Multi-Messenger Physics With the Pierre Auger Observatory

Autor(es):Mostrar menos -

Kampert, Karl-Heinz ^[1] ; Mostafa, Miguel Alejandro ^[2] ; Zas, Enrique ^[3] ; Aab, A. ^[4] ; Abreu, P. ^{[5, 6]} ; Aglietta, M. ^{[7, 8]} ; Albuquerque, I. F. M. ^[9] ; Albury, J. M. ^[10] ; Allekotte, I ^{[11, 12]} ; Almela, A. ^{[13, 14]} ; Alvarez Castillo, J. ^[15] ; Alvarez-Muniz, J. ^[16] ; Anastasi, G. A. ^{[17, 18]} ; Anchordoqui, L. ^[19] ; Andrada, B. ^[13] ; Andringa, S. ^{[5, 6]} ; Aramo, C. ^[20] ; Asorey, H. ^{[11, 12, 21]} ; Assis, P. ^{[5, 6]} ; Avila, G. ^{[22, 23]} ; Badescu, A. M. ^[24] ; Bakalova, A. ^[25] ; Balaceanu, A. ^[26] ; Barbato, F. ^{[20, 27]} ; Barreira Luz, R. J. ^{[5, 6]} ; Baur, S. ^[28] ; Becker, K. H. ^[29] ; Bellido, J. A. ^[10] ; Berat, C. ^[30] ; Bertaina, M. E. ^{[7, 31]} ; Bertou, X. ^{[11, 12]} ; Biermannb, P. L. ^[32] ; Biteau, J. ^[33] ; Blaess, S. G. ^[10] ; Blanco, A. ^{[5, 6]} ; Blazek, J. ^[25] ; Bleve, C. ^{[34, 35]} ; Bohacova, M. ^[25] ; Boncioli, D. ^{[17, 18]} ; Bonifazi, C. ^[36] ; Borodai, N. ^[37] ; Botti, A. M. ^{[13, 28]} ; Bracke, J. ^[38] ; Bretz, T. ^[39] ; Bridgeman, A. ^[40] ; Briechle, F. L. ^[39] ; Buchholz, P. ^[41] ; Bueno, A. ^{[42, 43]} ; Buitink, S. ^[44] ; Buscemi, M. ^{[45, 46]} ; Caballero-Mora, K. S. ^[47] ; Caccianiga, L. ^[48] ; Calcagni, L. ^{[49, 50]} ; Cancio, A. ^{[13, 14]} ; Canfora, F. ^{[4, 51]} ; Carceller, J. M. ^{[42, 43]} ; Caruso, R. ^{[45, 46]} ; Castellina, A. ^{[7, 8]} ; Catalani, F. ^[52] ; Cataldi, G. ^[35] ; Cazon, L. ^{[5, 6]} ; Cerda, M. ^[23] ; Chinellato, J. A. ^[53] ; Chudoba, J. ^[25] ; Chytka, L. ^[54] ; Clay, R. W. ^[10] ; Cobos Cerutti, A. C. ^{[55, 56]} ; Colalillo, R. ^{[20, 27]} ; Coleman, A. ^[57] ; Coluccia, M. R. ^{[34, 35]} ; Conceicao, R. ^{[5, 6]} ; Condorelli, A. ^{[17, 18]} ; Consolati, G. ^{[58, 59]} ; Contreras, F. ^{[22, 23]} ; Convenga, F. ^{[34, 35]} ; Cooper, M. J. ^[10] ; Coutu, S. ^[57] ; Covault, C. E. ^[60] ; Daniel, B. ^[53] ; Dasso, S. ^{[61, 62, 63, 64]} ; Daumiller, K. ^[28] ; Dawson, B. R. ^[10] ; Day, J. A. ^[10] ; de Almeida, R. M. ^[65] ; de Jong, S. J. ^{[4, 51]} ; De Mauro, G. ^{[4, 51]} ; de Mello Neto, J. R. T. ^{[36, 66]} ; De Mitri, I ^{[17, 18]} ; de Oliveira, J. ^[65] ; de Oliveira Salles, F. O. ^[67] ; de Souza, V ^[68] ; Debatin, J. ^[40] ; del Rio, M. ^{[22, 23]} ; Deligny, O. ^[33] ; Dhital, N. ^[37] ; Castro, M. L. Diaz ^[53] ; Diogo, F. ^{[5, 6]} ; Dobrigkeit, C. ^[53] ; D'Olivo, J. C. ^[15] ; Dorosti, Q. ^[41] ; dos Anjos, R. C. ^[69] ; Dova, M. T. ^{[49, 50]} ; Dundovic, A. ^[70] ; Ebr, J. ^[25] ; Engel, R. ^{[28, 40]} ; Erdmann, M. ^[39] ; Escobarc, C. O. ^[71] ; Etchegoyen, A. ^{[13, 14]} ; Falcke, H. ^{[4, 51, 72]} ; Farmer, J. ^[73] ; Farrar, G. ^[74] ; Fauth, A. C. ^[53] ; Fazzinic, N. ^[71] ; Feldbusch, F. ^[75] ; Fenu, F. ^{[7, 31]} ; Ferreyro, L. P. ^[13] ; Figueira, J. M. ^[13] ; Filipcic, A. ^{[76, 77]} ; Freire, M. M. ^{[78, 79]} ; Fujii, T. ^{[73, 80, 81]} ; Fuster, A. ^{[13, 14]} ; Garcia, B. ^{[55, 56]} ; Gemmeke, H. ^[75] ; Gherghel-Lascu, A. ^[26] ; Ghia, P. L. ^[33] ; Giaccari, U. ^[67] ; Giammarchi, M. ^[58] ; Giller, M. ^[82] ; Glas, D. ^[83] ; Glombitza, J. ^[39] ; Gobbi, F. ^[23] ; Golup, G. ^{[11, 12]} ; Gomez Berisso, M. ^{[11, 12]} ; Gomez Vitale, P. F. ^{[22, 23]} ; Gongora, J. P. ^[23] ; Gonzalez, N. ^[13] ; Goos, I ^{[28, 11, 12]} ; Gora, D. ^[37] ; Gorgi, A. ^{[7, 8]} ; Gottowik, M. ^[29] ; Grubb, T. D. ^[10] ; Guarino, F. ^{[20, 27]} ; Guedes, G. P. ^[84] ; Guido, E. ^{[7, 31]} ; Halliday, R. ^[60] ; Hampel, M. R. ^[13] ; Hansen, P. ^{[49, 50]} ; Harari, D. ^{[11, 12]} ; Harrison, T. A. ^[10] ; Harvey, V. M. ^[10] ; Haungs, A. ^[28] ; Hebbeker, T. ^[39] ; Heck, D. ^[28] ; Heimann, P. ^[41] ; Hill, G. C. ^[10] ; Hojvatc, C. ^[71] ; Holt, E. M. ^{[13, 40]} ; Homola, P. ^[37] ; Horandel, J. R. ^{[4, 51]} ; Horvath, P. ^[54] ; Hrabovsky, M. ^[54] ; Huege, T. ^{[28, 44]} ; Hulsman, J. ^{[13, 28]} ; Insolia, A. ^{[45, 46]} ; Isar, P. G. ^[85] ; Jandt, I ^[29] ; Johnsen, J. A. ^[86] ; Josebachuili, M. ^[13] ; Jurysek, J. ^[25] ; Kaeaepae, A. ^[29] ; Kampert, K. H. ^[29] ; Keilhauer, B. ^[28] ; Kemmerich, N. ^[9] ; Kemp, J. ^[39] ; Klages, H. O. ^[28] ; Kleifges, M. ^[75] ; Kleinfeller, J. ^[23] ; Krause, R. ^[39] ; Kuempel, D. ^[29] ; Mezek, G. Kukec ^[77] ; Awad, A. Kuotb ^[40] ; Lago, B. L. ^[87] ; LaHurd, D. ^[60] ; Lang, R. G. ^[68] ; Legumina, R. ^[82] ; Leigui de Oliveira, M. A. ^[88] ; Lenok, V ^[28] ; Letessier-Selvon, A. ^{[89, 90]} ; Lhenry-Yvon, I ^[33] ; Lippmann, O. C. ^[67] ; Lo Presti, D. ^{[45, 46]} ; Lopez, L. ^{[5, 6]} ; Lopez, R. ^[91] ; Lopez Casado, A. ^[16] ; Lorek, R. ^[60] ; Luce, Q. ^[33] ; Lucero, A. ^[13] ; Malacari, M. ^[73] ; Mancarella, G. ^{[34, 35]} ; Mandat, D. ^[25] ; Manning, B. C. ^[10] ; Mantschc, P. ^[71] ; Mariazzi, A. G. ^{[49, 50]} ; Maris, I. C. ^[92] ; Marsella, G. ^{[34, 35]} ; Martello, D. ^{[34, 35]} ; Martinez, H. ^[93] ; Martinez Bravo, O. ^[91] ; Mastrodicasa, M. ^{[17, 94]} ; Mathes, H. J. ^[28] ; Mathys, S. ^[29] ; Matthews, J. ^[95] ; Matthiae, G. ^{[96, 97]} ; Mayotte, E. ^[29] ; Mazurc, P. O. ^[71] ; Medina-Tanco, G. ^[15] ; Melo, D. ^[13] ; Menshikov, A. ^[75] ; Merenda, K-D ^[86] ; Michal, S. ^[54] ; Micheletti, I, M. ; Middendorf, L. ^[39] ; Miramonti, L. ^{[48, 58]} ; Mitrica, B. ^[26] ; Mockler, D. ^[40] ; Mollerach, S. ^{[11, 12]} ; Montanet, F. ^[30] ; Morello, C. ^{[7, 8]} ; Morlino, G. ^{[17, 18]} ; Mostafa, M. ^[57] ; Mueller, A. L. ^{[13, 28]} ; Muller, M. A. ^{[53, 98]} ; Mueller, S. ^{[13, 40]} ; Mussa, R. ^[7] ; Nellen, L. ^[15] ; Nguyen, P. H. ^[10] ; Niculescu-Oglinzanu, M. ^[26] ; Niechciol, M. ^[41] ; Nitz, D. ^{[99, 100]} ; Nosek, D. ^[101] ; Novotny, V ^[101] ; Nozka, L. ^[54] ; Nucita, A. ^{[34, 35]} ; Nunez, L. A. ^[21] ; Oikonomou, F. ^{[57, 102]} ; Olinto, A. ^[73] ; Palatka, M. ^[25] ; Pallotta, J. ^{[103, 104]} ; Panetta, M. P. ^{[34, 35]} ; Papenbreer, P. ^[29] ; Parente, G. ^[16] ; Parra, A. ^[91] ; Pech, M. ^[25] ; Pedreira, F. ^[16] ; Pekala, J. ^[37] ; Pelayo, R. ^[105] ; Pena-Rodriguez, J. ^[21] ; Pereira, L. A. S. ^[53] ; Perlin, M. ^[13] ; Perrone, L. ^{[34, 35]} ; Peters, C. ^[39] ; Petrera, S. ^{[17, 18]} ; Phuntsok, J. ^[57] ; Pierog, T. ^[28] ; Pimenta, M. ^{[5, 6]} ; Pirronello, V ^{[45, 46]} ; Platino, M. ^[13] ; Poh, J. ^[73] ; Pont, B. ^[4] ; Porowski, C. ^[37] ; Prado, R. R. ^[68] ; Privitera, P. ^[73] ; Prouza, M. ^[25] ; Puyleart, A. ^[99] ; Querchfeld, S. ^[29] ; Quinn, S. ^[60] ; Ramos-Pollan, R. ^[21] ; Rautenberg, J. ^[29] ; Ravignani, D. ^[13] ; Reininghaus, M. ^[28] ; Ridky, J. ^[25] ; Riehn, F. ^{[5, 6]} ; Risse, M. ^[41] ; Ristori, P. ^{[103, 104]} ; Rizi, V ^{[17, 94]} ; Rodrigues de Carvalho, W. ^[9] ; Rodriguez Rojo, J. ^[23] ; Roncoroni, M. J. ^[13] ; Roth, M. ^[28] ; Roulet, E. ^{[11, 12]} ; Rovero, A. C. ^[63] ; Ruehl, P. ^[41] ; Saffi, S. J. ^[10] ; Saftoiu, A. ^[26] ; Salamida, F. ^{[17, 94]} ; Salazar, H. ^[91] ; Salina, G. ^[96] ; Sanabria Gomez, J. D. ^[21] ; Sanchez, F. ^[13] ; Santos, E. M. ^[9] ; Santos, E. ^[25] ; Sarazin, F. ^[86] ; Sarmento, R. ^{[5, 6]} ; Sarmiento-Cano, C. ^[13] ; Sato, R. ^[23] ; Savina, P. ^{[34, 35]} ; Schauer, M. ^[29] ; Scherini, V ^[35] ; Schieler, H. ^[28] ; Schimassek, M. ^[40] ; Schimp, M. ^[29] ; Schlueter, F. ^[28] ; Schmidt, D. ^[40] ; Scholten, O. ^{[106, 44]} ; Schovanek, P. ^[25] ; Schroeder, F. G. ^{[28, 107]} ; Schroeder, S. ^[29] ; Schumacher, J. ^[39] ; Sciutto, S. J. ^{[49, 50]} ; Scornavacche, M. ^[13] ; Shellard, R. C. ^[67] ; Sigl, G. ^[70] ; Silli, G. ^{[13, 28]} ; Sima, O. ^{[26, 108]} ; Smida, R. ^[73] ; Snow, G. R. ^[109] ; Sommers, P. ^[57] ; Soriano, J. F. ^[19] ; Souchard, J. ^[30] ; Squartini, R. ^[23] ; Stanca, D. ^[26] ; Stanic, S. ^[77] ; Stasielak, J. ^[37] ; Stassi, P. ^[30] ; Stolpovskiy, M. ^[30] ; Streich, A. ^[40] ; Suarez, F. ^{[13, 14]} ; Suarez-Duran, M. ^[21] ; Sudholz, T. ^[10] ; Suomijarvi, T. ^[33] ; Supanitsky, A. D. ^[13] ; Supik, J. ^[54] ; Szadkowski, Z. ^[83] ; Taboada, A. ^[28] ; Taborda, O. A. ^{[11, 12]} ; Tapia, A. ^[110] ; Timmermans, C. ^{[4, 51]} ; Todero Peixoto, C. J. ^[52] ; Tome, B. ^{[5, 6]} ; Torralba Elipe, G. ^[16] ; Travaini, A. ^[23] ; Travnicek, P. ^[25] ; Trini, M. ^[77] ; Tueros, M. ^{[49, 50]} ; Ulrich, R. ^[28] ; Unger, M. ^[28] ; Urban, M. ^[39] ; Valdes Galicia, J. F. ^[15] ; Valino, I ^{[17, 18]} ; Valore, L. ^{[20, 27]} ; van Bodegom, P. ^[10] ; van den Berg, A. M. ^[106] ; van Vliet, A. ^[4] ; Varela, E. ^[91] ; Cardenas, B. Vargas ^[15] ; Veberic, D. ^[28] ; Ventura, C. ^[66] ; Vergara Quispe, I. D. ^{[49, 50]} ; Verzi, V. ^[96] ; Vicha, J. ^[25] ; Villasenor, L. ^[91] ; Vink, J. ^[111] ; Vorobiov, S. ^[77] ; Wahlberg, H. ^{[49, 50]} ; Watsona, A. A. ^[112] ; Weber, M. ^[75] ; Weindl, A. ^[28] ; Wiedenski, M. ^[83] ; Wiencke, L. ^[86] ; Wilczynski, H. ^[37] ; Winchen, T. ^[44] ; Wirtz, M. ^[39] ; Wittkowski, D. ^[29] ; Wundheiler, B. ^[13] ; Yang, L. ^[77] ; Yushkov, A. ^[25] ; Zas, E. ^[16] ; Zavrtanik, D. ^{[76, 77]} ; Zavrtanik, M. ^{[76, 77]} ; Zehrer, L. ^[77] ; Zepeda, A. ^[93] ; Zimmermann, B. ^[28] ; Ziolkowski, M. ^[41] ; Zong, Z. ^[33] ; Zuccarello, F. ^{[45, 46]} ; Collaboration, Pierre Auger

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

^[1] Univ Wuppertal, Wuppertal - Germany

^[2] Penn State Univ, State Coll, PA - USA

^[3] Univ Santiago de Compostela, Santiago De Compostela - Spain

^[4] Radboud Univ Nijmegen, IMAPP, Nijmegen - Netherlands

^[5] Univ Lisbon, Lab Instrumentacao & Fis Expt Particulas LIP, Lisbon - Portugal

^[6] Univ Lisbon, IST, Lisbon - Portugal

^[7] Ist Nazl Fis Nucl, Sez Torino, Turin - Italy

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

^[9] Univ Sao Paulo, Inst Fis, Sao Paulo, SP - Brazil

^[10] Univ Adelaide, Adelaide, SA - Australia

^[11] Ctr Atom Bariloche, San Carlos De Bariloche, Rio Negro - Argentina

^[12] Inst Balseiro CNEA UNCuyo CONICET, San Carlos De Bariloche, Rio Negro - Argentina

^[13] UNSAM, CONICET, CNEA, Inst Tecnol Detecc & Astroparticulas, Buenos Aires, DF - Argentina

^[14] Univ Tecnol Nacl, Fac Reg Buenos Aires, Buenos Aires, DF - Argentina

^[15] Univ Nacl Autonoma Mexico, Mexico City, DF - Mexico

^[16] Univ Santiago de Compostela, IGFAE, Santiago De Compostela - Spain

^[17] Ist Nazl Fis Nucl, Lab Nazl Gran Sasso, Laquila - Italy

^[18] Gran Sasso Sci Inst, Laquila - Italy

^[19] CUNY, Lehman Coll, Dept Phys & Astron, Bronx, NY - USA

^[20] Ist Nazl Fis Nucl, Sez Napoli, Naples - Italy

^[21] Univ Ind Santander, Bucaramanga - Colombia

^[22] Comis Nacl Energia Atom, Malargue - Argentina

^[23] Malargue - Argentina

^[24] Univ Politehn Bucuresti, Bucharest - Romania

^[25] Czech Acad Sci, Inst Phys, Prague - Czech Republic

^[26] Horia Hulubei Natl Inst Phys & Nucl Engn, Bucharest - Romania

^[27] Univ Napoli Federico II, Dipartimento Fis Ettore Pancini, Naples - Italy

^[28] Karlsruhe Inst Technol, Inst Kernphys, Karlsruhe - Germany

^[29] Berg Univ Wuppertal, Dept Phys, Wuppertal - Germany

^[30] Univ Grenoble Alpes, Grenoble Inst Engn, CNRS, LPSC, IN2P3, F-38000 Grenoble - France

^[31] Univ Torino, Dipartimento Fis, Turin - Italy

^[32] Max Planck Inst Radioastron, Bonn - Germany

^[33] Univ Paris Saclay, Univ Paris Sud, IPNO, CNRS, IN2P3, Orsay - France

^[34] Univ Salento, Dipartimento Matemat & Fis E De Giorgi, Lecce - Italy

^[35] Ist Nazl Fis Nucl, Sez Lecce, Lecce - Italy

^[36] Univ Fed Rio de Janeiro, Inst Fis, Rio De Janeiro, RJ - Brazil

^[37] Inst Nucl Phys PAN, Krakow - Poland

^[38] Colorado State Univ, Ft Collins, CO 80523 - USA

^[39] Rhein Westfal TH Aachen, Phys Inst A 3, Aachen - Germany

^[40] Karlsruhe Inst Technol, Inst Expt Particle Phys ETP, Karlsruhe - Germany

^[41] Univ Siegen, Fachbereich Phys Expt Teilchenphys 7, Siegen - Germany

^[42] Univ Granada, Granada - Spain

^[43] CAFPE, Granada - Spain

^[44] Vrije Univ Brussels, Brussels - Belgium

^[45] Ist Nazl Fis Nucl, Sez Catania, Catania - Italy

^[46] Univ Catania, Dipartimento Fis & Astron, Catania - Italy

^[47] Univ Autonoma Chiapas, Tuxtla Gutierrez, Chiapas - Mexico

^[48] Univ Milan, Dipartimento Fis, Milan - Italy

^[49] Consejo Nacl Invest Cient & Tecn, La Plata, Buenos Aires - Argentina

^[50] Univ Nacl La Plata, IFLP, La Plata, Buenos Aires - Argentina

^[51] Nikhef, Sci Pk, Amsterdam - Netherlands

^[52] Univ Sao Paulo, Escola Engn Lorena, Lorena, SP - Brazil

^[53] Univ Estadual Campinas, IFGW, Campinas, SP - Brazil

^[54] Palacky Univ, RCPTM, Olomouc - Czech Republic

^[55] Univ Tecnol Nacl, Fac Reg Mendoza, CONICET, CNEA, Mendoza - Argentina

^[56] UNSAM, CONICET, CNEA, Inst Tecnol Detect & Astroparticulas, Mendoza - Argentina

^[57] Penn State Univ, University Pk, PA 16802 - USA

^[58] Ist Nazl Fis Nucl, Sez Milano, Milan - Italy

^[59] Politecn Milan, Dipartimento Sci & Tecnol Aerosp, Milan - Italy

^[60] Case Western Reserve Univ, Cleveland, OH 44106 - USA

^[61] Univ Buenos Aires, Dept Fis, FCEyN, Buenos Aires, DF - Argentina

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

^[63] UBA, CONICET, IAFE, Buenos Aires, DF - Argentina

^[64] Univ Buenos Aires, Dept Ciencias Atmosfera & Oceanos, FCEyN, Buenos Aires, DF - Argentina

^[65] Univ Fed Fluminense, EEIMVR, Volta Redonda, RJ - Brazil

^[66] Univ Fed Rio de Janeiro, Observ Valongo, Rio de Janeiro, RJ - Brazil

^[67] Ctr Brasileiro Pesquisas Fis, Rio De Janeiro, RJ - Brazil

^[68] Univ Sao Paulo, Inst Fis Sao Carlos, Sao Carlos, SP - Brazil

^[69] Univ Fed Parana, Setor Palotina, Palotina - Brazil

^[70] Univ Hamburg, Inst Theoret Phys 2, Hamburg - Germany

^[71] Fermilab Natl Accelerator Lab, Batavia, IL 60510 - USA

^[72] Stichting Astron Onderzoek Nederland ASTRON, Dwingeloo - Netherlands

^[73] Univ Chicago, Enrico Fermi Inst, 5640 S Ellis Ave, Chicago, IL 60637 - USA

^[74] NYU, New York, NY - USA

^[75] Karlsruhe Inst Technol, Inst Prozessdatenverarbeitung & Elekt, Karlsruhe - Germany

^[76] J Stefan Inst, Expt Particle Phys Dept, Ljubljana - Slovenia

^[77] Univ Nova Gorica, CAC, Nova Gorica - Slovenia

^[78] I, UNR, Fac Ciencias Bioquim & Farmaceut, Rosario, Santa Fe - Argentina

^[79] I, UNR, CONICET, Inst Fis Rosario IFIR, Rosario, Santa Fe - Argentina

^[80] Kyoto Univ, Hakubi Ctr Adv Res, Kyoto - Japan

^[81] Kyoto Univ, Grad Sch Sci, Kyoto - Japan

^[82] Univ Lodz, Fac Astrophys, Lodz - Poland

^[83] Univ Lodz, Fac High Energy Astrophys, Lodz - Poland

^[84] Univ Estadual Feira de Santana, Feira De Santana - Brazil

^[85] Inst Space Sci, Bucharest - Romania

^[86] Colorado Sch Mines, Golden, CO 80401 - USA

^[87] Ctr Fed Educ Tecnol Celso Suckow da Fonseca, Nova Friburgo - Brazil

^[88] Univ Fed ABC, Santo Andre, SP - Brazil

^[89] Univ Paris 06, LPNHE, CNRS, IN2P3, Paris - France

^[90] Univ Paris 07, LPNHE, CNRS, IN2P3, Paris - France

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

^[92] Univ Libre Bruxelles, Brussels - Belgium

^[93] IPN, CINVESTAV, Ctr Invest & Estudios Avanzados, Mexico City, DF - Mexico

^[94] Univ Aquila, Dipartimento Sci Fis & Chim, Laquila - Italy

^[95] Louisiana State Univ, Baton Rouge, LA 70803 - USA

^[96] Ist Nazl Fis Nucl, Sez Roma Tor Vergata, Rome - Italy

^[97] Univ Roma Tor Vergata, Dipartimento Fis, Rome - Italy

^[98] Univ Fed Alfenas, Pocos De Caldas - Brazil

^[99] Michigan Technol Univ, Houghton, MI 49931 - USA

^[100] Karlsruhe Inst Technol, Karlsruhe - Germany

^[101] Charles Univ Prague, Fac Math & Phys, Inst Particle & Nucl Phys, Prague - Czech Republic

^[102] European Southern Observ, Garching - Germany

^[103] Consejo Nacl Invest Cient & Tecn, Villa Martelli - Argentina

^[104] CITEDEF, Ctr Invest Laseres & Aplicac, Villa Martelli - Argentina

^[105] IPN, UPIITA, Mexico City, DF - Mexico

^[106] Univ Groningen, KVI Ctr Adv Radiat Technol, Groningen - Netherlands

^[107] Univ Delaware, Bartol Res Inst, Dept Phys & Astron, Newark, DE 19716 - USA

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

^[109] Univ Nebraska, Lincoln, NE - USA

^[110] Univ Medellin, Medellin - Colombia

^[111] Univ Amsterdam, Fac Sci, Amsterdam - Netherlands

^[112] Univ Leeds, Sch Phys & Astron, Leeds, W Yorkshire - England

• Tipo de documento: Artigo de Revisão
• Fonte: FRONTIERS IN ASTRONOMY AND SPACE SCIENCES; v. 6, APR 24 2019.
• Citações Web of Science: 1

Resumo

An overview of the multi-messenger capabilities of the Pierre Auger Observatory is presented. The techniques and performance of searching for Ultra-High Energy neutrinos, photons and neutrons are described. Some of the most relevant results are reviewed, such as stringent upper bounds that were placed to a flux of diffuse cosmogenic neutrinos and photons, bounds placed on neutrinos emitted from compact binary mergers that were detected by LIGO and Virgo during their first and second observing runs, as well as searches for high energy photons and neutrons from the Galactic center that constrain the properties of the putative Galactic PeVatron, observed by the H.E.S.S. collaboration. The observation of directional correlations between ultra-high energy cosmic rays and either high energy astrophysical neutrinos or specific source populations, weighted by their electromagnetic radiation, are also discussed. They constitute additional multi-messenger approaches aimed at identifying the sources of high energy cosmic rays. (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