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Calibration of the logarithmic-periodic dipole antenna (LPDA) radio stations at the Pierre Auger Observatory using an octocopter

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Autor(es):
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Aab, A. [1, 2] ; Abreu, P. [3, 4] ; Aglietta, M. [5, 6] ; Al Samarai, I. [7] ; Albuquerque, I. F. M. [8] ; Allekotte, I. [9, 10] ; Almela, A. [11, 12] ; Castillo, J. Alvarez [13] ; Alvarez-Muiniz, J. [13] ; Anastasi, G. A. [14] ; Anchordoqui, L. [15] ; Andrada, B. [11] ; Andringa, S. [3, 4] ; Aramo, C. [16] ; Arqueros, F. [17] ; Arsene, N. [18] ; Asorey, H. [19, 9, 10] ; Assis, P. [3, 4] ; Avila, G. [20, 21] ; Badescu, A. M. [22] ; Balaceanu, A. [23] ; Barbato, F. [24] ; Luz, R. J. Barreira [3, 4] ; Beatty, J. J. [25] ; Becker, K. H. [26] ; Bellido, J. A. [27] ; Berat, C. [28] ; Bertaina, M. E. [29, 5] ; Bertou, X. [9, 10] ; Biermann, P. L. [30] ; Billoir, P. [7] ; Biteau, J. [31] ; Blaess, S. G. [27] ; Blanco, A. [4, 3] ; Blazek, J. [32] ; Bleve, C. [33, 34] ; Bohacova, M. [32] ; Boncioli, D. [35, 36] ; Bonifazi, D. C. [37] ; Borodai, N. [38] ; Botti, A. M. [11, 39] ; Brack, J. [40] ; Brancus, I. [23] ; Bretz, T. [41, 2] ; Bridgeman, A. [39] ; Briechle, F. L. [41, 2] ; Buchholz, P. [42] ; Bueno, A. [43, 44] ; Buitink, S. [1] ; Buscemi, M. [45, 46] ; Caballero-Mora, K. S. [47] ; Caccianiga, L. [48] ; Cancio, A. [11, 12] ; Canfora, F. [1] ; Caramete, L. [18] ; Caruso, R. [45, 46] ; Castellina, A. [5, 6] ; Cataldi, G. [33] ; Cazon, L. [3, 4] ; Chavez, A. G. [49] ; Chinellato, J. A. [50] ; Chudoba, J. [32] ; Clay, R. W. [27] ; Cobos, A. [11] ; Colalillo, R. [16, 24] ; Coleman, A. [51] ; Collica, L. [5] ; Coluccia, M. R. [33, 34] ; Conceicao, R. [4, 3] ; Consolati, G. [48] ; Contreras, F. [20, 21] ; Cooper, M. J. [27] ; Coutu, S. [51] ; Covault, C. E. [52] ; Cronin, J. [53] ; D'Amico, S. [33, 54] ; Daniel, B. [50] ; Dasso, S. [55, 56, 57] ; Daumiller, K. [39] ; Dawson, B. R. [27] ; de Almeida, M. [58] ; de Jong, S. J. [59, 1] ; De Mauro, G. [1] ; Neto, J. R. T. de Mello [37] ; De Mitri, I. [33, 34] ; de Oliveira, J. [58] ; de Souza, V. [60] ; Debatin, J. [39] ; Deligny, O. [31] ; Di Giulio, C. [61, 62] ; Di Matteo, A. [63, 64] ; Castro, M. L. Diaz [50] ; Diogo, F. [3, 4] ; Dobrigkeit, C. [50] ; D'Olivo, J. C. [13] ; Dorosti, Q. [42] ; dos Anjos, R. C. [65] ; Dova, M. T. [66, 67] ; Dundovic, A. ; Ebr, J. [32] ; Engel, R. [39] ; Erdmann, M. [41, 2] ; Erfani, M. [42] ; Escobar, C. O. [68] ; Espadanal, J. [3, 4] ; Etchegoyen, A. [11, 12] ; Farrar, G. [69] ; Fauth, A. C. [50] ; Fazzini, N. [68] ; Fenu, F. [29] ; Fick, B. [70] ; Figueira, J. M. [11] ; Filipcic, A. [71, 72] ; Fratu, O. [22] ; Freire, M. M. [73, 74] ; Fujii, T. [53] ; Fuster, A. [11, 12] ; Gaior, R. [7] ; Garcia, B. [75, 76] ; Garcia-Pinto, D. [17] ; Gate, F. [77] ; Gemmeke, H. [78] ; Gherghel-Lascu, A. [23] ; Ghia, P. L. [31] ; Giaccari, U. [37] ; Giammarchi, M. [79] ; Giller, M. [80] ; Glas, D. [81] ; Glaser, C. [41, 2] ; Golup, G. [9, 10] ; Berisso, M. Gomez [9, 10] ; Vitale, P. F. Gomez [20, 21] ; Gonzalez, N. [11, 39] ; Gorgi, A. [5, 6] ; Gorham, P. [82] ; Grillo, A. F. [35] ; Grubb, T. D. [27] ; Guarino, F. [62, 24] ; Guedes, G. P. [83] ; Hampel, M. R. [11] ; Hansen, P. [66, 67] ; Harari, D. [9, 10] ; Harrison, T. A. [27] ; Harton, J. L. [40] ; Haungs, A. [39] ; Hebbeker, T. [41, 2] ; Heck, D. [39] ; Heimann, P. [42] ; Herve, A. E. [84] ; Hill, G. C. [27] ; Hojvat, C. [68] ; Holt, E. [11, 39] ; Homola, P. [38] ; Horandel, J. R. [59, 1] ; Horvath, P. [85] ; Hrabovsky, M. [85] ; Huege, T. [39] ; Hulsman, J. [11, 39] ; Insolia, A. [45, 46] ; Isar, P. G. [18] ; Jandt, I. [26] ; Jansen, S. [59, 1] ; Johnsen, J. A. [86] ; Josebachuili, M. [11] ; Kaeaepae, A. [26] ; Kambeitz, O. [84] ; Kampert, K. H. [26] ; Katkov, I. [84] ; Keilhauer, B. [39] ; Kemmerich, N. [8] ; Kemp, E. [50] ; Kemp, J. [41, 2] ; Kieckhafer, R. M. [70] ; Klages, H. O. [39] ; Kleifges, M. [78] ; Kleinfeller, J. [20] ; Krause, R. [41, 2] ; Krohm, N. [26] ; Kuempel, D. [41, 2] ; Mezek, G. Kukec [72] ; Kunka, N. [78] ; Awad, A. Kuotb [39] ; LaHurd, D. [52] ; Lauscher, M. [41, 2] ; Legumina, R. [80] ; Leigui de Oliveira, M. A. [87] ; Letessier-Selvon, A. [7] ; Lhenry-Yvon, I. [31] ; Link, K. [84] ; Lo Presti, D. [46] ; Lopes, L. [4, 3] ; Lopez, R. [88] ; Lopez Casado, A. [89] ; Luce, Q. [31] ; Lucero, A. [11, 12] ; Malacari, M. [53] ; Mallamaci, M. [48, 79] ; Mandat, D. [32] ; Mantsch, P. [68] ; Mariazzi, A. G. [66, 67] ; Maris, I. C. [43, 44] ; Marsella, G. [33, 34] ; Martello, D. [35, 33] ; Martinez, H. [90] ; Martinez Bravo, O. [88] ; Masias Meza, J. J. [55, 57] ; Mathes, H. J. [39] ; Mathys, S. [26] ; Matthews, J. [91] ; Matthews, J. A. J. [92] ; Matthiae, G. [61, 62] ; Mayotte, E. [26] ; Mazur, P. O. [68] ; Medina, C. [86] ; Medina-Tanco, G. [13] ; Melo, D. [11] ; Menshikov, A. [78] ; Merenda, K. -D. [86] ; Micheletti, M. I. [73, 74] ; Middendorf, L. [41, 2] ; Minaya, I. A. [17] ; Miramonti, L. [79, 48] ; Mitrica, B. [23] ; Mockler, D. [84] ; Mollerach, S. [9, 10] ; Montanet, F. [28] ; Morello, C. [5, 6] ; Mostafa, M. [51] ; Mueller, A. L. [11, 39] ; Mueller, G. [41, 2] ; Muller, M. A. [93, 50] ; Mueller, S. [11, 39] ; Mussa, R. [5] ; Naranjo, I. [9, 10] ; Nellen, L. [13] ; Nguyen, P. H. [27] ; Niculescu-Oglinzanu, M. [23] ; Niechciol, M. [42] ; Niemietz, L. [26] ; Niggemann, T. [41, 2] ; Nitz, D. [70] ; Nosek, D. [94] ; Novotny, V. [94] ; Nozka, H. [85] ; Nunez, L. A. [19] ; Ochilo, L. [42] ; Oikonomou, F. [51] ; Olinto, A. [53] ; Palatka, M. [32] ; Pallotta, J. [95, 96] ; Papenbreer, P. [26] ; Parente, G. [89] ; Parra, A. [88] ; Paul, T. [97, 15] ; Pech, M. [32] ; Pedreira, F. [89] ; Pekala, J. [38] ; Pelayo, R. [98] ; Pena-Rodriguez, J. [19] ; Pereira, L. A. S. [50] ; Perlin, M. [11] ; Perrone, L. [33, 34] ; Peters, C. [41, 2] ; Petrera, S. [14, 63, 64] ; Phuntsok, J. [51] ; Piegaia, R. [55, 57] ; Pierog, T. [39] ; Pieroni, P. [55, 57] ; Pimenta, M. [4, 3] ; Pirronello, V. [45, 46] ; Platino, M. [11] ; Plum, M. [41, 2] ; Porowski, C. [38] ; Prado, R. R. [60] ; Privitera, P. [53] ; Prouza, M. [32] ; Quel, E. J. [95, 96] ; Querchfeld, S. [26] ; Quinn, S. [52] ; Ramos-Pollan, R. [19] ; Rautenberg, J. [26] ; Ravignani, D. [11] ; Revenu, B. [77] ; Ridky, J. [32] ; Risse, M. [42] ; Ristori, P. [95, 96] ; Rizi, V. [63, 64] ; de Carvalho, W. Rodrigues [8] ; Fernandez, G. Rodriguez [61, 62] ; Rojo, J. Rodriguez [20] ; Rogozin, D. [39] ; Roncoroni, M. J. [11] ; Roth, M. [39] ; Roulet, E. [9, 10] ; Rovero, A. C. [56] ; Ruehl, P. [42] ; Saffi, S. J. [27] ; Saftoiu, A. [23] ; Salamida, F. [63, 64] ; Salazar, H. [88] ; Saleh, A. [72] ; Greus, F. Salesa [51] ; Salina, G. [61] ; Sanchez, F. [11] ; Sanchez-Lucas, P. [43, 44] ; Santos, E. M. [8] ; Santos, E. [11] ; Sarazin, F. [86] ; Sarmento, R. [3, 4] ; Sarmiento, C. A. [11] ; Sato, R. [20] ; Schauer, M. [26] ; Scherini, V. [33] ; Schieler, H. [39] ; Schimp, M. [26] ; Schmidt, D. [11, 39] ; Scholten, O. [99, 100] ; Schovanek, P. [32] ; Schroder, F. G. [39] ; Schulz, A. [84] ; Schumacher, J. [41, 2] ; Sciutto, S. J. [66, 67] ; Segreto, A. [101, 45] ; Settimo, M. [7] ; Shadkam, A. [91] ; Shellard, R. C. [102] ; Sigl, G. ; Silli, G. [11, 39] ; Sima, O. [103] ; Smialkowski, A. [80] ; Smida, R. [39] ; Snow, G. R. [104] ; Sommers, P. [51] ; Sonntag, S. [42] ; Sorokin, J. [27] ; Squartini, R. [20] ; Stanca, D. [23] ; Stanic, S. [72] ; Stasielak, J. [38] ; Stassi, P. [28] ; Strafella, F. [33, 34] ; Suarez, F. [11, 12] ; Duran, M. Suarez [19] ; Sudholz, T. [27] ; Suomijarvi, T. [31] ; Supanitsky, A. D. [56] ; Swain, J. [97] ; Szadkowski, Z. [81] ; Taboada, A. [84] ; Taborda, O. A. [9, 10] ; Tapia, A. [11] ; Theodoro, V. M. [50] ; Timmermans, C. [59, 1] ; Peixoto, C. J. Todero [105] ; Tomankova, L. [39] ; Tome, B. [3, 4] ; Elipe, G. Torralba [89] ; Travnicek, P. [32] ; Trini, M. [72] ; Ulrich, R. [39] ; Unger, M. [39] ; Urban, M. [41, 2] ; Galicia, J. F. Valdes [13] ; Valino, I. [89] ; Valore, L. [16, 24] ; van Aar, G. [1] ; van Bodegom, P. [27] ; van den Berg, M. [100] ; van Vliet, A. [1] ; Varela, E. [88] ; Cardenas, B. Vargas [13] ; Varner, G. [82] ; Vazquez, R. A. [89] ; Veberic, D. [39] ; Quispe, I. D. Vergara [66, 67] ; Verzi, V. [61] ; Vicha, J. [32] ; Villasenor, L. [49] ; Vorobiov, S. [72] ; Wahlberg, H. [66, 67] ; Wainberg, O. [11, 12] ; Walz, D. [41, 2] ; Watson, A. A. [106] ; Weber, M. [78] ; Weindl, A. [39] ; Wiencke, L. [86] ; Wilczynski, H. [38] ; Winchen, T. [26] ; Wirtz, M. [41, 2] ; Wittkowski, D. [26] ; Wundheiler, B. [11] ; Yang, L. [72] ; Yelos, D. [11, 12] ; Yushkov, A. [11] ; Zas, E. [89] ; Zavrtanik, D. [71, 72] ; Zavrtanik, M. [71, 72] ; Zepeda, A. [90] ; Zimmermann, B. [78] ; Ziolkowski, M. [42] ; Zong, Z. [31] ; Zuccarello, F. [45, 46] ; Collaboration, Pierre Auger
Número total de Autores: 403
Afiliação do(s) autor(es):
Mostrar menos -
[1] Radboud Univ Nijmegen, Inst Math Astrophys & Particle Phys, Nijmegen - Netherlands
[2] Univ Hamburg, Phys Inst A 3, Hamburg - Germany
[3] Univ Lisbon, IST, Lisbon - Portugal
[4] Univ Lisbon, Lab Instrumentacao & Fis Expt Particulas, LIP, Lisbon - Portugal
[5] Ist Nazl Fis Nucl, Sez Torino, Turin - Italy
[6] INAF, Osserv Astrofis Torino, Turin - Italy
[7] Univ Paris 6 & Paris 7, CNRS, IN2P3, LPNHE, Paris - France
[8] Univ Sao Paulo, Inst Fis, Sao Paulo - Brazil
[9] Consejo Nacl Invest Cient & Tecn, Ctr Atom Bariloche, Buenos Aires, DF - Argentina
[10] Consejo Nacl Invest Cient & Tecn, Inst Balseiro, CNEA, UNCuyo, Buenos Aires, DF - Argentina
[11] UNSAM, CONICET, CNEA, Ctr Atom Constituyentes, Inst Tecnol Detecc & Astr, Buenos Aires, DF - Argentina
[12] Univ Tecnolog Nacl, Fac Reg Buenos Aires, Buenos Aires, DF - Argentina
[13] Univ Nacl Autonoma Mexico, Mexico City, DF - Mexico
[14] Gran Sasso Sci Inst INFN, Laquila - Italy
[15] CUNY, Lehman Coll, Dept Phys & Astron, New York, NY - USA
[16] Ist Nazl Fis Nucl, Sez Napoli, Naples - Italy
[17] Univ Complutense Madrid, Madrid - Spain
[18] Inst Space Sci, Magurele - Romania
[19] Univ Ind Santander, Bucaramanga - Colombia
[20] Observ Pierre Auger, Malargue - Argentina
[21] Comis Nacl Energia Atom, Buenos Aires, DF - Argentina
[22] Univ Politeh Bucharest, Bucharest - Romania
[23] Horia Hulubei Natl Inst Phys & Nucl Engn, Magurele - Romania
[24] Univ Naples Federico II, Dipartimento Fis Ettore Pancini, Naples - Italy
[25] Ohio State Univ, Columbus, OH 43210 - USA
[26] Berg Univ Wuppertal, Dept Phys, Wuppertal - Germany
[27] Univ Adelaide, Adelaide, SA - Australia
[28] Univ Grenoble Alpes, CNRS, IN2P3, LPSC, Grenoble - France
[29] Univ Turin, Dipartimento Fis, Turin - Italy
[30] Max Planck Inst Radioastron, Bonn - Germany
[31] Univ Paris Saclay, Univ Paris Sud, CNRS, IN2P3, IPNO, St Aubin - France
[32] Acad Sci Czech Republ, Inst Phys FZU, Prague - Czech Republic
[33] Ist Nazl Fis Nucl, Sez Lecce, Lecce - Italy
[34] Univ Salento, Dipartimento Matemat Fis E De Giorgi, Lecce - Italy
[35] Ist Nazl Fis Nucl, Lab Nazl Gran Sasso, Laquila - Italy
[36] Deutsch Elekt Synchrotron DESY, Zeuthen - Germany
[37] Univ Fed Rio de Janeiro, Inst Fis, Rio De Janeiro - Brazil
[38] Inst Nucl Phys PAN, Krakow - Poland
[39] Karlsruhe Inst Technol, Inst Kernphys IKP, Karlsruhe - Germany
[40] Colorado State Univ, Ft Collins, CO 80523 - USA
[41] Rhein Westfal TH Aachen, Phys Inst A 3, Aachen - Germany
[42] Univ Siegen, Fachbereich Phys Exp Teilchenphys 7, Siegen - Germany
[43] Univ Granada, Granada - Spain
[44] CAFPE, Granada - Spain
[45] Ist Nazl Fis Nucl, Sez Catania, Catania - Italy
[46] Univ Catania, Dipartimento Fis & Astron, Catania - Italy
[47] Univ Autonoma Chiapas, Tapachula - Mexico
[48] Univ Milan, Dipartimento Fis, Milan - Italy
[49] Univ Michoacana, Morelia, Michoacan - Mexico
[50] Univ Estadual Campinas UNICAMP, Campinas, SP - Brazil
[51] Penn State Univ, University Pk, PA 16802 - USA
[52] Case Western Reserve Univ, Cleveland, OH 44106 - USA
[53] Univ Chicago, Chicago, IL 60637 - USA
[54] Univ Salento, Dipartimento Ingn, Lecce - Italy
[55] Univ Buenos Aires, Dept Fis, Buenos Aires, DF - Argentina
[56] UBA, CONICET, IAFE, Buenos Aires, DF - Argentina
[57] Univ Buenos Aires, FCEyN, Dept Ciencias Atmosfera & Oceanos, Buenos Aires, DF - Argentina
[58] Univ Fed Fluminense, Niteroi, RJ - Brazil
[59] Nikhef, Amsterdam - Netherlands
[60] Univ Sao Paulo, Inst Fis Sao Carlos, Sao Carlos, SP - Brazil
[61] Ist Nazl Fis Nucl, Sez Roma Tor Vergata, Rome - Italy
[62] Univ Roma Tor Vergata, Dipartimento Fis, Rome - Italy
[63] Univ Aquila, Dipartimento Sci Fis & Chim, Laquila - Italy
[64] Ist Nazl Fis Nucl, Grp Collegato Aquila, Laquila - Italy
[65] Univ Fed Parana, Setor Palotina, Curitiba, Parana - Brazil
[66] Consejo Nacl Invest Cient & Tecn, La Plata, Buenos Aires - Argentina
[67] Univ Nacl La Plata, IFLP, La Plata, Buenos Aires - Argentina
[68] Fermilab Natl Accelerator Lab, Batavia, IL 60510 - USA
[69] NYU, New York, NY 10003 - USA
[70] Michigan Technol Univ, Houghton, MI 49931 - USA
[71] J Stefan Inst, Expt Particle Phys Dept, Ljubljana - Slovenia
[72] Univ Nova Gor, Lab Astroparticle Phys, Rozna Dolina - Slovenia
[73] UNR, CONICET, IFIR, Rosario, Santa Fe - Argentina
[74] UNR, Fac Ciencias Bioquim Farmaceut, Rosario, Santa Fe - Argentina
[75] Consejo Nacl Invest Cient & Tecn, UNSAM, CNEA, Inst Tecnol Detecc & Astroparticulas, Buenos Aires, DF - Argentina
[76] Consejo Nacl Invest Cient & Tecn, CNEA, Fac Reg Mendoza, Univ Tecnol Nacl, Buenos Aires, DF - Argentina
[77] Univ Nantes, CNRS, IN2P3, SUBATECH, Ecole Mines Nantes, Nantes - France
[78] Karlsruhe Inst Technol, Inst Prozessdatenverarbeitung & Elekt IPE, Karlsruhe - Germany
[79] Ist Nazl Fis Nucl, Sez Milano, Milan - Italy
[80] Univ Lodz, Fac Astrophys, Lodz - Poland
[81] Univ Lodz, Fac High Energy Astrophys, Lodz - Poland
[82] Univ Hawaii, Honolulu, HI 96822 - USA
[83] Univ Estadual Feira de Santana UEFS, Feira De Santana - Brazil
[84] Karlsruhe Inst Technol, Inst Exp Kernphys IEKP, Karlsruhe - Germany
[85] Palacky Univ, RCPTM, Olomouc - Czech Republic
[86] Colorado Sch Mines, Golden, CO 80401 - USA
[87] Univ Fed ABC UFABC, Santo Andre - Brazil
[88] Benemerita Univ Autonoma Puebla BUAP, Puebla - Mexico
[89] Univ Santiago Compostela, Santiago - Spain
[90] CINVESTAV, Ctr Invest & Estud Avanzados IPN, Mexico City, DF - Mexico
[91] Louisiana State Univ, Baton Rouge, LA 70803 - USA
[92] Univ New Mexico, Albuquerque, NM 87131 - USA
[93] Univ Fed Pelotas, Pelotas - Brazil
[94] Univ Prague, Inst Particle & Nucl Phys, Prague - Czech Republic
[95] CITEDEF, Ctr Invest Laseres & Aplicac, Buenos Aires, DF - Argentina
[96] Consejo Nacl Invest Cient & Tecn, Buenos Aires, DF - Argentina
[97] Northeastern Univ, Boston, MA - USA
[98] UPIITA, IPN, Mexico City, DF - Mexico
[99] Vrije Univ Brussels, Brussels - Belgium
[100] Univ Groningen, Ctr Adv Radiat Technol, KVI, Groningen - Netherlands
[101] INAF, Ist Astrofis Spaziale & Fis Cosm Palermo, Rome - Italy
[102] CBPF, Rio De Janeiro - Brazil
[103] Univ Bucharest, Phys Dept, Bucharest - Romania
[104] Univ Nebraska, Lincoln, NE 68583 - USA
[105] Univ Sao Paulo, Escola Engenharia Lorena, Sao Paulo - Brazil
[106] Univ Leeds, Sch Phys & Astron, Leeds, W Yorkshire - England
Número total de Afiliações: 106
Tipo de documento: Artigo Científico
Fonte: Journal of Instrumentation; v. 12, OCT 2017.
Citações Web of Science: 4
Resumo

An in-situ calibration of a logarithmic periodic dipole antenna with a frequency coverage of 30 MHz to 80 MHz is performed. Such antennas are part of a radio station system used for detection of cosmic ray induced air showers at the Engineering Radio Array of the Pierre Auger Observatory, the so-called Auger Engineering Radio Array (AERA). The directional and frequency characteristics of the broadband antenna are investigated using a remotely piloted aircraft carrying a small transmitting antenna. The antenna sensitivity is described by the vector effective length relating the measured voltage with the electric-field components perpendicular to the incoming signal direction. The horizontal and meridional components are determined with an overall uncertainty of 7.4(-0.3)(+0.9)%and 10.3(-1.7)(+2.8)% respectively. The measurement is used to correct a simulated response of the frequency and directional response of the antenna. In addition, the influence of the ground conductivity and permittivity on the antenna response is simulated. Both have a negligible influence given the ground conditions measured at the detector site. The overall uncertainties of the vector effective length components result in an uncertainty of 8.8(-1.3)(+2.1)% in the square root of the energy fluence for incoming signal directions with zenith angles smaller than 60 degrees. (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