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Improved limit to the diffuse flux of ultrahigh energy neutrinos from the Pierre Auger Observatory

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Autor(es):
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Aab, A. [1] ; Abreu, P. [2, 3] ; Aglietta, M. [4] ; Ahn, E. J. [5] ; Al Samarai, I. [6] ; Albuquerque, I. F. M. [7] ; Allekotte, I. [8] ; Allison, P. [9] ; Almela, A. [10, 11] ; Castillo, J. Alvarez [12] ; Alvarez-Muniz, J. [13] ; Batista, R. Alves [14] ; Ambrosio, M. [15] ; Aminaei, A. [16] ; Anchordoqui, L. [17] ; Andringa, S. [2, 3] ; Aramo, C. [15] ; Aranda, V. M. [18] ; Arqueros, F. [18] ; Arsene, N. [19] ; Asorey, H. [8, 20] ; Assis, P. [2, 3] ; Aublin, J. [21] ; Ave, M. [8] ; Avenier, M. [22] ; Avila, G. [23] ; Awal, N. [24] ; Badescu, A. M. [25] ; Barber, K. B. [26] ; Baeuml, J. [27] ; Baus, C. [27] ; Beatty, J. J. [9] ; Becker, K. H. [28] ; Bellido, J. A. [26] ; Berat, C. [22] ; Bertaina, M. E. [4] ; Bertou, X. [8] ; Biermann, P. L. [29] ; Billoir, P. [21] ; Blaess, S. G. [26] ; Blanco, A. [2, 3] ; Blanco, M. [21] ; Bleve, C. [30] ; Bluemer, H. [27, 31] ; Bohacova, M. [32] ; Boncioli, D. [33] ; Bonifazi, C. [34] ; Borodi, N. [35] ; Brack, J. [36] ; Brancus, I. [37] ; Bridgeman, A. [31] ; Brogueira, P. [2, 3] ; Brown, W. C. [38] ; Buchholz, P. [1] ; Bueno, A. [39, 40] ; Buitink, S. [16] ; Buscemi, M. [15] ; Caballero-Mora, K. S. [41] ; Caccianiga, B. [42] ; Caccianiga, L. [21] ; Candusso, M. [43] ; Caramete, L. [44] ; Caruso, R. [45] ; Castellina, A. [4] ; Cataldi, G. [30] ; Cazon, L. [2, 3] ; Cester, R. [46] ; Chavez, A. G. [47] ; Chiavassa, A. [4] ; Chinellato, J. A. [48] ; Chudoba, J. [32] ; Cilmo, M. [15] ; Clay, R. W. [26] ; Cocciolo, G. [30] ; Colalillo, R. [15] ; Coleman, A. [49] ; Collica, L. [42] ; Coluccia, M. R. [30] ; Conceicao, R. [2, 3] ; Contreras, F. [50] ; Cooper, M. J. [26] ; Cordier, A. [51] ; Coutu, S. [49] ; Covault, C. E. [52] ; Cronin, J. [53] ; Dallier, R. [54, 55] ; Daniel, B. [48] ; Dasso, S. [56, 57, 58] ; Daumiller, K. [31] ; Dawson, B. R. [26] ; de Almeida, R. M. [59] ; de Jong, S. J. [16, 60] ; De Mauro, G. [16] ; de Mello Neto, J. R. T. [34] ; De Mitri, I. [30] ; de Oliveira, J. [59] ; de Souza, V. [61] ; del Peral, L. [62] ; Deligny, O. [6] ; Dembinski, H. [31] ; Dhital, N. [63] ; Di Giulio, C. [43] ; Di Matteo, A. [64] ; Diaz, J. C. [63] ; Castro, M. L. Diaz [48] ; Diogo, F. [2, 3] ; Dobrigkeit, C. [48] ; Docters, W. [65] ; D'Olivo, J. C. [12] ; Dorofeev, A. [36] ; Hasankiadeh, Q. Dorosti [31] ; Dova, M. T. [66, 67] ; Ebr, J. [32] ; Enge, R. [31] ; Erdmann, M. [68] ; Erfani, M. [1] ; Escobar, C. O. [48, 5] ; Espadanal, J. [2, 3] ; Etchegoyen, A. [10, 11] ; Falcke, H. [16, 60, 69] ; Fang, K. [53] ; Farrar, G. [24] ; Fauth, A. C. [48] ; Fazzini, N. [5] ; Ferguson, A. P. [52] ; Fernandes, M. [34] ; Fick, B. [63] ; Figueira, J. M. [11] ; Filevich, A. [11] ; Filipcic, A. [70, 71] ; Fox, B. D. [72] ; Fratu, O. [25] ; Freire, M. M. [73, 74] ; Fuchs, B. [27] ; Fujii, T. [53] ; Garcia, B. [75, 76] ; Garcia-Pinto, D. [18] ; Gate, F. [54] ; Gemmeke, H. [31] ; Gherghel-Lascu, A. [37] ; Ghia, P. L. [21] ; Giaccari, U. [34] ; Giammarchi, M. [42] ; Giller, M. [77] ; Glas, D. [77] ; Glaser, C. [68] ; Glass, H. [5] ; Golup, G. [8] ; Berisso, M. Gomez [8] ; Vitale, P. F. Gomez [23] ; Gonzalez, N. [11] ; Gookin, B. [36] ; Gordon, J. [9] ; Gorgi, A. [4] ; Gorham, P. [72] ; Gouffon, P. [7] ; Griffith, N. [9] ; Grillo, A. F. [33] ; Grubb, T. D. [26] ; Guardincerri, Y. [56, 57] ; Guarino, F. [15] ; Guedes, G. P. [78] ; Hampe, M. R. [11] ; Hansen, P. [67, 66] ; Harari, D. [8] ; Harrison, T. A. [26] ; Hartmann, S. [68] ; Harton, J. L. [36] ; Haungs, A. [31] ; Hebbeker, T. [68] ; Heck, D. [31] ; Heimann, P. [1] ; Herve, A. E. [31] ; Hi, G. C. [26] ; Hojvat, C. [5] ; Hollon, N. [53] ; Holt, E. [31] ; Homola, P. [28] ; Horande, J. R. [16, 60] ; Horvath, P. [79] ; Hrabovsky, M. [32, 79] ; Huber, D. [27] ; Huege, T. [31] ; Insolia, A. [45] ; Isar, P. G. [44] ; Jandt, I. [28] ; Jansen, S. [16, 60] ; Jarne, C. [66, 67] ; Johnsen, J. A. [80] ; Josebachuili, M. [11] ; Kaeaepae, A. [28] ; Kambeitz, O. [27] ; Kampert, K. H. [28] ; Kasper, P. [5] ; Katkov, I. [27] ; Kegl, B. [51] ; Keilhauer, B. [31] ; Keivani, A. [49] ; Kemp, E. [48] ; Kieckhafer, R. M. [63] ; Klages, H. O. [31] ; Kleifges, M. [31] ; Kleinfeller, J. [50] ; Krause, R. [68] ; Krohm, N. [28] ; Kroemer, O. [31] ; Kuempel, D. [68] ; Kunka, N. [31] ; LaHurd, D. [52] ; Latronico, L. [4] ; Lauer, R. [81] ; Lauscher, M. [68] ; Lautridou, P. [54] ; Le Coz, S. [22] ; Lebrun, D. [22] ; Lebrun, P. [5] ; de Oliveira, M. A. Leigui [82] ; Letessier-Selvon, A. [21] ; Lhenry-Yvon, I. [6] ; Link, K. [27] ; Lopes, L. [2, 3] ; Lopez, R. [83] ; Casado, A. Lopez [13] ; Louedec, K. [22] ; Lu, L. [28, 84] ; Lucero, A. [11] ; Malacari, M. ; Maldera, S. [4] ; Mallamaci, M. [42] ; Maller, J. [54] ; Mandat, D. [32] ; Mantsch, R. [5] ; Mariazzi, A. G. [67, 66] ; Mann, V. [54] ; Maris, I. C. [39, 40] ; Marsella, G. [30] ; Martello, D. [30] ; Martin, L. [54, 55] ; Martinez, H. [85] ; Bravo, O. Martinez [83] ; Martraire, D. [6] ; Meza, J. J. Masias [56, 57] ; Mathes, H. J. [31] ; Mathys, S. [28] ; Matthews, J. [86] ; Matthews, J. A. J. [81] ; Matthiae, G. [43] ; Maurel, D. [27] ; Maurizio, D. [87] ; Mayotte, E. [80] ; Mazur, P. O. [5] ; Medina, C. [80] ; Medina-Tanco, G. [12] ; Meissner, R. [68] ; Mello, V. B. B. [34] ; Melo, D. [11] ; Menshikov, A. [31] ; Messina, S. [65] ; Meyhandan, R. [72] ; Micheletti, M. I. [73, 74] ; Middendorf, L. [68] ; Minaya, I. A. [18] ; Miramonti, L. [42] ; Mitrica, B. [37] ; Molina-Bueno, L. [39, 40] ; Mollerach, S. [8] ; Montanet, F. [22] ; Morello, C. [4] ; Mostafa, M. [49] ; Moura, C. A. [82] ; Muller, M. A. [48, 88] ; Mueller, G. [68] ; Mueller, S. [31] ; Mussa, R. [46] ; Navarra, G. [4] ; Navarro, J. L. [39, 40] ; Navas, S. [39, 40] ; Necesal, R. [32] ; Nellen, L. [12] ; Nelles, A. [16, 60] ; Neuser, J. [28] ; Nguyen, P. H. [26] ; Niculescu-Oglinzanu, M. [37] ; Niechciol, M. [1] ; Niemietz, L. [28] ; Niggemann, T. [68] ; Nitz, D. [63] ; Nosek, D. [89] ; Novotny, V. [89] ; Nozka, L. [79] ; Ochilo, L. [1] ; Oikonomou, F. [49] ; Olinto, A. [53] ; Pacheco, N. [62] ; Selmi-Dei, D. Pakk [48] ; Palatka, M. [32] ; Pallotta, J. [56, 90] ; Papenbreer, P. [28] ; Parente, G. [13] ; Parra, A. [83] ; Paul, T. [17, 91] ; Pech, M. [32] ; Pekala, J. [35] ; Pelayo, R. [92] ; Pepe, I. M. [93] ; Perrone, L. [30] ; Petermann, E. [94] ; Peters, C. [68] ; Petrera, S. [64, 95] ; Petrov, Y. [36] ; Phuntsok, J. [49] ; Piegaia, R. [56, 57] ; Pierog, T. [31] ; Pieroni, P. [56, 57] ; Pimenta, M. [2, 3] ; Pirronello, V. [45] ; Platino, M. [11] ; Plum, M. [68] ; Porcelli, A. [31] ; Porowski, C. [35] ; Prado, R. R. [61] ; Privitera, P. [53] ; Prouza, M. [32] ; Purrello, V. [8] ; Quel, E. J. [56, 90] ; Querchfeld, S. [28] ; Quinn, S. [52] ; Rautenberg, J. [28] ; Ravel, O. [54] ; Ravignani, D. [11] ; Revenu, B. [54] ; Ridky, J. [32] ; Riggi, S. [45] ; Risse, M. [1] ; Ristori, P. [56, 90] ; Rizi, V. [64] ; de Carvalho, W. Rodrigues [13] ; Fernandez, G. Rodriguez [43] ; Rojo, J. Rodriguez [50] ; Rodriguez-Frias, D. [62] ; Rogozin, D. [31] ; Rosado, J. [18] ; Roth, M. [31] ; Roulet, E. [8] ; Rovero, A. C. [58] ; Saffi, S. J. [26] ; Saftoiu, A. [37] ; Salamida, F. [6] ; Salazar, H. [83] ; Saleh, A. [70] ; Greus, F. Salesa [49] ; Salina, G. [43] ; Sanchez, F. [11] ; Sanchez-Lucas, P. [39, 40] ; Santos, E. [48] ; Santos, E. M. [7] ; Sarazin, F. [80] ; Sarkar, B. [28] ; Sarmento, R. [2, 3] ; Sato, R. [50] ; Scarso, C. [50] ; Schauer, M. [28] ; Scherini, V. [30] ; Schieler, H. [31] ; Schiffer, P. [14] ; Schmidt, D. [31] ; Scholten, O. [65] ; Schoorlemmer, H. [72] ; Schovanek, P. [32] ; Schroeder, F. G. [31] ; Schulz, A. [31] ; Schulz, J. [16] ; Schumacher, J. [68] ; Sciutto, S. J. [67, 66] ; Segreto, A. [96] ; Settimo, M. [21] ; Shadkam, A. [86] ; Shellard, R. C. [87] ; Sidelnik, I. [8] ; Sigl, G. [14] ; Sima, O. [19] ; Smialkowski, A. [77] ; Smida, R. [31] ; Snow, G. R. [94] ; Sommers, P. [49] ; Sorokin, J. [26] ; Sotuartini, R. [50] ; Srivastava, Y. N. [91] ; Stanca, D. [37] ; Stanic, S. [70] ; Stapleton, J. [9] ; Stasielak, J. [35] ; Stephan, M. [68] ; Stutz, A. [22] ; Suarez, F. ; Suomijaervi, T. [6] ; Supanitsky, A. D. [58] ; Sutherland, M. S. [9] ; Swain, J. [91] ; Szadkowski, Z. [77] ; Taborda, O. A. [8] ; Tapia, A. [11] ; Tepe, A. [1] ; Theodoro, V. M. [48] ; Tiffenberg, J. [56, 57] ; Timmermans, C. [16, 60] ; Peixoto, C. J. Todero [97] ; Toma, G. [37] ; Tomankova, L. [31] ; Tome, B. [2, 3] ; Tonachini, A. [46] ; Elipe, G. Torralba [13] ; Machado, D. Torres [34] ; Travnicek, P. [32] ; Ulrich, R. [31] ; Unger, M. [24] ; Urban, M. [68] ; Galicia, J. F. Valdes [12] ; Valino, I. [13] ; Valore, L. [15] ; van Aar, G. [16] ; van Bodegom, P. [26] ; van den Berg, A. M. [65] ; van Velzen, S. [16] ; van Vliet, A. [14] ; Varela, E. [83] ; Cardenas, B. Vargas [12] ; Varner, G. [72] ; Vasquez, R. [34] ; Vazquez, R. [18] ; Vazquez, R. A. [13] ; Veberic, D. [31] ; Verzi, V. [43] ; Vicha, J. [32] ; Videla, M. [11] ; Villasenor, L. [47] ; Vlcek, B. [62] ; Vorobiov, S. [70] ; Wahlberg, H. [66, 67] ; Wainberg, O. [10, 11] ; Walz, D. [68] ; Watson, A. A. [84] ; Weber, M. [31] ; Weidenhaupt, K. [68] ; Weindl, A. [31] ; Werner, F. [27] ; Widom, A. [91] ; Wiencke, L. [80] ; Wilczynski, H. [35] ; Winchen, T. [28] ; Wittkowski, D. [28] ; Wundheiler, B. [11] ; Wykes, S. [16] ; Yang, L. [70] ; Yapici, T. [63] ; Yushkov, A. [1] ; Zas, E. [13] ; Zawtanik, D. [70, 71] ; Zavrtanik, M. [70, 71] ; Zepeda, A. [85] ; Zhu, Y. [31] ; Zimmermann, B. [31] ; Ziolkowski, M. [1] ; Zuccarello, F. [45] ; Collaboration, Pierre Auger
Número total de Autores: 465
Afiliação do(s) autor(es):
Mostrar menos -
[1] Univ Siegen, D-57068 Siegen - Germany
[2] Univ Lisboa UL, Lab Instrumentacao & Expt Particulas LIP, Lisbon - Portugal
[3] Univ Lisboa UL, IST, Lisbon - Portugal
[4] Univ Turin, Osservatorio Astrofis Torino INAF, Turin - Italy
[5] Fermilab Natl Accelerator Lab, Batavia, IL - USA
[6] Univ Paris 11, CNRS IN2P3, IPNO, Orsay - France
[7] Univ Sao Paulo, Inst Fis, BR-01498 Sao Paulo, SP - Brazil
[8] CNEA UNCuyo CONICET, Ctr Atom Bariloche & Inst Balseiro, San Carlos De Bariloche, Rio Negro - Argentina
[9] Ohio State Univ, Columbus, OH 43210 - USA
[10] Univ Tecnol Nacl, Fac Reg Buenos Aires, Buenos Aires, DF - Argentina
[11] UNSAM, CONICET, Inst Tecnol Detecc & Astroparticulas, Buenos Aires, DF - Argentina
[12] Univ Nacl Autonoma Mexico, Mexico City 04510, DF - Mexico
[13] Univ Santiago Compostela, Santiago De Compostela - Spain
[14] Univ Hamburg, Hamburg - Germany
[15] Univ Naples Federico II, Sez INFN, Naples - Italy
[16] Radboud Univ Nijmegen, IMAPP, NL-6525 ED Nijmegen - Netherlands
[17] CUNY, Lehman Coll, Dept Phys & Astron, New York, NY 10021 - USA
[18] Univ Complutense Madrid, Madrid - Spain
[19] Univ Bucharest, Dept Phys, Bucharest - Romania
[20] Univ Ind Santander, Santander - Spain
[21] Univ Paris 6 & Paris 7, CNRS IN2P3, LPNHE, Paris - France
[22] Univ Grenoble Alpes, CNRS IN2P3, LPSC, Grenoble - France
[23] Observ Pierre Auger & Comis Nacl Energia Atom, Malargue - Argentina
[24] NYU, New York, NY - USA
[25] Univ Politehn Bucuresti, Bucharest - Romania
[26] Univ Adelaide, Adelaide, SA - Australia
[27] Karlsruhe Inst Technol, Campus South Inst Expet Kemphys IEKP, D-76021 Karlsruhe - Germany
[28] Berg Univ Wuppertal, Wuppertal - Germany
[29] Max Planck Ins Radioastron, Bonn - Germany
[30] E De Giorgi Univ Salento, Dipartimento Matemat & Fis, Sez INFN, Lecce - Italy
[31] Karlsruhe Inst Technol, D-76021 Karlsruhe - Germany
[32] Acad Sci Czech Republic, Inst Phys, Prague - Czech Republic
[33] INFN, Lab Nazl Gran Sasso, Assergi LAquila - Italy
[34] Univ Fed Rio de Janeiro, Inst Fis, Rio De Janeiro, RJ - Brazil
[35] Inst Nucl Phys, PAN, Krakow - Poland
[36] Colorado State Univ, Ft Collins, CO 80523 - USA
[37] Horia Hulubei Natl Inst Phys & Nucl Engn, Bucharest 077125 - Romania
[38] Colorado State Univ, Pueblo, CO - USA
[39] Univ Granada, Granada - Spain
[40] CAFPE, Granada - Spain
[41] Univ Autonoma Chiapas, Tuxtla Gutierrez, Chiapas - Mexico
[42] Univ Milan, Sez INFN, Milan - Italy
[43] Univ Roma Tor Vergata, Sez INFN, I-00173 Rome - Italy
[44] Inst Space Sci, Bucharest - Romania
[45] Univ Catania, Sez INFN, Catania - Italy
[46] Univ Turin, Sez INFN, Turin - Italy
[47] Univ Michoacana, Morelia, Michoacan - Mexico
[48] Univ Estadual Campinas, IFGW, Campinas, SP - Brazil
[49] Penn State Univ, University Pk, PA 16802 - USA
[50] Observ Pierre Auger, Malargue - Argentina
[51] Univ Paris 11, CNRS IN2P3, LAL, Orsay - France
[52] Case Western Reserve Univ, Cleveland, OH 44106 - USA
[53] Univ Chicago, Enrico Fermi Inst, Chicago, IL 60637 - USA
[54] Univ Nantes, CNRS IN2P3, Ecole Mines Nantes, SUBATECH, Nantes - France
[55] CNRS INSU, Observ Paris, Stn Radioastron Nancay, Nancay - France
[56] Consejo Nacl Invest Cient & Tecn, RA-1033 Buenos Aires, DF - Argentina
[57] Univ Buenos Aires, Dept Fis, FCEyN, RA-1053 Buenos Aires, DF - Argentina
[58] CONICET UBA, IAFE, Buenos Aires, DF - Argentina
[59] Univ Fed Fluminense, EEIMVR, Volta Redonda, RJ - Brazil
[60] Nikhef, Amsterdam - Netherlands
[61] Univ Sao Paulo, Inst Fis, Sao Carlos, SP - Brazil
[62] Univ Alcala De Henares, Alcala De Henares - Spain
[63] Michigan Technol Univ, Houghton, MI 49931 - USA
[64] Univ Aquila, Dipartimento Sci Fis & Chim, INFN, I-67100 Laquila - Italy
[65] Univ Groningen, KVI Ctr Adv Radiat Technol, Groningen - Netherlands
[66] Consejo Nacl Invest Cient & Tecn, La Plata, Buenos Aires - Argentina
[67] Univ Nacl La Plata, IFLP, RA-1900 La Plata, Buenos Aires - Argentina
[68] Rhein Westfal TH Aachen, Phys Inst A 3, Aachen - Germany
[69] ASTRON, Dwingeloo - Netherlands
[70] Univ Nova Gor, Lab Astroparticle Phys, Nova Gorica - Slovenia
[71] J Stefan Inst, Expt Particle Phys Dept, Ljubljana - Slovenia
[72] Univ Hawaii, Honolulu, HI 96822 - USA
[73] UNR, IFIR CONICET, Rosario, Santa Fe - Argentina
[74] UNR, Fac Ciencias Bioquim & Fannaceut, Rosario, Santa Fe - Argentina
[75] UNSAM, CONICET, CNEA, Inst Tecnol Detecc & Astroparticulas, Mendoza - Argentina
[76] Univ Tecnol Nacl, Fac Reg Mendoza, CONICET CNEA, Mendoza - Argentina
[77] Univ Lodz, PL-90131 Lodz - Poland
[78] Univ Estadual Feira de Santana, Feira De Santana, BA - Brazil
[79] Palacky Univ, RCPTM, CR-77147 Olomouc - Czech Republic
[80] Colorado Sch Mines, Golden, CO 80401 - USA
[81] Univ New Mexico, Albuquerque, NM 87131 - USA
[82] Univ Fed ABC, Santo Andre, SP - Brazil
[83] Benemerita Univ Autonoma Puebla, Puebla - Mexico
[84] Univ Leeds, Sch Phys & Astron, Leeds LS2 9JT, W Yorkshire - England
[85] CINVESTAV, IPN, Mexico City 14000, DF - Mexico
[86] Louisiana State Univ, Baton Rouge, LA 70803 - USA
[87] Ctr Brasileiro Pesquisas Fis, Rio De Janeiro, RJ - Brazil
[88] Univ Fed Pelotas, Pelotas, RS - Brazil
[89] Charles Univ Prague, Fac Math & Phys, Inst Particle & Nucl Phys, Prague - Czech Republic
[90] CITEDEF, Ctr Invest Laseres & Aplicaciones, Buenos Aires, DF - Argentina
[91] Northeastern Univ, Boston, MA 02115 - USA
[92] UPIITA IPN, Mexico City, DF - Mexico
[93] Univ Fed Bahia, Salvador, BA - Brazil
[94] Univ Nebraska, Lincoln, NE - USA
[95] Gran Sasso Sci Inst, INFN, Laquila - Italy
[96] Ist Astrofis Spaziale & Fis Cosm Palermo INAF, Palermo - Italy
[97] Univ Sao Paulo, Escola Engn Lorena, Lorena, SP - Brazil
Número total de Afiliações: 97
Tipo de documento: Artigo Científico
Fonte: Physical Review D; v. 91, n. 9 MAY 26 2015.
Citações Web of Science: 80
Resumo

Neutrinos in the cosmic ray flux with energies near 1 EeV and above are detectable with the Surface Detector array (SD) of the Pierre Auger Observatory. We report here on searches through Auger data from 1 January 2004 until 20 June 2013. No neutrino candidates were found, yielding a limit to the diffuse flux of ultrahigh energy neutrinos that challenges the Waxman-Bahcall bound predictions. Neutrino identification is attempted using the broad time structure of the signals expected in the SD stations, and is efficiently done for neutrinos of all flavors interacting in the atmosphere at large zenith angles, as well as for ``Earth-skimming{''} neutrino interactions in the case of tau neutrinos. In this paper the searches for downward-going neutrinos in the zenith angle bins 60 degrees-75 degrees and 75 degrees-90 degrees as well as for upward-going neutrinos, are combined to give a single limit. The 90% C.L. single-flavor limit to the diffuse flux of ultrahigh energy neutrinos with an E-2 spectrum in the energy range 1.0 x 10(17) eV-2.5 x 10(19) eV is E(nu)(2)dN(nu)/dE(nu) < 6.4 x 10(-9) GeV cm(-2) s(-1) sr(-1). (AU)

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