A TARGETED SEARCH FOR POINT SOURCES OF EeV NEUTRONS

Autor(es):Mostrar menos -

Aab, A. ^{[1, 2, 3, 4, 5]} ; Abreu, P. ^{[6, 7]} ; Aglietta, M. ^{[8, 9]} ; Ahlers, M. ^[10] ; Ahn, E. J. ^[11] ; Al Samarai, I. ^[12] ; Albuquerque, I. F. M. ^[13] ; Allekotte, I. ^{[14, 15]} ; Allen, J. ^[16] ; Allison, P. ^[17] ; Almela, A. ^{[18, 3, 4, 19]} ; Castillo, J. Alvarez ^[20] ; Alvarez-Muniz, J. ^[4] ; Batista, R. Alves ^[21] ; Ambrosio, M. ^{[22, 23]} ; Aminaei, A. ^{[3, 24]} ; Anchordoqui, L. ^[25] ; Andringa, S. ^[6] ; Aramo, C. ^{[22, 23]} ; Arqueros, F. ^[26] ; Asorey, H. ^{[14, 15]} ; Assis, P. ^{[6, 7]} ; Aublin, J. ^[27] ; Ave, M. ^[4] ; Avenier, M. ^[28] ; Avila, G. ^[29] ; Badescu, A. M. ^[30] ; Barber, K. B. ^[31] ; Baumel, J. ^[32] ; Baus, C. ^[32] ; Beatty, J. J. ^[17] ; Becker, K. H. ^[33] ; Bellido, J. A. ^[31] ; Berat, C. ^[28] ; Bertou, X. ^[14] ; Biermann, P. L. ^[34] ; Billoir, P. ^[27] ; Blanco, F. ^[26] ; Blanco, M. ^[27] ; Bleve, C. ^[33] ; Blumer, H. ^{[3, 32]} ; Boiiacova, M. ^[35] ; Boncioli, D. ^[36] ; Bonifazi, C. ^[37] ; Bonino, R. ^{[8, 9]} ; Borodai, N. ^[38] ; Brack, J. ^[39] ; Brancus, I. ; Brogueira, P. ^{[6, 7]} ; Brown, W. C. ^[40] ; Buchholz, P. ^[1] ; Bueno, A. ^{[41, 42, 3]} ; Buscemi, M. ^{[22, 23]} ; Caballero-Mora, K. S. ^{[43, 4, 44]} ; Caccianiga, B. ^{[45, 46]} ; Caccianiga, L. ^[27] ; Candusso, M. ^{[47, 48]} ; Caramete, L. ^[34] ; Caruso, R. ^{[49, 50]} ; Castellina, A. ^{[8, 9, 3]} ; Cataldi, G. ^{[51, 52]} ; Cazon, L. ^{[6, 7]} ; Cester, R. ^{[53, 9]} ; Chavez, A. G. ^[54] ; Cheng, S. H. ^[43] ; Chiavassa, A. ^{[8, 9, 19]} ; Chinellato, J. A. ^[55] ; Chudoba, J. ^[35] ; Cilmo, M. ^{[22, 23]} ; Clay, R. W. ^[31] ; Cocciolo, G. ^{[51, 52]} ; Colalillo, R. ^{[22, 23]} ; Collica, L. ^{[45, 46]} ; Coluccia, M. R. ^{[51, 52]} ; Conceicao, R. ^[6] ; Contreras, F. ^[56] ; Cooper, M. J. ^[31] ; Coutu, S. ^[43] ; Covault, C. E. ^[57] ; Criss, A. ^[43] ; Cronin, J. ^[58] ; Curutiu, A. ^[34] ; Dallier, R. ^{[59, 60]} ; Daniel, B. ^[55] ; Dasso, S. ^{[61, 62, 63]} ; Daumiller, K. ^[3] ; Dawson, B. R. ^[31] ; De Almeida, R. M. ^[2] ; De Domenico, M. ^{[49, 50]} ; De Jong, S. J. ^{[64, 24]} ; De Mello Neto, J. R. T. ^[37] ; De Mitri, I. ^{[51, 52]} ; De Oliveira, J. ^[2] ; De Souza, V. ^[65] ; Del Peral, L. ^[66] ; Deligny, O. ^[12] ; Dembinski, H. ^[3] ; Dhital, N. ^[67] ; Di Giulio, C. ^{[47, 48]} ; Di Matteo, A. ^[68] ; Diaz, J. C. ^[67] ; Castro, M. L. Diaz ^[55] ; Diep, P. N. ^[69] ; Diogo, F. ^{[6, 7]} ; Dobrigkeit, C. ^[55] ; Docters, W. ^[70] ; D'Olivo, J. C. ^[20] ; Dong, P. N. ^{[69, 12]} ; Dorofeev, A. ^[39] ; Dova, M. T. ^{[71, 72]} ; Ebr, J. ^[35] ; Engel, R. ^[3] ; Erdmann, M. ^[73] ; Erfani, M. ^[1] ; Escobar, C. O. ^{[55, 11]} ; Espadanal, J. ^{[6, 7]} ; Etchegoyen, A. ^{[18, 19]} ; Luis, P. Facal San ^[58] ; Falcke, H. ^{[64, 74, 24]} ; Fang, K. ^[58] ; Farrar, G. ^[16] ; Fauth, A. C. ^[55] ; Fazzini, N. ^[11] ; Ferguson, A. P. ^[57] ; Fernandes, M. ^[37] ; Fick, B. ^[67] ; Figueira, J. M. ^[19] ; Filevich, A. ^[19] ; Filipcic, A. ^{[75, 76]} ; Fox, B. D. ^[77] ; Fratu, O. ^[30] ; Frohlich, U. ^[1] ; Fuchs, B. ^[32] ; Fuji, T. ^[58] ; Gaior, R. ^[27] ; Garia, B. ^{[78, 79]} ; Roca, S. T. Garcia ^[4] ; Garcia-Gamez, D. ^[80] ; Garcia-Pinto, D. ^[26] ; Garilli, G. ^{[49, 50]} ; Bravo, A. Gascon ^{[41, 42]} ; Gate, F. ^[59] ; Gemmeke, H. ^[81] ; Ghia, P. L. ^[27] ; Giaccari, U. ^[37] ; Giammarchi, M. ^{[45, 46]} ; Giller, M. ; Glaser, C. ^[70] ; Glass, H. ^[11] ; Albarracin, F. Gomez ^{[71, 72]} ; Berisso, M. Gomez ^{[14, 15]} ; Vitale, P. F. Gomez ^[29] ; Goncalves, P. ^{[6, 7]} ; Gonzalez, J. G. ^[32] ; Gookin, B. ^[39] ; Gorgi, A. ^{[8, 9]} ; Gorham, P. ^[77] ; Gouffon, P. ^[13] ; Grebe, S. ^{[64, 24]} ; Griffith, N. ^[17] ; Grillo, A. F. ^[36] ; Grubb, T. D. ^[31] ; Guardincerri, Y. ^{[62, 63]} ; Guarino, F. ^{[22, 23]} ; Guedes, G. P. ^{[82, 83]} ; Hansen, P. ^{[71, 72]} ; Harari, D. ^{[14, 15]} ; Harrison, T. A. ^[31] ; Harton, J. L. ^[39] ; Hasankiadeh, Q. D. ^[3] ; Haungs, A. ^[3] ; Hebbeker, T. ^[73] ; Heck, D. ^[3] ; Heimann, P. ^[1] ; Herve, A. E. ^[3] ; Hill, G. C. ^[31] ; Hojvat, C. ^[11] ; Hollon, N. ^[58] ; Holt, E. ^[3] ; Homola, P. ^{[1, 38]} ; Horandel, J. R. ^{[64, 24]} ; Horvath, P. ^[84] ; Hrabovsky, M. ^{[35, 84]} ; Huber, D. ^[32] ; Huege, T. ^[3] ; Insolia, A. ^{[49, 50]} ; Isar, P. G. ^[85] ; Islo, K. ^[25] ; Jandt, I. ^[33] ; Jansen, S. ^{[64, 24]} ; Jarne, C. ^{[71, 72]} ; Josebachuili, M. ^[19] ; Kaapa, A. ^[33] ; Kambeitz, O. ; Kampert, K. H. ^[33] ; Kasper, P. ^[11] ; Katkov, I. ^[32] ; Kegl, B. ^[80] ; Keilhauer, B. ^[3] ; Keivani, A. ^[86] ; Kemp, E. ^[55] ; Kieckhafer, R. M. ^[67] ; Klages, H. O. ^[3] ; Kleifges, M. ^[81] ; Kleinfeller, J. ^[56] ; Krause, R. ^[73] ; Krohm, N. ^[33] ; Kromer, O. ^[81] ; Kruppke-Hansen, D. ^[33] ; Kuempel, D. ^[73] ; Kunka, N. ^[81] ; La Rosa, G. ^[87] ; LaHurd, D. ^[57] ; Latronico, L. ^{[8, 9]} ; Lauer, R. ^[88] ; Lauscher, M. ^[73] ; Lautridou, P. ^[59] ; Le Coz, S. ^[28] ; Leao, M. S. A. B. ^[89] ; Lebrun, D. ^[28] ; Lebrun, P. ^[11] ; De Oliveira, M. A. Leigui ^[90] ; Letessier-Selvon, A. ^[27] ; Lhenry-Yvon, I. ^[12] ; Link, K. ^[32] ; Lopez, R. ^[91] ; Aguera, A. Lopez ^[4] ; Louedec, K. ^[28] ; Bahilo, J. Lozano ^{[41, 42]} ; Lu, L. ^{[33, 92]} ; Lucero, A. ^[19] ; Ludwig, M. ^[32] ; Lyberis, H. ^[37] ; Maccarone, M. C. ^[87] ; Malacari, M. ^[31] ; Maldera, S. ^{[8, 9]} ; Maller, J. ^[59] ; Mandat, D. ^[35] ; Mantsch, P. ^[11] ; Mariazzi, A. G. ^{[71, 72]} ; Marin, V. ^[59] ; Maris, I. C. ^[27] ; Marsella, G. ^{[51, 52]} ; Martello, D. ^{[51, 52]} ; Martin, L. ^{[59, 60]} ; Martinez, H. ^[44] ; Bravo, O. Martinez ^[91] ; Martraire, D. ^[12] ; Meza, J. J. Masia ^{[62, 63]} ; Mathes, H. J. ^[3] ; Mathys, S. ; Matthews, A. J. ^[88] ; Matthews, J. ^[86] ; Matthiae, G. ^{[47, 48]} ; Maurel, D. ^[32] ; Maurizio, D. ^[93] ; Mayotte, E. ^[94] ; Mazur, P. O. ^[11] ; Medina, C. ^[94] ; Medina-Tanco, G. ^[20] ; Melissas, M. ^[32] ; Melo, D. ^[19] ; Menichetti, E. ^{[53, 9]} ; Menshikov, A. ^[81] ; Messina, S. ^[70] ; Meyhandan, R. ^[77] ; Micanovic, S. ^[95] ; Micheletti, M. I. ^{[5, 96]} ; Middendorf, L. ^[73] ; Minaya, I. A. ^[26] ; Miramonti, L. ^{[45, 46]} ; Mitrica, B. ^[97] ; Molina-Bueno, L. ^{[41, 42]} ; Mollerach, S. ^[14] ; Monasor, M. ^[58] ; Ragaigne, D. Monnier ^[80] ; Montanet, F. ^[28] ; Morello, C. ^{[8, 9]} ; Moreno, J. C. ^{[71, 72]} ; Mostafa, M. ^[43] ; Moura, C. A. ^[90] ; Muller, M. A. ^{[55, 98]} ; Muller, G. ^[73] ; Munchmeyer, M. ^[27] ; Mussa, R. ^{[53, 9]} ; Navarra, G. ^{[8, 9]} ; Navas, S. ^{[41, 42]} ; Necesal, P. ^[35] ; Nellen, L. ^[20] ; Nelles, A. ^{[64, 24]} ; Neuser, J. ^[33] ; Niechciol, M. ^[1] ; Niemietz, L. ^[33] ; Niggemann, T. ^[73] ; Nitz, D. ^[67] ; Nosek, D. ^[99] ; Novotny, V. ^[99] ; Nozka, L. ^[84] ; Ochilo, L. ^[1] ; Olinto, A. ^[58] ; Oliveira, M. ^{[6, 7]} ; Ortiz, M. ^[26] ; Pacheco, N. ^[66] ; Selmi-Dei, D. Pakk ^[55] ; Palatka, M. ^[35] ; Pallotta, J. ^{[100, 101]} ; Palmieri, N. ; Papenbreer, P. ; Parente, G. ^[4] ; Parra, A. ^[4] ; Pastor, S. ^[102] ; Paul, T. ^[25] ; Pech, M. ^[35] ; Pekala, J. ^[38] ; Pelayo, R. ^[91] ; Pepe, I. M. ^[103] ; Perrone, L. ^{[51, 52]} ; Pesce, R. ^{[104, 105]} ; Petermann, E. ^[106] ; Peters, C. ^[73] ; Petrera, S. ^{[68, 107]} ; Petrolini, A. ^{[104, 105]} ; Petrov, Y. ^[39] ; Piegaia, R. ^{[62, 63]} ; Pierog, T. ^[3] ; Pieroni, P. ^{[62, 63]} ; Pimenta, M. ^{[6, 7]} ; Pirronello, V. ^{[49, 50]} ; Platino, M. ^[19] ; Plum, M. ^[73] ; Porcelli, A. ^[3] ; Porowski, C. ^[38] ; Privitera, P. ^[58] ; Prouza, M. ^[35] ; Purrello, V. ^[14] ; Quel, E. J. ^{[100, 101]} ; Querchfeld, S. ; Quinn, S. ^[57] ; Rautenberg, J. ^[33] ; Ravel, O. ^[59] ; Ravignani, D. ^[19] ; Revenu, B. ^[59] ; Ridky, J. ^[35] ; Riggi, S. ^{[4, 87]} ; Risse, M. ^[1] ; Ristori, P. ^{[100, 101]} ; Rizi, V. ^[68] ; Roberts, J. ^[16] ; De Carvalho, W. Rodrigues ^[4] ; Cabo, I. Rodriguez ^[4] ; Fernandez, G. Rodriguez ^{[47, 4, 48]} ; Rojo, J. Rodriguez ^[56] ; Rodriguez-Frias, M. D. ^[66] ; Ros, G. ^[66] ; Rosado, J. ^[26] ; Rossler, T. ^[84] ; Roth, M. ^[3] ; Roulet, E. ^{[14, 15]} ; Rovero, A. C. ^[61] ; Ruhle, C. ^[81] ; Saffi, S. J. ^[31] ; Saftoiu, A. ^[97] ; Salamida, F. ^[12] ; Salazar, H. ^[91] ; Greus, F. Salesa ^[43] ; Salina, G. ^{[47, 48]} ; Sanchaz, F. ^[19] ; Sanchez-Lucas, P. ^{[41, 42]} ; Santo, C. E. ^{[6, 7]} ; Santos, E. ^{[6, 7]} ; Santos, E. M. ^[13] ; Sarazin, F. ^[94] ; Sarkar, B. ^[33] ; Sarmento, R. ^[6] ; Sato, R. ^[56] ; Scharf, N. ^[73] ; Scherini, V. ^[51] ; Schieler, H. ^[3] ; Schiffer, P. ^[21] ; Schmidt, A. ^[81] ; Scholten, O. ^[70] ; Schoorlemmer, H. ^{[64, 77, 24]} ; Schovanek, P. ^[35] ; Schulz, A. ^[3] ; Schulz, J. ^[24] ; Sciutto, S. J. ^{[71, 72]} ; Segreto, A. ^[87] ; Settimo, M. ^[27] ; Shadkam, A. ^[86] ; Shellard, R. C. ^[93] ; Sidelnik, I. ^{[14, 15]} ; Sigl, G. ^[21] ; Sima, O. ^[108] ; Smialkowski, A. ; Smida, R. ^[3] ; Snow, G. R. ^[106] ; Sommers, P. ^[43] ; Sorokin, J. ^[31] ; Squartini, R. ^[56] ; Srivastava, Y. N. ^[109] ; Stanic, S. ^[76] ; Stapleton, J. ^[17] ; Stasielak, J. ^[38] ; Stephan, M. ^[73] ; Stutz, A. ^[28] ; Suarez, F. ^[19] ; Suomijarvi, T. ^[12] ; Supanitsky, A. D. ^[61] ; Sutherland, M. S. ^[86] ; Swain, J. ^[109] ; Szadkowski, Z. ; Szuba, M. ^[3] ; Taborda, O. A. ^{[14, 15]} ; Tapia, A. ^[19] ; Tartare, M. ^[28] ; Thao, N. T. ^[69] ; Theodoro, V. M. ; Tiffenberg, J. ^{[62, 63]} ; Timmermans, C. ^{[64, 24]} ; Peixoto, C. J. Todero ^[110] ; Toma, G. ^[97] ; Tomankova, L. ^[3] ; Tome, B. ^{[6, 7]} ; Tonachini, A. ^{[53, 9]} ; Elipe, G. Torralba ^[4] ; Machado, D. Torres ^[59] ; Travnicek, P. ^[35] ; Trovato, E. ^{[49, 50]} ; Tueros, M. ^[4] ; Ulrich, R. ^[3] ; Unger, M. ^[3] ; Urban, M. ^[73] ; Galicia, J. F. Valdes ^[20] ; Valino, I. ^[4] ; Valore, L. ^{[22, 23]} ; Van Aar, G. ^[24] ; Van den Berg, A. M. ^[70] ; Van Velzen, S. ^[24] ; Van Vliet, A. ^[21] ; Varela, E. ^[91] ; Cardenas, B. Vargas ^[20] ; Varner, G. ^[77] ; Vazquez, J. R. ^[26] ; Vazquez, R. A. ^[4] ; Veberic, D. ^[80] ; Verzi, V. ^{[47, 48]} ; Vicha, J. ^[35] ; Videla, M. ^[19] ; Villasenor, L. ^[54] ; Vlcek, B. ^[25] ; Wahlberg, H. ^{[71, 72]} ; Wainberg, O. ^{[18, 19]} ; Walz, D. ^[73] ; Watson, A. A. ^[92] ; Weber, M. ^[81] ; Weidenhaupt, K. ^[73] ; Weindl, A. ^[3] ; Werner, F. ^[32] ; Whelan, B. J. ^[43] ; Widom, A. ^[109] ; Wiencke, L. ^[94] ; Wilczynska, B. ^[38] ; Wilczynski, H. ^[38] ; Will, M. ^[3] ; Williams, C. ^[58] ; Winchen, T. ^[73] ; Wittkowski, D. ^[33] ; Wundheiler, B. ^[19] ; Wykes, S. ^[24] ; Yamamoto, T. ^[58] ; Yapici, T. ^[67] ; Younk, P. ^[111] ; Yuan, G. ^[86] ; Yushkov, A. ^[1] ; Zamorano, B. ^{[41, 42]} ; Zas, E. ^[4] ; Zavrtanik, D. ^{[75, 76]} ; Zavrtanik, M. ^{[75, 76]} ; Zaw, I. ^[16] ; Zepeda, A. ^{[17, 44]} ; Zhou, J. ^[58] ; Zhu, Y. ^[80] ; Silva, M. Zimbres ^[55] ; Ziolkowski, M. ^[1] ; Collaboration, Pierre Auger

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

^[1] Univ Siegen, D-57068 Siegen - Germany

^[2] Univ Fed Fluminense, EEIMVR, Volta Redonda, RJ - Brazil

^[3] Karlsruhe Inst Technol, Inst Kernphys, Karlsruhe - Germany

^[4] Univ Santiago Compostela, Santiago De Compostela - Spain

^[5] Fac Ciencias Bioquim & Farmaceut UNR, Rosario - Argentina

^[6] UL, LIP, Lisbon - Portugal

^[7] UL, IST, Lisbon - Portugal

^[8] Univ Turin, Osservatorio Astrofis Torino INAF, Turin - Italy

^[9] Sezione Ist Nazl Fis Nucl, Turin - Italy

^[10] Univ Wisconsin, Madison, WI - USA

^[11] Fermilab Natl Accelerator Lab, Batavia, IL - USA

^[12] Univ Paris 11, IPNO, CNRS IN2P3, Orsay - France

^[13] Univ Sao Paulo, Inst Fis, BR-01498 Sao Paulo - Brazil

^[14] Ctr Atom Bariloche, San Carlos De Bariloche, Rio Negro - Argentina

^[15] Inst Balseiro CNEA UNCuyo CONICET, San Carlos De Bariloche, Rio Negro - Argentina

^[16] NYU, New York, NY - USA

^[17] Ohio State Univ, Columbus, OH 43210 - USA

^[18] Univ Tecnol Nacl, Fac Reg Buenos Aires, Buenos Aires, DF - Argentina

^[19] CNEA CONICET UNSAM, Inst Tecnol Detect & Astroparticulas, Buenos Aires, DF - Argentina

^[20] Univ Nacl Autonoma Mexico, Mexico City 04510, DF - Mexico

^[21] Univ Hamburg, Hamburg - Germany

^[22] Univ Naples Federico II, Naples - Italy

^[23] Sezione Ist Nazl Fis Nucl, Naples - Italy

^[24] Radboud Univ Nijmegen, IMAPP, Nijmegen - Netherlands

^[25] Univ Wisconsin, Milwaukee, WI 53201 - USA

^[26] Univ Complutense Madrid, Madrid - Spain

^[27] Univ Paris 06, LPNHE, CNRS IN2P3, Paris - France

^[28] Univ Grenoble Alpes, LPSC, CNRS IN2P3, Grenoble - France

^[29] Observatorio Pierre Auger & Comis Nacl Energia At, Malargue - Argentina

^[30] Univ Politehn Bucuresti, Bucharest - Romania

^[31] Univ Adelaide, Adelaide, SA - Australia

^[32] Karlsruhe Inst Technol, IEKP, Karlsruhe - Germany

^[33] Berg Univ Wuppertal, Wuppertal - Germany

^[34] Max Planck Inst Radioastron, D-53121 Bonn - Germany

^[35] Acad Sci Czech Republic, Inst Phys, Prague - Czech Republic

^[36] INFN, Lab Nazl Gran Sasso, Laquila - Italy

^[37] Univ Fed Rio de Janeiro, Inst Fis, Rio De Janeiro - Brazil

^[38] Inst Nucl Phys PAN, Krakow - Poland

^[39] Colorado State Univ, Ft Collins, CO 80523 - USA

^[40] Colorado State Univ, Pueblo, CO - USA

^[41] Univ Granada, Granada - Spain

^[42] CAFPE, Granada - Spain

^[43] Penn State Univ, University Pk, PA 16802 - USA

^[44] CINVESTAV, Mexico City, DF - Mexico

^[45] Univ Milan, Milan - Italy

^[46] Sezione Ist Nazl Fis Nucl, Milan - Italy

^[47] Sezione Ist Nazl Fis Nucl, Rome - Italy

^[48] Univ Roma Tor Vergata, Rome - Italy

^[49] Sezione Ist Nazl Fis Nucl, Catania - Italy

^[50] Catania Univ, Catania - Italy

^[51] Univ Salento, Dipartimento Matemat & Fis E De Giorgi, Lecce - Italy

^[52] Sezione Ist Nazl Fis Nucl, Lecce - Italy

^[53] Univ Turin, Turin - Italy

^[54] Univ Michoacana, Morelia, Michoacan - Mexico

^[55] Univ Estadual Campinas, Campinas, SP - Brazil

^[56] Observ Pierre Auger, Malargue - Argentina

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

^[58] Univ Chicago, Enrico Fermi Inst, Chicago, IL 60637 - USA

^[59] Univ Nantes, CNRS IN2P3, Ecole Mines Nantes, SUBATECH, Nantes - France

^[60] CNRS INSU, Observ Paris, Stn Radioastron Nacy, Paris - France

^[61] CONICET UBA, Inst Astron & Fis Espacio, Buenos Aires, DF - Argentina

^[62] Consejo Nacl Invest Cient & Tecn, Buenos Aires, DF - Argentina

^[63] Univ Buenos Aires, FCEyN, Dept Fis, Buenos Aires, DF - Argentina

^[64] Nikhef, Amsterdam - Netherlands

^[65] Univ Sao Paulo, Inst Fis, Sao Carlos, SP - Brazil

^[66] Univ Alcala De Henares, Madrid - Spain

^[67] Michigan Technol Univ, Houghton, MI 49931 - USA

^[68] Univ Aquila, Dipartimento Sci Fis & Chim, I-67100 Laquila - Italy

^[69] INST, Hanoi - Vietnam

^[70] Univ Groningen, KVI Ctr Adv Radiat Technol, Groningen - Netherlands

^[71] Consejo Nacl Invest Cient & Tecn, La Plata - Argentina

^[72] Univ Nacl Plata, IFLP, La Plata - Argentina

^[73] Rhein Westfal TH Aachen, Phys Inst A, Aachen - Germany

^[74] ASTRON, Dwingeloo - Netherlands

^[75] J Stefan Inst, Ljubljana - Slovenia

^[76] Univ Nova Gorica, Lab Astroparticle Phys, Pristava - Slovenia

^[77] Univ Hawaii, Honolulu, HI 96822 - USA

^[78] CNEA CONICET UNSAM, Inst Tecnol Detect & Astrparticulas, Mendoza - Argentina

^[79] Natl Technol Univ, CONICET CNEA, Fac Mendoza, Mendoza - Argentina

^[80] Univ Paris 11, LAL, Paris - France

^[81] Karlsruhe Inst Technol, North Inst Prozessdatenverarbeirung &Elect, Karlsruhe - Germany

^[82] Univ Lodz, PL-90131 Lodz - Poland

^[83] Univ Estadual Feira de Santana, Feira De Santana, BA - Brazil

^[84] Palacky Univ, RCPTM, Olomouc - Czech Republic

^[85] Inst Space Sci, Bucharest - Romania

^[86] Louisiana State Univ, Baton Rouge, LA 70803 - USA

^[87] INAF, Palermo - Italy

^[88] Univ New Mexico, Albuquerque, NM 87131 - USA

^[89] Fac Independente Nordeste, Vitoria Da Conquista - Brazil

^[90] Univ Fed ABC, Sante Andre, SP - Brazil

^[91] Benemerita Univ Autonoma Puebla, Puebla - Mexico

^[92] Univ Leeds, Sch Phys & Astron, Leeds LS2 9JT, W Yorkshire - England

^[93] Ctr Brasileiro Pesquisas Fis, Rio De Janeiro, RJ - Brazil

^[94] Colorado Sch Mines, Golden, CO 80401 - USA

^[95] Rudjer Boskovic Inst, Zagreb 10000 - Croatia

^[96] Consejo Nacl Invest Cient & Tecn, IFIR, UNR, Rosario - Argentina

^[97] Horia Hulubei Natl Inst Phys & Nucl Engn, Bucharest - Romania

^[98] Univ Fed Pelotas, Pelotas, RS - Brazil

^[99] Charles Univ Prague, Fac Math & Phys, Inst Particle & Nucl Phys, Prague - Czech Republic

^[100] Consejo Nacl Invest Cient & Tecn, RA-1033 Buenos Aires, DF - Argentina

^[101] CITEDEF, Ctr Invest Laseres & Aplicac, Buenos Aires, DF - Argentina

^[102] Univ Valencia, CSIC, Inst Fis Corpuscular, Valencia - Spain

^[103] Univ Fed Bahia, Salvador, BA - Brazil

^[104] Dipartimento Fis Univ, Genoa - Italy

^[105] INFN, Genoa - Italy

^[106] Univ Nebraska, Lincoln, NE - USA

^[107] Gran Sasso Sci Inst INFN, Laquila - Italy

^[108] Univ Bucharest, Dept Phys, Bucharest - Romania

^[109] Northeastern Univ, Boston, MA 02115 - USA

^[110] Univ Sao Paulo, Escola Engn Lorena, BR-05508 Sao Paulo - Brazil

^[111] Los Alamos Natl Lab, Los Alamos, NM - USA

• Tipo de documento: Artigo Científico
• Fonte: Astrophysical Journal Letters; v. 789, n. 2 JUL 10 2014.
• Citações Web of Science: 10

Resumo

A flux of neutrons from an astrophysical source in the Galaxy can be detected in the Pierre Auger Observatory as an excess of cosmic-ray air showers arriving from the direction of the source. To avoid the statistical penalty for making many trials, classes of objects are tested in combinations as nine ``target sets,{''} in addition to the search for a neutron flux from the Galactic center or from the Galactic plane. Within a target set, each candidate source is weighted in proportion to its electromagnetic flux, its exposure to the Auger Observatory, and its flux attenuation factor due to neutron decay. These searches do not find evidence for a neutron flux from any class of candidate sources. Tabulated results give the combined p-value for each class, with and without the weights, and also the flux upper limit for the most significant candidate source within each class. These limits on fluxes of neutrons significantly constrain models of EeV proton emission from non-transient discrete sources in the Galaxy. (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