. Santos, E. Roulet, E. Santos, E. Varela, E. Zas, F. Arqueros, F. Barbato, F. Canfora, F. Contreras, F. Diogo, F. Fenu, F. Gat\\'e, F.G. Schr\\\"oder, F. Guarino, F.L. Briechle, F. Montanet, F. Oikonomou, F. Pedreira, F. Riehn, F. Salamida, F. Salesa Greus, F. S\\'anchez, F. Sarazin, F. Strafella, F. Suarez, F. Zuccarello, G.A. Anastasi, G. Avila, G. Cataldi, G.C. Hill, G. Consolati, G. De Mauro, G. Farrar, G. Golup, G. Kukec Mezek, G. Marsella, G. Matthiae, G. Medina-Tanco, G. M\\\"uller, G. Parente, G.P. Guedes, G. Rodriguez Fernandez, G.R. Snow, G. Salina, G. Sigl, G. Silli, G. 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Kampert, K. Link, K.S. Caballero-Mora, L. Anchordoqui, L.A. N\\'u\\~nez, L. A. S. Pereira, L. Caccianiga, L. Caramete, L. Cazon, L. Collica, L. Lopes, L. Middendorf, L. Miramonti, L. Nellen, L. Niemietz, L. No\\v{z}ka, L. Ochilo, L. Perrone, L. Tomankova, L. Valore, L. Villase\\~nor, L. Wiencke, L. Yang, M. Aglietta, M.A. Leigui de Oliveira, M.A. Muller, M. Boh\\'a\\v{c}ov\\'a, M. Buscemi, M.E. Bertaina, M. Erdmann, M. Erfani, M. Giammarchi, M. Giller, M. G\\'omez Berisso, M. Hrabovsk\\'y, M.I. Micheletti, M.J. Cooper, M. Josebachuili, M.J. Roncoroni, M. Kleifges, M. Lauscher, M.L. D\\'iaz Castro, M. Malacari, M. Mallamaci, M.M. Freire, M. Mostaf\\'a, M. Niculescu-Oglinzanu, M. Niechciol, M. Palatka, M. Pech, M. Perl\\'in, M. Pimenta, M. Platino, M. Plum, M. Prouza, M.R. Coluccia, M.R. Hampel, M. Risse, M. Roth, M. Schauer, M. Schimp, M. Settimo, M. Suarez Dur\\'an, M.T. Dova, M. Trini, M. Unger, M. Urban, M. Weber, M. Wirtz, M. Zavrtanik, M. Ziolkowski, N. Arsene, N. Borodai, N. 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Sciutto, S. Mathys, S. Michal, S. Mollerach, S. M\\\"uller, S. Petrera, S. Querchfeld, S. Quinn, S. Sonntag, S. Stani\\v{c}, S. Vorobiov, T.A. Harrison, T. Bretz, T.D. Grubb, T. Fujii, T. Hebbeker, The Pierre Auger Collaboration: A. Aab, T. Huege, T. Niggemann, T. Paul, T. Pierog, T. Sudholz, T. Suomij\\\"arvi, U. Giaccari, V. de Souza, V.M. Theodoro, V. Novotny, V. Pirronello, V. Rizi, V. Scherini, V. Verzi, W. Rodrigues de Carvalho, X. Bertou, Z. Szadkowski, Z. Zong","submitted_at":"2017-09-21T13:42:10Z","abstract_excerpt":"Cosmic rays are atomic nuclei arriving from outer space that reach the highest energies observed in nature. Clues to their origin come from studying the distribution of their arrival directions. Using $3 \\times 10^4$ cosmic rays above $8 \\times 10^{18}$ electron volts, recorded with the Pierre Auger Observatory from a total exposure of 76,800 square kilometers steradian year, we report an anisotropy in the arrival directions. 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