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101 results on '"M. Melissas"'

1. Final results of the LOPES radio interferometer for cosmic-ray air showers

Author: W. D. Apel, J. C. Arteaga-Velázquez, L. Bähren, K. Bekk, M. Bertaina, P. L. Biermann, J. Blümer, H. Bozdog, E. Cantoni, A. Chiavassa, K. Daumiller, V. de Souza, F. Di Pierro, P. Doll, R. Engel, H. Falcke, B. Fuchs, H. Gemmeke, C. Grupen, A. Haungs, D. Heck, J. R. Hörandel, A. Horneffer, D. Huber, T. Huege, P. G. Isar, K.-H. Kampert, D. Kang, O. Krömer, J. Kuijpers, K. Link, P. Łuczak, M. Ludwig, H. J. Mathes, M. Melissas, C. Morello, S. Nehls, J. Oehlschläger, N. Palmieri, T. Pierog, J. Rautenberg, H. Rebel, M. Roth, C. Rühle, A. Saftoiu, H. Schieler, A. Schmidt, S. Schoo, F.G. Schröder, O. Sima, G. Toma, G. C. Trinchero, A. Weindl, J. Wochele, J. Zabierowski, J. A. Zensus, and LOPES Collaboration
Subjects: Astrophysics, QB460-466, Nuclear and particle physics. Atomic energy. Radioactivity, QC770-798
Abstract: Abstract LOPES, the LOFAR prototype station, was an antenna array for cosmic-ray air showers operating from 2003 to 2013 within the KASCADE-Grande experiment. Meanwhile, the analysis is finished and the data of air-shower events measured by LOPES are available with open access in the KASCADE Cosmic Ray Data Center (KCDC). This article intends to provide a summary of the achievements, results, and lessons learned from LOPES. By digital, interferometric beamforming the detection of air showers became possible in the radio-loud environment of the Karlsruhe Institute of Technology (KIT). As a prototype experiment, LOPES tested several antenna types, array configurations and calibration techniques, and pioneered analysis methods for the reconstruction of the most important shower parameters, i.e., the arrival direction, the energy, and mass-dependent observables such as the position of the shower maximum. In addition to a review and update of previously published results, we also present new results based on end-to-end simulations including all known instrumental properties. For this, we applied the detector response to radio signals simulated with the CoREAS extension of CORSIKA, and analyzed them in the same way as measured data. Thus, we were able to study the detector performance more accurately than before, including some previously inaccessible features such as the impact of noise on the interferometric cross-correlation beam. These results led to several improvements, which are documented in this paper and can provide useful input for the design of future cosmic-ray experiments based on the digital radio-detection technique.
Published: 2021
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2. A comparison of the cosmic-ray energy scales of Tunka-133 and KASCADE-Grande via their radio extensions Tunka-Rex and LOPES

Author: W.D. Apel, J.C. Arteaga-Velázquez, L. Bähren, P.A. Bezyazeekov, K. Bekk, M. Bertaina, P.L. Biermann, J. Blümer, H. Bozdog, I.M. Brancus, N.M. Budnev, E. Cantoni, A. Chiavassa, K. Daumiller, V. de Souza, F. Di Pierro, P. Doll, R. Engel, H. Falcke, O. Fedorov, B. Fuchs, H. Gemmeke, O.A. Gress, C. Grupen, A. Haungs, D. Heck, R. Hiller, J.R. Hörandel, A. Horneffer, D. Huber, T. Huege, P.G. Isar, K.-H. Kampert, D. Kang, Y. Kazarina, M. Kleifges, E.E. Korosteleva, D. Kostunin, O. Krömer, J. Kuijpers, L.A. Kuzmichev, K. Link, N. Lubsandorzhiev, P. Łuczak, M. Ludwig, H.J. Mathes, M. Melissas, R.R. Mirgazov, R. Monkhoev, C. Morello, J. Oehlschläger, E.A. Osipova, A. Pakhorukov, N. Palmieri, L. Pankov, T. Pierog, V.V. Prosin, J. Rautenberg, H. Rebel, M. Roth, G.I. Rubtsov, C. Rühle, A. Saftoiu, H. Schieler, A. Schmidt, S. Schoo, F.G. Schröder, O. Sima, G. Toma, G.C. Trinchero, A. Weindl, R. Wischnewski, J. Wochele, J. Zabierowski, A. Zagorodnikov, and J.A. Zensus
Subjects: Physics, QC1-999
Abstract: The radio technique is a promising method for detection of cosmic-ray air showers of energies around 100PeV and higher with an array of radio antennas. Since the amplitude of the radio signal can be measured absolutely and increases with the shower energy, radio measurements can be used to determine the air-shower energy on an absolute scale. We show that calibrated measurements of radio detectors operated in coincidence with host experiments measuring air showers based on other techniques can be used for comparing the energy scales of these host experiments. Using two approaches, first via direct amplitude measurements, and second via comparison of measurements with air shower simulations, we compare the energy scales of the air-shower experiments Tunka-133 and KASCADE-Grande, using their radio extensions, Tunka-Rex and LOPES, respectively. Due to the consistent amplitude calibration for Tunka-Rex and LOPES achieved by using the same reference source, this comparison reaches an accuracy of approximately 10% – limited by some shortcomings of LOPES, which was a prototype experiment for the digital radio technique for air showers. In particular we show that the energy scales of cosmic-ray measurements by the independently calibrated experiments KASCADE-Grande and Tunka-133 are consistent with each other on this level. Keywords: Cosmic rays, Radio detection, LOPES, Tunka-Rex, Tunka-133, KASCADE-Grande
Published: 2016
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3. DETECTION OF A CHANGE OF SLOPE IN THE SPECTRUM OF HEAVY MASS COSMIC RAYS PRIMARIES BY THE KASCADE-GRANDE EXPERIMENT

Author: A. Chiavassa, W. D. Apel, J. C. Arteaga-Velázquez, K. Bekk, M. Bertaina, J. Blümer, H. Bozdog, I. M. Brancus, E. Cantoni, F. Cossavella, K. Daumiller, V. de Souza, F. Di Pierro, P. Doll, R. Engel, J. Engler, M. Finger, B. Fuchs, D. Fuhrmann, F. Garino, H. J. Gils, R. Glasstetter, C. Grupen, A. Haungs, D. Heck, J. R. Hörandel, D. Huber, T. Huege, K.-H. Kampert, D. Kang, H. O. Klages, K. Link, P. Łuczak, M. Ludwig, H. J. Mathes, H. J. Mayer, M. Melissas, J. Milke, B. Mitrica, C. Morello, J. Oehlschläger, S. Ostapchenko, N. Palmieri, M. Petcu, T. Pierog, H. Rebel, M. Roth, H. Schieler, S. Schoo, F. G. Schröder, O. Sima, G. Toma, G. C. Trinchero, H. Ulrich, A. Weindl, J. Wochele, M. Wommer, and J. Zabierowski
Subjects: Engineering (General). Civil engineering (General), TA1-2040
Abstract: KASCADE-Grande is an extensive air shower experiment devoted to the study of cosmic rays in the 1016 ÷ 1018 eV energy range. The array is composed by different detectors allowing independent measurements of the number of muons (Nμ) and charged particles (Nch) of extensive air showers (EAS). These two observables are then used to study the primary energy spectrum, separating the events in two samples, on the basis of the shower size ratio, corrected for attenuation in the atmosphere, lnNμ/ lnNch. The two samples represent the light and heavy mass groups of the primaries. In the studied energy range only the spectrum of heavy primaries shows a significant change of slope, the energy (estimated using the QGSJET II hadronic interaction model) of this feature is in agreeement with the expectations of a rigidity dependent knee feature.
Published: 2013
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4. Ultrahigh Energy Neutrinos at the Pierre Auger Observatory

Author: P. Abreu, M. Aglietta, M. Ahlers, E. J. Ahn, I. F. M. Albuquerque, D. Allard, I. Allekotte, J. Allen, P. Allison, A. Almela, J. Alvarez Castillo, J. Alvarez-Muñiz, R. Alves Batista, M. Ambrosio, A. Aminaei, L. Anchordoqui, S. Andringa, T. Antičić, C. Aramo, E. Arganda, F. Arqueros, H. Asorey, P. Assis, J. Aublin, M. Ave, M. Avenier, G. Avila, T. Bäcker, A. M. Badescu, M. Balzer, K. B. Barber, A. F. Barbosa, R. Bardenet, S. L. C. Barroso, B. Baughman, J. Bäuml, J. J. Beatty, B. R. Becker, K. H. Becker, A. Bellétoile, J. A. Bellido, S. BenZvi, C. Berat, X. Bertou, P. L. Biermann, P. Billoir, F. Blanco, M. Blanco, C. Bleve, H. Blümer, M. Boháčová, D. Boncioli, C. Bonifazi, R. Bonino, N. Borodai, J. Brack, I. Brancus, P. Brogueira, W. C. Brown, R. Bruijn, P. Buchholz, A. Bueno, R. E. Burton, K. S. Caballero-Mora, B. Caccianiga, L. Caramete, R. Caruso, A. Castellina, O. Catalano, G. Cataldi, L. Cazon, R. Cester, J. Chauvin, S. H. Cheng, A. Chiavassa, J. A. Chinellato, J. Chirinos Diaz, J. Chudoba, M. Cilmo, R. W. Clay, M. R. Coluccia, R. Conceição, F. Contreras, H. Cook, M. J. Cooper, J. Coppens, A. Cordier, S. Coutu, C. E. Covault, A. Creusot, A. Criss, J. Cronin, A. Curutiu, S. Dagoret-Campagne, R. Dallier, B. Daniel, S. Dasso, K. Daumiller, B. R. Dawson, R. M. de Almeida, M. De Domenico, C. De Donato, S. J. de Jong, G. De La Vega, W. J. M. de Mello Junior, J. R. T. de Mello Neto, I. De Mitri, V. de Souza, K. D. de Vries, L. del Peral, M. del Río, O. Deligny, H. Dembinski, N. Dhital, C. Di Giulio, M. L. Díaz Castro, P. N. Diep, F. Diogo, C. Dobrigkeit, W. Docters, J. C. D'Olivo, P. N. Dong, A. Dorofeev, J. C. dos Anjos, M. T. Dova, D. D'Urso, I. Dutan, J. Ebr, R. Engel, M. Erdmann, C. O. Escobar, J. Espadanal, A. Etchegoyen, P. Facal San Luis, H. Falcke, G. Farrar, A. C. Fauth, N. Fazzini, A. P. Ferguson, B. Fick, A. Filevich, A. Filipčič, S. Fliescher, C. E. Fracchiolla, E. D. Fraenkel, O. Fratu, U. Fröhlich, B. Fuchs, R. Gaior, R. F. Gamarra, S. Gambetta, B. García, S. T. Garcia Roca, D. Garcia-Gamez, D. Garcia-Pinto, A. Gascon Bravo, H. Gemmeke, P. L. Ghia, M. Giller, J. Gitto, H. Glass, M. S. Gold, G. Golup, F. Gomez Albarracin, M. Gómez Berisso, P. F. Gómez Vitale, P. Gonçalves, J. G. Gonzalez, B. Gookin, A. Gorgi, P. Gouffon, E. Grashorn, S. Grebe, N. Griffith, M. Grigat, A. F. Grillo, Y. Guardincerri, F. Guarino, G. P. Guedes, P. Hansen, D. Harari, T. A. Harrison, J. L. Harton, A. Haungs, T. Hebbeker, D. Heck, A. E. Herve, C. Hojvat, N. Hollon, V. C. Holmes, P. Homola, J. R. Hörandel, P. Horvath, M. Hrabovský, D. Huber, T. Huege, A. Insolia, F. Ionita, A. Italiano, C. Jarne, S. Jiraskova, M. Josebachuili, K. Kadija, K. H. Kampert, P. Karhan, P. Kasper, I. Katkov, B. Kégl, B. Keilhauer, A. Keivani, J. L. Kelley, E. Kemp, R. M. Kieckhafer, H. O. Klages, M. Kleifges, J. Kleinfeller, J. Knapp, D.-H. Koang, K. Kotera, N. Krohm, O. Krömer, D. Kruppke-Hansen, F. Kuehn, D. Kuempel, J. K. Kulbartz, N. Kunka, G. La Rosa, C. Lachaud, D. LaHurd, L. Latronico, R. Lauer, P. Lautridou, S. Le Coz, M. S. A. B. Leão, D. Lebrun, P. Lebrun, M. A. Leigui de Oliveira, A. Letessier-Selvon, I. Lhenry-Yvon, K. Link, R. López, A. Lopez Agüera, K. Louedec, J. Lozano Bahilo, L. Lu, A. Lucero, M. Ludwig, H. Lyberis, M. C. Maccarone, C. Macolino, S. Maldera, D. Mandat, P. Mantsch, A. G. Mariazzi, J. Marin, V. Marin, I. C. Maris, H. R. Marquez Falcon, G. Marsella, D. Martello, L. Martin, H. Martinez, O. Martínez Bravo, H. J. Mathes, J. Matthews, J. A. J. Matthews, G. Matthiae, D. Maurel, D. Maurizio, P. O. Mazur, G. Medina-Tanco, M. Melissas, D. Melo, E. Menichetti, A. Menshikov, P. Mertsch, C. Meurer, S. Mićanović, M. I. Micheletti, I. A. Minaya, L. Miramonti, L. Molina-Bueno, S. Mollerach, M. Monasor, D. Monnier Ragaigne, F. Montanet, B. Morales, C. Morello, E. Moreno, J. C. Moreno, M. Mostafá, C. A. Moura, M. A. Muller, G. Müller, M. Münchmeyer, R. Mussa, G. Navarra, J. L. Navarro, S. Navas, P. Necesal, L. Nellen, A. Nelles, J. Neuser, P. T. Nhung, M. Niechciol, L. Niemietz, N. Nierstenhoefer, D. Nitz, D. Nosek, L. Nožka, J. Oehlschläger, A. Olinto, M. Ortiz, N. Pacheco, D. Pakk Selmi-Dei, M. Palatka, J. Pallotta, N. Palmieri, G. Parente, E. Parizot, A. Parra, S. Pastor, T. Paul, M. Pech, J. Pękala, R. Pelayo, I. M. Pepe, L. Perrone, R. Pesce, E. Petermann, S. Petrera, A. Petrolini, Y. Petrov, C. Pfendner, R. Piegaia, T. Pierog, P. Pieroni, M. Pimenta, V. Pirronello, M. Platino, M. Plum, V. H. Ponce, M. Pontz, A. Porcelli, P. Privitera, M. Prouza, E. J. Quel, S. Querchfeld, J. Rautenberg, O. Ravel, D. Ravignani, B. Revenu, J. Ridky, S. Riggi, M. Risse, P. Ristori, H. Rivera, V. Rizi, J. Roberts, W. Rodrigues de Carvalho, G. Rodriguez, I. Rodriguez Cabo, J. Rodriguez Martino, J. Rodriguez Rojo, M. D. Rodríguez-Frías, G. Ros, J. Rosado, T. Rossler, M. Roth, B. Rouillé-d'Orfeuil, E. Roulet, A. C. Rovero, C. Rühle, A. Saftoiu, F. Salamida, H. Salazar, F. Salesa Greus, G. Salina, F. Sánchez, C. E. Santo, E. Santos, E. M. Santos, F. Sarazin, B. Sarkar, S. Sarkar, R. Sato, N. Scharf, V. Scherini, H. Schieler, P. Schiffer, A. Schmidt, O. Scholten, H. Schoorlemmer, J. Schovancova, P. Schovánek, F. Schröder, S. Schulte, D. Schuster, S. J. Sciutto, M. Scuderi, A. Segreto, M. Settimo, A. Shadkam, R. C. Shellard, I. Sidelnik, G. Sigl, O. Sima, A. Śmiałkowski, R. Šmída, G. R. Snow, P. Sommers, J. Sorokin, H. Spinka, R. Squartini, Y. N. Srivastava, S. Stanic, J. Stapleton, J. Stasielak, M. Stephan, A. Stutz, F. Suarez, T. Suomijärvi, A. D. Supanitsky, T. Šuša, M. S. Sutherland, J. Swain, Z. Szadkowski, M. Szuba, A. Tapia, M. Tartare, O. Taşcău, R. Tcaciuc, N. T. Thao, D. Thomas, J. Tiffenberg, C. Timmermans, W. Tkaczyk, C. J. Todero Peixoto, G. Toma, L. Tomankova, B. Tomé, A. Tonachini, P. Travnicek, D. B. Tridapalli, G. Tristram, E. Trovato, M. Tueros, R. Ulrich, M. Unger, M. Urban, J. F. Valdés Galicia, I. Valiño, L. Valore, A. M. van den Berg, E. Varela, B. Vargas Cárdenas, J. R. Vázquez, R. A. Vázquez, D. Veberič, V. Verzi, J. Vicha, M. Videla, L. Villaseñor, H. Wahlberg, P. Wahrlich, O. Wainberg, D. Walz, A. A. Watson, M. Weber, K. Weidenhaupt, A. Weindl, F. Werner, S. Westerhoff, B. J. Whelan, A. Widom, G. Wieczorek, L. Wiencke, B. Wilczyñska, H. Wilczyñski, M. Will, C. Williams, T. Winchen, M. Wommer, B. Wundheiler, T. Yamamoto, T. Yapici, P. Younk, G. Yuan, A. Yushkov, B. Zamorano Garcia, E. Zas, D. Zavrtanik, M. Zavrtanik, I. Zaw, A. Zepeda, Y. Zhu, M. Zimbres Silva, and M. Ziolkowski
Subjects: Physics, QC1-999
Abstract: The observation of ultrahigh energy neutrinos (UHEνs) has become a priority in experimental astroparticle physics. UHEνs can be detected with a variety of techniques. In particular, neutrinos can interact in the atmosphere (downward-going ν) or in the Earth crust (Earth-skimming ν), producing air showers that can be observed with arrays of detectors at the ground. With the surface detector array of the Pierre Auger Observatory we can detect these types of cascades. The distinguishing signature for neutrino events is the presence of very inclined showers produced close to the ground (i.e., after having traversed a large amount of atmosphere). In this work we review the procedure and criteria established to search for UHEνs in the data collected with the ground array of the Pierre Auger Observatory. This includes Earth-skimming as well as downward-going neutrinos. No neutrino candidates have been found, which allows us to place competitive limits to the diffuse flux of UHEνs in the EeV range and above.
Published: 2013
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5. Rapid subduction in the deep North Western Mediterranean

Author: C. Richardt, D. Dornic, D. Lo Presti, G.E. Păvălaş, M. Morganti, Oleg Kalekin, Isabelle Taupier-Letage, K. Lyons, M. Circella, Uli Katz, A. Mazure, G. Halladjian, D. Zaborov, M. Ardid, A. Radu, Francisco Camarena, J. Hößl, H. Laschinsky, C. Curtil, A. Albert, M. Neff, Gisela Anton, Robert Lahmann, Vincenzo Cavasinni, C. Distefano, C. Donzaud, B. Vallage, A. Brown, U. Fritsch, Antonio Capone, P. Payre, C. M. Reed, Annarita Margiotta, J. J. Aubert, Jürgen Brunner, J.-L. Fuda, Maurizio Spurio, Anne Deschamps, R. Pillet, U. Emanuele, A.J. Heijboer, J. Carr, F. M. Schoeck, M. P. Decowski, C. Racca, F. Salesa, L. Tasca, Thierry Pradier, G. Guillard, J.J. Hernández-Rey, Gregory David Hallewell, H. Loehner, G. Lelaizant, C. Picq, S. Loucatos, Dominique Lefèvre, S.F. Biagi, E. A. De Wolf, Holger Motz, S. Basa, Vincent Bertin, M. Marcelin, N. Picot-Clemente, R. Auer, Juanan Aguilar, R. Ostasch, G. Wijnker, Manuela Vecchi, Ciro Bigongiari, Heide Costantini, Alexander Kappes, G. Riccobene, D. Castel, G.V. Russo, V. Flaminio, G. De Bonis, Giuseppina Larosa, J.P. Gómez-González, I. Dekeyser, F. Lucarelli, Jos Steijger, V. Van Elewyck, F. Fehr, Gilles Maurin, P. Vernin, Rezo Shanidze, P. Coyle, J. Zúñiga, Thomas Eberl, V. Popa, W. Kretschmer, J. P. Schuller, M.C. Bouwhuis, M. Rujoiu, Stephanie Escoffier, M. Bazzotti, J.-P. Ernenwein, P. Piattelli, Simona Toscano, K. Fratini, Manuel Bou-Cabo, Francesco Simeone, N. Cottini, Patrick Lamare, A. C.S. Assis Jesus, Tri L. Astraatmadja, Th. Stolarczyk, S. Anvar, S. Mangano, Yann Hello, Guillaume Lambard, J.A. Martínez-Mora, H. van Haren, E. Castorina, Kay Graf, Christian Tamburini, Ph. Charvis, J. Petrovic, G. Giacomelli, C. Naumann, G. Palioselitis, B. Baret, Doriane Drouhin, Antoine Kouchner, M. Melissas, H. Yepes, E. Presani, Tommaso Chiarusi, C. Kopper, Teresa Montaruli, R. Coniglione, J.D. Zornoza, Nasser Kalantar-Nayestanaki, M. de Jong, M. Anghinolfi, J. Busto, L. Moscoso, S. Cecchini, G. Lim, P. Kooijman, G. Carminati, Centre de Physique des Particules de Marseille (CPPM), Aix Marseille Université (AMU)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), AstroParticule et Cosmologie (APC (UMR_7164)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Laboratoire d'Astrophysique de Marseille (LAM), Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS), Centre d'océanologie de Marseille (COM), Université de la Méditerranée - Aix-Marseille 2-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Université Paris Cité (UPCité), Institut Pluridisciplinaire Hubert Curien (IPHC), and Université de Strasbourg (UNISTRA)-Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)
Subjects: Convection, [SDU.OCEAN]Sciences of the Universe [physics]/Ocean, Atmosphere, Subduction, Large detector systems for particle and astroparticle physics, Cherenkov detectors, visible and IR photons (vacuum), Vortex, Boundary current, law.invention, Telescope, Acoustic Doppler current profiler, Amplitude, Oceanography, Water column, law, [SDU]Sciences of the Universe [physics], Neutrino detectors, Photon detectors for UV, visible and IR photons (vacuum), Photon detectors for UV, Geology
Abstract: An Acoustic Doppler Current Profiler (ADCP) moored at the deep-sea ANTARES neutrino telescope site near Toulon, France, measured downward vertical currents of amplitudes up to 0.03 m s−1 in spring 2006. The currents were accompanied by enhanced levels of acoustic reflection by a factor of about 10 and by horizontal currents reaching 0.35 m s−1. These observations coincided with high levels of bioluminescence detected by the telescope. Although during winter 2006 deep dense-water formation occurred in this area, episodes of high levels of suspended particles and large vertical currents continuing into the summer are not direct evidence of this process. It is hypothesized that the main process allowing for particles to be moved across the entire water column (2500 m) within a few days, is local convection, triggered by small-mesoscale phenomena, such as meanders including a bipolar vortex, linked with boundary current instabilities.
Published: 2022

6. Final results of the LOPES radio interferometer for cosmic-ray air showers

Author: Béatrice Fuchs, W. D. Apel, D. Huber, A. Chiavassa, Heino Falcke, L. Bähren, H. Rebel, J. Blümer, H. J. Mathes, E. Cantoni, P. Łuczak, J. Wochele, Octavian Sima, N. Palmieri, S. Schoo, Frank G. Schröder, J. Rautenberg, C. Rühle, H. Schieler, H. Bozdog, D. Heck, M. Melissas, J. Oehlschläger, K. Bekk, T. Pierog, Karl-Heinz Kampert, Ralph Engel, A. Saftoiu, A. Horneffer, D. Kang, S. Nehls, Markus Roth, C. Grupen, Tim Huege, J. A. Zensus, P. Doll, A. Schmidt, O. Krömer, G. Toma, F. Di Pierro, M. Ludwig, C. Morello, Peter L. Biermann, K. Link, Paula Gina Isar, V. de Souza, A. Haungs, Jörg R. Hörandel, H. Gemmeke, Kai Daumiller, J. Zabierowski, J. C. Arteaga-Velázquez, M. E. Bertaina, G.C. Trinchero, A. Weindl, Jan Kuijpers, and Physics
Subjects: Beamforming, Physics and Astronomy (miscellaneous), Astronomy, FOS: Physical sciences, lcsh:Astrophysics, Cosmic ray, Antenna array, lcsh:QB460-466, ddc:530, lcsh:Nuclear and particle physics. Atomic energy. Radioactivity, Engineering (miscellaneous), Instrumentation and Methods for Astrophysics (astro-ph.IM), Remote sensing, Physics, High Energy Astrophysical Phenomena (astro-ph.HE), astro-ph.HE, LOPES, Detector, LOFAR, KASCADE, lcsh:QC770-798, Antenna (radio), Astrophysics - High Energy Astrophysical Phenomena, Astrophysics - Instrumentation and Methods for Astrophysics, RAIOS CÓSMICOS, astro-ph.IM
Abstract: LOPES, the LOFAR prototype station, was an antenna array for cosmic-ray air showers operating from 2003 - 2013 within the KASCADE-Grande experiment. Meanwhile, the analysis is finished and the data of air-shower events measured by LOPES are available with open access in the KASCADE Cosmic Ray Data Center (KCDC). This article intends to provide a summary of the achievements, results, and lessons learned from LOPES. By digital, interferometric beamforming the detection of air showers became possible in the radio-loud environment of the Karlsruhe Institute of Technology (KIT). As a prototype experiment, LOPES tested several antenna types, array configurations and calibration techniques, and pioneered analysis methods for the reconstruction of the most important shower parameters, i.e., the arrival direction, the energy, and mass-dependent observables such as the position of the shower maximum. In addition to a review and update of previously published results, we also present new results based on end-to-end simulations including all known instrumental properties. For this, we applied the detector response to radio signals simulated with the CoREAS extension of CORSIKA, and analyzed them in the same way as measured data. Thus, we were able to study the detector performance more accurately than before, including some previously inaccessible features such as the impact of noise on the interferometric cross-correlation beam. These results led to several improvements, which are documented in this paper and can provide useful input for the design of future cosmic-ray experiments based on the digital radio-detection technique., Comment: Accepted for publication by EPJ C
Published: 2021

7. Latest results from the KASCADE-Grande experiment

Author: P. Doll, C. Morello, F. Di Pierro, D. Fuhrmann, B. Mitrica, E. Cantoni, T. Huege, C. Curcio, J. Oehlschläger, D. Huber, K. Bekk, H. Bozdog, H. J. Mathes, Andreas Haungs, M. Ludwig, Claus Grupen, M. E. Bertaina, J. Milke, H. Ulrich, K. Link, T. Pierog, D. Kang, H.O. Klages, M. Petcu, J. Blümer, J. Zabierowski, K. H. Kampert, P. Łuczak, N. Palmieri, G.C. Trinchero, F.G. Schröder, R. Glasstetter, A. Weindl, J.C. Arteaga-Velázquez, H. Rebel, Kai Daumiller, I.M. Brancus, J. Wochele, Markus Roth, V. de Souza, Octavian Sima, W. D. Apel, M. Melissas, S. Schoo, Jörg R. Hörandel, J. Engler, D. Heck, A. Chiavassa, Béatrice Fuchs, H.J. Mayer, H. Schieler, Ralph Engel, G. Toma, F. Cossavella, S. Ostapchenko, and H.J. Gils
Subjects: Physics, Nuclear and High Energy Physics, Muon, Electromagnetic spectrum, Astronomy, Hadron, Cosmic ray, Spectral line, Charged particle, Nuclear physics, KASCADE, Maschinenbau, Anisotropy, Instrumentation
Abstract: The KASCADE-Grande experiment operated at KIT from January 2004 to November 2012, measuring EAS generated by primary cosmic rays in the 10 16 –10 18 eV energy range. The experiment detected, for each single event, with a high resolution, the total number of charged particles ( N ch ) and of muons ( N μ ). In this contribution we present the latest results about: (i) The measurement of the all particle energy spectrum, discussing the influence of the hadronic interaction model used to derive the energy calibration of the experimental data. (ii) The energy spectra derived separating the events according to the N μ / N ch ratio. This technique allowed us to unveil a steepening of the spectrum of heavy primaries at E ~ 10 16.92 ± 0.04 eV and a hardening of the spectrum of light primaries at E ~ 10 17.08 ± 0.08 eV . (iii) The elemental spectra (for five mass groups) obtained applying a detailed unfolding analysis technique. (iv) A search for large scale anisotropies.
Published: 2014
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8. Studies of a full-scale mechanical prototype line for the ANTARES neutrino telescope and tests of a prototype instrument for deep-sea acoustic measurements

Author: T. Legou, M. Ruppi, Chantal Compère, R. Ostasch, F. Urbano, Timo Karg, Diego Real, C. Gojak, V. Valente, G. Lamanna, V. Roca, V. Flaminio, C. Fiorello, I. Sokalski, J. Beltramelli, M. Taiuti, E. Kok, A. Rostovtsev, M.C. Bouwhuis, H. Loehner, A. Bigi, Chiara Roda, E. Falchini, Dominique Lefèvre, A. Le Van Suu, R. De Vita, F. Réthoré, V. Popa, H. Zaccone, J.R. Hubbard, Patrick Lamare, S. Cuneo, Julien Lavalle, Annarita Margiotta, K. Fratini, H. Laschinsky, Nicole Béthoux, R. Coniglione, Rosario Megna, C. Petta, L. Caponetto, C. Colnard, G. Wobbe, V. Niess, A. Ceres, Mario Musumeci, N. Randazzo, Thierry Pradier, G. Giacomelli, A. Heijboer, B. Vallage, B. Dinkespieler, J. Poinsignon, G. Damy, H. Le Provost, J. J. Aubert, R. Pillet, Nasser Kalantar-Nayestanaki, G. Vaudaine, G. Lelaizant, J.M. Gallone, F. Schmitt, F. Jouvenot, Paolo Sapienza, M. Jaquet, E. A. De Wolf, J. P. Schuller, G. Rusydi, Elie Aslanides, J. Carr, B. Hartmann, A. F. Yao, Holger Motz, A. Albert, P. Vernin, R. van Dantzig, R. Auer, S. Anvar, Juanan Aguilar, G. Wijnker, K. Salomon, M. de Jong, K. Streeb, Corinne Donzaud, J.J. Hernández-Rey, F. Salesa, J.-P. Pineau, D. Castel, G.V. Russo, S. Loucatos, M. Melissas, Robert Lahmann, Yvonne Becherini, Philippe Charvis, B. van Rens, J. P. Ernenwein, M. Marcelin, R. Masullo, Mohsen Harakeh, M. Circella, Alexander Kappes, F. Cafagna, L. A. M. Tasca, P. Valdy, D. Lo Presti, Gregory David Hallewell, Nathalie Palanque-Delabrouille, W. Kretschmer, V. Bertin, J. van Randwijk, Stephanie Escoffier, P. Payre, Tommaso Chiarusi, J.-L. Fuda, R. Blaes, M. Ageron, N. Cottini, G. Debonis, C. Kopper, V. Lyashuk, H. Peek, F. Lucarelli, S. Mangano, P. Lagier, J.D. Zornoza, M. Battaglieri, J.-X. Dessa, F. Fehr, G. Lim, Guillaume Lambard, Charling Tao, F.E. Ardellier-Desages, V. Rigaud, Jürgen Brunner, J.J. Destelle, E. Barbarito, U. F. Katz, C. Olivetto, S. Kuch, I. Dekeyser, L. Caillat, F. Guilloux, C. Naumann, Ana G. Pérez, F. Louis, P. Goret, C. De Marzo, Christian Tamburini, A. J. Noble, R. Bruijn, J. F. Drogou, T. Spona, F. Feinstein, J. Hößl, L. R. Sulak, M. Naumann-Godo, A. S. Cussatlegras, P. Piattelli, D. Zaborov, A. Kruijer, T. Montaruli, P. Chauchot, G. Loaec, J. Zúñiga, Anne Deschamps, S. Galeotti, Alain Mazure, J. Hogenbirk, Emanuele Castorina, C. Hoffman, G. Riccobene, D. Denans, F. Ameli, Vincenzo Cavasinni, C. Distefano, M. Billault, Y. Le Guen, M. Bazzotti, H. Kok, S. Basa, Eric Delagnes, J.-C. Languillat, M. Ripani, Jean-Francois Rolin, E. Carmona, Antoine Kouchner, G. Terreni, Dominique Durand, S. Cecchini, E. Heine, R. van Wijk, M. Morganti, Kay Graf, P. Coyle, Jean-Paul Kneib, Gisela Anton, T. Stolarczyk, C. Racca, J.-Y. Coail, Marc Régnier, S. Favard, A. Calzas, L. Moscoso, Rezo Shanidze, Antonio Capone, N. Girard, Maurizio Spurio, J. Roux, G. Venekamp, P. Kooijman, M. Jaspers, B. Verlaat, Yann Hello, P. Keller, G. van der Steenhoven, F. Mazéas, M. Anghinolfi, G. F. Burgio, J. Busto, P. Rewiersma, M. Mongelli, E. Migneco, F. Druillole, N. de Botton, High Energy Astrophys. & Astropart. Phys (API, FNWI), ANTARES (IHEF, IoP, FNWI), M. AGERON, J.A. AGUILAR, A. ALBERT, F. AMELI, M. ANGHINOLFI, G. ANTON, S. ANVAR, F. ARDELLIER-DESAGES, E. ASLANIDES, J-J. AUBERT, R. AUER, E. BARBARITO, S. BASA, M. BATTAGLIERI, M. BAZZOTTI, Y. BECHERINI, N. BETHOUX, J. BELTRAMELLI, V. BERTIN, A. BIGI, M. BILLAULT, R. BLAES, N. DE BOTTON, M.C. BOUWHUIS, R. BRUIJN, J. BRUNNER, G.F. BURGIO, J. BUSTO, F. CAFAGNA, L. CAILLAT, A. CALZAS, A. CAPONE, L. CAPONETTO, E. CARMONA, J. CARR, D. CASTEL, E. CASTORINA, V. CAVASINNI, S. CECCHINI, A. CERES, P. CHARVIS, P. CHAUCHOT, T. CHIARUSI, M. CIRCELLA, J-Y- COAIL, C. COLNARD, C. COMPERE, R. CONIGLIONE, N. COTTINI, P. COYLE, S. CUNEO, A-S. CUSSATLEGRAS, G. DAMY, R. VAN DANTZIG, G. DE BONIS, C. DE MARZO, R. DE VITA, I. DEKEYSER, E. DELAGNES, D. DENANS, A. DESCHAMPS, J.-X. DESSA, J-J. DESTELLE, B. DINKESPIELER, C. DISTEFANO, C. DONZAUD, J-F. DROGOU, F. DRUILLOLE, D. DURAND, J-P. ERNENWEIN, S. ESCOFFIER, E. FALCHINI, S. FAVARD, F. FEHR, F. FEINSTEIN, C. FIORELLO, V. FLAMINIO, K. FRATINI, J-L. FUDA, S. GALEOTTI, J-M. GALLONE, G. GIACOMELLI, N. GIRARD, C. GOJAK, PH. GORET, K. GRAF, G. HALLEWELL, M.N. HARAKEH, B. HARTMANN, A. HEIJBOER, E. HEINE, Y. HELLO, J.J. HERNANDEZ-REY, J. HOSSL, C. HOFFMAN, J. HOGENBIRK, J.R. HUBBARD, M. JAQUET, M. JASPERS, M. DE JONG, F. JOUVENOT, N. KALANTAR-NAYESTANAKI, A. KAPPES, T. KARG, U. KATZ, P. KELLER, J. P. KNEIB, E. KOK, H. KOK, P. KOOIJMAN, C. KOPPER, A. KOUCHNER, W. KRETSCHMER, A. KRUIJER, S. KUCH, P. LAGIER, R. LAHMANN, G. LAMANNA, P. LAMARE, G. LAMBARD, J-C. LANGUILLAT, H. LASCHINSKY, J. LAVALLE, Y. LE GUEN, H.LE PROVOST, A. LE VAN SUU, D. LEFEVRE, T. LEGOU, G. LELAIZANT, G. LIM, D.LO PRESTI, G. LOAEC, H. LOEHNER, S. LOUCATOS, F. LOUIS, F. LUCARELLI, V. LYASHUK, S. MANGANO, M. MARCELIN, A. MARGIOTTA, R. MASULLO, F. MAZEAS, A. MAZURE, R. MEGNA, M. MELISSAS, E. MIGNECO, M. MONGELLI, T. MONTARULI, M. MORGANTI, L. MOSCOSO, H. MOTZ, M. MUSUMECI, M. NAUMANN-GODO, C. NAUMANN, V. NIESS, T. NOBLE, C. OLIVETTO, R. OSTASCH, N. PALANQUE-DELABROUILLE, P. PAYRE, H. PEEK, A. PEREZ, C. PETTA, P. PIATTELLI, R. PILLET, J-P. PINEAU, J. POINSIGNON, V. POPA, T. PRADIER, C. RACCA, N. RANDAZZO, J. VAN RANDWIJK, D. REAL, M. REGNIER, B. VAN RENS, F. RETHORE, P. REWIERSMA, G. RICCOBENE, V. RIGAUD, M. RIPANI, V. ROCA, C. RODA, J.F. ROLIN, A. ROSTOVTSEV, J. ROUX, M. RUPPI, G.V. RUSSO, G. RUSYDI, F. SALESA, K. SALOMON, P. SAPIENZA, F. SCHMITT, J-P. SCHULLER, R. SHANIDZE, I. SOKALSKI, T. SPONA, M. SPURIO, G. VAN DER STEENHOVEN, T. STOLARCZYK, K. STREEB, L. SULAK, M. TAIUTI, C. TAMBURINI, C. TAO, L. TASCA, G. TERRENI, F. URBANO, P. VALDY, V. VALENTE, B. VALLAGE, G. VAUDAINE, G. VENEKAMP, B. VERLAAT, P. VERNIN, R. VAN WIJK, G. WIJNKER, G. WOBBE, E. DE WOLF, A-F. YAO, D. ZABOROV, H. ZACCONE, J.D. ZORNOZA, J. ZUNIGA, Centre de Physique des Particules de Marseille (CPPM), Aix Marseille Université (AMU)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Département d'Astrophysique, de physique des Particules, de physique Nucléaire et de l'Instrumentation Associée (DAPNIA), Commissariat à l'énergie atomique et aux énergies alternatives (CEA), Laboratoire d'Astrophysique de Marseille (LAM), Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS), Institut Pluridisciplinaire Hubert Curien (IPHC), Université Louis Pasteur - Strasbourg I-Centre National de la Recherche Scientifique (CNRS), APC - Astrophysique des Hautes Energies (APC - AHE), AstroParticule et Cosmologie (APC (UMR_7164)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Alma Mater Studiorum Università di Bologna [Bologna] (UNIBO), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), ANTARES, Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Aix Marseille Université (AMU), Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Aix Marseille Université (AMU)-Centre National d'Études Spatiales [Toulouse] (CNES), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Dipartimento di Astronomia, Universita degli Studi di Bologna, Università di Bologna [Bologna] (UNIBO)-Università di Bologna [Bologna] (UNIBO), PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Dipartimento di Astronomia, Universita degli Studi di Bologna, Alma Mater Studiorum Università di Bologna [Bologna] (UNIBO)-Alma Mater Studiorum Università di Bologna [Bologna] (UNIBO), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), KVI - Center for Advanced Radiation Technology, and Research unit Nuclear & Hadron Physics
Subjects: leak detection, Nuclear and High Energy Physics, Acoustics, ELECTROMECHANICAL CABLES, Full scale, electromechanical cable, 01 natural sciences, Optics, Data acquisition, Data logger, 0103 physical sciences, [PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex], optical time domain reflectometry, 14. Life underwater, Time domain, Electronics, sea deployment, 010306 general physics, Reflectometry, Instrumentation, Astroparticle physics, Physics, ANTARES, Hydrophone, antares, underwater neutrino telescope, 010308 nuclear & particles physics, business.industry, ANTARES, underwater neutrino telescope, leak detection, optical time domain reflectometry, electromechanical cable, sea deployment, UNDERWATER NEUTRINO TELESCOPES, 29.40.Ka, 29.90.+r, 92.10.Vz, business
Abstract: full-scale mechanical prototype line was deployed to a depth of 2500 m to test the leak tightness of the electronics containers and the pressure-resistant properties of an electromechanical cable under evaluation for use in the ANTARES deep-sea neutrino telescope. During a month-long immersion study, line parameter data were taken using miniature autonomous data loggers and shore-based optical time domain reflectometry. Details of the mechanical prototype line, the electromechanical cable and data acquisition are presented. Data taken during the immersion study revealed deficiencies in the pressure resistance of the electromechanical cable terminations at the entry points to the electronics containers. The improvements to the termination, which have been integrated into subsequent detection lines, are discussed. The line also allowed deep-sea acoustic measurements with a prototype hydrophone system. The technical setup of this system is described, and the first results of the data analysis are presented. (c) 2007 Elsevier B.V. All rights reserved.
Published: 2007
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9. Identifying clouds over the Pierre Auger Observatory using infrared satellite data

Author: M. Zavrtanik, N. Nierstenhoefer, R. Dallier, F. Salamida, J. F. Valdés Galicia, K. H. Becker, I. De Mitri, A. Gascon Bravo, A. Saftoiu, D. Garcia-Gamez, S. T. Garcia Roca, B. Gookin, D. Melo, David Walz, D. Pakk Selmi-Dei, R. Sato, M. Niechciol, D. B. Tridapalli, A. Segreto, A.M. van den Berg, Darko Veberič, I. Rodriguez Cabo, B. Sarkar, J. L. Navarro, M. Videla, J. C. Diaz, M. A. Leigui de Oliveira, R. Tcaciuc, F. Montanet, J. C. dos Anjos, Petr Schovanek, D. Maurizio, J. C. Moreno, C. Aramo, Lorenzo Caccianiga, Y. Guardincerri, G. Müller, J.M. Chirinos, B. Rouillé-D'Orfeuil, Bruno Daniel, Pham Ngoc Diep, D. Garcia-Pinto, Radomir Smida, T. Yapici, J. J. Masías Meza, R. Gaior, S. H. Cheng, Heino Falcke, B. Tome, L. Buroker, J. Knapp, R. Bonino, J. Vicha, G. Wieczorek, A. Lopez Agüera, F. Diogo, F. Suarez, Sergio Dasso, T. Niggemann, R. M. de Almeida, P. Allison, A. Tapia, G. Cocciolo, H. Gemmeke, C. Rühle, V. de Souza, M. Unger, H. Wahlberg, L. Nellen, B. Zamorano Garcia, M. Buscemi, N. Scharf, V. Pirronello, F. Guarino, John Matthews, Peter Buchholz, M. S. A. B. Leão, C. Macolino, C. Hojvat, C. Morello, K. D. de Vries, D. Nosek, T. Yamamoto, R. M. Kieckhafer, C. Jarne, M. Tueros, J. Rautenberg, B. Revenu, Jan Ebr, M. Melissas, O. Wainberg, I.M. Brancus, D. Huber, S. Westerhoff, H. Glass, Marco Aglietta, W. C. Brown, A. Nelles, Jaime Alvarez-Muñiz, D. Schuster, M. A. Muller, Lu Lu, G. Marsella, D. Martraire, S. Gambetta, Peter L. Biermann, D. Harari, Alessandro Petrolini, B. Mitrica, M. Ludwig, J. Rosado, A. van Vliet, A. Tonachini, L. Nožka, A. Weindl, N. Hollon, V. Verzi, P. Brogueira, M. Urban, A. C. Rovero, C. Bleve, B. Keilhauer, V. H. Ponce, S. J. Sciutto, J. Schovancova, Paolo Privitera, L. Perrone, Jiri Chudoba, D. Torres Machado, H.O. Klages, G. Torralba Elipe, D. Kruppke-Hansen, B. Wundheiler, R. Krause, Gregory R Snow, Alina Mihaela Badescu, M. Oliveira, M. Ave, E. Trovato, J. Lozano Bahilo, Segev BenZvi, Corbin Covault, Maria-Teresa Dova, M. Gómez Berisso, R. C. Shellard, Azadeh Keivani, A. P. Ferguson, R. Alves Batista, C. Baus, A. Aminaei, Y. Petrov, J. Gitto, P. Hansen, A. Chiavassa, A. E. Herve, Lino Miramonti, Vincenzo Rizi, M. D. Rodríguez-Frías, Paul Sommers, R. Cester, B. J. Whelan, P. Gouffon, W. Rodrigues de Carvalho, M. Risse, D. Martello, M. Ziolkowski, O. Martínez Bravo, P. N. Dong, M. J. Cooper, F. Sánchez, M. Ambrosio, M. De Domenico, Jing Zhou, G. Toma, S. Mićanović, B. M. Baughman, L. R. Wiencke, T. A. Harrison, A. Porcelli, M. Tartare, J. W. Cronin, B. D. Fox, N. T. Thao, G. Parente, A. Gorgi, V. Marin, J. Espadanal, M. Palatka, P. W. Younk, A. Śmiałkowski, P. Pieroni, Peter Schiffer, V. Scherini, Nataliia Borodai, H. R. Marquez Falcon, Alejandro Almela, S. van Velzen, E. Menichetti, G. Matthiae, G. Varner, H. Spinka, Antonio Bueno, Sergio Pastor, I. M. Pepe, J. Oehlschläger, A. F. Barbosa, Maria Rita Coluccia, Miguel Mostafá, Dusan Mandat, Gualberto Avila, Ingomar Allekotte, Angela V. Olinto, M. Monasor, F. Arqueros, P. Necesal, P. Gonçalves, N. Palmieri, Markus Ahlers, J. K. Kulbartz, H. Rivera, E. Varela, N. Griffith, J. A.J. Matthews, Xavier Bertou, R. E. Burton, S. Jiraskova, T. Rossler, J. D. Swain, A. Menshikov, J. C. Marin, H. Schieler, A. Zepeda, R. Ulrich, Karl-Heinz Kampert, Antonella Castellina, E. M. Santos, Pedro Assis, A. Etchegoyen, K. Kadija, Carola Dobrigkeit, A. Insolia, M. Kleifges, D. Zavrtanik, I. Katkov, Javier Tiffenberg, J. Allen, E. Mayotte, R. Mussa, J. J. Beatty, P. Wahrlich, K. Louedec, J. Pȩkala, Mariangela Settimo, Iván Sidelnik, Alexey Yushkov, H. Dembinski, N. Fazzini, K. Weidenhaupt, J. Kleinfeller, Jose Chinellato, Alan Watson, M. I. Micheletti, T. Huege, A. Parra, S. J. De Jong, I. Zaw, O. Fratu, H. Cook, Jeffrey Brack, Olaf Scholten, P. Lautridou, M. Avenier, D. Thomas, Bruce R. Dawson, Y. N. Srivastava, Humberto Ibarguen Salazar, T. Hebbeker, Julien Aublin, A. Widom, D. LaHurd, F. Werner, P.O. Mazur, J. Alvarez Castillo, F. Sarazin, Elton J. G. Santos, K. Link, M. Prouza, Piotr Homola, P. Facal San Luis, Rúben Conceição, P. Abreu, M. Josebachuili, D. Ravignani, Miroslav Hrabovský, Daniel Kuempel, Carlos Escobar, R. F. Gamarra, A. Haungs, J. Neuser, J. R. T. de Mello Neto, E. J. Ahn, A. Letessier-Selvon, L. Molina-Bueno, E. Kemp, S. Le Coz, Luis A. Anchordoqui, J. L. Harton, D. Monnier Ragaigne, Lorenzo Cazon, S. Maldera, C. Pfendner, I. A. Minaya, A. Bellétoile, A. Schmidt, H. Martinez, O. Krömer, P. Mantsch, Z. Szadkowski, Ivone F. M. Albuquerque, Ke Fang, N. Pacheco, Lukas Middendorf, M. Platino, G. Navarra, J. Bäuml, C. E. Santo, Francisco J. Blanco, Johannes Schulz, G. Golup, N. Kunka, F. Gomez Albarracin, M. Pimenta, C. A. Moura, Brian Fick, H. Blümer, Balázs Kégl, Moritz Münchmeyer, G. Rodriguez Fernandez, A. D. Supanitsky, Hernán Asorey, Christopher B. Williams, G. C. Hill, M. Zimbres Silva, T. Šuša, I. C. Mariş, Ralph Engel, M. Plum, E. Petermann, D. Nitz, J. Stapleton, Miroslav Pech, J. Ridky, M. L. Díaz Castro, G. Farrar, S. Fliescher, A. Stutz, Pavel Horvath, Kai Daumiller, M. S. Sutherland, Rémi Bardenet, Petr Travnicek, P. Lebrun, L. Tomankova, Trent D. Grubb, Sofia Andringa, R. Meyhandan, M. Ortiz, R. J. Lauer, Juan Manuel Figueira, Roberta Colalillo, P. Ristori, A. G. Mariazzi, S. Jansen, B. García, Mario Scuderi, S. Messina, G. Salina, A. Curutiu, Tobias Winchen, R. López, Karen S. Caballero-Mora, Olivier Deligny, B. Caccianiga, S. Stanič, H. Schoorlemmer, P.F. Gómez Vitale, Martina Bohacova, Martin Erdmann, A. Dorofeev, Guenter Sigl, J. Sorokin, M. Blanco, C. E. Fracchiolla, Roger W Clay, D. D'Urso, L. Latronico, Corinne Berat, M. Giller, S. Navas, G. P. Guedes, K. B. Barber, M. Weber, U. Fröhlich, R. A. Vázquez, L. Valore, P. Karhan, P. A. Kasper, A. Filipčič, M. Straub, D. Maurel, Markus Roth, A. Shadkam, C. Timmermans, S. Petrera, J. R. Vázquez, A. F. Grillo, Juan Carlos D'Olivo, T. Pierog, J. Maller, Rossella Caruso, W. J. M. de Mello, A. Lucero, G. La Rosa, P. L. Ghia, Octavian Sima, J. G. Gonzalez, V. C. Holmes, D. Lebrun, R. Pesce, Jörg R. Hörandel, F. Salesa Greus, G. Cataldi, G. Garilli, D. Heck, L. Villaseñor, L. Martin, I. Lhenry-Yvon, S. Mollerach, E. Roulet, Marco Cilmo, B. Wilczyńska, W. Docters, Peter Gorham, R. Pelayo, L. Collica, S. Querchfeld, J. L. Kelley, E. D. Fraenkel, S. J. Saffi, L. Niemietz, L. del Peral, J. Roberts, O. Ravel, R. Piegaia, J. Rodriguez Martino, H. J. Mathes, G. De La Vega, O. Taşcǎu, J. Rodriguez Rojo, M. Szuba, F.G. Schröder, Enrique Zas, C. Di Giulio, Fernando Contreras, L. Caramete, M. Will, W. Tkaczyk, G. Yuan, S. Riggi, T. Antičić, J. Stasielak, S. Coutu, M. Lauscher, M. Pontz, A. C. Fauth, M. Stephan, H. Lyberis, Carla Bonifazi, Jose A. Bellido, B. Morales, Denise Boncioli, German Ros, B. Vargas Cárdenas, Maria Concetta Maccarone, T. Suomijärvi, J. Pallotta, E. J. Quel, Béatrice Fuchs, Niraj Dhital, I. Valiño, A. Filevich, P. T. Nhung, S. Grebe, R. Squartini, T. Paul, G. Medina-Tanco, G. van Aar, A. Criss, C. J. Todero Peixoto, M. Malacari, Yunrong Zhu, N. Krohm, Christian Glaser, H. Wilczyński, P. Billoir, Laboratoire SUBATECH Nantes (SUBATECH), Mines Nantes (Mines Nantes)-Université de Nantes (UN)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Unité Scientifique de la Station de Nançay (USN), Observatoire des Sciences de l'Univers en région Centre (OSUC), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de l'Accélérateur Linéaire (LAL), Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de Physique Nucléaire et de Hautes Énergies (LPNHE), Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Centre National de la Recherche Scientifique (CNRS), Institut de Physique Nucléaire d'Orsay (IPNO), PIERRE AUGER, Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université de Nantes (UN)-Mines Nantes (Mines Nantes), Centre National de la Recherche Scientifique (CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire des Sciences de l'Univers en région Centre (OSUC), Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Université d'Orléans (UO)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Université d'Orléans (UO)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université d'Orléans (UO), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), Centre National de la Recherche Scientifique (CNRS)-Université Paris Diderot - Paris 7 (UPD7)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Pierre et Marie Curie - Paris 6 (UPMC), Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Joseph Fourier - Grenoble 1 (UJF)-Centre National de la Recherche Scientifique (CNRS), Research unit Astroparticle Physics, P., Abreu, M., Aglietta, M., Ahler, E. J., Ahn, I. F. M., Albuquerque, I., Allekotte, J., Allen, P., Allison, A., Almela, J., Alvarez Castillo, J., Alvarez Muñiz, R., Alves Batista, M., Ambrosio, A., Aminaei, L., Anchordoqui, S., Andringa, T., Antičić, C., Aramo, F., Arquero, H., Asorey, P., Assi, J., Aublin, M., Ave, M., Avenier, G., Avila, A. M., Badescu, K. B., Barber, A. F., Barbosa, R., Bardenet, B., Baughman, J., Bäuml, C., Bau, J. J., Beatty, K. H., Becker, A., Bellétoile, J. A., Bellido, S., Benzvi, C., Berat, X., Bertou, P. L., Biermann, P., Billoir, F., Blanco, M., Blanco, Bleve, Carla, H., Blümer, M., Boháčová, D., Boncioli, C., Bonifazi, R., Bonino, N., Borodai, J., Brack, I., Brancu, P., Brogueira, W. C., Brown, P., Buchholz, A., Bueno, L., Buroker, R. E., Burton, M., Buscemi, K. S., Caballero Mora, B., Caccianiga, L., Caccianiga, L., Caramete, R., Caruso, A., Castellina, G., Cataldi, L., Cazon, R., Cester, S. H., Cheng, A., Chiavassa, J. A., Chinellato, J., Chirino, J., Chudoba, M., Cilmo, R. W., Clay, Cocciolo, Giuseppe, R., Colalillo, L., Collica, Coluccia, MARIA RITA, R., Conceição, F., Contrera, H., Cook, M. J., Cooper, S., Coutu, C. E., Covault, A., Cri, J., Cronin, A., Curutiu, R., Dallier, B., Daniel, S., Dasso, K., Daumiller, B. R., Dawson, R. M., de Almeida, M., De Domenico, S. J., de Jong, G., De La Vega, W. J. M., de Mello, J. R. T., de Mello Neto, DE MITRI, Ivan, V., de Souza, K. D., de Vrie, L., del Peral, O., Deligny, H., Dembinski, N., Dhital, C., Di Giulio, J. C., Diaz, M. L., Díaz Castro, P. N., Diep, F., Diogo, C., Dobrigkeit, W., Docter, J. C., D’Olivo, P. N., Dong, A., Dorofeev, J. C., dos Anjo, M. T., Dova, D., D’Urso, J., Ebr, R., Engel, M., Erdmann, C. O., Escobar, J., Espadanal, A., Etchegoyen, P., Facal San Lui, H., Falcke, K., Fang, G., Farrar, A. C., Fauth, N., Fazzini, A. P., Ferguson, B., Fick, J. M., Figueira, A., Filevich, A., Filipčič, S., Fliescher, B. D., Fox, C. E., Fracchiolla, E. D., Fraenkel, O., Fratu, U., Fröhlich, B., Fuch, R., Gaior, R. F., Gamarra, S., Gambetta, B., García, S. T., Garcia Roca, D., Garcia Gamez, D., Garcia Pinto, G., Garilli, A., Gascon Bravo, H., Gemmeke, P. L., Ghia, M., Giller, J., Gitto, C., Glaser, H., Gla, G., Golup, F., Gomez Albarracin, M., Gómez Berisso, P. F., Gómez Vitale, P., Gonçalve, J. G., Gonzalez, B., Gookin, A., Gorgi, P., Gorham, P., Gouffon, S., Grebe, N., Griffith, A. F., Grillo, T. D., Grubb, Y., Guardincerri, F., Guarino, G. P., Guede, P., Hansen, D., Harari, T. A., Harrison, J. L., Harton, A., Haung, T., Hebbeker, D., Heck, A. E., Herve, G. C., Hill, C., Hojvat, N., Hollon, V. C., Holme, P., Homola, J. R., Hörandel, P., Horvath, M., Hrabovský, D., Huber, T., Huege, A., Insolia, S., Jansen, C., Jarne, S., Jiraskova, M., Josebachuili, K., Kadija, K. H., Kampert, P., Karhan, P., Kasper, I., Katkov, B., Kégl, B., Keilhauer, A., Keivani, J. L., Kelley, E., Kemp, R. M., Kieckhafer, H. O., Klage, M., Kleifge, J., Kleinfeller, J., Knapp, R., Krause, N., Krohm, O., Krömer, D., Kruppke Hansen, D., Kuempel, J. K., Kulbartz, N., Kunka, G., La Rosa, D., Lahurd, L., Latronico, R., Lauer, M., Lauscher, P., Lautridou, S., Le Coz, M. S. A. B., Leão, D., Lebrun, P., Lebrun, M. A., Leigui de Oliveira, A., Letessier Selvon, I., Lhenry Yvon, K., Link, R., López, A., Lopez Agüera, K., Louedec, J., Lozano Bahilo, L., Lu, A., Lucero, M., Ludwig, H., Lyberi, M. C., Maccarone, C., Macolino, M., Malacari, S., Maldera, J., Maller, D., Mandat, P., Mantsch, A. G., Mariazzi, J., Marin, V., Marin, I. C., Mariş, H. R., Marquez Falcon, Marsella, Giovanni, Martello, Daniele, L., Martin, H., Martinez, O., Martínez Bravo, D., Martraire, J. J., Masías Meza, H. J., Mathe, J., Matthew, J. A. J., Matthew, G., Matthiae, D., Maurel, D., Maurizio, E., Mayotte, P. O., Mazur, G., Medina Tanco, M., Melissa, D., Melo, E., Menichetti, A., Menshikov, S., Messina, R., Meyhandan, S., Mićanović, M. I., Micheletti, L., Middendorf, I. A., Minaya, L., Miramonti, B., Mitrica, L., Molina Bueno, S., Mollerach, M., Monasor, D., Monnier Ragaigne, F., Montanet, B., Morale, C., Morello, J. C., Moreno, M., Mostafá, C. A., Moura, M. A., Muller, G., Müller, M., Münchmeyer, R., Mussa, G., Navarra, J. L., Navarro, S., Nava, P., Necesal, L., Nellen, A., Nelle, J., Neuser, P. T., Nhung, M., Niechciol, L., Niemietz, N., Nierstenhoefer, T., Niggemann, D., Nitz, D., Nosek, L., Nožka, J., Oehlschläger, A., Olinto, M., Oliveira, M., Ortiz, N., Pacheco, D., Pakk Selmi Dei, M., Palatka, J., Pallotta, N., Palmieri, G., Parente, A., Parra, S., Pastor, T., Paul, M., Pech, J., Pe¸kala, R., Pelayo, I. M., Pepe, Perrone, Lorenzo, R., Pesce, E., Petermann, S., Petrera, A., Petrolini, Y., Petrov, C., Pfendner, R., Piegaia, T., Pierog, P., Pieroni, M., Pimenta, V., Pirronello, M., Platino, M., Plum, V. H., Ponce, M., Pontz, A., Porcelli, P., Privitera, M., Prouza, E. J., Quel, S., Querchfeld, J., Rautenberg, O., Ravel, D., Ravignani, B., Revenu, J., Ridky, S., Riggi, M., Risse, P., Ristori, H., Rivera, V., Rizi, J., Robert, W., Rodrigues de Carvalho, I., Rodriguez Cabo, G., Rodriguez Fernandez, J., Rodriguez Martino, J., Rodriguez Rojo, M. D., Rodríguez Fría, G., Ro, J., Rosado, T., Rossler, M., Roth, B., Rouillé d’Orfeuil, E., Roulet, A. C., Rovero, C., Rühle, S. J., Saffi, A., Saftoiu, F., Salamida, H., Salazar, F., Salesa Greu, G., Salina, F., Sánchez, C. E., Santo, E., Santo, E. M., Santo, F., Sarazin, B., Sarkar, R., Sato, N., Scharf, Scherini, Viviana, H., Schieler, P., Schiffer, A., Schmidt, O., Scholten, H., Schoorlemmer, J., Schovancova, P., Schovánek, F. G., Schröder, J., Schulz, D., Schuster, S. J., Sciutto, M., Scuderi, A., Segreto, M., Settimo, A., Shadkam, R. C., Shellard, I., Sidelnik, G., Sigl, O., Sima, A., Śmiałkowski, R., Šmída, G. R., Snow, P., Sommer, J., Sorokin, H., Spinka, R., Squartini, Y. N., Srivastava, S., Stanič, J., Stapleton, J., Stasielak, M., Stephan, M., Straub, A., Stutz, F., Suarez, T., Suomijärvi, A. D., Supanitsky, T., Šuša, M. S., Sutherland, J., Swain, Z., Szadkowski, M., Szuba, A., Tapia, M., Tartare, O., Taşcău, R., Tcaciuc, N. T., Thao, D., Thoma, J., Tiffenberg, C., Timmerman, W., Tkaczyk, C. J., Todero Peixoto, G., Toma, L., Tomankova, B., Tomé, A., Tonachini, G., Torralba Elipe, D., Torres Machado, P., Travnicek, D. B., Tridapalli, E., Trovato, M., Tuero, R., Ulrich, M., Unger, M., Urban, J. F., Valdés Galicia, I., Valiño, L., Valore, G., van Aar, A. M., van den Berg, S., van Velzen, A., van Vliet, E., Varela, B., Vargas Cárdena, G., Varner, J. R., Vázquez, R. A., Vázquez, D., Veberič, V., Verzi, J., Vicha, M., Videla, L., Villaseñor, H., Wahlberg, P., Wahrlich, O., Wainberg, D., Walz, A. A., Watson, M., Weber, K., Weidenhaupt, A., Weindl, F., Werner, S., Westerhoff, B. J., Whelan, A., Widom, G., Wieczorek, L., Wiencke, B., Wilczyńska, H., Wilczyński, M., Will, C., William, T., Winchen, B., Wundheiler, T., Yamamoto, T., Yapici, P., Younk, G., Yuan, A., Yushkov, B., Zamorano Garcia, E., Za, D., Zavrtanik, M., Zavrtanik, I., Zaw, A., Zepeda, J., Zhou, Y., Zhu, M., Zimbres Silva, M., Ziolkowski, P. Abreu, M. Aglietta, M. Ahler, E.J. Ahn, I.F.M. Albuquerque, I. Allekotte, J. Allen, P. Allison, A. Almela, J. Alvarez Castillo, J. Alvarez-Muñiz, R. Alves Batista, M. Ambrosio, A. Aminaei, L. Anchordoqui, S. Andringa, T. Antičić, C. Aramo, F. Arquero, H. Asorey, P. Assi, J. Aublin, M. Ave, M. Avenier, G. Avila, A.M. Badescu, K.B. Barber, A.F. Barbosa, R. Bardenet, B. Baughman, J. Bäuml, C. Bau, J.J. Beatty, K.H. Becker, A. Bellétoile, J.A. Bellido, S. BenZvi, C. Berat, X. Bertou, P.L. Biermann, P. Billoir, F. Blanco, M. Blanco, C. Bleve, H. Blümer, M. Boháčová, D. Boncioli, C. Bonifazi, R. Bonino, N. Borodai, J. Brack, I. Brancu, P. Brogueira, W.C. Brown, P. Buchholz, A. Bueno, L. Buroker, R.E. Burton, M. Buscemi, K.S. Caballero-Mora, B. Caccianiga, L. Caccianiga, L. Caramete, R. Caruso, A. Castellina, G. Cataldi, L. Cazon, R. Cester, S.H. Cheng, A. Chiavassa, J.A. Chinellato, J. Chirino, J. Chudoba, M. Cilmo, R.W. Clay, G. Cocciolo, R. Colalillo, L. Collica, M.R. Coluccia, R. Conceição, F. Contrera, H. Cook, M.J. Cooper, S. Coutu, C.E. Covault, A. Cri, J. Cronin, A. Curutiu, R. Dallier, B. Daniel, S. Dasso, K. Daumiller, B.R. Dawson, R.M. de Almeida, M. De Domenico, S.J. de Jong, G. De La Vega, W.J.M. de Mello, J.R.T. de Mello Neto, I. De Mitri, V. de Souza, K.D. de Vrie, L. del Peral, O. Deligny, H. Dembinski, N. Dhital, C. Di Giulio, J.C. Diaz, M.L. Díaz Castro, P.N. Diep, F. Diogo, C. Dobrigkeit, W. Docter, J.C. D’Olivo, P.N. Dong, A. Dorofeev, J.C. dos Anjo, M.T. Dova, D. D’Urso, J. Ebr, R. Engel, M. Erdmann, C.O. Escobar, J. Espadanal, A. Etchegoyen, P. Facal San Lui, H. Falcke, K. Fang, G. Farrar, A.C. Fauth, N. Fazzini, A.P. Ferguson, B. Fick, J.M. Figueira, A. Filevich, A. Filipčič, S. Fliescher, B.D. Fox, C.E. Fracchiolla, E.D. Fraenkel, O. Fratu, U. Fröhlich, B. Fuch, R. Gaior, R.F. Gamarra, S. Gambetta, B. García, S.T. Garcia Roca, D. Garcia-Gamez, D. Garcia-Pinto, G. Garilli, A. Gascon Bravo, H. Gemmeke, P.L. Ghia, M. Giller, J. Gitto, C. Glaser, H. Gla, G. Golup, F. Gomez Albarracin, M. Gómez Berisso, P.F. Gómez Vitale, P. Gonçalve, J.G. Gonzalez, B. Gookin, A. Gorgi, P. Gorham, P. Gouffon, S. Grebe, N. Griffith, A.F. Grillo, T.D. Grubb, Y. Guardincerri, F. Guarino, G.P. Guede, P. Hansen, D. Harari, T.A. Harrison, J.L. Harton, A. Haung, T. Hebbeker, D. Heck, A.E. Herve, G.C. Hill, C. Hojvat, N. Hollon, V.C. Holme, P. Homola, J.R. Hörandel, P. Horvath, M. Hrabovský, D. Huber, T. Huege, A. Insolia, S. Jansen, C. Jarne, S. Jiraskova, M. Josebachuili, K. Kadija, K.H. Kampert, P. Karhan, P. Kasper, I. Katkov, B. Kégl, B. Keilhauer, A. Keivani, J.L. Kelley, E. Kemp, R.M. Kieckhafer, H.O. Klage, M. Kleifge, J. Kleinfeller, J. Knapp, R. Krause, N. Krohm, O. Krömer, D. Kruppke-Hansen, D. Kuempel, J.K. Kulbartz, N. Kunka, G. La Rosa, D. LaHurd, L. Latronico, R. Lauer, M. Lauscher, P. Lautridou, S. Le Coz, M.S.A.B. Leão, D. Lebrun, P. Lebrun, M.A. Leigui de Oliveira, A. Letessier-Selvon, I. Lhenry-Yvon, K. Link, R. López, A. Lopez Agüera, K. Louedec, J. Lozano Bahilo, L. Lu, A. Lucero, M. Ludwig, H. Lyberi, M.C. Maccarone, C. Macolino, M. Malacari, S. Maldera, J. Maller, D. Mandat, P. Mantsch, A.G. Mariazzi, J. Marin, V. Marin, I.C. Mariş, H.R. Marquez Falcon, G. Marsella, D. Martello, L. Martin, H. Martinez, O. Martínez Bravo, D. Martraire, J.J. Masías Meza, H.J. Mathe, J. Matthew, J.A.J. Matthew, G. Matthiae, D. Maurel, D. Maurizio, E. Mayotte, P.O. Mazur, G. Medina-Tanco, M. Melissa, D. Melo, E. Menichetti, A. Menshikov, S. Messina, R. Meyhandan, S. Mićanović, M.I. Micheletti, L. Middendorf, I.A. Minaya, L. Miramonti, B. Mitrica, L. Molina-Bueno, S. Mollerach, M. Monasor, D. Monnier Ragaigne, F. Montanet, B. Morale, C. Morello, J.C. Moreno, M. Mostafá, C.A. Moura, M.A. Muller, G. Müller, M. Münchmeyer, R. Mussa, G. Navarra, J.L. Navarro, S. Nava, P. Necesal, L. Nellen, A. Nelle, J. Neuser, P.T. Nhung, M. Niechciol, L. Niemietz, N. Nierstenhoefer, T. Niggemann, D. Nitz, D. Nosek, L. Nožka, J. Oehlschläger, A. Olinto, M. Oliveira, M. Ortiz, N. Pacheco, D. Pakk Selmi-Dei, M. Palatka, J. Pallotta, N. Palmieri, G. Parente, A. Parra, S. Pastor, T. Paul, M. Pech, J. Pe¸kala, R. Pelayo, I.M. Pepe, L. Perrone, R. Pesce, E. Petermann, S. Petrera, A. Petrolini, Y. Petrov, C. Pfendner, R. Piegaia, T. Pierog, P. Pieroni, M. Pimenta, V. Pirronello, M. Platino, M. Plum, V.H. Ponce, M. Pontz, A. Porcelli, P. Privitera, M. Prouza, E.J. Quel, S. Querchfeld, J. Rautenberg, O. Ravel, D. Ravignani, B. Revenu, J. Ridky, S. Riggi, M. Risse, P. Ristori, H. Rivera, V. Rizi, J. Robert, W. Rodrigues de Carvalho, I. Rodriguez Cabo, G. Rodriguez Fernandez, J. Rodriguez Martino, J. Rodriguez Rojo, M.D. Rodríguez-Fría, G. Ro, J. Rosado, T. Rossler, M. Roth, B. Rouillé-d’Orfeuil, E. Roulet, A.C. Rovero, C. Rühle, S.J. Saffi, A. Saftoiu, F. Salamida, H. Salazar, F. Salesa Greu, G. Salina, F. Sánchez, C.E. Santo, E. Santo, E.M. Santo, F. Sarazin, B. Sarkar, R. Sato, N. Scharf, V. Scherini, H. Schieler, P. Schiffer, A. Schmidt, O. Scholten, H. Schoorlemmer, J. Schovancova, P. Schovánek, F.G. Schröder, J. Schulz, D. Schuster, S.J. Sciutto, M. Scuderi, A. Segreto, M. Settimo, A. Shadkam, R.C. Shellard, I. Sidelnik, G. Sigl, O. Sima, A. Śmiałkowski, R. Šmída, G.R. Snow, P. Sommer, J. Sorokin, H. Spinka, R. Squartini, Y.N. Srivastava, S. Stanič, J. Stapleton, J. Stasielak, M. Stephan, M. Straub, A. Stutz, F. Suarez, T. Suomijärvi, A.D. Supanitsky, T. Šuša, M.S. Sutherland, J. Swain, Z. Szadkowski, M. Szuba, A. Tapia, M. Tartare, O. Taşcău, R. Tcaciuc, N.T. Thao, D. Thoma, J. Tiffenberg, C. Timmerman, W. Tkaczyk, C.J. Todero Peixoto, G. Toma, L. Tomankova, B. Tomé, A. Tonachini, G. Torralba Elipe, D. Torres Machado, P. Travnicek, D.B. Tridapalli, E. Trovato, M. Tuero, R. Ulrich, M. Unger, M. Urban, J.F. Valdés Galicia, I. Valiño, L. Valore, G. van Aar, A.M. van den Berg, S. van Velzen, A. van Vliet, E. Varela, B. Vargas Cárdena, G. Varner, J.R. Vázquez, R.A. Vázquez, D. Veberič, V. Verzi, J. Vicha, M. Videla, L. Villaseñor, H. Wahlberg, P. Wahrlich, O. Wainberg, D. Walz, A.A. Watson, M. Weber, K. Weidenhaupt, A. Weindl, F. Werner, S. Westerhoff, B.J. Whelan, A. Widom, G. Wieczorek, L. Wiencke, B. Wilczyńska, H. Wilczyński, M. Will, C. William, T. Winchen, B. Wundheiler, T. Yamamoto, T. Yapici, P. Younk, G. Yuan, A. Yushkov, B. Zamorano Garcia, E. Za, D. Zavrtanik, M. Zavrtanik, I. Zaw, A. Zepeda, J. Zhou, Y. Zhu, M. Zimbres Silva, M. Ziolkowski, J., Alvarez Mu?iz, T., Anti?i?, Aramo, Carla, J., B?uml, A., Bell?toile, C., Bleve, H., Bl?mer, M., Boh??ov?, Buscemi, Mario, Cilmo, Marco, G., Cocciolo, Colalillo, Roberta, M. R., Coluccia, R., Concei??o, I., De Mitri, M. L., D?az Castro, J. C., D?olivo, D., D'Urso, A., Filip?i?, U., Fr?hlich, B., Garc?a, M., G?mez Berisso, P. F., G?mez Vitale, P., Gon?alve, Guarino, Fausto, J. R., H?randel, M., Hrabovsk?, B., K?gl, O., Kr?mer, M. S. A. B., Le?o, R., L?pez, A., Lopez Ag?era, I. C., Mari?, G., Marsella, D., Martello, O., Mart?nez Bravo, J. J., Mas?as Meza, S., Mi?anovi?, M., Mostaf?, G., M?ller, M., M?nchmeyer, L., No?ka, J., Oehlschl?ger, J., Pe?kala, L., Perrone, M. D., Rodr?guez Fr?a, B., Rouill? d?Orfeuil, C., R?hle, F., S?nchez, V., Scherini, P., Schov?nek, F. G., Schr?der, A., ?mia?kowski, R., ?m?da, S., Stani?, T., Suomij?rvi, T., ?u?a, O., Ta?c?u, B., Tom?, J. F., Vald?s Galicia, I., Vali?o, Valore, Laura, B., Vargas C?rdena, J. R., V?zquez, R. A., V?zquez, D., Veberi?, L., Villase?or, B., Wilczy?ska, and H., Wilczy?ski
Subjects: [PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], [PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM], Atmospheric Monitoring, Satellites, Infrared, Astronomy, Cloud cover, FOS: Physical sciences, Atmospheric monitoring, 01 natural sciences, Ciencias de la Tierra y relacionadas con el Medio Ambiente, Auger, purl.org/becyt/ford/1 [https], purl.org/becyt/ford/1.5 [https], Observatory, Clouds, 0103 physical sciences, Extensive air showers, 010306 general physics, DETECTOR, Instrumentation and Methods for Astrophysics (astro-ph.IM), Image resolution, Ciencias Exactas, Physics, Pierre Auger Observatory, UHE Cosmic Rays, atmosphere, 010308 nuclear & particles physics, [SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], Física, Astronomy and Astrophysics, Ultra-high energy cosmic rays, [SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM], INFRAVERMELHO, Experimental High Energy Physics, ComputingMethodologies_DOCUMENTANDTEXTPROCESSING, Pierre Auger observatory, ultra-high energy cosmic rays, extensive air showers, atmospheric monitoring, clouds, satellites, Física nuclear, Satellite, Central Laser Facility, Extensive Air Showers, Astrophysics - Instrumentation and Methods for Astrophysics, Meteorología y Ciencias Atmosféricas, SYSTEM, CIENCIAS NATURALES Y EXACTAS
Abstract: We describe a new method of identifying night-time clouds over the Pierre Auger Observatory using infrared data from the Imager instruments on the GOES-12 and GOES-13 satellites. We compare cloud. identifications resulting from our method to those obtained by the Central Laser Facility of the Auger Observatory. Using our new method we can now develop cloud probability maps for the 3000 km(2) of the Pierre Auger Observatory twice per hour with a spatial resolution of similar to 2.4 km by similar to 5.5 km. Our method could also be applied to monitor cloud cover for other ground-based observatories and for space-based observatories. (C) 2013 Elsevier B.V. All rights reserved., The successful installation, commissioning, and operation of the Pierre Auger Observatory would not have been possible without the strong commitment and effort from the technical and adminis- trative staff in Malargüe. We are very grateful to the following agencies and organiza- tions for financial support: Comisión Nacional de Energía Atómica, Fundación Antorchas, Gobierno De La Provincia de Mendoza, Municipalidad de Malargüe, NDM Holdings and Valle Las Leñas, in gratitude for their continuing cooperation over land access, Argentina; the Australian Research Council; Conselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq), Financiadora de Estudos e Projetos (FINEP), Fundação de Amparo à Pesquisa do Estado de Rio de Janeiro (FAPERJ), Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP), Ministério de Ciência e Tecnolo- gia (MCT), Brazil; AVCR AV0Z10100502 and AV0Z10100522, GAAV KJB100100904, MSMT-CR LA08016, LG11044, MEB111003, MSM0021620859, LA08015, TACR TA01010517 and GA UK 119810, Czech Republic; Centre de Calcul IN2P3/CNRS, Centre Na- tional de la Recherche Scientifique (CNRS), Conseil Régional Ile-de- France, Département Physique Nucléaire et Corpusculaire (PNC- IN2P3/CNRS), Département Sciences de l’Univers (SDU-INSU/ CNRS), France; Bundesministerium für Bildung und Forschung (BMBF), Deutsche Forschungsgemeinschaft (DFG), Finanzministeri- um Baden-Württemberg, Helmholtz-Gemeinschaft Deutscher Forschungszentren (HGF), Ministerium für Wissenschaft und Forschung, Nordrhein-Westfalen, Ministerium für Wissenschaft, Forschung und Kunst, Baden-Württemberg, Germany; Istituto Nazionale di Fisica Nucleare (INFN), Ministero dell’Istruzione, dell’Università e della Ricerca (MIUR), Italy; Consejo Nacional de Ciencia y Tecnología (CONACYT), Mexico; Ministerie van Ond- erwijs, Cultuur en Wetenschap, Nederlandse Organisatie voor Wet- enschappelijk Onderzoek (NWO), Stichting voor Fundamenteel Onderzoek der Materie (FOM), Netherlands; Ministry of Science and Higher Education, Grant Nos. N N202 200239 and N N202 207238, Poland; Portuguese national funds and FEDER funds with- in COMPETE - Programa Operacional Factores de Competitividade through Fundação para a Ciência e a Tecnologia, Portugal; Roma- nian Authority for Scientific Research ANCS, CNDI-UEFISCDI part- nership projects nr.20/2012 and nr.194/2012, project nr.1/ ASPERA2/2012 ERA-NET and PN-II-RU-PD-2011-3-0145-17, Roma- nia; Ministry for Higher Education, Science, and Technology, Slove- nian Research Agency, Slovenia; Comunidad de Madrid, FEDER funds, Ministerio de Ciencia e Innovación and Consolider-Ingenio 2010 (CPAN), Xunta de Galicia, Spain; The Leverhulme Foundation, Science and Technology Facilities Council, United Kingdom; Department of Energy, Contract Nos. DE-AC02-07CH11359, DE- FR02-04ER41300, DE-FG02-99ER41107, National Science Founda- tion, Grant No. 0450696, The Grainger Foundation USA; NAFO- STED, Vietnam; Marie Curie-IRSES/EPLANET, European Particle Physics Latin American Network, European Union 7th Framework Program, Grant No. PIRSES-2009-GA-246806; and UNESCO. We would like to thank the former Michigan Tech students: Nathan Kelley-Hoskins, Kyle Luck and Arin Nelson for their impor- tant contribution to the development of this paper. We would like to thank NOAA for the GOES satellite data that we freely down- loaded from their website. Also, we would like to mention in these acknowledgments Dr. Steve Ackerman and Dr. Tony Schreiner for very valuable conversations
Published: 2013
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10. Lopes-3D - vectorial measurements of radio emission from cosmic ray induced air showers

Author: J. C. Arteaga-Velázquez, I.M. Brancus, A. Horneffer, T. Pierog, J. Blümer, H. Bozdog, P. Łuczak, N. Palmieri, A. Saftoiu, Andrea Chiavassa, C. Rühle, A. Weindl, Jan Kuijpers, K. Link, K. H. Kampert, A. Haungs, Claus Grupen, Markus Roth, J. A. Zensus, J. Zabierowski, A. Schmidt, O. Krömer, H. J. Mathes, M. E. Bertaina, V. de Souza, Béatrice Fuchs, P. Doll, D. Huber, J. Wochele, G. Toma, J.R. Hörandel, D. Fuhrmann, K. Bekk, H. Rebel, D. Heck, M. Ludwig, W. D. Apel, G. C. Trinchero, Octavian Sima, H. Schieler, Heino Falcke, R. Engel, J. Rautenberg, Kai Daumiller, Frank G. Schröder, D. Kang, L. Bähren, F. Di Pierro, C. Morello, Peter L. Biermann, Paula Gina Isar, H. Gemmeke, M. Melissas, Tim Huege, and J. Oehlschläger
Subjects: Physics, High Energy Astrophysical Phenomena (astro-ph.HE), LOPES, business.industry, Astronomy, Astrophysics::High Energy Astrophysical Phenomena, Measure (physics), Astrophysics::Instrumentation and Methods for Astrophysics, FOS: Physical sciences, Cosmic ray, Optics, Electric field, ComputingMethodologies_DOCUMENTANDTEXTPROCESSING, Sensitivity (control systems), business, Astrophysics - High Energy Astrophysical Phenomena
Abstract: LOPES 3D is able to measure all three components of the electric field vector of the radio emission from air showers. This allows a better comparison with emission models. The measurement of the vertical component increases the sensitivity to inclined showers. By measuring all three components of the electric field vector LOPES 3D demonstrates by how much the reconstruction accuracy of primary cosmic ray parameters increases. Thus LOPES 3D evaluates the usefulness of vectorial measurements for large scale applications., Proceedings ARENA 2012
Published: 2013

11. Cosmic ray measurements with LOPES: Status and recent results

Author: P. Łuczak, N. Palmieri, O. Krömer, M. Ludwig, Claus Grupen, A. Schmidt, H. Bozdog, M. Melissas, H. Gemmeke, J.R. Hörandel, J. Rautenberg, J. Oehlschläger, Andrea Chiavassa, V. de Souza, J. C. Arteaga-Velázquez, Kai Daumiller, F. Di Pierro, C. Morello, Heino Falcke, H. J. Mathes, A. Weindl, L. Bähren, Jan Kuijpers, C. Rühle, M. E. Bertaina, R. Engel, K. Link, Peter L. Biermann, T. Pierog, A. Haungs, Markus Roth, J. Zabierowski, H. Rebel, Octavian Sima, Béatrice Fuchs, D. Fuhrmann, H. Schieler, J. Wochele, A. Horneffer, D. Kang, D. Heck, K. H. Kampert, Tim Huege, P. Doll, J. Blümer, D. Huber, Frank G. Schröder, Paula Gina Isar, I.M. Brancus, K. Bekk, G. C. Trinchero, G. Toma, A. Saftoiu, W. D. Apel, and J. A. Zensus
Subjects: Physics, Atmosphere, Antenna array, Interferometry, LOPES, Astronomy, ComputingMethodologies_DOCUMENTANDTEXTPROCESSING, Cosmic ray, Digital radio, Energy (signal processing)
Abstract: LOPES is a digital antenna array at the Karlsruhe Institute of Technology, Germany, for cosmic-ray air-shower measurements. Triggered by the co-located KASCADE-Grande air-shower array, LOPES detects the radio emission of air showers via digital radio interferometry. We summarize the status of LOPES and recent results. In particular, we present an update on the reconstruction of the primary-particle properties based on almost 500 events above 100PeV. With LOPES, the arrival direction can be reconstructed with a precision of at least 0.65°, and the energy with a precision of at least 20%, which, however, does not include systematic uncertainties on the absolute energy scale. For many particle and astrophysics questions the reconstruction of the atmospheric depth of the shower maximum, Xmax, is important, since it yields information on the type of the primary particle and its interaction with the atmosphere. Recently, we found experimental evidence that the slope of the radio lateral distribution is indeed s...
Published: 2013

12. Revised absolute amplitude calibration of the LOPES experiment

Author: M. Melissas, J. Oehlschläger, H. Bozdog, R. Hiller, C. Rühle, O. Krömer, Heino Falcke, H. Rebel, Markus Roth, H. Gemmeke, A. Chiavassa, N. Palmieri, K. Bekk, P. Doll, V. de Souza, J. Rautenberg, A. Horneffer, E. Cantoni, S. Schoo, Katrin Link, D. Kang, Ralph Engel, Andreas Haungs, A. Weindl, T. Pierog, Jan Kuijpers, L. Bähren, M. Ludwig, A. Schmidt, F. Di Pierro, C. Morello, Tim Huege, J. Wochele, Octavian Sima, D. Heck, M. E. Bertaina, J. Zabierowski, Kai Daumiller, D. Huber, Claus Grupen, Béatrice Fuchs, A. Saftoiu, G. Toma, and H. Schieler
Subjects: Physics, Amplitude, Optics, LOPES, business.industry, Monte Carlo method, Calibration, Cosmic ray, business, Signal, Energy (signal processing), Radio wave, Computational physics
Abstract: One of the main aims of the LOPES experiment was the evaluation of the absolute amplitudeof the radio signal of air showers. This is of special interest since the radio technique offers the pos-sibility for an independent and highly precise determination of the energy scale of cosmic rays onthe basis of signal predictions from Monte Carlo simulations. For the calibration of the amplitudemeasured by LOPES we used an external source. Previous comparisons of LOPES measurementsand simulations of the radio signal amplitude predicted by CoREAS revealed a discrepancy of theorder of a factor of two. A re-measurement of the reference calibration source, now performed forthe free ﬁeld, was recently performed by the manufacturer. The updated calibration values leadto a lowering of the reconstructed electric ﬁeld measured by LOPES by a factor of 2:6 0:2 andtherefore to a signiﬁcantly better agreement with CoREAS simulations. We discuss the updatedcalibration and its impact on the LOPES analysis results.2
Published: 2016
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13. A comparison of the cosmic-ray energy scales of Tunka-133 and KASCADE-Grande via their radio extensions Tunka-Rex and LOPES

Author: R. D. Monkhoev, Harald Schieler, Hermann-Josef Mathes, J.C. Arteaga-Velázquez, Kai Daumiller, V. V. Prosin, Alexandra Saftoiu, C. Grupen, A. Chiavassa, N. B. Lubsandorzhiev, I.M. Brancus, J. Zabierowski, G. Toma, P. Łuczak, N. Palmieri, M. E. Bertaina, R. Wischnewski, Jan Kuijpers, E. E. Korosteleva, J. Blümer, Andreas Weindl, J. Wochele, Dmitriy Kostunin, O. A. Gress, G.C. Trinchero, Octavian Sima, Julian Rautenberg, M. Kleifges, F. Di Pierro, W. D. Apel, Katrin Link, Tanguy Pierog, C. Rühle, Grigory Rubtsov, J. A. Zensus, H. Bozdog, E. A. Osipova, O. Krömer, M. Melissas, A. Schmidt, Yulia Kazarina, Pavel Bezyazeekov, A. L. Pakhorukov, R. Hiller, Markus Roth, Ralph Engel, Tim Huege, Jörg R. Hörandel, J. Oehlschläger, C. Morello, Andreas Haungs, H. Rebel, Peter L. Biermann, Paula Gina Isar, D. Huber, P. Doll, B. Fuchs, A. Horneffer, L. V. Pankov, L. Bähren, D. Kang, R. R. Mirgazov, M. Ludwig, Oleg Fedorov, S. Schoo, Karl-Heinz Kampert, Dieter Heck, V. de Souza, Heino Falcke, E. Cantoni, A. V. Zagorodnikov, F. G. Schröder, L. A. Kuzmichev, K. Bekk, H. Gemmeke, and N. M. Budnev
Subjects: Nuclear and High Energy Physics, Cosmic rays, KASCADE-Grande, LOPES, Radio detection, Tunka-133, Tunka-Rex, Physics::Instrumentation and Detectors, Astronomy, Astrophysics::High Energy Astrophysical Phenomena, FOS: Physical sciences, Cosmic ray, Astrophysics, 01 natural sciences, Air showers, 0103 physical sciences, ddc:530, 010306 general physics, GeneralLiterature_REFERENCE(e.g.,dictionaries,encyclopedias,glossaries), Instrumentation and Methods for Astrophysics (astro-ph.IM), Physics, High Energy Astrophysical Phenomena (astro-ph.HE), 010308 nuclear & particles physics, Detector, Astrophysics::Instrumentation and Methods for Astrophysics, Digital radio, ASTROFÍSICA, lcsh:QC1-999, Computational physics, Air shower, Amplitude, KASCADE, Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - High Energy Astrophysical Phenomena, lcsh:Physics, Radio wave
Abstract: Physics letters / B 763, 179 - 185(2016). doi:10.1016/j.physletb.2016.10.031, The radio technique is a promising method for detection of cosmic-ray air showers of energies around View the MathML source100PeV and higher with an array of radio antennas. Since the amplitude of the radio signal can be measured absolutely and increases with the shower energy, radio measurements can be used to determine the air-shower energy on an absolute scale. We show that calibrated measurements of radio detectors operated in coincidence with host experiments measuring air showers based on other techniques can be used for comparing the energy scales of these host experiments. Using two approaches, first via direct amplitude measurements, and second via comparison of measurements with air shower simulations, we compare the energy scales of the air-shower experiments Tunka-133 and KASCADE-Grande, using their radio extensions, Tunka-Rex and LOPES, respectively. Due to the consistent amplitude calibration for Tunka-Rex and LOPES achieved by using the same reference source, this comparison reaches an accuracy of approximately 10%10% – limited by some shortcomings of LOPES, which was a prototype experiment for the digital radio technique for air showers. In particular we show that the energy scales of cosmic-ray measurements by the independently calibrated experiments KASCADE-Grande and Tunka-133 are consistent with each other on this level., Published by North-Holland Publ., Amsterdam
Published: 2016
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14. The nature and origin of ultra high-energy cosmic rays

Author: J. R. Hörandel, P. Abreu, M. Aglietta, M. Ahlers, E. J. Ahn, I. F. M. Albuquerque, D. Allard, I. Allekotte, J. Allen, P. Allison, A. Almela, J. Alvarez Castillo, J. Alvarez Muñiz, M. Ambrosio, A. Aminaei, L. Anchordoqui, S. Andringa, T. Antičić, C. Aramo, E. Arganda, F. Arqueros, H. Asorey, P. Assis, J. Aublin, M. Ave, M. Avenier, G. Avila, T. Bäcker, A. M. Badescu, M. Balzer, K. B. Barber, A. F. Barbosa, R. Bardenet, S. L. C. Barroso, B. Baughman f, J. Bäuml, J. J. Beatty, B. R. Becker, K. H. Becker, A. Bellétoile, J. A. Bellido, S. BenZvi, C. Berat, X. Bertou, P. L. Biermann, P. Billoir, F. Blanco, M. Blanco, C. Bleve, H. Blümer, M. Boháčová, D. Boncioli, C. Bonifazi, R. Bonino, N. Borodai, J. Brack, I. Brancus, P. Brogueira, W. C. Brown, R. Bruijn i, P. Buchholz, A. Bueno, R. E. Burton, K. S. Caballero Mora, B. Caccianiga, L. Caramete, R. Caruso, A. Castellina, O. Catalano, G. Cataldi, L. Cazon, R. Cester, J. Chauvin, S. H. Cheng, A. Chiavassa, J. A. Chinellato, J. Chirinos Diaz, J. Chudoba, M. Cilmo, R. W. Clay, R. Conceição, F. Contreras, H. Cook, M. J. Cooper, J. Coppens, A. Cordier, S. Coutu, C. E. Covault, A. Creusot, A. Criss, J. Cronin, A. Curutiu, S. Dagoret Campagne, R. Dallier, B. Daniel, S. Dasso, K. Daumiller, B. R. Dawson, R. M. de Almeida, M. De Domenico, C. De Donato, S. J. de Jong, G. De La Vega, W. J. M. de Mello Junior, J. R. T. de Mello Neto, V. de Souza, K. D. de Vries, L. del Peral, M. del Río, O. Deligny, H. Dembinski, N. Dhital, C. Di Giulio, M. L. Díaz Castro, P. N. Diep, F. Diogo, C. Dobrigkeit, W. Docters, J. C. D'Olivo, P. N. Dong, A. Dorofeev, J. C. dos Anjos, M. T. Dova, D. D'Urso, I. Dutan, J. Ebr, R. Engel, M. Erdmann, C. O. Escobar, J. Espadanal, A. Etchegoyen, P. Facal San Luis, I. Fajardo Tapia, H. Falcke, G. Farrar, A. C. Fauth, N. Fazzini, A. P. Ferguson, B. Fick, A. Filevich, A. Filipčič, S. Fliescher, C. E. Fracchiolla, E. D. Fraenkel, O. Fratu, U. Fröhlich, B. Fuchs, R. Gaior, R. F. Gamarra, S. Gambetta, B. García, S. T. Garcia Roca, D. Garcia Gamez, D. Garcia Pinto, A. Gascon, H. Gemmeke, P. L. Ghia, U. Giaccari, M. Giller, H. Glass, M. S. Gold, G. Golup, F. Gomez Albarracin, M. Gómez Berisso, P. F. Gómez Vitale, P. Gonçalves, D. Gonzalez, J. G. Gonzalez, B. Gookin, A. Gorgi, P. Gouffon, E. Grashorn, S. Grebe, N. Griffith, M. Grigat, A. F. Grillo, Y. Guardincerri, F. Guarino, G. P. Guedes, A. Guzman, P. Hansen, D. Harari, T. A. Harrison, J. L. Harton, A. Haungs, T. Hebbeker, D. Heck, A. E. Herve, C. Hojvat, N. Hollon, V. C. Holmes, P. Homola, A. Horneffer, P. Horvath, M. Hrabovský, D. Huber, T. Huege, A. Insolia, F. Ionita, A. Italiano, C. Jarne, S. Jiraskova, M. Josebachuili, K. Kadija, K. H. Kampert, P. Karhan, P. Kasper, B. Kégl, B. Keilhauer, A. Keivani, J. L. Kelley, E. Kemp, R. M. Kieckhafer, H. O. Klages, M. Kleifges, J. Kleinfeller, J. Knapp, D. H. Koang, K. Kotera, N. Krohm, O. Krömer, D. Kruppke Hansen, F. Kuehn, D. Kuempel, J. K. Kulbartz, N. Kunka, G. La Rosa, C. Lachaud, D. LaHurd, L. Latronico, R. Lauer, P. Lautridou, S. Le Coz, M. S. A. B. Leão, D. Lebrun, P. Lebrun, M. A. Leigui de Oliveira, A. Letessier Selvon, I. Lhenry Yvon, K. Link, R. López, A. Lopez Agüera, K. Louedec, J. Lozano Bahilo, L. Lu, A. Lucero, M. Ludwig, H. Lyberis, M. C. Maccarone, C. Macolino, S. Maldera, D. Mandat, P. Mantsch, A. G. Mariazzi, J. Marin, V. Marin, I. C. Maris, H. R. Marquez Falcon, L. Martin, H. Martinez, O. Martínez Bravo, H. J. Mathes, J. Matthews, J. A. J. Matthews, G. Matthiae, D. Maurel, D. Maurizio, P. O. Mazur, G. Medina Tanco, M. Melissas, D. Melo, E. Menichetti, A. Menshikov, P. Mertsch, C. Meurer, S. Mićanović, M. I. Micheletti, I. A. Minaya, L. Miramonti, L. Molina Bueno, S. Mollerach, M. Monasor, D. Monnier Ragaigne, F. Montanet, B. Morales, C. Morello, E. Moreno, J. C. Moreno, M. Mostafá, C. A. Moura, M. A. Muller, G. Müller, M. Münchmeyer, R. Mussa, G. Navarra ‡, J. L. Navarro, S. Navas, P. Necesal, L. Nellen, A. Nelles, J. Neuser, P. T. Nhung, M. Niechciol, L. Niemietz, N. Nierstenhoefer, D. Nitz, D. Nosek, L. Nožka, J. Oehlschläger, A. Olinto, M. Ortiz, N. Pacheco, D. Pakk Selmi Dei, M. Palatka, J. Pallotta, N. Palmieri, G. Parente, E. Parizot, A. Parra, S. Pastor, T. Paul, M. Pech, J. Pękala, R. Pelayo, I. M. Pepe, R. Pesce, E. Petermann, S. Petrera, P. Petrinca, A. Petrolini, Y. Petrov, C. Pfendner, R. Piegaia, T. Pierog, P. Pieroni, M. Pimenta, V. Pirronello, M. Platino, M. Plum, V. H. Ponce, M. Pontz, A. Porcelli, P. Privitera, M. Prouza, E. J. Quel, S. Querchfeld, J. Rautenberg, O. Ravel, D. Ravignani, B. Revenu, J. Ridky, S. Riggi, M. Risse, P. Ristori, H. Rivera, V. Rizi, J. Roberts, W. Rodrigues de Carvalho, G. Rodriguez, J. Rodriguez Martino, J. Rodriguez Rojo, I. Rodriguez Cabo, M. D. Rodríguez Frías, G. Ros, J. Rosado, T. Rossler, M. Roth, B. Rouillé d'Orfeuil, E. Roulet, A. C. Rovero, C. Rühle, A. Saftoiu, F. Salamida, H. Salazar, F. Salesa Greus, G. Salina, F. Sánchez, C. E. Santo, E. Santos, E. M. Santos, F. Sarazin, B. Sarkar, S. Sarkar, R. Sato, N. Scharf, V. Scherini, H. Schieler, P. Schiffer, A. Schmidt, O. Scholten, H. Schoorlemmer, J. Schovancova, P. Schovánek, F. Schröder, S. Schulte, D. Schuster, S. J. Sciutto, M. Scuderi, A. Segreto, M. Settimo, A. Shadkam, R. C. Shellard, I. Sidelnik, G. Sigl, H. H. Silva Lopez, O. Sima, A. Śmiałkowski, R. Šmída, G. R. Snow, P. Sommers, J. Sorokin, H. Spinka, R. Squartini, Y. N. Srivastava, S. Stanic, J. Stapleton, J. Stasielak, M. Stephan, A. Stutz, F. Suarez, T. Suomijärvi, A. D. Supanitsky, T. Šuša, M. S. Sutherland, J. Swain, Z. Szadkowski, M. Szuba, A. Tapia, M. Tartare, O. Taşcău, C. G. Tavera Ruiz, R. Tcaciuc, N. T. Thao, D. Thomas, J. Tiffenberg, C. Timmermans, W. Tkaczyk, C. J. Todero Peixoto, G. Toma, L. Tomankova, B. Tomé, A. Tonachini, P. Travnicek, D. B. Tridapalli, G. Tristram, E. Trovato, M. Tueros, R. Ulrich, M. Unger, M. Urban, J. F. Valdés Galicia, I. Valiño, L. Valore, A. M. van den Berg, E. Varela, B. Vargas Cárdenas, J. R. Vázquez, R. A. Vázquez, D. Veberič, V. Verzi, J. Vicha, M. Videla, L. Villaseñor, H. Wahlberg, P. Wahrlich, O. Wainberg, D. Walz, A. A. Watson, M. Weber, K. Weidenhaupt, A. Weindl, F. Werner, S. Westerhoff, B. J. Whelan, A. Widom, G. Wieczorek, L. Wiencke, B. Wilczyńska, H. Wilczyński, M. Will, C. Williams, T. Winchen, M. Wommer, B. Wundheiler, T. Yamamoto a, T. Yapici, P. Younk, G. Yuan, A. Yushkov, B. Zamorano, E. Zas, D. Zavrtanik, M. Zavrtanik, I. Zaw h, A. Zepeda, Y. Zhu, M. Zimbres Silva, M. Ziolkowski, COLUCCIA, MARIA RITA, DE MITRI, Ivan, MARSELLA, GIOVANNI, MARTELLO, Daniele, PERRONE, Lorenzo, J. R., Hörandel for the Auger Collaboration, M., Ambrosio, Aramo, Carla, M., Cilmo, D'Urso, Domenico, Guarino, Fausto, Valore, Laura, J. R., Hörandel, P., Abreu, M., Aglietta, M., Ahler, E. J., Ahn, I. F. M., Albuquerque, D., Allard, I., Allekotte, J., Allen, P., Allison, A., Almela, J., Alvarez Castillo, J., Alvarez Muñiz, A., Aminaei, L., Anchordoqui, S., Andringa, T., Antičić, C., Aramo, E., Arganda, F., Arquero, H., Asorey, P., Assi, J., Aublin, M., Ave, M., Avenier, G., Avila, T., Bäcker, A. M., Badescu, M., Balzer, K. B., Barber, A. F., Barbosa, R., Bardenet, S. L. C., Barroso, B., Baughman f, J., Bäuml, J. J., Beatty, B. R., Becker, K. H., Becker, A., Bellétoile, J. A., Bellido, S., Benzvi, C., Berat, X., Bertou, P. L., Biermann, P., Billoir, F., Blanco, M., Blanco, C., Bleve, H., Blümer, M., Boháčová, D., Boncioli, C., Bonifazi, R., Bonino, N., Borodai, J., Brack, I., Brancu, P., Brogueira, W. C., Brown, R., Bruijn i, P., Buchholz, A., Bueno, R. E., Burton, K. S., Caballero Mora, B., Caccianiga, L., Caramete, R., Caruso, A., Castellina, O., Catalano, G., Cataldi, L., Cazon, R., Cester, J., Chauvin, S. H., Cheng, A., Chiavassa, J. A., Chinellato, J., Chirinos Diaz, J., Chudoba, R. W., Clay, Coluccia, MARIA RITA, R., Conceição, F., Contrera, H., Cook, M. J., Cooper, J., Coppen, A., Cordier, S., Coutu, C. E., Covault, A., Creusot, A., Cri, J., Cronin, A., Curutiu, S., Dagoret Campagne, R., Dallier, B., Daniel, S., Dasso, K., Daumiller, B. R., Dawson, R. M., de Almeida, M., De Domenico, C., De Donato, S. J., de Jong, G., De La Vega, W. J. M., de Mello Junior, J. R. T., de Mello Neto, DE MITRI, Ivan, V., de Souza, K. D., de Vrie, L., del Peral, M., del Río, O., Deligny, H., Dembinski, N., Dhital, C., Di Giulio, M. L., Díaz Castro, P. N., Diep, F., Diogo, C., Dobrigkeit, W., Docter, J. C., D'Olivo, P. N., Dong, A., Dorofeev, J. C., dos Anjo, M. T., Dova, D., D'Urso, I., Dutan, J., Ebr, R., Engel, M., Erdmann, C. O., Escobar, J., Espadanal, A., Etchegoyen, P., Facal San Lui, I., Fajardo Tapia, H., Falcke, G., Farrar, A. C., Fauth, N., Fazzini, A. P., Ferguson, B., Fick, A., Filevich, A., Filipčič, S., Fliescher, C. E., Fracchiolla, E. D., Fraenkel, O., Fratu, U., Fröhlich, B., Fuch, R., Gaior, R. F., Gamarra, S., Gambetta, B., García, S. T., Garcia Roca, D., Garcia Gamez, D., Garcia Pinto, A., Gascon, H., Gemmeke, P. L., Ghia, U., Giaccari, M., Giller, H., Gla, M. S., Gold, G., Golup, F., Gomez Albarracin, M., Gómez Berisso, P. F., Gómez Vitale, P., Gonçalve, D., Gonzalez, J. G., Gonzalez, B., Gookin, A., Gorgi, P., Gouffon, E., Grashorn, S., Grebe, N., Griffith, M., Grigat, A. F., Grillo, Y., Guardincerri, F., Guarino, G. P., Guede, A., Guzman, P., Hansen, D., Harari, T. A., Harrison, J. L., Harton, A., Haung, T., Hebbeker, D., Heck, A. E., Herve, C., Hojvat, N., Hollon, V. C., Holme, P., Homola, A., Horneffer, P., Horvath, M., Hrabovský, D., Huber, T., Huege, A., Insolia, F., Ionita, A., Italiano, C., Jarne, S., Jiraskova, M., Josebachuili, K., Kadija, K. H., Kampert, P., Karhan, P., Kasper, B., Kégl, B., Keilhauer, A., Keivani, J. L., Kelley, E., Kemp, R. M., Kieckhafer, H. O., Klage, M., Kleifge, J., Kleinfeller, J., Knapp, D. H., Koang, K., Kotera, N., Krohm, O., Krömer, D., Kruppke Hansen, F., Kuehn, D., Kuempel, J. K., Kulbartz, N., Kunka, G., La Rosa, C., Lachaud, D., Lahurd, L., Latronico, R., Lauer, P., Lautridou, S., Le Coz, M. S. A. B., Leão, D., Lebrun, P., Lebrun, M. A., Leigui de Oliveira, A., Letessier Selvon, I., Lhenry Yvon, K., Link, R., López, A., Lopez Agüera, K., Louedec, J., Lozano Bahilo, L., Lu, A., Lucero, M., Ludwig, H., Lyberi, M. C., Maccarone, C., Macolino, S., Maldera, D., Mandat, P., Mantsch, A. G., Mariazzi, J., Marin, V., Marin, I. C., Mari, H. R., Marquez Falcon, Marsella, Giovanni, Martello, Daniele, L., Martin, H., Martinez, O., Martínez Bravo, H. J., Mathe, J., Matthew, J. A. J., Matthew, G., Matthiae, D., Maurel, D., Maurizio, P. O., Mazur, G., Medina Tanco, M., Melissa, D., Melo, E., Menichetti, A., Menshikov, P., Mertsch, C., Meurer, S., Mićanović, M. I., Micheletti, I. A., Minaya, L., Miramonti, L., Molina Bueno, S., Mollerach, M., Monasor, D., Monnier Ragaigne, F., Montanet, B., Morale, C., Morello, E., Moreno, J. C., Moreno, M., Mostafá, C. A., Moura, M. A., Muller, G., Müller, M., Münchmeyer, R., Mussa, G., Navarra ‡, J. L., Navarro, S., Nava, P., Necesal, L., Nellen, A., Nelle, J., Neuser, P. T., Nhung, M., Niechciol, L., Niemietz, N., Nierstenhoefer, D., Nitz, D., Nosek, L., Nožka, J., Oehlschläger, A., Olinto, M., Ortiz, N., Pacheco, D., Pakk Selmi Dei, M., Palatka, J., Pallotta, N., Palmieri, G., Parente, E., Parizot, A., Parra, S., Pastor, T., Paul, M., Pech, J., Pękala, R., Pelayo, I. M., Pepe, Perrone, Lorenzo, R., Pesce, E., Petermann, S., Petrera, P., Petrinca, A., Petrolini, Y., Petrov, C., Pfendner, R., Piegaia, T., Pierog, P., Pieroni, M., Pimenta, V., Pirronello, M., Platino, M., Plum, V. H., Ponce, M., Pontz, A., Porcelli, P., Privitera, M., Prouza, E. J., Quel, S., Querchfeld, J., Rautenberg, O., Ravel, D., Ravignani, B., Revenu, J., Ridky, S., Riggi, M., Risse, P., Ristori, H., Rivera, V., Rizi, J., Robert, W., Rodrigues de Carvalho, G., Rodriguez, J., Rodriguez Martino, J., Rodriguez Rojo, I., Rodriguez Cabo, M. D., Rodríguez Fría, G., Ro, J., Rosado, T., Rossler, M., Roth, B., Rouillé d'Orfeuil, E., Roulet, A. C., Rovero, C., Rühle, A., Saftoiu, F., Salamida, H., Salazar, F., Salesa Greu, G., Salina, F., Sánchez, C. E., Santo, E., Santo, E. M., Santo, F., Sarazin, B., Sarkar, S., Sarkar, R., Sato, N., Scharf, V., Scherini, H., Schieler, P., Schiffer, A., Schmidt, O., Scholten, H., Schoorlemmer, J., Schovancova, P., Schovánek, F., Schröder, S., Schulte, D., Schuster, S. J., Sciutto, M., Scuderi, A., Segreto, M., Settimo, A., Shadkam, R. C., Shellard, I., Sidelnik, G., Sigl, H. H., Silva Lopez, O., Sima, A., Śmiałkowski, R., Šmída, G. R., Snow, P., Sommer, J., Sorokin, H., Spinka, R., Squartini, Y. N., Srivastava, S., Stanic, J., Stapleton, J., Stasielak, M., Stephan, A., Stutz, F., Suarez, T., Suomijärvi, A. D., Supanitsky, T., Šuša, M. S., Sutherland, J., Swain, Z., Szadkowski, M., Szuba, A., Tapia, M., Tartare, O., Taşcău, C. G., Tavera Ruiz, R., Tcaciuc, N. T., Thao, D., Thoma, J., Tiffenberg, C., Timmerman, W., Tkaczyk, C. J., Todero Peixoto, G., Toma, L., Tomankova, B., Tomé, A., Tonachini, P., Travnicek, D. B., Tridapalli, G., Tristram, E., Trovato, M., Tuero, R., Ulrich, M., Unger, M., Urban, J. F., Valdés Galicia, I., Valiño, L., Valore, A. M., van den Berg, E., Varela, B., Vargas Cárdena, J. R., Vázquez, R. A., Vázquez, D., Veberič, V., Verzi, J., Vicha, M., Videla, L., Villaseñor, H., Wahlberg, P., Wahrlich, O., Wainberg, D., Walz, A. A., Watson, M., Weber, K., Weidenhaupt, A., Weindl, F., Werner, S., Westerhoff, B. J., Whelan, A., Widom, G., Wieczorek, L., Wiencke, B., Wilczyńska, H., Wilczyński, M., Will, C., William, T., Winchen, M., Wommer, B., Wundheiler, T., Yamamoto a, T., Yapici, P., Younk, G., Yuan, A., Yushkov, B., Zamorano, E., Za, D., Zavrtanik, M., Zavrtanik, I., Zaw h, A., Zepeda, Y., Zhu, M., Zimbres Silva, and M., Ziolkowski
Subjects: Physics, business.industry, Astronomy, Astrophysical source, General Physics and Astronomy, Pierre Auger Observatory, Cosmic Ray, Particle detector, Cosmology, Radiation flux, Optics, Measuring instrument, Ultra-high-energy cosmic ray, business
Abstract: The Earth is exposed to a permanent rain of cosmic particles from outer space [1]. Most of the particles are fully ionised atomic nuclei, moving with relativistic energies. The bulk of them with energies up to 1017 eV originate within our Milky Way. They are most likely accel- erated in supernova remnants. Some particles have a thousand times higher energies, i.e., around 1020 eV. This corresponds to the kinetic energy of a tennis ball with a mass of 50 g and a velocity of 90 km/h
Published: 2012
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15. The cosmic ray energy spectrum in the range 1016–1018 eV measured by KASCADE-Grande

Author: Kai Daumiller, T. Huege, G. Navarra, H. J. Mathes, B. Mitrica, Peter Buchholz, F.G. Schröder, I.M. Brancus, Claus Grupen, Markus Roth, J. Engler, W. D. Apel, A. Chiavassa, M. Finger, P. Łuczak, J.R. Hörandel, M. Wommer, J. Oehlschläger, N. Palmieri, P. Doll, M. Petcu, Ralph Engel, M. E. Bertaina, E. Cantoni, J. Blümer, J. Milke, K. Link, H. Rebel, A. Weindl, A. Haungs, J. Wochele, Octavian Sima, F. Di Pierro, C. Morello, J. Zabierowski, D. Kang, D. Heck, G.C. Trinchero, H.O. Klages, H. Schieler, K. Bekk, Karl-Heinz Kampert, J.C. Arteaga-Velázquez, S. Over, G. Toma, M. Melissas, D. Fuhrmann, R. Glasstetter, H.J. Mayer, H. Bozdog, H. Ulrich, S. Ostapchenko, H.J. Gils, F. Cossavella, M. Ludwig, P.G. Isar, D. Kickelbick, V. de Souza, T. Pierog, Piera Luisa Ghia, and S. Nehls
Subjects: Nuclear physics, Physics, Range (particle radiation), Air shower, Muon, Physics and Astronomy (miscellaneous), KASCADE, Monte Carlo method, Calibration, Astronomy and Astrophysics, Cosmic ray, Charged particle
Abstract: The KASCADE-Grande experiment, located at Campus North of the Karlsruhe Institute of Technology (Ger- many) is a multi-component extensive air-shower experiment devoted to the study of cosmic rays and their interactions at primary energies 10 14 − 10 18 eV. One of the main goals of the experiment is the measurement of the all particle en- ergy spectrum in the 10 16 − 10 18 eV range, i.e. extending the range accessible by KASCADE alone. The Grande detec- tor samples the charged component (Nch) of the air shower while the original KASCADE array provides in addition a measurement of the muon component (Nµ). The combined information of Nch and Nµ is used to estimate the energy on an event-by-event basis and to derive the all-particle energy spectrum. Since the calibration of the observables in terms of the primary energy depends on Monte Carlo simulations, three different methods with partially different sources of un
Published: 2011
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16. The measurement of the cosmic ray primary energy spectrum at 1016–1018 eV with the KASCADE-Grande experiment

Author: H. Rebel, B. Mitrica, M. Finger, Kai Daumiller, H. Schieler, Karl-Heinz Kampert, J. Wochele, R. Glasstetter, F. Cossavella, Octavian Sima, J. Blümer, M. Petcu, D. Heck, Peter Buchholz, F. Di Pierro, J.C. Arteaga-Velázquez, C. Morello, I.M. Brancus, M. Melissas, W. D. Apel, H. Bozdog, J. Oehlschläger, Markus Roth, Elena Cantoni, H.J. Mayer, A. Chiavassa, J. Engler, S. Ostapchenko, H.J. Gils, H. Ulrich, M. Ludwig, P.G. Isar, M. E. Bertaina, J.R. Hörandel, M. Wommer, T. Huege, Ralph Engel, J. Milke, K. Link, H. J. Mathes, T. Pierog, A. Haungs, Piera Luisa Ghia, J. Zabierowski, G.C. Trinchero, F.G. Schröder, S. Nehls, G. Toma, D. Kang, G. Navarra, H.O. Klages, D. Kickelbick, V. de Souza, S. Over, D. Fuhrmann, A. Weindl, P. Łuczak, N. Palmieri, C. Grupen, K. Bekk, and P. Doll
Subjects: Physics, Nuclear and High Energy Physics, Range (particle radiation), Muon, Astrophysics::High Energy Astrophysical Phenomena, Detector, Astrophysics::Instrumentation and Methods for Astrophysics, Cosmic ray, Radiation, Atomic and Molecular Physics, and Optics, Charged particle, Nuclear physics, Air shower, KASCADE
Abstract: The KASCADE-Grande experiment operates at Karlsruhe Institute of Technology (KIT) in Germany. Itʼs aim is the study of the primary cosmic radiation, through Extensive Air Shower detection, in the range 1016–1018 eV. Here, measurements are of main interest to understand the high energy evolution of cosmic radiation: a change in the slope of the heavy primary spectrum is expected (as measured at lower energies for lighter primaries) as a possible confirmation of the predicted astrophysical mechanisms; moreover, in this range the transition from galactic to extragalactic radiation is supposed to take place and the observations could clarify the features of this transition, putting the basis for the interpretation of the data at the highest energies. For these tasks KASCADE-Grande fulfills very well the requirements, both concerning the acceptance and the experimental performances. The experiment is constituted by two co-operating arrays of detectors: the KASCADE array, with its 252 detectors in a dense grid of 200×200 m2 and the Grande array, made of 37 detectors arranged on a wider area of 700×700 m2. The Grande array samples the total charged particles size of the air shower, while the KASCADE array provides the muon size In this contribution, KASCADE-Grande measurement of the cosmic ray primary energy spectrum is presented. The exploited technique, calibrated with simulations, combines the charged particles component and muon component on a shower by shower basis, performing the energy estimation of each primary event. Other techniques are also performed, for a better evaluation of systematics and a check of consistency of the hadronic interaction model used in simulations.
Published: 2011
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17. New measurements of cosmic ray air showers with the digital radio interferometer LOPES

Author: P. Łuczak, H. Gemmeke, N. Palmieri, M. Finger, Claus Grupen, A. Chiavassa, J. Wochele, Octavian Sima, M. Ludwig, D. Kang, D. Heck, H. Bozdog, S.J. Lafebre, Heino Falcke, J. Blümer, H. J. Mathes, Tim Huege, L. Bähren, A. Weindl, F.G. Schröder, O. Krömer, Jan Kuijpers, D. Huber, J. A. Zensus, E. Cantoni, Ralph Engel, M. Wommer, Alexandra Saftoiu, J.C. Arteaga, A. Schmidt, A. Horneffer, K. Bekk, C. Rühle, C. Morello, T. Asch, D. Fuhrmann, W. D. Apel, Peter L. Biermann, Markus Roth, J. Rautenberg, Peter Buchholz, G. Toma, T. Pierog, I.M. Brancus, S. Nehls, Kai Daumiller, V. de Souza, Jörg R. Hörandel, P.G. Isar, G.C. Trinchero, J. Oehlschläger, M. E. Bertaina, Stijn Buitink, K. Link, A. Haungs, H. Rebel, J. Zabierowski, H. Schieler, M. Melissas, P. Doll, and K. H. Kampert
Subjects: Physics, Physics and Astronomy (miscellaneous), LOPES, Frequency band, Astrophysics::High Energy Astrophysical Phenomena, Astronomy, Astrophysics::Instrumentation and Methods for Astrophysics, Astronomy and Astrophysics, Cosmic ray, Aetiology, screening and detection [ONCOL 5], Astrophysics::Cosmology and Extragalactic Astrophysics, Digital radio, law.invention, Radio telescope, Interferometry, Air shower, law, RÁDIO, Dipole antenna, GeneralLiterature_REFERENCE(e.g.,dictionaries,encyclopedias,glossaries)
Abstract: LOPES is a digital radio interferometer which measures the radio emission of extensive cosmic ray air showers. It mainly consists of 30 dipole antennas installed in co-location with KASCADE-Grande at the Karlsruhe Insti- tute of Technology (KIT) in Germany. KASCADE-Grande measures the secondary air shower particles at ground. Whenever KASCADE-Grande detects a high-energy cosmic ray event (� 10 16 eV), it triggers LOPES which then digi- tally records the radio signal in the frequency band from 40 to 80 MHz. Using interferometric methods, LOPES is able to successfully detect air shower induced radio pulses, even in the noisy environment at the KIT. In the present studies, a considerable progress in understanding the radio emission mechanism is shown: The latest version of the "radio emis
Published: 2011
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18. The exposure of the hybrid detector of the Pierre Auger Observatory

Author: E. J. Ahn, B. Rouillé-D'Orfeuil, J. Knapp, A. Lopez Agüera, Maria-Teresa Dova, F. Guarino, John Matthews, Peter Buchholz, T. Huege, A. Parra, E. Petermann, H. Glass, Marco Aglietta, A. F. Barbosa, D. Nosek, T. Yamamoto, D. Nitz, D. García Gámez, Miroslav Pech, B. García, M. S. Sutherland, A. Filipcic, R. F. Gamarra, E. Moreno, S. R. Gozzini, Sofia Andringa, Mario Scuderi, Tobias Winchen, Jeffrey Brack, Olaf Scholten, Humberto Ibarguen Salazar, Carola Dobrigkeit, I. Valiño, Christopher Morris, M. A. Muller, G. Marsella, M. S. A. B. Leão, Jaime Alvarez-Muñiz, D. Schuster, B. Kégl, Fabian Schmidt, P. Wahrlich, C. Macolino, C. Hojvat, Jan Ebr, M. Melissas, H.O. Klages, Alan Watson, R. López, Karen S. Caballero-Mora, K. B. Barber, G. Salina, Olivier Deligny, R. E. Burton, S. Mićanović, B. M. Baughman, G. Rodriguez, J. Alvarez Castillo, F. Sarazin, K. Link, U. Fröhlich, C. De Donato, Miguel Mostafá, Martin Erdmann, L. Valore, J. Allen, A. P. Ferguson, J. G. Gonzalez, V. C. Holmes, D. Lebrun, I. Dutan, Ugo Giaccari, Dariusz Gora, G. P. Guedes, A. Gorgi, A. Shadkam, M. Palatka, J. Pe¸kala, A. Śmiałkowski, P. Karhan, V. Scherini, A. Lemiere, P. W. Younk, B. Keilhauer, Roger W Clay, M. Urban, Miroslav Hrabovský, A. Haungs, G. Navarra, F. Schüssler, C. Timmermans, B. Zamorano, A. C. Rovero, C. Bleve, K. Louedec, P. Gonçalves, Mariangela Settimo, S. J. Sciutto, D. Maurizio, J. C. Moreno, J. L. Harton, Alexey Yushkov, Azadeh Keivani, J. Oehlschläger, Markus Roth, Paul Sommers, N. Palmieri, A. F. Grillo, Juan Carlos D'Olivo, C. Aramo, S. L.C. Barroso, T. Pierog, Dusan Mandat, O. Tascau, Brian Fick, P. Mantsch, A.M. van den Berg, K. Payet, Darko Veberič, D. Heck, Aaron S. Chou, Jose Chinellato, Pham Ngoc Diep, D. Allard, P. Lautridou, A. C. Fauth, S. Jiraskova, F. Kuehn, S. Mollerach, E. Menichetti, P. Gouffon, P. N. Dong, M. J. Cooper, Heino Falcke, Z. Szadkowski, T. Rossler, Vasiliki Pavlidou, P. L. Ghia, Osvaldo Catalano, J. R. Vázquez, Piotr Homola, P. Facal San Luis, E. Roulet, G. Wieczorek, M. Stephan, R. M. Kieckhafer, J. W. Cronin, A. Menshikov, G. Matthiae, H. Spinka, J. D. Hague, F. Sánchez, M. Ambrosio, M. De Domenico, T. Schmidt, P. Hansen, A. Chiavassa, Vincenzo Rizi, A. E. Herve, A. Letessier-Selvon, J. Rautenberg, H. Schieler, D. Martello, H. Lyberis, C. Riviere, R. Ulrich, J. D. Swain, M. G. Winnick, L. R. Wiencke, Antonio Bueno, Sergio Pastor, B. Revenu, Karl-Heinz Kampert, T. Tarutina, J. Rosado, O. Krömer, J. Petrovic, H. J. Mathes, O. Wainberg, Antonella Castellina, E. Strazzeri, M. Ziolkowski, Domenico Tegolo, M. Ludwig, K. Weidenhaupt, Lorenzo Cazon, M. Risse, Jörg R. Hörandel, T. Bergmann, R. Bonino, Nataliia Borodai, Carla Bonifazi, Jose A. Bellido, Marcos Santander, M. Prouza, O. Martínez Bravo, V. H. Ponce, P. Abreu, I. M. Pepe, Maria Rita Coluccia, I. Lhenry-Yvon, G. Golup, J. Kleinfeller, F. Suarez, N. Kunka, A. Insolia, M. Kleifges, D. Zavrtanik, Sergio Dasso, H. Blümer, G. De La Vega, L. Perrone, Jiri Chudoba, Denis Tcherniakhovski, Gualberto Avila, Ingomar Allekotte, M. Pimenta, D. Ravignani, B. Wilczyńska, Warner A. Miller, R. M. de Almeida, A. Horneffer, P. Petrinca, W. C. Brown, N. Scharf, V. Pirronello, N. T. Thao, Angela V. Olinto, M. Monasor, Luis A. Anchordoqui, G. Parente, M. Ave, E. Trovato, Daniel Kuempel, M. Gómez Berisso, Carlos Escobar, A. Creusot, R. C. Shellard, K. Kotera, J. Stapleton, J. Rodriguez Rojo, S. Maldera, E. Kemp, S. Dagoret-Campagne, A. Tonachini, M. Platino, H. R. Marquez Falcon, A. Tamashiro, F. Arqueros, D. Monnier Ragaigne, S. Harmsma, A. Tapia, P. Necesal, L. Nožka, H. Gemmeke, Enrique Zas, A. D. Supanitsky, Y. Petrov, Hernán Asorey, P. Brogueira, C. Pfendner, D.V. Semikoz, M. Unger, Martina Bohacova, S. Westerhoff, J. Sorokin, T. Bäcker, D. Warner, C. E. Santo, R. D. Parsons, M. Wommer, Graciela B. Gelmini, J. Lozano Bahilo, Segev BenZvi, Kai Daumiller, M. Grigat, P. Lebrun, A. Schmidt, H. Wahlberg, B. R. Becker, G. Tristram, T. Šuša, C. Di Giulio, N. Pacheco, F. Ionita, Fernando Contreras, Corbin Covault, R. Bruijn, Francisco J. Blanco, M. Ortiz, V. Marin, B. Gookin, B. Morales, I. Rodriguez-Cabo, D. Harari, Alessandro Petrolini, D. Kruppke-Hansen, Nicolás G. Busca, M. I. Micheletti, Lino Miramonti, S. J. De Jong, J. Chauvin, I. Zaw, D. B. Tridapalli, F. Gomez Albarracin, R. Mussa, J. J. Beatty, M. Avenier, A. Segreto, D. Thomas, B. Wundheiler, Gregory R Snow, M. D. Rodríguez-Frías, A. Cordier, J. Coppens, Rossella Caruso, Pietro Oliva, A. Lucero, G. La Rosa, B. Vargas Cárdenas, Maria Concetta Maccarone, H. Dembinski, N. Fazzini, T. Suomijärvi, J. Pallotta, J. F. Valdés Galicia, K. H. Becker, R. Cester, B. J. Whelan, X. Garrido, I. De Mitri, E. J. Quel, S. Mueller, T. Hebbeker, Julien Aublin, K. Gesterling, Radomir Smida, Béatrice Fuchs, J. R. T. de Mello Neto, T. Karova, A. Filevich, M. A. Leigui de Oliveira, R. Tcaciuc, A. Ferrero, F. Schroeder, F. Montanet, R. Pesce, J. C. dos Anjos, A. Bellétoile, J. 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Todero Peixoto, German Ros, N. Krohm, L. Nellen, C. Morello, K. D. de Vries, H. Wilczyński, Matthias Balzer, P. Billoir, M. Tueros, L. del Peral, W. Fulgione, O. Ravel, Peter L. Biermann, W. J. M. de Mello Junior, J. Rodriguez Martino, Paolo Privitera, M. Gold, H. Rivera, Daniel Omar Badagnani, D. Melo, U. Cotti, D. Pakk Selmi-Dei, R. Sato, J. Parrisius, A. Weindl, Iván Sidelnik, M. Kaducak, G. Cataldi, V. Verzi, C. Meurer, H. Cook, J. K. Kulbartz, E. M. Santos, Bruce R. Dawson, P.O. Mazur, A. Della Selva, J. L. Navarro, Ernesto Arganda, C. E. Fracchiolla, M. L. Díaz Castro, G. Farrar, D. D'Urso, Corinne Berat, M. Giller, Daniel Gonzalez, M. Videla, E. Parizot, J. C. Diaz, R. Dallier, F. Salamida, Y. Guardincerri, B. Tome, M. McEwen, Moritz Münchmeyer, Christopher B. Williams, Ralph Engel, D. H. Koang, J. Ridky, A. Stutz, APC - Astrophysique des Hautes Energies (APC - AHE), AstroParticule et Cosmologie (APC (UMR_7164)), Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Dipartimento di Astronomia, Universita degli Studi di Bologna, Alma Mater Studiorum Università di Bologna [Bologna] (UNIBO)-Alma Mater Studiorum Università di Bologna [Bologna] (UNIBO), Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Institut polytechnique de Grenoble - 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C., Moreno, C., Morri, M., Mostafá, S., Mueller, M. A., Muller, R., Mussa, G., Navarra ‡, J. L., Navarro, S., Nava, P., Necesal, L., Nellen, P. T., Nhung, N., Nierstenhoefer, D., Nitz, D., Nosek, L., Nožka, M., Nyklicek, J., Oehlschläger, A., Olinto, P., Oliva, V. M., Olmos Gilbaja, M., Ortiz, N., Pacheco, D., Pakk Selmi Dei, M., Palatka, J., Pallotta, N., Palmieri, G., Parente, E., Parizot, A., Parra, J., Parrisiu, R. D., Parson, S., Pastor, T., Paul, V., Pavlidou c, K., Payet, M., Pech, J., Pekala, R., Pelayo, I. M., Pepe, Perrone, Lorenzo, R., Pesce, E., Petermann, S., Petrera, P., Petrinca, A., Petrolini, Y., Petrov, J., Petrovic, C., Pfendner, N., Phan, R., Piegaia, T., Pierog, M., Pimenta, V., Pirronello, M., Platino, V. H., Ponce, M., Pontz, P., Privitera, M., Prouza, E. 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R., Snow, P., Sommer, J., Sorokin, H., Spinka, R., Squartini, J., Stapleton, J., Stasielak, M., Stephan, E., Strazzeri, A., Stutz, F., Suarez, T., Suomijärvi, A. D., Supanitsky, T., Šuša, M. S., Sutherland, J., Swain, Z., Szadkowski, A., Tamashiro, A., Tapia, T., Tarutina, O., Tascau, R., Tcaciuc, D., Tcherniakhovski, D., Tegolo, N. T., Thao, D., Thoma, J., Tiffenberg, C., Timmerman, D. K., Tiwari, W., Tkaczyk, C. J., Todero Peixoto, B., Tomé, A., Tonachini, P., Travnicek, D. B., Tridapalli, G., Tristram, E., Trovato, M., Tuero, R., Ulrich, M., Unger, M., Urban, J. F., Valdés Galicia, I., Valiño, L., Valore, A. M., van den Berg, B., Vargas Cárdena, J. R., Vázquez, R. A., Vázquez, D., Veberic, T., Venter, V., Verzi, M., Videla, L., Villaseñor, H., Wahlberg, P., Wahrlich, O., Wainberg, D., Warner, A. A., Watson, K., Weidenhaupt, A., Weindl, S., Westerhoff, B. J., Whelan, G., Wieczorek, L., Wiencke, B., Wilczynska, H., Wilczynski, M., Will, C., William, T., Winchen, L., Winder, M. G., Winnick, M., Wommer, B., Wundheiler, T., Yamamoto a, P., Younk, G., Yuan, A., Yushkov, B., Zamorano, E., Za, D., Zavrtanik, M., Zavrtanik, I., Zaw, A., Zepeda, M., Ziolkowski, Guarino, Fausto, D'Urso, Domenico, Valore, Laura, Aramo, Carla, DELLA SELVA, Angelo, A. V., Yushkov, The Pierre Auger, Collaboration, Abreu, P, Aglietta, M, Ahn, E.J, Allard, D, Allekotte, I, Allen, J, Alvarez Castillo, J, Alvarez-Muñiz, J, Ambrosio, M, Aminaei, A, Anchordoqui, L, Andringa, S, Antičić, T, Anzalone, A, Aramo, C, Arganda, E, Arisaka, K, Arqueros, F, Asorey, H, Assis, P, Aublin, J, Ave, M, Avenier, M, Avila, G, Bäcker, T, Badagnani, D, Balzer, M, Barber, K.B, Barbosa, A.F, Bardenet, R, Barroso, S.L.C, Baughman, B, Beatty, J.J, Becker, B.R, Becker, K.H, Bellétoile, A, Bellido, J.A, Benzvi, S, Berat, C, Bergmann, T, Bertou, X, Biermann, P.L, Billoir, P, Blanco, F, Blanco, M, Bleve, C, Blümer, H, Boháčová, M, Boncioli, D, Bonifazi, C, Bonino, R, Borodai, N, Brack, J, Brogueira, P, Brown, W.C, Bruijn, R, Buchholz, P, Bueno, A, Burton, R.E, Busca, N.G, Caballero-Mora, K.S, Caramete, L, Caruso, R, Castellina, A, Catalano, O, Cataldi, G, Cazon, L, Cester, R, Chauvin, J, Chiavassa, A, Chinellato, J.A, Chou, A, Chudoba, J, Clay, R.W, Colombo, E, Coluccia, M.R, Conceião, R, Contreras, F, Cook, H, Cooper, M.J, Coppens, J, Cordier, A, Cotti, U, Coutu, S, Covault, C.E, Creusot, A, Criss, A, Cronin, J, Curutiu, A, Dagoret-Campagne, S, Dallier, R, Dasso, S, Daumiller, K, Dawson, B.R, De Almeida, R.M, De Domenico, M, De Donato, C, De Jong, S.J, De La Vega, G, De Mello Junior, W.J.M, De Mello Neto, J.R.T, De Mitri, I, De Souza, V, De Vries, K.D, Decerprit, G, Del Peral, L, Deligny, O, Della Selva, A, Dembinski, H, Denkiewicz, A, Di Giulio, C, Diaz, J.C, Díaz Castro, M.L, Diep, P.N, Dobrigkeit, C, D'Olivo, J.C, Dong, P.N, Dorofeev, A, Dos Anjos, J.C, Dova, M.T, D'Urso, D, Dutan, I, Ebr, J, Engel, R, Erdmann, M, Escobar, C.O, Etchegoyen, A, Facal San Luis, P, Falcke, H, Farrar, G, Fauth, A.C, Fazzini, N, Ferguson, A.P, Ferrero, A, Fick, B, Filevich, A, Filipčič, A, Fleck, I, Fliescher, S, Fracchiolla, C.E, Fraenkel, E.D, Fröhlich, U, Fuchs, B, Fulgione, W, Gamarra, R.F, Gambetta, S, García, B, García Gámez, D, Garcia-Pinto, D, Garrido, X, Gascon, A, Gelmini, G, Gemmeke, H, Gesterling, K, Ghia, P.L, Giaccari, U, Giller, M, Glass, H, Gold, M.S, Golup, G, Gomez Albarracin, F, Gómez Berisso, M, Gonalves, P, Gonzalez, D, Gonzalez, J.G, Gookin, B, Góra, D, Gorgi, A, Gouffon, P, Gozzini, S.R, Grashorn, E, Grebe, S, Grigat, M, Grillo, A.F, Guardincerri, Y, Guarino, F, Guedes, G.P, Hague, J.D, Hansen, P, Harari, D, Harmsma, S, Harton, J.L, Haungs, A, Hebbeker, T, Heck, D, Herve, A.E, Hojvat, C, Holmes, V.C, Homola, P, Hörandel, J.R, Horneffer, A, Hrabovský, M, Huege, T, Insolia, A, Ionita, F, Italiano, A, Jiraskova, S, Kadija, K, Kaducak, M, Kampert, K.H, Karhan, P, Karova, T, Kasper, P, Kégl, B, Keilhauer, B, Keivani, A, Kelley, J.L, Kemp, E, Kieckhafer, R.M, Klages, H.O, Kleifges, M, Kleinfeller, J, Knapp, J, Koang, D.-H, Kotera, K, Krohm, N, Krömer, O, Kruppke-Hansen, D, Kuehn, F, Kuempel, D, Kulbartz, J.K, Kunka, N, La Rosa, G, Lachaud, C, Lautridou, P, Leão, M.S.A.B, Lebrun, D, Lebrun, P, Leigui De Oliveira, M.A, Lemiere, A, Letessier-Selvon, A, Lhenry-Yvon, I, Link, K, López, R, Lopez Agüera, A, Louedec, K, Lozano Bahilo, J, Lucero, A, Ludwig, M, Lyberis, H, MacCarone, M.C, MacOlino, C, Maldera, S, Mandat, D, Mantsch, P, Mariazzi, A.G, Marin, V, Maris, I.C, Marquez Falcon, H.R, Marsella, G, Martello, D, Martin, L, Martínez Bravo, O, Mathes, H.J, Matthews, J, Matthews, J.A.J, Matthiae, G, Maurizio, D, Mazur, P.O, McEwen, M, Medina-Tanco, G, Melissas, M, Melo, D, Menichetti, E, Menshikov, A, Meurer, C, Mičanović, S, Micheletti, M.I, Miller, W, Miramonti, L, Mollerach, S, Monasor, M, Monnier Ragaigne, D, Montanet, F, Morales, B, Morello, C, Moreno, E, Moreno, J.C, Morris, C, Mostafá, M, Mueller, S, Muller, M.A, Münchmeyer, M, Mussa, R, Navarra, G, Navarro, J.L, Navas, S, Necesal, P, Nellen, L, Nhung, P.T, Nierstenhoefer, N, Nitz, D, Nosek, D, Nožka, L, Nyklicek, M, Oehlschläger, J, Olinto, A, Oliva, P, Olmos-Gilbaja, V.M, Ortiz, M, Pacheco, N, Pakk Selmi-Dei, D, Palatka, M, Pallotta, J, Palmieri, N, Parente, G, Parizot, E, Parra, A, Parrisius, J, Parsons, R.D, Pastor, S, Paul, T, Pavlidou, V, Payet, K, Pech, M, Pȩkala, J, Pelayo, R, Pepe, I.M, Perrone, L, Pesce, R, Petermann, E, Petrera, S, Petrinca, P, Petrolini, A, Petrov, Y, Petrovic, J, Pfendner, C, Phan, N, Piegaia, R, Pierog, T, Pimenta, M, Pirronello, V, Platino, M, Ponce, V.H, Pontz, M, Privitera, P, Prouza, M, Quel, E.J, Rautenberg, J, Ravel, O, Ravignani, D, Revenu, B, Ridky, J, Riggi, S, Risse, M, Ristori, P, Rivera, H, Rivire, C, Rizi, V, Robledo, C, Rodriguez, G, Rodriguez Martino, J, Rodriguez Rojo, J, Rodriguez-Cabo, I, Rodríguez-Frías, M.D, Ros, G, Rosado, J, Rossler, T, Roth, M, Rouillé-D'Orfeuil, B, Roulet, E, Rovero, A.C, Salamida, F, Salazar, H, Salina, G, Sánchez, F, Santander, M, Santo, C.E, Santos, E, Santos, E.M, Sarazin, F, Sarkar, S, Sato, R, Scharf, N, Scherini, V, Schieler, H, Schiffer, P, Schmidt, A, Schmidt, F, Schmidt, T, Scholten, O, Schoorlemmer, H, Schovancova, J, Schovánek, P, Schroeder, F, Schulte, S, Schüssler, F, Schuster, D, Sciutto, S.J, Scuderi, M, Segreto, A, Semikoz, D, Settimo, M, Shadkam, A, Shellard, R.C, Sidelnik, I, Sigl, G, Śmiałkowski, A, Šmída, R, Snow, G.R, Sommers, P, Sorokin, J, Spinka, H, Squartini, R, Stapleton, J, Stasielak, J, Stephan, M, Strazzeri, E, Stutz, A, Suarez, F, Suomijärvi, T, Supanitsky, A.D, Šuša, T, Sutherland, M.S, Swain, J, Szadkowski, Z, Tamashiro, A, Tapia, A, Tarutina, T, Tacu, O, Tcaciuc, R, Tcherniakhovski, D, Tegolo, D, Thao, N.T, Thomas, D, Tiffenberg, J, Timmermans, C, Tiwari, D.K, Tkaczyk, W, Todero Peixoto, C.J, Tomé, B, Tonachini, A, Travnicek, P, Tridapalli, D.B, Tristram, G, Trovato, E, Tueros, M, Ulrich, R, Unger, M, Urban, M, Valdés Galicia, J.F, Valiño, I, Valore, L, Van Den Berg, A.M, Vargas Cárdenas, B, Vázquez, J.R, Vázquez, R.A, Veberič, D, Venters, T, Verzi, V, Videla, M, Villaseñor, L, Wahlberg, H, Wahrlich, P, Wainberg, O, Warner, D, Watson, A.A, Weidenhaupt, K, Weindl, A, Westerhoff, S, Whelan, B.J, Wieczorek, G, Wiencke, L, Wilczyńska, B, Wilczyński, H, Will, M, Williams, C, Winchen, T, Winders, L, Winnick, M.G, Wommer, M, Wundheiler, B, Yamamoto, T, Younk, P, Yuan, G, Yushkov, A, Zamorano, B, Zas, E, Zavrtanik, D, Zavrtanik, M, Zaw, I, Zepeda, A, Ziolkowski, M., Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Dipartimento di Astronomia, Universita degli Studi di Bologna, Università di Bologna [Bologna] (UNIBO)-Università di Bologna [Bologna] (UNIBO), Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA), PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), and PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Institut für theoretische Physik
Subjects: Physics::Instrumentation and Detectors, Astronomy, 01 natural sciences, Coincidence, Auger, Fluorescence detector, Data acquisition, Auger experiment, High Energy Astrophysical Phenomena (astro-ph.HE), Physics, FÍSICA DE PARTÍCULAS, Settore INF/01 - Informatica, Cascada atmosférica extensa, Detector, Astrophysics::Instrumentation and Methods for Astrophysics, Pierre Auger Observatory, ultra high energy cosmic rays, extensive air showers, trigger, exposure, fluorescence detector, hybrid, ENERGY-SPECTRUM, Radiación cósmica, SIMULATION, ComputingMethodologies_DOCUMENTANDTEXTPROCESSING, Fluorescencia, Física nuclear, Astrophysics - High Energy Astrophysical Phenomena, [PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM], Astrophysics::High Energy Astrophysical Phenomena, Extensive air shower, Measure (physics), FOS: Physical sciences, Cosmic ray, Cosmic Ray, Fluorescence spectroscopy, Ultra high energy cosmic ray, Exposure, Nuclear physics, Optics, SHOWERS, 0103 physical sciences, Extensive air showers, 010306 general physics, Ciencias Exactas, 010308 nuclear & particles physics, business.industry, Física, Astronomy and Astrophysics, Ultra high energy cosmic rays, Hybrid, [SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM], flux, Trigger, Experimental High Energy Physics, business, SYSTEM
Abstract: The Pierre Auger Observatory is a detector for ultra-high energy cosmic rays. It consists of a surface array to measure secondary particles at ground level and a fluorescence detector to measure the development of air showers in the atmosphere above the array. The ‘‘hybrid” detection mode combines the information from the two subsystems. We describe the determination of the hybrid exposure for events observed by the fluorescence telescopes in coincidence with at least one water-Cherenkov detector of the surface array. A detailed knowledge of the time dependence of the detection operations is crucial for an accurate evaluation of the exposure. We discuss the relevance of monitoring data collected during operations, such as the status of the fluorescence detector, background light and atmospheric conditions, that are used in both simulation and reconstruction., Facultad de Ciencias Exactas
Published: 2011
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19. Muon production height studies with the air shower experiment KASCADE-Grande

Author: P. Doll, Jörg R. Hörandel, M. Wommer, F. Di Pierro, C. Morello, M. Ludwig, J. Oehlschläger, P.G. Isar, H. J. Mathes, A. Chiavassa, S. Ostapchenko, H.J. Gils, G.C. Trinchero, R. Obenland, F.G. Schröder, B. Mitrica, Markus Roth, H. Bozdog, H. Rebel, M. E. Bertaina, J. Engler, R. Glasstetter, J. Milke, H. Ulrich, M. Melissas, H. Schieler, Karl-Heinz Kampert, J. Wochele, Octavian Sima, T. Pierog, D. Heck, Kai Daumiller, G. Schatz, Piera Luisa Ghia, S. Nehls, F. Cossavella, T. Huege, D. Kang, H.O. Klages, H.J. Mayer, G. Navarra, D. Kickelbick, V. de Souza, S. Over, D. Fuhrmann, C. Büttner, J.C. Arteaga, J. Blümer, K. Bekk, G. Toma, P. Łuczak, N. Palmieri, Claus Grupen, M. Petcu, Peter Buchholz, I.M. Brancus, A. Weindl, K. Link, J. Zabierowski, E. Cantoni, Ralph Engel, Andreas Haungs, W. D. Apel, M. Finger, Karlsruher Institut für Technologie - Campus Nord, Karlsruher Institut für Technologie - Campus Süd, Dipartimento di Fı'sica Generale dell'Università, National Institute of Physics and Nuclear Engineering, Istituto di Fisica dello Spazio Interplanetario (IFSI), Consiglio Nazionale delle Ricerche (CNR), The Andrzej Soltan Institute for Nuclear Studies, Department of Physics, and University of Bucharest (UniBuc)
Subjects: Air shower, Physics::Instrumentation and Detectors, [SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], Astronomy, Astrophysics::High Energy Astrophysical Phenomena, Cosmic ray, Tracking (particle physics), 01 natural sciences, Nuclear physics, [PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], Shower, 0103 physical sciences, 010306 general physics, Cosmic rays, Muon production height, Physics, Muons, Muon, 010308 nuclear & particles physics, Detector, Astrophysics::Instrumentation and Methods for Astrophysics, Astronomy and Astrophysics, ASTROFÍSICA, KASCADE, Electromagnetic shielding, High Energy Physics::Experiment
Abstract: International audience; A large area (128 m) muon tracking detector, located within the KASCADE experiment, has been built with the aim to identify muons (E> 0.8 GeV) and their angular correlation in extensive air showers by track measurements under 18 r.l. shielding. Orientation of the muon track with respect to the shower axis is expressed in terms of the radial and tangential angles, which are the basic tools for all muon investigations with the tracking detector. By means of triangulation the muon production height is determined. Distributions of measured production heights are compared to CORSIKA shower simulations. Analysis of these heights reveals a transition from light to heavy cosmic ray primary particles with increasing shower energy in the energy region of the 'Knee' of the cosmic ray spectrum.
Published: 2011
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20. Recent results of the LOPES experiment

Author: K. Link, A. Haungs, H. Rebel, G. Toma, H. Bozdog, M. Wommer, H. Gemmeke, T. Huege, B. Mitrica, Heino Falcke, F. Cossavella, F. Di Pierro, J. Zabierowski, C. Morello, D. Kickelbick, M. Ludwig, A. Nigl, Wolfgang Walkowiak, Peter L. Biermann, A. Saftoiu, P. Łuczak, N. Palmieri, V. de Souza, M. Finger, G. Navarra, W. D. Apel, K. Singh, Jörg R. Hörandel, Frank G. Schröder, T. Asch, J. A. Zensus, J.C. Arteaga, J. Wochele, M. Melissas, R. Engel, E. Cantoni, Octavian Sima, J. Oehlschläger, A. Horneffer, D. Kang, Peter Buchholz, O. Krömer, S. Over, J. Blümer, I.M. Brancus, D. Fuhrmann, H. Schieler, D. Heck, Karl-Heinz Kampert, Markus Roth, L. Bähren, T. Pierog, Y. Kolotaev, M. Brüggemann, H. Ulrich, Piera Luisa Ghia, S. Nehls, G.C. Trinchero, H. J. Mathes, M. Petcu, P. Doll, Paula Gina Isar, A. Schmidt, R. Glasstetter, J. Rautenberg, Kai Daumiller, M. E. Bertaina, Stijn Buitink, H.J. Mayer, Andrea Chiavassa, C. Grupen, Moses Ender, A. Weindl, Jan Kuijpers, S.J. Lafebre, F. Badea, and K. Bekk
Subjects: Physics, Nuclear and High Energy Physics, Data processing, Interferometry, Air shower, Meteorology, LOPES, Digital radio, Signal, Atomic and Molecular Physics, and Optics, Remote sensing
Abstract: LOPES measures radio pulses from extensive air showers and aims to calibrate the emitted signal in the primary energy range of 1016–1018 eV. LOPES, a digital radio interferometer using high bandwidths and fast data processing, is set up at the location of the KASCADE-Grande extensive air shower experiment in Karlsruhe, Germany and profits from the reconstructed air shower observables of KASCADE-Grande. We report about recent analysis results of the radio signals measured by LOPES.
Published: 2009
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21. Recent Results from KASCADE-Grande and LOPES

Author: K.-H. Kampert, W.D. Apel, J.C. Arteaga, T. Asch, F. Badea, L. Bähren, K. Bekk, M. Bertaina, P.L. Biermann, J. Blümer, H. Bozdog, I.M. Brancus, M. Brüggemann, P. Buchholz, S. Buitink, E. Cantoni, A. Chiavassa, F. Cossavella, K. Daumiller, V. de Souza, F. Di Pierro, P. Doll, M. Ender, R. Engel, J. Engler, H. Falcke, M. Finger, D. Fuhrmann, H. Gemmeke, P.L. Ghia, H.J. Gils, R. Glasstetter, C. Grupen, A. Haungs, D. Heck, J.R. Hörandel, A. Horneffer, T. Huege, P.G. Isar, D. Kang, D. Kickelbick, H.O. Klages, Y. Kolotaev, O. Krömer, J. Kuijpers, S. Lafebre, K. Link, P. Łuczak, M. Ludwig, H.J. Mathes, H.J. Mayer, J. Milke, M. Melissas, B. Mitrica, C. Morello, G. Navarra, S. Nehls, A. Nigl, J. Oehlschläger, S. Ostapchenko, S. Over, N. Palmieri, M. Petcu, T. Pierog, J. Rautenberg, H. Rebel, M. Roth, A. Saftoiu, H. Schieler, A. Schmidt, F. Schröder, O. Sima, K. Singh, M. Stümpert, G. Toma, G. Trinchero, H. Ulrich, W. Walkowiak, A. Weindl, J. Wochele, M. Wommer, J. Zabierowski, and J.A. Zensus
Subjects: Physics, Nuclear and High Energy Physics, Muon, LOPES, business.industry, Detector, Electrical engineering, Cosmic ray, Tracking (particle physics), Signal, Atomic and Molecular Physics, and Optics, Computational physics, KASCADE, business, Energy (signal processing)
Abstract: KASCADE-Grande is an extensive air-shower experiment located at Forschungszentrum Karlsruhe, Germany. Main parts of the experiment are the Grande array spread over an area of 700 × 700 m 2 , the original KASCADE array covering 200 × 200 m 2 with unshielded and shielded detectors, and additional muon tracking devices. This multi-detector system allows to investigate the energy spectrum, composition, and anisotropies of cosmic rays in the energy range up to 1 EeV. LOPES is co-located at the same site to measure radio pulses from extensive air showers in coincidence with KASCADE-Grande. It consists of 30 digital antennas operated in different geometrical configurations. Read out is performed at high bandwidths and rate data processing with the aim to calibrate the emitted signal in the primary energy range of 10 16 − 10 18 eV by making use of reconstructed air-shower observables of KASCADE-Grande. An overview on the performance of both experiments will be given and recent analysis results be reported.
Published: 2009
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22. Large scale distribution of ultra high energy cosmic rays detected at the Pierre Auger Observatory with zenith angles up to 80°

Author: M. L. Díaz Castro, D. Martraire, G. Farrar, M. Urban, A. C. Rovero, C. Bleve, Francesca Zuccarello, A. Tepe, M. Oliveira, B. García, Tobias Winchen, Carla Aramo, Vincenzo Rizi, D. Martello, P. Lebrun, R. López, M. Ziolkowski, O. Martínez Bravo, Maurice Stephan, B. Kégl, Karen S. Caballero-Mora, Alberto Filevich, Peter Hansen, L. Perrone, Jiri Chudoba, Thomas Harrison, Marcus Niechciol, A. Tonachini, B. Revenu, J. R. Vázquez, P. Sanchez-Lucas, D. Harari, Alberto Daniel Supanitsky, U. Fröhlich, F. Guarino, Azadeh Keivani, D. Kruppke-Hansen, M. Zavrtanik, J. Kleinfeller, Richard Dallier, A. Nelles, F. Diogo, R. M. de Almeida, M. Ludwig, S. Hartmann, Peter Buchholz, M. Szuba, I.M. Brancus, Miguel Mostafá, Marcio Aparecido Muller, Jaime Alvarez-Muñiz, W. Rodrigues de Carvalho, Martin Erdmann, Yogendra N. Srivastava, M. I. Micheletti, R. Pelayo, H. Glass, V. M. Aranda, Rúben Conceição, Marco Aglietta, Daniel Kuempel, Carlos Escobar, J. W. Cronin, Lu Lu, P. van Bodegom, P.F. Gómez Vitale, L. Nellen, E.M. Holt, A. Saleh, Harm Schoorlemmer, P. Pieroni, F. Arqueros, S. Maldera, M. Videla, David Wittkowski, G. Salina, Danielle LaHurd, Olivier Deligny, S. Querchfeld, R. Gaior, P. Abreu, D. Ravignani, G. Toma, Nataliia Borodai, C. Morello, Maria-Teresa Dova, M. R. Hampel, R. Alves Batista, R. Mussa, J. J. Beatty, E. Petermann, Miroslav Pech, Ivone F. M. Albuquerque, Ke Fang, E. Varela, N. Griffith, N. Kunka, Petr Schovanek, Roger W Clay, Silvia Mollerach, H. Dembinski, N. Fazzini, Pavel Horvath, S. Riggi, Sarka Wykes, L. Ochilo, I. A. Minaya, B. Keilhauer, M. S. Sutherland, Jing Zhou, R. Meissner, Julien Aublin, Markus Roth, P. Necesal, Martina Bohacova, Patrick Allison, J. Sorokin, A. Śmiałkowski, Alex Kääpä, J. Allen, André Schulz, S. J. Sciutto, F. Suarez, Thomas Hebbeker, Paulo J. S. Gonçalves, Sergio Dasso, Martín Miguel Freire, V. Pirronello, G. Cocciolo, Peter L. Biermann, Paul Sommers, L. del Peral, D. Nosek, Alina Mihaela Badescu, M. Prouza, Jörg R. Hörandel, G. Garilli, Johannes Schumacher, Colin Baus, P. Gouffon, M. J. Cooper, F. Sánchez, Carlos Medina, M. De Domenico, O. Ravel, B. Vargas Cárdenas, M. Ave, Iuri Muniz Pepe, T. Suomijärvi, C. Jarne, Octavian Fratu, Maria Rita Coluccia, Sofia Andringa, Bruno Daniel, G. Marsella, T. Yapici, Foteini Oikonomou, J. J. Masías Meza, D. Maurel, T. Huege, N. Awal, S. Müller, C. Hojvat, Jan Ebr, F. Salamida, Jeffrey Brack, Olaf Scholten, M. Platino, I. Jandt, M. Monasor, Michael Unger, N. Scharf, P. Heimann, J. Pallotta, Paolo Privitera, A. Tapia, Humberto Ibarguen Salazar, Lorenzo Caccianiga, A. Weindl, I. Lhenry-Yvon, Q. Dorosti Hasankiadeh, Stijn Buitink, H. Schieler, V. M. Theodoro, M. Fernandes, Ralf Ulrich, H. Gemmeke, B. Mitrica, Heino Falcke, K. Louedec, E. Kemp, Serguei Vorobiov, Dusan Mandat, H.O. Klages, Luis A. Anchordoqui, O. Kambeitz, D. Monnier Ragaigne, V. Novotny, J. Bäuml, Rossella Caruso, A. Lucero, S. Mathys, M. Erfani, G. Cataldi, Mariangela Settimo, N. Hollon, V. Verzi, Peter Schiffer, David Schmidt, J. Vicha, S. Quinn, A. Segreto, D. Nitz, M. Ambrosio, O. A. Taborda, S. Messina, Philipp Papenbreer, E. J. Quel, Nicolás González, C. E. Santo, A. van Vliet, B. Tome, G. Müller, Eric Mayotte, K. H. Kampert, Alexey Yushkov, Antonella Castellina, A. P. Ferguson, M. Palatka, S. J. De Jong, Petr Travnicek, B. Zamorano, Radomir Smida, B. Vlcek, H. Martinez, Octavian Sima, J. G. Gonzalez, D. Lebrun, L. Nožka, L. Tomankova, G. Navarra, R. Piegaia, A. Chiavassa, A. E. Herve, K. B. Barber, M. Gómez Berisso, R. C. Shellard, W. Docters, Alan Coleman, V. Scherini, V. Purrello, J. Lozano Bahilo, A. Porcelli, C. A. Moura, T. Yamamoto, Brian Fick, L. R. Wiencke, Trent D. Grubb, D. Huber, Béatrice Fuchs, Samo Stanič, L. Molina-Bueno, D. Melo, Moritz Münchmeyer, David Walz, G. C. Hill, Niraj Dhital, Pierre Billoir, M. Avenier, A. Curutiu, D. Heck, M. Mallamaci, Florian Gaté, I. Valiño, H. Blümer, Max Malacari, Darko Veberič, D. Pakk Selmi-Dei, R. Sato, Ralph Engel, Corinne Berat, M. Giller, V. de Souza, Juan Manuel Figueira, Corbin Covault, Alexandra Saftoiu, Mario Buscemi, F. Werner, Roberta Colalillo, G. Matthiae, Ugo Giaccari, A. G. Mariazzi, Iván Sidelnik, J. Ridky, Y. Petrov, A. Cordier, Guenter Sigl, M. Candusso, Peter Gorham, A. Stutz, J. Neuser, G. P. Guedes, G. Torralba Elipe, Eva Santos, Antonio Bueno, M. Josebachuili, D. Maurizio, Kai Daumiller, Piotr Homola, P. Facal San Luis, M. Blanco, Toshihiro Fujii, Charles Timmermans, L. Collica, R. Krause, L. Valore, Lino Miramonti, J. R. T. de Mello Neto, R. Meyhandan, R. Bonino, Gualberto Avila, A. Shadkam, Amin Aminaei, J. C. Diaz, Jose Chinellato, P. Lautridou, A. Gorgi, J. A.J. Matthews, Xavier Bertou, A. Zepeda, A. F. Grillo, Juan Carlos D'Olivo, T. Pierog, Esteban Roulet, A. Widom, Angela V. Olinto, E. Trovato, S. Navas, M. S. A. B. Leão, Pedro Assis, A. Etchegoyen, van den Ad M Berg, Luca Latronico, A. Letessier-Selvon, B. Gookin, M. D. Rodríguez-Frías, P. L. Ghia, Lorenzo Cazon, N. Palmieri, P. H. Nguyen, S. Le Coz, Lukas Middendorf, Christine Peters, Eun-Joo Ahn, Carola Dobrigkeit, M. Melissas, Joshua A. Gordon, R. A. Vázquez, A. Filipčič, A. C. Fauth, Carla Bonifazi, Jose A. Bellido, A. Menshikov, E. M. Santos, M. Risse, J. D. Swain, B. Wilczynska, John N. Matthews, R. M. Kieckhafer, J. Rautenberg, François Montanet, M. Plum, C. L. Williams, Bruce R. Dawson, O. Krömer, O. Wainberg, F. Sarazin, S. van Velzen, S. Petrera, J. Maller, Jaime Rosado, R. Cester, M. E. Bertaina, W. C. Brown, P.O. Mazur, K. Weidenhaupt, I. Al Samarai, Sasa Micanovic, B. D. Fox, G. Parente, Marc Weber, Alan Watson, Marco Giammarchi, J. Alvarez Castillo, A. Insolia, M. Kleifges, D. Zavrtanik, J. F. Valdés Galicia, I. De Mitri, A. Gascon Bravo, D. Garcia-Gamez, I. C. Mariş, Hernan Wahlberg, G. Rodriguez Fernandez, Hernán Asorey, K. Link, J. Pȩkala, V. Marin, M. A. Leigui de Oliveira, D. Rogozin, J. de Oliveira, Alejandro Almela, Johannes Schulz, K.-H. Becker, M. Pimenta, R. R. Prado, D. Torres Machado, Miroslav Hrabovský, A. Haungs, A. Parra, R. J. Lauer, D. Garcia-Pinto, Yingchun Zhu, J. L. Harton, P. Ristori, Paula Gina Isar, Pedro Brogueira, F. Salesa Greus, S. G. Blaess, M. Zimbres Silva, P. Mantsch, Z. Szadkowski, J. Stapleton, A. Di Matteo, B. Wundheiler, B. Caccianiga, I. Allekotte, L. Caramete, Gregory R Snow, P. H. Kasper, G. S. Varner, T. Rossler, A. Bridgeman, L. Niemietz, N. Pacheco, S. J. Saffi, S. Grebe, Tim Niggemann, Markus Lauscher, J. Phuntsok, Raul Sarmento, R. Squartini, T. Paul, H. J. Mathes, G. Medina-Tanco, G. van Aar, C. J. Todero Peixoto, J. Rodriguez Rojo, N. Krohm, B. Sarkar, Christian Glaser, A. G. Chavez, F.G. Schröder, J. Espadanal, H. Wilczyński, Enrique Zas, C. Di Giulio, Fernando Contreras, A. Aab, A. Dorofeev, G. Yuan, Igor Katkov, J. Stasielak, S. Coutu, L. Villaseñor, L. Martin, Marco Cilmo, C. Porowski, Denise Boncioli, German Ros, S. Jansen, Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Centre National de la Recherche Scientifique (CNRS), Unité Scientifique de la Station de Nançay (USN), Observatoire des Sciences de l'Univers en région Centre (OSUC), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS), Laboratoire SUBATECH Nantes (SUBATECH), Mines Nantes (Mines Nantes)-Université de Nantes (UN)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Institut de Physique Nucléaire d'Orsay (IPNO), Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de l'Accélérateur Linéaire (LAL), Pierre Auger, ANR-11-IDEX-0004,SUPER,Sorbonne Universités à Paris pour l'Enseignement et la Recherche(2011), European Project: 246806,EC:FP7:PEOPLE,FP7-PEOPLE-2009-IRSES,EPLANET(2011), Aab, A., Abreu, P., Aglietta, M., Ahn, E. . J., Al Samarai, I., Albuquerque, I. . F. . M., Allekotte, I., Allison, P., Almela, A., Alvarez Castillo, J., Alvarez Muñiz, J., Alves Batista, R., Ambrosio, M., Aminaei, A., Anchordoqui, L., Andringa, S., Aramo, C., Aranda, V. . M., Arqueros, F., Arsene, N., Asorey, H., Assis, P., Aublin, J., Ave, M., Avenier, M., Avila, G., Awal, N., Badescu, A. . M., Barber, K. . B., Bäuml, J., Baus, C., Beatty, J. . J., Becker, K. . H., Bellido, J. . A., Berat, C., Bertaina, M. . E., Bertou, X., Biermann, P. . L., Billoir, P., Blaess, S. . G., Blanco, A., Blanco, M., Bleve, Carla, Blümer, H., Boháčová, M., Boncioli, D., Bonifazi, C., Borodai, N., Brack, J., Brancus, I., Bridgeman, A., Brogueira, P., Brown, W. . C., Buchholz, P., Bueno, A., Buitink, S., Buscemi, M., Caballero Mora, K. . S., Caccianiga, B., Caccianiga, L., Candusso, M., Caramete, L., Caruso, R., Castellina, A., Cataldi, G., Cazon, L., Cester, R., Chavez, A. . G., Chiavassa, A., Chinellato, J. . A., Chudoba, J., Cilmo, M., Clay, R. . W., Cocciolo, G., Colalillo, R., Coleman, A., Collica, L., Coluccia, MARIA RITA, Conceição, R., Contreras, F., Cooper, M. . J., Cordier, A., Coutu, S., Covault, C. . E., Cronin, J., Dallier, R., Daniel, B., Dasso, S., Daumiller, K., Dawson, B. . R., de Almeida, R. . M., de Jong, S. . J., De Mauro, G., de Mello Neto, J. . R. . T., DE MITRI, Ivan, de Oliveira, J., de Souza, V., del Peral, L., Deligny, O., Dembinski, H., Dhital, N., Di Giulio, C., Di Matteo, A., Diaz, J. . C., Díaz Castro, M. . L., Diogo, F., Dobrigkeit, C., Docters, W., D’Olivo, J. . C., Dorofeev, A., Dorosti Hasankiadeh, Q., Dova, M. . T., Ebr, J., Engel, R., Erdmann, M., Erfani, M., Escobar, C. . O., Espadanal, J., Etchegoyen, A., Falcke, H., Fang, K., Farrar, G., Fauth, A. . C., Fazzini, N., Ferguson, A. . P., Fernandes, M., Fick, B., Figueira, J. . M., Filevich, A., Filipčič, A., Fox, B. . D., Fratu, O., Freire, M. . M., Fuchs, B., Fujii, T., García, B., Garcia Pinto, D., Gate, F., Gemmeke, H., Gherghel Lascu, A., Ghia, P. . L., Giaccari, U., Giammarchi, M., Giller, M., Głas, D., Glaser, C., Glass, H., Golup, G., Gómez Berisso, M., Gómez Vitale, P. . F., González, N., Gookin, B., Gordon, J., Gorgi, A., Gorham, P., Gouffon, P., Griffith, N., Grillo, A. . F., Grubb, T. . D., Guardincerri, Y., Guarino, F., Guedes, G. . P., Hampel, M. . R., Hansen, P., Harari, D., Harrison, T. . A., Hartmann, S., Harton, J. . L., Haungs, A., Hebbeker, T., Heck, D., Heimann, P., Herve, A. . E., Hill, G. . C., Hojvat, C., Hollon, N., Holt, E., Homola, P., Hörandel, J. . R., Horvath, P., Hrabovský, M., Huber, D., Huege, T., Insolia, A., Isar, P. . G., Jandt, I., Jansen, S., Jarne, C., Johnsen, J. . A., Josebachuili, M., Kääpä, A., Kambeitz, O., Kampert, K. . H., Kasper, P., Katkov, I., Kégl, B., Keilhauer, B., Keivani, A., Kemp, E., Kieckhafer, R. . M., Klages, H. . O., Kleifges, M., Kleinfeller, J., Krause, R., Krohm, N., Krömer, O., Kuempel, D., Kunka, N., Lahurd, D., Latronico, L., Lauer, R., Lauscher, M., Lautridou, P., Le Coz, S., Lebrun, D., Lebrun, P., Leigui de Oliveira, M. . A., Letessier Selvon, A., Lhenry Yvon, I., Link, K., Lopes, L., López, R., López Casado, A., Louedec, K., Lu, L., Lucero, A., Malacari, M., Maldera, S., Mallamaci, M., Maller, J., Mandat, D., Mantsch, P., Mariazzi, A. . G., Marin, V., Mariş, I. . C., Marsella, Giovanni, Martello, Daniele, Martin, L., Martinez, H., Martínez Bravo, O., Martraire, D., Masías Meza, J. . J., Mathes, H. . J., Mathys, S., Matthews, J., Matthews, J. . A. . J., Matthiae, G., Maurel, D., Maurizio, D., Mayotte, E., Mazur, P. . O., Medina, C., Medina Tanco, G., Meissner, R., Mello, V. . B. . B., Melo, D., Menshikov, A., Messina, S., Meyhandan, R., Micheletti, M. . I., Middendorf, L., Minaya, I. . A., Miramonti, L., Mitrica, B., Molina Bueno, L., Mollerach, S., Montanet, F., Morello, C., Mostafá, M., Moura, C. . A., Muller, M. . A., Müller, G., Müller, S., Mussa, R., Navarra, G., Navarro, J. . L., Navas, S., Necesal, P., Nellen, L., Nelles, A., Neuser, J., Nguyen, P. . H., Niculescu Oglinzanu, M., Niechciol, M., Niemietz, L., Niggemann, T., Nitz, D., Nosek, D., Novotny, V., Nožka, L., Ochilo, L., Oikonomou, F., Olinto, A., Pacheco, N., Pakk Selmi Dei, D., Palatka, M., Pallotta, J., Papenbreer, P., Parente, G., Parra, A., Paul, T., Pech, M., Pȩkala, J., Pelayo, R., Pepe, I. . M., Perrone, Lorenzo, Petermann, E., Peters, C., Petrera, S., Petrov, Y., Phuntsok, J., Piegaia, R., Pierog, T., Pieroni, P., Pimenta, M., Pirronello, V., Platino, M., Plum, M., Porcelli, A., Porowski, C., Prado, R. . R., Privitera, P., Prouza, M., Purrello, V., Quel, E. . J., Querchfeld, S., Quinn, S., Rautenberg, J., Ravel, O., Ravignani, D., Revenu, B., Ridky, J., Riggi, S., Risse, M., Ristori, P., Rizi, V., Rodrigues de Carvalho, W., Rodriguez Fernandez, G., Rodriguez Rojo, J., Rodríguez Frías, M. . D., Rogozin, D., Rosado, J., Roth, M., Roulet, E., Rovero, A. . C., Saffi, S. . J., Saftoiu, A., Salamida, F., Salazar, H., Saleh, A., Salesa Greus, F., Salina, G., Sánchez, F., Sanchez Lucas, P., Santos, E., Santos, E. . M., Sarazin, F., Sarkar, B., Sarmento, R., Sato, R., Scarso, C., Schauer, M., Scherini, Viviana, Schieler, H., Schiffer, P., Schmidt, D., Scholten, O., Schoorlemmer, H., Schovánek, P., Schröder, F. . G., Schulz, A., Schulz, J., Schumacher, J., Sciutto, S. . J., Segreto, A., Settimo, M., Shadkam, A., Shellard, R. . C., Sidelnik, I., Sigl, G., Sima, O., Śmiałkowski, A., Šmída, R., Snow, G. . R., Sommers, P., Sorokin, J., Squartini, R., Srivastava, Y. . N., Stanca, D., Stanič, S., Stapleton, J., Stasielak, J., Stephan, M., Stutz, A., Suarez, F., Suomijärvi, T., Supanitsky, A. . D., Sutherland, M. . S., Swain, J., Szadkowski, Z., Taborda, O. . A., Tapia, A., Tepe, A., Theodoro, V. . M., Tiffenberg, J., Timmermans, C., Todero Peixoto, C. . J., Toma, G., Tomankova, L., Tomé, B., Tonachini, A., Torralba Elipe, G., Torres Machado, D., Travnicek, P., Ulrich, R., Unger, M., Urban, M., Valdés Galicia, J. . F., Valiño, I., Valore, L., van Aar, G., van Bodegom, P., van den Berg, A. . M., van Velzen, S., van Vliet, A., Varela, E., Vargas Cárdenas, B., Varner, G., Vasquez, R., Vázquez, J. . R., Vázquez, R. . A., Veberič, D., Verzi, V., Vicha, J., Videla, M., Villaseñor, L., Vlcek, B., Vorobiov, S., Wahlberg, H., Wainberg, O., Walz, D., Watson, A. . A., Weber, M., Weidenhaupt, K., Weindl, A., Werner, F., Widom, A., Wiencke, L., Wilczyński, H., Winchen, T., Wittkowski, D., Wundheiler, B., Wykes, S., Yang, L., Yapici, T., Yushkov, A., Zas, E., Zavrtanik, D., Zavrtanik, M., Zepeda, A., Zhu, Y., Zimmermann, B., Ziolkowski, M., Zuccarello, F., Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Joseph Fourier - Grenoble 1 (UJF)-Centre National de la Recherche Scientifique (CNRS), Centre National de la Recherche Scientifique (CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire des Sciences de l'Univers en région Centre (OSUC), Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Université d'Orléans (UO)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Université d'Orléans (UO)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université d'Orléans (UO), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université de Nantes (UN)-Mines Nantes (Mines Nantes), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), Valore, Laura, Guarino, Fausto, Colalillo, Roberta, Mario, Buscemi, The Pierre Auger, Collaboration, Physics, Elementary Particle Physics, and Research unit Astroparticle Physics
Subjects: Astrofísica, Nuclear and High Energy Physics, [PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], Astronomy, FOS: Physical sciences, Cosmic ray, Astrophysics, 01 natural sciences, Declination, Observatory, 0103 physical sciences, Ultra-high-energy cosmic ray, astroparticle physics, cosmic rays, Cosmic rays, 010303 astronomy & astrophysics, Zenith, Ciencias Exactas, astroparticle physics, cosmic rays, High Energy Astrophysical Phenomena (astro-ph.HE), Pierre Auger Observatory, Physics, 010308 nuclear & particles physics, Física, Astronomy and Astrophysics, ASTROFÍSICA, Astroparticle physics, Azimuth, Space and Planetary Science, Experimental High Energy Physics, ComputingMethodologies_DOCUMENTANDTEXTPROCESSING, Astrophysics - High Energy Astrophysical Phenomena, Right ascension, physics
Abstract: We present the results of an analysis of the large angular scale distribution of the arrival directions of cosmic rays with energy above 4 EeV detected at the Pierre Auger Observatory including for the first time events with zenith angle between $60^\circ$ and $80^\circ$. We perform two Rayleigh analyses, one in the right ascension and one in the azimuth angle distributions, that are sensitive to modulations in right ascension and declination, respectively. The largest departure from isotropy appears in the $E > 8$ EeV energy bin, with an amplitude for the first harmonic in right ascension $r_1^\alpha =(4.4 \pm 1.0){\times}10^{-2}$, that has a chance probability $P(\ge r_1^\alpha)=6.4{\times}10^{-5}$, reinforcing the hint previously reported with vertical events alone., Comment: Text matching the published version, figure 3 corrected
Published: 2015
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23. Muons in air showers at the Pierre Auger Observatory

Author: D. Pakk Selmi-Dei, D. Maurizio, Johannes Schumacher, F. Salamida, Lorenzo Caccianiga, V. M. Theodoro, Y. Guardincerri, B. Tome, G. Müller, A. J. Matthews, R. Mussa, Alberto Daniel Supanitsky, A. Śmiałkowski, Markus Roth, C. Morello, Fausto Guarino, Matthias Kleifges, David Wittkowski, Germano Guedes, Danielle LaHurd, Olivier Deligny, Peter L. Biermann, Dusan Mandat, A. van Vliet, Eric Mayotte, Paolo Privitera, M. Gómez Berisso, R. C. Shellard, W. Docters, Yogendra N. Srivastava, M. I. Micheletti, E. Varela, N. Griffith, S. Grebe, M. Zavrtanik, Markus Risse, B. Wilczynska, R. Squartini, John L. Harton, Fred Sarazin, Lukas Nellen, T. Paul, Arnulfo Zepeda, R. Meyhandan, P. Abreu, Antonio Insolia, G. Torralba Elipe, F. Sánchez, Sergio Sciutto, L. Ochilo, D. Ravignani, G. Cocciolo, Eva Santos, R. Krause, Federico Suarez, B. Zamorano, Iván Sidelnik, Luis A. Anchordoqui, I. Al Samarai, Sasa Micanovic, Gaetano Salina, Rúben Conceição, L. Valore, Amin Aminaei, E.M. Holt, J. J. Beatty, Norbert Kunka, S. Messina, Azadeh Keivani, Ricardo Vázquez, W. Rodrigues de Carvalho, Maria Giller, A. Saleh, Maria-Teresa Dova, D. Nitz, Silvia Mollerach, B. Vlcek, H. Dembinski, G. Matthiae, M. Tartare, Darko Veberič, I. Zaw, M. Platino, M. Monasor, C. Aramo, J. W. Cronin, G. van Aar, Moritz Münchmeyer, R. Alves Batista, M. Ambrosio, G. C. Hill, Q. Dorosti Hasankiadeh, Tobias Winchen, P. Lebrun, Karen S. Caballero-Mora, B. Mitrica, Heino Falcke, Ralph Engel, V. Marin, Valerio Pirronello, L. Perrone, Sarka Wykes, Marco Giammarchi, J. Vicha, S. Quinn, A. Segreto, M. Ludwig, S. Hartmann, Jing Zhou, Julien Aublin, F. Werner, Jan Ridky, A. Stutz, P. Allison, V. Scherini, Martin Erdmann, G. Toma, Nataliia Borodai, E. J. Ahn, Paul Sommers, D. Martello, M. Blanco, R. Bonino, Michael Unger, S. Jansen, P. Gouffon, François Montanet, S. van Velzen, K. H. Becker, A. G. Mariazzi, K. Islo, Radomir Smida, Beatriz García, Octavian Fratu, D. Torres Machado, D. Melo, Roger W Clay, M. J. Cooper, A. Gorgi, Miroslav Palatka, S. J. De Jong, N. Krohm, Jose Chinellato, P. Lautridou, S. Navas, Johannes Schulz, M. Melissas, M. Will, B. Sarkar, Christian Glaser, M. Pimenta, Carlos Medina, M. De Domenico, Joshua A. Gordon, M. Avenier, A. Curutiu, A. Widom, Daniel Kuempel, M. Ave, Carlos Escobar, A. Filipčič, A. C. Rovero, Paula Gina Isar, C. Bleve, Pedro Brogueira, F. Salesa Greus, G. Cataldi, J. Espadanal, J. F. Valdés Galicia, I. De Mitri, A. Gascon Bravo, Dieter Heck, Martin Urban, V. de Souza, N. Palmieri, Ugo Giaccari, M. Zimbres Silva, A. Cordier, S. Maldera, P. W. Younk, Ivone F. M. Albuquerque, Ke Fang, C. J. Todero Peixoto, R. López, E. Trovato, J. Stapleton, Marc Weber, P. Billoir, Tanguy Pierog, M. E. Bertaina, Jörg R. Hörandel, G. Garilli, Lorenzo Cazon, Vincenzo Rizi, A. Menshikov, B. Gookin, S. T. Garcia Roca, Toshihiro Fujii, R. Sato, J. R. T. de Mello Neto, M. Ziolkowski, L. del Peral, O. Ravel, O. Martínez Bravo, E. M. Santos, K. Louedec, Mariangela Settimo, A. Shadkam, M. Buscemi, Maria Rita Coluccia, Alexey Yushkov, Bruno Daniel, K. Weidenhaupt, Bruce R. Dawson, N. Scharf, Antonio Bueno, M. Josebachuili, V. Purrello, P. Heimann, Tim Huege, H. Blümer, Max Malacari, Carlos Hojvat, D. Nosek, Juan Carlos D'Olivo, T. Yapici, D. Newton, Ernesto Kemp, Esteban Roulet, Piotr Homola, Lukas Middendorf, Jan Ebr, Serguei Vorobiov, Sergio Petrera, Christine Peters, J. J. Masías Meza, P. Facal San Luis, D. Maurel, H. Schoorlemmer, Gualberto Avila, Gustavo Medina-Tanco, Nicolás González, Ingomar Allekotte, S. Le Coz, D. Monnier Ragaigne, M. A. Leigui de Oliveira, T. Rossler, Piera Luisa Ghia, Guenter Sigl, Thomas Hebbeker, C. L. Williams, Angela V. Olinto, O. Krömer, O. A. Taborda, Sergio Dasso, Balázs Kégl, C. Di Giulio, S. J. Saffi, H. Martinez, G. Rodriguez Fernandez, A. P. Ferguson, Hernán Asorey, Corinne Berat, C. E. Santo, B. Revenu, U. Fröhlich, A. Tapia, C. Jarne, J. de Oliveira, J. R. Vázquez, Henryk Wilczyński, Hermann-Josef Mathes, Antoine Letessier-Selvon, van den Ad M Berg, Luca Latronico, Alejandro Almela, P. Sanchez-Lucas, D. Harari, M. Oliveira, Markus Lauscher, Kai Daumiller, J. Phuntsok, M. Videla, V. M. Aranda, Jeffrey Brack, Olaf Scholten, Humberto Ibarguen Salazar, Raul Sarmento, A. Aab, F. Gate, L. Caramete, H. Gemmeke, L. Tomankova, M. Mallamaci, G. Navarra, C. A. Moura, T. Yamamoto, Brian Fick, Samo Stanič, J. Lozano Bahilo, John Swain, Philipp Papenbreer, J. S. Díaz, D. Garcia-Pinto, Petr Travnicek, Alan Coleman, Trent D. Grubb, D. Huber, Petr Schovanek, Carla Bonifazi, Juan Manuel Figueira, Roberta Colalillo, Jose A. Bellido, M. Prouza, G. Yuan, Corbin Covault, Y. Petrov, Matías Rolf Hampel, J. A.J. Matthews, Xavier Bertou, J. Rodriguez Rojo, Bianca Keilhauer, A. G. Chavez, Pedro Assis, S. Riggi, Jaime Rosado, Alina Mihaela Badescu, F.G. Schröder, Enrique Zas, I. M. Pepe, Alexander Grillo, J. Stasielak, R. Cester, S. Coutu, Norberto Fazzini, Lino Miramonti, Fernando Contreras, M. D. Rodríguez-Frías, M. A. Muller, Peter Schiffer, Paulo J. S. Gonçalves, D. Kruppke-Hansen, D. Garcia-Gamez, Alberto Etchegoyen, I. C. Mariş, J. Allen, Hernan Wahlberg, C. Porowski, Alexandra Saftoiu, A. Dorofeev, I. Jandt, A. Tepe, I. Lhenry-Yvon, Octavian Sima, J. G. Gonzalez, Ralf Ulrich, Igor Katkov, R. R. Prado, Denise Boncioli, German Ros, A. Di Matteo, Paul M. Mantsch, B. Wundheiler, A. Parra, L. Villaseñor, Miguel Mostafá, Marcus Niechciol, Anderson Fauth, Gregory R Snow, P. H. Kasper, L. Martin, M. S. A. B. Leão, D. Lebrun, R. J. Lauer, L. Nožka, G. Parente, R. Piegaia, Marco Cilmo, P. Ristori, Alex Kääpä, Peter Mazur, S. Querchfeld, Colin Baus, V. M. Olmos-Gilbaja, L. Niemietz, N. Pacheco, J. Roberts, Tim Niggemann, Yingchun Zhu, H. Schieler, M. Fernandes, B. Caccianiga, Karl-Heinz Kampert, Antonella Castellina, B. Vargas Cárdenas, R. M. Kieckhafer, J. Rautenberg, T. Suomijärvi, J. Pallotta, G. S. Varner, O. Wainberg, E. J. Quel, Béatrice Fuchs, Niraj Dhital, W. C. Brown, I. Valiño, J. Neuser, M. Candusso, Peter Gorham, Charles Timmermans, L. Collica, Jiri Chudoba, Thomas Harrison, Richard Dallier, A. Nelles, Jaime Alvarez-Muñiz, Lu Lu, P. Pieroni, I. A. Minaya, André Schulz, F. Arqueros, P. Necesal, Martina Bohacova, Jan Pękala, Hans Klages, A. Chiavassa, A. E. Herve, K. B. Barber, L. R. Wiencke, J. Sorokin, A. Porcelli, B. D. Fox, M. L. Díaz Castro, G. Farrar, Francesca Zuccarello, Maurice Stephan, A. Tonachini, P.F. Gómez Vitale, J. Maller, G. Marsella, A. Weindl, N. Hollon, V. Verzi, V. Novotny, J. Bäuml, Rossella Caruso, A. Lucero, S. Mathys, M. Erfani, E. Petermann, Miroslav Pech, Pavel Horvath, M. S. Sutherland, Danilo Zavrtanik, Sofia Andringa, K. Link, D. Martraire, Miroslav Hrabovský, A. Haungs, O. Kambeitz, F. Diogo, R. M. de Almeida, Zbigniew Szadkowski, Rodrigo Pelayo, Stijn Buitink, Alberto Filevich, Peter Hansen, R. Gaior, Peter Buchholz, M. Szuba, I.M. Brancus, Carola Dobrigkeit, H. Glass, M. Plum, Marco Aglietta, Alan Watson, Jonny Kleinfeller, J. Alvarez Castillo, L. Molina-Bueno, David Walz, Laboratoire de Physique Subatomique et de Cosmologie ( LPSC ), Université Joseph Fourier - Grenoble 1 ( UJF ) -Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Centre National de la Recherche Scientifique ( CNRS ) -Université Grenoble Alpes ( UGA ), Unité Scientifique de la Station de Nançay ( USN ), Observatoire de Paris-Université d'Orléans ( UO ) -Centre National de la Recherche Scientifique ( CNRS ), Laboratoire SUBATECH Nantes ( SUBATECH ), Mines Nantes ( Mines Nantes ) -Université de Nantes ( UN ) -Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Centre National de la Recherche Scientifique ( CNRS ), Laboratoire de l'Accélérateur Linéaire ( LAL ), Université Paris-Sud - Paris 11 ( UP11 ) -Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Centre National de la Recherche Scientifique ( CNRS ), Institut de Physique Nucléaire d'Orsay ( IPNO ), Pierre AUGER, ANR-10-LABX-63,ANR-10-LABX-63, European Project : 328826,EC:FP7:PEOPLE,FP7-PEOPLE-2012-IEF,AUGER2FUTURE ( 2013 ), European Project : 246806,EC:FP7:PEOPLE,FP7-PEOPLE-2009-IRSES,EPLANET ( 2011 ), UNIVERSIDADE DE ESTADUAL DE CAMPINAS, Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Joseph Fourier - Grenoble 1 (UJF)-Centre National de la Recherche Scientifique (CNRS), Unité Scientifique de la Station de Nançay (USN), Centre National de la Recherche Scientifique (CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire des Sciences de l'Univers en région Centre (OSUC), Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Université d'Orléans (UO)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Université d'Orléans (UO)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université d'Orléans (UO), Laboratoire SUBATECH Nantes (SUBATECH), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université de Nantes (UN)-Mines Nantes (Mines Nantes), Laboratoire de l'Accélérateur Linéaire (LAL), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), Institut de Physique Nucléaire d'Orsay (IPNO), ANR-10-LABX-0063,ILP,Institute Lagrange of Paris(2010), European Project: 328826,EC:FP7:PEOPLE,FP7-PEOPLE-2012-IEF,AUGER2FUTURE(2013), European Project: 246806,EC:FP7:PEOPLE,FP7-PEOPLE-2009-IRSES,EPLANET(2011), Aab A., Abreu P., Aglietta M., Ahn E. J., Al Samarai I., Albuquerque I. F. M., Allekotte I., Allison P., Almela A., Alvarez Castillo J., Alvarez-Muñiz J., Alves Batista R., Ambrosio M., Aminaei A., Anchordoqui L., Andringa S., Aramo C., Aranda V. M., Arqueros F., Arsene N., Asorey H., Assis P., Aublin J., Ave M., Avenier M., Avila G., Awal N., Badescu A. M., Barber K. B., Bäuml J., Baus C., Beatty J. J., Becker K. H., Bellido J. A., Berat C., Bertaina M. E., Bertou X., Biermann P. L., Billoir P., Blaess S. G., Blanco A., Blanco M., Bleve C., Blümer H., Boháčová M., Boncioli D., Bonifazi C., Borodai N., Brack J., Brancus I., Bridgeman A., Brogueira P., Brown W. C., Buchholz P., Bueno A., Buitink S., Buscemi M., Caballero-Mora K. S., Caccianiga B., Caccianiga L., Candusso M., Caramete L., Caruso R., Castellina A., Cataldi G., Cazon L., Cester R., Chavez A. G., Chiavassa A., Chinellato J. A., Chudoba J., Cilmo M., Clay R. W., Cocciolo G., Colalillo R., Coleman A., Collica L., Coluccia M. R., Conceição R., Contreras F., Cooper M. J., Cordier A., Coutu S., Covault C. E., Cronin J., Dallier R., Daniel B., Dasso S., Daumiller K., Dawson B. R., de Almeida R. M., de Jong S. J., De Mauro G., de Mello Neto J. R. T., De Mitri I., de Oliveira J., de Souza V., del Peral L., Deligny O., Dembinski H., Dhital N., Di Giulio C., Di Matteo A., Diaz J. C., Díaz Castro M. L., Diogo F., Dobrigkeit C., Docters W., D’Olivo J. C., Dorofeev A., Dorosti Hasankiadeh Q., Dova M. T., Ebr J., Engel R., Erdmann M., Erfani M., Escobar C. O., Espadanal J., Etchegoyen A., Falcke H., Fang K., Farrar G., Fauth A. C., Fazzini N., Ferguson A. P., Fernandes M., Fick B., Figueira J. M., Filevich A., Filipčič A., Fox B. D., Fratu O., Freire M. M., Fuchs B., Fujii T., García B., Garcia-Pinto D., Gate F., Gemmeke H., Gherghel-Lascu A., Ghia P. L., Giaccari U., Giammarchi M., Giller M., Głas D., Glaser C., Glass H., Golup G., Gómez Berisso M., Gómez Vitale P. F., González N., Gookin B., Gordon J., Gorgi A., Gorham P., Gouffon P., Griffith N., Grillo A. F., Grubb T. D., Guardincerri Y., Guarino F., Guedes G. P., Hampel M. R., Hansen P., Harari D., Harrison T. A., Hartmann S., Harton J. L., Haungs A., Hebbeker T., Heck D., Heimann P., Herve A. E., Hill G. C., Hojvat C., Hollon N., Holt E., Homola P., Hörandel J. R., Horvath P., Hrabovský M., Huber D., Huege T., Insolia A., Isar P. G., Jandt I., Jansen S., Jarne C., Johnsen J. A., Josebachuili M., Kääpä A., Kambeitz O., Kampert K. H., Kasper P., Katkov I., Kégl B., Keilhauer B., Keivani A., Kemp E., Kieckhafer R. M., Klages H. O., Kleifges M., Kleinfeller J., Krause R., Krohm N., Krömer O., Kuempel D., Kunka N., LaHurd D., Latronico L., Lauer R., Lauscher M., Lautridou P., Le Coz S., Lebrun D., Lebrun P., Leigui de Oliveira M. A., Letessier-Selvon A., Lhenry-Yvon I., Link K., Lopes L., López R., López Casado A., Louedec K., Lu L., Lucero A., Malacari M., Maldera S., Mallamaci M., Maller J., Mandat D., Mantsch P., Mariazzi A. G., Marin V., Mariş I. C., Marsella G., Martello D., Martin L., Martinez H., Martínez Bravo O., Martraire D., Masías Meza J. J., Mathes H. J., Mathys S., Matthews J., Matthews J. A. J., Matthiae G., Maurel D., Maurizio D., Mayotte E., Mazur P. O., Medina C., Medina-Tanco G., Meissner R., Mello V. B. B., Melo D., Menshikov A., Messina S., Meyhandan R., Micheletti M. I., Middendorf L., Minaya I. A., Miramonti L., Mitrica B., Molina-Bueno L., Mollerach S., Montanet F., Morello C., Mostafá M., Moura C. A., Muller M. A., Müller G., Müller S., Mussa R., Navarra G., Navarro J. L., Navas S., Necesal P., Nellen L., Nelles A., Neuser J., Nguyen P. H., Niculescu-Oglinzanu M., Niechciol M., Niemietz L., Niggemann T., Nitz D., Nosek D., Novotny V., Nožka L., Ochilo L., Oikonomou F., Olinto A., Pacheco N., Pakk Selmi-Dei D., Palatka M., Pallotta J., Papenbreer P., Parente G., Parra A., Paul T., Pech M., Pȩkala J., Pelayo R., Pepe I. M., Perrone L., Petermann E., Peters C., Petrera S., Petrov Y., Phuntsok J., Piegaia R., Pierog T., Pieroni P., Pimenta M., Pirronello V., Platino M., Plum M., Porcelli A., Porowski C., Prado R. R., Privitera P., Prouza M., Purrello V., Quel E. J., Querchfeld S., Quinn S., Rautenberg J., Ravel O., Ravignani D., Revenu B., Ridky J., Riggi S., Risse M., Ristori P., Rizi V., Rodrigues de Carvalho W., Rodriguez Fernandez G., Rodriguez Rojo J., Rodríguez-Frías M. D., Rogozin D., Rosado J., Roth M., Roulet E., Rovero A. C., Saffi S. J., Saftoiu A., Salamida F., Salazar H., Saleh A., Salesa Greus F., Salina G., Sánchez F., Sanchez-Lucas P., Santos E., Santos E. M., Sarazin F., Sarkar B., Sarmento R., Sato R., Scarso C., Schauer M., Scherini V., Schieler H., Schiffer P., Schmidt D., Scholten O., Schoorlemmer H., Schovánek P., Schröder F. G., Schulz A., Schulz J., Schumacher J., Sciutto S. J., Segreto A., Settimo M., Shadkam A., Shellard R. C., Sidelnik I., Sigl G., Sima O., Śmiałkowski A., Šmída R., Snow G. R., Sommers P., Sorokin J., Squartini R., Srivastava Y. N., Stanca D., Stanič S., Stapleton J., Stasielak J., Stephan M., Stutz A., Suarez F., Suomijärvi T., Supanitsky A. D., Sutherland M. S., Swain J., Szadkowski Z., Taborda O. A., Tapia A., Tepe A., Theodoro V. M., Tiffenberg J., Timmermans C., Todero Peixoto C. J., Toma G., Tomankova L., Tomé B., Tonachini A., Torralba Elipe G., Torres Machado D., Travnicek P., Ulrich R., Unger M., Urban M., Valdés Galicia J. F., Valiño I., Valore L., van Aar G., van Bodegom P., van den Berg A. M., van Velzen S., van Vliet A., Varela E., Vargas Cárdenas B., Varner G., Vasquez R., Vázquez J. R., Vázquez R. A., Veberič D., Verzi V., Vicha J., Videla M., Villaseñor L., Vlcek B., Vorobiov S., Wahlberg H., Wainberg O., Walz D., Watson A. A., Weber M., Weidenhaupt K., Weindl A., Werner F., Widom A., Wiencke L., Wilczyński H., Winchen T., Wittkowski D., Wundheiler B., Wykes S., Yang L., Yapici T., Yushkov A., Zas E., Zavrtanik D., Zavrtanik M., Zepeda A., Zhu Y., Zimmermann B., Ziolkowski M., Zuccarello F., Aab, A., Abreu, P., Aglietta, M., Ahn, E. . J., Al Samarai, I., Albuquerque, I. . F. . M., Allekotte, I., Allison, P., Almela, A., Alvarez Castillo, J., Alvarez Muñiz, J., Alves Batista, R., Ambrosio, M., Aminaei, A., Anchordoqui, L., Andringa, S., Aramo, C., Aranda, V. . M., Arqueros, F., Arsene, N., Asorey, H., Assis, P., Aublin, J., Ave, M., Avenier, M., Avila, G., Awal, N., Badescu, A. . M., Barber, K. . B., Bäuml, J., Baus, C., Beatty, J. . J., Becker, K. . H., Bellido, J. . A., Berat, C., Bertaina, M. . E., Bertou, X., Biermann, P. . L., Billoir, P., Blaess, S. . G., Blanco, A., Blanco, M., Bleve, Carla, Blümer, H., Boháčová, M., Boncioli, D., Bonifazi, C., Borodai, N., Brack, J., Brancus, I., Bridgeman, A., Brogueira, P., Brown, W. . C., Buchholz, P., Bueno, A., Buitink, S., Buscemi, M., Caballero Mora, K. . S., Caccianiga, B., Caccianiga, L., Candusso, M., Caramete, L., Caruso, R., Castellina, A., Cataldi, G., Cazon, L., Cester, R., Chavez, A. . G., Chiavassa, A., Chinellato, J. . A., Chudoba, J., Cilmo, M., Clay, R. . W., Cocciolo, G., Colalillo, R., Coleman, A., Collica, L., Coluccia, MARIA RITA, Conceição, R., Contreras, F., Cooper, M. . J., Cordier, A., Coutu, S., Covault, C. . E., Cronin, J., Dallier, R., Daniel, B., Dasso, S., Daumiller, K., Dawson, B. . R., de Almeida, R. . M., de Jong, S. . J., De Mauro, G., de Mello Neto, J. . R. . T., DE MITRI, Ivan, de Oliveira, J., de Souza, V., del Peral, L., Deligny, O., Dembinski, H., Dhital, N., Di Giulio, C., Di Matteo, A., Diaz, J. . C., Díaz Castro, M. . L., Diogo, F., Dobrigkeit, C., Docters, W., D’Olivo, J. . C., Dorofeev, A., Dorosti Hasankiadeh, Q., Dova, M. . T., Ebr, J., Engel, R., Erdmann, M., Erfani, M., Escobar, C. . O., Espadanal, J., Etchegoyen, A., Falcke, H., Fang, K., Farrar, G., Fauth, A. . C., Fazzini, N., Ferguson, A. . P., Fernandes, M., Fick, B., Figueira, J. . M., Filevich, A., Filipčič, A., Fox, B. . D., Fratu, O., Freire, M. . M., Fuchs, B., Fujii, T., García, B., Garcia Pinto, D., Gate, F., Gemmeke, H., Gherghel Lascu, A., Ghia, P. . L., Giaccari, U., Giammarchi, M., Giller, M., Głas, D., Glaser, C., Glass, H., Golup, G., Gómez Berisso, M., Gómez Vitale, P. . F., González, N., Gookin, B., Gordon, J., Gorgi, A., Gorham, P., Gouffon, P., Griffith, N., Grillo, A. . F., Grubb, T. . D., Guardincerri, Y., Guarino, F., Guedes, G. . P., Hampel, M. . R., Hansen, P., Harari, D., Harrison, T. . A., Hartmann, S., Harton, J. . L., Haungs, A., Hebbeker, T., Heck, D., Heimann, P., Herve, A. . E., Hill, G. . C., Hojvat, C., Hollon, N., Holt, E., Homola, P., Hörandel, J. . R., Horvath, P., Hrabovský, M., Huber, D., Huege, T., Insolia, A., Isar, P. . G., Jandt, I., Jansen, S., Jarne, C., Johnsen, J. . A., Josebachuili, M., Kääpä, A., Kambeitz, O., Kampert, K. . H., Kasper, P., Katkov, I., Kégl, B., Keilhauer, B., Keivani, A., Kemp, E., Kieckhafer, R. . M., Klages, H. . O., Kleifges, M., Kleinfeller, J., Krause, R., Krohm, N., Krömer, O., Kuempel, D., Kunka, N., Lahurd, D., Latronico, L., Lauer, R., Lauscher, M., Lautridou, P., Le Coz, S., Lebrun, D., Lebrun, P., Leigui de Oliveira, M. . A., Letessier Selvon, A., Lhenry Yvon, I., Link, K., Lopes, L., López, R., López Casado, A., Louedec, K., Lu, L., Lucero, A., Malacari, M., Maldera, S., Mallamaci, M., Maller, J., Mandat, D., Mantsch, P., Mariazzi, A. . G., Marin, V., Mariş, I. . C., Marsella, Giovanni, Martello, Daniele, Martin, L., Martinez, H., Martínez Bravo, O., Martraire, D., Masías Meza, J. . J., Mathes, H. . 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A., Weber, M., Weidenhaupt, K., Weindl, A., Werner, F., Widom, A., Wiencke, L., Wilczyński, H., Winchen, T., Wittkowski, D., Wundheiler, B., Wykes, S., Yang, L., Yapici, T., Yushkov, A., Zas, E., Zavrtanik, D., Zavrtanik, M., Zepeda, A., Zhu, Y., Zimmermann, B., Ziolkowski, M., Zuccarello, F., Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Centre National de la Recherche Scientifique (CNRS), Observatoire des Sciences de l'Univers en région Centre (OSUC), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS), Mines Nantes (Mines Nantes)-Université de Nantes (UN)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), M., Ambrosio, Aramo, Carla, Buscemi, Mario, Cilmo, Marco, Colalillo, Roberta, Guarino, Fausto, Valore, Laura, The Pierre Auger, Collaboration, Research unit Astroparticle Physics, and Research unit Nuclear & Hadron Physics
Subjects: [PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], Nuclear and High Energy Physics, Physics::Instrumentation and Detectors, Cosmic-ray interactions, Astronomy, Astrophysics::High Energy Astrophysical Phenomena, FOS: Physical sciences, Cosmic ray, extensive atmospherical showers, muon density, muon number, Pierre Auger Observatory, cosmic radiation UHE, Hadronic interaction models, 7. Clean energy, Auger, Settore FIS/04 - Fisica Nucleare e Subnucleare, Nuclear physics, Altitude, Settore FIS/05 - Astronomia e Astrofisica, Observatory, NERGY COSMIC-RAYS, DETECTOR, MODEL, Extensive air showers, cosmic radiation UHE, DETECTOR, Scaling, Cosmic rays, Zenith, High Energy Astrophysical Phenomena (astro-ph.HE), Physics, Pierre Auger Observatory, Muon, NERGY COSMIC-RAYS, Settore FIS/01 - Fisica Sperimentale, energy cosmic-rays, detector, model, Astrophysics::Instrumentation and Methods for Astrophysics, Física, [ PHYS.ASTR.HE ] Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], ASTROFÍSICA, extensive atmospherical showers, muon number, MODEL, muon density, Experimental High Energy Physics, ComputingMethodologies_DOCUMENTANDTEXTPROCESSING, Física nuclear, High Energy Physics::Experiment, Astrophysics - High Energy Astrophysical Phenomena
Abstract: We present the first hybrid measurement of the average muon number in air showers at ultrahigh energies, initiated by cosmic rays with zenith angles between 62° and 80°. The measurement is based on 174 hybrid events recorded simultaneously with the surface detector array and the fluorescence detector of the Pierre Auger Observatory. The muon number for each shower is derived by scaling a simulated reference profile of the lateral muon density distribution at the ground until it fits the data. A 1019eV shower with a zenith angle of 67°, which arrives at the surface detector array at an altitude of 1450 m above sea level, contains on average (2.68±0.04±0.48(sys))×107 muons with energies larger than 0.3 GeV. The logarithmic gain dlnNμ/dlnE of muons with increasing energy between 4×1018eV and 5×1019eV is measured to be (1.029±0.024±0.030(sys))., La lista completa de autores que integran el documento puede consultarse en el archivo, Instituto de Física La Plata
Published: 2015
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24. The KASCADE-Grande observatory and the composition of very high-energy cosmic rays

Author: A. Weindl, H. Rebel, T. Huege, B. Mitrica, K. Link, J. C. Arteaga-Velázquez, D. Kang, P. Łuczak, A. Haungs, N. Palmieri, H.O. Klages, K. Bekk, Béatrice Fuchs, J. Blümer, J. Zabierowski, G.C. Trinchero, A. Chiavassa, H. Schieler, H. Ulrich, H. J. Mathes, F. Cossavella, R. Glasstetter, Kai Daumiller, Claus Grupen, Jörg R. Hörandel, C. Morello, K. H. Kampert, V. de Souza, F.G. Schröder, S. Ostapchenko, H.J. Gils, P. Doll, J. Wochele, Octavian Sima, M. Ludwig, D. Heck, G. Toma, Markus Roth, J. Engler, D. Huber, H.J. Mayer, Ralph Engel, E. Cantoni, F. Di Pierro, W. D. Apel, T. Pierog, M. Melissas, J. Oehlschläger, D. Fuhrmann, M. E. Bertaina, I.M. Brancus, J. Milke, M. Petcu, and H. Bozdog
Subjects: Physics, History, Range (particle radiation), Muon, Astrophysics::High Energy Astrophysical Phenomena, Astronomy, Chemie, Astrophysics::Instrumentation and Methods for Astrophysics, Cosmic ray, Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, Charged particle, Computer Science Applications, Education, KASCADE, Observatory, Cosmic infrared background, ddc:530, Ultra-high-energy cosmic ray, GeneralLiterature_REFERENCE(e.g.,dictionaries,encyclopedias,glossaries)
Abstract: KASCADE-Grande is an air-shower observatory devoted to the detection of cosmic rays with energies in the range of 1016 to 1018 eV. This energy region is of particular interest for the cosmic ray astrophysics, since it is the place where some models predict the existence of a transition from galactic to extragalactic origin of cosmic rays and the presence of a break in the flux of its heavy component. The detection of these features requires detailed and simultaneous measurements of the energy and composition of cosmic rays with sufficient statistics. These kinds of studies are possible for the first time in KASCADE-Grande due to the accurate measurements of several air-shower observables, i.e., the number of charged particles, electrons and muons in the shower, using the different detector systems of the observatory. In this contribution, a detailed look into the composition of 1016 — 1018 eV cosmic rays with KASCADE-Grande is presented.
Published: 2015

25. LOPES — Recent Results and Open Questions on the Radio Detection of Air Showers

Author: M. Melissas, A. Horneffer, J. C. Arteaga-Velázquez, J. Oehlschläger, D. Kang, K. Link, G.C. Trinchero, Heino Falcke, A. Schmidt, A. Haungs, J. Zabierowski, Kai Daumiller, V. de Souza, H. Rebel, E. Cantoni, D. Huber, A. Weindl, J. Wochele, A. Saftoiu, S. Schoo, T. Pierog, Jan Kuijpers, Octavian Sima, Jörg R. Hörandel, H. Schieler, J. A. Zensus, D. Heck, M. E. Bertaina, Ralph Engel, P. Doll, H. J. Mathes, K. Bekk, F.G. Schröder, H. Gemmeke, L. Bähren, I.M. Brancus, Béatrice Fuchs, G. Toma, M. Ludwig, J. Rautenberg, C. Morello, F. Di Pierro, H. Bozdog, K. H. Kampert, C. Rühle, W. D. Apel, Peter L. Biermann, J. Blümer, Markus Roth, C. Grupen, A. Chiavassa, O. Krömer, Paula Gina Isar, Tim Huege, P. Łuczak, and N. Palmieri
Subjects: Beamforming, Wavefront, Physics, History, LOPES, business.industry, Astronomy, Computer Science Applications, Education, Antenna array, Interferometry, Optics, Amplitude, Antenna (radio), business, GeneralLiterature_REFERENCE(e.g.,dictionaries,encyclopedias,glossaries), Energy (signal processing)
Abstract: LOPES was a digital antenna array operating for approximately 10 years until spring 2013 at the Karlsruhe Institute of Technology (KIT). Triggered by the co-located KASCADE-Grande air-shower experiment, it measured the radio signal of around 1000 cosmic-ray air showers with energies E ≳ 1017 eV in an effective band of 43 - 74 MHz. Using the interferometric technique of cross-correlation beamforming, LOPES could reconstruct the shower direction with an accuracy < 0.7°, the shower energy with a precision < 20%, and the atmospheric depth of the shower maximum, Xmax, with a precision < 95g/cm2. In particular the reconstruction of the shower maximum suffers from significant measurement uncertainties due to the radio-loud environment of the site. This article summarizes our latest results on the reconstruction of the shower maximum, using two independent methods: the steepness of the hyperbolic radio wavefront and the slope of the lateral distribution of the radio amplitude. Moreover, we show vectorial measurements of the electric field with the tripole antennas of the latest LOPES setup. Finally, we discuss open questions as well as the potential impact of the lessons learned at LOPES for future antenna arrays.
Published: 2015

26. The Pierre Auger cosmic ray observatory

Author: A. Haungs, F. Diogo, R. M. de Almeida, J. L. Harton, Harm Schoorlemmer, F. Arneodo, Stijn Buitink, S. Westerhoff, Z. Szadkowski, F. Salamida, Carola Dobrigkeit, M. Plum, M. Chiosso, M. E. Bertaina, S. G. Blaes, Alan Watson, J. Alvarez Castillo, D. Nicotra, Paul Sommers, P. Gouffon, M. J. Cooper, Dragos Varnav, C. Aramo, Carlos Medina, M. De Domenico, M. Sutter, Maria Rita Coluccia, Bruno Daniel, Q. Dorosti Hasankiadeh, T. Yapici, Foteini Oikonomou, J. J. Masías Meza, D. Maurel, Luis Villaseñor, P. Abreu, D. Ravignani, Yingchun Zhu, B. Mitrica, Heino Falcke, J. Vicha, G. Cocciolo, B. Genolini, Luis A. Anchordoqui, M. Ambrosio, G. S. Varner, H. Gemmeke, M. Monasor, M. Iarlori, C. E. Santo, L. Martina, Yogendra N. Srivastava, Andreas Kopmann, E. J. Ahn, V. Tunnicliffe, A. F. Barbosa, Dusan Mandat, Martina Bohacova, Patrick Allison, E. Varela, N. Griffith, J. Sorokin, M. Boratav, B. Revenua, T. Porter, G. Torralba Elipe, A. Gorgi, Peter Schiffer, Benedikt Zimmermann, Rúben Conceição, R. Vasquez, Pascal Lautridou, D. V. Camin, Luis N. Epele, M. Blanco, V. Scherini, Alexandra Saftoiu, O. Kambeitz, H. Martinez, A. Di Matteo, N. Martínez, N. Palmieri, B. Wundheiler, D. Nitz, I. Lhenry-Yvon, Eva Santos, R. Krause, Vincent Marin, P. Walker, Gregory R Snow, Jan Pękala, A. Chiavassa, A. Menshikov, R. Habraken, M. S. A. B. Leão, J. D. Swain, Philipp Papenbreer, Petr Travnicek, John Kelley, S. Mueller, R. Bilhaut, Alan Coleman, M. Roberts, L. Ochilo, Federico Suarez, L. Valore, Amin Aminaei, A. E. Herve, K. B. Barber, L. R. Wiencke, K. Weidenhaupt, C. O. Escobar, A. Insolia, M. Kleifges, D. Zavrtanik, Trent D. Grubb, D. Huber, L. Nellen, Juan Manuel Figueira, A. Dorofeev, M. Melissas, Peter Mazur, Thomas Hebbeker, Joshua A. Gordon, R. A. Vázquez, A. Schmidt, Sergio Dasso, Denis Tcherniakhovski, Roberta Colalillo, John N. Matthews, R. M. Kieckhafer, A. G. Mariazzi, Igor Katkov, M. Muenchmeyer, V. Novotny, A. F. Grillo, G. P. Guedes, Rossella Caruso, Toshihiro Fujii, G. Sequeiros, J. Rautenberg, A. Lucero, J. R. Hoerandel, F. Sanchez, O. Wainberg, Stefano Argiro, S. Mathys, C. Morello, K. D. de Vries, Matthias Balzer, J. A.J. Matthews, F. Schreuder, F. Sarazin, W. Fulgione, W. C. Brown, Patricia María Hansen, Richard Dallier, A. Nelles, M. Erfani, L. Molina-Bueno, D. Melo, H. Verkooijen, T. Pierog, Marco Giammarchi, T. Ohnuki, David Walz, V. Pirronello, J. F. Valdés Galicia, I. De Mitri, A. Gascon Bravo, Iuri Muniz Pepe, Jaime Alvarez-Muñiz, Pedro Assis, A. Etchegoyen, Esteban Roulet, R. Randriatoamanana, C. Jarne, A. Stutz, P. L. Ghia, J. N. Albert, M. Horvat, Marco Cilmo, Arnulfo Zepeda, Alberto Daniel Supanitsky, Lu Lu, R. Sato, Octavian Sima, J. G. Gonzalez, A. Tepe, Dariusz Gora, Peter L. Biermann, R. Mussa, J. J. Beatty, Manuel Platino, J. Grygar, M. A. Leigui de Oliveira, F. Schroeder, Jeffrey A. Johnsen, F. Werner, J. Knapp, J. R. Vázquez, D. Garcia-Gamez, S. Quinn, D. PakkSelmi-Dei, G. Matthiae, T. Rossler, A. Bridgeman, Antonio Bueno, A. Segreto, Günter Sigl, Silvia Mollerach, J. Coppens, Markus Roth, H. Dembinski, H. Vorenholt, I. A. Minaya, B. Keilhauer, E. Petermann, S. J. Saffi, T. Wijnen, P. Sanchez-Lucas, G. Garilli, D. Maurizio, D. Garcia-Pinto, M. Risse, Paolo Privitera, H. Hucker, J. Allen, André Schulz, P. Kasper, S. J. Sciutto, Radomir Smida, Kai Daumiller, G. Mueller, D. Heck, R. Meyhandan, V. Purrello, M. Josebachuili, J. C. Diaz, Alberto Filevich, F. Guarino, Lorenzo Caccianiga, V. M. Theodoro, S. Colonges, B. D. Fox, Markus Lauscher, B. Zamorano, J. Pouryamout, A. Ferrero, Julien Aublin, A. Shadkam, F. Bracci, Florian Gaté, G. Parente, J. Phuntsok, Raul Sarmento, Carlos Hojvat, O. Kroemer, S. J. De Jong, Marcio Aparecido Muller, Peter Buchholz, M. M. Freire, Jeffrey Brack, Olaf Scholten, T. N. Trung, Humberto Ibarguen Salazar, V. de Souza, A. Curutiu, S. Sánchez Navas, T. Asch, H. J. 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Robbins, Michael Unger, S. Jansen, M. Fernandes, J. R. T. de Mello Neto, A. G. K. Smith, Maria-Teresa Dova, M. R. Hampel, R. Alves Batista, G. C. Hill, D. Torres Machado, Miroslav Pech, Colin Baus, Thomas Harrison, Ralph Engel, J. Ridky, N. Barenthien, Pavel Horvath, P. Pieroni, H. Schieler, Sarka Wykes, Karl-Heinz Kampert, Antonella Castellina, Heiko Geenen, C. Pryke, Jing Zhou, F. Arqueros, P. Necesal, M. S. Sutherland, R. Meissner, B. Vargas Cárdenas, S. van Velzen, K. H. Becker, N. Guardone, L. Guglielmi, M. Videla, J. Pallotta, K. Louedec, David Wittkowski, M. Urban, A. C. Rovero, Paula Gina Isar, C. Bleve, E. J. Quel, Pedro Brogueira, F. Salesa Greus, T. Bergmann, G. Cataldi, A. Filipcic, Azadeh Keivani, Béatrice Fuchs, Niraj Dhital, Octavian Fratu, W. Gotink, I. Valiño, D. Lebrun, U. Froehlich, G. Salina, Danielle LaHurd, Olivier Deligny, Nicolás González, W. Rodrigues de Carvalho, Sofia Andringa, J. W. Cronin, R. Speelman, P. van Bodegom, P. Lebrun, K. Gibbs, M. Palatka, A. 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Querchfeld, R. López, Karen S. Caballero-Mora, A. Castera, L. Niemietz, B. Caccianiga, N. Pacheco, A. Porcelli, Tim Niggemann, M. Mallamaci, M. Ludwig, S. Hartmann, Martin Erdmann, G. Yuan, M. L. Díaz Castro, G. Farrar, G. Vitali, Francesca Zuccarello, Roger W Clay, Maurice Stephan, Johannes Schulz, M. Ave, J. Pouthas, M. Pimenta, P. Clark, A. Tonachini, C. Bonifaz, J. Baeuml, Tobias Winchen, M. Zimbres Silva, P.F. Gómez Vitale, J. Stapleton, Giovanni Marsella, D. Nosek, A. Weindl, N. Hollon, V. Verzi, David Schmidt, Paulo J. S. Gonçalves, T. Suomijaervi, I. Jandt, Ralf Ulrich, Paul M. Mantsch, R. Piegaia, M. Zavrtanik, A. Kaeaepae, N. Giudice, K. Arisaka, H. Glass, V. M. Aranda, Petr Schovanek, J. Kleinfeller, M. Barkhausen, Daniel Kuempel, S. Maldera, Ivone F. M. Albuquerque, Ke Fang, Darko Veberič, R. Bonino, Marc Weber, M. Buscemi, M. Hrabovsky, Jan Ebr, Sergio Petrera, H.O. Klages, S. Messina, A. P. Ferguson, G. Woerner, C. J. Todero Peixoto, C. H. Wiebusch, J. Maller, N. Krohm, B. Sarkar, Christian Glaser, J. Espadanal, H. Wilczyński, P. Billoir, L. del Peral, M. Avenier, N. Awal, D. Martraire, S. Grebe, R. Squartini, T. Paul, Olivier Ravel, E. Menichetti, G. Medina-Tanco, G. van Aar, K. Link, Research unit Astroparticle Physics, Institut de Physique Nucléaire d'Orsay (IPNO), Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de l'Accélérateur Linéaire (LAL), Laboratoire de Physique Nucléaire et de Hautes Énergies (LPNHE), Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Centre National de la Recherche Scientifique (CNRS), AstroParticule et Cosmologie (APC (UMR_7164)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Laboratoire SUBATECH Nantes (SUBATECH), Mines Nantes (Mines Nantes)-Université de Nantes (UN)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Comisión Nacional de Energía Atómica, Fundación Antorchas, Gobierno De La Provincia de Mendoza, Municipalidad de Malargüe, NDM Holdings and Valle Las Leñas, in gratitude for their continuing cooperation over land access, Argentina, the Australian Research Council, Conselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq), Financiadora de Estudos e Projetos (FINEP), Fundação de Amparo à Pesquisa do Estado de Rio de Janeiro (FAPERJ), São Paulo Research Foundation (FAPESP) Grants # 2010/07359-6 and # 1999/05404-3, Ministério de Ciência e Tecnologia (MCT), Brazil, MSMT-CRLG13007, 7AMB14AR005, CZ.1.05/2.1.00/03.0058 and the Czech Science Foundation Grant 14-17501S, Czech Republic, Centre de Calcul IN2P3/CNRS, Centre National de la Recherche Scientifique (CNRS), Conseil Régional Ile-de-France, Département Physique Nucléaire et Corpusculaire (PNC-IN2P3/CNRS), Département Sciences de l׳Univers (SDU-INSU/CNRS),Bundesministerium für Bildung und Forschung (BMBF), Deutsche Forschungsgemeinschaft (DFG), Finanzministerium Baden-Württemberg, Helmholtz Alliance for Astroparticle Physics (HAP), Helmholtz-Gemeinschaft Deutscher Forschungszentren (HGF), Ministerium für Wissenschaft und Forschung, Nordrhein Westfalen, Ministerium für Wissenschaft, Forschung und Kunst, Baden-Württemberg, Germany, Istituto Nazionale di Astrofisica (INAF), Istituto Nazionale di Fisica Nucleare (INFN), Ministero dell׳Istruzione, dell׳Università e della Ricerca (MIUR), Gran Sasso Center for Astroparticle Physics (CFA), CETEMPS Center of Excellence, Italy, Consejo Nacional de Ciencia y Tecnología (CONACYT), Mexico, Ministerie van Onderwijs, Cultuur en Wetenschap, Nederlandse Organisatie voor Wetenschappelijk Onderzoek (NWO), Stichting voor Fundamenteel Onderzoek der Materie (FOM), Netherlands, National Centre for Research and Development, Grant nos. ERA-NET-ASPERA/01/11 and ERA-NET-ASPERA/02/11, National Science Centre, Grant nos. 2013/08/M/ST9/00322, and 2013/08/M/ST9/00728 and HARMONIA 5 – 2013/10/M/ST9/00062, Poland, Portuguese national funds and FEDER funds within COMPETE – Programa Operacional Factores de Competitividade through Fundação para a Ciencia e a Tecnologia, Portugal, Romanian Authority for Scientific Research ANCS, CNDI-UEFISCDI partnership projects nos. 20/2012 and nr.194/2012, project nos. 1/ASPERA2/2012 ERA-NET, PN-II-RU-PD-2011-3-0145-17, and PN-II-RU-PD-2011-3-0062, the Minister of National Education, Programme for research – Space Technology and Advanced Research – STAR, project number 83/2013, Romania, Slovenian Research Agency, Slovenia, Comunidad de Madrid, FEDER funds, Ministerio de Educación y Ciencia, Xunta de Galicia, Spain, Science and Technology Facilities Council, United Kingdom, Department of Energy, Contract no. DE-AC02-07CH11359, DE-FR02-04ER41300, DE-FG02-99ER41107 and DE-SC0011689, National Science Foundation, Grant no. 0450696, The Grainger Foundation, USA, NAFOSTED, Vietnam, Marie Curie-IRSES/EPLANET, European Particle Physics Latin American Network, European Union 7th Framework Program, Grant no. PIRSES-2009-GA-246806, and UNESCO., Pierre AUGER, ANR-11-IDEX-0004,SUPER,Sorbonne Universités à Paris pour l'Enseignement et la Recherche(2011), European Project: 328826,EC:FP7:PEOPLE,FP7-PEOPLE-2012-IEF,AUGER2FUTURE(2013), Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Joseph Fourier - Grenoble 1 (UJF)-Centre National de la Recherche Scientifique (CNRS), Unité Scientifique de la Station de Nançay (USN), Centre National de la Recherche Scientifique (CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire des Sciences de l'Univers en région Centre (OSUC), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS)-Université d'Orléans (UO), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université de Nantes (UN)-Mines Nantes (Mines Nantes), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), Irish Agriculture and Food Development Authority, Fiocruz Minas - René Rachou Research Center / Instituto René Rachou [Belo Horizonte, Brésil], Fundação Oswaldo Cruz (FIOCRUZ), Réseau International des Instituts Pasteur (RIIP)-Réseau International des Instituts Pasteur (RIIP), STMicroelectronics [Crolles] (ST-CROLLES), Dipartimento de Ingenieria Quimica y Quimica Inorganica, Universidad de Cantabria [Santander], Centre National de la Recherche Scientifique (CNRS)-Université Paris Diderot - Paris 7 (UPD7)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Pierre et Marie Curie - Paris 6 (UPMC), Istituto Nazionale di Fisica Nucleare, Sezione di Catania (INFN), Università degli studi di Catania [Catania], Département d'Astrophysique, de physique des Particules, de physique Nucléaire et de l'Instrumentation Associée (DAPNIA), Commissariat à l'énergie atomique et aux énergies alternatives (CEA), Laboratoire d'aérologie (LAERO), Centre National de la Recherche Scientifique (CNRS)-Observatoire Midi-Pyrénées (OMP), Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Université Toulouse III - Paul Sabatier (UT3), Université Fédérale Toulouse Midi-Pyrénées, Aab, A., Abreu, P., Aglietta, M., Ahn, E. J., Al Samarai, I., Albert, J. N., Albuquerque, I. F. M., Allekotte, I., Allen, J., Allison, P., Almela, A., Alvarez Castillo, J., Alvarez Muñiz, J., Alves Batista, R., Ambrosio, M., Aminaei, A., Anchordoqui, L., Andringa, S., Aramo, C., Aranda, V. M., Argirò, S., Arisaka, K., Arneodo, F., Arqueros, F., Asch, T., Asorey, H., Assis, P., Aublin, J., Ave, M., Avenier, M., Avila, G., Awal, N., Badescu, A. M., Balzer, M., Barber, K. B., Barbosa, A., Barenthien, N., Bäuml, J., Baus, C., Beatty, J. J., Becker, K. H., Bellido, J. A., Benzvi, S., Berat, C., Bergmann, T., Bertaina, M. E., Biermann, P. L., Bilhaut, R., Billoir, P., Blaess, S. G., Blanco, M., Bleve, C., Blümer, H., Boháčová, M., Bolz, H., Boncioli, D., Bonifazi, C., Bonino, R., Boratav, M., Borodai, N., Bracci, F., Brack, J., Brancus, I., Bridgeman, A., Brogueira, P., Brown, W. C., Buchholz, P., Bueno, A., Buitink, S., Buscemi, Mario, Caballero Mora, K. S., Caccianiga, B., Caccianiga, L., Camin, D., Candusso, M., Caramete, L., Caruso, R., Castellina, A., Castera, A., Cataldi, G., Cazon, L., Cester, R., Chavez, A. G., Chiavassa, A., Chinellato, J. A., Chiosso, M., Chudoba, J., Cilmo, M., Clark, P. D. J., Clay, R. W., Cocciolo, G., Colalillo, Roberta, Coleman, A., Collica, L., Colombo, E., Colonges, S., Coluccia, M. R., Conceiçáo, R., Contreras, F., Cooper, M. J., Coppens, J., Cordier, A., Courty, B., Coutu, S., Covault, C. E., Cronin, J., Curutiu, A., Dallier, R., Daniel, B., Dasso, S., Daumiller, K., Dawson, B. R., De Almeida, R. M., De Domenico, M., De Donato, C., De Jong, S. J., De Mello Neto, J. R. T., De Mitri, I., De Oliveira, J., De Souza, V., De Vries, K. D., Del Peral, L., Deligny, O., Dembinski, H., Dhital, N., Di Giulio, C., Di Matteo, A., Diaz, J. C., Díaz Castro, M. L., Diogo, F., Dobrigkeit, C., Docters, W., D'Olivo, J. C., Dolron, P., Dorofeev, A., Dorosti Hasankiadeh, Q., Dova, M. T., D'Urso, D., Ebr, J., Engel, R., Epele, L. N., Erdmann, M., Erfani, M., Escobar, C. O., Espadanal, J., Etchegoyen, A., Facal San Luis, P., Falcke, H., Fang, K., Farrar, G., Fauth, A. C., Fazzini, N., Ferguson, A. P., Fernandes, M., Ferrero, A., Fick, B., Figueira, J. M., Filevich, A., Filipčič, A., Fox, B. D., Fraenkel, E. D., Fratu, O., Freire, M. M., Fröhlich, U., Fuchs, B., Fulgione, W., Fujii, T., García, B., Garcia Gamez, D., Garcia Pinto, D., Garilli, G., Gascon Bravo, A., Gate, F., Geenen, H., Gemmeke, H., Genolini, B., Ghia, P. L., Giaccari, U., Giammarchi, M., Gibbs, K., Giller, M., Giudice, N., Glass, H., Gómez Berisso, M., Gómez Vitale, P. F., Gonçalves, P., Gonzalez, J. G., González, N., Gookin, B., Góra, D., Gordon, J., Gorgi, A., Gorham, P., Gotink, W., Gouffon, P., Grebe, S., Griffith, N., Grillo, A. F., Grubb, T. D., Grygar, J., Guardone, N., Guarino, Fausto, Guedes, G. P., Guglielmi, L., Habraken, R., Hampel, M. R., Hansen, P., Harari, D., Harmsma, S., Harrison, T. A., Hartmann, S., Harton, J. L., Haungs, A., Hebbeker, T., Heck, D., Heimann, P., Herve, A. E., Hill, G. C., Hojvat, C., Hollon, N., Holt, E., Homola, P., Hörandel, J. R., Horneffer, A., Horvat, M., Horvath, P., Hrabovský, M., Huber, D., Hucker, H., Huege, T., Iarlori, M., Insolia, A., Isar, P. G., Jandt, I., Jansen, S., Jarne, C., Johnsen, J. A., Josebachuili, M., Kääpä, A., Kambeitz, O., Kampert, K. H., Kasper, P., Katkov, I., Kégl, B., Keilhauer, B., Keivani, A., Kelley, J., Kemp, E., Kieckhafer, R. M., Klages, H. O., Kleifges, M., Kleinfeller, J., Knapp, J., Kopmann, A., Krause, R., Krohm, N., Kröpmer, O., Kuempel, D., Kunka, N., La Hurd, D., Latronico, L., Lauer, R., Lauscher, M., Lautridou, P., Le Coz, S., Leão, M. S. A. B., Lebrun, D., Lebrun, P., Leiguide Oliveira, M. A., Letessier Selvon, A., Lhenry Yvon, I., Link, K., López, R., López Casado, A., Louedec, K., Lozano Bahilo, J., Lu, L., Lucero, A., Ludwig, M., Malacari, M., Maldera, S., Mallamaci, M., Maller, J., Mandat, D., Mantsch, P., Mariazzi, A. G., Marin, V., Mariş, I. C., Marsella, G., Martello, D., Martin, L., Martinez, H., Martinez, N., Martínez Bravo, O., Martraire, D., Masías Meza, J. J., Mathes, H. J., Mathys, S., Matthews, J., Matthews, J. A. J., Matthiae, G., Maurel, D., Maurizio, D., Mayotte, E., Mazur, P. O., Medina, C., Medina Tanco, G., Meissner, R., Melissas, M., Mello, V. B. B., Melo, D., Menichetti, E., Menshikov, A., Messina, S., Meyhandan, R., Mićanović, S., Micheletti, M. I., Middendorf, L., Minaya, I. A., Miramonti, L., Mitrica, B., Molina Bueno, L., Mollerach, S., Monasor, M., Montanet, F., Morello, C., Mostafá, M., Moura, C. A., Muller, M. A., Muller, G., Muller, S., Mussa, R., Navarra, G., Navas, S., Necesal, P., Nellen, L., Nelles, A., Neuser, J., Nguyen, P. H., Nicotra, D., Niechciol, M., Niemietz, L., Niggemann, T., Nitz, D., Nosek, D., Novotny, V., Nožka, L., Ochilo, L., Ohnuki, T., Oikonomou, F., Olinto, A., Oliveira, M., Olmos Gilbaja, V. M., Pacheco, N., Pakk Selmi Dei, D., Palatka, M., Pallotta, J., Palmieri, N., Papenbreer, P., Parente, G., Parra, A., Patel, M., Paul, T., Pech, M., Pȩkala, J., Pelayo, R., Pepe, I. M., Perrone, L., Petermann, E., Peters, C., Petrera, S., Petrinca, P., Petrov, Y., Phuntsok, J., Piegaia, R., Pierog, T., Pieroni, P., Pimenta, M., Pirronello, V., Platino, M., Plum, M., Porcelli, A., Porowski, C., Porter, T., Pouryamout, J., Pouthas, J., Prado, R. R., Privitera, P., Prouza, M., Pryke, C. L., Purrello, V., Quel, E. J., Querchfeld, S., Quinn, S., Randriatoamanana, R., Rautenberg, J., Ravel, O., Ravignani, D., Revenu, B., Ridky, J., Risse, M., Ristori, P., Rizi, V., Robbins, S., Roberts, M., Rodrigues De Carvalho, W., Rodriguez Fernandez, G., Rodriguez Rojo, J., Rodríguez Frías, M. D., Rogozin, D., Ros, G., Rosado, J., Rossler, T., Roth, M., Roulet, E., Rovero, A. C., Saffi, S. J., Saftoiu, A., Salamida, F., Salazar, H., Saleh, A., Salesa Greus, F., Salina, G., Sánchez, F., Sanchez Lucas, P., Santo, C. E., Santos, E., Santos, E. M., Sarazin, F., Sarkar, B., Sarmento, R., Sato, R., Scharf, N., Scherini, V., Schieler, H., Schiffer, P., Schmidt, A., Schmidt, D., Scholten, O., Schoorlemmer, H., Schovánek, P., Schreuder, F., Schröder, F. G., Schulz, A., Schulz, J., Schüssler, F., Schumacher, J., Sciutto, S. J., Segreto, A., Sequeiros, G., Settimo, M., Shadkam, A., Shellard, R. C., Sidelnik, I., Sigl, G., Sima, O., ͆miałkowski, A., Šmída, R., Smith, A. G. K., Snow, G. R., Sommers, P., Sorokin, J., Speelman, R., Spinka, H., Squartini, R., Srivastava, Y. N., Stanič, S., Stapleton, J., Stasielak, J., Stephan, M., Stutz, A., Suarez, F., Suomijärvi, T., Supanitsky, A. D., Sutherland, M. S., Sutter, M., Swain, J., Szadkowski, Z., Szuba, M., Taborda, O. A., Tapia, A., Tcherniakhovski, D., Tepe, A., Theodoro, V. M., Timmermans, C., Tkaczyk, W., Todero Peixoto, C. J., Toma, G., Tomankova, L., Tomé, B., Tonachini, A., Torralba Elipe, G., Torres Machado, D., Travnicek, P., Trovato, E., Trung, T. N., Tunnicliffe, V., Tusi, E., Ulrich, R., Unger, M., Urban, M., Valdés Galicia, J. F., Valiño, I., Valore, Laura, Van Aar, G., Van Bodegom, P., Van Den Berg, A. M., Van Velzen, S., Van Vliet, A., Varela, E., Vargas Cárdenas, B., Varnav, D. M., Varner, G., Vasquez, R., Vázquez, J. R., Vázquez, R. A., Veberič, D., Verkooijen, H., Verzi, V., Vicha, J., Videla, M., Villaseñor, L., Vitali, G., Vlcek, B., Vorenholt, H., Vorobiov, S., Voyvodic, L., Wahlberg, H., Wainberg, O., Walker, P., Walz, D., Watson, A. A., Weber, M., Weidenhaupt, K., Weindl, A., Werner, F., Westerhoff, S., Widom, A., Wiebusch, C., Wiencke, L., Wijnen, T., Wilczyńska, B., Wilczyński, H., Wild, N., Winchen, T., Wörner, G., Wundheiler, B., Wykes, S., Yamamoto, T., Yapici, T., Yuan, G., Yushkov, A., Zamorano, B., Zas, E., Zavrtanik, M., Zepeda, A., Zhou, J., Zhu, Y., Zimbres Silva, M., Zimmermann, B., Ziolkowski, M., Zuccarello, F., Ahn, E. . J., Albuquerque, I. . F. . M., Aranda, V. . M., Arsene, N., Badescu, A. . M., Barber, K. . B., Beatty, J. . J., Becker, K. . H., Bellido, J. . A., Bertaina, M. . E., Bertou, X., Biermann, P. . L., Blaess, S. . G., Blanco, A., Bleve, Carla, Brown, W. . C., Buscemi, M., Caballero Mora, K. . S., Chavez, A. . G., Chinellato, J. . A., Clay, R. . W., Colalillo, R., Coluccia, MARIA RITA, Conceição, R., Cooper, M. . J., Covault, C. . E., Dawson, B. . R., de Almeida, R. . M., de Jong, S. . J., De Mauro, G., de Mello Neto, J. . R. . T., DE MITRI, Ivan, de Oliveira, J., de Souza, V., del Peral, L., Diaz, J. . C., Díaz Castro, M. . L., D’Olivo, J. . C., Dova, M. . T., Escobar, C. . O., Fauth, A. . C., Ferguson, A. . P., Figueira, J. . M., Fox, B. . D., Freire, M. . M., Gherghel Lascu, A., Ghia, P. . L., Głas, D., Glaser, C., Golup, G., Gómez Vitale, P. . F., Grillo, A. . F., Grubb, T. . D., Guardincerri, Y., Guarino, F., Guedes, G. . P., Hampel, M. . R., Harrison, T. . A., Harton, J. . L., Herve, A. . E., Hill, G. . C., Hörandel, J. . R., Isar, P. . G., Johnsen, J. . A., Kampert, K. . H., Kieckhafer, R. . M., Klages, H. . O., Krömer, O., Lahurd, D., Leigui de Oliveira, M. . A., Lopes, L., Mariazzi, A. . G., Mariş, I. . C., Marsella, Giovanni, Martello, Daniele, Masías Meza, J. . J., Mathes, H. . J., Matthews, J. . A. . J., Mazur, P. . O., Mello, V. . B. . B., Micheletti, M. . I., Minaya, I. . A., Moura, C. . A., Muller, M. . A., Müller, G., Müller, S., Navarro, J. . L., Nguyen, P. . H., Niculescu Oglinzanu, M., Pepe, I. . M., Perrone, Lorenzo, Prado, R. . R., Quel, E. . J., Riggi, S., Rodrigues de Carvalho, W., Rodríguez Frías, M. . D., Rovero, A. . C., Saffi, S. . J., Santos, E. . M., Scarso, C., Schauer, M., Scherini, Viviana, Schröder, F. . G., Sciutto, S. . J., Shellard, R. . C., Śmiałkowski, A., Snow, G. . R., Srivastava, Y. . N., Stanca, D., Supanitsky, A. . D., Sutherland, M. . S., Taborda, O. . A., Theodoro, V. . M., Tiffenberg, J., Todero Peixoto, C. . J., Valdés Galicia, J. . F., Valore, L., van Aar, G., van Bodegom, P., van den Berg, A. . M., van Velzen, S., van Vliet, A., Vázquez, J. . R., Vázquez, R. . A., Watson, A. . A., Wittkowski, D., Yang, L., Zavrtanik, D., Physics, Elementary Particle Physics, Observatoire des Sciences de l'Univers en région Centre (OSUC), Université Paris sciences et lettres (PSL)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS), Fundação Oswaldo Cruz / Oswaldo Cruz Foundation (FIOCRUZ), Università degli studi di Catania = University of Catania (Unict), Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Observatoire Midi-Pyrénées (OMP), Institut de Recherche pour le Développement (IRD)-Université Toulouse III - Paul Sabatier (UT3), and Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Centre National de la Recherche Scientifique (CNRS)
Subjects: detector [cosmic radiation], interaction [cosmic radiation], FLUORESCENCE YIELD, Physics - Instrumentation and Detectors, Air fluorescence detectors, hybrid observatory, Astronomy, Air fluorescence detector, Astrophysics, Auger, High energy cosmic ray, design [detector], Observatory, SURFACE DETECTOR ARRAY, High energy cosmic rays, Astrophysics::Solar and Stellar Astrophysics, fluorescence [air], Ultra-high-energy cosmic ray, ATMOSPHERIC MULTIPLE-SCATTERING, GeneralLiterature_REFERENCE(e.g.,dictionaries,encyclopedias,glossaries), Instrumentation, High Energy Astrophysical Phenomena (astro-ph.HE), Physics, performance [detector], Detector, Astrophysics::Instrumentation and Methods for Astrophysics, Pierre Auger Observatory, Instrumentation and Detectors (physics.ins-det), water Cherenkov detectors, LIGHT, Water Cherenkov detector, network [detector], LOWER IONOSPHERE, ddc:620, Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - High Energy Astrophysical Phenomena, Hybrid observatory, Water Cherenkov detectors, Nuclear and High Energy Physics, physics, air fluorescence detectors, Air fluorescence detectors, High energy cosmic rays, Hybrid observatory, Pierre Auger Observatory, Water Cherenkov detectors, Nuclear and High Energy Physics, Instrumentation, [PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM], Astrophysics::High Energy Astrophysical Phenomena, FOS: Physical sciences, Cosmic ray, EXTENSIVE AIR-SHOWERS, Particle detector, VHE [cosmic radiation], ddc:530, RECONSTRUCTION, Cosmic-ray observatory, Instrumentation and Methods for Astrophysics (astro-ph.IM), Engineering & allied operations, Astrophysique, Ciencias Exactas, Nuclear and High Energy Physic, fluorescence [detector], high energy cosmic rays, Física, ASTROFÍSICA, ULTRA-HIGH ENERGY, Pierre Auger Observatory, High energy cosmic rays, Hybrid observatory, Water Cherenkov detectors, Air fluorescence detectors, Experimental High Energy Physics, RADIATION, EMISSION
Abstract: The successful installation, commissioning, and operation of the Pierre Auger Observatory would not have been possible without the strong commitment and effort from the technical and administrative staff in Malargüe. We are very grateful to the following agencies and organizations for financial support: Comisión Nacional de Energía Atómica, Fundación Antorchas, Gobierno De La Provincia de Mendoza, Municipalidad de Malargüe, NDM Holdings and Valle Las Leñas, in gratitude for their continuing cooperation over land access, Argentina; the Australian Research Council; Conselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq), Financiadora de Estudos e Projetos (FINEP), Fundação de Amparo à Pesquisa do Estado de Rio de Janeiro (FAPERJ), São Paulo Research Foundation (FAPESP) Grants # 2010/07359-6 and # 1999/05404-3, Ministério de Ciência e Tecnologia (MCT), Brazil; MSMT-CR LG13007, 7AMB14AR005, CZ.1.05/2.1.00/03.0058 and the Czech Science Foundation Grant 14-17501S, Czech Republic; Centre de Calcul IN2P3/CNRS, Centre National de la Recherche Scientifique (CNRS), Conseil Régional Ile-de-France, Département Physique Nucléaire et Corpusculaire (PNC-IN2P3/CNRS), Département Sciences de l'Univers (SDU-INSU/CNRS), Institut Lagrange de Paris, ILP LABEX ANR-10-LABX-63, within the Investissements d'Avenir ProgrammeANR-11-IDEX-0004-02, France; Bundesministerium für Bildung und Forschung (BMBF), Deutsche Forschungsgemeinschaft (DFG), Finanzministerium Baden-Württemberg, Helmholtz Alliance for Astroparticle Physics (HAP), Helmholtz-Gemeinschaft Deutscher Forschungszentren (HGF), Ministerium für Wissenschaft und Forschung, Nordrhein Westfalen, Ministerium für Wissenschaft, Forschung und Kunst, Baden-Württemberg, Germany; Istituto Nazionale di Astrofisica (INAF), Istituto Nazionale di Fisica Nucleare (INFN), Ministero dell'Istruzione, dell'Università e della Ricerca (MIUR), Gran Sasso Center for Astroparticle Physics (CFA), CETEMPS Center of Excellence, Italy; Consejo Nacional de Ciencia y Tecnología (CONACYT), Mexico; Ministerie van Onderwijs, Cultuur en Wetenschap, Nederlandse Organisatie voor Wetenschappelijk Onderzoek (NWO), Stichting voor Fundamenteel Onderzoek der Materie (FOM), Netherlands; National Centre for Research and Development, Grant nos. ERA-NETASPERA/01/11 and ERA-NET-ASPERA/02/11, National Science Centre, Grant nos. 2013/08/M/ST9/00322, and 2013/08/M/ST9/00728 and HARMONIA 5 – 2013/10/M/ST9/00062, Poland; Portuguese national funds and FEDER funds within COMPETE – Programa Operacional Factores de Competitividade through Fundação para a Ciencia e a Tecnologia, Portugal; Romanian Authority for Scientific Research ANCS, CNDI-UEFISCDI partnership projects nos. 20/2012 and nr.194/2012, project nos. 1/ASPERA2/2012 ERA-NET, PN-II-RU-PD-2011-3-0145-17, and PN-II-RU-PD-2011- 3-0062, the Minister of National Education, Programme for research – Space Technology and Advanced Research – STAR, project number 83/2013, Romania; Slovenian Research Agency, Slovenia; Comunidad de Madrid, FEDER funds, Ministerio de Educación y Ciencia, Xunta de Galicia, European Community 7th Framework Program, Grant no. FP7-PEOPLE-2012-IEF-328826, Spain; Science and Technology Facilities Council, United Kingdom; Department of Energy, Contract no. DE-AC02-07CH11359, DE-FR02-04ER41300, DE-FG02-99ER41107 and DE-SC0011689, National Science Foundation, Grant no. 0450696, The Grainger Foundation, USA; NAFOSTED, Vietnam; Marie Curie-IRSES/EPLANET, European Particle Physics Latin American Network, European Union 7th Framework Program, Grant no. PIRSES-2009- GA-246806; and UNESCO., The Pierre Auger Observatory, located on a vast, high plain in western Argentina, is the world׳s largest cosmic ray observatory. The objectives of the Observatory are to probe the origin and characteristics of cosmic rays above 1017 eV and to study the interactions of these, the most energetic particles observed in nature. The Auger design features an array of 1660 water Cherenkov particle detector stations spread over 3000 km2 overlooked by 24 air fluorescence telescopes. In addition, three high elevation fluorescence telescopes overlook a 23.5 km2, 61-detector infilled array with 750 m spacing. The Observatory has been in successful operation since completion in 2008 and has recorded data from an exposure exceeding 40,000 km2 sr yr. This paper describes the design and performance of the detectors, related subsystems and infrastructure that make up the Observatory., Comision Nacional de Energia Atomica, Fundacion Antorchas, Gobierno De La Provincia de Mendoza, Municipalidad de Malargue, NDM Holdings and Valle Las Lenas, Australian Research Council, National Council for Scientific and Technological Development (CNPq), Ciencia Tecnologia e Inovacao (FINEP), Carlos Chagas Filho Foundation for Research Support of the State of Rio de Janeiro (FAPERJ), Fundacao de Amparo a Pesquisa do Estado de Sao Paulo (FAPESP) 2010/07359-6 1999/05404-3, Ministerio de Ciencia e Tecnologia (MCT), Brazil, Ministry of Education, Youth & Sports - Czech Republic LG13007 7AMB14AR005 CZ.1.05/2.1.00/03.0058, Grant Agency of the Czech Republic Czech Republic Government 14-17501S, Centre National de la Recherche Scientifique (CNRS), Region Ile-de-France, Departement Physique Nucleaire et Corpusculaire PNC-IN2P3/CNRS, Departement Sciences de l'Univers (SDU-INSU/CNRS), Institut Lagrange de Paris, French National Research Agency (ANR) ANR-11-IDEX-0004-02 ANR-10-LABX-63, Federal Ministry of Education & Research (BMBF), German Research Foundation (DFG), Finanzministerium Baden-Wurttemberg, Helmholtz Alliance for Astroparticle Physics (HAP), Helmholtz Association, Ministerium fur Wissenschaft und Forschung, Nordrhein Westfalen, Ministerium fur Wissenschaft, Forschung und Kunst, Baden-Wurttemberg, Germany, Istituto Nazionale Astrofisica (INAF), Istituto Nazionale di Fisica Nucleare (INFN), Ministry of Education, Universities and Research (MIUR), Gran Sasso Center for Astroparticle Physics (CFA), CETEMPS Center of Excellence, Italy, Consejo Nacional de Ciencia y Tecnologia (CONACyT), Ministerie van Onderwijs, Cultuur en Wetenschap, Netherlands Organization for Scientific Research (NWO), FOM (The Netherlands) Netherlands Government, National Centre for Research and Development ERA-NET-ASPERA/01/11 ERA-NET-ASPERA/02/11, National Science Centre, Poland 2013/08/M/ST9/00322 2013/08/M/ST9/00728 HARMONIA 5 - 2013/10/M/ST9/00062, Portuguese national funds, FEDER funds within COMPETE - Programa Operacional Factores de Competitividade through Fundacao para a Ciencia e a Tecnologia, Portugal, Romanian Authority for Scientific Research ANCS, CNDI-UEFISCDI 20/2012 194/2012 1/ASPERA2/2012 ERA-NET PN-II-RU-PD-2011-3-0145-17 PN-II-RU-PD-2011-3-0062, Programme for research - Space Technology and Advanced Research - STAR, Romania 83/2013, Slovenian Research Agency - Slovenia, Comunidad de Madrid Instituto de Salud Carlos III, European Union (EU), Spanish Government, Xunta de Galicia, European Community, Spain FP7-PEOPLE-2012-IEF-328826, Science & Technology Facilities Council (STFC), United States Department of Energy (DOE) DE-AC02-07CH11359 DE-FR02-04ER41300 DE-FG02-99ER41107 DE-SC0011689, National Science Foundation (NSF) 0450696, Grainger Foundation, USA, National Foundation for Science & Technology Development (NAFOSTED), Marie Curie-IRSES/EPLANET, European Particle Physics Latin American Network, European Union (EU) PIRSES-2009-GA-246806, UNESCO
Published: 2015
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27. Search for patterns by combining cosmic-ray energy and arrival directions at the Pierre Auger Observatory

Author: G. Torralba Elipe, Eva Santos, Richard Dallier, A. Nelles, R. Krause, Jaime Alvarez-Muñiz, L. Valore, Amin Aminaei, Peter Schiffer, H. J. Mathes, M. Ambrosio, V. Scherini, Lu Lu, Alexandra Saftoiu, Alex Kääpä, Colin Baus, I. A. Minaya, B. Wilczynska, B. Keilhauer, B. Vargas Cárdenas, T. Suomijärvi, J. Pallotta, I. Zaw, J. Maller, J. Rodriguez Rojo, J. Allen, André Schulz, E. J. Quel, Lorenzo Caccianiga, S. J. Sciutto, H. Schieler, Niraj Dhital, L. Perrone, Jiri Chudoba, Marco Giammarchi, I. Valiño, M. Buscemi, I. Al Samarai, M. Fernandes, Karl-Heinz Kampert, A. G. Chavez, F.G. Schröder, V. M. Theodoro, R. Gaior, Antonella Castellina, Sasa Micanovic, G. Matthiae, J. Neuser, K. Link, Miroslav Hrabovský, J. D. Swain, A. Haungs, Enrique Zas, J. L. Harton, S. G. Blaess, A. Cordier, D. Nosek, P. Mantsch, Z. Szadkowski, J. Lozano Bahilo, C. Hojvat, Jan Ebr, L. Nellen, P. Abreu, Fernando Contreras, K. Louedec, Mariangela Settimo, Antonio Bueno, M. Josebachuili, M. Zavrtanik, Alexey Yushkov, Moritz Münchmeyer, G. C. Hill, B. Tome, Thomas Harrison, Corbin Covault, Y. Petrov, G. Müller, D. Ravignani, G. Cocciolo, Carola Dobrigkeit, M. Plum, M. E. Bertaina, C. O. Escobar, Alan Watson, V. Purrello, C. Morello, V. Marin, Ralph Engel, G. Marsella, Philipp Papenbreer, Petr Travnicek, Gualberto Avila, Ingomar Allekotte, J. Alvarez Castillo, A. Insolia, M. Kleifges, D. Zavrtanik, F. Suarez, Thomas Hebbeker, F. Diogo, Sergio Dasso, R. M. de Almeida, H. Blümer, A. Weindl, J. Ridky, H.O. Klages, Luca Latronico, Lino Miramonti, A. Aab, Harm Schoorlemmer, Luis A. Anchordoqui, J. Pȩkala, Max Malacari, B. Kégl, A. Stutz, L. Caramete, A. C. Fauth, Jörg R. Hörandel, G. Garilli, Alan Coleman, Trent D. Grubb, D. Huber, P. Pieroni, B. Vlcek, Stijn Buitink, Angela V. Olinto, V. M. Aranda, D. Nitz, Piotr Homola, N. Hollon, V. Verzi, P. Facal San Luis, M. D. Rodríguez-Frías, S. Messina, C. Di Giulio, A. Chiavassa, Carla Bonifazi, Jose A. Bellido, G. P. Guedes, David Schmidt, A. P. Ferguson, I. Lhenry-Yvon, Toshihiro Fujii, Juan Manuel Figueira, V. Pirronello, S. Le Coz, M. L. Díaz Castro, G. Farrar, A. E. Herve, K. B. Barber, Iuri Muniz Pepe, M. Platino, L. R. Wiencke, F. Arqueros, B. Zamorano, Jaime Rosado, M. Monasor, Peter L. Biermann, P. Necesal, C. L. Williams, Petr Schovanek, Paulo J. S. Gonçalves, I. Jandt, Ralf Ulrich, R. Cester, I. C. Mariş, Hernan Wahlberg, Octavian Sima, J. G. Gonzalez, D. Lebrun, R. R. Prado, M. Videla, R. J. Lauer, P. Ristori, David Wittkowski, G. Salina, Danielle LaHurd, Olivier Deligny, B. Caccianiga, O. Krömer, B. García, Tobias Winchen, P. Lebrun, R. López, Karen S. Caballero-Mora, M. Ludwig, S. Hartmann, Martin Erdmann, Roger W Clay, Johannes Schulz, M. Pimenta, Dusan Mandat, Roberta Colalillo, A. G. Mariazzi, M. Blanco, A.M. van den Berg, Darko Veberič, I. Rodriguez Cabo, R. Bonino, A. Shadkam, A. F. Grillo, Francesca Zuccarello, Juan Carlos D'Olivo, T. Pierog, Esteban Roulet, P. L. Ghia, Maurice Stephan, A. Tonachini, S. Quinn, A. Segreto, Günter Sigl, P.F. Gómez Vitale, Radomir Smida, Alberto Daniel Supanitsky, U. Fröhlich, A. Porcelli, Markus Roth, A. Dorofeev, Igor Katkov, A. van Vliet, L. Villaseñor, G. Yuan, Matias Tueros, S. Riggi, N. Scharf, P. Heimann, E. Kemp, Serguei Vorobiov, D. Monnier Ragaigne, O. A. Taborda, J. Stasielak, S. Coutu, H. Martinez, C. Porowski, Paul Sommers, P. Gouffon, M. J. Cooper, Denise Boncioli, F. Sánchez, Carlos Medina, M. De Domenico, Maria Rita Coluccia, Bruno Daniel, T. Yapici, J. J. Masías Meza, D. Maurel, E.M. Holt, A. Saleh, Maria-Teresa Dova, M. R. Hampel, S. Müller, R. Alves Batista, A. Tapia, Sarka Wykes, H. Gemmeke, Jing Zhou, R. Meissner, Octavian Fratu, Yingchun Zhu, M. Palatka, G. S. Varner, Paolo Privitera, C. Jarne, T. Huege, A. Parra, Jeffrey Brack, Olaf Scholten, Humberto Ibarguen Salazar, E. Varela, N. Griffith, Miguel Mostafa, L. Tomankova, G. Navarra, L. Ochilo, C. Aramo, C. E. Santo, M. Zimbres Silva, J. Stapleton, L. Nožka, R. Piegaia, S. Navas, M. Melissas, Joshua A. Gordon, R. A. Vázquez, A. Filipčič, F. Sarazin, S. Petrera, Marc Weber, A. Śmiał kowski, B. Revenu, Eric Mayotte, M. Ave, M. Gómez Berisso, R. C. Shellard, W. Docters, German Ros, Marcus Niechciol, M. Risse, J. Kleinfeller, J. R. Vázquez, Jose Chinellato, P. Lautridou, A. Widom, A. Letessier-Selvon, Lorenzo Cazon, J. A.J. Matthews, Xavier Bertou, L. Martin, Marco Cilmo, T. Rossler, A. Bridgeman, S. J. Saffi, Markus Lauscher, J. Phuntsok, Raul Sarmento, M. Mallamaci, S. Jansen, P. Sanchez-Lucas, D. Harari, D. Martraire, Yogendra N. Srivastava, M. I. Micheletti, Daniel Kuempel, Q. Dorosti Hasankiadeh, B. Mitrica, Heino Falcke, J. Vicha, A. Gorgi, D. Heck, S. Maldera, A. Zepeda, Rúben Conceição, R. Pelayo, Ivone F. M. Albuquerque, Ke Fang, M. Will, M. Urban, A. C. Rovero, N. Palmieri, Pedro Assis, A. Etchegoyen, Johannes Schumacher, Alina Mihaela Badescu, S. Querchfeld, C. Bleve, M. Candusso, M. Prouza, L. Niemietz, B. D. Fox, M. Oliveira, Peter Gorham, A. Menshikov, F. Salamida, Iván Sidelnik, L. Molina-Bueno, D. Melo, Florian Gaté, G. Parente, Vincenzo Rizi, David Walz, N. Pacheco, D. Martello, D. Pakk Selmi-Dei, Tim Niggemann, K. Weidenhaupt, M. Ziolkowski, R. Sato, L. Collica, Martina Bohacova, O. Martínez Bravo, F. Werner, Patrick Allison, V. de Souza, C. J.W.P. Timmermans, D. Maurizio, J. Sorokin, J. C. Diaz, Eun-Joo Ahn, François Montanet, D. Rogozin, J. de Oliveira, S. van Velzen, Alejandro Almela, K. H. Becker, V. Novotny, J. Bäuml, Rossella Caruso, A. Lucero, S. Mathys, M. Erfani, D. Kruppke-Hansen, Marcio Aparecido Muller, N. Kunka, Nicolás González, Corinne Berat, M. Giller, E. Trovato, B. Gookin, P. H. Nguyen, E. M. Santos, J. F. Valdés Galicia, I. De Mitri, A. Gascon Bravo, D. Garcia-Gamez, Bruce R. Dawson, P.O. Mazur, S. T. Garcia Roca, Bryan C. Fuchs, D. Torres Machado, M. A. Leigui de Oliveira, Paula Gina Isar, Pedro Brogueira, F. Salesa Greus, G. Cataldi, D. Garcia-Pinto, A. Di Matteo, B. Wundheiler, Gregory R Snow, P. H. Kasper, M. S. A. B. Leão, John N. Matthews, R. M. Kieckhafer, J. Rautenberg, O. Wainberg, W. C. Brown, C. J. Todero Peixoto, C. A. Moura, T. Yamamoto, Brian Fick, Samo Stanič, N. Krohm, Kai Daumiller, R. Meyhandan, B. Sarkar, Christian Glaser, J. Espadanal, H. Wilczyński, P. Billoir, L. del Peral, O. Ravel, N. Awal, E. Petermann, Miroslav Pech, Pavel Horvath, M. S. Sutherland, Sofia Andringa, S. Grebe, O. Kambeitz, R. Squartini, T. Paul, A. Tepe, A. Lopez Agüera, Alberto Filevich, Peter Hansen, F. Guarino, Peter Buchholz, M. Szuba, I.M. Brancus, H. Glass, Marco Aglietta, G. Medina-Tanco, R. Mussa, J. J. Beatty, Silvia Mollerach, H. Dembinski, N. Fazzini, G. van Aar, Julien Aublin, Michael Unger, S. J. De Jong, M. Avenier, A. Curutiu, Ugo Giaccari, J. R. T. de Mello Neto, Lukas Middendorf, Christine Peters, G. Rodriguez Fernandez, Hernán Asorey, Azadeh Keivani, W. Rodrigues de Carvalho, M. Tartare, J. W. Cronin, P. van Bodegom, G. Toma, Nataliia Borodai, Laboratoire de Physique Nucléaire et de Hautes Énergies (LPNHE), Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Unité Scientifique de la Station de Nançay (USN), Observatoire des Sciences de l'Univers en région Centre (OSUC), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS), Laboratoire SUBATECH Nantes (SUBATECH), Mines Nantes (Mines Nantes)-Université de Nantes (UN)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de l'Accélérateur Linéaire (LAL), Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Centre National de la Recherche Scientifique (CNRS), Institut de Physique Nucléaire d'Orsay (IPNO), PIERRE AUGER, European Project: 328826,EC:FP7:PEOPLE,FP7-PEOPLE-2012-IEF,AUGER2FUTURE(2013), Aab, A., Abreu, P., Aglietta, M., Ahn, E. . J., Al Samarai, I., Albuquerque, I. . F. . M., Allekotte, I., Allison, P., Almela, A., Alvarez Castillo, J., Alvarez Muñiz, J., Alves Batista, R., Ambrosio, M., Aminaei, A., Anchordoqui, L., Andringa, S., Aramo, C., Aranda, V. . M., Arqueros, F., Arsene, N., Asorey, H., Assis, P., Aublin, J., Ave, M., Avenier, M., Avila, G., Awal, N., Badescu, A. . M., Barber, K. . B., Bäuml, J., Baus, C., Beatty, J. . J., Becker, K. . H., Bellido, J. . A., Berat, C., Bertaina, M. . E., Bertou, X., Biermann, P. . L., Billoir, P., Blaess, S. . G., Blanco, A., Blanco, M., Bleve, Carla, Blümer, H., Boháčová, M., Boncioli, D., Bonifazi, C., Borodai, N., Brack, J., Brancus, I., Bridgeman, A., Brogueira, P., Brown, W. . C., Buchholz, P., Bueno, A., Buitink, S., Buscemi, M., Caballero Mora, K. . S., Caccianiga, B., Caccianiga, L., Candusso, M., Caramete, L., Caruso, R., Castellina, A., Cataldi, G., Cazon, L., Cester, R., Chavez, A. . G., Chiavassa, A., Chinellato, J. . A., Chudoba, J., Cilmo, M., Clay, R. . W., Cocciolo, G., Colalillo, R., Coleman, A., Collica, L., Coluccia, MARIA RITA, Conceição, R., Contreras, F., Cooper, M. . J., Cordier, A., Coutu, S., Covault, C. . E., Cronin, J., Dallier, R., Daniel, B., Dasso, S., Daumiller, K., Dawson, B. . R., de Almeida, R. . M., de Jong, S. . J., De Mauro, G., de Mello Neto, J. . R. . T., DE MITRI, Ivan, de Oliveira, J., de Souza, V., del Peral, L., Deligny, O., Dembinski, H., Dhital, N., Di Giulio, C., Di Matteo, A., Diaz, J. . C., Díaz Castro, M. . L., Diogo, F., Dobrigkeit, C., Docters, W., D’Olivo, J. . C., Dorofeev, A., Dorosti Hasankiadeh, Q., Dova, M. . T., Ebr, J., Engel, R., Erdmann, M., Erfani, M., Escobar, C. . O., Espadanal, J., Etchegoyen, A., Falcke, H., Fang, K., Farrar, G., Fauth, A. . C., Fazzini, N., Ferguson, A. . P., Fernandes, M., Fick, B., Figueira, J. . M., Filevich, A., Filipčič, A., Fox, B. . D., Fratu, O., Freire, M. . M., Fuchs, B., Fujii, T., García, B., Garcia Pinto, D., Gate, F., Gemmeke, H., Gherghel Lascu, A., Ghia, P. . L., Giaccari, U., Giammarchi, M., Giller, M., Głas, D., Glaser, C., Glass, H., Golup, G., Gómez Berisso, M., Gómez Vitale, P. . F., González, N., Gookin, B., Gordon, J., Gorgi, A., Gorham, P., Gouffon, P., Griffith, N., Grillo, A. . F., Grubb, T. . D., Guardincerri, Y., Guarino, F., Guedes, G. . P., Hampel, M. . R., Hansen, P., Harari, D., Harrison, T. . A., Hartmann, S., Harton, J. . L., Haungs, A., Hebbeker, T., Heck, D., Heimann, P., Herve, A. . E., Hill, G. . C., Hojvat, C., Hollon, N., Holt, E., Homola, P., Hörandel, J. . R., Horvath, P., Hrabovský, M., Huber, D., Huege, T., Insolia, A., Isar, P. . G., Jandt, I., Jansen, S., Jarne, C., Johnsen, J. . A., Josebachuili, M., Kääpä, A., Kambeitz, O., Kampert, K. . H., Kasper, P., Katkov, I., Kégl, B., Keilhauer, B., Keivani, A., Kemp, E., Kieckhafer, R. . M., Klages, H. . O., Kleifges, M., Kleinfeller, J., Krause, R., Krohm, N., Krömer, O., Kuempel, D., Kunka, N., Lahurd, D., Latronico, L., Lauer, R., Lauscher, M., Lautridou, P., Le Coz, S., Lebrun, D., Lebrun, P., Leigui de Oliveira, M. . A., Letessier Selvon, A., Lhenry Yvon, I., Link, K., Lopes, L., López, R., López Casado, A., Louedec, K., Lu, L., Lucero, A., Malacari, M., Maldera, S., Mallamaci, M., Maller, J., Mandat, D., Mantsch, P., Mariazzi, A. . G., Marin, V., Mariş, I. . C., Marsella, Giovanni, Martello, Daniele, Martin, L., Martinez, H., Martínez Bravo, O., Martraire, D., Masías Meza, J. . J., Mathes, H. . J., Mathys, S., Matthews, J., Matthews, J. . A. . J., Matthiae, G., Maurel, D., Maurizio, D., Mayotte, E., Mazur, P. . O., Medina, C., Medina Tanco, G., Meissner, R., Mello, V. . B. . B., Melo, D., Menshikov, A., Messina, S., Meyhandan, R., Micheletti, M. . I., Middendorf, L., Minaya, I. . A., Miramonti, L., Mitrica, B., Molina Bueno, L., Mollerach, S., Montanet, F., Morello, C., Mostafá, M., Moura, C. . A., Muller, M. . A., Müller, G., Müller, S., Mussa, R., Navarra, G., Navarro, J. . L., Navas, S., Necesal, P., Nellen, L., Nelles, A., Neuser, J., Nguyen, P. . H., Niculescu Oglinzanu, M., Niechciol, M., Niemietz, L., Niggemann, T., Nitz, D., Nosek, D., Novotny, V., Nožka, L., Ochilo, L., Oikonomou, F., Olinto, A., Pacheco, N., Pakk Selmi Dei, D., Palatka, M., Pallotta, J., Papenbreer, P., Parente, G., Parra, A., Paul, T., Pech, M., Pȩkala, J., Pelayo, R., Pepe, I. . M., Perrone, Lorenzo, Petermann, E., Peters, C., Petrera, S., Petrov, Y., Phuntsok, J., Piegaia, R., Pierog, T., Pieroni, P., Pimenta, M., Pirronello, V., Platino, M., Plum, M., Porcelli, A., Porowski, C., Prado, R. . R., Privitera, P., Prouza, M., Purrello, V., Quel, E. . J., Querchfeld, S., Quinn, S., Rautenberg, J., Ravel, O., Ravignani, D., Revenu, B., Ridky, J., Riggi, S., Risse, M., Ristori, P., Rizi, V., Rodrigues de Carvalho, W., Rodriguez Fernandez, G., Rodriguez Rojo, J., Rodríguez Frías, M. . D., Rogozin, D., Rosado, J., Roth, M., Roulet, E., Rovero, A. . C., Saffi, S. . J., Saftoiu, A., Salamida, F., Salazar, H., Saleh, A., Salesa Greus, F., Salina, G., Sánchez, F., Sanchez Lucas, P., Santos, E., Santos, E. . M., Sarazin, F., Sarkar, B., Sarmento, R., Sato, R., Scarso, C., Schauer, M., Scherini, Viviana, Schieler, H., Schiffer, P., Schmidt, D., Scholten, O., Schoorlemmer, H., Schovánek, P., Schröder, F. . G., Schulz, A., Schulz, J., Schumacher, J., Sciutto, S. . J., Segreto, A., Settimo, M., Shadkam, A., Shellard, R. . C., Sidelnik, I., Sigl, G., Sima, O., Śmiałkowski, A., Šmída, R., Snow, G. . R., Sommers, P., Sorokin, J., Squartini, R., Srivastava, Y. . N., Stanca, D., Stanič, S., Stapleton, J., Stasielak, J., Stephan, M., Stutz, A., Suarez, F., Suomijärvi, T., Supanitsky, A. . D., Sutherland, M. . S., Swain, J., Szadkowski, Z., Taborda, O. . A., Tapia, A., Tepe, A., Theodoro, V. . M., Tiffenberg, J., Timmermans, C., Todero Peixoto, C. . J., Toma, G., Tomankova, L., Tomé, B., Tonachini, A., Torralba Elipe, G., Torres Machado, D., Travnicek, P., Ulrich, R., Unger, M., Urban, M., Valdés Galicia, J. . F., Valiño, I., Valore, L., van Aar, G., van Bodegom, P., van den Berg, A. . M., van Velzen, S., van Vliet, A., Varela, E., Vargas Cárdenas, B., Varner, G., Vasquez, R., Vázquez, J. . R., Vázquez, R. . A., Veberič, D., Verzi, V., Vicha, J., Videla, M., Villaseñor, L., Vlcek, B., Vorobiov, S., Wahlberg, H., Wainberg, O., Walz, D., Watson, A. . A., Weber, M., Weidenhaupt, K., Weindl, A., Werner, F., Widom, A., Wiencke, L., Wilczyński, H., Winchen, T., Wittkowski, D., Wundheiler, B., Wykes, S., Yang, L., Yapici, T., Yushkov, A., Zas, E., Zavrtanik, D., Zavrtanik, M., Zepeda, A., Zhu, Y., Zimmermann, B., Ziolkowski, M., Zuccarello, F., UNIVERSIDADE DE ESTADUAL DE CAMPINAS, Laboratoire de Physique Nucléaire et de Hautes Énergies ( LPNHE ), Université Pierre et Marie Curie - Paris 6 ( UPMC ) -Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Université Paris Diderot - Paris 7 ( UPD7 ) -Centre National de la Recherche Scientifique ( CNRS ), Unité Scientifique de la Station de Nançay ( USN ), Institut national des sciences de l'Univers ( INSU - CNRS ) -Observatoire de Paris-Université d'Orléans ( UO ) -Centre National de la Recherche Scientifique ( CNRS ), Laboratoire SUBATECH Nantes ( SUBATECH ), Mines Nantes ( Mines Nantes ) -Université de Nantes ( UN ) -Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Centre National de la Recherche Scientifique ( CNRS ), Laboratoire de l'Accélérateur Linéaire ( LAL ), Université Paris-Sud - Paris 11 ( UP11 ) -Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Centre National de la Recherche Scientifique ( CNRS ), Laboratoire de Physique Subatomique et de Cosmologie ( LPSC ), Université Joseph Fourier - Grenoble 1 ( UJF ) -Institut polytechnique de Grenoble - Grenoble Institute of Technology ( Grenoble INP ) -Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Centre National de la Recherche Scientifique ( CNRS ) -Université Grenoble Alpes ( UGA ), Institut de Physique Nucléaire d'Orsay ( IPNO ), European Project : 328826,EC:FP7:PEOPLE,FP7-PEOPLE-2012-IEF,AUGER2FUTURE ( 2013 ), Bergische Universität Wuppertal, University of Łódź, tobias.winchen@rwth-aachen.de, Ahn, E. J., Samarai, I. Al, Albuquerque, I. F. M., Allekotte, I, Allen, J., Castillo, J. Alvarez, Batista, R. Alve, Aranda, V. M., Badescu, A. M., Barber, K. B., Beatty, J. J., Becker, K. H., Bellido, J. A., Bertaina, M. E., Biermann, P. L., Blaess, S., Bleve, C., Bonino, R., Brown, W. C., Buscemi, Mario, Caballero Mora, K. S., Chavez, A. G., Chinellato, J. A., Clay, R. W., Colalillo, Roberta, Coluccia, M. R., Cooper, M. J., Covault, C. E., Curutiu, A., Dawson, B. R., Almeida, R. M. de, Domenico, M. De, Jong, S. J. de, Neto, J. R. T. de Mello, Mitri, I. De, Oliveira, J. de, Souza, V. de, Peral, L. del, Giulio, C. Di, Matteo, A. Di, Diaz, J. C., Castro, M. L. Díaz, D’Olivo, J. C., Hasankiadeh, Q. Dorosti, Dova, M. T., Escobar, C. O., Luis, P. Facal San, Fauth, A. C., Ferguson, A. P., Figueira, J. M., Fox, B. D., Fröhlich, U., Gaior, R., Roca, S. T. Garcia, Garcia Gamez, D., Garilli, G., Bravo, A. Gascon, Ghia, P. L., Berisso, M. Gómez, Vitale, P. F. Gómez, Gonçalves, P., Gonzalez, J. G., Grebe, S., Grillo, A. F., Grubb, T. D., Guarino, Fausto, Guedes, G. P., Hampel, M. R., Harrison, T. A., Harton, J. L., Herve, A. E., Hill, G. C., Hörandel, J. R., Isar, P. G., Kampert, K. H., Kieckhafer, R. M., Klages, H. O., Kruppke Hansen, D., Coz, S. Le, Leão, M. S. A. B., Oliveira, M. A. Leigui de, Agüera, A. Lopez, Bahilo, J. Lozano, Ludwig, M., Mariazzi, A. G., Mariş, I. C., Marsella, G., Martello, D., Bravo, O. Martínez, Meza, J. J. Masía, Mathes, H. J., Matthews, J. A. J., Mazur, P. O., Melissas, M., Mićanović, S., Micheletti, M. I., Minaya, I. A., Monasor, M., Ragaigne, D. Monnier, Moura, C. A., Muller, M. A., Münchmeyer, M., Nguyen, P., Oliveira, M., Selmi Dei, D. Pakk, Palmieri, N., Pepe, I. M., Perrone, L., Prado, R. R., Quel, E. J., Carvalho, W. Rodrigues de, Cabo, I. Rodriguez, Fernandez, G. Rodriguez, Rojo, J. Rodriguez, Rodríguez Frías, M. D., Ros, G., Rossler, T., Rovero, A. C., Saffi, S. J., Greus, F. Salesa, Santo, C. E., Santos, E. M., Scharf, N., Scherini, V., Schröder, F. G., Sciutto, S. J., Shellard, R. C., Kowski, A. Śmiał, Snow, G. R., Srivastava, Y. N., Supanitsky, A. D., Sutherland, M. S., Szuba, M., Taborda, O. A., Tartare, M., Theodoro, V. M., Peixoto, C. J. Todero, Elipe, G. Torralba, Machado, D. Torre, Trovato, E., Tueros, M., Galicia, J. F. Valdé, Valore, Laura, Aar, G. van, Bodegom, P. van, Berg, A. M. van den, Velzen, S. van, Vliet, A. van, Vázquez, J. R., Vázquez, R. A., Watson, A. A., Wilczyńska, B., Will, M., Williams, C., Yamamoto, T., Yuan, G., Zamorano, B., Zaw, I., Zhou, J., Silva, M. Zimbre, Centre National de la Recherche Scientifique (CNRS)-Université Paris Diderot - Paris 7 (UPD7)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Pierre et Marie Curie - Paris 6 (UPMC), Centre National de la Recherche Scientifique (CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire des Sciences de l'Univers en région Centre (OSUC), Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Université d'Orléans (UO)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Université d'Orléans (UO)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université d'Orléans (UO), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université de Nantes (UN)-Mines Nantes (Mines Nantes), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Joseph Fourier - Grenoble 1 (UJF)-Centre National de la Recherche Scientifique (CNRS), Research unit Astroparticle Physics, Aab A., Abreu P., Aglietta M., Ahn E. J., Al Samarai I., Albuquerque I. F. M., Allekotte I., Allison P., Almela A., Alvarez Castillo J., Alvarez-Muñiz J., Alves Batista R., Ambrosio M., Aminaei A., Anchordoqui L., Andringa S., Aramo C., Aranda V. M., Arqueros F., Arsene N., Asorey H., Assis P., Aublin J., Ave M., Avenier M., Avila G., Awal N., Badescu A. M., Barber K. B., Bäuml J., Baus C., Beatty J. J., Becker K. H., Bellido J. A., Berat C., Bertaina M. E., Bertou X., Biermann P. L., Billoir P., Blaess S. G., Blanco A., Blanco M., Bleve C., Blümer H., Boháčová M., Boncioli D., Bonifazi C., Borodai N., Brack J., Brancus I., Bridgeman A., Brogueira P., Brown W. C., Buchholz P., Bueno A., Buitink S., Buscemi M., Caballero-Mora K. S., Caccianiga B., Caccianiga L., Candusso M., Caramete L., Caruso R., Castellina A., Cataldi G., Cazon L., Cester R., Chavez A. G., Chiavassa A., Chinellato J. A., Chudoba J., Cilmo M., Clay R. W., Cocciolo G., Colalillo R., Coleman A., Collica L., Coluccia M. R., Conceição R., Contreras F., Cooper M. J., Cordier A., Coutu S., Covault C. E., Cronin J., Dallier R., Daniel B., Dasso S., Daumiller K., Dawson B. R., de Almeida R. M., de Jong S. J., De Mauro G., de Mello Neto J. R. T., De Mitri I., de Oliveira J., de Souza V., del Peral L., Deligny O., Dembinski H., Dhital N., Di Giulio C., Di Matteo A., Diaz J. C., Díaz Castro M. L., Diogo F., Dobrigkeit C., Docters W., D’Olivo J. C., Dorofeev A., Dorosti Hasankiadeh Q., Dova M. T., Ebr J., Engel R., Erdmann M., Erfani M., Escobar C. O., Espadanal J., Etchegoyen A., Falcke H., Fang K., Farrar G., Fauth A. C., Fazzini N., Ferguson A. P., Fernandes M., Fick B., Figueira J. M., Filevich A., Filipčič A., Fox B. D., Fratu O., Freire M. M., Fuchs B., Fujii T., García B., Garcia-Pinto D., Gate F., Gemmeke H., Gherghel-Lascu A., Ghia P. L., Giaccari U., Giammarchi M., Giller M., Głas D., Glaser C., Glass H., Golup G., Gómez Berisso M., Gómez Vitale P. F., González N., Gookin B., Gordon J., Gorgi A., Gorham P., Gouffon P., Griffith N., Grillo A. F., Grubb T. D., Guardincerri Y., Guarino F., Guedes G. P., Hampel M. R., Hansen P., Harari D., Harrison T. A., Hartmann S., Harton J. L., Haungs A., Hebbeker T., Heck D., Heimann P., Herve A. E., Hill G. C., Hojvat C., Hollon N., Holt E., Homola P., Hörandel J. R., Horvath P., Hrabovský M., Huber D., Huege T., Insolia A., Isar P. G., Jandt I., Jansen S., Jarne C., Johnsen J. A., Josebachuili M., Kääpä A., Kambeitz O., Kampert K. H., Kasper P., Katkov I., Kégl B., Keilhauer B., Keivani A., Kemp E., Kieckhafer R. M., Klages H. O., Kleifges M., Kleinfeller J., Krause R., Krohm N., Krömer O., Kuempel D., Kunka N., LaHurd D., Latronico L., Lauer R., Lauscher M., Lautridou P., Le Coz S., Lebrun D., Lebrun P., Leigui de Oliveira M. A., Letessier-Selvon A., Lhenry-Yvon I., Link K., Lopes L., López R., López Casado A., Louedec K., Lu L., Lucero A., Malacari M., Maldera S., Mallamaci M., Maller J., Mandat D., Mantsch P., Mariazzi A. G., Marin V., Mariş I. C., Marsella G., Martello D., Martin L., Martinez H., Martínez Bravo O., Martraire D., Masías Meza J. J., Mathes H. J., Mathys S., Matthews J., Matthews J. A. J., Matthiae G., Maurel D., Maurizio D., Mayotte E., Mazur P. O., Medina C., Medina-Tanco G., Meissner R., Mello V. B. B., Melo D., Menshikov A., Messina S., Meyhandan R., Micheletti M. I., Middendorf L., Minaya I. A., Miramonti L., Mitrica B., Molina-Bueno L., Mollerach S., Montanet F., Morello C., Mostafá M., Moura C. A., Muller M. A., Müller G., Müller S., Mussa R., Navarra G., Navarro J. L., Navas S., Necesal P., Nellen L., Nelles A., Neuser J., Nguyen P. H., Niculescu-Oglinzanu M., Niechciol M., Niemietz L., Niggemann T., Nitz D., Nosek D., Novotny V., Nožka L., Ochilo L., Oikonomou F., Olinto A., Pacheco N., Pakk Selmi-Dei D., Palatka M., Pallotta J., Papenbreer P., Parente G., Parra A., Paul T., Pech M., Pȩkala J., Pelayo R., Pepe I. M., Perrone L., Petermann E., Peters C., Petrera S., Petrov Y., Phuntsok J., Piegaia R., Pierog T., Pieroni P., Pimenta M., Pirronello V., Platino M., Plum M., Porcelli A., Porowski C., Prado R. R., Privitera P., Prouza M., Purrello V., Quel E. J., Querchfeld S., Quinn S., Rautenberg J., Ravel O., Ravignani D., Revenu B., Ridky J., Riggi S., Risse M., Ristori P., Rizi V., Rodrigues de Carvalho W., Rodriguez Fernandez G., Rodriguez Rojo J., Rodríguez-Frías M. D., Rogozin D., Rosado J., Roth M., Roulet E., Rovero A. C., Saffi S. J., Saftoiu A., Salamida F., Salazar H., Saleh A., Salesa Greus F., Salina G., Sánchez F., Sanchez-Lucas P., Santos E., Santos E. M., Sarazin F., Sarkar B., Sarmento R., Sato R., Scarso C., Schauer M., Scherini V., Schieler H., Schiffer P., Schmidt D., Scholten O., Schoorlemmer H., Schovánek P., Schröder F. G., Schulz A., Schulz J., Schumacher J., Sciutto S. J., Segreto A., Settimo M., Shadkam A., Shellard R. C., Sidelnik I., Sigl G., Sima O., Śmiałkowski A., Šmída R., Snow G. R., Sommers P., Sorokin J., Squartini R., Srivastava Y. N., Stanca D., Stanič S., Stapleton J., Stasielak J., Stephan M., Stutz A., Suarez F., Suomijärvi T., Supanitsky A. D., Sutherland M. S., Swain J., Szadkowski Z., Taborda O. A., Tapia A., Tepe A., Theodoro V. M., Tiffenberg J., Timmermans C., Todero Peixoto C. J., Toma G., Tomankova L., Tomé B., Tonachini A., Torralba Elipe G., Torres Machado D., Travnicek P., Ulrich R., Unger M., Urban M., Valdés Galicia J. F., Valiño I., Valore L., van Aar G., van Bodegom P., van den Berg A. M., van Velzen S., van Vliet A., Varela E., Vargas Cárdenas B., Varner G., Vasquez R., Vázquez J. R., Vázquez R. A., Veberič D., Verzi V., Vicha J., Videla M., Villaseñor L., Vlcek B., Vorobiov S., Wahlberg H., Wainberg O., Walz D., Watson A. A., Weber M., Weidenhaupt K., Weindl A., Werner F., Widom A., Wiencke L., Wilczyński H., Winchen T., Wittkowski D., Wundheiler B., Wykes S., Yang L., Yapici T., Yushkov A., Zas E., Zavrtanik D., Zavrtanik M., Zepeda A., Zhu Y., Zimmermann B., Ziolkowski M., and Zuccarello F.
Subjects: Astrofísica, Physics and Astronomy (miscellaneous), Ray, cosmic radiation anisotropy, cosmic radiation propagation, cosmic radiation deflection, Astronomy, magnetic field, Astrophysics, anisotropy [cosmic radiation], 01 natural sciences, Settore FIS/04 - Fisica Nucleare e Subnucleare, Auger, Pierre, purl.org/becyt/ford/1 [https], Observatory, Jets, Quantum Chromodynamics, cosmic radiation: VHE, energy: correlation, Patterns, Monte Carlo, 010303 astronomy & astrophysics, High Energy Astrophysical Phenomena (astro-ph.HE), Physics, cosmic radiation: propagation, Energy, COSMIC cancer database, Angular distance, [SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], Settore FIS/01 - Fisica Sperimentale, Search, Astrophysics::Instrumentation and Methods for Astrophysics, cosmic radiation anisotropy, Pierre Auger Observatory, cosmic radiation: deflection, Radiación cósmica, Surface Detector Array, Cosmic, Arrival, ComputingMethodologies_DOCUMENTANDTEXTPROCESSING, Física nuclear, Astrophysics - High Energy Astrophysical Phenomena, Principal axis theorem, [PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], Regular Article - Experimental Physics, Astrophysics::High Energy Astrophysical Phenomena, Physics and Astronomy (miscellaneous), Engineering (miscellaneous), FOS: Physical sciences, Cosmic ray, cosmic radiation: anisotropy, Particle detector, Settore FIS/05 - Astronomia e Astrofisica, VHE [cosmic radiation], statistical analysis, Spectrum, 0103 physical sciences, thrust, ddc:530, Engineering (miscellaneous), Astrophysique, Ciencias Exactas, air: showers, cosmic radiation propagation, 010308 nuclear & particles physics, turbulence, [ PHYS.ASTR.HE ] Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], Física, Astroparticles, purl.org/becyt/ford/1.3 [https], ASTROFÍSICA, Galactic Magnetic-field, correlation [energy], Direction, Experimental High Energy Physics, cosmic radiation deflection, propagation [cosmic radiation], direct detection, galaxy, [ SDU.ASTR.HE ] Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], deflection [cosmic radiation], showers [air], Model
Abstract: Energy-dependent patterns in the arrival directions of cosmic rays are searched for using data of the Pierre Auger Observatory. We investigate local regions around the highest-energy cosmic rays with E ≥ 6×1019 eV by analyzing cosmic rays with energies above E ≥ 5×1018 eV arriving within an angular separation of approximately 15∘. We characterize the energy distributions inside these regions by two independent methods, one searching for angular dependence of energy-energy correlations and one searching for collimation of energy along the local system of principal axes of the energy distribution. No significant patterns are found with this analysis. The comparison of these measurements with astrophysical scenarios can therefore be used to obtain constraints on related model parameters such as strength of cosmic-ray deflection and density of point sources. © 2015, The Author(s)., 0, info:eu-repo/semantics/published
Published: 2015
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28. Searches for anisotropies in the arrival directions of the highest energy cosmic rays detected by the Pierre Auger Observatory

Author: Markus Risse, M. Urban, A. C. Rovero, C. Bleve, M. Oliveira, S. Riggi, Vincenzo Rizi, Toshihiro Fujii, Bruno Daniel, T. Yapici, Foteini Oikonomou, J. J. Masías Meza, D. Torres Machado, A. Shadkam, D. Maurel, M. Ziolkowski, O. Martínez Bravo, G. Matthiae, Johannes Schumacher, Iván Sidelnik, A. Cordier, Juan Carlos D'Olivo, T. Pierog, Esteban Roulet, P. Abreu, D. Ravignani, Paulo J. S. Gonçalves, A. Tapia, Paula Gina Isar, A. Chiavassa, Antonio Bueno, Pedro Brogueira, F. Salesa Greus, M. Josebachuili, A. E. Herve, K. B. Barber, H. Gemmeke, G. Cocciolo, A. Dorofeev, L. R. Wiencke, Yingchun Zhu, A. Tepe, Richard Dallier, A. Nelles, Jaime Alvarez-Muñiz, Lu Lu, F. Salamida, Luis A. Anchordoqui, B. Revenu, I. A. Minaya, B. Keilhauer, André Schulz, M. Ave, Gualberto Avila, Piera Luisa Ghia, Nicolás González, J. R. Vázquez, Ingomar Allekotte, Angela V. Olinto, Igor Katkov, R. Mussa, J. J. Beatty, D. Nitz, Silvia Mollerach, H. Dembinski, N. Fazzini, I. Jandt, L. Perrone, B. Kégl, Jose Chinellato, S. Quinn, A. Segreto, P. Sanchez-Lucas, D. Harari, Lorenzo Caccianiga, M. Platino, Alberto Filevich, Peter Hansen, P. Lautridou, M. Monasor, Ralf Ulrich, L. Martin, Marco Cilmo, F. Guarino, G. S. Varner, Peter Buchholz, V. M. Theodoro, S. Messina, A. Widom, K. Link, Paul M. Mantsch, M. Szuba, Miroslav Hrabovský, Julien Aublin, Paul Sommers, F. Werner, Stefan E. Müller, Alberto Daniel Supanitsky, U. Fröhlich, Lukas Middendorf, A. Letessier-Selvon, Radomir Smida, Corinne Berat, M. Giller, I.M. Brancus, T. Rossler, A. Bridgeman, H. Glass, P. Gouffon, Marco Aglietta, M. J. Cooper, Alina Mihaela Badescu, Eun-Joo Ahn, M. Prouza, F. Sánchez, Lorenzo Cazon, C. Aramo, A. Haungs, C. E. Santo, D. Martello, S. G. Blaess, Q. Dorosti Hasankiadeh, Markus Roth, Michael Unger, A. Śmiałkowski, François Montanet, S. van Velzen, E.M. Holt, A. Saleh, Maria-Teresa Dova, M. R. Hampel, R. Alves Batista, Carlos Medina, M. De Domenico, S. J. Saffi, M. Videla, B. Tome, G. Müller, B. Vlcek, Christine Peters, Martina Bohacova, Patrick Allison, Florian Gaté, V. de Souza, L. del Peral, C. J.W.P. Timmermans, N. Scharf, Sarka Wykes, L. Villase nor, P. Heimann, L. Molina-Bueno, D. Melo, Jing Zhou, R. Meissner, David Walz, David Wittkowski, Germano Guedes, L. Nožka, R. Piegaia, E. Petermann, Miroslav Pech, Guenter Sigl, Markus Lauscher, J. Phuntsok, Raul Sarmento, J. Sorokin, B. Mitrica, Z. Szadkowski, Danielle LaHurd, Olivier Deligny, Maria Rita Coluccia, Yogendra N. Srivastava, M. I. Micheletti, Pavel Horvath, O. Ravel, A. Di Matteo, N. Awal, B. Wundheiler, G. Cataldi, Peter Schiffer, Octavian Fratu, D. Pakk Selmi-Dei, Heino Falcke, R. Sato, J. Vicha, Jörg R. Hörandel, G. Garilli, A. Gorgi, V. M. Aranda, Gregory R Snow, L. Nellen, M. Blanco, M. Palatka, Serguei Vorobiov, D. Monnier Ragaigne, Rúben Conceição, G. Rodriguez Fernandez, C. Morello, I. Lhenry-Yvon, M. Ambrosio, V. Scherini, J. Allen, M. S. Sutherland, D. Maurizio, O. A. Taborda, Dusan Mandat, H. Martinez, A. van Vliet, Alexandra Saftoiu, Carola Dobrigkeit, M. Plum, B. Wilczynska, N. Palmieri, S. Navas, M. Melissas, Peter L. Biermann, P. H. Kasper, J. F. Valdés Galicia, Eric Mayotte, M. Gómez Berisso, R. C. Shellard, I. De Mitri, A. Gascon Bravo, A. Menshikov, Sofia Andringa, Dieter Heck, M. Mallamaci, W. Docters, Moritz Münchmeyer, M. Zavrtanik, Hernán Asorey, J. Rodriguez Rojo, Paolo Privitera, G. C. Hill, Joshua A. Gordon, R. A. Vázquez, A. Filipčič, J. D. Swain, Antonio Insolia, M. E. Bertaina, Alan Watson, G. Torralba Elipe, Eva Santos, V. Novotny, A. G. Chavez, Fred Sarazin, Mario Buscemi, Ralph Engel, Petr Schovanek, D. Garcia-Gamez, J. Alvarez Castillo, E. Varela, N. Griffith, K. Weidenhaupt, F.G. Schröder, R. Krause, Enrique Zas, I. M. Pepe, J. Ridky, F. Diogo, J. Bäuml, Rossella Caruso, A. Lucero, S. Petrera, O. Kambeitz, Marc Weber, M. Kleifges, D. Zavrtanik, L. Valore, Amin Aminaei, Peter Mazur, R. M. de Almeida, C. Di Giulio, A. Stutz, S. Mathys, M. Erfani, J. Pȩkala, Fernando Contreras, Harm Schoorlemmer, Octavian Sima, J. G. Gonzalez, S. J. De Jong, M. A. Leigui de Oliveira, J. Maller, Marco Giammarchi, Sergio Sciutto, I. Al Samarai, Stijn Buitink, Sasa Micanovic, D. Lebrun, Pierre Billoir, M. Avenier, L. Ochilo, A. Curutiu, Ugo Giaccari, D. Garcia-Pinto, Jeffrey Brack, Olaf Scholten, M. S. A. B. Leão, J. R. T. de Mello Neto, Humberto Ibarguen Salazar, B. Zamorano, V. Marin, Azadeh Keivani, W. Rodrigues de Carvalho, J. W. Cronin, P. van Bodegom, M. Candusso, G. Toma, John N. Matthews, R. M. Kieckhafer, Nataliia Borodai, J. Rautenberg, O. Wainberg, Peter Gorham, W. C. Brown, L. Collica, Jiri Chudoba, L. Tomankova, G. Navarra, Thomas Harrison, P. Pieroni, F. Arqueros, P. Necesal, C. A. Moura, T. Yamamoto, Brian Fick, Samo Stanič, Hermann-Josef Mathes, J. A.J. Matthews, Xavier Bertou, Kai Daumiller, A. Zepeda, R. Meyhandan, Pedro Assis, A. Etchegoyen, R. Gaior, F. Suarez, Thomas Hebbeker, Sergio Dasso, Martín Miguel Freire, J. Lozano Bahilo, D. Kruppke-Hansen, Corbin Covault, Y. Petrov, C. Jarne, E. Trovato, B. Gookin, P. H. Nguyen, I. C. Mariş, E. M. Santos, Hernan Wahlberg, Alexander Grillo, Lino Miramonti, Bruce R. Dawson, Tim Huege, R. R. Prado, Marcio Aparecido Muller, A. Parra, R. J. Lauer, P. Ristori, M. D. Rodríguez-Frías, B. Caccianiga, N. Kunka, Luca Latronico, A. C. Fauth, Carla Bonifazi, Jose A. Bellido, Jaime Rosado, R. Cester, B. Vargas Cárdenas, T. Suomijärvi, J. Pallotta, E. J. Quel, Béatrice Fuchs, Niraj Dhital, I. Valiño, B. D. Fox, J. Neuser, Philipp Papenbreer, J. S. Díaz, Petr Travnicek, G. Parente, Ernesto Kemp, Alan Coleman, Trent D. Grubb, D. Huber, Juan Manuel Figueira, Roberta Colalillo, A. G. Mariazzi, D. Rogozin, J. de Oliveira, Alejandro Almela, Miguel Mostafá, Alex Kääpä, Colin Baus, H. Schieler, M. Fernandes, Karl-Heinz Kampert, Antonella Castellina, K. Louedec, Mariangela Settimo, Alexey Yushkov, V. Purrello, H. Blümer, Max Malacari, Piotr Homola, P. Facal San Luis, S. Le Coz, C. L. Williams, O. Krömer, C. Hojvat, Jan Ebr, Johannes Schulz, H.O. Klages, K.-H. Becker, M. Pimenta, A. P. Ferguson, M. Zimbres Silva, Gaetano Salina, A.M. van den Berg, Darko Veberič, J. Stapleton, R. Bonino, B. García, Tobias Winchen, P. Lebrun, R. López, Karen S. Caballero-Mora, J. Kleinfeller, Daniel Kuempel, Carlos Escobar, M. Ludwig, S. Hartmann, S. Maldera, Ivone F. M. Albuquerque, Ke Fang, Martin Erdmann, Roger W Clay, D. Nosek, G. Marsella, Marcus Niechciol, A. Weindl, N. Hollon, V. Verzi, David Schmidt, M. L. Díaz Castro, G. Farrar, R. Pelayo, Francesca Zuccarello, S. Querchfeld, Maurice Stephan, A. Tonachini, L. Niemietz, P.F. Gómez Vitale, N. Pacheco, Tim Niggemann, A. Porcelli, A. Aab, L. Caramete, G. Yuan, J. Stasielak, S. Coutu, C. Porowski, Denise Boncioli, German Ros, Valerio Pirronello, C. J. Todero Peixoto, N. Krohm, B. Sarkar, Christian Glaser, J. Espadanal, H. Wilczyński, S. Grebe, R. Squartini, John L. Harton, T. Paul, G. Medina-Tanco, G. van Aar, S. Jansen, D. Martraire, Aab A., Abreu P., Aglietta M., Ahn E. J., Al Samarai I., Albuquerque I. F. M., Allekotte I., Allison P., Almela A., Alvarez Castillo J., Alvarez-Muñiz J., Alves Batista R., Ambrosio M., Aminaei A., Anchordoqui L., Andringa S., Aramo C., Aranda V. M., Arqueros F., Arsene N., Asorey H., Assis P., Aublin J., Ave M., Avenier M., Avila G., Awal N., Badescu A. M., Barber K. B., Bäuml J., Baus C., Beatty J. J., Becker K. H., Bellido J. A., Berat C., Bertaina M. E., Bertou X., Biermann P. L., Billoir P., Blaess S. G., Blanco A., Blanco M., Bleve C., Blümer H., Boháčová M., Boncioli D., Bonifazi C., Borodai N., Brack J., Brancus I., Bridgeman A., Brogueira P., Brown W. C., Buchholz P., Bueno A., Buitink S., Buscemi M., Caballero-Mora K. S., Caccianiga B., Caccianiga L., Candusso M., Caramete L., Caruso R., Castellina A., Cataldi G., Cazon L., Cester R., Chavez A. G., Chiavassa A., Chinellato J. A., Chudoba J., Cilmo M., Clay R. W., Cocciolo G., Colalillo R., Coleman A., Collica L., Coluccia M. R., Conceição R., Contreras F., Cooper M. J., Cordier A., Coutu S., Covault C. E., Cronin J., Dallier R., Daniel B., Dasso S., Daumiller K., Dawson B. R., de Almeida R. M., de Jong S. J., De Mauro G., de Mello Neto J. R. T., De Mitri I., de Oliveira J., de Souza V., del Peral L., Deligny O., Dembinski H., Dhital N., Di Giulio C., Di Matteo A., Diaz J. C., Díaz Castro M. L., Diogo F., Dobrigkeit C., Docters W., D’Olivo J. C., Dorofeev A., Dorosti Hasankiadeh Q., Dova M. T., Ebr J., Engel R., Erdmann M., Erfani M., Escobar C. O., Espadanal J., Etchegoyen A., Falcke H., Fang K., Farrar G., Fauth A. C., Fazzini N., Ferguson A. P., Fernandes M., Fick B., Figueira J. M., Filevich A., Filipčič A., Fox B. D., Fratu O., Freire M. M., Fuchs B., Fujii T., García B., Garcia-Pinto D., Gate F., Gemmeke H., Gherghel-Lascu A., Ghia P. L., Giaccari U., Giammarchi M., Giller M., Głas D., Glaser C., Glass H., Golup G., Gómez Berisso M., Gómez Vitale P. F., González N., Gookin B., Gordon J., Gorgi A., Gorham P., Gouffon P., Griffith N., Grillo A. F., Grubb T. D., Guardincerri Y., Guarino F., Guedes G. P., Hampel M. R., Hansen P., Harari D., Harrison T. A., Hartmann S., Harton J. L., Haungs A., Hebbeker T., Heck D., Heimann P., Herve A. E., Hill G. C., Hojvat C., Hollon N., Holt E., Homola P., Hörandel J. R., Horvath P., Hrabovský M., Huber D., Huege T., Insolia A., Isar P. G., Jandt I., Jansen S., Jarne C., Johnsen J. A., Josebachuili M., Kääpä A., Kambeitz O., Kampert K. H., Kasper P., Katkov I., Kégl B., Keilhauer B., Keivani A., Kemp E., Kieckhafer R. M., Klages H. O., Kleifges M., Kleinfeller J., Krause R., Krohm N., Krömer O., Kuempel D., Kunka N., LaHurd D., Latronico L., Lauer R., Lauscher M., Lautridou P., Le Coz S., Lebrun D., Lebrun P., Leigui de Oliveira M. A., Letessier-Selvon A., Lhenry-Yvon I., Link K., Lopes L., López R., López Casado A., Louedec K., Lu L., Lucero A., Malacari M., Maldera S., Mallamaci M., Maller J., Mandat D., Mantsch P., Mariazzi A. G., Marin V., Mariş I. C., Marsella G., Martello D., Martin L., Martinez H., Martínez Bravo O., Martraire D., Masías Meza J. J., Mathes H. J., Mathys S., Matthews J., Matthews J. A. J., Matthiae G., Maurel D., Maurizio D., Mayotte E., Mazur P. O., Medina C., Medina-Tanco G., Meissner R., Mello V. B. B., Melo D., Menshikov A., Messina S., Meyhandan R., Micheletti M. I., Middendorf L., Minaya I. A., Miramonti L., Mitrica B., Molina-Bueno L., Mollerach S., Montanet F., Morello C., Mostafá M., Moura C. A., Muller M. A., Müller G., Müller S., Mussa R., Navarra G., Navarro J. L., Navas S., Necesal P., Nellen L., Nelles A., Neuser J., Nguyen P. H., Niculescu-Oglinzanu M., Niechciol M., Niemietz L., Niggemann T., Nitz D., Nosek D., Novotny V., Nožka L., Ochilo L., Oikonomou F., Olinto A., Pacheco N., Pakk Selmi-Dei D., Palatka M., Pallotta J., Papenbreer P., Parente G., Parra A., Paul T., Pech M., Pȩkala J., Pelayo R., Pepe I. M., Perrone L., Petermann E., Peters C., Petrera S., Petrov Y., Phuntsok J., Piegaia R., Pierog T., Pieroni P., Pimenta M., Pirronello V., Platino M., Plum M., Porcelli A., Porowski C., Prado R. R., Privitera P., Prouza M., Purrello V., Quel E. J., Querchfeld S., Quinn S., Rautenberg J., Ravel O., Ravignani D., Revenu B., Ridky J., Riggi S., Risse M., Ristori P., Rizi V., Rodrigues de Carvalho W., Rodriguez Fernandez G., Rodriguez Rojo J., Rodríguez-Frías M. D., Rogozin D., Rosado J., Roth M., Roulet E., Rovero A. C., Saffi S. J., Saftoiu A., Salamida F., Salazar H., Saleh A., Salesa Greus F., Salina G., Sánchez F., Sanchez-Lucas P., Santos E., Santos E. M., Sarazin F., Sarkar B., Sarmento R., Sato R., Scarso C., Schauer M., Scherini V., Schieler H., Schiffer P., Schmidt D., Scholten O., Schoorlemmer H., Schovánek P., Schröder F. G., Schulz A., Schulz J., Schumacher J., Sciutto S. J., Segreto A., Settimo M., Shadkam A., Shellard R. C., Sidelnik I., Sigl G., Sima O., Śmiałkowski A., Šmída R., Snow G. R., Sommers P., Sorokin J., Squartini R., Srivastava Y. N., Stanca D., Stanič S., Stapleton J., Stasielak J., Stephan M., Stutz A., Suarez F., Suomijärvi T., Supanitsky A. D., Sutherland M. S., Swain J., Szadkowski Z., Taborda O. A., Tapia A., Tepe A., Theodoro V. M., Tiffenberg J., Timmermans C., Todero Peixoto C. J., Toma G., Tomankova L., Tomé B., Tonachini A., Torralba Elipe G., Torres Machado D., Travnicek P., Ulrich R., Unger M., Urban M., Valdés Galicia J. F., Valiño I., Valore L., van Aar G., van Bodegom P., van den Berg A. M., van Velzen S., van Vliet A., Varela E., Vargas Cárdenas B., Varner G., Vasquez R., Vázquez J. R., Vázquez R. A., Veberič D., Verzi V., Vicha J., Videla M., Villaseñor L., Vlcek B., Vorobiov S., Wahlberg H., Wainberg O., Walz D., Watson A. A., Weber M., Weidenhaupt K., Weindl A., Werner F., Widom A., Wiencke L., Wilczyński H., Winchen T., Wittkowski D., Wundheiler B., Wykes S., Yang L., Yapici T., Yushkov A., Zas E., Zavrtanik D., Zavrtanik M., Zepeda A., Zhu Y., Zimmermann B., Ziolkowski M., Zuccarello F., Research unit Astroparticle Physics, Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Joseph Fourier - Grenoble 1 (UJF)-Centre National de la Recherche Scientifique (CNRS), Unité Scientifique de la Station de Nançay (USN), Centre National de la Recherche Scientifique (CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire des Sciences de l'Univers en région Centre (OSUC), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS)-Université d'Orléans (UO), Laboratoire SUBATECH Nantes (SUBATECH), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université de Nantes (UN)-Mines Nantes (Mines Nantes), Institut de Physique Nucléaire d'Orsay (IPNO), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), Laboratoire de l'Accélérateur Linéaire (LAL), Pierre Auger, ANR-11-IDEX-0004,SUPER,Sorbonne Universités à Paris pour l'Enseignement et la Recherche(2011), European Project: 246806,EC:FP7:PEOPLE,FP7-PEOPLE-2009-IRSES,EPLANET(2011), European Project: 328826,EC:FP7:PEOPLE,FP7-PEOPLE-2012-IEF,AUGER2FUTURE(2013), Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Centre National de la Recherche Scientifique (CNRS), Observatoire des Sciences de l'Univers en région Centre (OSUC), Université Paris sciences et lettres (PSL)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS), Mines Nantes (Mines Nantes)-Université de Nantes (UN)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Aab, A., Abreu, P., Aglietta, M., Ahn, E. J., Samarai, I. Al, Albuquerque, I. F. M., Allekotte, I., Allen, J., Allison, P., Almela, A., Castillo, J. Alvarez, Alvarez Muniz, J., Batista, R. Alve, Ambrosio, M., Aminaei, A., Anchordoqui, L., Andringa, S., Aramo, C., Aranda, V. M., Arqueros, F., Asorey, H., Assis, P., Aublin, J., Ave, M., Avenier, M., Avila, G., Awal, N., Badescu, A. M., Barber, K. B., Bäuml, J., Baus, C., Beatty, J. J., Becker, K. H., Bellido, J. A., Berat, C., Bertaina, M. E., Bertou, X., Biermann, P. L., Billoir, P., Blaess, S. G., Blanco, M., Bleve, C., Blumer, H., Bohačova, M., Boncioli, D., Bonifazi, C., Bonino, R., Borodai, N., Brack, J., Brancus, I., Bridgeman, A., Brogueira, P., Brown, W. C., Buchholz, P., Bueno, A., Buitink, S., Buscemi, M., Caballero Mora, K. S., Caccianiga, B., Caccianiga, L., Candusso, M., Caramete, L., Caruso, R., Castellina, A., Cataldi, G., Cazon, L., Cester, R., Chavez, A. G., Chiavassa, A., Chinellato, J. A., Chudoba, J., Cilmo, M., Clay, R. W., Cocciolo, G., Colalillo, Roberta, Coleman, A., Collica, L., Coluccia, M. R., Conceicao, R., Contreras, F., Cooper, M. J., Cordier, A., Coutu, S., Covault, C. E., Cronin, J., Curutiu, A., Dallier, R., Daniel, B., Dasso, S., Daumiller, K., Dawson, B. R., Almeida, R. M. De, Domenico, M. De, Jong, S. J. De, De Mello Neto, J. R. T., Mitri, I. De, Oliveira, J. De, Souza, V. De, Peral, L. Del, Deligny, O., Dembinski, H., Dhital, N., Giulio, C. Di, Matteo, A. Di, Diaz, J. C., Castro, M. L. Diaz, Diogo, F., Dobrigkeit, C., Docters, W., D'Olivo, J. C., Dorofeev, A., Hasankiadeh, Q. Dorosti, Dova, M. T., Ebr, J., Engel, R., Erdmann, M., Erfani, M., Escobar, C. O., Espadanal, J., Etchegoyen, A., Luis, P. Facal San, Falcke, H., Fang, K., Farrar, G., Fauth, A. C., Fazzini, N., Ferguson, A. P., Fernandes, M., Fick, B., Figueira, J. M., Filevich, A., Filipčič, A., Fox, B. D., Fratu, O., Freire, M. M., Frohlich, U., Fuchs, B., Fujii, T., Gaior, R., Garcia, B., Gamez, D. Garcia, Pinto, D. 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A., Muller, G., Muller, S., Munchmeyer, M., Mussa, R., Navarra, G., Navas, S., Necesal, P., Nellen, L., Nelles, A., Neuser, J., Nguyen, P. H., Niechciol, M., Niemietz, L., Niggemann, T., Nitz, D., Nosek, D., Novotny, V., Nožka, L., Ochilo, L., Oikonomou, F., Olinto, A., Oliveira, M., Pacheco, N., Dei, D. Pakk Selmi, Palatka, M., Pallotta, J., Palmieri, N., Papenbreer, P., Parente, G., Parra, A., Paul, T., Pech, M., Pkala, J., Pelayo, R., Pepe, I. M., Perrone, L., Petermann, E., Peters, C., Petrera, S., Petrov, Y., Phuntsok, J., Piegaia, R., Pierog, T., Pieroni, P., Pimenta, M., Pirronello, V., Platino, M., Plum, M., Porcelli, A., Porowski, C., Prado, R. R., Privitera, P., Prouza, M., Purrello, V., Quel, E. J., Querchfeld, S., Quinn, S., Rautenberg, J., Ravel, O., Ravignani, D., Revenu, B., Ridky, J., Riggi, S., Risse, M., Ristori, P., Rizi, V., Carvalho, W. Rodrigues De, Fernandez, G. Rodriguez, Rojo, J. Rodriguez, Frias, M. D. Rodriguez, Rogozin, D., Ros, G., Rosado, J., Rossler, T., Roth, M., Roulet, E., Rovero, A. C., Saffi, S. J., Saftoiu, A., Salamida, F., Salazar, H., Saleh, A., Greus, F. Salesa, Salina, G., Sanchez, F., Lucas, P. Sanchez, Santo, C. E., Santos, E., Santos, E. M., Sarazin, F., Sarkar, B., Sarmento, R., Sato, R., Scharf, N., Scherini, V., Schieler, H., Schiffer, P., Schmidt, D., Scholten, O., Schoorlemmer, H., Schovanek, P., Schroder, F. G., Schulz, A., Schulz, J., Schumacher, J., Sciutto, S. J., Segreto, A., Settimo, M., Shadkam, A., Shellard, R. C., Sidelnik, I., Sigl, G., Sima, O., ͆miałkowski, A., Šmada, R., Snow, G. R., Sommers, P., Sorokin, J., Squartini, R., Srivastava, Y. N., Stanič, S., Stapleton, J., Stasielak, J., Stephan, M., Stutz, A., Suarez, F., Suomijarvi, T., Supanitsky, A. D., Sutherland, M. S., Swain, J., Szadkowski, Z., Szuba, M., Taborda, O. A., Tapia, A., Tepe, A., Theodoro, V. M., Timmermans, C., Peixoto, C. J. Todero, Toma, G., Tomankova, L., Tomé, B., Tonachini, A., Elipe, G. Torralba, Machado, D. Torre, Travnicek, P., Trovato, E., Ulrich, R., Unger, M., Urban, M., Galicia, J. F. Valdé, Valino, I., Valore, Laura, Aar, G. Van, Bodegom, P. Van, Berg, A. M. Van Den, Velzen, S. Van, Vliet, A. Van, Varela, E., Cardenas, B. Varga, Varner, G., Vazquez, J. R., Vazquez, R. A., Veberič, D., Verzi, V., Vicha, J., Videla, M., Nor, L. Villase, Vlcek, B., Vorobiov, S., Wahlberg, H., Wainberg, O., Walz, D., Watson, A. A., Weber, M., Weidenhaupt, K., Weindl, A., Werner, F., Widom, A., Wiencke, L., Wilczyńska, B., Wilczyński, H., Williams, C., Winchen, T., Wittkowski, D., Wundheiler, B., Wykes, S., Yamamoto, T., Yapici, T., Yuan, G., Yushkov, A., Zamorano, B., Zas, E., Zavrtanik, D., Zavrtanik, M., Zepeda, A., Zhou, J., Zhu, Y., Silva, M. Zimbre, Ziolkowski, M., Zuccarello, F., Laboratoire de Physique Subatomique et de Cosmologie ( LPSC ), Université Joseph Fourier - Grenoble 1 ( UJF ) -Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Centre National de la Recherche Scientifique ( CNRS ) -Université Grenoble Alpes ( UGA ), Unité Scientifique de la Station de Nançay ( USN ), Observatoire de Paris-Université d'Orléans ( UO ) -Centre National de la Recherche Scientifique ( CNRS ), Laboratoire SUBATECH Nantes ( SUBATECH ), Mines Nantes ( Mines Nantes ) -Université de Nantes ( UN ) -Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Centre National de la Recherche Scientifique ( CNRS ), Institut de Physique Nucléaire d'Orsay ( IPNO ), Université Paris-Sud - Paris 11 ( UP11 ) -Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Centre National de la Recherche Scientifique ( CNRS ), Laboratoire de l'Accélérateur Linéaire ( LAL ), ANR-11-IDEX-0004-02/10-LABX-0063,ILP,Institute Lagrange of Paris ( 2011 ), European Project : 246806,EC:FP7:PEOPLE,FP7-PEOPLE-2009-IRSES,EPLANET ( 2011 ), European Project : 328826,EC:FP7:PEOPLE,FP7-PEOPLE-2012-IEF,AUGER2FUTURE ( 2013 ), UNIVERSIDADE DE ESTADUAL DE CAMPINAS, Physics, Elementary Particle Physics, Ahn, E. . J., Al Samarai, I., Albuquerque, I. . F. . M., Alvarez Castillo, J., Alvarez Muñiz, J., Alves Batista, R., Aranda, V. . M., Arsene, N., Badescu, A. . M., Barber, K. . B., Beatty, J. . J., Becker, K. . H., Bellido, J. . A., Bertaina, M. . E., Biermann, P. . L., Blaess, S. . G., Blanco, A., Bleve, Carla, Blümer, H., Boháčová, M., Brown, W. . C., Caballero Mora, K. . S., Chavez, A. . G., Chinellato, J. . A., Clay, R. . W., Colalillo, R., Coluccia, MARIA RITA, Conceição, R., Cooper, M. . J., Covault, C. . E., Dawson, B. . R., de Almeida, R. . M., de Jong, S. . J., De Mauro, G., de Mello Neto, J. . R. . T., DE MITRI, Ivan, de Oliveira, J., de Souza, V., del Peral, L., Di Giulio, C., Di Matteo, A., Diaz, J. . C., Díaz Castro, M. . L., D’Olivo, J. . C., Dorosti Hasankiadeh, Q., Dova, M. . T., Escobar, C. . O., Fauth, A. . C., Ferguson, A. . P., Figueira, J. . M., Fox, B. . D., Freire, M. . M., García, B., Garcia Pinto, D., Gherghel Lascu, A., Ghia, P. . L., Głas, D., Golup, G., Gómez Berisso, M., Gómez Vitale, P. . F., González, N., Grillo, A. . F., Grubb, T. . D., Guardincerri, Y., Guarino, F., Guedes, G. . P., Hampel, M. . R., Harrison, T. . A., Harton, J. . L., Herve, A. . E., Hill, G. . C., Hörandel, J. . R., Hrabovský, M., Isar, P. . G., Johnsen, J. . A., Kääpä, A., Kampert, K. . H., Kieckhafer, R. . M., Klages, H. . O., Krömer, O., Le Coz, S., Leigui de Oliveira, M. . A., Lopes, L., López, R., López Casado, A., Mariazzi, A. . G., Mariş, I. . C., Marsella, Giovanni, Martello, Daniele, Martínez Bravo, O., Masías Meza, J. . J., Mathes, H. . J., Matthews, J. . A. . J., Mazur, P. . O., Medina Tanco, G., Mello, V. . B. . B., Micheletti, M. . I., Minaya, I. . A., Molina Bueno, L., Mostafá, M., Moura, C. . A., Muller, M. . A., Müller, G., Müller, S., Navarro, J. . L., Nguyen, P. . H., Niculescu Oglinzanu, M., Pakk Selmi Dei, D., Pȩkala, J., Pepe, I. . M., Perrone, Lorenzo, Prado, R. . R., Quel, E. . J., Rodrigues de Carvalho, W., Rodriguez Fernandez, G., Rodriguez Rojo, J., Rodríguez Frías, M. . D., Rovero, A. . C., Saffi, S. . J., Salesa Greus, F., Sánchez, F., Sanchez Lucas, P., Santos, E. . M., Scarso, C., Schauer, M., Scherini, Viviana, Schovánek, P., Schröder, F. . G., Sciutto, S. . J., Shellard, R. . C., Śmiałkowski, A., Šmída, R., Snow, G. . R., Srivastava, Y. . N., Stanca, D., Suomijärvi, T., Supanitsky, A. . D., Sutherland, M. . S., Taborda, O. . A., Theodoro, V. . M., Tiffenberg, J., Todero Peixoto, C. . J., Torralba Elipe, G., Torres Machado, D., Valdés Galicia, J. . F., Valiño, I., Valore, L., van Aar, G., van Bodegom, P., van den Berg, A. . M., van Velzen, S., van Vliet, A., Vargas Cárdenas, B., Vasquez, R., Vázquez, J. . R., Vázquez, R. . A., Villaseñor, L., Watson, A. . A., Yang, L., and Zimmermann, B.
Subjects: acceleration of particles, astroparticle physics, Nuclear and High Energy Physics, [PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], Upper Limit, Astronomy, Ciencias Físicas, Astrophysics::High Energy Astrophysical Phenomena, FOS: Physical sciences, Field, Cosmic ray, Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, Otras Ciencias Físicas, 01 natural sciences, Settore FIS/04 - Fisica Nucleare e Subnucleare, Settore FIS/05 - Astronomia e Astrofisica, Observatory, Spectrum, 0103 physical sciences, acceleration of particles, astroparticle physics, Surface Detector, 010303 astronomy & astrophysics, acceleration of particle, Astrophysics::Galaxy Astrophysics, Physics, Pierre Auger Observatory, High Energy Astrophysical Phenomena (astro-ph.HE), 010308 nuclear & particles physics, Settore FIS/01 - Fisica Sperimentale, Array, Astrophysics::Instrumentation and Methods for Astrophysics, [ PHYS.ASTR.HE ] Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], astroparticle physic, Astronomy and Astrophysics, ASTROFÍSICA, Nuclei, Space and Planetary Science, Experimental High Energy Physics, ComputingMethodologies_DOCUMENTANDTEXTPROCESSING, Física nuclear, Catalog, Sky, Astrophysics - High Energy Astrophysical Phenomena, CIENCIAS NATURALES Y EXACTAS
Abstract: We analyze the distribution of arrival directions of ultra-high energy cosmic rays recorded at the Pierre Auger Observatory in 10 years of operation. The data set, about three times larger than that used in earlier studies, includes arrival directions with zenith angles up to $80^\circ$, thus covering from $-90^\circ$ to $+45^\circ$ in declination. After updating the fraction of events correlating with the active galactic nuclei (AGNs) in the V��ron-Cetty and V��ron catalog, we subject the arrival directions of the data with energies in excess of 40 EeV to different tests for anisotropy. We search for localized excess fluxes and for self-clustering of event directions at angular scales up to $30^\circ$ and for different threshold energies between 40~EeV and 80~EeV. We then look for correlations of cosmic rays with celestial structures both in the Galaxy (the Galactic Center and Galactic Plane) and in the local Universe (the Super-Galactic Plane). We also examine their correlation with different populations of nearby extragalactic objects: galaxies in the 2MRS catalog, AGNs detected by Swift-BAT, radio galaxies with jets and the Centaurus~A galaxy. None of the tests shows a statistically significant evidence of anisotropy. The strongest departures from isotropy (post-trial probability ${\sim}1.4$\%) are obtained for cosmic rays with $E>58$~EeV in rather large windows around Swift AGNs closer than 130~Mpc and brighter than $10^{44}$~erg/s (18$^\circ$ radius) and around the direction of Centaurus~A (15$^\circ$ radius)., Replaced with published version. Added Journal reference and DOI
Published: 2015
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29. Erratum to ‘‘Measurement of the atmospheric muon flux with a 4 GeV threshold in the ANTARES neutrino telescope'

Author: M. Ageron, J. A. Aguilar, A. Albert, F. Ameli, M. Anghinolfi, G. Anton, S. Anvar, M. Ardid, J. J. Aubert, J. Aublin, R. Auer, S. Basa, M. Bazzotti, V. Bertin, C. Bigongiari, M. Bou Cabo, M. C. Bouwhuis, R. Bruijn, J. Brunner, G. F. Burgio, J. Busto, F. Camarena, A. Capone, J. Carr, D. Castel, E. C.a.s.t.o.r.i.n.a., .V. Cavasinni, P.h. Charvis, M. Circella, C. Colnard, R. Coniglione, H. Costantini, N. Cottini, P. Coyle, G. De Bonis, P. Decowski, I. Dekeyser, A. D.e.s.c.h.a.m.p.s., .C. Donzaud, D. D.o.r.n.i.c., .D. Drouhin, F. Druillole, T. Eberl, J. P. Ernenwein, S. Escoffier, E. F.a.l.c.h.i.n.i., .F. Fehr, V. Flaminio, K. Fratini, J. L. Fuda, K. Graf, G. Guillard, G. Hallewell, Y. Hello, J. J. Hernández Rey, J. Hößl, M. de Jong, N. Kalantar Nayestanaki, O. Kalekin, A. Kappes, U. Katz, P. Kooijman, C. Kopper, A. Kouchner, W. K.r.e.t.s.c.h.m.e.r., .S. Kuch, R. Lahmann, P. Lamare, G. L.a.m.b.a.r.d., .H. Laschinsky, J. Lavalle, H. Le Provost, D. Lefèvre, G. Lelaizant, G. Lim, D. Lo Presti, H. Loehner, S. L.o.u.c.a.t.o.s., .F. Louis, F. L.u.c.a.r.e.l.l.i., .K. Lyons, S. M.a.n.g.a.n.o., .M. Marcelin, J. A. Martinez Mora, G. M.a.u.r.i.n., .A. Mazure, M. Melissas, E. Migneco, T. Montaruli, M. M.o.r.g.a.n.t.i., .L. Moscoso, H. Motz, C. N.a.u.m.a.n.n., .R. Ostasch, G. E. Pa, 728, va, 728, l.a.s., P. Payre, J. Petrovic, C. Petta, P. Piattelli, C. Picq, R. Pillet, V. Popa, T. P.r.a.d.i.e.r., .E. Presani, C. R.a.c.c.a., .A. Radu, C. Reed, C. Richardt, M. Rujoiu, M. Ruppi, G. V. Russo, F. S.a.l.e.s.a., .P. Sapienza, F. Schoeck, J. P. Schuller, R. Shanidze, G. van der Steenhoven, C. T.a.m.b.u.r.i.n.i., .L. Tasca, S. Toscano, M. Vecchi, P. Vernin, G. Wijnker, E. de Wolf, D. Zaborov, J. D. Zornoza, J. Zúñiga, BIAGI, SIMONE, CARMINATI, GIADA, CECCHINI, STEFANO, CHIARUSI, TOMMASO, GIACOMELLI, GIORGIO MARIA, MARGIOTTA, ANNARITA, SPURIO, MAURIZIO, M. Ageron, J.A. Aguilar , A. Albert , F. Ameli , M. Anghinolfi , G. Anton, S. Anvar , M. Ardid , J.-J. Aubert , J. Aublin ,R. Auer ,S. Basa ,M. Bazzotti ,V. Bertin ,S. Biagi,A. Bigi,C. Bigongiari , M. Bou-Cabo ,M.C. Bouwhuis ,R. Bruijn ,J. Brunner ,G.F. Burgio ,J. Busto ,F. Camarena ,A. Capone , G. Carminati ,J. Carr ,D. Castel ,E. Castorina,V. Cavasinni,S. Cecchini ,Ph. Charvis ,T. Chiarusi ,M. Circella ,C. Colnard ,R. Coniglione ,H. Costantini ,N. Cottini ,P. Coyle ,G. De Bonis ,P. Decowski , I. Dekeyser ,A. Deschamps,C. Donzaud,D. Dornic,D. Drouhin,F. Druillole ,T. Eberl,J.-P. Ernenwein , S. Escoffier ,E. Falchini,F. Fehr,V. Flaminio,K. Fratini ,J.-L. Fuda,G. Giacomelli ,K. Graf ,G. Guillard, G. Hallewell ,Y. Hello ,J.J. Hernández-Rey ,J. Hößl,M. de Jong,N. Kalantar-Nayestanaki ,O. Kalekin , A. Kappes ,U. Katz,P. Kooijman ,C. Kopper ,A. Kouchner ,W. Kretschmer,S. Kuch,R. Lahmann, P. Lamare ,G. Lambard,H. Laschinsky,J. Lavalle,H.Le Provost,D. Lefèvre ,G. Lelaizant ,G. Lim, D. Lo Presti ,H. Loehner ,S. Loucatos,F. Louis,F. Lucarelli,K. Lyons,S. Mangano,M. Marcelin,A. Margiotta ,J.A. Martinez-Mora ,G. Maurin,A. Mazure,M. Melissas ,E.Migneco,T. Montaruli, M. Morganti,L. Moscoso,H. Motz ,C. Naumann,R. Ostasch,G.E. Pa&#728, va&#728, and las,P. Payre,J. Petrovic , C. Petta ,P. Piattelli ,C. Picq,R. Pillet ,V. Popa ,T. Pradier,E. Presani,C. Racca,A. Radu,C. Reed, C. Richardt ,M. Rujoiu ,M. Ruppi,G.V. Russo ,F. Salesa,P. Sapienza,F. Schoeck ,J.-P. Schuller , R. Shanidze ,F. Simeone,M. Spurio,G. van der Steenhoven ,C. Tamburini,L. Tasca,S. Toscano , M. Vecchi ,P. Vernin,G. Wijnker ,E. de Wolf,D. Zaborov,J.D. Zornoza ,J. Zúñiga.
Subjects: ATMOSPHERIC MUONS
Published: 2010

30. Depth of maximum of air-shower profiles at the Pierre Auger Observatory. I. Measurements at energies above1017.8 eV

Author: M. Ambrosio, E. Petermann, Miroslav Pech, A. van Vliet, A. Dorofeev, K. Louedec, Mariangela Settimo, K. H. Kampert, Pavel Horvath, Alexey Yushkov, Igor Katkov, Eric Mayotte, M. Ave, M. Gómez Berisso, S. Quinn, C. J.W.P. Timmermans, E. J. Ahn, V. Purrello, H. Blümer, Max Malacari, H. Schoorlemmer, R. C. Shellard, W. Docters, L. Villaseñor, Piotr Homola, A. Segreto, P. Facal San Luis, M. Josebachuili, Alex Kääpä, Günter Sigl, S. Le Coz, D. Nitz, C. L. Williams, L. Martin, O. Krömer, Marco Cilmo, Colin Baus, A. Chiavassa, A. E. Herve, K. B. Barber, Sofia Andringa, Radomir Smida, J. F. Valdés Galicia, I. De Mitri, A. Gascon Bravo, H. Schieler, H. J. Mathes, S. T. Garcia Roca, Azadeh Keivani, M. Fernandes, Antonella Castellina, V. de Souza, B. García, L. R. Wiencke, Tobias Winchen, P. Lebrun, R. López, Karen S. Caballero-Mora, M. Ludwig, S. Hartmann, Martin Erdmann, Roger W Clay, A. Gorgi, R. Mussa, J. J. Beatty, H. Dembinski, Jörg R. Hörandel, G. Garilli, J. Rodriguez Rojo, D. Nosek, W. Rodrigues de Carvalho, M. Tartare, J. W. Cronin, Johannes Schulz, K.-H. Becker, M. Pimenta, M. Videla, J. Lozano Bahilo, B. Wilczynska, A. G. Chavez, Enrique Zas, B. Zamorano, J. Maller, Corbin Covault, D. Garcia-Pinto, Leigui de Oliveira, B. Revenu, U. Fröhlich, J. R. Vázquez, D. Garcia-Gamez, P. Sanchez-Lucas, D. Harari, G. Marsella, Y. Petrov, Matías Rolf Hampel, C. Di Giulio, Fernando Contreras, P. van Bodegom, G. Toma, Jose Chinellato, E.M. Holt, A. Saleh, Maria-Teresa Dova, M. Zimbres Silva, J. Stapleton, P. Lautridou, Richard Dallier, Alberto Daniel Supanitsky, I. Al Samarai, O. Kambeitz, Lino Miramonti, N. Fazzini, Julien Aublin, Sasa Micanovic, S. Grebe, A. Widom, A. Nelles, Kai Daumiller, N. Palmieri, Yingchun Zhu, R. Alves Batista, Sarka Wykes, Markus Roth, Jaime Alvarez-Muñiz, Lu Lu, A.M. van den Berg, L. Perrone, Jiri Chudoba, F. Salamida, V. Marin, A. Weindl, Nataliia Borodai, G. P. Guedes, A. Tepe, I. Rodriguez Cabo, Toshihiro Fujii, A. Letessier-Selvon, M. Risse, R. Meyhandan, A. Menshikov, B. Vargas Cárdenas, T. Suomijärvi, J. Pallotta, E. J. Quel, Alina Mihaela Badescu, L. Caramete, A. Shadkam, R. Squartini, G. Torralba Elipe, Eva Santos, T. Paul, Jing Zhou, R. Meissner, M. Will, A. Di Matteo, I. A. Minaya, B. Keilhauer, Thomas Harrison, T. Rossler, A. Bridgeman, J. Allen, André Schulz, S. J. Sciutto, A. F. Grillo, S. J. Saffi, B. Wundheiler, Lorenzo Cazon, Gregory R Snow, P. H. Kasper, G. Parente, G. S. Varner, R. Krause, M. Avenier, P. Pieroni, Octavian Fratu, R. Gaior, L. Valore, Amin Aminaei, N. Hollon, V. Verzi, S. Jansen, Juan Carlos D'Olivo, K. Weidenhaupt, T. Pierog, R. Bonino, Darko Veberic, Béatrice Fuchs, Niraj Dhital, P. L. Ghia, I. Valiño, M. S. A. B. Leão, David Schmidt, Carola Dobrigkeit, M. Plum, A. Lopez Agüera, M. Buscemi, F. Arqueros, Peter Hansen, F. Guarino, John Matthews, M. Blanco, Markus Lauscher, Muller, J. Phuntsok, Raul Sarmento, Peter Buchholz, F. Suarez, Thomas Hebbeker, M. Szuba, M. Urban, A. C. Rovero, P. Necesal, C. Bleve, I. Zaw, M. Oliveira, Sergio Dasso, A. Filevich, C. Hojvat, Jan Ebr, David Wittkowski, M. Palatka, I.M. Brancus, H. Glass, Marco Aglietta, J. Neuser, S. Navas, M. Melissas, D. Rogozin, J. de Oliveira, Alejandro Almela, Paul Sommers, M. Prouza, P. Abreu, R. M. Kieckhafer, M. E. Bertaina, H.O. Klages, D. Ravignani, G. Salina, Danielle LaHurd, Olivier Deligny, S. Messina, Octavian Sima, J. G. Gonzalez, D. Lebrun, Joshua A. Gordon, R. A. Vázquez, A. Filipčič, V. Pirronello, Iuri Muniz Pepe, C. Jarne, T. Huege, A. Parra, Marco Giammarchi, F. Sarazin, P. Gouffon, M. J. Cooper, A. P. Ferguson, Dusan Mandat, G. Cocciolo, F. Sánchez, Carlos Medina, M. De Domenico, G. Cataldi, Peter Schiffer, V. Scherini, Alexandra Saftoiu, I. Lhenry-Yvon, J. Rautenberg, O. Wainberg, D. Heck, W. C. Brown, G. Matthiae, J. Kleinfeller, Jeffrey Brack, Olaf Scholten, Humberto Ibarguen Salazar, I. C. Mariş, S. Petrera, Marc Weber, Hernan Wahlberg, Vincenzo Rizi, D. Martello, Sutherland, M. Ziolkowski, Silvia Mollerach, O. Martínez Bravo, N. Scharf, P. Heimann, F. Gate, Daniel Kuempel, E. Kemp, Serguei Vorobiov, Carlos Escobar, D. Monnier Ragaigne, Miguel Mostafa, Antonio Bueno, Alan Watson, J. Alvarez Castillo, J. D. Swain, M. Platino, M. Monasor, M. Candusso, Peter Gorham, G. Medina-Tanco, R. R. Prado, Iván Sidelnik, A. Cordier, S. Maldera, O. A. Taborda, Ivone F. M. Albuquerque, Ke Fang, L. Tomankova, Johannes Schumacher, R. J. Lauer, H. Martinez, Maria Rita Coluccia, Bruno Daniel, T. Yapici, J. J. Masías Meza, G. Navarra, Gualberto Avila, Moritz Münchmeyer, G. C. Hill, L. Collica, Martina Bohacova, D. Maurel, Ingomar Allekotte, G. van Aar, Patrick Allison, Jan P{ ke}kala, C. A. Moura, T. Yamamoto, Brian Fick, Samo Stanič, P. Ristori, A. Insolia, M. Kleifges, D. Zavrtanik, S. Müller, Ralph Engel, J. Sorokin, J. Ridky, Angela V. Olinto, L. Nellen, F. Diogo, M. Mallamaci, R. M. de Almeida, A. Tapia, B. D. Fox, A. Porcelli, A. Stutz, H. Gemmeke, M. Unger, C. Morello, Yogendra N. Srivastava, M. I. Micheletti, Lorenzo Caccianiga, V. M. Theodoro, V. Novotny, B. Caccianiga, Rúben Conceição, J. Bäuml, Rossella Caruso, A. Lucero, Luca Latronico, S. Mathys, M. Erfani, M. L. Díaz Castro, G. Farrar, A. C. Fauth, Carla Bonifazi, Jose A. Bellido, Francesca Zuccarello, B. Tome, G. Müller, Stijn Buitink, Nicolas Martin Gonzalez, Peter L. Biermann, Maurice Stephan, B. Vlcek, Jaime Rosado, R. Cester, Paolo Privitera, A. Tonachini, K. Link, L. Molina-Bueno, D. Melo, David Walz, Miroslav Hrabovský, P.F. Gómez Vitale, D. Pakk Selmi-Dei, R. Sato, A. Haungs, J. L. Harton, S. G. Blaess, F. Werner, P. Mantsch, Z. Szadkowski, D. Maurizio, J. C. Diaz, E. Varela, N. Griffith, François Montanet, S. van Velzen, L. Ochilo, J. Stasielak, S. Coutu, C. Aramo, A. ͆miałkowski, Q. Dorosti Hasankiadeh, B. Mitrica, Heino Falcke, J. Vicha, C. Porowski, Paulo J. S. Gonçalves, I. Jandt, Denise Boncioli, Ralf Ulrich, German Ros, J. A.J. Matthews, Xavier Bertou, Marcus Niechciol, A. Zepeda, Pedro Assis, A. Etchegoyen, R. Pelayo, L. Nožka, R. Piegaia, S. Querchfeld, M. Zavrtanik, L. Niemietz, N. Pacheco, V. M. Aranda, Tim Niggemann, D. Kruppke-Hansen, Petr Schovanek, A. Aab, N. Kunka, G. Yuan, Matias Tueros, S. Riggi, Luis A. Anchordoqui, Philipp Papenbreer, Petr Travnicek, Rodríguez-Frías, E. Trovato, Alan Coleman, B. Gookin, Trent D. Grubb, D. Huber, Juan Manuel Figueira, P. H. Nguyen, Roberta Colalillo, A. G. Mariazzi, E. M. Santos, Bruce R. Dawson, P.O. Mazur, C. J. Todero Peixoto, N. Krohm, B. Sarkar, Christian Glaser, J. Espadanal, S. J. De Jong, H. Wilczyński, Pierre Billoir, A. Curutiu, L. del Peral, O. Ravel, Ugo Giaccari, D. Torres Machado, N. Awal, Paula Gina Isar, Pedro Brogueira, F. Salesa Greus, J. R. T. de Mello Neto, Esteban Roulet, Corinne Berat, D. Martraire, M. Giller, C. E. Santo, Lukas Middendorf, Christine Peters, Balázs Kégl, G. Rodriguez Fernandez, and Hernán Asorey
Subjects: Pierre Auger Observatory, Physics, Nuclear and High Energy Physics, Mass distribution, 010308 nuclear & particles physics, Astrophysics::High Energy Astrophysical Phenomena, Astrophysics::Instrumentation and Methods for Astrophysics, Cosmic ray, Astrophysics, 01 natural sciences, Standard deviation, Computational physics, Auger, Air shower, Observatory, 0103 physical sciences, Mass spectrum, 010303 astronomy & astrophysics
Abstract: We report a study of the distributions of the depth of maximum, X-max, of extensive air-shower profiles with energies above 10(17.8) eV as observed with the fluorescence telescopes of the Pierre Auger Observatory. The analysis method for selecting a data sample with minimal sampling bias is described in detail as well as the experimental cross-checks and systematic uncertainties. Furthermore, we discuss the detector acceptance and the resolution of the X-max measurement and provide parametrizations thereof as a function of energy. The energy dependence of the mean and standard deviation of the X-max distributions are compared to air-shower simulations for different nuclear primaries and interpreted in terms of the mean and variance of the logarithmic mass distribution at the top of the atmosphere.
Published: 2014
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31. Muons in air showers at the Pierre Auger Observatory: Measurement of atmospheric production depth

Author: Adrian J. Matthews, L. Molina-Bueno, D. Melo, David Walz, F. Suarez, Thomas Hebbeker, Sergio Dasso, T. Huege, A. Parra, Jeffrey Brack, Olaf Scholten, V. Pirronello, Humberto Ibarguen Salazar, F. Gate, Iuri Muniz Pepe, L. Tomankova, G. Navarra, C. A. Moura, T. Yamamoto, Brian Fick, Samo Stanič, van den Ad M Berg, C. Jarne, M. Prouza, J. Kleinfeller, A. Aab, L. Caramete, R. Mussa, J. J. Beatty, D. Pakk Selmi-Dei, R. Sato, A. C. Fauth, Kai Daumiller, Peter Schiffer, B. Vlcek, H. Dembinski, N. Fazzini, L. del Peral, P. Abreu, M. S. A. B. Leão, H. Lyberis, E.M. Holt, D. Ravignani, A. Saleh, Maria-Teresa Dova, R. Alves Batista, D. Kruppke-Hansen, O. Ravel, G. Yuan, Matias Tueros, D. Nosek, Johannes Schulz, A. van Vliet, V. Scherini, Carla Bonifazi, Jose A. Bellido, Daniel Kuempel, Carlos Escobar, S. Maldera, M. Pimenta, F. Diogo, M. Videla, G. Cocciolo, Luis A. Anchordoqui, Marcio Aparecido Muller, D. Maurizio, Richard Dallier, A. Nelles, B. Revenu, Sarka Wykes, Jaime Alvarez-Muñiz, Jing Zhou, J. C. Diaz, M. Risse, Julien Aublin, Alexandra Saftoiu, Jaime Rosado, Ivone F. M. Albuquerque, Ke Fang, M. Zimbres Silva, O. Kambeitz, R. M. de Almeida, F. Werner, Markus Ahlers, S. Riggi, T. Rossler, Eric Mayotte, M. Ave, M. Gómez Berisso, S. J. De Jong, Octavian Fratu, B. Wilczynska, J. D. Swain, E. Varela, T. Suomijaervi, N. Griffith, Lu Lu, N. T. Thao, J. Maller, S. J. Saffi, U. Froehlich, R. Cester, M. Avenier, J. Stapleton, M. Zavrtanik, B. Vargas Cárdenas, J. Pallotta, N. Kunka, G. Marsella, J. R. Vázquez, D. Garcia-Gamez, E. J. Quel, Michael Unger, M. Platino, M. Monasor, Iván Sidelnik, N. Scharf, P. Sanchez-Lucas, D. Harari, M. Buscemi, A. Curutiu, A. Lopez Agueera, A. Kaeaepae, M. Palatka, A. Insolia, M. Kleifges, D. Zavrtanik, I. A. Minaya, P. Heimann, R. C. Shellard, W. Docters, M. Will, K. Louedec, Mariangela Settimo, Ugo Giaccari, B. Keilhauer, Béatrice Fuchs, P. W. Younk, Niraj Dhital, M. Hrabovsky, Alexey Yushkov, Jörg R. Hörandel, G. Garilli, E. Kemp, Serguei Vorobiov, C. Hojvat, Francisco J. Blanco, Jan Ebr, J. Allen, S. J. Sciutto, R. Pesce, A. Weindl, I. Valiño, Xavier Bertou, V. Purrello, Paul Sommers, L. Nellen, Max Malacari, Markus Lauscher, A. Zepeda, A. Filevich, Alina Mihaela Badescu, A. Smialkowski, Dusan Mandat, Raul Sarmento, F. Gomez Albarracin, P. Gouffon, P. N. Dong, D. Monnier Ragaigne, O. A. Taborda, Piotr Homola, M. J. Cooper, John N. Matthews, C. Morello, R. M. Kieckhafer, Juan Moreno, J. Rautenberg, Yingchun Zhu, I. Al Samarai, J. Neuser, F. Salamida, Pedro Assis, G. Matthiae, F. Sánchez, P. Facal San Luis, A. Etchegoyen, M. Josebachuili, C. J. Todero Peixoto, A. Schmidt, H.O. Klages, H. Martinez, Lorenzo Caccianiga, V. M. Theodoro, M. Ambrosio, Antonio Bueno, A. Petrolini, S. Le Coz, Carlos Medina, M. De Domenico, G. Parente, I. Lhenry-Yvon, Libor Nozka, Javier Tiffenberg, Sergio Pastor, Sasa Micanovic, O. Wainberg, D. Nitz, J. R. T. de Mello Neto, H. Bluemer, A. Gorgi, Y. Guardincerri, S. Messina, N. Krohm, C. J.W.P. Timmermans, M. Muenchmeyer, A. P. Ferguson, Peter L. Biermann, Petr Schovanek, Esteban Roulet, Jan Pękala, A. Chiavassa, G. S. Varner, Hernan Wahlberg, L. Ochilo, N. Hollon, V. Verzi, B. Sarkar, B. Tome, H. Schoorlemmer, A. E. Herve, K. B. Barber, S. Jansen, E. Petermann, Gualberto Avila, B. García, Tobias Winchen, P. Lebrun, Christian Glaser, A. Criss, Miroslav Pech, Guenter Sigl, R. López, Karen S. Caballero-Mora, Paolo Privitera, L. R. Wiencke, D. Martraire, Lukas Middendorf, Christine Peters, Ingomar Allekotte, N. Palmieri, J. Espadanal, Corinne Berat, M. Giller, W. C. Brown, K. Link, R. R. Prado, M. C. Maccarone, A. Dorofeev, Darko Veberič, Pavel Horvath, A. Menshikov, L. Latronico, G. Torralba Elipe, R. Krause, Maria Rita Coluccia, Yogendra N. Srivastava, M. I. Micheletti, M. Ludwig, C. E. Santo, Angela V. Olinto, M. Urban, R. J. Lauer, H. Wilczyński, P. Billoir, M. S. Sutherland, J. de Oliveira, A. C. Rovero, L. Valore, S. Navas, Martin Erdmann, M. Melissas, Igor Katkov, J. F. Valdés Galicia, P. Ristori, Amin Aminaei, C. Bleve, C. Aramo, K. Weidenhaupt, Rúben Conceição, R. A. Vázquez, A. Filipčič, I. De Mitri, A. Gascon Bravo, S. Grebe, A. Haungs, Eun-Joo Ahn, L. Villaseñor, I. Rodriguez Cabo, Alberto Daniel Supanitsky, J. L. Harton, V. Marin, Pham Ngoc Diep, C. Di Giulio, Q. Dorosti Hasankiadeh, Paulo J. S. Gonçalves, F. Sarazin, L. Martin, M. Oliveira, Balázs Kégl, G. P. Guedes, S. Petrera, Marc Weber, S. T. Garcia Roca, Sofia Andringa, Marco Cilmo, Philipp Papenbreer, I. Zaw, G. Rodriguez Fernandez, B. Mitrica, Heino Falcke, R. Squartini, François Montanet, Petr Travnicek, Vincenzo Rizi, H. J. Mathes, D. Martello, Bruno Daniel, Alejandro Almela, P. Mantsch, T. Paul, Z. Szadkowski, S. van Velzen, K. H. Becker, M.E. Ortiz, B. Caccianiga, J. Vicha, Trent D. Grubb, Hernán Asorey, T. Yapici, J. J. Masías Meza, D. Huber, M. Ziolkowski, D. Maurel, Roger W Clay, Silvia Mollerach, O. Martínez Bravo, Juan Manuel Figueira, M. A. Leigui de Oliveira, Marco Giammarchi, Roberta Colalillo, J. Rodriguez Rojo, R. Bonino, A. Shadkam, I. Jandt, A. G. Mariazzi, Markus Roth, E. Menichetti, R. Gaior, A. G. Chavez, Enrique Zas, B. Zamorano, Ralf Ulrich, A. Porcelli, A. F. Grillo, Juan Carlos D'Olivo, T. Pierog, Peter Hansen, Azadeh Keivani, Fernando Contreras, G. Medina-Tanco, Carola Dobrigkeit, M. Plum, G. van Aar, P. L. Ghia, F. Guarino, J. Lozano Bahilo, A. Tapia, D. Garcia-Pinto, Alan Watson, W. Rodrigues de Carvalho, Peter Buchholz, H. Gemmeke, Paula Gina Isar, Pedro Brogueira, F. Salesa Greus, J. Alvarez Castillo, M. Tartare, J. W. Cronin, M. L. Díaz Castro, G. Farrar, M. Szuba, I.M. Brancus, R. Piegaia, S. Quinn, G. Toma, H. Glass, Marco Aglietta, A. Segreto, G. Cataldi, Nataliia Borodai, K. Islo, Radomir Smida, G. Mueller, Maurice Stephan, Corbin Covault, Y. Petrov, A. Schulz, E. Trovato, A. Tonachini, V. de Souza, A. Di Matteo, Lino Miramonti, J. Baeuml, B. Gookin, C. Ruehle, P.F. Gómez Vitale, B. Wundheiler, M. Blanco, M. D. Rodríguez-Frías, Gregory R Snow, E. M. Santos, S. H. Cheng, Bruce R. Dawson, P.O. Mazur, Marcus Niechciol, R. Pelayo, P. H. Kasper, B. J. Whelan, S. Querchfeld, L. Niemietz, Miguel Mostafá, Ioana Codrina Maris, N. Pacheco, J. Roberts, Tim Niggemann, J. Stasielak, S. Coutu, Christopher B. Williams, G. C. Hill, Colin Baus, Ralph Engel, J. Ridky, C. Porowski, H. Schieler, A. Stutz, M. Fernandes, Karl-Heinz Kampert, E. Santos, Antonella Castellina, Denise Boncioli, German Ros, O. Kroemer, Jose Chinellato, P. Lautridou, A. Widom, A. Letessier-Selvon, Lorenzo Cazon, David Wittkowski, G. Salina, Danielle LaHurd, Olivier Deligny, R. Meyhandan, T. Fuji, Martina Bohacova, Patrick Allison, J. Sorokin, B. D. Fox, V. Novotny, Rossella Caruso, A. Lucero, G. La Rosa, S. Mathys, M. Erfani, Octavian Sima, J. G. Gonzalez, D. Lebrun, D. Heck, M. Candusso, Peter Gorham, L. Collica, L. Perrone, Jiri Chudoba, D. Torres Machado, Thomas Harrison, P. Pieroni, F. Arqueros, P. Necesal, Research unit Astroparticle Physics, A. Aab, P. Abreu, M. Aglietta, M. Ahler, E. Ahn, I. A. Samarai, I. Albuquerque, I. Allekotte, J. Allen, P. Allison, A. l. Almela, J. A. Castillo, J. Alvarez-Muñiz, R. A. Batista, M. Ambrosio, A. Aminaei, L. s. Anchordoqui, S. Andringa, C. Aramo, F. Arquero, H. Asorey, P. Assi, J. Aublin, M. Ave, M. Avenier, G. Avila, A. Badescu, K. Barber, J. Bäuml, C. Bau, J. Beatty, K. Becker, J. Bellido, C. Berat, X. Bertou, P. Biermann, P. Billoir, F. Blanco, M. Blanco, C. Bleve, H. a. Blümer, M. Boháčová, D. Boncioli, C. Bonifazi, R. Bonino, N. Borodai, J. Brack, I. Brancu, P. Brogueira, W. Brown, P. Buchholz, A. Bueno, M. Buscemi, K. a. am, B. Caccianiga, L. Caccianiga, M. Candusso, L. Caramete, R. Caruso, A. Castellina, G. Cataldi, L. Cazon, R. Cester, A. Chavez, S. Cheng, A. Chiavassa, J. Chinellato, J. Chudoba, M. Cilmo, R. Clay, G. Cocciolo, R. Colalillo, L. 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Gonçalve, J. Gonzalez, B. Gookin, A. Gorgi, P. Gorham, P. Gouffon, S. b. Grebe, N. Griffith, A. Grillo, T. Grubb, Y. Guardincerri, F. Guarino, G. Guede, P. Hansen, D. Harari, T. Harrison, J. Harton, A. Haung, T. Hebbeker, D. Heck, P. Heimann, A. Herve, G. Hill, C. Hojvat, N. Hollon, E. Holt, P. a. Homola, J. b. Hörandel, P. Horvath, M. b. Hrabovský, D. Huber, T. Huege, A. Insolia, P. Isar, K. Islo, I. Jandt, S. b. Jansen, C. Jarne, M. Josebachuili, A. Kääpä, O. Kambeitz, K. Kampert, P. Kasper, I. Katkov, B. Kégl, B. Keilhauer, A. Keivani, E. Kemp, R. Kieckhafer, H. Klage, M. Kleifge, J. Kleinfeller, R. Krause, N. Krohm, O. Krömer, D. Kruppke-Hansen, D. Kuempel, N. Kunka, G. L. Rosa, D. Lahurd, L. Latronico, R. Lauer, M. Lauscher, P. Lautridou, S. L. Coz, M. Leão, D. Lebrun, P. Lebrun, M. L. De, A. Letessier-Selvon, I. Lhenry-Yvon, K. Link, R. López, A. L. Agüera, K. Louedec, J. L. Bahilo, L. c. Lu, A. Lucero, M. Ludwig, H. Lyberi, M. Maccarone, M. Malacari, S. Maldera, J. Maller, D. Mandat, P. Mantsch, A. Mariazzi, V. Marin, I. Mariş, G. Marsella, D. Martello, L. a. Martin, H. Martinez, O. M. Bravo, D. Martraire, J. M. Meza, H. Mathe, S. Mathy, A. Matthew, J. Matthew, G. Matthiae, D. Maurel, D. Maurizio, E. Mayotte, P. Mazur, C. Medina, G. Medina-Tanco, M. Melissa, D. Melo, E. Menichetti, A. Menshikov, S. Messina, R. Meyhandan, S. Mićanović, M. Micheletti, L. Middendorf, I. Minaya, L. Miramonti, B. Mitrica, L. Molina-Bueno, S. Mollerach, M. Monasor, D. M. Ragaigne, F. Montanet, C. Morello, J. Moreno, M. Mostafá, C. Moura, M. c. Muller, G. Müller, M. Münchmeyer, R. Mussa, G. Navarra, S. Nava, P. Necesal, L. Nellen, A. b. Nelle, J. Neuser, M. Niechciol, L. Niemietz, T. Niggemann, D. Nitz, D. Nosek, V. Novotny, L. NoŽka, L. Ochilo, A. Olinto, M. Oliveira, M. Ortiz, N. Pacheco, D. P. Selmi-Dei, M. Palatka, J. Pallotta, N. Palmieri, P. Papenbreer, G. Parente, A. Parra, S. Pastor, T. c. Paul, M. Pech, J. Pkala, R. Pelayo, I. Pepe, L. Perrone, R. Pesce, E. Petermann, C. Peter, S. c. Petrera, A. Petrolini, Y. Petrov, R. Piegaia, T. Pierog, P. Pieroni, M. Pimenta, V. Pirronello, M. Platino, M. Plum, A. Porcelli, C. Porowski, R. Prado, P. Privitera, M. Prouza, V. Purrello, E. Quel, S. Querchfeld, S. Quinn, J. Rautenberg, O. Ravel, D. Ravignani, B. Revenu, J. Ridky, S. b. Riggi, M. Risse, P. Ristori, V. Rizi, J. Robert, W. R. De, I. R. Cabo, G. a. Rodriguez, J. R. Rojo, M. Rodríguez-Fría, G. Ro, J. Rosado, T. Rossler, M. Roth, E. Roulet, A. Rovero, C. Rühle, S. Saffi, A. Saftoiu, F. Salamida, H. Salazar, A. Saleh, F. S. Greu, G. Salina, F. Sánchez, P. Sanchez-Luca, C. Santo, E. Santo, F. Sarazin, B. Sarkar, R. Sarmento, R. Sato, N. Scharf, V. Scherini, H. Schieler, P. Schiffer, A. Schmidt, O. Scholten, H. b. bo, P. Schovánek, A. Schulz, J. Schulz, S. Sciutto, A. Segreto, M. Settimo, A. Shadkam, R. Shellard, I. Sidelnik, G. Sigl, O. Sima, A. Śmiałkowski, R. Šmída, G. Snow, P. Sommer, J. Sorokin, R. Squartini, Y. Srivastava, S. Stanič, J. Stapleton, J. Stasielak, M. Stephan, A. Stutz, F. Suarez, T. Suomijärvi, A. Supanitsky, M. Sutherland, J. Swain, Z. Szadkowski, M. Szuba, O. Taborda, A. Tapia, M. Tartare, N. Thao, V. Theodoro, J. Tiffenberg, C. b. Timmerman, C. T. Peixoto, G. Toma, L. Tomankova, B. Tomé, A. Tonachini, G. T. Elipe, D. T. Machado, P. Travnicek, E. Trovato, M. Tuero, R. Ulrich, M. Unger, M. Urban, J. V. Galicia, I. Valiño, L. Valore, G. V. Aar, A. V. Den, S. V. Velzen, A. V. Vliet, E. Varela, B. V. Cárdena, G. Varner, J. Vázquez, R. Vázquez, D. Veberič, V. Verzi, J. Vicha, M. Videla, L. Villaseñor, B. Vlcek, S. Vorobiov, H. Wahlberg, O. l. Wainberg, D. Walz, A. Watson, M. Weber, K. Weidenhaupt, A. Weindl, F. Werner, B. Whelan, A. Widom, L. Wiencke, B. Wilczyńska, H. Wilczyński, M. Will, C. William, T. Winchen, D. Wittkowski, B. Wundheiler, S. Wyke, T. Yamamoto, T. Yapici, P. Younk, G. Yuan, A. Yushkov, B. Zamorano, E. Za, D. b. Zavrtanik, M. b. Zavrtanik, I. Zaw, A. Zepeda, J. Zhou, Y. Zhu, M. Z. Silva, M. Ziolkowski, Unité Scientifique de la Station de Nançay ( USN ), Observatoire de Paris-Université d'Orléans ( UO ) -Centre National de la Recherche Scientifique ( CNRS ), Laboratoire SUBATECH Nantes ( SUBATECH ), Mines Nantes ( Mines Nantes ) -Université de Nantes ( UN ) -Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Centre National de la Recherche Scientifique ( CNRS ), Laboratoire de Physique Nucléaire et de Hautes Énergies ( LPNHE ), Université Pierre et Marie Curie - Paris 6 ( UPMC ) -Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Université Paris Diderot - Paris 7 ( UPD7 ) -Centre National de la Recherche Scientifique ( CNRS ), Laboratoire de l'Accélérateur Linéaire ( LAL ), Université Paris-Sud - Paris 11 ( UP11 ) -Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Centre National de la Recherche Scientifique ( CNRS ), Laboratoire de Physique Subatomique et de Cosmologie ( LPSC ), Université Joseph Fourier - Grenoble 1 ( UJF ) -Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Centre National de la Recherche Scientifique ( CNRS ) -Université Grenoble Alpes ( UGA ), Institut de Physique Nucléaire d'Orsay ( IPNO ), PIERRE AUGER, ANR-11-IDEX-0004-02/10-LABX-0063,ILP,Institute Lagrange of Paris ( 2011 ), ANR-11-IDEX-0004-02/11-IDEX-0004,SUPER,SUPER ( 2011 ), ANR-2010-COSI-002 (SIMINOLE),ANR-2010-COSI-002 (SIMINOLE), European Project : 246806,EC:FP7:PEOPLE,FP7-PEOPLE-2009-IRSES,EPLANET ( 2011 ), Université Joseph Fourier - Grenoble 1 ( UJF ) -Institut polytechnique de Grenoble - Grenoble Institute of Technology ( Grenoble INP ) -Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Centre National de la Recherche Scientifique ( CNRS ) -Université Grenoble Alpes ( UGA ), Unité Scientifique de la Station de Nançay (USN), Centre National de la Recherche Scientifique (CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire des Sciences de l'Univers en région Centre (OSUC), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS)-Université d'Orléans (UO), Laboratoire SUBATECH Nantes (SUBATECH), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université de Nantes (UN)-Mines Nantes (Mines Nantes), Laboratoire de Physique Nucléaire et de Hautes Énergies (LPNHE), Centre National de la Recherche Scientifique (CNRS)-Université Paris Diderot - Paris 7 (UPD7)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Pierre et Marie Curie - Paris 6 (UPMC), Laboratoire de l'Accélérateur Linéaire (LAL), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Joseph Fourier - Grenoble 1 (UJF)-Centre National de la Recherche Scientifique (CNRS), Institut de Physique Nucléaire d'Orsay (IPNO), ANR-11-IDEX-0004,SUPER,Sorbonne Universités à Paris pour l'Enseignement et la Recherche(2011), ANR-10-COSI-0002,SIMINOLE,Méthodes de simulations pour des applications de grande échelle en physique expérimentale : inférence statistique, optimisation et apprentissage discriminant(2010), European Project: 246806,EC:FP7:PEOPLE,FP7-PEOPLE-2009-IRSES,EPLANET(2011), Observatoire des Sciences de l'Univers en région Centre (OSUC), Université Paris sciences et lettres (PSL)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS), Mines Nantes (Mines Nantes)-Université de Nantes (UN)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Centre National de la Recherche Scientifique (CNRS), A., Aab, P., Abreu, M., Aglietta, M., Ahler, E., Ahn, I. A., Samarai, I., Albuquerque, I., Allekotte, J., Allen, P., Allison, A. l., Almela, J. A., Castillo, J., Alvarez Muñiz, R. 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L., Bahilo, L. c., Lu, A., Lucero, M., Ludwig, H., Lyberi, M., Maccarone, M., Malacari, S., Maldera, J., Maller, D., Mandat, P., Mantsch, A., Mariazzi, V., Marin, I., Mariş, Marsella, Giovanni, Martello, Daniele, L. a., Martin, H., Martinez, O. M., Bravo, D., Martraire, J. M., Meza, H., Mathe, S., Mathy, A., Matthew, J., Matthew, G., Matthiae, D., Maurel, D., Maurizio, E., Mayotte, P., Mazur, C., Medina, G., Medina Tanco, M., Melissa, D., Melo, E., Menichetti, A., Menshikov, S., Messina, R., Meyhandan, S., Mićanović, M., Micheletti, L., Middendorf, I., Minaya, L., Miramonti, B., Mitrica, L., Molina Bueno, S., Mollerach, M., Monasor, D. M., Ragaigne, F., Montanet, C., Morello, J., Moreno, M., Mostafá, C., Moura, M. c., Muller, G., Müller, M., Münchmeyer, R., Mussa, G., Navarra, S., Nava, P., Necesal, L., Nellen, A. b., Nelle, J., Neuser, M., Niechciol, L., Niemietz, T., Niggemann, D., Nitz, D., Nosek, V., Novotny, L., Nožka, L., Ochilo, A., Olinto, M., Oliveira, M., Ortiz, N., Pacheco, D. P., Selmi Dei, M., Palatka, J., Pallotta, N., Palmieri, P., Papenbreer, G., Parente, A., Parra, S., Pastor, T. c., Paul, M., Pech, J., Pkala, R., Pelayo, I., Pepe, Perrone, Lorenzo, R., Pesce, E., Petermann, C., Peter, S. c., Petrera, A., Petrolini, Y., Petrov, R., Piegaia, T., Pierog, P., Pieroni, M., Pimenta, V., Pirronello, M., Platino, M., Plum, A., Porcelli, C., Porowski, R., Prado, P., Privitera, M., Prouza, V., Purrello, E., Quel, S., Querchfeld, S., Quinn, J., Rautenberg, O., Ravel, D., Ravignani, B., Revenu, J., Ridky, S. b., Riggi, M., Risse, P., Ristori, V., Rizi, J., Robert, W. R., De, I. R., Cabo, G. a., Rodriguez, J. R., Rojo, M., Rodríguez Fría, G., Ro, J., Rosado, T., Rossler, M., Roth, E., Roulet, A., Rovero, C., Rühle, S., Saffi, A., Saftoiu, F., Salamida, H., Salazar, A., Saleh, F. S., Greu, G., Salina, F., Sánchez, P., Sanchez Luca, C., Santo, E., Santo, F., Sarazin, B., Sarkar, R., Sarmento, R., Sato, N., Scharf, Scherini, Viviana, H., Schieler, P., Schiffer, A., Schmidt, O., Scholten, H. b., Bo, P., Schovánek, A., Schulz, J., Schulz, S., Sciutto, A., Segreto, M., Settimo, A., Shadkam, R., Shellard, I., Sidelnik, G., Sigl, O., Sima, A., Śmiałkowski, R., Šmída, G., Snow, P., Sommer, J., Sorokin, R., Squartini, Y., Srivastava, S., Stanič, J., Stapleton, J., Stasielak, M., Stephan, A., Stutz, F., Suarez, T., Suomijärvi, A., Supanitsky, M., Sutherland, J., Swain, Z., Szadkowski, M., Szuba, O., Taborda, A., Tapia, M., Tartare, N., Thao, V., Theodoro, J., Tiffenberg, C. b., Timmerman, C. T., Peixoto, G., Toma, L., Tomankova, B., Tomé, A., Tonachini, G. T., Elipe, D. T., Machado, P., Travnicek, E., Trovato, M., Tuero, R., Ulrich, M., Unger, M., Urban, J. V., Galicia, I., Valiño, L., Valore, G. V., Aar, A. V., Den, S. V., Velzen, A. V., Vliet, E., Varela, B. V., Cárdena, G., Varner, J., Vázquez, R., Vázquez, D., Veberič, V., Verzi, J., Vicha, M., Videla, L., Villaseñor, B., Vlcek, S., Vorobiov, H., Wahlberg, O. l., Wainberg, D., Walz, A., Watson, M., Weber, K., Weidenhaupt, A., Weindl, F., Werner, B., Whelan, A., Widom, L., Wiencke, B., Wilczyńska, H., Wilczyński, M., Will, C., William, T., Winchen, D., Wittkowski, B., Wundheiler, S., Wyke, T., Yamamoto, T., Yapici, P., Younk, G., Yuan, A., Yushkov, B., Zamorano, E., Za, D. b., Zavrtanik, M. b., Zavrtanik, I., Zaw, A., Zepeda, J., Zhou, Y., Zhu, M. Z., Silva, M., Ziolkowski, Ahn, E. ?. J., I., Al Samarai, Albuquerque, I. ?. F. ?. M., A., Almela, J., Alvarez Castillo, J., Alvarez Mu?iz, R., Alves Batista, L., Anchordoqui, Aramo, Carla, Badescu, A. ?. M., Barber, K. ?. B., J., B?uml, Beatty, J. ?. J., Becker, K. ?. H., Bellido, J. ?. A., Biermann, P. ?. L., C., Bleve, H., Bl?mer, M., Boh??ov?, Brown, W. ?. C., Buscemi, Mario, Caballero Mora, K. ?. S., Chavez, A. ?. G., Cheng, S. ?. H., Chinellato, J. ?. A., Cilmo, Marco, Clay, R. ?. W., G., Cocciolo, Colalillo, Roberta, Coluccia, M. ?. R., R., Concei??o, Cooper, M. ?. J., Covault, C. ?. E., R., Dallier, S., Dasso, Dawson, B. ?. R., de Almeida, R. ?. M., M., De Domenico, de Jong, S. ?. J., de Mello Neto, J. ?. R. ?. T., I., De Mitri, J., de Oliveira, V., de Souza, L., del Peral, C., Di Giulio, A., Di Matteo, Diaz, J. ?. C., D?az Castro, M. ?. L., Diep, P. ?. N., D?olivo, J. ?. C., Dong, P. ?. N., Q., Dorosti Hasankiadeh, Dova, M. ?. T., Escobar, C. ?. O., A., Etchegoyen, P., Facal San Lui, H., Falcke, Fauth, A. ?. C., Ferguson, A. ?. P., Figueira, J. ?. M., A., Filip?i?, Fox, B. ?. D., U., Fr?hlich, B., Garc?a, Garcia Roca, S. ?. T., A., Gascon Bravo, Ghia, P. ?. L., F., Gomez Albarracin, M., G?mez Berisso, G?mez Vitale, P. ?. F., P., Gon?alve, Gonzalez, J. ?. G., S., Grebe, Grillo, A. ?. F., Grubb, T. ?. D., Guarino, Fausto, Guedes, G. ?. P., Harrison, T. ?. A., Harton, J. ?. L., Herve, A. ?. E., Hill, G. ?. C., P., Homola, H?randel, J. ?. R., M., Hrabovsk?, Isar, P. ?. G., S., Jansen, A., K??p?, Kampert, K. ?. H., B., K?gl, Kieckhafer, R. ?. M., Klages, H. ?. O., O., Kr?mer, G., La Rosa, S., Le Coz, Le?o, M. ?. S. ?. A. ?. B., Leigui de Oliveira, M. ?. A., R., L?pez, A., Lopez Ag?era, J., Lozano Bahilo, L., Lu, Maccarone, M. ?. C., Mariazzi, A. ?. G., Mari?, I. ?. C., G., Marsella, D., Martello, L., Martin, O., Mart?nez Bravo, Mas?as Meza, J. ?. J., Mathes, H. ?. J., Matthews, A. ?. J., Mazur, P. ?. O., S., Mi?anovi?, Micheletti, M. ?. I., Minaya, I. ?. A., D., Monnier Ragaigne, Moreno, J. ?. C., M., Mostaf?, Moura, C. ?. A., Muller, M. ?. A., G., M?ller, M., M?nchmeyer, A., Nelle, L., No?ka, D., Pakk Selmi Dei, T., Paul, J., P?kala, Pepe, I. ?. M., L., Perrone, S., Petrera, Prado, R. ?. R., Quel, E. ?. J., S., Riggi, W., Rodrigues de Carvalho, I., Rodriguez Cabo, G., Rodriguez Fernandez, J., Rodriguez Rojo, Rodr?guez Fr?as, M. ?. D., Rovero, A. ?. C., C., R?hle, Saffi, S. ?. J., F., Salesa Greu, F., S?nchez, Santo, C. ?. E., Santos, E. ?. M., V., Scherini, H., Schoorlemmer, P., Schov?nek, Sciutto, S. ?. J., Shellard, R. ?. C., A., ?mia?kowski, R., ?m?da, Snow, G. ?. R., Srivastava, Y. ?. N., S., Stani?, T., Suomij?rvi, Supanitsky, A. ?. D., Sutherland, M. ?. S., Taborda, O. ?. A., Thao, N. ?. T., Theodoro, V. ?. M., C., Timmerman, Todero Peixoto, C. ?. J., B., Tom?, G., Torralba Elipe, D., Torres Machado, Galicia, J. ?. F. Vald?s., I., Vali?o, Valore, Laura, G., van Aar, van den Berg, A. ?. M., S., van Velzen, A., van Vliet, B., Vargas C?rdena, V?zquez, J. ?. R., V?zquez, R. ?. A., D., Veberi?, L., Villase?or, O., Wainberg, Watson, A. ?. A., Whelan, B. ?. J., B., Wilczy?ska, H., Wilczy?ski, D., Zavrtanik, M., Zavrtanik, and M., Zimbres Silva
Subjects: Astrofísica, Physics - Instrumentation and Detectors, Physics::Instrumentation and Detectors, Astronomy, Ciencias Físicas, muons, hadronic interaction models, Astrophysics, 01 natural sciences, High Energy Physics - Experiment, Auger, purl.org/becyt/ford/1 [https], High Energy Physics - Experiment (hep-ex), Air showers, Production depth, SURFACE DETECTOR ARRAY, [PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex], [ PHYS.PHYS.PHYS-INS-DET ] Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], High Energy Astrophysical Phenomena (astro-ph.HE), Physics, High-Energy Cosmic Rays, [SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], Detector, Astrophysics::Instrumentation and Methods for Astrophysics, [ SDU.ASTR.IM ] Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM], Pierre Auger Observatory, Observable, Instrumentation and Detectors (physics.ins-det), COSMIC-RAYS, longitudinal development, Core (optical fiber), ComputingMethodologies_DOCUMENTANDTEXTPROCESSING, Física nuclear, Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - High Energy Astrophysical Phenomena, CIENCIAS NATURALES Y EXACTAS, [PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], Nuclear and High Energy Physics, [PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM], Astrophysics::High Energy Astrophysical Phenomena, FOS: Physical sciences, Cosmic ray, Nuclear physics, cosmic rays, [ PHYS.HEXP ] Physics [physics]/High Energy Physics - Experiment [hep-ex], 0103 physical sciences, extensive air showers, [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], 010306 general physics, Instrumentation and Methods for Astrophysics (astro-ph.IM), Zenith, Ciencias Exactas, Muon, 010308 nuclear & particles physics, [ PHYS.ASTR.HE ] Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], Física, purl.org/becyt/ford/1.3 [https], ASTROFÍSICA, [SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM], Astronomía, MODEL, Experimental High Energy Physics, High Energy Physics::Experiment, [ SDU.ASTR.HE ] Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], [ PHYS.ASTR.IM ] Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM], muonic component, SYSTEM
Abstract: The surface detector array of the Pierre Auger Observatory provides information about the longitudinal development of the muonic component of extensive air showers. Using the timing information from the flash analog-to-digital converter traces of surface detectors far from the shower core, it is possible to reconstruct a muon production depth distribution. We characterize the goodness of this reconstruction for zenith angles around 60° and different energies of the primary particle. From these distributions, we define Xμmax as the depth along the shower axis where the production of muons reaches maximum. We explore the potentiality of Xμmax as a useful observable to infer the mass composition of ultrahigh-energy cosmic rays. Likewise, we assess its ability to constrain hadronic interaction models., La lista completa de autores que integran el documento puede consultarse en el archivo., Facultad de Ciencias Exactas, Instituto de Física La Plata
Published: 2014
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32. The KASCADE-Grande energy spectrum of cosmic rays and the role of hadronic interaction models

Author: J. Wochele, Jörg R. Hörandel, Octavian Sima, B. Mitrica, Andreas Haungs, G. Toma, D. Huber, J.C. Arteaga-Velázquez, M. Petcu, A. Weindl, Kai Daumiller, G.C. Trinchero, H. J. Mathes, T. Huege, M. Wommer, K. Bekk, H. Rebel, D. Heck, A. Chiavassa, S. Ostapchenko, H.J. Gils, E. Cantoni, F.G. Schröder, M. Finger, Claus Grupen, J. Blümer, Markus Roth, M. Melissas, J. Engler, R. Glasstetter, I.M. Brancus, C. Morello, F. Cossavella, T. Pierog, P. Łuczak, N. Palmieri, Béatrice Fuchs, P. Doll, W. D. Apel, H. Ulrich, J. Oehlschläger, Ralph Engel, V. de Souza, M. E. Bertaina, J. Milke, K. Link, S. Schoo, J. Zabierowski, H. Schieler, Karl-Heinz Kampert, H.J. Mayer, H. Bozdog, M. Ludwig, F. Di Pierro, D. Fuhrmann, D. Kang, and H.O. Klages
Subjects: Physics, Atmospheric Science, FÍSICA DE PARTÍCULAS, Astronomy, Hadron, Monte Carlo method, Chemie, Aerospace Engineering, Astronomy and Astrophysics, Cosmic ray, Interaction model, Astrophysics, Mass composition, Nuclear physics, Geophysics, KASCADE, Space and Planetary Science, Energy spectrum, General Earth and Planetary Sciences
Abstract: Previous results obtained by KASCADE-Grande using the QGSjetII-02 hadronic interaction model have shown that the energy spectrum of cosmic rays between 10 16 eV and 10 18 eV exhibits a significant hardening at approximately 2 × 10 16 eV and a slight but statistically significant steepening close to 10 17 eV. Moreover, the analysis with QGSjetII-02 suggests that the break observed around 10 17 eV is caused by the heavy component of primary cosmic rays. In this paper, we report on the results of similar analyses performed using the SIBYLL 2.1 and EPOS 1.99 hadronic interaction models to interpret the data. The present results confirm qualitatively the previous findings. However, the intensity of the all-particle spectrum, the positions of the hardening and steepening of the spectrum, as well as the relative abundance of the heavy and light mass groups depend on the hadronic interaction model used to interpret the data.
Published: 2014

33. Reconstruction of the energy and depth of maximum of cosmic-ray air showers from LOPES radio measurements

Author: R. Engel, Béatrice Fuchs, J. Rautenberg, O. Krömer, A. Chiavassa, H. Rebel, C. Rühle, Markus Roth, M. Melissas, Katrin Link, M. Ludwig, Claus Grupen, F. Di Pierro, C. Morello, J. Oehlschläger, Octavian Sima, Peter L. Biermann, P. Łuczak, H. Schieler, Karl-Heinz Kampert, N. Palmieri, Heino Falcke, A. Horneffer, J. C. Arteaga-Velázquez, Paula Gina Isar, D. Kang, V. de Souza, A. Weindl, Jan Kuijpers, M. E. Bertaina, L. Bähren, K. Bekk, P. Doll, T. Pierog, H. J. Mathes, Jörg R. Hörandel, J. Wochele, Tim Huege, D. Heck, Gian Carlo Trinchero, Kai Daumiller, H. Gemmeke, A. Schmidt, I.M. Brancus, E. Cantoni, J. A. Zensus, G. Toma, D. Huber, Frank G. Schröder, J. Blümer, W. D. Apel, Alexandra Saftoiu, D. Fuhrmann, A. Haungs, H. Bozdog, and J. Zabierowski
Subjects: Physics, High Energy Astrophysical Phenomena (astro-ph.HE), Nuclear and High Energy Physics, FÍSICA DE PARTÍCULAS, LOPES, Astronomy, FOS: Physical sciences, Cosmic ray, Digital radio, Astrophysics, Coincidence, High Energy Physics - Experiment, Interferometry, High Energy Physics - Experiment (hep-ex), KASCADE, ComputingMethodologies_DOCUMENTANDTEXTPROCESSING, Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - High Energy Astrophysical Phenomena, Instrumentation and Methods for Astrophysics (astro-ph.IM), Energy (signal processing), Noise (radio)
Abstract: LOPES is a digital radio interferometer located at Karlsruhe Institute of Technology (KIT), Germany, which measures radio emission from extensive air showers at MHz frequencies in coincidence with KASCADE-Grande. In this article, we explore a method (slope method) which leverages the slope of the measured radio lateral distribution to reconstruct crucial attributes of primary cosmic rays. First, we present an investigation of the method on the basis of pure simulations. Second, we directly apply the slope method to LOPES measurements. Applying the slope method to simulations, we obtain uncertainties on the reconstruction of energy and depth of shower maximum Xmax of 13% and 50 g/cm^2, respectively. Applying it to LOPES measurements, we are able to reconstruct energy and Xmax of individual events with upper limits on the precision of 20-25% for the primary energy and 95 g/cm^2 for Xmax, despite strong human-made noise at the LOPES site., 16 pages, accepted by Physical Review D
Published: 2014

34. A Targeted Search for Point Sources of EeV Neutrons

Author: J. F. Valdés Galicia, K. H. Becker, I. De Mitri, A. Gascon Bravo, A. Saftoiu, Mariangela Settimo, D. Garcia-Gamez, S. T. Garcia Roca, H. J. Mathes, Alexey Yushkov, O. Fratu, V. Purrello, E. Petermann, D. Nitz, Q. Hasankiadeh, Miroslav Pech, M. Prouza, Luis Villaseñor, A. Śmiałkowski, J. Rodriguez Rojo, A. G. Chavez, M. Szuba, Piotr Homola, M. A. Leigui de Oliveira, F. Montanet, Christian Glaser, M. Zavrtanik, Enrique Zas, Adrian J. Matthews, P. Facal San Luis, C. Di Giulio, Fernando Contreras, P. Abreu, D. Ravignani, M. Josebachuili, J. Neuser, Pavel Horvath, R. Gaior, S. H. Cheng, M. S. Sutherland, S. Le Coz, Luis A. Anchordoqui, Markus Ahlers, Dusan Mandat, D. Garcia-Pinto, O. Krömer, H. Schoorlemmer, A. Dorofeev, D. Martraire, Guenter Sigl, Paula Gina Isar, F. Salesa Greus, Petr Schovanek, E. Varela, N. Griffith, S. J. Saffi, Raul Sarmento, P. Gouffon, M. Platino, G. Cataldi, M. Urban, A. C. Rovero, C. Bleve, L. Nellen, Sofia Andringa, K. B. Barber, M. Weber, Elton J. G. Santos, K. Link, B. Revenu, A. Nelles, F. Suarez, Sergio Dasso, M. Ludwig, John N. Matthews, R. M. Kieckhafer, J. Lozano Bahilo, C. Morello, R. Pesce, J. Rautenberg, A. C. Fauth, Jose Chinellato, N. Kunka, B. García, Tobias Winchen, M. Stephan, N. Scharf, V. Pirronello, U. Fröhlich, C. E. Santo, R. López, Karen S. Caballero-Mora, D. Melo, L. Martin, M. Oliveira, Marco Cilmo, Jaime Alvarez-Muñiz, G. P. Guedes, J. Stasielak, O. Wainberg, D. Huber, W. C. Brown, H. Blümer, P. Sanchez-Lucas, M. Tueros, P. Lautridou, Lu Lu, C. Jarne, David Walz, Corbin Covault, D. Harari, S. Coutu, Alessandro Petrolini, M. Lauscher, Vincenzo Rizi, D. Martello, T. Huege, M. Ziolkowski, A. Widom, Francisco J. Blanco, L. Perrone, H. Lyberis, D. LaHurd, Carla Bonifazi, D. Pakk Selmi-Dei, Jiri Chudoba, D. Torres Machado, F. Gomez Albarracin, A. Shadkam, C. Timmermans, R. Sato, Miroslav Hrabovský, M. Niechciol, Jose A. Bellido, O. Martínez Bravo, B. Mitrica, Markus Roth, A. Parra, Peter L. Biermann, Jeffrey Brack, Olaf Scholten, Humberto Ibarguen Salazar, A. Lopez Agüera, M. Buscemi, Bruno Daniel, Lino Miramonti, J. Allen, A. F. Grillo, Juan Carlos D'Olivo, T. Pierog, E. Mayotte, L. Ochilo, A. Letessier-Selvon, Martin Erdmann, I. Jandt, P. Brogueira, B. Sarkar, P. L. Ghia, A. Gorgi, B. Keilhauer, A. Haungs, Alina Mihaela Badescu, Paolo Privitera, I. Katkov, S. J. Sciutto, J. L. Harton, F. Guarino, Peter Buchholz, A. Tonachini, L. Nožka, C. Porowski, C. Baus, A. Aminaei, M. Blanco, Lorenzo Cazon, P. Heimann, I. A. Minaya, Xavier Bertou, Bruce R. Dawson, Y. N. Srivastava, J. R. Vázquez, A. Zepeda, T. Yapici, M. Videla, R. Cester, L. Molina-Bueno, J. J. Masías Meza, B. J. Whelan, Roger W Clay, D. Kruppke-Hansen, A. Di Matteo, Lukas Middendorf, P. Gonçalves, P.O. Mazur, J. Rosado, I.M. Brancus, Christine Peters, D. Maurizio, J. C. Moreno, C. Hojvat, Jan Ebr, Lorenzo Caccianiga, V. M. Theodoro, P. Pieroni, G. Navarra, M. Melissas, H. Glass, Marco Aglietta, I. C. Mariş, A. Porcelli, E. Kemp, L. Latronico, D. Monnier Ragaigne, M.D. Rodríguez-Frías, M. Risse, B. Wundheiler, A. van Vliet, P. Mantsch, Denise Boncioli, Gregory R Snow, Pedro Assis, O. A. Taborda, A. Etchegoyen, N. Palmieri, German Ros, A. Schmidt, H. Martinez, M. Ave, E. Trovato, P. Hansen, A. Chiavassa, C. A. Moura, C. Aramo, Pham Ngoc Diep, Brian Fick, N. Pacheco, R. Piegaia, M. Gómez Berisso, R. C. Shellard, B. D. Fox, E.M. Holt, Y. Guardincerri, A. E. Herve, A. Menshikov, B. Tome, G. Müller, L. R. Wiencke, H.O. Klages, Javier Tiffenberg, Heino Falcke, N. T. Thao, J. Vicha, T. A. Harrison, I. Al Samarai, Y. Petrov, Jörg R. Hörandel, G. Garilli, P. Allison, A. Tapia, H. Gemmeke, R. J. Lauer, P. Ristori, I. Lhenry-Yvon, M. Unger, S. van Velzen, Moritz Münchmeyer, Christopher B. Williams, G. C. Hill, F. Arqueros, P. Necesal, Octavian Sima, J. G. Gonzalez, Johannes Schulz, M. Pimenta, M. S. A. B. Leão, Peter Schiffer, G. Parente, D. Lebrun, M. Zimbres Silva, S. Jansen, R. Mussa, J. J. Beatty, V. Marin, B. Vlcek, H. Dembinski, A. Aab, L. Caramete, M. Will, V. Scherini, Balázs Kégl, G. Rodriguez Fernandez, A. D. Supanitsky, Hernán Asorey, Maria-Teresa Dova, Ralph Engel, R. Alves Batista, M. Plum, K. Weidenhaupt, Corinne Berat, Sarka Wykes, A. Criss, N. Fazzini, M. Giller, I. M. Pepe, H. Wahlberg, Z. Szadkowski, G. Varner, Jing Zhou, E. J. Ahn, O. Kambeitz, S. Messina, D. Nosek, T. Yamamoto, Kai Daumiller, P. Lebrun, J. Ridky, S. Navas, R. A. Vázquez, P. A. Kasper, C. J. Todero Peixoto, J. Stapleton, T. Hebbeker, Julien Aublin, B. Gookin, S. Quinn, A. Segreto, Edivaldo Moura Santos, A. Stutz, G. Toma, S. Mićanović, A. P. Ferguson, G. Yuan, J. Kleinfeller, F. Werner, D. Heck, M. Malacari, J. de Oliveira, A. Filipčič, R. Dallier, J. D. Swain, B. Wilczyńska, A. Curutiu, W. Docters, B. Caccianiga, Paul Sommers, L. Tomankova, R. Meyhandan, M. Ortiz, M. A. Muller, S. J. De Jong, I. Zaw, Alejandro Almela, B. Vargas Cárdenas, Maria Concetta Maccarone, M. Avenier, J. Pȩkala, Yunrong Zhu, N. Krohm, S. Riggi, K. Islo, Radomir Smida, J. Espadanal, M. Palatka, P. W. Younk, S. Mollerach, Philipp Papenbreer, J. Bäuml, J. S. Díaz, T. Suomijärvi, A. Insolia, M. Kleifges, D. Zavrtanik, J. Pallotta, Petr Travnicek, E. J. Quel, Ugo Giaccari, G. Marsella, P. N. Dong, M. J. Cooper, Miguel Mostafá, A. Weindl, E. Roulet, F. Sánchez, S. Petrera, Daniel Kuempel, A. Schulz, E. Menichetti, Florian Gaté, Carlos Escobar, H. Wilczyński, Trent D. Grubb, S. Maldera, G. Cocciolo, Béatrice Fuchs, Niraj Dhital, Peter Gorham, J. R. T. de Mello Neto, I. Valiño, P. Billoir, Ivone F. M. Albuquerque, Ke Fang, C. Rühle, Juan Manuel Figueira, Roberta Colalillo, V. de Souza, L. del Peral, F. Diogo, G. Matthiae, Antonio Bueno, Sergio Pastor, O. Ravel, A. G. Mariazzi, Alex Kääpä, Carlos Medina, M. Ambrosio, M. De Domenico, David Wittkowski, G. Salina, Olivier Deligny, Iván Sidelnik, A. Filevich, F. Salamida, N. Hollon, V. Verzi, B. Zamorano, Gualberto Avila, Ingomar Allekotte, L. Collica, R. Pelayo, T. Rossler, Martina Bohacova, S. Querchfeld, Azadeh Keivani, M. L. Díaz Castro, G. Farrar, T. Niggemann, R. M. de Almeida, Angela V. Olinto, M. Monasor, G. Torralba Elipe, R. Krause, L. Valore, L. Niemietz, W. Rodrigues de Carvalho, H. Schieler, R. Ulrich, M. Fernandes, M. Tartare, J. Sorokin, Karl-Heinz Kampert, Antonella Castellina, T. Fuji, J. W. Cronin, S. Grebe, Maria Rita Coluccia, J. Roberts, R. Squartini, T. Paul, Nataliia Borodai, G. Medina-Tanco, M. Candusso, G. van Aar, M. I. Micheletti, D. Maurel, J. Maller, Marco Giammarchi, Carola Dobrigkeit, V. Novotny, Rossella Caruso, A. Lucero, S. Stanič, Alan Watson, J. Alvarez Castillo, F. Sarazin, G. La Rosa, S. Mathys, M. Erfani, P.F. Gómez Vitale, Rúben Conceição, A.M. van den Berg, Darko Veberič, I. Rodriguez Cabo, R. Bonino, K. Louedec, Laboratoire SUBATECH Nantes (SUBATECH), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université de Nantes (UN)-Mines Nantes (Mines Nantes), Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Joseph Fourier - Grenoble 1 (UJF)-Centre National de la Recherche Scientifique (CNRS), Institut de Physique Nucléaire d'Orsay (IPNO), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), Laboratoire de l'Accélérateur Linéaire (LAL), PIERRE AUGER, Research unit Astroparticle Physics, A., Aab, P., Abreu, M., Aglietta, M., Ahler, E. J., Ahn, I., Al Samarai, I. F. M., Albuquerque, I., Allekotte, J., Allen, P., Allison, A., Almela, J., Alvarez Castillo, J., Alvarez Mu?iz, R., Alves Batista, M., Ambrosio, A., Aminaei, L., Anchordoqui, S., Andringa, Aramo, Carla, F., Arquero, H., Asorey, P., Assi, J., Aublin, M., Ave, M., Avenier, G., Avila, A. M., Badescu, K. B., Barber, J., B?uml, C., Bau, J. J., Beatty, K. H., Becker, J. A., Bellido, C., Berat, X., Bertou, P. L., Biermann, P., Billoir, F., Blanco, M., Blanco, C., Bleve, H., Bl?mer, M., Boh??ov?, D., Boncioli, C., Bonifazi, R., Bonino, N., Borodai, J., Brack, I., Brancu, P., Brogueira, W. C., Brown, P., Buchholz, A., Bueno, Buscemi, Mario, K. S., Caballero Mora, B., Caccianiga, L., Caccianiga, M., Candusso, L., Caramete, R., Caruso, A., Castellina, G., Cataldi, L., Cazon, R., Cester, A. G., Chavez, S. H., Cheng, A., Chiavassa, J. A., Chinellato, J., Chudoba, Cilmo, Marco, R. W., Clay, G., Cocciolo, Colalillo, Roberta, L., Collica, M. R., Coluccia, R., Concei??o, F., Contrera, M. J., Cooper, S., Coutu, C. E., Covault, A., Cri, J., Cronin, A., Curutiu, R., Dallier, B., Daniel, S., Dasso, K., Daumiller, B. R., Dawson, R. M., de Almeida, M., De Domenico, S. J., de Jong, J. R. T., de Mello Neto, I., De Mitri, J., de Oliveira, V., de Souza, L., del Peral, O., Deligny, H., Dembinski, N., Dhital, C., Di Giulio, A., Di Matteo, J. C., Diaz, M. L., D?az Castro, P. N., Diep, F., Diogo, C., Dobrigkeit, W., Docter, J. C., D'Olivo, P. N., Dong, A., Dorofeev, M. T., Dova, J., Ebr, R., Engel, M., Erdmann, M., Erfani, C. O., Escobar, J., Espadanal, A., Etchegoyen, P., Facal San Lui, H., Falcke, K., Fang, G., Farrar, A. C., Fauth, N., Fazzini, A. P., Ferguson, M., Fernande, B., Fick, J. M., Figueira, A., Filevich, A., Filip?i?, B. D., Fox, O., Fratu, U., Fr?hlich, B., Fuch, T., Fuji, R., Gaior, B., Garc?a, S. T., Garcia Roca, D., Garcia Gamez, D., Garcia Pinto, G., Garilli, A., Gascon Bravo, F., Gate, H., Gemmeke, P. L., Ghia, U., Giaccari, M., Giammarchi, M., Giller, C., Glaser, H., Gla, F., Gomez Albarracin, M., G?mez Berisso, P. F., G?mez Vitale, P., Gon?alve, J. G., Gonzalez, B., Gookin, A., Gorgi, P., Gorham, P., Gouffon, S., Grebe, N., Griffith, A. F., Grillo, T. D., Grubb, Y., Guardincerri, Guarino, Fausto, G. P., Guede, P., Hansen, D., Harari, T. A., Harrison, J. L., Harton, Q. D., Hasankiadeh, A., Haung, T., Hebbeker, D., Heck, P., Heimann, A. E., Herve, G. C., Hill, C., Hojvat, N., Hollon, E., Holt, P., Homola, J. R., H?randel, P., Horvath, M., Hrabovsk?, D., Huber, T., Huege, A., Insolia, P. G., Isar, K., Islo, I., Jandt, S., Jansen, C., Jarne, M., Josebachuili, A., K??p?, O., Kambeitz, K. H., Kampert, P., Kasper, I., Katkov, B., K?gl, B., Keilhauer, A., Keivani, E., Kemp, R. M., Kieckhafer, H. 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D., Rodríguez Fría, C., Rühle, F., Sánchez, Scherini, Viviana, P., Schovánek, A., Śmiałkowski, R., Šmída, S., Stanič, T., Suomijärvi, B., Tomé, J. F., Valdés Galicia, I., Valiño, L., Valore, B., Vargas Cárdena, J. R., Vázquez, R. A., Vázquez, D., Veberič, L., Villaseñor, B., Wilczyńska, and H., Wilczyński
Subjects: Astrofísica, [PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], Astronomy, Astrophysics::High Energy Astrophysical Phenomena, FOS: Physical sciences, Astrophysics, 01 natural sciences, Galaxy: disk, cosmic rays, Neutron flux, Observatory, 0103 physical sciences, data analysis [methods], Neutron, 010306 general physics, 010303 astronomy & astrophysics, High Energy Astrophysical Phenomena (astro-ph.HE), Pierre Auger Observatory, Physics, [SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], Galactic Center, cosmic ray, neutrons, Astrophysics::Instrumentation and Methods for Astrophysics, Física, Astronomy and Astrophysics, Galactic plane, methods: data analysis, Magnetic flux, Galaxy, Astronomía, Space and Planetary Science, Experimental High Energy Physics, ComputingMethodologies_DOCUMENTANDTEXTPROCESSING, ddc:520, Física nuclear, Astrophysics - High Energy Astrophysical Phenomena, disk [Galaxy]
Abstract: 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., La lista completa de autores puede verse en el archivo asociado., Facultad de Ciencias Exactas
Published: 2014
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35. Probing the radio emission from air showers with polarization measurements

Author: Marcus Niechciol, R. Mussa, J. J. Beatty, Alain Hervé, I. M. Pepe, R. Pelayo, H. Dembinski, B. Zamorano, L. del Peral, Johannes Schulz, Maurice Stephan, A. Parra, Jeffrey Brack, Olaf Scholten, O. Ravel, A. van Vliet, Azadeh Keivani, M. Pimenta, Humberto Ibarguen Salazar, P. Lebrun, Julien Aublin, S. Querchfeld, F. Werner, D. Kruppke-Hansen, L. Perrone, Jiri Chudoba, D. Torres Machado, E.M. Holt, Maria-Teresa Dova, A. Tonachini, L. Tomankova, W. J. M. de Mello Junior, G. Navarra, Eric Mayotte, M. Ave, J. Rodriguez Martino, Markus Ahlers, E. Varela, C. A. Moura, T. Yamamoto, Brian Fick, Samo Stanič, N. Griffith, Richard Dallier, Marcio Aparecido Muller, A. Nelles, R. Alves Batista, W. Rodrigues de Carvalho, P. O. Mazur, L. Niemietz, M. Tartare, M. Zimbres Silva, M. Gómez Berisso, R. C. Shellard, W. Docters, N. Pacheco, J. W. Cronin, P. Mantsch, Thomas Harrison, Kai Daumiller, Sarka Wykes, Jaime Alvarez-Muñiz, Jing Zhou, J. Stapleton, I. Zaw, F. Suarez, Thomas Hebbeker, Sergio Dasso, P.F. Gómez Vitale, V. Pirronello, C. Jarne, Tim Niggemann, N. Kunka, P. Pieroni, Lu Lu, J. Roberts, M. Risse, G. Toma, O. Taşcǎu, M. Buscemi, Yingchun Zhu, Octavian Fratu, Nataliia Borodai, F. Arqueros, N. Foerster, N. Scharf, J. PeÂķala, L. Nožka, P. Necesal, B. Vargas Cárdenas, S. Grebe, S. Messina, I. A. Minaya, B. Keilhauer, D. Nosek, Octavian Sima, J. G. Gonzalez, M. Will, E. Kemp, R. Squartini, J. Stasielak, S. Coutu, Jan Ebr, S. J. De Jong, M. Prouza, D. Lebrun, G. Parente, O. Kambeitz, C. Aramo, M. Avenier, T. Paul, M. Palatka, J. Maller, G. S. Varner, Pham Ngoc Diep, Jose Chinellato, D. B. Tridapalli, J. Allen, P. W. Younk, S. J. Sciutto, R. Pesce, K. Link, P. Abreu, D. Heck, T. Suomijärvi, J. Pallotta, E. J. Quel, D. Ravignani, G. Cocciolo, D. Monnier Ragaigne, G. Marsella, P. Lautridou, Rémi Bardenet, A. Curutiu, Petr Travnicek, A. Śmiałkowski, E. Menichetti, A. Weindl, P. Karhan, K. Louedec, Mariangela Settimo, B. Mitrica, Heino Falcke, Trent D. Grubb, D. Huber, J. Vicha, A. Widom, Alexey Yushkov, M. Candusso, Peter Gorham, Luis A. Anchordoqui, D. Martraire, H. Martinez, Kreso Kadija, P. Kasper, H.O. Klages, C. Rühle, Juan Manuel Figueira, Miroslav Hrabovský, G. Medina-Tanco, A. Haungs, J. R. T. de Mello Neto, G. Wieczorek, N. Hollon, V. Verzi, H. R. Marquez Falcon, Alejandro Almela, Roberta Colalillo, A. Schmidt, A. Dorofeev, A. G. Mariazzi, J. L. Harton, G. Matthiae, A. Letessier-Selvon, Béatrice Fuchs, Niraj Dhital, I. Valiño, G. van Aar, S. Jansen, A. P. Ferguson, Alberto Daniel Supanitsky, M. Platino, E. Santos, H. Blümer, Max Malacari, C. Hojvat, Denise Boncioli, B. Rouillé-D'Orfeuil, J. Lozano Bahilo, Segev BenZvi, Piotr Homola, P. Facal San Luis, Antonio Bueno, Sergio Pastor, M. Monasor, D. Nitz, L. Collica, Lorenzo Cazon, J. Knapp, A. Lopez Agüera, C. J. Todero Peixoto, Peter Schiffer, V. Scherini, Alexandra Saftoiu, Lukas Middendorf, Corbin Covault, Y. Petrov, Alberto Filevich, Peter Hansen, Markus Roth, German Ros, M. Videla, A. Aab, L. Caramete, Gualberto Avila, Ingomar Allekotte, Lino Miramonti, A. Chiavassa, A. C. Rovero, C. Bleve, Francisco J. Blanco, K. B. Barber, Z. Szadkowski, M. Oliveira, F. Guarino, John Matthews, Peter Buchholz, Darko Veberič, Igor Katkov, L. Villaseñor, M. Szuba, Dusan Mandat, J. A.J. Matthews, Xavier Bertou, I.M. Brancus, M. Josebachuili, A. Porcelli, N. Krohm, Martina Bohacova, Patrick Allison, B. Sarkar, S. Le Coz, Marco Aglietta, K. Weidenhaupt, M. D. Rodríguez-Frías, Balázs Kégl, Angela V. Olinto, C. Di Giulio, J. Sorokin, L. Martin, G. Rodriguez Fernandez, G. Salina, Danielle LaHurd, Olivier Deligny, Marco Cilmo, J. Gitto, Jörg R. Hörandel, Hernán Asorey, A. Zepeda, Pedro Assis, A. Etchegoyen, Javier Tiffenberg, G. Garilli, J. Neuser, M. S. A. B. Leão, P. T. Nhung, L. R. Wiencke, F. Gomez Albarracin, Vincenzo Rizi, D. Martello, M. Ziolkowski, Silvia Mollerach, O. Martínez Bravo, I. 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R., Marsella, Giovanni, Martello, Daniele, L., Martin, H., Martinez, O., Martínez Bravo, D., Martraire, Masías Meza, J. . J., Mathes, H. . J., J., Matthew, Matthews, J. . A. . J., G., Matthiae, D., Maurel, D., Maurizio, E., Mayotte, Mazur, P. . O., C., Medina, G., Medina Tanco, M., Melissa, D., Melo, E., Menichetti, A., Menshikov, S., Messina, R., Meyhandan, S., Mićanović, Micheletti, M. . I., L., Middendorf, Minaya, I. . A., L., Miramonti, B., Mitrica, L., Molina Bueno, S., Mollerach, M., Monasor, D., Monnier Ragaigne, F., Montanet, B., Morale, C., Morello, Moreno, J. . C., M., Mostafá, Moura, C. . A., Muller, M. . A., G., Müller, M., Münchmeyer, R., Mussa, G., Navarra, Navarro, J. . L., S., Nava, P., Necesal, L., Nellen, A., Nelle, J., Neuser, Nhung, P. . T., M., Niechciol, L., Niemietz, T., Niggemann, D., Nitz, D., Nosek, L., Nožka, J., Oehlschläger, A., Olinto, M., Oliveira, M., Ortiz, N., Pacheco, D., Pakk Selmi Dei, M., Palatka, J., Pallotta, N., Palmieri, G., Parente, A., Parra, S., Pastor, T., Paul, M., Pech, J., Pe¸kala, R., Pelayo, Pepe, I. . M., Perrone, Lorenzo, R., Pesce, E., Petermann, S., Petrera, A., Petrolini, Y., Petrov, R., Piegaia, T., Pierog, P., Pieroni, M., Pimenta, V., Pirronello, M., Platino, M., Plum, M., Pontz, A., Porcelli, T., Preda, P., Privitera, M., Prouza, Quel, E. . J., S., Querchfeld, S., Quinn, J., Rautenberg, O., Ravel, D., Ravignani, B., Revenu, J., Ridky, S., Riggi, M., Risse, P., Ristori, H., Rivera, V., Rizi, J., Robert, W., Rodrigues de Carvalho, I., Rodriguez Cabo, G., Rodriguez Fernandez, J., Rodriguez Martino, J., Rodriguez Rojo, Rodríguez Frías, M. . D., G., Ro, J., Rosado, T., Rossler, M., Roth, B., Rouillé d’Orfeuil, E., Roulet, Rovero, A. . C., C., Rühle, Saffi, S. . J., A., Saftoiu, F., Salamida, H., Salazar, F., Salesa Greu, G., Salina, F., Sánchez, P., Sanchez Luca, Santo, C. . E., E., Santo, Santos, E. . M., F., Sarazin, B., Sarkar, R., Sarmento, R., Sato, N., Scharf, Scherini, Viviana, H., Schieler, P., Schiffer, A., Schmidt, O., Scholten, H., Schoorlemmer, P., Schovánek, Schröder, F. . G., A., Schulz, J., Schulz, Sciutto, S. . J., M., Scuderi, A., Segreto, M., Settimo, A., Shadkam, Shellard, R. . C., I., Sidelnik, G., Sigl, O., Sima, A., Śmiałkowski, R., Šmída, Snow, G. . R., P., Sommer, J., Sorokin, H., Spinka, R., Squartini, Srivastava, Y. . N., S., Stanič, J., Stapleton, J., Stasielak, M., Stephan, M., Straub, A., Stutz, F., Suarez, T., Suomijärvi, Supanitsky, A. . D., T., Šuša, Sutherland, M. . S., J., Swain, Z., Szadkowski, M., Szuba, A., Tapia, M., Tartare, O., Taşcău, Thao, N. . T., J., Tiffenberg, C., Timmerman, W., Tkaczyk, Todero Peixoto, C. . J., G., Toma, L., Tomankova, B., Tomé, A., Tonachini, G., Torralba Elipe, D., Torres Machado, P., Travnicek, Tridapalli, D. . B., E., Trovato, M., Tuero, R., Ulrich, M., Unger, Valdés Galicia, J. . F., I., Valiño, L., Valore, G., van Aar, van den Berg, A. . M., S., van Velzen, A., van Vliet, E., Varela, B., Vargas Cárdena, G., Varner, Vázquez, J. . R., Vázquez, R. . A., D., Veberič, V., Verzi, J., Vicha, M., Videla, L., Villaseñor, H., Wahlberg, P., Wahrlich, O., Wainberg, D., Walz, Watson, A. . A., M., Weber, K., Weidenhaupt, A., Weindl, F., Werner, S., Westerhoff, Whelan, B. . J., A., Widom, G., Wieczorek, L., Wiencke, B., Wilczyńska, H., Wilczyński, M., Will, C., William, T., Winchen, B., Wundheiler, S., Wyke, T., Yamamoto, T., Yapici, P., Younk, G., Yuan, A., Yushkov, B., Zamorano, E., Za, D., Zavrtanik, M., Zavrtanik, I., Zaw, A., Zepeda, J., Zhou, Y., Zhu, M., Zimbres Silva, M., Ziolkowski, Research unit Astroparticle Physics, Universidade Estadual de Campinas, Ahn, E. ?. J., Albuquerque, I. ?. F. ?. M., J., Alvarez Mu?iz, T., Anti?i?, Badescu, A. ?. M., Barber, K. ?. B., J., B?uml, Beatty, J. ?. J., Becker, K. ?. H., Bellido, J. ?. A., Biermann, P. ?. L., C., Bleve, H., Bl?mer, M., Boh??ov?, Brown, W. ?. C., Buscemi, Mario, Caballero Mora, K. ?. S., Cheng, S. ?. H., Chinellato, J. ?. A., Cilmo, Marco, Clay, R. ?. W., G., Cocciolo, Colalillo, Roberta, Coluccia, M. ?. R., R., Concei??o, Cooper, M. ?. J., Covault, C. ?. E., Dawson, B. ?. R., de Almeida, R. ?. M., de Jong, S. ?. J., de Mello Junior, W. ?. J. ?. M., de Mello Neto, J. ?. R. ?. T., I., De Mitri, de Vries, K. ?. D., Diaz, J. ?. C., D?az Castro, M. ?. L., Diep, P. ?. N., D?olivo, J. ?. C., Dong, P. ?. N., dos Anjos, J. ?. C., Dova, M. ?. T., Escobar, C. ?. O., Fauth, A. ?. C., Ferguson, A. ?. P., Figueira, J. ?. M., A., Filip?i?, Fox, B. ?. D., Fracchiolla, C. ?. E., Fraenkel, E. ?. D., U., Fr?hlich, Gamarra, R. ?. F., B., Garc?a, Garcia Roca, S. ?. T., Ghia, P. ?. L., M., G?mez Berisso, G?mez Vitale, P. ?. F., P., Gon?alve, Gonzalez, J. ?. G., Grillo, A. ?. F., Grubb, T. ?. D., Guarino, Fausto, Guedes, G. ?. P., Harrison, T. ?. A., Harton, J. ?. L., Herve, A. ?. E., Hill, G. ?. C., H?randel, J. ?. R., M., Hrabovsk?, Isar, P. ?. G., Kampert, K. ?. H., B., K?gl, Kieckhafer, R. ?. M., Klages, H. ?. O., O., Kr?mer, Le?o, M. ?. S. ?. A. ?. B., Leigui de Oliveira, M. ?. A., R., L?pez, A., Lopez Ag?era, Maccarone, M. ?. C., Mariazzi, A. ?. G., Mari?, I. ?. C., Marquez Falcon, H. ?. R., G., Marsella, D., Martello, O., Mart?nez Bravo, Mas?as Meza, J. ?. J., Mathes, H. ?. J., Matthews, J. ?. A. ?. J., Mazur, P. ?. O., S., Mi?anovi?, Micheletti, M. ?. I., Minaya, I. ?. A., Moreno, J. ?. C., M., Mostaf?, Moura, C. ?. A., Muller, M. ?. A., G., M?ller, M., M?nchmeyer, Navarro, J. ?. L., Nhung, P. ?. T., L., No?ka, J., Oehlschl?ger, J., Pe?kala, Pepe, I. ?. M., L., Perrone, Quel, E. ?. J., Rodr?guez Fr?as, M. ?. D., B., Rouill? d?Orfeuil, Rovero, A. ?. 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J., B., Wilczy?ska, H., Wilczy?ski, Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Joseph Fourier - Grenoble 1 (UJF)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de Physique Nucléaire et de Hautes Énergies (LPNHE), Centre National de la Recherche Scientifique (CNRS)-Université Paris Diderot - Paris 7 (UPD7)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Pierre et Marie Curie - Paris 6 (UPMC), Unité Scientifique de la Station de Nançay (USN), Centre National de la Recherche Scientifique (CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire des Sciences de l'Univers en région Centre (OSUC), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS)-Université d'Orléans (UO), Laboratoire SUBATECH Nantes (SUBATECH), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université de Nantes (UN)-Mines Nantes (Mines Nantes), Laboratoire de l'Accélérateur Linéaire (LAL), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), Institut de Physique Nucléaire d'Orsay (IPNO), PIERRE AUGER, Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Centre National de la Recherche Scientifique (CNRS), Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Observatoire des Sciences de l'Univers en région Centre (OSUC), Université Paris sciences et lettres (PSL)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS), Mines Nantes (Mines Nantes)-Université de Nantes (UN)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), and Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)
Subjects: Signals, Astronomy, 01 natural sciences, Electric field, Computational physics, Cosmic-rays, Composition energy spectra and interactions, cosmic ray, Radio wave, Physics, Earth's magnetic field, High Energy Astrophysical Phenomena (astro-ph.HE), Radiation, [SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph], [SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], Astrophysics::Instrumentation and Methods for Astrophysics, Polarization (waves), Bolometers, Thunderstorms, Magnetic field, ComputingMethodologies_DOCUMENTANDTEXTPROCESSING, Física nuclear, Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - High Energy Astrophysical Phenomena, CAMPO MAGNÉTICO, radio emission, Nuclear and High Energy Physics, [PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], [PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM], Air shower, Solar electromagnetic emission, Astrophysics::High Energy Astrophysical Phenomena, infrared submillimeter wave microwave and radiowave receivers and detectors, Field, FOS: Physical sciences, Pierre Auger Observatory, air shower, Monte-carlo Simulations, Optics, 0103 physical sciences, ddc:530, Pierre auger observatory, 010306 general physics, Pulses, Instrumentation and Methods for Astrophysics (astro-ph.IM), 010308 nuclear & particles physics, business.industry, Física, Detector, [SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM], Experimental High Energy Physics, business, Codalema
Abstract: The emission of radio waves from air showers has been attributed to the so-called geomagnetic emission process. At frequencies around 50 MHz this process leads to coherent radiation which can be observed with rather simple setups. The direction of the electric field induced by this emission process depends only on the local magnetic field vector and on the incoming direction of the air shower. We report on measurements of the electric field vector where, in addition to this geomagnetic component, another component has been observed which cannot be described by the geomagnetic emission process. The data provide strong evidence that the other electric field component is polarized radially with respect to the shower axis, in agreement with predictions made by Askaryan who described radio emission from particle showers due to a negative charge-excess in the front of the shower. Our results are compared to calculations which include the radiation mechanism induced by this charge-excess process., Comment: Accepted for publication in Phys. Rev. D; 50 pages, 15 figures
Published: 2014
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36. The wavefront of the radio signal emitted by cosmic ray air showers

Author: A. Chiavassa, E. Cantoni, T. Pierog, Tim Huege, A. Horneffer, D. Kang, Paula Gina Isar, Katrin Link, W. D. Apel, M. Melissas, P. Doll, J. Rautenberg, J. Oehlschläger, Alexandra Saftoiu, J. Wochele, Heino Falcke, Octavian Sima, M. E. Bertaina, D. Heck, M. Ludwig, A. Weindl, Ralph Engel, Jan Kuijpers, F. Di Pierro, J. Zabierowski, P. Łuczak, N. Palmieri, Andreas Haungs, D. Huber, A. Schmidt, C. Rühle, H. J. Mathes, K. Bekk, H. Rebel, H. Bozdog, J. A. Zensus, Markus Roth, F.G. Schröder, S. Schoo, J. Blümer, L. Bähren, O. Krömer, I.M. Brancus, H. Schieler, Karl-Heinz Kampert, Béatrice Fuchs, H. Gemmeke, G. Toma, Claus Grupen, C. Morello, Peter L. Biermann, V. de Souza, Jörg R. Hörandel, J.C. Arteaga-Velázquez, Kai Daumiller, and G.C. Trinchero
Subjects: Astrophysics::High Energy Astrophysical Phenomena, Astronomy, FOS: Physical sciences, Cosmic ray, High Energy Physics - Experiment, Antenna array, High Energy Physics - Experiment (hep-ex), Optics, ddc:530, Ligand cone angle, Instrumentation and Methods for Astrophysics (astro-ph.IM), Zenith, Cherenkov radiation, High Energy Astrophysical Phenomena (astro-ph.HE), Physics, Wavefront, LOPES, business.industry, Astrophysics::Instrumentation and Methods for Astrophysics, Astronomy and Astrophysics, ASTROFÍSICA, KASCADE, ComputingMethodologies_DOCUMENTANDTEXTPROCESSING, Astrophysics - High Energy Astrophysical Phenomena, Astrophysics - Instrumentation and Methods for Astrophysics, business
Abstract: Analyzing measurements of the LOPES antenna array together with corresponding CoREAS simulations for more than 300 measured events with energy above $10^{17}\,$eV and zenith angles smaller than $45^\circ$, we find that the radio wavefront of cosmic-ray air showers is of approximately hyperbolic shape. The simulations predict a slightly steeper wavefront towards East than towards West, but this asymmetry is negligible against the measurement uncertainties of LOPES. At axis distances $\gtrsim 50\,$m, the wavefront can be approximated by a simple cone. According to the simulations, the cone angle is clearly correlated with the shower maximum. Thus, we confirm earlier predictions that arrival time measurements can be used to study the longitudinal shower development, but now using a realistic wavefront. Moreover, we show that the hyperbolic wavefront is compatible with our measurement, and we present several experimental indications that the cone angle is indeed sensitive to the shower development. Consequently, the wavefront can be used to statistically study the primary composition of ultra-high energy cosmic rays. At LOPES, the experimentally achieved precision for the shower maximum is limited by measurement uncertainties to approximately $140\,$g/cm$^2$. But the simulations indicate that under better conditions this method might yield an accuracy for the atmospheric depth of the shower maximum, $X_\mathrm{max}$, better than $30\,$g/cm$^2$. This would be competitive with the established air-fluorescence and air-Cherenkov techniques, where the radio technique offers the advantage of a significantly higher duty-cycle. Finally, the hyperbolic wavefront can be used to reconstruct the shower geometry more accurately, which potentially allows a better reconstruction of all other shower parameters, too., Comment: accepted by JCAP
Published: 2014
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37. Erratum to 'Atmospheric effects on extensive air showers observed with the surface detector of the Pierre Auger observatory'[Astroparticle Physics 32(2) (2009), 89-99]

Author: P. Lebrun, R. López, Karen S. Caballero-Mora, L. Valore, M. Gold, Martin Erdmann, I. Zaw, V. C. Holmes, D. Lebrun, C. Macolino, J. Oehlschläger, I. Dutan, Roger W Clay, W. J. M. de Mello, Markus Risse, U. Cotti, D. Heck, Carola Dobrigkeit, R. F. Gamarra, I. Valiño, P. Wahrlich, T. Suomijärvi, J. Pallotta, E. J. Quel, I. Torres, Alan Watson, L. Cazon, S. Navas, M. Melissas, M. Hrabovsky, C. Hojvat, R. A. Vázquez, O. Taşcaǧu, F. Sánchez, K. Louedec, Paulo J. S. Gonçalves, V. Rizzi, Mariangela Settimo, K. H. Kampert, J. PeĶala, E. Trovato, Wagner Carvalho, Iván Sidelnik, M.E. Ortiz, A. Filipčič, A. Rouillé-d'Orfeuil, H.O. Klages, A. Redondo, D.V. Semikoz, H. Blümer, Charles Timmermans, C. Riviere, F. Sarazin, Kai Daumiller, M. S. A. B. Leão, M. Urban, S. Petrera, G. Parente, E. M. Santos, Piotr Homola, P. Facal San Luis, M. Grigat, Ralf Ulrich, R. M. de Almeida, J. Pochon, Richard Dallier, A. C. Rovero, Luis A. Anchordoqui, Bruce R. Dawson, M. D. Healy, P. T. Nhung, H. R. Marquez Falcon, Jaime Alvarez-Muñiz, D. Schuster, K. Payet, P.O. Mazur, Darko Veberič, C. Bleve, F. Arneodo, S. Gambetta, J. Kleinfeller, Petr Travnicek, R. Ticona, Martina Bohacova, Patrick Allison, J. G. Gonzalez, C. Morris, V. Pirrpnello, A. Schmidt, R. Bonino, D. Allard, Rodrigo Pelayo, S. Westerhoff, L. Nellen, Miguel Mostafá, C. Morello, K. D. de Vries, Vasiliki Pavlidou, H. M. Spinka, R. Piegaia, O. Krömer, J. Sorokin, van den Ad M Berg, A. C. Fauth, R. M. Kieckhafer, Juan Moreno, Daniel Kuempel, Carlos Escobar, A. Creusot, S. Maldera, B. Revenu, J. R. Vázquez, A. Italiano, D. Melo, T. Huege, Jeffrey Brack, J. Rautenberg, O. Wainberg, Maria-Teresa Dova, T. Schmidt, S. Grebe, Olaf Scholten, W. Fulgione, H. Lyberis, Jose A. Bellido, Stefano Argiro, Humberto Ibarguen Salazar, B. Keilhauer, Catherine Newman-Holmes, D. B. Tridapalli, P. Bernardini, J. Allen, D. Harari, M. Zavrtanik, H. Schieler, Matthias Leuthold, Fabrizio Ortolani, W. C. Brown, Peter L. Biermann, E. Petermann, D. D'Urso, N. T. Thao, Gennaro Miele, Jaime Rosado, K.-H. Becker, D. Warner, Corinne Berat, M. Giller, S. J. Sciutto, D. García Gámez, R. Pesce, Miroslav Pech, J. Schovancova, Antonella Castellina, Paul Sommers, Lisa M. Goggin, R. Bruijn, Graciela B. Gelmini, J. Lozano Bahilo, Segev BenZvi, N. Nierstenhoefer, M. Monasor, A. Horneffer, M. Pimenta, A. G. Mariazzi, C. Robledo, A. Haungs, John G. Lee, J. L. Harton, E. Parizot, R. Squartini, C. E. Santo, Corbin Covault, T. Paul, Y. Petrov, D. Martello, C. De Donato, R. Luna García, P. Gouffon, P. N. Dong, R. Cester, W. Tkaczyk, J. D. Hague, Jörg R. Hörandel, B. Morales, Paolo Privitera, K. Arisaka, S. Fliescher, Lino Miramonti, M. S. Sutherland, P. Petrinca, M. Ziolkowski, D. Nitz, P. Mantsch, F. A. S. Rezende, C. Lachaud, U. Giaccari, C. Bonifazi, O. Martínez Bravo, H. Wu, M. D. Rodríguez-Frías, J. Gutiérrez, M. De Domenico, José Eduardo Martinez, J. A.J. Matthews, Xavier Bertou, G. Navarra, Olivier Ravel, E. Menichetti, R. Knapik, F. Schüssler, D. Pakk Selmi-Dei, I. Lhenry-Yvon, Hernan Wahlberg, Francesc Ferrer, A. Chiavassa, Sofia Andringa, K. B. Barber, A. Smialkowski, C. A. Moura, S. L.C. Barroso, T. Yamamoto, Antonio Velarde, A. Zepeda, Rossella Caruso, Pietro Oliva, A. Lucero, Pedro Assis, A. Etchegoyen, G. Medina-Tanco, Warner A. Miller, Onofrio A. Catalano, G. La Rosa, L. R. Wiencke, Petr Schovanek, R. Meyhandan, J. Knapp, X. Garrido, M. Ambrosio, A. Criss, A. Lopez Agüera, M. Pontz, R. Sato, B. Connolly, B. M. Baughman, Eun-Joo Ahn, N. Scharf, V. Tuci, Javier Tiffenberg, Alberto Filevich, Peter Hansen, E. D. Fraenkel, F. Guarino, John Matthews, V. M. Olmos-Gilbaja, N. Pacheco, A. Petrolini, Peter Buchholz, Dusan Mandat, H. Glass, Nicolás G. Busca, M. I. Micheletti, B. Wilczyn' Ska, Marco Aglietta, Tonia M. Venters, A. Chou, A. D. Supanitsky, D. Dornic, Hernán Asorey, A. Tamburro, I. Allekotte, F. Suarez, Thomas Hebbeker, M. Kaducak, F. Ionita, D. Tcherniakhovski, H. Schoorlemmer, T. Bäcker, A. Bellétoile, G. Decerprit, Pedro Brogueira, M. Palatka, C. J. Todero Peixoto, Rúben Conceição, Pascal Lautridou, Iuri Muniz Pepe, E. Kemp, Serguei Vorobiov, D. Kruppke-Hansen, P. W. Younk, B. E. Smith, Beatriz B. Siffert, P. Schiffer, S. Parlati, S. Schulte, T. Pinto, J. L. Navarro, B. Wundheiler, Gregory R Snow, Marcio Aparecido Muller, P. H. Kasper, D. Newton, V. H. Ponce, L. Perrone, Jiri Chudoba, E. Colombo, A. Tamashiro, G. P. Guedes, Daniel Gonzalez, D. Monnier Ragaigne, S. Harmsma, E. Strazzeri, J. C. Diaz, G. Golup, Ivor Fleck, S. Dagoret-Campagne, L. del Peral, H. Gemmeke, N. Kunka, C. Pfendner, A. Cordier, M. Unger, J. F. Valdés Galicia, I. De Mitri, J. Rodriguez Martino, G. Yuan, S. Riggi, J. Chye, G. Matthiae, Matias Tueros, J. Abraham, E. Grashorn, J. W. Cronin, Antonio Bueno, Sergio Pastor, Daniel Omar Badagnani, Nataliia Borodai, H. Wilczyn' Ski, F. Salamida, M. A. Leigui de Oliveira, R. Tcaciuc, F. Schroeder, S. J. De Jong, Y. Guardincerri, Gualberto Avila, P. Bauleo, Pierre Billoir, D. Thomas, A. Curutiu, B. Tome, A. F. Grillo, Juan Carlos D'Olivo, T. Pierog, S. Coutu, M. Nyklicek, Esteban Roulet, J. R. T. de Mello Neto, Angela V. Olinto, V. Halenka, M. Hussain, T. Karova, B. Kégl, Fabian Schmidt, F. Montanet, J. C. dos Anjos, P. L. Ghia, Michael DuVernois, M. McEwen, M. C. Maccarone, L. Voyvodic, Subir Sarkar, Alexander Kusenko, German Ros, F. Arqueros, C. Wileman, P. Necesal, D. Garcia-Pinto, R. Mussa, J. J. Beatty, Silvia Mollerach, J. Coppens, J. Chauvin, N. Fazzini, A. Segreto, Julien Aublin, Markus Roth, M. Patel, Radomir Smida, C. Delle Fratte, A. Ferrero, A. Anzalone, V. de Souza, T. Tarutina, M. Gómez Berisso, R. C. Shellard, I. Rodriguez-Cabo, Jose Chinellato, A. F. Barbosa, M. Ave, D. Nosek, R. E. Burton, A. Letessier-Selvon, H. J. Mathes, V. Verzi, H. Dembinski, G. De La Vega, Ofelia Pisanti, B. J. Whelan, D. Maurizio, J. Rodriguez Rojo, C. Aramo, Enrique Zas, Pham Ngoc Diep, O. Blanch-Bigas, A. Krieger, A. Dorofeev, C. Di Giulio, Heino Falcke, Fernando Contreras, G. Wieczorek, Marco Iarlori, J. Petrovic, S. Reucroft, M. Prouza, S. Mueller, P. Abreu, A. Della Selva, M. Videla, D. Ravignani, Ernesto Arganda, C. E. Fracchiolla, G. Farrar, L. Villaseñor, R. R. McNeil, Dariusz Gora, G. Salina, Olivier Deligny, T. Rossler, A. Lemiere, B. Fick, A. Tonachini, T. Asch, M. Gonçalves do Amaral, J. D. Swain, G. Rodriguez, M. G. Winnick, M. Platino, Marcos Santander, A. Insolia, M. Kleifges, D. Zavrtanik, L. Nožka, L. Caramete, G. Tristram, B. L. Lago, C. Aguirre, Francisco J. Blanco, F. Gomez Albarracin, V. Scherini, G. Hebrero, A. Gorgi, Z. Szadowski, S. Jiraskova, Ioana Codrina Maris, A. Menshikov, B. R. Becker, Ralph Engel, D. H. Koang, J. Ridky, Tristan Beau, A. Stutz, B. García, Mario Scuderi, APC - Astrophysique des Hautes Energies (APC - AHE), AstroParticule et Cosmologie (APC (UMR_7164)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Alma Mater Studiorum Università di Bologna [Bologna] (UNIBO), Laboratoire de Physique Nucléaire et de Hautes Énergies (LPNHE), Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Centre National de la Recherche Scientifique (CNRS), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de l'Accélérateur Linéaire (LAL), Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Laboratoire SUBATECH Nantes (SUBATECH), Mines Nantes (Mines Nantes)-Université de Nantes (UN)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Institut de Physique Nucléaire d'Orsay (IPNO), APC - THEORIE, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut für theoretische Physik, Universität Hamburg (UHH)-Universität Hamburg (UHH), PIERRE AUGER, Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Dipartimento di Astronomia, Universita degli Studi di Bologna, Alma Mater Studiorum Università di Bologna [Bologna] (UNIBO)-Alma Mater Studiorum Università di Bologna [Bologna] (UNIBO), Centre National de la Recherche Scientifique (CNRS)-Université Paris Diderot - Paris 7 (UPD7)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Pierre et Marie Curie - Paris 6 (UPMC), Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Joseph Fourier - Grenoble 1 (UJF)-Centre National de la Recherche Scientifique (CNRS), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université de Nantes (UN)-Mines Nantes (Mines Nantes), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Institut für theoretische Physik, Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Dipartimento di Astronomia, Universita degli Studi di Bologna, Università di Bologna [Bologna] (UNIBO)-Università di Bologna [Bologna] (UNIBO), Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA), PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Institut für theoretische Physik, D'Urso, Domenico, Guarino, Fausto, Valore, Laura, and The Pierre Auger, Collaboration
Subjects: Astroparticle physics, Physics, Pierre Auger Observatory, [PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM], 010308 nuclear & particles physics, Astronomy, Detector, Astronomy and Astrophysics, Astrophysics, 01 natural sciences, Auger, [SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM], Experimental High Energy Physics, 0103 physical sciences, 010303 astronomy & astrophysics, ComputingMilieux_MISCELLANEOUS
Abstract: The Pierre Auger Collaboration... K.B. Barber... J.A. Bellido... R.W. Clay... B.R. Dawson... V.C. Holmes... J. Sorokin... P. Wahrlich... B.J. Whelan... M.G. Winnick... et al.
Published: 2010
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38. The data acquisition system for the ANTARES neutrino telescope

Author: D. Zaborov, G.D. Hallewell, M. Morganti, Anne Deschamps, S. Galeotti, P. Chauchot, K. Salomon, V. Rigaud, C. Racca, Philippe Charvis, B. van Rens, J. Hogenbirk, S. L. Cartwright, M. Billault, C. Hoffman, H. Le Provost, P. Coyle, J.-C. Languillat, R. Bruijn, Chantal Compère, V. Flaminio, J.R. Hubbard, J. van Randwijk, L Lo Nigro, M. Romita, Paolo Sapienza, V. Roca, A. Calzas, V. Popa, M. Jaspers, C. Donzaud, V. Niess, S. Anvar, Yvonne Becherini, D. Lo Presti, Roberto Bellotti, J. Zúñiga, J. F. Drogou, M. Anghinolfi, P. Rewiersma, Robert Lahmann, C. Petta, P.K.A. de Witt Huberts, S. Basa, L. Caillat, U. F. Katz, D. Lachartre, H. Peek, T. Legou, Nathalie Palanque-Delabrouille, F. Lucarelli, Yann Hello, J. Carr, J. Busto, M. Ripani, Jean-Francois Rolin, E. Carmona, N. Cottini, A. Capone, S. Loucatos, Stephanie Escoffier, J-J. Aubert, Giorgio Riccobene, G. van der Steenhoven, F. Mazéas, G. F. Burgio, I. Sokalski, J. P. Schuller, M. Jaquet, M. Mongelli, E. Migneco, L. Moscoso, Eric Delagnes, F. Réthoré, J. P. Pineau, G. Venekamp, P. Kooijman, P. Goret, V. Lyashuk, J.D. Zornoza, M. Battaglieri, R. Ostasch, Emanuele Castorina, E. A. De Wolf, L. Caponetto, J. P. Ernenwein, Rosario Megna, Charling Tao, F. Louis, Juanan Aguilar, Timo Karg, G. Damy, V. A. Kudryavstev, F. Schmitt, T. Pradier, Diego Real, G. Lamanna, C. De Marzo, M. de Jong, V. Valente, T. Spona, I. Dekeyser, Tommaso Chiarusi, M. Naumann-Godo, A.-S. Cussatlegras, E. Falchini, A. Le Van Suu, R. De Vita, B. Dinkespieler, J. Hößl, F. Druillole, H. Lafoux, P. Piattelli, N. de Botton, F. Ameli, P. Payre, A.-F. Yao, J. Roux, C. Kopper, J.-J. Destelle, A. Milovanovic, M. Melissas, Chiara Roda, F. Feinstein, Mohsen Harakeh, Kay Graf, Lester D.R. Thompson, B. Vallage, P. Valdy, S. Cecchini, M.C. Bouwhuis, A. Heijboer, M. Circella, T. Montaruli, H. Zaccone, G. Wobbe, D. Denans, N. Girard, J. Beltramelli, Vincenzo Cavasinni, C. Distefano, H. Kok, R. van Wijk, Juan José Hernández-Rey, Maurizio Spurio, P. Keller, J. M. Gallone, R. Coniglione, G. de Vries, F. Dessages-Ardellier, H. Laschinsky, M. Ruppi, C. Olivetto, B. Hartmann, C. Gojak, M. Taiuti, M. Marcelin, Annarita Margiotta, R. van Dantzig, F. Jouvenot, A. Albert, K. Streeb, J. E. McMillan, H. J. Rose, S. M. Bradbury, Gisela Anton, T. Stolarczyk, J. Poinsignon, Nasser Kalantar-Nayestanaki, G. Terreni, V. Bertin, P. Lagier, G. Lim, F. Cafagna, R. Masullo, S. Favard, Elie Aslanides, Christian Tamburini, B. Verlaat, D. Festy, Alexander Kappes, Rezo Shanidze, S. Kuch, C. Naumann, F. Salesa, C. Colnard, Mario Musumeci, N. Randazzo, A. Kruijer, A. Rostovtsev, C. Fiorello, P. Vernin, E. V. Korolkova, A. Ceres, H. Loehner, Jürgen Brunner, E. Barbarito, S. Ferry, Y. Le Guen, D. Castel, G.V. Russo, G. Giacomelli, S. Karkar, W. Kretschmer, Antoine Kouchner, R. Blaes, Dominique Durand, S. Cuneo, Lawrence Sulak, E. Heine, P. Lamare, A. Mazure, A. Bigi, D. Stubert, KVI - Center for Advanced Radiation Technology, J.A. AGUILAR, A. ALBERT, F. AMELI, M. ANGHINOLFI, G. ANTON, S. ANVAR, E. ASLANIDES, J.-J. AUBERT, E. BARBARITO, S. BASA, M. BATTAGLIERI, Y. BECHERINI, R. BELLOTTI, J. BELTRAMELLI, V. BERTIN, A. BIGI, M. BILLAULT, R. BLAES, N. DE BOTTON, M.C. BOUWHUIS, S.M. BRADBURY, R. BRUIJN, J. BRUNNER, G.F. BURGIO, J. BUSTO, F. CAFAGNA, L. CAILLAT, A. CALZAS, A. CAPONE, L. CAPONETTO, E. CARMONA, J. CARR, S.L. CARTWRIGHT, D. CASTEL, E. CASTORINA, V. CAVASINNI, S. CECCHINI, A. CERES, P. CHARVIS, P. CHAUCHOT, T. CHIARUSI, M. CIRCELLA, C. COLNARD, C. COMPÈRE, R. CONIGLIONE, N. COTTINI, P. COYLE, S. CUNEO, A.-S. CUSSATLEGRAS, G. DAMY, R. VAN DANTZIG, C. DE MARZO, I. DEKEYSER, E. DELAGNES, D. DENANS, A. DESCHAMPS, F. DESSAGES-ARDELLIER, J.-J. DESTELLE, B. DINKESPIELER, C. DISTEFANO, C. DONZAUD, J.-F. DROGOU, F. DRUILLOLE, D. DURAND, J.-P. ERNENWEIN, S. ESCOFFIER, E. FALCHINI, S. FAVARD, F. FEINSTEIN, S. FERRY, D. FESTY, C. FIORELLO, V. FLAMINIO, S. GALEOTTI, J.-M. GALLONE, G. GIACOMELLI, N. GIRARD, C. GOJAK, PH. GORET, K. GRAF, G. HALLEWELL, M.N. HARAKEH, B. HARTMANN, A. HEIJBOER, E. HEINE, Y. HELLO, J.J. HERNÁNDEZ-REY, J. HÖßL, C. HOFFMAN, J. HOGENBIRK, J.R. HUBBARD, M. JAQUET, M. JASPERS, M. DE JONG, F. JOUVENOT, N. KALANTAR-NAYESTANAKI, A. KAPPES, T. KARG, S. KARKAR, U. KATZ, P. KELLER, H. KOK, P. KOOIJMAN, C. KOPPER, E.V. KOROLKOVA, A. KOUCHNER, W. KRETSCHMER, A. KRUIJER, S. KUCH, V.A. KUDRYAVSTEV, D. LACHARTRE, H. LAFOUX, P. LAGIER, R. LAHMANN, G. LAMANNA, P. LAMARE, J.C. LANGUILLAT, H. LASCHINSKY, Y. LE GUEN, H. LE PROVOST, A. LE VAN SUU, T. LEGOU, G. LIM, L. LO NIGRO, D. LO PRESTI, H. LOEHNER, S. LOUCATOS, F. LOUIS, F. LUCARELLI, V. LYASHUK, M. MARCELIN, A. MARGIOTTA, R. MASULLO, F. MAZÉAS, A. MAZURE, J.E. MCMILLAN, R. MEGNA, M. MELISSAS, E. MIGNECO, A. MILOVANOVIC, M. MONGELLI, T. MONTARULI, M. MORGANTI, L. MOSCOSO, M. MUSUMECI, C. NAUMANN, M. NAUMANN-GODO, V. NIESS, C. OLIVETTO, R. OSTASCH, N. PALANQUE-DELABROUILLE, P. PAYRE, H. PEEK, C. PETTA, P. PIATTELLI, J.-P. PINEAU, J. POINSIGNON, V. POPA, T. PRADIER, C. RACCA, N.RANDAZZO, J. VAN RANDWIJK, D. REAL, B. VAN RENS, F. RÉTHORÉ, P. REWIERSMA, G. RICCOBENE, V. RIGAUD, M. RIPANI, V. ROCA, C. RODA, J.F. ROLIN, M. ROMITA, H.J. ROSE, A. ROSTOVTSEV, J. ROUX, M. RUPPI, G.V. RUSSO, F. SALESA, K. SALOMON, P. SAPIENZA, F. SCHMITT, J.-P. SCHULLER, R. SHANIDZE, I. SOKALSKI, T. SPONA, M. SPURIO, G. VAN DER STEENHOVEN, T. STOLARCZYK, K. STREEB, D. STUBERT, L. SULAK, M. TAIUTI, C. TAMBURINI, C. TAO, G. TERRENI, L.F. THOMPSON, P. VALDY, V. VALENTE, B. VALLAGE, G. VENEKAMP, B. VERLAAT, P. VERNIN, R. DE VITA, G. DE VRIES, R. VAN WIJK, P. DE WITT HUBERTS, G. WOBBE, E. DE WOLF, A.-F. YAO, D. ZABOROV, H. ZACCONE, J.D. ZORNOZA, J. ZÚÑIGA, Groupe de Recherche en Physique des Hautes Energies (GRPHE), Institut Universitaire de Technologie de Colmar-Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA)), Département d'Astrophysique, de physique des Particules, de physique Nucléaire et de l'Instrumentation Associée (DAPNIA), Commissariat à l'énergie atomique et aux énergies alternatives (CEA), Centre de Physique des Particules de Marseille (CPPM), Aix Marseille Université (AMU)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Laboratoire d'Astrophysique de Marseille (LAM), Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS), Géoazur (GEOAZUR 6526), Institut de Recherche pour le Développement (IRD)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Université Nice Sophia Antipolis (... - 2019) (UNS), COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de la Côte d'Azur, Université Côte d'Azur (UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-Centre National de la Recherche Scientifique (CNRS), Institut Français de Recherche pour l'Exploitation de la Mer - Brest (IFREMER Centre de Bretagne), Institut Français de Recherche pour l'Exploitation de la Mer (IFREMER), Centre d'océanologie de Marseille (COM), Université de la Méditerranée - Aix-Marseille 2-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), IFREMER - Centre de Toulon/La Seyne Sur Mer (IFREMER), Département Recherches Subatomiques (DRS-IPHC), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Louis Pasteur - Strasbourg I-Centre National de la Recherche Scientifique (CNRS), APC - Astrophysique des Hautes Energies (APC - AHE), AstroParticule et Cosmologie (APC (UMR_7164)), Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Dipartimento di Astronomia, Universita degli Studi di Bologna, Alma Mater Studiorum Università di Bologna [Bologna] (UNIBO)-Alma Mater Studiorum Università di Bologna [Bologna] (UNIBO), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), ANTARES, Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-IUT de Colmar, Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA)), Institut de Recherche pour le Développement (IRD)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Université Nice Sophia Antipolis (1965 - 2019) (UNS), COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-Université Côte d'Azur (UCA)-Centre National de la Recherche Scientifique (CNRS), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Alma Mater Studiorum Università di Bologna [Bologna] (UNIBO), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-Institut Universitaire de Technologie de Colmar, Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Aix Marseille Université (AMU), Observatoire de la Côte d'Azur, Université Côte d'Azur (UCA)-Université Côte d'Azur (UCA)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Nice Sophia Antipolis (... - 2019) (UNS), Université Côte d'Azur (UCA)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut de Recherche pour le Développement (IRD)-Centre National de la Recherche Scientifique (CNRS), Institut Français de Recherche pour l'Exploitation de la Mer - Brest (IFREMER), Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Université de la Méditerranée - Aix-Marseille 2, Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Dipartimento di Astronomia, Universita degli Studi di Bologna, Università di Bologna [Bologna] (UNIBO)-Università di Bologna [Bologna] (UNIBO), and PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)
Subjects: Nuclear and High Energy Physics, [SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], Physics::Instrumentation and Detectors, Data management, Astrophysics::High Energy Astrophysical Phenomena, Neutrino telescope, ComputingMethodologies_IMAGEPROCESSINGANDCOMPUTERVISION, FOS: Physical sciences, Astrophysics, 01 natural sciences, [PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], Data filtering, Data acquisition, 0103 physical sciences, 14. Life underwater, Electronics, 010306 general physics, Instrumentation, data acquisition system, neutrino telescope, Remote sensing, Astroparticle physics, Physics, neutrino telescope, data acquisition system, [SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph], 010308 nuclear & particles physics, business.industry, Detector, Astrophysics (astro-ph), Astrophysics::Instrumentation and Methods for Astrophysics, Astronomy, Computer data storage, Física nuclear, business
Abstract: The ANTARES neutrino telescope is being constructed in the Mediterranean Sea. It consists of a large three-dimensional array of photo-multiplier tubes. The data acquisition system of the detector takes care of the digitisation of the photo-multiplier tube signals, data transport, data filtering, and data storage. The detector is operated using a control program interfaced with all elements. The design and the implementation of the data acquisition system are described., 20 pages, 6 figures, accepted for publication in Nucl. Instrum. Meth. A
Published: 2007
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39. The ANTARES Optical Beacon System

Author: E. Falchini, Dominique Lefèvre, J. F. Drogou, H. J. Rose, R. De Vita, A. Rostovtsev, D. Zaborov, J. P. Ernenwein, G. Lim, Guillaume Lambard, S. Cuneo, Lawrence Sulak, D. Lo Presti, Anne Deschamps, S. Galeotti, G. de Vries-Uiterweerd, Antoine Kouchner, H. Laschinsky, Christian Tamburini, H. Peek, Chantal Compère, J. Hogenbirk, V. Flaminio, A. S. Cussatlegras, V. Popa, Eric Delagnes, C. Petta, K. Streeb, Dominique Durand, F. Cafagna, E. Heine, G. Lelaizant, P. Lamare, C. Hoffman, M. Morganti, Stephanie Escoffier, H. Le Provost, E. Castorina, B. Vallage, Giorgio Riccobene, V. Lyashuk, J.D. Zornoza, M. Battaglieri, J. M. Gallone, R. Coniglione, T. Pradier, C. De Marzo, J. Beltramelli, G. Giacomelli, P. Goret, A. Capone, G. Venekamp, P. Kooijman, C. Olivetto, F. Urbano, A. Mazure, S. Kuch, Charling Tao, F. Louis, F. Jouvenot, I. Dekeyser, M. Jaquet, Annarita Margiotta, S. Favard, A. Milovanovic, M. Billault, Philippe Charvis, B. van Rens, J.-C. Languillat, R. Ostasch, J.R. Hubbard, G. Damy, F. Ameli, A. Albert, C. Fiorello, A. Bigi, D. Denans, E. A. De Wolf, C. Gojak, Timo Karg, J. Poinsignon, D. Castel, Nasser Kalantar-Nayestanaki, S. Anvar, G.V. Russo, Lester D.R. Thompson, Robert Lahmann, Juanan Aguilar, S. Cecchini, G. Wijnker, Chiara Roda, Vincenzo Cavasinni, C. Distefano, Jürgen Brunner, H. Kok, E. Barbarito, F. Réthoré, R. van Wijk, Juan José Hernández-Rey, J. P. Schuller, V. Valente, S. Loucatos, Nathalie Palanque-Delabrouille, P. Lagier, Paolo Piattelli, F.E. Ardellier-Desages, A. Calzas, J. P. Pineau, Diego Real, S. Ferry, J. van Randwijk, Julien Lavalle, J.-L. Fuda, E. V. Korolkova, Yvonne Becherini, F. Lucarelli, V. Bertin, F. Fehr, N. Girard, Elie Aslanides, W. Kretschmer, M. Taiuti, G. De Bonis, Y. Le Guen, I. Sokalski, J. Roux, R. Blaes, H. Zaccone, J.J. Destelle, T. Legou, A. Ceres, E. Kok, P. Valdy, G. Wobbe, V. Niess, T. Spona, L. Moscoso, A. Heijboer, G. Vaudaine, V. A. Kudryavstev, M. Melissas, Maurizio Spurio, M. Naumann-Godo, B. Verlaat, V. Roca, J. Hößl, P. Coyle, Rosario Megna, H. Loehner, B. Dinkespieler, Gregory David Hallewell, V. Rigaud, R. Auer, L. Caponetto, Paolo Sapienza, C. Racca, M. Ripani, Jean-Francois Rolin, E. Carmona, G. van der Steenhoven, Kay Graf, R. van Dantzig, Alexander Kappes, F. Mazéas, G. Terreni, S. L. Cartwright, C. Donzaud, G. F. Burgio, Tommaso Chiarusi, C. Kopper, M. Ruppi, S. Basa, Mohsen Harakeh, M. Circella, M. Jaspers, M. Ageron, Gisela Anton, T. Stolarczyk, R. Bruijn, M. Anghinolfi, J. Busto, P. Rewiersma, P. Keller, U. F. Katz, T. Noble, C. Naumann, P.K.A. de Witt Huberts, A. Le Van Suu, Yann Hello, C. Colnard, Mario Musumeci, N. Randazzo, J. J. Aubert, N. Cottini, L. Caillat, R. Pillet, P. Vernin, G. Lamanna, M. Mongelli, E. Migneco, J. Carr, F. Schmitt, K. Salomon, M. de Jong, F. Druillole, P. Payre, N. de Botton, M. Marcelin, Rezo Shanidze, M.C. Bouwhuis, G. Rusydi, A. F. Yao, K. Fratini, T. Montaruli, A. Perez, F. Salesa, A. Kruijer, F. Feinstein, P. Chauchot, J. Zúñiga, B. Hartmann, J. E. McMillan, S. M. Bradbury, R. Masullo, Centre de Physique des Particules de Marseille (CPPM), Aix Marseille Université (AMU)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Groupe de Recherche en Physique des Hautes Energies (GRPHE), Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-Institut Universitaire de Technologie de Colmar, Laboratoire d'Astrophysique de Marseille (LAM), Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Aix Marseille Université (AMU)-Centre National d'Études Spatiales [Toulouse] (CNES), Géoazur (GEOAZUR 6526), Institut de Recherche pour le Développement (IRD)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Université Nice Sophia Antipolis (... - 2019) (UNS), COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de la Côte d'Azur, Université Côte d'Azur (UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-Centre National de la Recherche Scientifique (CNRS), Institut Français de Recherche pour l'Exploitation de la Mer - Brest (IFREMER Centre de Bretagne), Institut Français de Recherche pour l'Exploitation de la Mer (IFREMER), Centre d'océanologie de Marseille (COM), Université de la Méditerranée - Aix-Marseille 2-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), IFREMER - Centre de Toulon/La Seyne sur Mer (IFREMER - CENTRE DE TOULON/LA SEYNE SUR MER), Commissariat à l'énergie atomique et aux énergies alternatives (CEA), Département Recherches Subatomiques (DRS-IPHC), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Louis Pasteur - Strasbourg I-Centre National de la Recherche Scientifique (CNRS), APC - Astrophysique des Hautes Energies (APC - AHE), AstroParticule et Cosmologie (APC (UMR_7164)), Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Dipartimento di Astronomia, Universita degli Studi di Bologna, Alma Mater Studiorum Università di Bologna [Bologna] (UNIBO)-Alma Mater Studiorum Università di Bologna [Bologna] (UNIBO), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), ANTARES, Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-IUT de Colmar, Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA)), Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS), Institut de Recherche pour le Développement (IRD)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Université Nice Sophia Antipolis (1965 - 2019) (UNS), COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-Université Côte d'Azur (UCA)-Centre National de la Recherche Scientifique (CNRS), Laboratoire Biogéochimie des Contaminants Métalliques (LBCM), Biogéochimie et Ecotoxicologie (BE), Institut Français de Recherche pour l'Exploitation de la Mer (IFREMER)-Institut Français de Recherche pour l'Exploitation de la Mer (IFREMER), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Alma Mater Studiorum Università di Bologna [Bologna] (UNIBO), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), M. AGERON, J.A. AGUILAR, A. ALBERT, F. AMELI, M. ANGHINOLFI, G. ANTON, S. ANVAR, F. ARDELLIER-DESAGES, E. ASLANIDES, J-J. AUBERT, R. AUER, E. BARBARITO, S. BASA, M. BATTAGLIERI, Y. BECHERINI, J. BELTRAMELLI, V. BERTIN, A. BIGI, M. BILLAULT, R. BLAES, N. DE BOTTON, M.C. BOUWHUIS, S.M. BRADBURY, R. BRUIJN, J. BRUNNER, G.F. BURGIO, J. BUSTO, F. CAFAGNA, L. CAILLAT, A. CALZAS, A. CAPONE, L. CAPONETTO, E. CARMONA, J. CARR, S.L. CARTWRIGHT, D. CASTEL, E. CASTORINA, V. CAVASINNI, S. CECCHINI, A. CERES, P. CHARVIS, P. CHAUCHOT, T. CHIARUSI, M. CIRCELLA, C. COLNARD, C. COMPERE, R. CONIGLIONE, N. COTTINI, P. COYLE, S. CUNEO, A-S. CUSSATLEGRAS, G. DAMY, R. VAN DANTZIG, G. DE BONIS, C. DE MARZO, R. DE VITA, I. DEKEYSER, E. DELAGNES, D. DENANS, A. DESCHAMPS, J-J. DESTELLE, B. DINKESPIELER, C. DISTEFANO, C. DONZAUD, J-F. DROGOU, F. DRUILLOLE, D. DURAND, J-P. ERNENWEIN, S. ESCOFFIER, E. FALCHINI, S. FAVARD, F. FEHR, F. FEINSTEIN, S. FERRY, C. FIORELLO, V. FLAMINIO, K. FRATINI, J-L. FUDA, S. GALEOTTI, J-M. GALLONE, G. GIACOMELLI, N. GIRARD, C. GOJAK, PH. GORET, K. GRAF, G. HALLEWELL, M.N. HARAKEH, B. HARTMANN, A. HEIJBOER, E. HEINE, Y. HELLO, J.J. HERNANDEZ-REY, J. HOSSL, C. HOFFMAN, J. HOGENBIRK, J.R. HUBBARD, M. JAQUET, M. JASPERS, M. DE JONG, F. JOUVENOT, N. KALANTAR-NAYESTANAKI, A. KAPPES, T. KARG, U. KATZ, P. KELLER, E. KOK, H. KOK, P. KOOIJMAN, C. KOPPER, E.V. KOROLKOVA, A. KOUCHNER, W. KRETSCHMER, A. KRUIJER, S. KUCH, V.A. KUDRYAVSTEV, P. LAGIER, R. LAHMANN, G. LAMANNA, P. LAMARE, G. LAMBARD, J-C. LANGUILLAT, H. LASCHINSKY, J. LAVALLE, Y. LE GUEN, H.LE PROVOST, A. LE VAN SUU, D. LEFEVRE, T. LEGOU, G. LELAIZANT, G. LIM, D.LO PRESTI, H. LOEHNER, S. LOUCATOS, F. LOUIS, F. LUCARELLI, V. LYASHUK, M. MARCELIN, A. MARGIOTTA, R. MASULLO, F. MAZEAS, MAZURE A.R, J.E. MCMILLAN, R. MEGNA, M. MELISSAS, E. MIGNECO, A. MILOVANOVIC, M. MONGELLI, T. MONTARULI, M. MORGANTI, L. MOSCOSO, M. MUSUMECI, M. NAUMANN-GODO, C. NAUMANN, V. NIESS, T. NOBLE, C. OLIVETTO, R. OSTASCH, N. PALANQUE-DELABROUILLE, P. PAYRE, H. PEEK, A. PEREZ, C. PETTA, P. PIATTELLI, R. PILLET, J-P. PINEAU, J. POINSIGNON, V. POPA, T. PRADIER, C. RACCA, N. RANDAZZO, J. VAN RANDWIJK, D. REAL, B. VAN RENS, F. RETHORE, P. REWIERSMA, G. RICCOBENE, V. RIGAUD, M. RIPANI, V. ROCA, C. RODA, J.F. ROLIN, H.J. ROSE, A. ROSTOVTSEV, J. ROUX, M. RUPPI, G.V. RUSSO, G. RUSYDI, F. SALESA, K. SALOMON, P. SAPIENZA, F. SCHMITT, J-P. SCHULLER, R. SHANIDZE, I. SOKALSKI, T. SPONA, M. SPURIO, G. VAN DER STEENHOVEN, T. STOLARCZYK, K. STREEB, L. SULAK, M. TAIUTI, C. TAMBURINI, C. TAO, G. TERRENI, L.F. THOMPSON, F. URBANO, P. VALDY, V. VALENTE, B. VALLAGE, G. VAUDAINE, G. VENEKAMP, B. VERLAAT, P. VERNIN, G. DE VRIES-UITERWEERD, R. VAN WIJK, G. WIJNKER, P. DE WITT HUBERTS, G. WOBBE, E. DE WOLF, A-F. YAO, D. ZABOROV, H. ZACCONE, J.D. ZORNOZA, J. ZUNIGA, KVI - Center for Advanced Radiation Technology, Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Aix Marseille Université (AMU), Observatoire de la Côte d'Azur, Université Côte d'Azur (UCA)-Université Côte d'Azur (UCA)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Nice Sophia Antipolis (... - 2019) (UNS), Université Côte d'Azur (UCA)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut de Recherche pour le Développement (IRD)-Centre National de la Recherche Scientifique (CNRS), Institut Français de Recherche pour l'Exploitation de la Mer - Brest (IFREMER), Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Université de la Méditerranée - Aix-Marseille 2, Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Dipartimento di Astronomia, Universita degli Studi di Bologna, Università di Bologna [Bologna] (UNIBO)-Università di Bologna [Bologna] (UNIBO), and PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)
Subjects: Nuclear and High Energy Physics, Photomultiplier, Physics::Instrumentation and Detectors, [SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], Astrophysics::High Energy Astrophysical Phenomena, FOS: Physical sciences, neutrino telescope, optical beacon, time calibration, Astrophysics, 01 natural sciences, law.invention, Telescope, [PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], Optics, law, 0103 physical sciences, Calibration, Angular resolution, 14. Life underwater, 010306 general physics, Instrumentation, Cherenkov radiation, Physics, [SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph], neutrino telescope, time calibration, optical beacon, 010308 nuclear & particles physics, business.industry, Detector, Astrophysics (astro-ph), Astrophysics::Instrumentation and Methods for Astrophysics, SITE, Astronomy, Beacon, LIGHT, Física nuclear, Neutrino, business
Abstract: ANTARES is a neutrino telescope being deployed in the Mediterranean Sea. It consists of a three dimensional array of photomultiplier tubes that can detect the Cherenkov light induced by charged particles produced in the interactions of neutrinos with the surrounding medium. High angular resolution can be achieved, in particular when a muon is produced, provided that the Cherenkov photons are detected with sufficient timing precision. Considerations of the intrinsic time uncertainties stemming from the transit time spread in the photomultiplier tubes and the mechanism of transmission of light in sea water lead to the conclusion that a relative time accuracy of the order of 0.5 ns is desirable. Accordingly, different time calibration systems have been developed for the ANTARES telescope. In this article, a system based on Optical Beacons, a set of external and well-controlled pulsed light sources located throughout the detector, is described. This calibration system takes into account the optical properties of sea water, which is used as the detection volume of the ANTARES telescope. The design, tests, construction and first results of the two types of beacons, LED and laser-based, are presented., 21 pages, 18 figures, submitted to Nucl. Instr. and Meth. Phys. Res. A
Published: 2007
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40. Ankle-like Feature in the Energy Spectrum of Light Elements of Cosmic Rays Observed with KASCADE-Grande

Author: Kai Daumiller, M. Melissas, J. Oehlschläger, D. Fuhrmann, G. C. Trinchero, P. Łuczak, M. Wommer, J. C. Arteaga-Velázquez, N. Palmieri, H. Bozdog, Béatrice Fuchs, K. Bekk, V. de Souza, J. Blümer, D. Kang, D. Huber, Frank G. Schröder, H.O. Klages, T. Huege, F. Di Pierro, C. Morello, F. Cossavella, B. Mitrica, Jörg R. Hörandel, A. Chiavassa, T. Pierog, Markus Roth, J. Engler, M. Finger, Claus Grupen, H. J. Mathes, R. Glasstetter, H.J. Gils, H. Rebel, M. Ludwig, A. Weindl, M. Petcu, I.M. Brancus, S. Ostapchenko, G. Toma, S. Schoo, H. Schieler, K. Link, Karl-Heinz Kampert, J. Zabierowski, P. Doll, H.J. Mayer, M. E. Bertaina, J. Milke, J. Wochele, Octavian Sima, D. Heck, H. Ulrich, Andreas Haungs, E. Cantoni, Ralph Engel, and W. D. Apel
Subjects: High Energy Astrophysical Phenomena (astro-ph.HE), Physics, Nuclear and High Energy Physics, KASCADE, Astronomy, Energy spectrum, ComputingMethodologies_DOCUMENTANDTEXTPROCESSING, FOS: Physical sciences, LUZ (MEDIÇÃO), Cosmic ray, Astrophysics, Astrophysics - High Energy Astrophysical Phenomena, Power law
Abstract: Recent results of the KASCADE-Grande experiment provided evidence for a mild knee-like structure in the all-particle spectrum of cosmic rays at $E = 10^{16.92 \pm 0.10} \, \mathrm{eV}$, which was found to be due to a steepening in the flux of heavy primary particles. The spectrum of the combined components of light and intermediate masses was found to be compatible with a single power law in the energy range from $10^{16.3} \, \mathrm{eV}$ to $10^{18} \, \mathrm{eV}$. In this paper, we present an update of this analysis by using data with increased statistics, originating both from a larger data set including more recent measurements and by using a larger fiducial area. In addition, optimized selection criteria for enhancing light primaries are applied. We find a spectral feature for light elements, namely a hardening at $E = 10^{17.08 \pm 0.08} \, \mathrm{eV}$ with a change of the power law index from $-3.25 \pm 0.05$ to $-2.79 \pm 0.08$., 6 pages, 5 figures, 1 table; this is the authors' version; the definite version has been published in Phys. Rev. D (http://link.aps.org/doi/10.1103/PhysRevD.87.081101)
Published: 2013

41. Thunderstorm Observations by Air-Shower Radio Antenna Arrays

Author: H. J. Mathes, Jörg R. Hörandel, M. Ludwig, C. Rühle, A. Horneffer, Claus Grupen, J.C. Arteaga, F.G. Schröder, D. Huber, Markus Roth, Kai Daumiller, J. Blümer, G.C. Trinchero, Peter Buchholz, Moses Ender, G. Toma, I.M. Brancus, F. Di Pierro, C. Morello, A. Weindl, L. Bähren, Jan Kuijpers, O. Krömer, P.G. Isar, Peter L. Biermann, H. Gemmeke, A. Schmidt, T. Pierog, M. Wommer, M. Melissas, J. Rautenberg, S. Nehls, D. Kang, Heino Falcke, M. Finger, Tim Huege, K. Bekk, J. Wochele, V. de Souza, Octavian Sima, D. Heck, K. Link, J. A. Zensus, A. Haungs, E. Cantoni, J. Zabierowski, P. Doll, Ralph Engel, J. Oehlschläger, M. E. Bertaina, Stijn Buitink, A. Chiavassa, H. Rebel, W. D. Apel, H. Schieler, Karl-Heinz Kampert, P. Łuczak, N. Palmieri, H. Bozdog, Alexandra Saftoiu, and D. Fuhrmann
Subjects: Atmospheric Science, Astronomy, Astrophysics::High Energy Astrophysical Phenomena, FOS: Physical sciences, Aerospace Engineering, Cosmic ray, Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, Broadband, Instrumentation and Methods for Astrophysics (astro-ph.IM), High Energy Astrophysical Phenomena (astro-ph.HE), Physics, LOPES, Astrophysics::Instrumentation and Methods for Astrophysics, Astronomy and Astrophysics, Lightning, Computational physics, Lightning strike, Geophysics, Air shower, Space and Planetary Science, Thunderstorm, RÁDIO, General Earth and Planetary Sciences, Astrophysics - High Energy Astrophysical Phenomena, Astrophysics - Instrumentation and Methods for Astrophysics, Radio wave
Abstract: Relativistic, charged particles present in extensive air showers (EAS) lead to a coherent emission of radio pulses which are measured to identify the shower initiating high-energy cosmic rays. Especially during thunderstorms, there are additional strong electric fields in the atmosphere, which can lead to further multiplication and acceleration of the charged particles and thus have influence on the form and strength of the radio emission. For a reliable energy reconstruction of the primary cosmic ray by means of the measured radio signal it is very important to understand how electric fields affect the radio emission. In addition, lightning strikes are a prominent source of broadband radio emissions that are visible over very long distances. This, on the one hand, causes difficulties in the detection of the much lower signal of the air shower. On the other hand the recorded signals can be used to study features of the lightning development. The detection of cosmic rays via the radio emission and the influence of strong electric fields on this detection technique is investigated with the LOPES experiment in Karlsruhe, Germany. The important question if a lightning is initiated by the high electron density given at the maximum of a high-energy cosmic-ray air shower is also investigated, but could not be answered by LOPES. But, these investigations exhibit the capabilities of EAS radio antenna arrays for lightning studies. We report about the studies of LOPES measured radio signals of air showers taken during thunderstorms and give a short outlook to new measurements dedicated to search for correlations of lightning and cosmic rays.
Published: 2013

42. LOPES-3D, an antenna array for full signal detection of air-shower radio emission

Author: D. Kang, P. Doll, Heino Falcke, Béatrice Fuchs, Jörg R. Hörandel, A. Horneffer, F. Di Pierro, C. Morello, J.C. Arteaga, A. Chiavassa, M. Wommer, J. Rautenberg, A. Weindl, Jan Kuijpers, Peter L. Biermann, Kai Daumiller, L. Bähren, O. Krömer, K. Bekk, C. Rühle, J. Oehlschläger, J. Blümer, Claus Grupen, P.G. Isar, V. de Souza, H. Bozdog, M. Finger, M. E. Bertaina, G.C. Trinchero, Markus Roth, H. Rebel, P. Łuczak, K. Link, N. Palmieri, A. Haungs, M. Melissas, J. Zabierowski, H. J. Mathes, H. Schieler, M. Ludwig, Alexandra Saftoiu, Karl-Heinz Kampert, G. Toma, F.G. Schröder, D. Huber, A. Schmidt, D. Fuhrmann, T. Pierog, E. Cantoni, Ralph Engel, W. D. Apel, Peter Buchholz, J. A. Zensus, I.M. Brancus, H. Gemmeke, Tim Huege, J. Wochele, Octavian Sima, and D. Heck
Subjects: High Energy Astrophysical Phenomena (astro-ph.HE), Physics, Nuclear and High Energy Physics, LOPES, business.industry, Astronomy, Astrophysics::High Energy Astrophysical Phenomena, Astrophysics::Instrumentation and Methods for Astrophysics, FOS: Physical sciences, Cosmic ray, Astrophysics::Cosmology and Extragalactic Astrophysics, Antenna array, Optics, Air shower, Detection theory, Antenna (radio), business, Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - High Energy Astrophysical Phenomena, Instrumentation and Methods for Astrophysics (astro-ph.IM), Instrumentation, Sensitivity (electronics), Energy (signal processing)
Abstract: To better understand the radio signal emitted by extensive air-showers and to further develop the radio detection technique of high-energy cosmic rays, the LOPES experiment was reconfigured to LOPES-3D. LOPES-3D is able to measure all three vectorial components of the electric field of radio emission from cosmic ray air showers. The additional measurement of the vertical component ought to increase the reconstruction accuracy of primary cosmic ray parameters like direction and energy, provides an improved sensitivity to inclined showers, and will help to validate simulation of the emission mechanisms in the atmosphere. LOPES-3D will evaluate the feasibility of vectorial measurements for large scale applications. In order to measure all three electric field components directly, a tailor-made antenna type (tripoles) was deployed. The change of the antenna type necessitated new pre-amplifiers and an overall recalibration. The reconfiguration and the recalibration procedure are presented and the operationality of LOPES-3D is demonstrated.
Published: 2013

43. KASCADE-Grande measurements of energy spectra for elemental groups of cosmic rays

Author: S. Ostapchenko, H.J. Gils, A. Chiavassa, Béatrice Fuchs, M. Wommer, V. de Souza, F. Cossavella, H. Rebel, P. Łuczak, F. Di Pierro, G.C. Trinchero, N. Palmieri, D. Fuhrmann, S. Schoo, Markus Roth, H. Bozdog, J. Engler, D. Kang, E. Cantoni, C. Morello, Jörg R. Hörandel, H. Schieler, H.O. Klages, Karl-Heinz Kampert, M. Ludwig, T. Pierog, M. Finger, P. Doll, M. Melissas, B. Mitrica, R. Glasstetter, H. J. Mathes, K. Bekk, Ralph Engel, F.G. Schröder, W. D. Apel, Andreas Haungs, A. Weindl, Claus Grupen, J.C. Arteaga-Velázquez, Kai Daumiller, H.J. Mayer, J. Oehlschläger, I.M. Brancus, M. E. Bertaina, J. Milke, K. Link, J. Zabierowski, T. Huege, M. Petcu, G. Toma, J. Wochele, D. Huber, Octavian Sima, J. Blümer, D. Heck, and H. Ulrich
Subjects: Physics, High Energy Astrophysical Phenomena (astro-ph.HE), Range (particle radiation), Muon, Astronomy, Astrophysics::High Energy Astrophysical Phenomena, Astrophysics::Instrumentation and Methods for Astrophysics, FOS: Physical sciences, Astronomy and Astrophysics, Cosmic ray, Astrophysics, ASTROFÍSICA, Scintillator, Spectral line, Nuclear physics, Air shower, KASCADE, Scintillation counter, ComputingMethodologies_DOCUMENTANDTEXTPROCESSING, Astrophysics - High Energy Astrophysical Phenomena
Abstract: The KASCADE-Grande air shower experiment [W. Apel, et al. (KASCADE-Grande collaboration), Nucl. Instrum. Methods A 620 (2010) 202] consists of, among others, a large scintillator array for measurements of charged particles, Nch, and of an array of shielded scintillation counters used for muon counting, Nmu. KASCADE-Grande is optimized for cosmic ray measurements in the energy range 10 PeV to about 2000 PeV, where exploring the composition is of fundamental importance for understanding the transition from galactic to extragalactic origin of cosmic rays. Following earlier studies of the all-particle and the elemental spectra reconstructed in the knee energy range from KASCADE data [T. Antoni, et al. (KASCADE collaboration), Astropart. Phys. 24 (2005) 1], we have now extended these measurements to beyond 200 PeV. By analysing the two-dimensional shower size spectrum Nch vs. Nmu for nearly vertical events, we reconstruct the energy spectra of different mass groups by means of unfolding methods over an energy range where the detector is fully efficient. The procedure and its results, which are derived based on the hadronic interaction model QGSJET-II-02 and which yield a strong indication for a dominance of heavy mass groups in the covered energy range and for a knee-like structure in the iron spectrum at around 80 PeV, are presented. This confirms and further refines the results obtained by other analyses of KASCADE-Grande data, which already gave evidence for a knee-like structure in the heavy component of cosmic rays at about 80 PeV [W. Apel, et al. (KASCADE-Grande collaboration), Phys. Rev. Lett. 107 (2011) 171104]., Accepted for publication in Astropart. Phys. (2013)
Published: 2013

44. All-particle energy spectrum of KASCADE-Grande based on shower size and different hadronic interaction models

Author: G. Toma, J. C. Arteaga-Velázquez, J. Bluemer, E. Cantoni, N. Palmieri, Kai Daumiller, T. Pierog, H. Bozdog, J. R. Hoerandel, H.J. Mayer, Andrea Chiavassa, Markus Roth, J. Engler, B. Mitrica, D. Wochele, H. J. Mathes, Béatrice Fuchs, S. Ostapchenko, M. Melissas, T. Huege, M. E. Bertaina, D. Huber, J. Milke, R. Glasstetter, K. Link, M. Petcu, W. D. Apel, V. de Souza, J. Oehlschlaeger, A. Haungs, I.M. Brancus, F. Di Pierro, C. Morello, H. Ulrich, J. Wochele, D. Heck, D. Fuhrmann, K. H. Kampert, G. C. Trinchero, C. Curcio, K. Bekk, Claus Grupen, D. Kang, H.O. Klages, S. Schoo, Octavian Sima, A. Weindl, H. Schieler, M. Ludwig, P. Doll, H. Rebel, R. Engel, F. Cossavella, P. Luczak, H.J. Gils, and Frederic Schroeder
Subjects: Physics, History, Range (particle radiation), Muon, Astrophysics::High Energy Astrophysical Phenomena, Astronomy, Hadron, Astrophysics::Instrumentation and Methods for Astrophysics, Interaction model, Cosmic ray, Electron, Charged particle, Computer Science Applications, Education, Nuclear physics, KASCADE, GeneralLiterature_REFERENCE(e.g.,dictionaries,encyclopedias,glossaries)
Abstract: KASCADE-Grande is dedicated for investigations of cosmic-ray air showers in the primary energy range from 10 PeV to 1 EeV. The multi-detector system allows us to reconstruct charged particles, electron and muon numbers for individual air showers with high accuracies. Based on the shower size ($N_{ch}$) spectra of the charged particle component, the all-particle energy spectrum of cosmic rays is reconstructed, where attenuation effects in the atmosphere are corrected by applying the constant intensity cut method. The energy calibration is performed by using CORSIKA simulations with high-energy interaction models QGSJET-II-2, QGSJET-II-4, EPOS 1.99 and SIBYLL 2.1, where FLUKA has been used as low-energy interaction model for all cases. In the different hadronic models, different abundances for shower particles are predicted. Such model differences in the observables will be compared and discussed in this contribution. Furthermore, by using data with increasing statistics, the updated energy spectra by means of different interaction models will be presented.
Published: 2013

45. Radio Measurements of Air Showers with LOPES

Author: A. Horneffer, D. Kang, C. Grupen, M. Ludwig, I.M. Brancus, J. Wochele, Octavian Sima, M. E. Bertaina, A. Schmidt, H. Gemmeke, J. Rautenberg, Tim Huege, P. Łuczak, N. Palmieri, D. Heck, E. Cantoni, Ralph Engel, D. Fuhrmann, Paula Gina Isar, K. Link, A. Haungs, F. Di Pierro, C. Morello, J. Zabierowski, W. D. Apel, Peter L. Biermann, O. Krömer, L. Bähren, P. Doll, Heino Falcke, H. Bozdog, A. Weindl, Jan Kuijpers, Kai Daumiller, H. Rebel, H. Schieler, Béatrice Fuchs, A. Saftoiu, K. H. Kampert, T. Pierog, Frank G. Schröder, Jörg R. Hörandel, J. A. Zensus, V. de Souza, J. Blümer, J. C. Arteaga-Velázquez, G. Toma, G.C. Trinchero, M. Melissas, J. Oehlschläger, D. Huber, C. Rühle, Markus Roth, Andrea Chiavassa, H. J. Mathes, and K. Bekk
Subjects: Physics, History, Meteorology, LOPES, Astronomy, Ambient noise level, Computer Science Applications, Education, Antenna array, Amplitude, Calibration, Angular resolution, GeneralLiterature_REFERENCE(e.g.,dictionaries,encyclopedias,glossaries), Energy (signal processing), Noise (radio), Remote sensing
Abstract: LOPES is a digital antenna array for the radio measurement of cosmic-ray air showers at energies around 1017 eV. It is triggered by the KASCADE-Grande air-shower array at the Karlsruhe Institute of Technology (KIT), Germany. Because of an absolute amplitude calibration and a sophisticated data analysis, LOPES can test models for the radio emission to an up-to-now unachieved level, thus improving our understanding of the radio emission mechanisms. Recent REAS simulations of the air-shower radio emission come closer to the measurements than any previously tested simulations. We have determined the radio-reconstruction precision of interesting air-shower parameters by comparing LOPES reconstructions to both REAS simulations and KASCADE-Grande measurements, and present our latest results for the angular resolution, the energy and the Xmax reconstruction based on the radio measurement of about 500 air showers. Although the precision of LOPES is limited by the high level of anthropogenic noise at KIT, it opens a promising perspective for next-generation radio arrays in regions with a lower ambient noise level.
Published: 2013

46. Comparison of LOPES measurements with CoREAS and REAS 3.11 simulations

Author: D. Kang, M. Haug, G. C. Trinchero, K. Bekk, T. Pierog, J. Wochele, H. J. Mathes, H. Gemmeke, D. Heck, A. Schmidt, Claus Grupen, H. Rebel, A. Horneffer, P. Doll, M. Melissas, L. Bähren, P. Łuczak, N. Palmieri, J. Oehlschläger, D. Fuhrmann, H. Bozdog, V. de Souza, F. Di Pierro, C. Morello, A. Weindl, Heino Falcke, Jan Kuijpers, Tim Huege, C. Rühle, M. Ludwig, Peter L. Biermann, O. Krömer, Béatrice Fuchs, R. Engel, K. H. Kampert, A. Saftoiu, Markus Roth, Paula Gina Isar, Kai Daumiller, J. A. Zensus, W. D. Apel, J. Rautenberg, Octavian Sima, H. Schieler, G. Toma, J.R. Hörandel, D. Huber, Frank G. Schröder, I.M. Brancus, J. Blümer, J. C. Arteaga-Velázquez, M. E. Bertaina, K. Link, A. Haungs, J. Zabierowski, and Andrea Chiavassa
Subjects: Physics, Formalism (philosophy of mathematics), Optics, Amplitude, LOPES, business.industry, Monte carlo code, Astronomy, ComputingMethodologies_DOCUMENTANDTEXTPROCESSING, business, Computational physics
Abstract: In the previous years, LOPES emerged as a very successful experiment measuring the radio emission from air showers in the MHz frequency range. In parallel, the theoretical description of radio emission was developed further and REAS became a widely used simulation Monte Carlo code. REAS 3 as well as CoREAS are based on the endpoint formalism, i.e. they calculate the emission of the air-shower without assuming specific emission mechanisms. While REAS 3 is based on histograms derived from CORSIKA simulations, CoREAS is directly implemented into CORSIKA without loss of information due to histogramming of the particle distributions. In contrast to the earlier versions of REAS, the newest version REAS 3.11 and CoREAS take into account a realistic atmospheric refractive index. To improve the understanding of the emission processes and judge the quality of the simulations, we compare their predictions with high-quality events measured by LOPES. We present results concerning the lateral distribution measured with 30 east-west aligned LOPES antennas. Only the simulation codes including the refractive index (REAS 3.11 and CoREAS) are able to reproduce the slope of measured lateral distributions, but REAS 3.0 predicts too steep lateral distributions, and does not predict rising lateral distributions as seen in a few LOPES events. Moreover, REAS 3.11 predicts an absolute amplitude compatible with the LOPES measurements.
Published: 2013
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47. Comparing LOPES measurements of air-shower radio emission with REAS 3.11 and CoREAS simulations

Author: Alexandra Saftoiu, Béatrice Fuchs, D. Huber, Jörg R. Hörandel, K. Link, G.C. Trinchero, F. Di Pierro, A. Haungs, C. Morello, C. Rühle, D. Fuhrmann, W. D. Apel, J. Blümer, H. Bozdog, Paula Gina Isar, J. Rautenberg, M. Melissas, Markus Roth, Peter L. Biermann, J. Zabierowski, J.C. Arteaga-Velázquez, T. Pierog, A. Chiavassa, G. Toma, Tim Huege, P. Łuczak, N. Palmieri, Kai Daumiller, J. Oehlschläger, E. Cantoni, Ralph Engel, A. Schmidt, Heino Falcke, M. E. Bertaina, J. A. Zensus, I.M. Brancus, A. Horneffer, Claus Grupen, K. Bekk, P. Doll, V. de Souza, A. Weindl, Jan Kuijpers, H. Gemmeke, H. Rebel, H. Schieler, Karl-Heinz Kampert, J. Wochele, Octavian Sima, D. Heck, M. Ludwig, H. J. Mathes, F.G. Schröder, L. Bähren, O. Krömer, and D. Kang
Subjects: Physics, High Energy Astrophysical Phenomena (astro-ph.HE), LOPES, Astronomy, Astrophysics::High Energy Astrophysical Phenomena, Monte Carlo method, Astrophysics::Instrumentation and Methods for Astrophysics, FOS: Physical sciences, Astronomy and Astrophysics, Cosmic ray, Astrophysics, Askaryan effect, Amplitude, Air shower, Earth's magnetic field, ComputingMethodologies_DOCUMENTANDTEXTPROCESSING, Astrophysics - High Energy Astrophysical Phenomena, RAIOS CÓSMICOS, Radio wave
Abstract: Cosmic ray air showers emit radio pulses at MHz frequencies, which can be measured with radio antenna arrays - like LOPES at the Karlsruhe Institute of Technology in Germany. To improve the understanding of the radio emission, we test theoretical descriptions with measured data. The observables used for these tests are the absolute amplitude of the radio signal, and the shape of the radio lateral distribution. We compare lateral distributions of more than 500 LOPES events with two recent and public Monte Carlo simulation codes, REAS 3.11 and CoREAS (v 1.0). The absolute radio amplitudes predicted by REAS 3.11 are in good agreement with the LOPES measurements. The amplitudes predicted by CoREAS are lower by a factor of two, and marginally compatible with the LOPES measurements within the systematic scale uncertainties. In contrast to any previous versions of REAS, REAS 3.11 and CoREAS now reproduce the shape of the measured lateral distributions correctly. This reflects a remarkable progress compared to the situation a few years ago, and it seems that the main processes for the radio emission of air showers are now understood: The emission is mainly due to the geomagnetic deflection of the electrons and positrons in the shower. Less important but not negligible is the Askaryan effect (net charge variation). Moreover, we confirm that the refractive index of the air plays an important role, since it changes the coherence conditions for the emission: Only the new simulations including the refractive index can reproduce rising lateral distributions which we observe in a few LOPES events. Finally, we show that the lateral distribution is sensitive to the energy and the mass of the primary cosmic ray particles., Comment: Attention: results and conclusion partly changed due to updated calibration. See Astroparticle Physics 75 (2016) 72-74; arXiv:1507.07389
Published: 2013
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48. Bounds on the density of sources of ultra-high energy cosmic rays from the Pierre Auger Observatory

Author: Martina Bohacova, N. Nierstenhoefer, J. Sorokin, R. F. Gamarra, L. Nozka, G. P. Guedes, J. Knapp, A. Lopez Agüera, Petr Schovanek, D. Maurel, J. Stasielak, S. Coutu, A. Shadkam, C. Timmermans, A. F. Grillo, Juan Carlos D'Olivo, T. Pierog, F. Guarino, John Matthews, T. Huege, A. Parra, Philipp Mertsch, D. Veberǐc, G. Golup, P. L. Ghia, Peter Buchholz, Jeffrey Brack, Olaf Scholten, Humberto Ibarguen Salazar, A. F. Barbosa, M. Lauscher, A. Belĺetoile, I.M. Brancus, Rossella Caruso, A. Lucero, H. Glass, N. Kunka, H. Blümer, Marco Aglietta, K. B. Barber, G. La Rosa, L. del Peral, Markus Ahlers, B. Revenu, O. Ravel, D. Harari, Alessandro Petrolini, H. J. Mathes, B. García, Mario Scuderi, B. Mitrica, B. Gookin, M. Weber, J. Schovancova, U. Fröhlich, Alina Mihaela Badescu, C. Baus, A. Aminaei, L. Molina-Bueno, E. Kemp, J. Chauvin, D. B. Tridapalli, A. Segreto, D. Monnier Ragaigne, E. Varela, N. Griffith, W. J. M. de Mello Junior, J. Rodriguez Martino, L. Villasẽnor, C. De Donato, Tobias Winchen, R. López, Karen S. Caballero-Mora, P. Karhan, J. A.J. Matthews, Xavier Bertou, Carola Dobrigkeit, Octavian Sima, J. G. Gonzalez, V. C. Holmes, G. De La Vega, M. Pontz, R. E. Burton, C. Pfendner, A. Schmidt, H. Martinez, N. Pacheco, E. Menichetti, A. Smia Lkowski, J. Kleinfeller, D. Nosek, T. Yamamoto, E. J. Ahn, A. Tonachini, J. Chirinos Diaz, A. Zepeda, Pedro Assis, A. Etchegoyen, K. Kadija, P. Wahrlich, G. Navarra, G. Matthiae, R. Şḿida, H. Spinka, D. Lebrun, B. Rouilĺe-Dörfeuil, B. Vargas Cárdenas, Maria Concetta Maccarone, T. Suomijärvi, Markus Roth, J. R. Ḧorandel, G. Cocciolo, Javier Tiffenberg, Alan Watson, J. Pallotta, R. Mussa, J. J. Beatty, J. Coppens, E. J. Quel, J. Rodriguez Rojo, H. Dembinski, M. A. Muller, M. Prouza, Martin Erdmann, C. A. Moura, C. Rühle, V. de Souza, Antonio Bueno, Sergio Pastor, Subir Sarkar, D. Heck, J. Alvarez Castillo, F. Sarazin, L. Nellen, M. Szuba, G. Garilli, Brian Fick, G. Salina, Olivier Deligny, J. Allen, E. Mayotte, F.G. Schröder, G. Marsella, Enrique Zas, S. Mollerach, S. Grebe, Daniel Kuempel, Carlos Escobar, N. Fazzini, T. Hebbeker, Julien Aublin, Béatrice Fuchs, Niraj Dhital, A. Filevich, F. Werner, C. Morauthello, J. Bäuml, R. Squartini, A. Weindl, Denise Boncioli, E. Roulet, I. Lhenry-Yvon, Elton J. G. Santos, T. Paul, K. Link, P. Abreu, Gualberto Avila, C. Di Giulio, S. Maldera, Peter Gorham, Fernando Contreras, S. Gambetta, B. Wilczyńska, R. Piegaia, German Ros, D. Ravignani, J. R. Vázquez, Ingomar Allekotte, J. Alvarez-Mũniz, K. D. de Vries, Roger W Clay, J. Lozano Bahilo, Segev BenZvi, L. Collica, W. Docters, M. Ludwig, N. Hollon, V. Verzi, K. Louedec, Mariangela Settimo, Alexey Yushkov, E. Petermann, D. Nitz, Miroslav Pech, D. Maurizio, A. Haungs, J. L. Harton, Corbin Covault, Angela V. Olinto, M. Monasor, R. Gaior, S. H. Cheng, P. T. Nhung, J. Rosado, O. Fratu, M. L. Díaz Castro, Ivone F. M. Albuquerque, Ke Fang, V. H. Ponce, D. Martraire, L. Perrone, Azadeh Keivani, Jiri Chudoba, D. Torres Machado, G. Farrar, J. C. Moreno, G. Medina-Tanco, Rémi Bardenet, Petr Travnicek, A. C. Fauth, C. Aramo, M. Tueros, Pavel Horvath, Y. Petrov, M. S. Sutherland, M. Urban, G. van Aar, T. A. Harrison, Piotr Homola, Luis A. Anchordoqui, V. Marin, M. Stephan, P. Mantsch, A. van Vliet, F. Suarez, H. H. Silva Lopez, Sergio Dasso, A. C. Rovero, S. J. Saffi, H. Lyberis, Carla Bonifazi, C. Bleve, M. Oliveira, M. Ave, E. Trovato, A. Criss, Vincenzo Rizi, Jose A. Bellido, Maria-Teresa Dova, P. Facal San Luis, Juan Manuel Figueira, Pham Ngoc Diep, Lino Miramonti, Z. Szadkowski, M. Josebachuili, J. Neuser, K. Kotera, Dusan Mandat, Sofia Andringa, Peter Schiffer, V. Scherini, R. Alves Batista, C. J. Todero Peixoto, M. Gómez Berisso, Moritz Münchmeyer, Christopher B. Williams, S. Le Coz, R. C. Shellard, D. Martello, M. Ziolkowski, N. Scharf, V. Pirronello, R. Pelayo, P. Pieroni, Roberta Colalillo, O. Martínez Bravo, W. Rodrigues de Carvalho, G. C. Hill, A. G. Mariazzi, G. Torralba Elipe, M. Malacari, J. Gitto, Peter L. Biermann, Heino Falcke, M. Platino, F. Diogo, T. Niggemann, Ralph Engel, M. Plum, G. Varner, J. Oehlschläger, C. Jarne, Jing Zhou, Yunrong Zhu, T. Antǐci'c, D. H. Koang, J. Ridky, B. Ḱegl, F. Arqueros, S. Querchfeld, J. L. Kelley, P. Necesal, R. Cester, B. J. Whelan, N. Krohm, L. Valore, L. Buroker, J. Vicha, B. Morales, R. M. de Almeida, O. Krömer, A. Stutz, A.M. van den Berg, G. Wieczorek, E. D. Fraenkel, M. Tartare, G. Toma, L. Niemietz, I. C. Mariş, C. E. Santo, Francisco J. Blanco, J. W. Cronin, M. Wommer, S. Stanič, H. Wilczyński, P. Billoir, Paolo Privitera, S. Mićanović, B. Zamorano Garcia, S. Fliescher, M. Risse, M. S.A.B. Lẽao, J. D. Swain, I. Rodriguez Cabo, F. Gomez Albarracin, Kai Daumiller, Jose Chinellato, P. Lebrun, L. Tomankova, P.F. Gómez Vitale, P. Lautridou, B. Toḿe, J. Espadanal, Johannes Schulz, R. Meyhandan, M. Pimenta, A. Widom, M. Ortiz, D. LaHurd, J. Roberts, M. Palatka, B. D. Fox, N. T. Thao, J. Maller, G. Parente, P. W. Younk, R. J. Lauer, R. M. Kieckhafer, A. Gorgi, S. Westerhoff, A. Letessier-Selvon, A. Insolia, M. Kleifges, D. Zavrtanik, P. Ristori, B. Baughmanc, J. Pȩkala, R. Bonino, Lorenzo Cazon, M. Zimbres Silva, I. A. Minaya, J. Stapleton, S. Jansen, H. R. Marquez Falcon, J. Rautenberg, P. Gonçalves, O. Wainberg, A. Porcelli, N. Palmieri, M. Buscemi, Alejandro Almela, S. Jiraskova, Miguel Mostafá, C. Macolino, C. Hojvat, Jan Ebr, S. Messina, L. Caramete, M. Will, D. Huber, Nataliia Borodai, S. van Velzen, A. Menshikov, A. Filip̧cǐc, M. Melissas, A. Curutiu, M. Hrabovsḱy, K. Weidenhaupt, M. D. Rodŕiguez-Fŕias, R. Pesce, M. Gold, O. Tascau, W. C. Brown, B. Caccianiga, H.O. Klages, H. Rivera, W. Tkaczyk, A. Nelles, T. Rossler, J. C. Marin, D. Schuster, H. Schieler, R. Ulrich, Karl-Heinz Kampert, Antonella Castellina, Iván Sidelnik, G. Yuan, A. P. Ferguson, E. Grashorn, S. Riggi, I. Valĩno, H. Cook, Paul Sommers, L. Martin, Lu Lu, P. Brogueira, Marco Cilmo, G. Rodriguez Fernandez, P. Gouffon, A. D. Supanitsky, Hernán Asorey, T. Šuša, B. Keilhauer, P. N. Dong, S. J. Sciutto, M. J. Cooper, F. Ionita, D. Kruppke-Hansen, S. J. De Jong, B. Wundheiler, F. Sánchez, I. Zaw, M. Ambrosio, M. De Domenico, Gregory R Snow, M. Avenier, D. Thomas, J. F. Valdés Galicia, K. H. Becker, P. Hansen, A. Chiavassa, A. E. Herve, I. De Mitri, A. Gascon Bravo, A. Saftoiu, D. Garcia-Gamez, S. T. Garcia Roca, J. R. T. de Mello Neto, M. Blanco, L. R. Wiencke, M. A. Leigui de Oliveira, R. Tcaciuc, L. Latronico, F. Montanet, J. C. dos Anjos, I. M. Pepe, S. Navas, R. A. Vázquez, P. A. Kasper, D. Garcia-Pinto, S. Petrera, Maria Rita Coluccia, H. Schoorlemmer, A. Dorofeev, Guenter Sigl, Bruno Daniel, T. Yapici, P. Allison, A. Tapia, H. Gemmeke, C. E. Fracchiolla, M. Unger, H. Wahlberg, R. Dallier, D. D'Urso, Corinne Berat, M. Giller, M. I. Micheletti, Rúben Conceição, C. Meurer, J. J. Maśias Meza, J. K. Kulbartz, F. Salamida, E. M. Santos, D. Melo, I. Katkov, David Walz, Bruce R. Dawson, Y. N. Srivastava, P.O. Mazur, D. Pakk Selmi-Dei, M. Straub, R. Sato, M. Niechciol, B. Sarkar, J. L. Navarro, M. Videla, F. Salesa Greus, G. Cataldi, Y. Guardincerri, G. Müller, M. Zavrtanik, KVI - Center for Advanced Radiation Technology, Research unit Astroparticle Physics, European Commission, Centro Nacional de Física de Partículas, Astropartículas y Nuclear (España), Laboratoire de l'Accélérateur Linéaire (LAL), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), Laboratoire SUBATECH Nantes (SUBATECH), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université de Nantes (UN)-Mines Nantes (Mines Nantes), Unité Scientifique de la Station de Nançay (USN), Centre National de la Recherche Scientifique (CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire des Sciences de l'Univers en région Centre (OSUC), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS)-Université d'Orléans (UO), Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Joseph Fourier - Grenoble 1 (UJF)-Centre National de la Recherche Scientifique (CNRS), Institut de Physique Nucléaire d'Orsay (IPNO), PIERRE AUGER, P., Abreu, M., Aglietta, M., Ahler, E. J., Ahn, I. F. M., Albuquerque, D., Allard, I., Allekotte, J., Allen, P., Allison, A., Almela, J., Alvarez Castillo, J., Alvarez Muñiz, R., Alves Batista, M., Ambrosio, A., Aminaei, L., Anchordoqui, S., Andringa, T., Antičić, C., Aramo, E., Arganda, F., Arquero, H., Asorey, P., Assi, J., Aublin, M., Ave, M., Avenier, G., Avila, A. M., Badescu, M., Balzer, K. B., Barber, A. F., Barbosa, R., Bardenet, S. L. C., Barroso, B., Baughman f, J., Bäuml, C., Bau, J. J., Beatty, K. H., Becker, A., Bellétoile, J. A., Bellido, S., Benzvi, C., Berat, X., Bertou, P. L., Biermann, P., Billoir, F., Blanco, M., Blanco, C., Bleve, H., Blümer, M., Boháčová, D., Boncioli, C., Bonifazi, R., Bonino, N., Borodai, J., Brack, I., Brancu, P., Brogueira, W. C., Brown, R., Bruijn i, P., Buchholz, A., Bueno, L., Buroker, R. E., Burton, K. S., Caballero Mora, B., Caccianiga, L., Caramete, R., Caruso, A., Castellina, O., Catalano, G., Cataldi, L., Cazon, R., Cester, J., Chauvin, S. H., Cheng, A., Chiavassa, J. A., Chinellato, J., Chirinos Diaz, J., Chudoba, M., Cilmo, R. W., Clay, Cocciolo, Giuseppe, L., Collica, Coluccia, MARIA RITA, R., Conceição, F., Contrera, H., Cook, M. J., Cooper, J., Coppen, A., Cordier, S., Coutu, C. E., Covault, A., Creusot, A., Cri, J., Cronin, A., Curutiu, S., Dagoret Campagne, R., Dallier, B., Daniel, S., Dasso, K., Daumiller, B. R., Dawson, R. M., de Almeida, M., De Domenico, C., De Donato, S. J., de Jong, G., De La Vega, W. J. M., de Mello Junior, J. R. T., de Mello Neto, DE MITRI, Ivan, V., de Souza, K. D., de Vrie, L., del Peral, M., del Río, O., Deligny, H., Dembinski, N., Dhital, C., Di Giulio, M. L., Díaz Castro, P. N., Diep, F., Diogo, C., Dobrigkeit, W., Docter, J. C., D'Olivo, P. N., Dong, A., Dorofeev, J. C., dos Anjo, M. T., Dova, D., D'Urso, I., Dutan, J., Ebr, R., Engel, M., Erdmann, C. O., Escobar, J., Espadanal, A., Etchegoyen, P., Facal San Lui, H., Falcke, K., Fang, G., Farrar, A. C., Fauth, N., Fazzini, A. P., Ferguson, B., Fick, J. M., Figueira, A., Filevich, A., Filipčič, S., Fliescher, C. E., Fracchiolla, E. D., Fraenkel!, O., Fratu, U., Fröhlich, B., Fuch, R., Gaior, R. F., Gamarra, S., Gambetta, B., García, S. T., Garcia Roca, D., Garcia Gamez, D., Garcia Pinto, G., Garilli, A., Gascon Bravo, H., Gemmeke, P. L., Ghia, M., Giller, J., Gitto, H., Gla, M. S., Gold, G., Golup, F., Gomez Albarracin, M., Gómez Berisso, P. F., Gómez Vitale, P., Gonçalve, J. G., Gonzalez, B., Gookin, A., Gorgi, P., Gouffon, E., Grashorn, S., Grebe, N., Griffith, A. F., Grillo, Y., Guardincerri, F., Guarino, G. P., Guede, P., Hansen, D., Harari, T. A., Harrison, J. L., Harton, A., Haung, T., Hebbeker, D., Heck, A. E., Herve, C., Hojvat, N., Hollon, V. C., Holme, P., Homola, J. R., Hörandel, P., Horvath, M., Hrabovský, D., Huber, T., Huege, A., Insolia, F., Ionita, A., Italiano, S., Jansen, C., Jarne, S., Jiraskova, M., Josebachuili, K., Kadija, K. H., Kampert, P., Karhan, P., Kasper, I., Katkov, B., Kégl, B., Keilhauer, A., Keivani, J. L., Kelley, E., Kemp, R. M., Kieckhafer, H. O., Klage, M., Kleifge, J., Kleinfeller, J., Knapp, D. H., Koang, K., Kotera, N., Krohm, O., Krömer, D., Kruppke Hansen, D., Kuempel, J. K., Kulbartz, N., Kunka, G., La Rosa, C., Lachaud, D., Lahurd, L., Latronico, R., Lauer, P., Lautridou, S., Le Coz, M. S. A. B., Leão, D., Lebrun, P., Lebrun, M. A., Leigui de Oliveira, A., Letessier Selvon, I., Lhenry Yvon, K., Link, R., López, A., Lopez Agüera, K., Louedec, J., Lozano Bahilo, L., Lu, A., Lucero, M., Ludwig, H., Lyberi, M. C., Maccarone, C., Macolino, S., Maldera, J., Maller, D., Mandat, P., Mantsch, A. G., Mariazzi, J., Marin, V., Marin, I. C., Mari, H. R., Marquez Falcon, Marsella, Giovanni, Martello, Daniele, L., Martin, H., Martinez, O., Martínez Bravo, D., Martraire, J. J., Masías Meza, H. J., Mathe, J., Matthew, J. A. J., Matthew, G., Matthiae, D., Maurel, D., Maurizio, P. O., Mazur, G., Medina Tanco, M., Melissa, D., Melo, E., Menichetti, A., Menshikov, P., Mertsch, C., Meurer, R., Meyhandan, S., Mićanović, M. I., Micheletti, I. A., Minaya, L., Miramonti, L., Molina Bueno, S., Mollerach, M., Monasor, D., Monnier Ragaigne, F., Montanet, B., Morale, C., Morello, E., Moreno, J. C., Moreno, M., Mostafá, C. A., Moura, M. A., Muller, G., Müller, M., Münchmeyer, R., Mussa, G., Navarra ‡, J. L., Navarro, S., Nava, P., Necesal, L., Nellen, A., Nelle, J., Neuser, P. T., Nhung, M., Niechciol, L., Niemietz, N., Nierstenhoefer, D., Nitz, D., Nosek, L., Nožka, J., Oehlschläger, A., Olinto, M., Ortiz, N., Pacheco, D., Pakk Selmi Dei, M., Palatka, J., Pallotta, N., Palmieri, G., Parente, E., Parizot, A., Parra, S., Pastor, T., Paul, M., Pech, J., Pękala, R., Pelayo, I. M., Pepe, Perrone, Lorenzo, R., Pesce, E., Petermann, S., Petrera, A., Petrolini, Y., Petrov, C., Pfendner, R., Piegaia, T., Pierog, P., Pieroni, M., Pimenta, V., Pirronello, M., Platino, M., Plum, V. H., Ponce, M., Pontz, A., Porcelli, P., Privitera, M., Prouza, E. J., Quel, S., Querchfeld, J., Rautenberg, O., Ravel, D., Ravignani, B., Revenu, J., Ridky, S., Riggi, M., Risse, P., Ristori, H., Rivera, V., Rizi, J., Robert, W., Rodrigues de Carvalho, G., Rodriguez, I., Rodriguez Cabo, J., Rodriguez Martino, J., Rodriguez Rojo, M. D., Rodríguez Fría, G., Ro, J., Rosado, T., Rossler, M., Roth, B., Rouillé d'Orfeuil, E., Roulet, A. C., Rovero, C., Rühle, A., Saftoiu, F., Salamida, H., Salazar, F., Salesa Greu, G., Salina, F., SÃ! ¡nchez, C. E., Santo, E., Santo, E. M., Santo, F., Sarazin, B., Sarkar, S., Sarkar, R., Sato, N., Scharf, Scherini, Viviana, H., Schieler, P., Schiffer, A., Schmidt, O., Scholten, H., Schoorlemmer, J., Schovancova, P., Schovánek, F., Schröder, S., Schulte, D., Schuster, S. J., Sciutto, M., Scuderi, A., Segreto, M., Settimo, A., Shadkam, R. C., Shellard, I., Sidelnik, G., Sigl, H. H., Silva Lopez, O., Sima, A., Śmiałkowski, R., Šmída, G. R., Snow, P., Sommer, J., Sorokin, H., Spinka, R., Squartini, Y. N., Srivastava, S., Stanic, J., Stapleton, J., Stasielak, M., Stephan, A., Stutz, F., Suarez, T., Suomijärvi, A. D., Supanitsky, T., Šuša, M. S., Sutherland, J., Swain, Z., Szadkowski, M., Szuba, A., Tapia, M., Tartare, O., Taşcău, R., Tcaciuc, N. T., Thao, D., Thoma, J., Tiffenberg, C., Timmerman, W., Tkaczyk, C. J., Todero Peixoto, G., Toma, L., Tomankova, B., Tomé, A., Tonachini, P., Travnicek, D. B., Tridapalli, G., Tristram, E., Trovato, M., Tuero, R., Ulrich, M., Unger, M., Urban, J. F., Valdés Galicia, I., Valiño, L., Valore, G., van Aar, A. M., van den Berg, A., van Vliet, E., Varela, B., Vargas Cárdena, J. R., Vázquez, R. A., Vázquez, D., Veberič, V., Verzi, J., Vicha, M., Videla, L., Villaseñor, H., Wahlberg, P., Wahrlich, O., Wainberg, D., Walz, A. A., Watson, M., Weber, K., Weidenhaupt, A., Weindl, F., Werner, S., Westerhoff, B. J., Whelan, A., Widom, G., Wieczorek, L., Wiencke, B., Wilczyńska, H., Wilczyński, M., Will, C., William, T., Winchen, M., Wommer, B., Wundheiler, T., Yamamoto a, T., Yapici, P., Younk, G., Yuan, A., Yushkov, B., Zamorano Garcia, E., Za, D., Zavrtanik, M., Zavrtanik, I., Zaw h, A., Zepeda b, J., Zhou, Y., Zhu, M., Zimbres Silva, M., Ziolkowski, P. Abreu, M. Aglietta, M. Ahler, E.J. Ahn, I.F.M. Albuquerque, D. Allard, I. Allekotte, J. Allen, P. Allison, A. Almela, J. Alvarez Castillo, J. Alvarez-Muñiz, R. Alves Batista, M. Ambrosio, A. Aminaei, L. Anchordoqui, S. Andringa, T. Antičić, C. Aramo, E. Arganda, F. Arquero, H. Asorey, P. Assi, J. Aublin, M. Ave, M. Avenier, G. Avila, A.M. Badescu, M. Balzer, K.B. Barber, A.F. Barbosa, R. Bardenet, S.L.C. Barroso, B. Baughman f, J. Bäuml, C. Bau, J.J. Beatty, K.H. Becker, A. Bellétoile, J.A. Bellido, S. BenZvi, C. Berat, X. Bertou, P.L. Biermann, P. Billoir, F. Blanco, M. Blanco, C. Bleve, H. Blümer, M. Boháčová, D. Boncioli, C. Bonifazi, R. Bonino, N. Borodai, J. Brack, I. Brancu, P. Brogueira, W.C. Brown, R. Bruijn i, P. Buchholz, A. Bueno, L. Buroker, R.E. Burton, K.S. Caballero-Mora, B. Caccianiga, L. Caramete, R. Caruso, A. Castellina, O. Catalano, G. Cataldi, L. Cazon, R. Cester, J. Chauvin, S.H. Cheng, A. Chiavassa, J.A. Chinellato, J. Chirinos Diaz, J. Chudoba, M. Cilmo, R.W. Clay, G. Cocciolo, L. Collica, M.R. Coluccia, R. Conceição, F. Contrera, H. Cook, M.J. Cooper, J. Coppen, A. Cordier, S. Coutu, C.E. Covault, A. Creusot, A. Cri, J. Cronin, A. Curutiu, S. Dagoret-Campagne, R. Dallier, B. Daniel, S. Dasso, K. Daumiller, B.R. Dawson, R.M. de Almeida, M. De Domenico, C. De Donato, S.J. de Jong, G. De La Vega, W.J.M. de Mello Junior, J.R.T. de Mello Neto, I. De Mitri, V. de Souza, K.D. de Vrie, L. del Peral, M. del Río, O. Deligny, H. Dembinski, N. Dhital, C. Di Giulio, M.L. Díaz Castro, P.N. Diep, F. Diogo, C. Dobrigkeit, W. Docter, J.C. D'Olivo, P.N. Dong, A. Dorofeev, J.C. dos Anjo, M.T. Dova, D. D'Urso, I. Dutan, J. Ebr, R. Engel, M. Erdmann, C.O. Escobar, J. Espadanal, A. Etchegoyen, P. Facal San Lui, H. Falcke, K. Fang, G. Farrar, A.C. Fauth, N. Fazzini, A.P. Ferguson, B. Fick, J.M. Figueira, A. Filevich, A. Filipčič, S. Fliescher, C.E. Fracchiolla, E.D. Fraenkel!, O. Fratu, U. Fröhlich, B. Fuch, R. Gaior, R.F. Gamarra, S. Gambetta, B. García, S.T. Garcia Roca, D. Garcia-Gamez, D. Garcia-Pinto, G. Garilli, A. Gascon Bravo, H. Gemmeke, P.L. Ghia, M. Giller, J. Gitto, H. Gla, M.S. Gold, G. Golup, F. Gomez Albarracin, M. Gómez Berisso, P.F. Gómez Vitale, P. Gonçalve, J.G. Gonzalez, B. Gookin, A. Gorgi, P. Gouffon, E. Grashorn, S. Grebe, N. Griffith, A.F. Grillo, Y. Guardincerri, F. Guarino, G.P. Guede, P. Hansen, D. Harari, T.A. Harrison, J.L. Harton, A. Haung, T. Hebbeker, D. Heck, A.E. Herve, C. Hojvat, N. Hollon, V.C. Holme, P. Homola, J.R. Hörandel, P. Horvath, M. Hrabovský, D. Huber, T. Huege, A. Insolia, F. Ionita, A. Italiano, S. Jansen, C. Jarne, S. Jiraskova, M. Josebachuili, K. Kadija, K.H. Kampert, P. Karhan, P. Kasper, I. Katkov, B. Kégl, B. Keilhauer, A. Keivani, J.L. Kelley, E. Kemp, R.M. Kieckhafer, H.O. Klage, M. Kleifge, J. Kleinfeller, J. Knapp, D.-H. Koang, K. Kotera, N. Krohm, O. Krömer, D. Kruppke-Hansen, D. Kuempel, J.K. Kulbartz, N. Kunka, G. La Rosa, C. Lachaud, D. LaHurd, L. Latronico, R. Lauer, P. Lautridou, S. Le Coz, M.S.A.B. Leão, D. Lebrun, P. Lebrun, M.A. Leigui de Oliveira, A. Letessier-Selvon, I. Lhenry-Yvon, K. Link, R. López, A. Lopez Agüera, K. Louedec, J. Lozano Bahilo, L. Lu, A. Lucero, M. Ludwig, H. Lyberi, M.C. Maccarone, C. Macolino, S. Maldera, J. Maller, D. Mandat, P. Mantsch, A.G. Mariazzi, J. Marin, V. Marin, I.C. Mari, H.R. Marquez Falcon, G. Marsella, D. Martello, L. Martin, H. Martinez, O. Martínez Bravo, D. Martraire, J.J. Masías Meza, H.J. Mathe, J. Matthew, J.A.J. Matthew, G. Matthiae, D. Maurel, D. Maurizio, P.O. Mazur, G. Medina-Tanco, M. Melissa, D. Melo, E. Menichetti, A. Menshikov, P. Mertsch, C. Meurer, R. Meyhandan, S. Mićanović, M.I. Micheletti, I.A. Minaya, L. Miramonti, L. Molina-Bueno, S. Mollerach, M. Monasor, D. Monnier Ragaigne, F. Montanet, B. Morale, C. Morello, E. Moreno, J.C. Moreno, M. Mostafá, C.A. Moura, M.A. Muller, G. Müller, M. Münchmeyer, R. Mussa, G. Navarra ‡, J.L. Navarro, S. Nava, P. Necesal, L. Nellen, A. Nelle, J. Neuser, P.T. Nhung, M. Niechciol, L. Niemietz, N. Nierstenhoefer, D. Nitz, D. Nosek, L. Nožka, J. Oehlschläger, A. Olinto, M. Ortiz, N. Pacheco, D. Pakk Selmi-Dei, M. Palatka, J. Pallotta, N. Palmieri, G. Parente, E. Parizot, A. Parra, S. Pastor, T. Paul, M. Pech, J. Pękala, R. Pelayo, I.M. Pepe, L. Perrone, R. Pesce, E. Petermann, S. Petrera, A. Petrolini, Y. Petrov, C. Pfendner, R. Piegaia, T. Pierog, P. Pieroni, M. Pimenta, V. Pirronello, M. Platino, M. Plum, V.H. Ponce, M. Pontz, A. Porcelli, P. Privitera, M. Prouza, E.J. Quel, S. Querchfeld, J. Rautenberg, O. Ravel, D. Ravignani, B. Revenu, J. Ridky, S. Riggi, M. Risse, P. Ristori, H. Rivera, V. Rizi, J. Robert, W. Rodrigues de Carvalho, G. Rodriguez, I. Rodriguez Cabo, J. Rodriguez Martino, J. Rodriguez Rojo, M.D. Rodríguez-Fría, G. Ro, J. Rosado, T. Rossler, M. Roth, B. Rouillé-d'Orfeuil, E. Roulet, A.C. Rovero, C. Rühle, A. Saftoiu, F. Salamida, H. Salazar, F. Salesa Greu, G. Salina, F. SÃ! ¡nchez, C.E. Santo, E. Santo, E.M. Santo, F. Sarazin, B. Sarkar, S. Sarkar, R. Sato, N. Scharf, V. Scherini, H. Schieler, P. Schiffer, A. Schmidt, O. Scholten, H. Schoorlemmer, J. Schovancova, P. Schovánek, F. Schröder, S. Schulte, D. Schuster, S.J. Sciutto, M. Scuderi, A. Segreto, M. Settimo, A. Shadkam, R.C. Shellard, I. Sidelnik, G. Sigl, H.H. Silva Lopez, O. Sima, A. Śmiałkowski, R. Šmída, G.R. Snow, P. Sommer, J. Sorokin, H. Spinka, R. Squartini, Y.N. Srivastava, S. Stanic, J. Stapleton, J. Stasielak, M. Stephan, A. Stutz, F. Suarez, T. Suomijärvi, A.D. Supanitsky, T. Šuša, M.S. Sutherland, J. Swain, Z. Szadkowski, M. Szuba, A. Tapia, M. Tartare, O. Taşcău, R. Tcaciuc, N.T. Thao, D. Thoma, J. Tiffenberg, C. Timmerman, W. Tkaczyk, C.J. Todero Peixoto, G. Toma, L. Tomankova, B. Tomé, A. Tonachini, P. Travnicek, D.B. Tridapalli, G. Tristram, E. Trovato, M. Tuero, R. Ulrich, M. Unger, M. Urban, J.F. Valdés Galicia, I. Valiño, L. Valore, G. van Aar, A.M. van den Berg, A. van Vliet, E. Varela, B. Vargas Cárdena, J.R. Vázquez, R.A. Vázquez, D. Veberič, V. Verzi, J. Vicha, M. Videla, L. Villaseñor, H. Wahlberg, P. Wahrlich, O. Wainberg, D. Walz, A.A. Watson, M. Weber, K. Weidenhaupt, A. Weindl, F. Werner, S. Westerhoff, B.J. Whelan, A. Widom, G. Wieczorek, L. Wiencke, B. Wilczyńska, H. Wilczyński, M. Will, C. William, T. Winchen, M. Wommer, B. Wundheiler, T. Yamamoto a, T. Yapici, P. Younk, G. Yuan, A. Yushkov, B. Zamorano Garcia, E. Za, D. Zavrtanik, M. Zavrtanik, I. Zaw h, A. Zepeda b, J. Zhou, Y. Zhu, M. Zimbres Silva, M. Ziolkowski, Buscemi, Mario, Colalillo, Roberta, Cilmo, Marco, Guarino, Fausto, Valore, Laura, and The Pierre Auger, Collaboration
Subjects: [PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], Ciencias Físicas, Astronomy, Astrophysics::High Energy Astrophysical Phenomena, FOS: Physical sciences, ultra-high energy cosmic rays, Cosmic ray, Astrophysics, ultra high energy cosmic rays, Astrophysics::Cosmology and Extragalactic Astrophysics, 01 natural sciences, Auger, NUMBER, Observatory, Cosmic ray experiments, 0103 physical sciences, ultra-high energy cosmic ray, Ultra-high-energy cosmic ray, 010303 astronomy & astrophysics, DETECTOR, Luminosity function, Pierre Auger Observatory, Physics, High Energy Astrophysical Phenomena (astro-ph.HE), FÍSICA DE PARTÍCULAS, Range (particle radiation), SPECTRUM, Cosmologia, 010308 nuclear & particles physics, [SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], Astronomy and Astrophysics, Ultra high energy cosmic rays, Astronomía, LUMINOSITY FUNCTION, Magnitude (astronomy), Experimental High Energy Physics, ComputingMethodologies_DOCUMENTANDTEXTPROCESSING, Astronomia, Física nuclear, cosmic ray experiments, Astrophysics - High Energy Astrophysical Phenomena, CIENCIAS NATURALES Y EXACTAS
Abstract: We derive lower bounds on the density of sources of ultra-high energy cosmic rays from the lack of significant clustering in the arrival directions of the highest energy events detected at the Pierre Auger Observatory. The density of uniformly distributed sources of equal intrinsic intensity was found to be larger than similar to (0.06 – 5) x 10(-4) Mpc(-3) at 95% CL, depending on the magnitude of the magnetic defections. Similar bounds, in the range (0.2 – 7) x 10(-4) Mpc(-3), were obtained for sources following the local matter distribution., We are very grateful to the following agencies and organizations for financial support,: Comision Nacional de Energia Atomica, Fundacion Antorchas, Gobierno De La, Provincia de Ailendoza. Municipalidad de Malargile. INDM floldings and Valle Las Lenas, in gratitude for their continuing cooperation over land access. Argentina; the Australian Research Council; Conselho Nacional de Desenvolvimento Cientifico e 'Tecnologico (CNPq), Financiadora de Estudos e Projetos (FINEP), Fundacdo de Amparo a Pesquisa do Est ado de Rio de Janeiro (FAP HRJ), Fundacdo de Amparo Pesquisa do Estado de Sdo Paulo (FAPESP), Ministerio de Ciencia e Tecnologia (IVICT), Brazil; AVCR AVOZ10100502 and AVOZ10100522, GAAV KJB100100904, AISMT-CR LA08016, LG11044, 1VIEB111003, MSAI0021620859, LA08015, TACR TA01010517 and GA U.K. 119810, Czech Republic; Centre de Calcul I-N2P3/CNRS, Centre National de la -Recherche Scientifique ((1 NRS), Conseil Regional Ile-de-France, f)epartement, Physique Nuclealre et Corpusculaire (I N( Departement Sciences de l'Univers (SDU-INSU/CNRS), France; Bundesministerium fur Bildung und Forschung (BMBF), Deutsche Forschungsgemeinschaft (DITG), Finanzministerium Baden-Wurttemberg, flelmholtz-Gemeinschaft Deutscher Forschungszentren Ministerium fur Wissenschaft und Forschung, Nordrhein-Westfalen, Ministerimn fur Wissenschaft, Forschung und Kunst, Baden-WUrttemberg, Germany; Istituto Nazion ale di Fisica Nucleare (INFN), Ministero dell'Istruzione, delhLniversita e della Ricerca (MIUR), Italy: Consejo Nacional de Ciencia y Tecnologia (CONACYT), Mexico; Ministerie van Onden s Cultuur on NVetenschap Nederlandse Organisatie voor Wetenschappelijk Onderzoek (NWO), Stichting voor Rmdamenteel Onderzoek der Materie (FOM), Netherlands; Ministry of Science and Higher Education, Grant Nos. N N202 200239 and N N202 207238, Poland; Portuguese national funds and FEDER funds within COMPETE - Programa Operacional Factores de Competitividade through Fundacao para a Ciencia e a Tecnologia, Portugal; Romanian Authority for Scientific Research ANCS, CNDI-UEFISETD1 partnership projects nr.20/2012 and nr.194/2012, project nr.1 /ASPERA2/20I2 ERA-NET and PN-IIRU-PD-2011-3-0145-17, Romania; Ministry for Higher Education, Science, and 'Technology, Slovenian Research Agency, Slovenia; Comunidad de Madrid, FEDER funds, Ministerio de Ciencia e Innovacion and Consolider-Ingenio 2010 (( PAN), X unta de Galicia Spain; Science and Technology Facilities Council, United kingdom; Department of Luergy, Contract Nos. DE-ACO2-07(11-111359, DE-FR02-04E1(41300, DE-FG02-99E1(41107, National Science Foundation, Grant No. 0450696, The Grainger Foundation U.S.A.; NAFOSTED, Vietnam; Marie Curie-IRSES/HPLANET, European Particle Physics Latin American Network, European Union 7th Frarneworlc Program. Grant No. IIRSES-2009-GA-246806; and UNESCO.
Published: 2013
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49. KASCADE-Grande observation of features in the cosmic ray spectrum between knee and ankle

Author: E. Cantoni, M. Ludwig, R. Glasstetter, T. Huege, C. Morello, J. Blümer, S. Ostapchenko, H.J. Gils, T. Pierog, K. Link, H. Bozdog, M. Wommer, J. C. Arteaga-Velázquez, A. Weindl, A. Haungs, D. Kang, M. Petcu, H.O. Klages, M. Finger, G.C. Trinchero, J. Zabierowski, C. Grupen, Jörg R. Hörandel, Ralph Engel, F. Di Pierro, Kai Daumiller, V. de Souza, Markus Roth, F. Cossavella, J. Engler, A. Chiavassa, G. Toma, I.M. Brancus, P. Łuczak, N. Palmieri, D. Fuhrmann, H.J. Mayer, M. Melissas, J. Wochele, Béatrice Fuchs, W. D. Apel, Octavian Sima, D. Huber, J. Oehlschläger, D. Heck, M. E. Bertaina, H. Ulrich, J. Milke, K. Bekk, H. J. Mathes, F.G. Schröder, H. Rebel, S. Schoo, H. Schieler, P. Doll, and K. H. Kampert
Subjects: Physics, History, Elemental composition, Muon, Astronomy, Astrophysics::High Energy Astrophysical Phenomena, Detector, Astrophysics::Instrumentation and Methods for Astrophysics, Cosmic ray, Astrophysics, Charged particle, Computer Science Applications, Education, Nuclear physics, KASCADE, Energy spectrum, ComputingMethodologies_DOCUMENTANDTEXTPROCESSING
Abstract: The detection of high-energy cosmic rays above a few hundred TeV is realized by the observation of extensive air-showers. By using the multi-detector setup of KASCADE-Grande, and here in particular the detectors of the large Grande array, the energy spectrum and the elemental composition of high-energy cosmic rays in the energy range from 10 PeV to 1 EeV are investigated. The estimation of energy and mass of the high-energy primary particles is based on the combined analysis of the total number of charged particles and the total number of muons measured by the detector arrays of Grande and KASCADE, respectively. The latest analysis results have shown that in the all-particle spectrum two features are present: a hardening of the spectrum at energies around 20 PeV and a steepening, i.e. a knee-like structure, at 80-90 PeV. The latter one was found to be due to a decrease of flux of the heavy mass component.
Published: 2013

50. Separation of the light and heavy mass groups of 10 16 – 10 18 eV cosmic rays by studying the ratio muon size to shower size of KASCADE-Grande data

Author: D. Kang, P. Doll, H.O. Klages, J. Blümer, H. Bozdog, M. Finger, Markus Roth, H. Rebel, S. Schoo, F. Di Pierro, M. Ludwig, F. Garino, J. Engler, H. Schieler, G. Toma, Jörg R. Hörandel, C. Morello, K. H. Kampert, S. Ostapchenko, H.J. Gils, D. Huber, A. Chiavassa, V. de Souza, M. Wommer, P. Łuczak, N. Palmieri, M. Melissas, J. Oehlschläger, W. D. Apel, B. Mitrica, E. Cantoni, K. Bekk, F. Cossavella, Béatrice Fuchs, J. C. Arteaga-Velázquez, D. Fuhrmann, Claus Grupen, T. Pierog, G.C. Trinchero, R. Glasstetter, Ralph Engel, H. J. Mathes, F.G. Schröder, J. Wochele, Octavian Sima, A. Weindl, D. Heck, H. Ulrich, T. Huege, M. Petcu, M. E. Bertaina, J. Milke, Kai Daumiller, I.M. Brancus, H.J. Mayer, K. Link, A. Haungs, and J. Zabierowski
Subjects: Physics, History, Range (particle radiation), Muon, Astronomy, Astrophysics::High Energy Astrophysical Phenomena, Astrophysics::Instrumentation and Methods for Astrophysics, Cosmic ray, Charged particle, Spectral line, Computer Science Applications, Education, Atmosphere, Nuclear physics, KASCADE, Observatory, GeneralLiterature_REFERENCE(e.g.,dictionaries,encyclopedias,glossaries)
Abstract: KASCADE-Grande is an air-shower observatory devoted to the study of cosmic rays with energies in the range 1016 – 1018 eV. In KASCADE-Grande, different detector systems allow independent measurements of the number of muons (Nμ) and charged particles (Nch) of air showers, which are the basis for several energy and composition studies of cosmic rays. In this contribution, a composition analysis using the shower size ratio lgNμ/lgNch, corrected for attenuation in the atmosphere, is described. Using QGSJET II-based simulations of different primaries, it is shown that an energy independent cut on the shower ratio can be chosen in order to separate the cosmic ray events into light and heavy mass groups. The analysis is applied to the KASCADE-Grande data. The energy spectra derived from the analysis are presented.
Published: 2013

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