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1. 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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2. Summary of the main results of the KASCADE and KASCADE-Grande experiments

Author: H. J. Mathes, Claus Grupen, F.G. Schröder, H. Rebel, S. Schoo, H. Schieler, J. Oehlschläger, E. Cantoni, W. D. Apel, A. Weindl, M. E. Bertaina, T. Pierog, J. Milke, K. Bekk, A. Chiavassa, G. Toma, P. Łuczak, B. Mitrica, N. Palmieri, D. Fuhrmann, H.J. Mayer, K. Link, K. H. Kampert, H. Bozdog, A. Haungs, V. de Souza, Alexandru Gherghel-Lascu, H.J. Gils, C. Morello, Jörg R. Hörandel, Ralph Engel, R. Glasstetter, J. Blümer, S. Ostapchenko, P. Doll, F. Cossavella, D. Huber, T. Huege, I.M. Brancus, H. Ulrich, J. Wochele, Octavian Sima, G.C. Trinchero, D. Heck, D. Kang, H.O. Klages, F. Di Pierro, J.C. Arteaga-Velázquez, Kai Daumiller, J. Zabierowski, and Markus Roth
Subjects: Physics, Elemental composition, Range (particle radiation), QC1-999, Astronomy, Hadron, Cosmic ray, 01 natural sciences, Nuclear physics, KASCADE, 0103 physical sciences, ddc:530, 010306 general physics, 010303 astronomy & astrophysics
Abstract: The KASCADE and KASCADE-Grande experiments operated in KIT-Campus North, Karlsruhe (Germany) from 1993 to 2012. The two experiments studied primary cosmic rays in the energy range from 1014 eV to 1018 eV, investigating the change of slope of the spectrum detected at 2 - 4 × 1015 eV, the so called knee. We briefly review the performance of the experiments and then the main results obtained in the operation of both experiments: the test of hadronic interaction models, the all particle primary spectrum, the elemental composition of primary cosmic rays (with the first claim of a knee-like feature of the heavy primaries spectrum) and the search for large scale anisotropies.
Published: 2019

3. The KASCADE Cosmic-ray Data Centre KCDC: granting open access to astroparticle physics research data

Author: J.C. Arteaga-Velázquez, H. J. Mathes, Alexandru Gherghel-Lascu, Kai Daumiller, F.G. Schröder, Jörg R. Hörandel, T. Huege, C. Morello, H. Rebel, S. Schoo, B. Mitrica, V. de Souza, E. Cantoni, G. Toma, H. Ulrich, J. Wochele, A. Chiavassa, Octavian Sima, D. Fuhrmann, H.J. Gils, D. Heck, H. Schieler, Karl-Heinz Kampert, T. Pierog, G.C. Trinchero, J. Oehlschläger, D. Wochele, F. Di Pierro, H. Bozdog, D. Kang, H.O. Klages, B. Fuchs, C. Grupen, P. Łuczak, J. Milke, K. Link, M. E. Bertaina, F. Cossavella, A. Weindl, P. Doll, J. Zabierowski, K. Bekk, I.M. Brancus, J. Blümer, H.J. Mayer, M. Petcu, S. Ostapchenko, Markus Roth, R. Glasstetter, Andreas Haungs, Ralph Engel, and W. D. Apel
Subjects: Physics and Astronomy (miscellaneous), Astronomy, Big data, FOS: Physical sciences, lcsh:Astrophysics, Cosmic ray, 01 natural sciences, Documentation, Data acquisition, lcsh:QB460-466, 0103 physical sciences, lcsh:Nuclear and particle physics. Atomic energy. Radioactivity, ddc:530, Engineering (miscellaneous), 010303 astronomy & astrophysics, Instrumentation and Methods for Astrophysics (astro-ph.IM), Astroparticle physics, Physics, High Energy Astrophysical Phenomena (astro-ph.HE), 010308 nuclear & particles physics, business.industry, ASTROFÍSICA, Physik (inkl. Astronomie), Data science, Metadata, KASCADE, lcsh:QC770-798, Data center, Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - High Energy Astrophysical Phenomena, business
Abstract: The `KASCADE Cosmic ray Data Centre' is a web portal (\url{https://kcdc.ikp.kit.edu}), where the data of the astroparticle physics experiment KASCADE-Grande are made available for the interested public. The KASCADE experiment was a large-area detector for the measurement of high-energy cosmic rays via the detection of extensive air showers. The multi-detector installations KASCADE and its extension KASCADE-Grande stopped the active data acquisition in 2013 of all its components end of 2012 after more than 20 years of data taking. In several updates since our first release in 2013 with KCDC we provide the public measured and reconstructed parameters of more than 433 million air showers. In addition, KCDC provides meta data information and documentation to enable a user outside the community of experts to perform their own data analysis. Simulation data from three different high energy interaction models have been made available as well as a compilation of measured and published spectra from various experiments. In addition, detailed educational examples shall encourage high-school students and early stage researchers to learn about astroparticle physics, cosmic radiation as well as the handling of Big Data and about the sustainable and public provision of scientific data., Comment: 16 pages, submitted to The European Physical Journal C
Published: 2018

4. Muon density measurements for the light and heavy mass groups of cosmic rays at the KASCADE-Grande observatory

Author: H. Bozdog, E. Cantoni, A. Weindl, M. E. Bertaina, J. Milke, S. Ostapchenko, H. J. Mathes, Claus Grupen, K. Bekk, J. C. Arteaga-Velázquez, T. Pierog, F.G. Schröder, P. Łuczak, D. Kang, H.O. Klages, J. Blümer, Ralph Engel, J. Oehlschläger, Markus Roth, H.J. Gils, G.C. Trinchero, V. de Souza, Kai Daumiller, D. Fuhrmann, G. Toma, Jörg R. Hörandel, C. Morello, B. Mitrica, R. Glasstetter, F. Cossavella, T. Huege, F. Di Pierro, K. H. Kampert, P. Doll, W. D. Apel, H. Rebel, S. Schoo, H. Schieler, Alexandru Gherghel-Lascu, A. Chiavassa, H.J. Mayer, K. Link, A. Haungs, J. Zabierowski, I.M. Brancus, J. Wochele, Octavian Sima, D. Heck, and H. Ulrich
Subjects: Physics, Nuclear and High Energy Physics, Particle physics, Muon, Physics::Instrumentation and Detectors, 010308 nuclear & particles physics, Astrophysics::High Energy Astrophysical Phenomena, Detector, Astrophysics::Instrumentation and Methods for Astrophysics, Cosmic ray, Physik (inkl. Astronomie), 01 natural sciences, Charged particle, Nuclear physics, KASCADE, Observatory, 0103 physical sciences, 010303 astronomy & astrophysics, Zenith
Abstract: KASCADE-Grande was an air-shower experiment aimed to investigate cosmic rays between 1016 and 1018 eV. The instrument was located at the site of the Karlsruhe Institute of Technology, Germany at an altitude of 110 m a.s.l. and covered an area of 0.5 km2. KASCADE-Grande consisted of several detector systems dedicated to measure different components of the cosmic ray induced air showers, e.g. the muon content (Eth > 230 MeV) and the number of charged particles (Eth > 3 MeV) at ground, which are the basis for several energy and composition studies of cosmic rays. In this contribution, using these observables, the KASCADE-Grande data is divided into light and heavy mass groups and their respective muon densities are reconstructed at different zenith angle intervals. The results are compared with the expectations of the post-LHC hadronic-interaction models, EPOS-LHC and QGSJET-II-04, in order to test the validity of the model predictions.
Published: 2017

5. Probing the evolution of the EAS muon content in the atmosphere with KASCADE-Grande

Author: A. Chiavassa, Alexandru Gherghel-Lascu, H.J. Gils, I.M. Brancus, F. Di Pierro, D. Fuhrmann, B. Mitrica, G. Toma, H. Bozdog, F. Cossavella, C. Morello, D. Kang, H.O. Klages, V. de Souza, M. E. Bertaina, E. Cantoni, J. Milke, K. Link, J. Zabierowski, Andreas Haungs, P. Łuczak, H.J. Mayer, J. Blümer, T. Pierog, R. Glasstetter, H. Ulrich, J. Wochele, Octavian Sima, A. Weindl, D. Heck, H. Rebel, S. Schoo, H. Schieler, Ralph Engel, Karl-Heinz Kampert, P. Doll, W. D. Apel, S. Ostapchenko, J. Oehlschläger, Jörg R. Hörandel, G.C. Trinchero, Claus Grupen, Markus Roth, T. Huege, J.C. Arteaga-Velázquez, Kai Daumiller, H. J. Mathes, F.G. Schröder, and K. Bekk
Subjects: Particle physics, Physics::Instrumentation and Detectors, Astronomy, Astrophysics::High Energy Astrophysical Phenomena, FOS: Physical sciences, Cosmic ray, Hadronic interaction models, 01 natural sciences, KASCADE-Grande, Nuclear physics, Atmosphere, Maschinenbau, Observatory, 0103 physical sciences, Extensive air showers, 010306 general physics, Cosmic rays, Zenith, High Energy Astrophysical Phenomena (astro-ph.HE), Physics, Muon, 010308 nuclear & particles physics, Attenuation length, Muon component, Astronomy and Astrophysics, Attenuation, ASTROFÍSICA, KASCADE, High Energy Physics::Experiment, Astrophysics - High Energy Astrophysical Phenomena
Abstract: The evolution of the muon content of very high energy air showers (EAS) in the atmosphere is investigated with data of the KASCADE-Grande observatory. For this purpose, the muon attenuation length in the atmosphere is obtained to $\Lambda_\mu = 1256 \, \pm 85 \, ^{+229}_{-232}(\mbox{syst})\, \mbox{g/cm}^2$ from the experimental data for shower energies between $10^{16.3}$ and $10^{17.0} \, \mbox{eV}$. Comparison of this quantity with predictions of the high-energy hadronic interaction models QGSJET-II-02, SIBYLL 2.1, QGSJET-II-04 and EPOS-LHC reveals that the attenuation of the muon content of measured EAS in the atmosphere is lower than predicted. Deviations are, however, less significant with the post-LHC models. The presence of such deviations seems to be related to a difference between the simulated and the measured zenith angle evolutions of the lateral muon density distributions of EAS, which also causes a discrepancy between the measured absorption lengths of the density of shower muons and the predicted ones at large distances from the EAS core. The studied deficiencies show that all four considered hadronic interaction models fail to describe consistently the zenith angle evolution of the muon content of EAS in the aforesaid energy regime., Comment: Published in Astroparticle Physics 95 (2017) 25-43
Published: 2017

6. Recent results from the KASCADE-Grande data analysis

Author: K. Link, T. Huege, A. Haungs, P. Łuczak, N. Palmieri, J. Oehlschläger, H. Rebel, Markus Roth, Claus Grupen, S. Schoo, S. Ostapchenko, H. Schieler, A. Weindl, H. Bozdog, F. Cossavella, H. J. Mathes, A. Chiavassa, R. Glasstetter, C. Morello, M. E. Bertaina, J. Blümer, P. Doll, H. Ulrich, J. Milke, Jörg R. Hörandel, V. de Souza, B. Mitrica, J.C. Arteaga-Velázquez, F.G. Schröder, K. Bekk, F. Di Pierro, H.J. Gils, I.M. Brancus, Kai Daumiller, W. D. Apel, D. Huber, D. Kang, H.O. Klages, J. Wochele, J. Zabierowski, K. H. Kampert, Alexandru Gherghel-Lascu, Octavian Sima, E. Cantoni, H.J. Mayer, G.C. Trinchero, D. Heck, Ralph Engel, T. Pierog, D. Fuhrmann, and G. Toma
Subjects: Physics, Data collection, 010308 nuclear & particles physics, Astronomy, Astrophysics::High Energy Astrophysical Phenomena, QC1-999, Gamma ray, Astrophysics::Instrumentation and Methods for Astrophysics, Cosmic ray, 01 natural sciences, Nuclear physics, KASCADE, 0103 physical sciences, ddc:530, 010306 general physics
Abstract: KASCADE, together with its extension KASCADE-Grande measured individual air showers of cosmic rays in the primary energy range of 100 TeV to 1 EeV. The data collection was fully completed at the end of 2013 and the experiment was dismantled. However, the data analysis is still in progress. Recently, we published a new result on upper limits to the flux of ultra-high energy gamma rays, which set constraints on some fundamental astrophysical models. We also use the data to investigate the validity of the new hadronic interactions models like SIBYLL version 2.3c or EPOS-LHC. In addition, we updated and improved the webbased platform of the KASCADE Cosmic Ray Data Centre (KCDC), where now the data from KASCADE and KASCADE-Grande of more than 20 years measurements is available, including corresponding Monte-Carlo simulated events based on three different hadronic interaction models. In this contribution, recent results from KASCADE-Grande and the update of KCDC is briefly discussed.
Published: 2019
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7. Study of themuon content of high-energy air showers with KASCADE-Grande

Author: A. Chiavassa, J. Blümer, C. Morello, T. Huege, A. Weindl, H. Bozdog, D. Rivera-Rangel, V. de Souza, Claus Grupen, Jörg R. Hörandel, E. Cantoni, D. Kang, H.O. Klages, Kai Daumiller, T. Pierog, Alexandru Gherghel-Lascu, Markus Roth, J. Oehlschläger, J. C. Arteaga-Velázquez, P. Łuczak, G.C. Trinchero, F. Di Pierro, K. Bekk, H. J. Mathes, F.G. Schröder, I.M. Brancus, R. Glasstetter, G. Toma, J. Wochele, Octavian Sima, K. H. Kampert, D. Heck, H.J. Gils, H.J. Mayer, P. Doll, K. Link, A. Haungs, J. Zabierowski, D. Fuhrmann, M. E. Bertaina, H. Rebel, J. Milke, F. Cossavella, S. Schoo, W. D. Apel, H. Schieler, S. Ostapchenko, Ralph Engel, H. Ulrich, and B. Mitrica
Subjects: Physics, Technology, Muon, 010308 nuclear & particles physics, Physics::Instrumentation and Detectors, Astronomy, Astrophysics::High Energy Astrophysical Phenomena, QC1-999, Hadron, Attenuation length, Astrophysics::Instrumentation and Methods for Astrophysics, Cosmic ray, 01 natural sciences, Charged particle, Nuclear physics, Shower, KASCADE, 0103 physical sciences, High Energy Physics::Experiment, 010306 general physics, ddc:600, Zenith
Abstract: In this work, we report measurements on the muon content (Eth > 230 MeV) of extensive air showers (EAS) induced by cosmic rays with primary energy from 10 PeV up to 1 EeV performed with the KASCADE-Grande experiment. The measurements are confronted with SIBYLL 2.3. The results are focused on the dependence of the total muon number and the lateral density distribution of muons in EAS on the zenith angle and the total number of charged particles in the shower. We also present updated results of a detailed study of the attenuation length of shower muons, which reveal a deviation between the measured data and the predictions of the post-LHC hadronic interaction models SIBYLL 2.3, QGSJET-II-04 and EPOS-LHC.
Published: 2019

8. Tests of the SIBYLL 2.3 high-energy hadronic interaction model using the KASCADE-Grande muon data

Author: H. Rebel, J. Wochele, S. Schoo, P. Łuczak, Octavian Sima, Markus Roth, H. Schieler, H. Bozdog, G. Toma, D. Heck, J. Blümer, W. D. Apel, F. Cossavella, Alexandru Gherghel-Lascu, B. Mitrica, K. Bekk, G.C. Trinchero, Ralph Engel, H.J. Mayer, K. H. Kampert, D. Kang, H.O. Klages, Jörg R. Hörandel, D. Fuhrmann, C. Morello, H. Ulrich, P. Doll, A. Weindl, H.J. Gils, M. E. Bertaina, D. Rivera-Rangel, A. Chiavassa, J. Milke, Claus Grupen, K. Link, A. Haungs, J. Zabierowski, I.M. Brancus, H. J. Mathes, F.G. Schröder, V. de Souza, E. Cantoni, F. Di Pierro, T. Pierog, T. Huege, J. Oehlschläger, J.C. Arteaga-Velázquez, Kai Daumiller, R. Glasstetter, and S. Ostapchenko
Subjects: Physics, Muon, 010308 nuclear & particles physics, Physics::Instrumentation and Detectors, Astrophysics::High Energy Astrophysical Phenomena, QC1-999, Attenuation length, Astrophysics::Instrumentation and Methods for Astrophysics, Cosmic ray, 01 natural sciences, Charged particle, Nuclear physics, Air shower, KASCADE, Maschinenbau, Observatory, 0103 physical sciences, ddc:530, High Energy Physics::Experiment, 010306 general physics, Zenith
Abstract: The KASCADE-Grande observatory was a ground-based air shower array dedicated to study the energy and composition of cosmic rays in the energy interval E = 1 PeV –1 EeV. The experiment consisted of different detector systems which allowed the simultaneous measurement of distinct components of air showers (EAS), such as the muon content. In this contribution, we study the total muon number and the lateral density distribution of muons in EAS detected by KASCADE-Grande as a function of the zenith angle and the total number of charged particles. The attenuation length of the muon content of EAS is also measured. The results are compared with the predictions of the SIBYLL 2.3 high-energy hadronic interaction model.
Published: 2018

9. Cosmic Ray Physics with the KASCADE-Grande Observatory

Author: D. Kang, H.O. Klages, H. J. Mathes, Alexandru Gherghel-Lascu, H.J. Gils, H. Ulrich, R. Glasstetter, P. Doll, J.C. Arteaga-Velázquez, Jörg R. Hörandel, F.G. Schröder, K. Bekk, Kai Daumiller, V. de Souza, A. Chiavassa, J. Blümer, E. Cantoni, J. Wochele, F. Cossavella, Octavian Sima, H. Rebel, G.C. Trinchero, F. Di Pierro, D. Heck, T. Pierog, H. Bozdog, S. Schoo, H. Schieler, J. Oehlschläger, Ralph Engel, T. Huege, Markus Roth, S. Ostapchenko, K. H. Kampert, W. D. Apel, A. Weindl, C. Morello, I.M. Brancus, B. Mitrica, H.J. Mayer, D. Fuhrmann, M. E. Bertaina, J. Milke, K. Link, A. Haungs, J. Zabierowski, Claus Grupen, P. Łuczak, G. Toma, and Kawata, K.
Subjects: Physics, KASCADE, Observatory, Astronomy, JPS Conference Proceedings, Flux, Cosmic ray, GeneralLiterature_REFERENCE(e.g.,dictionaries,encyclopedias,glossaries)
Abstract: Contains fulltext : 184360.pdf (Publisher’s version ) (Open Access)
Published: 2018

10. Lateral distributions of EAS muons (Eμ>800 MeV) measured with the KASCADE-Grande Muon Tracking Detector in the primary energy range 1016–1017eV

Author: A. Chiavassa, Markus Roth, J. Engler, F. Cossavella, P. Łuczak, N. Palmieri, M. Petcu, M. E. Bertaina, K. H. Kampert, J. Milke, K. Link, H. Rebel, Alexandru Gherghel-Lascu, J. Oehlschläger, A. Haungs, F. Di Pierro, G. Toma, S. Ostapchenko, S. Schoo, J. Zabierowski, H. Schieler, W. D. Apel, H.J. Gils, K. Bekk, P. Doll, B. Fuchs, H. J. Mathes, B. Mitrica, Ralph Engel, J. Blümer, T. Huege, F.G. Schröder, Claus Grupen, R. Glasstetter, D. Kang, H.J. Mayer, H.O. Klages, I.M. Brancus, G. C. Trinchero, Kai Daumiller, D. Huber, D. Fuhrmann, V. de Souza, H. Bozdog, E. Cantoni, T. Pierog, H. Ulrich, J. Wochele, Octavian Sima, D. Heck, C. Morello, A. Weindl, Jörg R. Hörandel, and J. C. Arteaga-Velázquez
Subjects: Physics, Muon, Physics::Instrumentation and Detectors, Astrophysics::High Energy Astrophysical Phenomena, Detector, Astrophysics::Instrumentation and Methods for Astrophysics, Astronomy and Astrophysics, Cosmic ray, Scintillator, Tracking (particle physics), Nuclear physics, KASCADE, Scintillation counter, High Energy Physics::Experiment, Zenith
Abstract: The KASCADE-Grande large area (128 m2) Muon Tracking Detector has been built with the aim to identify muons ( E μ thr = 800 MeV) in Extensive Air Showers by track measurements under 18 r.l. shielding. This detector provides high-accuracy angular information (approx. 0.3 ° ) for muons up to 700 m distance from the shower core. In this work we present the lateral density distributions of muons in EAS measured with the Muon Tracking Detector of the KASCADE-Grande experiment. The density is calculated by counting muon tracks in a muon-to-shower-axis distance range from 100 m to 610 m from showers with reconstructed energy of 10 16 – 10 17 eV and zenith angle θ 18 ° . In the distance range covered by the experiment, these distributions are well described by functions phenomenologically determined already in the fifties (of the last century) by Greisen. They are compared also with the distributions obtained with the KASCADE scintillator array ( E μ thr = 230 MeV) and with distributions obtained using simulated showers.
Published: 2015

11. KASCADE-Grande Limits on the Isotropic Diffuse Gamma-Ray Flux between 100 TeV and 1 EeV

Author: J. Wochele, Octavian Sima, H. J. Mathes, Alexandru Gherghel-Lascu, E. Cantoni, K. Bekk, D. Heck, W. D. Apel, F.G. Schröder, T. Pierog, G. Toma, P. Łuczak, Jörg R. Hörandel, P. Doll, H. Bozdog, Claus Grupen, M. E. Bertaina, F. Cossavella, Ralph Engel, H.J. Mayer, A. Chiavassa, Z. Feng, F. Di Pierro, K. Link, A. Haungs, H.J. Gils, C. Morello, I.M. Brancus, J. Zabierowski, H. Ulrich, B. Mitrica, R. Glasstetter, S. Ostapchenko, Markus Roth, V. de Souza, J. Blümer, J. Milke, G.C. Trinchero, D. Fuhrmann, K. H. Kampert, H. Rebel, S. Schoo, H. Schieler, D. Kang, H.O. Klages, A. Weindl, J. Oehlschläger, J.C. Arteaga-Velázquez, Kai Daumiller, and T. Huege
Subjects: Physics::Instrumentation and Detectors, Astronomy, Astrophysics::High Energy Astrophysical Phenomena, Flux, FOS: Physical sciences, Cosmic ray, 01 natural sciences, cosmic rays, gamma rays: diffuse background, Astronomy and Astrophysics, Space and Planetary Science, Nuclear physics, 0103 physical sciences, 010303 astronomy & astrophysics, Physics, High Energy Astrophysical Phenomena (astro-ph.HE), Muon, 010308 nuclear & particles physics, Isotropy, Gamma ray, Astrophysics::Instrumentation and Methods for Astrophysics, ASTROFÍSICA, Physik (inkl. Astronomie), KASCADE, ComputingMethodologies_DOCUMENTANDTEXTPROCESSING, Astrophysics - High Energy Astrophysical Phenomena
Abstract: KASCADE and KASCADE-Grande were multi-detector installations to measure individual air showers of cosmic rays at ultra-high energy. Based on data sets measured by KASCADE and KASCADE-Grande, 90% C.L. upper limits to the flux of gamma-rays in the primary cosmic ray flux are determined in an energy range of ${10}^{14} - {10}^{18}$ eV. The analysis is performed by selecting air showers with a low muon content as expected for gamma-ray-induced showers compared to air showers induced by energetic nuclei. The best upper limit of the fraction of gamma-rays to the total cosmic ray flux is obtained at $3.7 \times {10}^{15}$ eV with $1.1 \times {10}^{-5}$. Translated to an absolute gamma-ray flux this sets constraints on some fundamental astrophysical models, such as the distance of sources for at least one of the IceCube neutrino excess models., Published in The Astrophysical Journal, Volume 848, Number 1. Posted on: October 5, 2017
Published: 2017

12. Latest Results of KASCADE-Grande

Author: J. Wochele, H. Bozdog, S. Schoo, J. Oehlschläger, D. Heck, K.Y. Oyulmaz, H. J. Mathes, Octavian Sima, H. Schieler, H.J. Gils, K. Link, T. Pierog, Markus Roth, A. Haungs, K. Bekk, A. Weindl, K. H. Kampert, J. Blümer, Alexandru Gherghel-Lascu, F. Di Pierro, D. Fuhrmann, Kai Daumiller, J. Zabierowski, F. Cossavella, B. Mitrica, V. de Souza, E. Cantoni, T. Huege, P. Doll, H. Rebel, G. Toma, P. Łuczak, H.J. Mayer, N. Palmieri, Andrea Chiavassa, I.M. Brancus, M. E. Bertaina, H. Ulrich, G. C. Trinchero, D. Huber, J. Milke, Frank G. Schröder, J.R. Hörandel, W. D. Apel, D. Kang, J. C. Arteaga-Velázquez, H.O. Klages, R. Engel, Claus Grupen, S. Ostapchenko, C. Morello, and R. Glasstetter
Subjects: Nuclear physics, Physics, Data set, KASCADE, Astrophysics::High Energy Astrophysical Phenomena, High Energy Physics::Phenomenology, Energy spectrum, Astrophysics::Instrumentation and Methods for Astrophysics, Cosmic ray
Abstract: The KASCADE-Grande experiment has significantly contributed to the current knowledge about the energy spectrum and composition of cosmic rays for energies between the knee and the ankle. Meanwhile, post-LHC versions of the hadronic interaction models are available and used to interpret the entire data set of KASCADE-Grande. A new, combined analysis of both arrays, KASCADE and Grande, were developed increasing significantly the accuracy of the shower observables. Latest results from the analysis of the entire data set as well as recent activities related to scientific outreach of the KASCADE-Grande experiment are presented.
Published: 2017

13. Measurements of the muon content of EAS in KASCADE-Grande compared with SIBYLL 2.3 predictions

Author: J. Oehlschläger, K. Bekk, B. Mitrica, C. Morello, P. Łuczak, D. Rivera-Rangel, N. Palmieri, A. Weindl, K. Link, T. Pierog, A. Haungs, Alexandru Gherghel-Lascu, H.J. Gils, J. Zabierowski, R. Engel, Claus Grupen, Kai Daumiller, T. Huege, G. C. Trinchero, Juan Carlos Arteaga-Velázquez, Emilio Chiavassa, H.J. Mayer, D. Kang, H.O. Klages, D. Huber, Frank G. Schröder, M. E. Bertaina, H. Ulrich, F. Cossavella, F. Di Pierro, H. Rebel, D. Fuhrmann, H. Bozdog, R. Glasstetter, Vitor de Souza, H. J. Mathes, J. Blümer, J. Wochele, D. Heck, G. Toma, I.M. Brancus, S. Ostapchenko, E. Cantoni, J. Milke, W. D. Apel, P. Doll, Markus Roth, J.R. Hörandel, S. Schoo, Octavian Sima, H. Schieler, and K. H. Kampert
Subjects: Physics, Muon, Physics::Instrumentation and Detectors, Astrophysics::High Energy Astrophysical Phenomena, Astrophysics::Instrumentation and Methods for Astrophysics, Attenuation length, Cosmic ray, Charged particle, Nuclear physics, Air shower, KASCADE, Observatory, High Energy Physics::Experiment, Zenith
Abstract: The KASCADE-Grande observatory was a ground-based air shower array devoted to the study of the energy and composition of cosmic rays with energies from $1$ PeV to $1$ EeV. The experiment consisted of different detector systems which allowed the simultaneous measurement of distinct components of the air showers (EAS), such as the muon content. In this contribution, we study the total muon number and the lateral density distribution of muons in EAS detected by KASCADE-Grande. The data are analyzed as a function of the zenith angle and the total number of charged particles. The attenuation length of the muon content of EAS is also measured. The results are compared with the predictions of the SIBYLL $2.3$ hadronic interaction model.
Published: 2017

14. A new analysis of the combined data from both KASCADE and KASCADE-Grande

Author: H. Bozdog, S. Ostapchenko, R. Engel, H. Rebel, M. E. Bertaina, G. C. Trinchero, Claus Grupen, J. Milke, E. Cantoni, H. J. Mathes, K. Link, S. Schoo, Octavian Sima, A. Haungs, J.R. Hörandel, D. Kang, P. Łuczak, N. Palmieri, H. Schieler, H.O. Klages, J. Zabierowski, F. Di Pierro, F. Cossavella, A. Weindl, D. Fuhrmann, Alexandru Gherghel-Lascu, I.M. Brancus, K. H. Kampert, Markus Roth, K. Bekk, C. Morello, J. Oehlschläger, B. Mitrica, T. Pierog, H.J. Mayer, Andrea Chiavassa, H.J. Gils, P. Doll, W. D. Apel, T. Huege, J. C. Arteaga-Velázquez, D. Huber, Frank G. Schröder, Kai Daumiller, J. Blümer, Vitor de Souza, R. Glasstetter, J. Wochele, D. Heck, H. Ulrich, and G. Toma
Subjects: Nuclear physics, Physics, KASCADE, Astrophysics::High Energy Astrophysical Phenomena, Detector, Astrophysics::Instrumentation and Methods for Astrophysics, Cosmic ray
Abstract: KASCADE and KASCADE-Grande were detector arrays for the measurement of extensive air showers generated by high-energy cosmic rays in the PeV to EeV energy range. KASCADE-Grande has been operated for more than two decades and completed the data taking at the end of 2013. Now, a new analysis of the combined data from the arrays of KASCADE and KASCADE-Grande was performed, increasing both the effective area and the accuracy of the shower reconstruction. In addition, new versions of post-LHC hadronic interaction models are used to interpret the combined data. First results from the new combined analysis confirming earlier observations of spectral features, but also unveiling still existing inconsistencies of the models, will be discussed in this contribution.
Published: 2017

15. A new release of the KASCADE Cosmic Ray Data Centre (KCDC)

Author: K. Link, A. Haungs, D. Wochele, H. Bozdog, B. Mitrica, J. Zabierowski, J. Blümer, K. H. Kampert, J. C. Arteaga-Velázquez, J. Oehlschläger, Kai Daumiller, F. Di Pierro, G. Toma, Alexandru Gherghel-Lascu, C. Morello, I.M. Brancus, D. Huber, H.J. Mayer, Andrea Chiavassa, P. Doll, Frank G. Schröder, W. D. Apel, K. Bekk, H.J. Gils, A. Weindl, M. E. Bertaina, Andreas Haungs, J. Milke, Dieter Heck, S. Schoo, T. Huege, Octavian Sima, T. Pierog, H. Schieler, D. Fuhrmann, Markus Roth, F. Cossavella, Vitor de Souza, G. C. Trinchero, R. Glasstetter, E. Cantoni, P. Łuczak, N. Palmieri, J.R. Hörandel, S. Ostapchenko, R. Engel, H. J. Mathes, D. Kang, H.O. Klages, H. Rebel, J. Wochele, Claus Grupen, and H. Ulrich
Subjects: Astroparticle physics, Information retrieval, Software, KASCADE, Computer science, business.industry, Cosmic ray, Data center, Detector array, business, Data availability, Original data
Abstract: The KASCADE Cosmic Ray Data Centre (KCDC) is a web-based platform to provide scientific data for the general public. KASCADE and its extension KASCADE-Grande fully completed the data accumulation at the end of 2013 after more than 20 years of measurements. The main purpose of KCDC is to archive original data such as from KASCADE to offer long-term scientific data for the high-energy astroparticle physics community as well as for students and the interested public via a sophisticated web portal. Recently, a new version named NABOO was released, based on a completely new back-end database and software. In addition, the amount of data increased by factor 3 compared to the previous release. Data from the Grande detector array are now also available. In this contribution, the KCDC web portal and the data availability as well as future plans will be discussed.
Published: 2017

16. Astrophysical interpretation of Pierre Auger Observatory measurements of the UHECR energy spectrum and mass composition

Author: R. Conceição, Miroslav Hrabovský, A. Haungs, J. L. Harton, S. G. Blaess, P. Mantsch, Z. Szadkowski, Carola Dobrigkeit, M. Plum, M. E. Bertaina, Alan Watson, Mihai Niculescu-Oglinzanu, J. Alvarez Castillo, F. Diogo, M. Zavrtanik, R. M. de Almeida, D. Reinert, Stijn Buitink, Andrea Chiavassa, M. Malacari, C. Scarso, P. Heimann, Andrej Filipcic, M. Suarez Durán, L. Lopes, E. Kemp, Serguei Vorobiov, L. Molina-Bueno, D. Melo, D. Nitz, M. Settimo, Hernan Wahlberg, David Walz, O. A. Taborda, R. Squartini, R. R. Prado, D. Pakk Selmi-Dei, Petr Schovanek, M. T. Dova, Radomir Smida, J.E. Swain, R. Sato, G. Torralba Elipe, E.M. Holt, L. R. Wiencke, R. Krause, P. Ristori, O. Kambeitz, A. Saleh, M. Gómez Berisso, R. C. Shellard, Ph. Lebrun, Denis Stanca, Olivier Ravel, S. Jansen, A. Fuster, M. Trini, Alejandro Almela, G. Cataldi, E. Varela, J.D. Sanabria Gomez, L. Valore, P.H. Nguyen, E. Mayotte, M. Ambrosio, V. Scherini, A. Śmiałkowski, Philipp Papenbreer, G. Medina-Tanco, David Wittkowski, A. C. Rovero, Lili Yang, G. van Aar, Alexandra Saftoiu, J.R. Hörandel, Mario Buscemi, Sarka Wykes, Stefan Müller, Alexandru Balaceanu, I. Jandt, Ana Martina Botti, Manuela Mallamaci, Jaime Alvarez-Muñiz, Alexandru Gherghel-Lascu, Piotr Homola, R. Ramos-Pollant, Carla Aramo, Vincenzo Rizi, D. Martello, Ralf Ulrich, A. Bridgeman, Muller, B. Caccianiga, I. Allekotte, M. Ziolkowski, Silvia Mollerach, W. R. de Carvalho, O. Martínez Bravo, C. J. Todero Peixoto, J. J. Beatty, Paul Sommers, L. Ochilo, I. A. Minaya, B. Keilhauer, S. J. Saffi, B. Vargas Cárdenas, T. Suomijärvi, Marco Giammarchi, A. Blanco, R. Piegaia, N. Fazzini, N. Krohm, P. Gouffon, B. Sarkar, Christian Glaser, S. J. Sciutto, Dusan Mandat, J. Pallotta, E. J. Quel, M. J. Cooper, A. Insolia, M. Kleifges, D. Zavrtanik, Tobias Winchen, Julien Aublin, Karen S. Caballero-Mora, Octavian Fratu, H. Martinez, Bruce Rafael Mellado Garcia, C. Medina, Miroslav Pech, J. Chudoba, R.C. dos Anjos, J. Espadanal, J. Pȩkala, H. Wilczyński, Markus Lauscher, J. Phuntsok, Markus Roth, H. J. Mathes, Pavel Horvath, L. del Peral, D. LaHurd, M. Palatka, Günter Sigl, G. De Mauro, Martin Erdmann, I. Valiño, Gioacchino Alex Anastasi, Andrej Dundovic, Lorenzo Caccianiga, Maria Rita Coluccia, V. M. Theodoro, Roger W Clay, I. Lhenry-Yvon, Stefano D'Amico, M. I. Micheletti, G. Matthiae, A. N. Yushkov, Antonio Bueno, M. Josebachuili, J. Neuser, Johannes Schulz, R. Engel, K.-H. Becker, M. Pimenta, G. S. Varner, B. Mitrica, Heino Falcke, Sofia Andringa, Valerio Verzi, J. Hulsman, J. Vicha, A. Valbuena-Delgado, Lenka Tomankova, Dariusz Glas, J. Rodriguez Rojo, A. Tepe, Florian Lukas Briechle, A. G. Chavez, Gualberto Avila, Brian Fick, Enrique Zas, Jose Chinellato, B. Tome, Benedikt Zimmermann, Luca Latronico, Pascal Lautridou, A. C. Fauth, Angela V. Olinto, A. Letessier-Selvon, Lorenzo Cazon, C. Di Giulio, Fernando Contreras, Darko Veberic, Alberto Filevich, Bruno Daniel, Carla Bonifazi, Jose A. Bellido, A. van Vliet, Foteini Oikonomou, J. J. Masías Meza, T. Paul, R. Pelayo, G. Salina, Olivier Deligny, S. Querchfeld, S. Sonntag, Francesco Strafella, J. A. Matthews, Jaime Rosado, Ugo Giaccari, R. Cester, A. Cancio, Ioana Codrina Maris, Nicusor Arsene, P. Privitera, A. Tapia, F. Guarino, Peter Buchholz, Jesús Peña-Rodríguez, Ricardo Vázquez, G. C. Hill, Takahiro Fujii, I.M. Brancus, H. Gemmeke, M. Unger, A. Dorofeev, J. Ridky, Igor Katkov, H. Glass, Marco Aglietta, L. Villaseñor, Lukas Middendorf, Christine Peters, G. Rodriguez Fernandez, Daniela Mockler, J. W. Cronin, P. van Bodegom, Nataliia Borodai, S. J. De Jong, Gregory R. Snow, Pierre Billoir, J. R. T. de Mello Neto, Xavier Bertou, A. Zepeda, Pedro Assis, A. Etchegoyen, A. Gorgi, L. Perrone, D. Torres Machado, D. Nosek, A.M. van den Berg, Thomas Harrison, P. Pieroni, F. Arqueros, A. Weindl, H. Nožka, M. Schauer, G. Kukec Mezek, P. H. Hansen, Carla Bleve, Belén Andrada, G. Golup, N. Kunka, D. Heck, D. Yelos, Peter Gorham, M. L. Díaz Castro, L. Collica, Martina Bohacova, Patrick Allison, G. Farrar, C. Hojvat, Jan Ebr, A. Menshikov, Luis A. Anchordoqui, J. Sorokin, L.A.S. Pereira, A. Di Matteo, Francesca Zuccarello, Petr Travnicek, Rodríguez-Frías, Alan Coleman, Raul Sarmento, Trent D. Grubb, H.O. Klages, B. Wundheiler, R. Rebolo Lopez, P. H. Kasper, Juan Manuel Figueira, Frank G. Schröder, Marco Torri, Roberta Colalillo, A. G. Mariazzi, S. Messina, V. Novotny, Rossella Caruso, A. Lucero, S. Mathys, M. Erfani, J. Kleinfeller, A. Tonachini, Daniel Kuempel, Carlos Escobar, P.F. Gómez Vitale, P. Abreu, D. Ravignani, C. J.W.P. Timmermans, Ivone F. M. Albuquerque, Ke Fang, Marcus Niechciol, A.D. Supanitsky, Sutherland, R. M. Kieckhafer, J. Rautenberg, Kai Daumiller, O. Wainberg, Richard Dallier, Francisco Pedreira, Thomas Bretz, Corbin Covault, Matías Rolf Hampel, S. Navas, Lino Miramonti, Joshua A. Gordon, Gaia Silli, F. Sanchez, F. Sarazin, K. H. Kampert, S. Petrera, Leigui de Oliveira, J. F. Valdés Galicia, A. Hervé, B. Revenu, I. De Mitri, J. R. Vázquez, M. Platino, T. Huege, Hernán Gonzalo Asorey, A. Parra, P. Sanchez-Lucas, D. Harari, G. Müller, Ivo Nicolas Naranjo, Alina Mihaela Badescu, M. Prouza, Jeffrey Brack, M. Risse, Olaf Scholten, Jonathan Blazek, A. Schulz, Humberto Ibarguen Salazar, G. Parente, Fabrizia Canfora, Miguel Mostafa, R. Legumina, D. Garcia-Pinto, G. Marsella, A. López Casado, D. Rogozin, J. de Oliveira, Samo Stanič, Quentin Luce, Alex Kääpä, F. Suarez, Thomas Hebbeker, Sergio Dasso, Tristan Sudholz, Colin Baus, Martín Miguel Freire, M. Weber, Octavian Sima, V. Pirronello, H. Schieler, Antonella Castellina, G. P. Guedes, Jorn Schumacher, J. Debatin, A. Shadkam, A. F. Grillo, Juan Carlos D'Olivo, T. Pierog, P. L. Ghia, David Schmidt, Michael Urban, I. Al Samarai, Jeffrey A. Johnsen, S. Quinn, A. Segreto, Florian Gaté, V. de Souza, Eun-Joo Ahn, François Montanet, L. Caramete, Christian Sarmiento-Cano, L. Nellen, C. Morello, Peter L. Biermann, A. M. Kuotb Awad, J. A. J. Matthews, Paula Gina Isar, F. Salesa Greus, Nicolás González, Esteban Roulet, Corinne Berat, M. Giller, Q. Hasankiadeh, Z. Zong, B. Gookin, E. M. Santos, Bruce R. Dawson, P.O. Mazur, L. Niemietz, Tim Niggemann, J. Stasielak, S. Coutu, C. Porowski, Denise Boncioli, A. Aab, J. Biteau, Luis A. Nunez, Elton J. G. Santos, and K. Link
Subjects: Physics, Pierre Auger Observatory, High Energy Astrophysical Phenomena (astro-ph.HE), 010308 nuclear & particles physics, QC1-999, Astrophysics::High Energy Astrophysical Phenomena, Astrophysics::Instrumentation and Methods for Astrophysics, Spectral density, FOS: Physical sciences, Généralités, Astrophysics, 01 natural sciences, Auger, Interpretation (model theory), Acceleration, Physics and Astronomy (all), Observatory, 0103 physical sciences, Energy spectrum, Mass spectrum, Astrophysics - High Energy Astrophysical Phenomena, 010306 general physics
Abstract: We present a combined fit of a simple astrophysical model of UHECR sources to both the energy spectrum and mass composition data measured by the Pierre Auger Observatory. The fit has been performed for energies above 5 EeV, i.e. the region of the all-particle spectrum above the so-called "ankle"' feature. The astrophysical model we adopted consists of identical sources uniformly distributed in a comoving volume, where nuclei are accelerated with a rigidity-dependent mechanism. The fit results suggest sources characterized by relatively low maximum injection energies and hard spectral indices. The impact of various systematic uncertainties on the above result is discussed., 0, SCOPUS: cp.p, info:eu-repo/semantics/published
Published: 2017
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17. Impact of atmospheric effects on the energy reconstruction of air showers observed by the surface detectors of the Pierre Auger Observatory

Author: Marco Torri, Denis Stanca, P. Abreu, D. Ravignani, M. Platino, M. Urban, A. C. Rovero, Alexandru Balaceanu, Vincenzo Rizi, D. Martello, M. Ziolkowski, Silvia Mollerach, O. Martínez Bravo, I. Jandt, Ralf Ulrich, R. Piegaia, G. Cataldi, V. Scherini, C. J. Todero Peixoto, N. Krohm, Alexandra Saftoiu, B. Sarkar, Christian Glaser, J. Espadanal, H. Wilczyński, B. García, Tobias Winchen, P. Lebrun, R. López, Karen S. Caballero-Mora, Alberto Daniel Supanitsky, Jose Chinellato, J. Kleinfeller, J. D. Swain, Martin Erdmann, E. Santos, Daniel Kuempel, Carlos Escobar, G. Torralba Elipe, Markus Roth, A. Letessier-Selvon, Gioacchino Alex Anastasi, Jesús Peña-Rodríguez, R. Krause, A. Śmiałkowski, Roger W Clay, D. Melo, P. Ruehl, A. Insolia, M. Kleifges, D. Zavrtanik, Stefano D'Amico, Lorenzo Cazon, A. Fuster, A. C. Fauth, Carla Bonifazi, Jose A. Bellido, S. Sonntag, J. J. Beatty, J. Pȩkala, L. Valore, I.D. Vergara Quispe, Mariangela Settimo, L. Nellen, N. Fazzini, Jeffrey A. Johnsen, B. Vargas Cárdenas, T. Suomijärvi, J. Pallotta, E. J. Quel, A. van Vliet, Max Malacari, Lili Yang, Thomas Bretz, I. Valiño, C. Morello, J. Neuser, Corbin Covault, M. Zavrtanik, Piotr Homola, Julien Aublin, M. Josebachuili, David Walz, Ivone F. M. Albuquerque, M. Suarez Durán, Matías Rolf Hampel, Gaia Silli, A. Filipčič, R. M. Kieckhafer, David Wittkowski, Hernan Wahlberg, G. Salina, Igor Katkov, Eric Mayotte, M. Gómez Berisso, M. I. Micheletti, R. R. Prado, J. Rautenberg, Danielle LaHurd, Olivier Deligny, A. Parra, O. Wainberg, P. Ristori, Peter L. Biermann, M. Trini, S. Quinn, G. Kukec Mezek, Lino Miramonti, F. Sarazin, R. C. Shellard, A. Cancio, E. Varela, I. Allekotte, Dusan Mandat, Johannes Schulz, K.-H. Becker, M. Pimenta, J.D. Sanabria Gomez, Paolo Privitera, L. Villaseñor, S. Petrera, J. F. Valdés Galicia, Brian Fick, Marc Weber, Michael Unger, Francesco Strafella, I. De Mitri, Mario Buscemi, A. Segreto, Günter Sigl, Benedikt Zimmermann, Rúben Conceição, P. Heimann, Florian Lukas Briechle, J. Hulsman, A. Menshikov, Z. Zong, Petr Schovanek, A. Aab, Julian Kemp, G. Matthiae, M. A. Leigui de Oliveira, Roberto Mussa, D. Pakk Selmi-Dei, E. Kemp, R. Sato, Marco Giammarchi, L. Caramete, Serguei Vorobiov, J. R. Vázquez, D. Torres Machado, Alex Kääpä, Antonio Bueno, P. Sanchez-Lucas, D. Harari, D. Garcia-Pinto, Colin Baus, O. A. Taborda, Lourenco Lopes, Paul Sommers, A. Blanco, François Montanet, R. Squartini, G. S. Varner, T. Paul, Alfred Müller, L. Ochilo, P. Gouffon, H. Schieler, M. J. Cooper, H. Martinez, Carla Bleve, Karl-Heinz Kampert, F. Sánchez, Belén Andrada, Carlos Medina, Federico Suarez, Ricardo Vázquez, Ivo Nicolas Naranjo, Antonella Castellina, Paula Gina Isar, F. Salesa Greus, Gualberto Avila, M. Risse, Jonathan Blazek, G. C. Hill, Alina Mihaela Badescu, Radomir Smida, G. Medina-Tanco, G. van Aar, A. Di Matteo, Maria Rita Coluccia, Bruno Daniel, I. C. Mariç, Ralph Engel, M. Mallamaci, B. Wundheiler, Foteini Oikonomou, J. J. Masías Meza, G. De Mauro, C. Aramo, Gregory R Snow, P. H. Kasper, Jonathan Biteau, M. Prouza, Nicolás González, A.M. van den Berg, Darko Veberič, J. Ridky, Angela V. Olinto, Jörg R. Hörandel, B. Mitrica, S. Müller, Heino Falcke, E.M. Holt, Nicusor Arsene, A. Tapia, G. Parente, Fabrizia Canfora, R. Legumina, Esteban Roulet, H. Gemmeke, J. Vicha, I. Lhenry-Yvon, Corinne Berat, M. Giller, G. Marsella, A. Saleh, Maria-Teresa Dova, Q. Hasankiadeh, M. Perlin, D. Rogozin, J. de Oliveira, P. H. Nguyen, D. Nosek, C. Hojvat, Jan Ebr, R.J. Barreira Luz, E. M. Santos, Alejandro Almela, H.O. Klages, Bruce R. Dawson, P.O. Mazur, S. Messina, Johannes Schumacher, Andrej Dundovic, Lorenzo Caccianiga, V. M. Theodoro, Octavian Fratu, Valerio Verzi, B. Tome, G. Müller, Dariusz Glas, R.C. dos Anjos, V. de Souza, M. Palatka, A. Bridgeman, Luis A. Nunez, J. Stasielak, S. Coutu, S. J. Saffi, C. Porowski, Denise Boncioli, Marcus Niechciol, S. Querchfeld, M. J. Roncoroni, L. Niemietz, M. L. Díaz Castro, G. Farrar, Francesca Zuccarello, Tim Niggemann, I. Al Samarai, A. Criss, L. A. S. Pereira, Q. Luce, A. Taboada, G. P. Guedes, P.F. Gómez Vitale, Toshihiro Fujii, J. Debatin, A. Shadkam, Markus Lauscher, A. F. Grillo, Juan Carlos D'Olivo, T. Pierog, F. Pedreira, J. Phuntsok, Piera Luisa Ghia, Raul Sarmento, H. J. Mathes, A. Weindl, P. Stassi, David Schmidt, J. Rodriguez Rojo, A. G. Chavez, F.G. Schröder, Enrique Zas, Octavian Sima, C. Di Giulio, Fernando Contreras, M. Schauer, B. Revenu, D. Heck, Peter Gorham, Charles Timmermans, L. Collica, T. Huege, Jeffrey Brack, Olaf Scholten, Humberto Ibarguen Salazar, C. A. Sarmiento, F. Gate, Peter Hansen, Miguel Mostafa, L. Perrone, Jiri Chudoba, L. Tomankova, Alessio Gorgi, F. Guarino, John Matthews, A. López Casado, Samo Stanič, Peter Buchholz, R. Gaior, I.M. Brancus, Thomas Hebbeker, Sergio Dasso, Tristan Sudholz, Thomas Harrison, H. Glass, Martín Miguel Freire, Carola Dobrigkeit, M. Plum, V. Pirronello, Marco Aglietta, P. Pieroni, M. E. Bertaina, F. Arqueros, Alan Watson, Kai Daumiller, Martina Bohacova, Mihai Niculescu-Oglinzanu, J. Alvarez Castillo, K. Link, J. Sorokin, A. Lucero, Miroslav Hrabovský, O. Kambeitz, M. Schimp, A. Haungs, A. Kuotb Awad, J. L. Harton, S. G. Blaess, P. Mantsch, Z. Szadkowski, Ana Martina Botti, F. Diogo, V. Novotny, Rossella Caruso, S. Mathys, M. Erfani, R. M. de Almeida, Lukas Middendorf, Christine Peters, Miroslav Pech, A. Yushkov, Rodrigo Pelayo, Stijn Buitink, Pavel Horvath, D. Yelos, G. Rodriguez Fernandez, Hernán Asorey, R. Ramos-Pollan, Sofia Andringa, Marcio Aparecido Muller, H. Nožka, Daniela Mockler, W. Rodrigues de Carvalho, J. W. Cronin, P. van Bodegom, G. Golup, Nataliia Borodai, N. Kunka, S. J. De Jong, Pierre Billoir, Ugo Giaccari, J. R. T. de Mello Neto, J. A.J. Matthews, Xavier Bertou, A. Zepeda, Pedro Assis, A. Etchegoyen, Luis A. Anchordoqui, Jaime Alvarez-Muñiz, Philipp Papenbreer, Alexandru Gherghel-Lascu, Petr Travnicek, Alan Coleman, Trent D. Grubb, Juan Manuel Figueira, Roberta Colalillo, A. G. Mariazzi, I. A. Minaya, B. Keilhauer, André Schulz, S. J. Sciutto, D. Nitz, A. E. Herve, L. R. Wiencke, S. Jansen, 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 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 Subatomique et de Cosmologie (LPSC), Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes [2016-2019] (UGA [2016-2019]), Pierre AUGER, Aab, A., Abreu, P., Aglietta, M., Samarai, I. Al, Albuquerque, I. F. M., Allekotte, I., Almela, A., Castillo, J. Alvarez, Alvarez Muñiz, J., Anastasi, G. A., Anchordoqui, L., Andrada, B., Andringa, S., Aramo, C., Arqueros, F., Arsene, N., Asorey, H., Assis, P., Aublin, J., Avila, G., Badescu, A. M., Balaceanu, A., Luz, R. J. Barreira, Baus, C., Beatty, J. J., Becker, K. H., Bellido, J. A., Berat, C., Bertaina, M. E., Bertou, X., Biermann, P. L., Billoir, P., Biteau, J., Blaess, S. G., Blanco, A., Blazek, J., Bleve, C., Boháčová, M., Boncioli, D., Bonifazi, C., Borodai, N., Botti, A. M., Brack, J., Brancus, I., Bretz, T., Bridgeman, A., Briechle, F. L., Buchholz, P., Bueno, A., Buitink, S., Buscemi, M., Caballero Mora, K. S., Caccianiga, L., Cancio, A., Canfora, F., Caramete, L., Caruso, R., Castellina, A., Cataldi, G., Cazon, L., Chavez, A. G., Chinellato, J. A., Chudoba, J., Clay, R. W., Colalillo, Roberta, Coleman, A., Collica, L., Coluccia, M. R., Conceição, R., Contreras, F., Cooper, M. J., Coutu, S., Covault, C. E., Criss, A., Cronin, J., D'Amico, S., Daniel, B., Dasso, S., Daumiller, K., Dawson, B. R., de Almeida, R. M., de Jong, S. J., Mauro, G. De, Neto, J. R. T. de Mello, Mitri, I. De, de Oliveira, J., de Souza, V., Debatin, J., Deligny, O., Giulio, C. Di, Matteo, A. Di, Castro, M. L. Díaz, Diogo, F., Dobrigkeit, C., D'Olivo, J. C., Anjos, R. C. do, Dova, M. T., Dundovic, A., Ebr, J., Engel, R., Erdmann, M., Erfani, M., Escobar, C. O., Espadanal, J., Etchegoyen, A., Falcke, H., Farrar, G., Fauth, A. C., Fazzini, N., Fick, B., Figueira, J. M., Filipčič, A., Fratu, O., Freire, M. M., Fujii, T., Fuster, A., Gaior, R., García, B., Garcia Pinto, D., Gaté, F., Gemmeke, H., Gherghel Lascu, A., Ghia, P. L., Giaccari, U., Giammarchi, M., Giller, M., Głas, D., Glaser, C., Glass, H., Golup, G., Berisso, M. Gómez, Vitale, P. F. Gómez, González, N., Gorgi, A., Gorham, P., Gouffon, P., Grillo, A. F., Grubb, T. D., Guarino, Fausto, Guedes, G. P., Hampel, M. R., Hansen, P., Harari, D., Harrison, T. A., Harton, J. L., Hasankiadeh, Q., Haungs, A., Hebbeker, T., Heck, D., Heimann, P., Herve, A. E., Hill, G. C., Hojvat, C., Holt, E., Homola, P., Hörandel, J. R., Horvath, P., Hrabovský, M., Huege, T., Hulsman, J., Insolia, A., Isar, P. G., Jandt, I., Jansen, S., Johnsen, J. A., Josebachuili, M., Kääpä, A., Kambeitz, O., Kampert, K. H., Kasper, P., Katkov, I., Keilhauer, B., Kemp, E., Kemp, J., Kieckhafer, R. M., Klages, H. O., Kleifges, M., Kleinfeller, J., Krause, R., Krohm, N., Kuempel, D., Mezek, G. Kukec, Kunka, N., Awad, A. Kuotb, Lahurd, D., Lauscher, M., Lebrun, P., Legumina, R., de Oliveira, M. A. Leigui, Letessier Selvon, A., Lhenry Yvon, I., Link, K., Lopes, L., López, R., Casado, A. López, Luce, Q., Lucero, A., Malacari, M., Mallamaci, M., Mandat, D., Mantsch, P., Mariazzi, A. G., Mariç, I. C., Marsella, G., Martello, D., Martinez, H., Bravo, O. Martínez, Meza, J. J. Masía, Mathes, H. J., Mathys, S., Matthews, J., Matthews, J. A. J., Matthiae, G., Mayotte, E., Mazur, P. O., Medina, C., Medina Tanco, G., Melo, D., Menshikov, A., Messina, S., Micheletti, M. I., Middendorf, L., Minaya, I. A., Miramonti, L., Mitrica, B., Mockler, D., Mollerach, S., Montanet, F., Morello, C., Mostafá, M., Müller, A. L., Müller, G., Muller, M. A., Müller, S., Mussa, R., Naranjo, I., Nellen, L., Neuser, J., Nguyen, P. H., Niculescu Oglinzanu, M., Niechciol, M., Niemietz, L., Niggemann, T., Nitz, D., Nosek, D., Novotny, V., Nožka, H., Núñez, L. A., Ochilo, L., Oikonomou, F., Olinto, A., Selmi Dei, D. Pakk, Palatka, M., Pallotta, J., Papenbreer, P., Parente, G., Parra, A., Paul, T., Pech, M., Pedreira, F., Pȩkala, J., Pelayo, R., Peña Rodriguez, J., Pereira, L. A. S., Perlín, M., Perrone, L., Peters, C., Petrera, S., Phuntsok, J., Piegaia, R., Pierog, T., Pieroni, P., Pimenta, M., Pirronello, V., Platino, M., Plum, M., Porowski, C., Prado, R. R., Privitera, P., Prouza, M., Quel, E. J., Querchfeld, S., Quinn, S., Ramos Pollan, R., Rautenberg, J., Ravignani, D., Revenu, B., Ridky, J., Risse, M., Ristori, P., Rizi, V., de Carvalho, W. Rodrigue, Fernandez, G. Rodriguez, Rojo, J. Rodriguez, Rogozin, D., Roncoroni, M. J., Roth, M., Roulet, E., Rovero, A. C., Ruehl, P., Saffi, S. J., Saftoiu, A., Salazar, H., Saleh, A., Greus, F. Salesa, Salina, G., Gomez, J. D. Sanabria, Sánchez, F., Sanchez Lucas, P., Santos, E. M., Santos, E., Sarazin, F., Sarkar, B., Sarmento, R., Sarmiento, C. A., Sato, R., Schauer, M., Scherini, V., Schieler, H., Schimp, M., Schmidt, D., Scholten, O., Schovánek, P., Schröder, F. G., Schulz, A., Schulz, J., Schumacher, J., Sciutto, S. J., Segreto, A., Settimo, M., Shadkam, A., Shellard, R. C., Sigl, G., Silli, G., Sima, O., Śmiałkowski, A., Šmída, R., Snow, G. R., Sommers, P., Sonntag, S., Sorokin, J., Squartini, R., Stanca, D., Stanič, S., Stasielak, J., Stassi, P., Strafella, F., Suarez, F., Durán, M. Suarez, Sudholz, T., Suomijärvi, T., Supanitsky, A. D., Swain, J., Szadkowski, Z., Taboada, A., Taborda, O. A., Tapia, A., Theodoro, V. M., Timmermans, C., Peixoto, C. J. Todero, Tomankova, L., Tomé, B., Elipe, G. Torralba, Machado, D. Torre, Torri, M., Travnicek, P., Trini, M., Ulrich, R., Unger, M., Urban, M., Galicia, J. F. Valdé, Valiño, I., Valore, Laura, Aar, G. van, Bodegom, P. van, Berg, A. M. van den, Vliet, A. van, Varela, E., Cárdenas, B. Varga, Varner, G., Vázquez, J. R., Vázquez, R. A., Veberič, D., Quispe, I. D. Vergara, Verzi, V., Vicha, J., Villaseñor, L., Vorobiov, S., Wahlberg, H., Wainberg, O., Walz, D., Watson, A. A., Weber, M., Weindl, A., Wiencke, L., Wilczyński, H., Winchen, T., Wittkowski, D., Wundheiler, B., Yang, L., Yelos, D., Yushkov, A., Zas, E., Zavrtanik, D., Zavrtanik, M., Zepeda, A., Zimmermann, B., Ziolkowski, M., Zong, Z., Zuccarello, F., Bleve, Carla, Colalillo, R., Coluccia, MARIA RITA, D'Amico, Stefano, DE MITRI, Ivan, Guarino, F., Marsella, Giovanni, Martello, Daniele, Perrone, Lorenzo, Strafella, Francesco, Valore, L., Physics, Elementary Particle Physics, 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), and 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)
Subjects: [PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], Astronomy, Astrophysics::High Energy Astrophysical Phenomena, Cherenkov detectors, Data analysis, Large detector systems for particle and astroparticle physics, Systematic effects, FOS: Physical sciences, Cosmic ray, Cherenkov detectors Data analysis, Instrumentation, Mathematical Physics, 01 natural sciences, Auger, Nuclear physics, Observatory, 0103 physical sciences, Density of air, High Energy Physics, 010303 astronomy & astrophysics, Instrumentation and Methods for Astrophysics (astro-ph.IM), Physics::Atmospheric and Oceanic Physics, Pierre Auger Observatory, Physics, High Energy Astrophysical Phenomena (astro-ph.HE), 010308 nuclear & particles physics, Detector, Astrophysics::Instrumentation and Methods for Astrophysics, Física, 13. Climate action, Experimental High Energy Physics, RECONHECIMENTO DE PADRÕES, ComputingMethodologies_DOCUMENTANDTEXTPROCESSING, Física nuclear, Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - High Energy Astrophysical Phenomena, Event (particle physics), ultra-high energy cosmic rays, extensive air showers, atmospheric effects, Energy (signal processing)
Abstract: Atmospheric conditions, such as the pressure (P), temperature (T) or air density ( / P=T), affect the development of extended air showers initiated by energetic cosmic rays. We study the impact of the atmospheric variations on the reconstruction of air showers with data from the arrays of surface detectors of the Pierre Auger Observatory, considering separately the one with detector spacings of 1500m and the one with 750m spacing. We observe modulations in the event rates that are due to the influence of the air density and pressure variations on the measured signals, from which the energy estimators are obtained. We show how the energy assignment can be corrected to account for such atmospheric effects., La lista completa de autores puede verse al final del archivo asociado a este registro., Instituto de Física La Plata
Published: 2017

18. KASCADE-Grande energy reconstruction based on the lateral density distribution using the QGSJet-II.04 interaction model

Author: R. Engel, K. Link, J. Oehlschläger, H. Bozdog, A. Haungs, Alexandru Gherghel-Lascu, G. C. Trinchero, J.R. Hörandel, H.J. Gils, D. Huber, J. Zabierowski, G. Toma, T. Pierog, H. Rebel, Frank G. Schröder, P. Łuczak, S. Schoo, Octavian Sima, N. Palmieri, H. Schieler, H. J. Mathes, Claus Grupen, S. Ostapchenko, W. D. Apel, Markus Roth, J. C. Arteaga-Velázquez, M. Bertania, K. H. Kampert, F. Cossavella, D. Kang, J. Milke, H.O. Klages, P. Doll, F. Di Pierro, I.M. Brancus, E. Cantoni, D. Fuhrmann, K. Bekk, J. Blümer, B. Mitrica, R. Glasstetter, H.J. Mayer, Andrea Chiavassa, A. Weindl, H. Ulrich, J. Wochele, C. Morello, D. Heck, Kai Daumiller, V. de Souza, and T. Huege
Subjects: Physics, Primary energy, 010308 nuclear & particles physics, Astrophysics::High Energy Astrophysical Phenomena, Astronomy, Hadron, Interaction model, 01 natural sciences, Charged particle, Nuclear physics, KASCADE, Density distribution, Simulated data, 0103 physical sciences, Atomic physics, 010306 general physics, GeneralLiterature_REFERENCE(e.g.,dictionaries,encyclopedias,glossaries), Energy (signal processing)
Abstract: The charged particle densities obtained from CORSIKA simulated EAS, using the QGSJet-II.04 hadronic interaction model are used for primary energy reconstruction. Simulated data are reconstructed by using Lateral Energy Correction Functions computed with a new realistic model of the Grande stations implemented in Geant4.10.
Published: 2017
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19. 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

20. 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

21. Studies of radio emission from neutrino induced showers generated in rock salt

Author: Denis Stanca, G. Toma, H. Rebel, Alexandra Saftoiu, I. Lazanu, B. Mitrica, Octavian Sima, I.M. Brancus, Alina Mihaela Badescu, and A. Haungs
Subjects: Physics, Range (particle radiation), Neutral current, Physics::Instrumentation and Detectors, Astrophysics::High Energy Astrophysical Phenomena, Astronomy and Astrophysics, Askaryan effect, Nuclear physics, Neutrino detector, High Energy Physics::Experiment, Neutrino, Charged current, Cherenkov radiation, Radio wave
Abstract: Radio emission from particle showers can be used as a method of neutrino detection in the high and very high energy range as a Cherenkov pulse originates from the charge excess developing in the medium. Our study presents simulations of neutrino induced showers in rock salt and the radio emission that they generate, using the HERWIG, GEANT4 and AIRES codes. We have performed a complete study of all neutrino flavours interacting on nuclei, both for charged-current and neutral-current interactions, using the knowledge and codes available today. As primary neutrino energies we have chosen three values: 10 12 eV, 10 15 eV and 10 17 eV. We have injected all the particles resulting from the first interactions into shower simulation codes. Salt is one of the dielectric media proposed for radio detection of neutrinos already in the sixties of last century, and can be found in large volumes throughout the world. The calculation of the radio signal was performed considering the entire shower evolution, by approximating the shower with a current density. We have taken into account, in the equations, only the longitudinal profile. The aim of this study is to investigate whether different interactions can be discriminated in an experiment for detection of high energy particles based on the radio emission from the showers they initiate in a dense medium. For this we have performed and systematically analyzed simulations from several points of view.
Published: 2013

22. 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

23. 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

24. Evidence for a mixed mass composition at the 'ankle' in the cosmic-ray spectrum

Author: S. Stanič, Denis Stanca, J. A.J. Matthews, Xavier Bertou, M. L. Díaz Castro, C. Porowski, Jakub Vicha, Francesca Zuccarello, Pedro Assis, R. Sato, Jose Chinellato, I. Jandt, Hermann-Josef Mathes, M. Ziolkowski, Denise Boncioli, Markus Risse, Muller, F. Canfora, J. Blazek, A. Tonachini, Antonio Bueno, M. Josebachuili, J.D. Sanabria Gomez, Eric Mayotte, A. C. Rovero, J. Biteau, P.F. Gómez Vitale, G. A. Anastasi, Kai Daumiller, Alberto Filevich, Peter Hansen, John Matthews, Christian Sarmiento-Cano, Gualberto Avila, W. Rodrigues de Carvalho, Marco Torri, Nicolás González, M. Gómez Berisso, R. C. Shellard, Leigui de Oliveira, Paul M. Mantsch, Diego Ravignani, J. R. Vázquez, P. Sanchez-Lucas, S. Vorobiov, Ingomar Allekotte, F. Sánchez, J. W. Cronin, Lorenzo Cazon, Peter Buchholz, R. Piegaia, I. Al Samarai, Ivo Nicolas Naranjo, Antonio Insolia, A. Aab, L. Caramete, Alina Mihaela Badescu, P. Heimann, Anderson Fauth, M. Zavrtanik, G. Marsella, R. Ramos-Pollant, Valerio Pirronello, G. Torralba Elipe, O. Ravel, P. van Bodegom, Angela V. Olinto, C. Di Giulio, S. Navas, I.M. Brancus, H. Glass, Marco Aglietta, Johannes Schumacher, Joshua A. Gordon, Bruno Daniel, Corinne Berat, R. Krause, Gaia Silli, A. Filipčič, Foteini Oikonomou, G. S. Varner, Alessio Gorgi, Fred Sarazin, H. Gemmeke, Lukas Nellen, M. I. Micheletti, L. A. S. Pereira, Maria Giller, J. J. Masías Meza, C. J. Todero Peixoto, A.E. Herve, Octavian Sima, Nataliia Borodai, D. Mockler, Manuel Platino, E.M. Holt, B. Wundheiler, A. Fuster, Q. Hasankiadeh, A. Saleh, Jeffrey Brack, J. F. Valdés Galicia, Olaf Scholten, Ioana Codrina Maris, I. De Mitri, Dieter Heck, Martin Urban, Hans Klages, H. Nožka, A. Chiavassa, Maria-Teresa Dova, M. R. Hampel, O. A. Taborda, Carlos Hojvat, Miroslav Palatka, A. Menshikov, Diego Harari, B. Gookin, S. Müller, Carola Dobrigkeit, M. Schauer, Humberto Ibarguen Salazar, Ricardo Vázquez, Antoine Letessier-Selvon, Ernesto Kemp, R. Legumina, P. H. Nguyen, Lawrence Wiencke, B. Sarkar, Sarka Wykes, C. Morello, E. M. Santos, G. Kukec Mezek, L. Molina-Bueno, M. Plum, Z. Zong, David Walz, Harald Schieler, O. Kambeitz, Jeffrey A. Johnsen, Sven Querchfeld, L. Perrone, Marco Giammarchi, Bruce R. Dawson, S. Quinn, Christian Glaser, J. Espadanal, Octavian Fratu, M. E. Bertaina, Alan Watson, Mihai Niculescu-Oglinzanu, Jonny Kleinfeller, Sergio Sciutto, L. Ochilo, M. Mallamaci, Alberto Segreto, Nicusor Arsene, D. Rogozin, J. de Oliveira, R.R. Prado, Alejandro Almela, P. Billoir, Tim Huege, Ana Martina Botti, Belén Andrada, J. Alvarez Castillo, G. C. Hill, R.C. dos Anjos, Lukas Middendorf, D. Pakk Selmi-Dei, F. Diogo, G. De Mauro, Henryk Wilczyński, Ralph Engel, J. J. Beatty, Norbert Kunka, D. Nitz, Günter Sigl, Silvia Mollerach, A. Śmiałkowski, Jörg R. Hörandel, Sutherland, Julian Rautenberg, Peter L. Biermann, F. Montanet, L. Niemietz, R. M. de Almeida, L. Tomankova, Christine Peters, Radomir Smida, Alberto Etchegoyen, John L. Harton, Peter Gorham, T. Paul, Paolo Privitera, Federico Suarez, A. Schulz, D. Reinert, A. López Casado, G. Matthiae, Andreas Weindl, D. Garcia-Pinto, Paul Sommers, Petr Schovanek, A. Di Matteo, Charles Timmermans, Luis A. Nunez, A. Blanco, P. Gouffon, N. Krohm, D. Torres Machado, L. Collica, P. Abreu, Brian Fick, Zbigniew Szadkowski, Alberto Daniel Supanitsky, D. Melo, Julien Aublin, A. Shadkam, M. J. Cooper, Miguel Mostafá, Mário Pimenta, Gregory R Snow, Pablo Ristori, Miroslav Pech, P. H. Kasper, Carlos Medina, M. Settimo, R. Ulrich, Rodrigo Pelayo, Stijn Buitink, E. Varela, D. Yelos, Andrej Dundovic, Marcus Niechciol, D. Martello, Luis A. Anchordoqui, Pavel Horvath, Danilo Zavrtanik, Lorenzo Caccianiga, V. M. Theodoro, Paula Gina Isar, F. Salesa Greus, G. Cataldi, Florian Gaté, Michael Unger, S. Jansen, Gero Müller, P. W. Younk, Sofia Andringa, Eun-Joo Ahn, P. Lautridou, C. Scarso, Elton J. G. Santos, Jiri Chudoba, Markus Roth, G. van Aar, Dusan Mandat, Q. Luce, V. de Souza, Alex Kääpä, Maria Rita Coluccia, A. van Vliet, Tanguy Pierog, R. Cester, Gustavo Medina-Tanco, Miroslav Hrabovský, L. del Peral, Jaroslaw Stasielak, Andreas Haungs, Matthias Kleifges, V. Verzi, Philipp Papenbreer, Colin Baus, Glennys R. Farrar, David Schmidt, J. Sorokin, K. H. Becker, H. Martinez, A. G. Mariazzi, A. Kuotb Awad, S. G. Blaess, C. Aramo, Sergio Dasso, Tristan Sudholz, Fausto Guarino, Juan Pallotta, R. López, B. Tome, C. Bleve, Alexandru Balaceanu, Petr Travnicek, Rodríguez-Frías, V. Scherini, Arnulfo Zepeda, Eduardo Quel, David Wittkowski, Laura Valore, Martín Miguel Freire, Thomas Harrison, Benoît Revenu, Germano Guedes, Danielle LaHurd, Olivier Deligny, P. Pieroni, Alan Coleman, T. Hebbeker, Vincenzo Rizi, Trent D. Grubb, G. Rodriguez Fernandez, Benedikt Zimmermann, Rúben Conceição, Toshihiro Fujii, M. Ambrosio, L. Lopes, J. Debatin, O. Martínez Bravo, Dariusz Glas, Juan Manuel Figueira, F. Arqueros, Alexandra Saftoiu, Tim Niggemann, Roberta Colalillo, J. Hulsman, B. Mitrica, Hernán Asorey, Francesco Strafella, Martina Bohacova, Patrick Allison, Heino Falcke, Jaime Alvarez-Muñiz, Alexandru Gherghel-Lascu, I. Lhenry-Yvon, A. Lucero, Juan Carlos D'Olivo, O. Wainberg, A. Valbuena-Delgado, Esteban Roulet, T. Suomijärvi, Karl-Heinz Kampert, Antonella Castellina, Piera Luisa Ghia, V. Novotny, Rossella Caruso, S. Mathys, M. Erfani, John Swain, Thomas Bretz, Ruben Squartini, I. A. Minaya, Corbin Covault, Peter Mazur, J. Pȩkala, Geraldina Golup, Alexander Grillo, S. J. De Jong, Katrin Link, Lino Miramonti, Ugo Giaccari, A. Tepe, J. R. T. de Mello Neto, M. Prouza, J. Rodriguez Rojo, Bianca Keilhauer, A. G. Chavez, F.G. Schröder, Enrique Zas, Fernando Contreras, Jesús Peña-Rodríguez, A. Dorofeev, L. Villaseñor, A. Bridgeman, S. J. Saffi, Markus Lauscher, F. Pedreira, J. Phuntsok, Raul Sarmento, M. Suarez Durán, H. Wahlberg, A. Parra, G. Parente, M. Trini, Johannes Schulz, Florian Lukas Briechle, A. Cancio, B. Caccianiga, Alexey Yushkov, Max Malacari, Lili Yang, Luca Latronico, Piotr Homola, Alex Tapia, Tobias Winchen, P. Lebrun, Karen S. Caballero-Mora, Martin Erdmann, Carla Bonifazi, Beatriz García, Roger W Clay, Stefano D'Amico, Jose A. Bellido, Daniel Kuempel, S. Sonntag, Carlos Escobar, Jaime Rosado, R.M. Kieckhafer, B. Vargas Cárdenas, I. Valiño, J. Neuser, Ivone F. M. Albuquerque, Ke Fang, I. Katkov, Richard Dallier, Gaetano Salina, A.M. van den Berg, Darko Veberič, Jan Ridky, Marc Weber, M. Buscemi, D. Nosek, Jan Ebr, Sergio Petrera, S. Messina, S. Coutu, Norberto Fazzini, 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., Ambrosio, M., Anastasi, G. A., Anchordoqui, L., Andrada, B., Andringa, S., Aramo, C., Arqueros, F., Arsene, N., Asorey, H., Assis, P., Aublin, J., Avila, G., Badescu, A. M., Balaceanu, A., Baus, C., Beatty, J. J., Becker, K. H., Bellido, J. A., Berat, C., Bertaina, M. E., Bertou, X., Biermann, P. L., Billoir, P., Biteau, J., Blaess, S. G., Blanco, A., Blazek, J., Bleve, Carla, Boháčová, M., Boncioli, D., Bonifazi, C., Borodai, N., Botti, A. M., Brack, J., Brancus, I., Bretz, T., Bridgeman, A., Briechle, F. L., Buchholz, P., Bueno, A., Buitink, S., Buscemi, M., Caballero Mora, K. S., Caccianiga, B., Caccianiga, L., Cancio, A., Canfora, F., Caramete, L., Caruso, R., Castellina, A., Cataldi, G., Cazon, L., Cester, R., Chavez, A. G., Chiavassa, A., Chinellato, J. A., Chudoba, J., Clay, R. W., Colalillo, R., Coleman, A., Collica, L., Coluccia, MARIA RITA, Conceição, R., Contreras, F., Cooper, M. J., Coutu, S., Covault, C. E., Cronin, J., Dallier, R., D'Amico, Stefano, 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., Debatin, J., del Peral, L., Deligny, O., Di Giulio, C., Di Matteo, A., Díaz Castro, M. L., Diogo, F., Dobrigkeit, C., D'Olivo, J. C., Dorofeev, A., dos Anjos, R. C., Dova, M. T., Dundovic, A., 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., Fick, B., Figueira, J. M., Filevich, A., Filipčič, A., Fratu, O., Freire, M. M., Fujii, T., Fuster, A., García, B., Garcia Pinto, D., Gaté, 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., Grillo, A. F., Grubb, T. D., Guarino, F., Guedes, G. P., Hampel, M. R., Hansen, P., Harari, D., Harrison, T. A., Harton, J. L., Hasankiadeh, Q., Haungs, A., Hebbeker, T., Heck, D., Heimann, P., Herve, A. E., Hill, G. C., Hojvat, C., Holt, E., Homola, P., Hörandel, J. R., Horvath, P., Hrabovský, M., Huege, T., Hulsman, J., Insolia, A., Isar, P. G., Jandt, I., Jansen, S., Johnsen, J. A., Josebachuili, M., Kääpä, A., Kambeitz, O., Kampert, K. H., Kasper, P., Katkov, I., Keilhauer, B., Kemp, E., Kieckhafer, R. M., Klages, H. O., Kleifges, M., Kleinfeller, J., Krause, R., Krohm, N., Kuempel, D., Kukec Mezek, G., Kunka, N., Kuotb Awad, A., Lahurd, D., Latronico, L., Lauscher, M., Lautridou, P., Lebrun, P., Legumina, R., Leigui de Oliveira, M. A., Letessier Selvon, A., Lhenry Yvon, I., Link, K., Lopes, L., López, R., López Casado, A., Luce, Q., Lucero, A., Malacari, M., Mallamaci, M., Mandat, D., Mantsch, P., Mariazzi, A. G., Mariş, I. C., Marsella, Giovanni, Martello, Daniele, Martinez, H., Martínez Bravo, O., Masías Meza, J. J., Mathes, H. J., Mathys, S., Matthews, J., Matthews, J. A. J., Matthiae, G., Mayotte, E., Mazur, P. O., Medina, C., Medina Tanco, G., Melo, D., Menshikov, A., Messina, S., Micheletti, M. I., Middendorf, L., Minaya, I. A., Miramonti, L., Mitrica, B., Mockler, D., Molina Bueno, L., Mollerach, S., Montanet, F., Morello, C., Mostafá, M., Müller, G., Muller, M. A., Müller, S., Naranjo, I., Navas, S., Nellen, L., Neuser, J., Nguyen, P. H., Niculescu Oglinzanu, M., Niechciol, M., Niemietz, L., Niggemann, T., Nitz, D., Nosek, D., Novotny, V., Nožka, H., Núñez, L. A., Ochilo, L., Oikonomou, F., Olinto, A., Pakk Selmi Dei, D., Palatka, M., Pallotta, J., Papenbreer, P., Parente, G., Parra, A., Paul, T., Pech, M., Pedreira, F., Pękala, J., Pelayo, R., Peña Rodriguez, J., Pereira, L. A. S., Perrone, Lorenzo, Peters, C., Petrera, S., Phuntsok, J., Piegaia, R., Pierog, T., Pieroni, P., Pimenta, M., Pirronello, V., Platino, M., Plum, M., Porowski, C., Prado, R. R., Privitera, P., Prouza, M., Quel, E. J., Querchfeld, S., Quinn, S., Ramos Pollant, R., Rautenberg, J., Ravel, O., Ravignani, D., Reinert, D., Revenu, B., Ridky, J., 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., Salazar, H., Saleh, A., Salesa Greus, F., Salina, G., Sanabria Gomez, J. D., Sánchez, F., Sanchez Lucas, P., Santos, E. M., Santos, E., Sarazin, F., Sarkar, B., Sarmento, R., Sarmiento Cano, C., Sato, R., Scarso, C., Schauer, M., Scherini, Viviana, Schieler, H., Schmidt, D., Scholten, O., Schovánek, P., Schröder, F. G., Schulz, A., Schulz, J., Schumacher, J., Sciutto, S. J., Segreto, A., Settimo, Mariangela, Shadkam, A., Shellard, R. C., Sigl, G., Silli, G., Sima, O., Śmiałkowski, A., Šmída, R., Snow, G. R., Sommers, P., Sonntag, S., Sorokin, J., Squartini, R., Stanca, D., Stanič, S., Stasielak, J., Strafella, Francesco, Suarez, F., Suarez Durán, M., Sudholz, T., Suomijärvi, T., Supanitsky, A. D., Sutherland, M. S., Swain, J., Szadkowski, Z., Taborda, O. A., Tapia, A., Tepe, A., Theodoro, V. M., Timmermans, C., Todero Peixoto, C. J., Tomankova, L., Tomé, B., Tonachini, A., Torralba Elipe, G., Torres Machado, D., Torri, M., Travnicek, P., Trini, M., Ulrich, R., Unger, M., Urban, M., Valbuena Delgado, A., Valdés Galicia, J. F., Valiño, I., Valore, L., van Aar, G., van Bodegom, P., van den Berg, A. M., van Vliet, A., Varela, E., Vargas Cárdenas, B., Varner, G., Vázquez, J. R., Vázquez, R. A., Veberič, D., Verzi, V., Vicha, J., Villaseñor, L., Vorobiov, S., Wahlberg, H., Wainberg, O., Walz, D., Watson, A. A., Weber, M., Weindl, A., Wiencke, L., Wilczyński, H., Winchen, T., Wittkowski, D., Wundheiler, B., Wykes, S., Yang, L., Yelos, D., Younk, P., Yushkov, A., Zas, E., Zavrtanik, D., Zavrtanik, M., Zepeda, A., Zimmermann, B., Ziolkowski, M., Zong, Z., Zuccarello, F., Bleve, C., Colalillo, Roberta, Coluccia, M. R., D'Amico, S., De Mitri, I., Guarino, Fausto, Marsella, G., Martello, D., Pȩkala, J., Perrone, L., Scherini, V., Settimo, M., Strafella, F., Valore, Laura, Physics, Astronomy and Astrophysics Research Group, Elementary Particle Physics, Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes [2016-2019] (UGA [2016-2019]), and Pierre Auger Collaboration
Subjects: [PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], Nuclear and High Energy Physics, Proton, Pierre Auger Observatory, Cosmic Rays, Mass Composition, Astronomy, Astrophysics::High Energy Astrophysical Phenomena, Flux, FOS: Physical sciences, Cosmic ray, Ankle, Cosmic rays, Mass composition, Astrophysics, 01 natural sciences, Auger, Observatory, 0103 physical sciences, ddc:530, High Energy Physics, 010303 astronomy & astrophysics, GeneralLiterature_REFERENCE(e.g.,dictionaries,encyclopedias,glossaries), Cherenkov radiation, Ciencias Exactas, Physics, High Energy Astrophysical Phenomena (astro-ph.HE), Range (particle radiation), 010308 nuclear & particles physics, OBSERVATÓRIOS, Astrophysics::Instrumentation and Methods for Astrophysics, Física, lcsh:QC1-999, Physique atomique et nucléaire, Experimental High Energy Physics, Física nuclear, Astrophysics - High Energy Astrophysical Phenomena, lcsh:Physics
Abstract: We report a first measurement for ultrahigh energy cosmic rays of the correlation between the depth of shower maximum and the signal in the water Cherenkov stations of air-showers registered simultaneously by the fluorescence and the surface detectors of the Pierre Auger Observatory. Such a correlation measurement is a unique feature of a hybrid air-shower observatory with sensitivity to both the electromagnetic and muonic components. It allows an accurate determination of the spread of primary masses in the cosmic-ray flux. Up till now, constraints on the spread of primary masses have been dominated by systematic uncertainties. The present correlation measurement is not affected by systematics in the measurement of the depth of shower maximum or the signal in the water Cherenkov stations. The analysis relies on general characteristics of air showers and is thus robust also with respect to uncertainties in hadronic event generators. The observed correlation in the energy range around the ‘ankle’ at lg⁡(E/eV)=18.5–19.0 differs significantly from expectations for pure primary cosmic-ray compositions. A light composition made up of proton and helium only is equally inconsistent with observations. The data are explained well by a mixed composition including nuclei with mass A>4. Scenarios such as the proton dip model, with almost pure compositions, are thus disfavored as the sole explanation of the ultrahigh-energy cosmic-ray flux at Earth., 0, SCOPUS: ar.j, info:eu-repo/semantics/published
Published: 2016

25. Cosmic ray energy reconstruction from the S(500) observable recorded in the KASCADE-Grande air shower experiment

Author: Markus Roth, D. Huber, E. Cantoni, P. Doll, P. Łuczak, N. Palmieri, H. Bozdog, H. J. Mathes, Alexandru Gherghel-Lascu, G.C. Trinchero, J. Wochele, T. Pierog, J. Oehlschläger, Ralph Engel, Octavian Sima, F.G. Schröder, Claus Grupen, G. Toma, B. Mitrica, H. Rebel, Andreas Haungs, S. Schoo, D. Heck, M. E. Bertaina, J. Blümer, H. Schieler, J. Milke, Karl-Heinz Kampert, M. Petcu, A. Chiavassa, K. Link, Jörg R. Hörandel, D. Kang, H.O. Klages, I.M. Brancus, H. Ulrich, J. Zabierowski, V. de Souza, W. D. Apel, K. Bekk, H.J. Mayer, F. Cossavella, C. Morello, S. Ostapchenko, H.J. Gils, A. Weindl, F. Di Pierro, D. Fuhrmann, J.C. Arteaga-Velázquez, Kai Daumiller, T. Huege, and R. Glasstetter
Subjects: Astronomy, Astrophysics::High Energy Astrophysical Phenomena, Cosmic ray, Hadronic interaction model, 01 natural sciences, KASCADE-Grande, Nuclear physics, S(500), 0103 physical sciences, Calibration, 010306 general physics, Primary energy, Physics, Muon, 010308 nuclear & particles physics, Attenuation, Astrophysics::Instrumentation and Methods for Astrophysics, Astronomy and Astrophysics, ASTROFÍSICA, Physik (inkl. Astronomie), Charged particle, Air shower, KASCADE, Energy (signal processing)
Abstract: The energy reconstruction at KASCADE-Grande is based on a combination of the shower size and the total muon number, which are both estimated for each individual air shower event. We present investigations where we employed a second method to reconstruct the primary energy using S(500), which are the charged particle densities inferred with the KASCADE-Grande detector at a distance of 500 m from the shower axis. We considered the attenuation of inclined showers by applying the “Constant Intensity Cut” method and we employed a simulation-derived calibration to convert the recorded S(500) into primary energy. We observed a systematic shift in the S(500)-derived energy compared with previously reported results obtained using the standard reconstruction technique. However, a comparison of the two methods based on simulated and measured data showed that this shift only appeared in the measured data. Our investigations showed that this shift was caused mainly by the inadequate description of the shape of the lateral density distribution in the simulations.
Published: 2016

26. KASCADE-Grande Review, Recent Results, Future Endeavors

Author: T. Pierog, H. J. Mathes, E. Cantoni, J. C. Arteaga-Velázquez, D. Fuhrmann, H.J. Mayer, Alexandru Gherghel-Lascu, Andrea Chiavassa, B. Mitrica, H. Bozdog, J.R. Hörandel, Claus Grupen, A. Weindl, R. Glasstetter, S. Ostapchenko, F. Di Pierro, M. E. Bertaina, C. Morello, F. Cossavella, V. de Souza, J. Milke, J. Oehlschläger, K. Link, W. D. Apel, P. Łuczak, K. Beck, N. Palmieri, Andreas Haungs, Markus Roth, J. Zabierowski, G. C. Trinchero, H.J. Gils, M. Petcu, I.M. Brancus, P. Doll, S. Schoo, Octavian Sima, H. Schieler, K. H. Kampert, G. Toma, J. Wochele, Kai Daumiller, D. Heck, T. Huege, D. Huber, Frank G. Schröder, H. Ulrich, J. Blümer, H. Rebel, R. Engel, D. Kang, and H.O. Klages
Subjects: History, KASCADE, Astronomy, JPS Conference Proceedings, Cosmic ray, Engineering physics, GeneralLiterature_REFERENCE(e.g.,dictionaries,encyclopedias,glossaries)
Abstract: Contains fulltext : 166007.pdf (Publisher’s version ) (Open Access) UHECR 2014 : International Symposium for Ultra-High Energy Cosmic Rays, October 12-15, 2014, Springdale, Utah, USA
Published: 2016

27. 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

28. Ultrahigh-energy neutrino follow-up of gravitational wave events GW150914 and GW151226 with the Pierre Auger Observatory

Author: F. Canfora, P. Heimann, Q. Luce, P. Abreu, R.J. Barreira Luz, G. A. Anastasi, E. Kemp, D. Ravignani, Serguei Vorobiov, D. Mockler, Luis A. Anchordoqui, C. Aramo, John N. Matthews, R. M. Kieckhafer, O. A. Taborda, Johannes Schumacher, G. Matthiae, M. Platino, Antonio Bueno, M. Josebachuili, O. Wainberg, K. H. Becker, Gualberto Avila, B. Mitrica, Heino Falcke, E.M. Holt, Ingomar Allekotte, G. De Mauro, A. Fuster, Maria-Teresa Dova, M. R. Hampel, S. Petrera, G. S. Varner, Sarka Wykes, Octavian Fratu, Angela V. Olinto, R.C. dos Anjos, Julian Rautenberg, M. Palatka, C. Di Giulio, G. C. Hill, M. Mallamaci, S. J. De Jong, Jörg R. Hörandel, J. Vicha, Petr Travnicek, Trent D. Grubb, R. Squartini, Jeffrey A. Johnsen, Juan Manuel Figueira, Roberta Colalillo, A. G. Mariazzi, Ralph Engel, T. Paul, J. Ridky, M. Suarez Durán, J. Stasielak, S. Coutu, Ugo Giaccari, F. Montanet, S. Quinn, Günter Sigl, M. Trini, David Wittkowski, M. Urban, Norberto Fazzini, J. F. Valdés Galicia, I. De Mitri, L. Molina-Bueno, D. Melo, David Walz, G. Medina-Tanco, D. Pakk Selmi-Dei, R. Sato, J. R. T. de Mello Neto, M. Hrabovský, G. van Aar, Radomir Smida, A. C. Rovero, C. Bleve, Alexandru Balaceanu, Hernan Wahlberg, Andreas Weindl, M. Zavrtanik, H. Nožka, R. Gaior, Dieter Heck, Lourenco Lopes, A. Gorgi, A. Saleh, Vincenzo Rizi, Octavian Sima, M. A. Leigui de Oliveira, G. Müller, N. Kunka, H. Glass, M. Ambrosio, V. Scherini, G. Torralba Elipe, R. R. Prado, G. Kukec Mezek, L. Nellen, Alexandra Saftoiu, M. Schauer, D. Yelos, C. Porowski, Florian Gaté, M. Erdmann, A. van Vliet, Andreas Haungs, A. Coleman, M. Ziolkowski, O. Martínez Bravo, C. J. Todero Peixoto, C. Morello, Dusan Mandat, A. Parra, I. Lhenry-Yvon, M. E. Bertaina, V. de Souza, L. Valore, O. Kambeitz, H. Martinez, I. Naranjo, A. Menshikov, F. Suarez, Thomas Hebbeker, M. A. Muller, J. J. Beatty, N. Krohm, Andrej Dundovic, P. Ristori, Danielle LaHurd, Olivier Deligny, E. Mayotte, E. Varela, J.D. Sanabria Gomez, Petr Schovanek, Sergio Dasso, Tristan Sudholz, W. Rodrigues de Carvalho, Paul Sommers, A. Blanco, B. Sarkar, Lorenzo Caccianiga, V. M. Theodoro, A. Kääpä, P. H. Nguyen, A. Segreto, Silvia Mollerach, D. Garcia-Pinto, Christian Glaser, P. Gouffon, J. W. Cronin, Philipp Papenbreer, J. Espadanal, Peter L. Biermann, P. Stassi, Denise Boncioli, J. Rodriguez Rojo, R. Krause, J. A.J. Matthews, Xavier Bertou, J. D. Swain, P. van Bodegom, A. Kuotb Awad, V. Pirronello, A. G. Chavez, Alberto Daniel Supanitsky, Francesco Strafella, J. L. Harton, P. Lebrun, Julien Aublin, D. Nosek, Paolo Privitera, M. J. Cooper, S. G. Blaess, Jaime Alvarez-Muñiz, F. Sánchez, Alexandru Gherghel-Lascu, A. Aab, J. Biteau, H. Wilczyński, P. Billoir, Tanguy Pierog, Pedro Assis, A. Insolia, B. Tome, Ana Martina Botti, M. Kleifges, D. Zavrtanik, A. Cancio, A. Etchegoyen, Peter Mazur, A. Shadkam, Carlos Medina, Nataliia Borodai, Hermann-Josef Mathes, Enrique Zas, A. Di Matteo, I. Al Samarai, G. Marsella, L. Caramete, Marco Giammarchi, Markus Roth, H. Gemmeke, Dariusz Glas, Denis Stanca, T. Suomijärvi, D. Martello, Jose Chinellato, C. Peters, Michael Unger, B. Wundheiler, L. A. S. Pereira, Maria Giller, M. I. Micheletti, Peter Gorham, Charles Timmermans, Lukas Middendorf, Fernando Contreras, Gregory R Snow, L. Collica, I. Jandt, A. Letessier-Selvon, J. Hulsman, I. A. Minaya, B. Keilhauer, G. P. Guedes, Toshihiro Fujii, S. Jansen, Kai Daumiller, S. Müller, Lorenzo Cazon, Ralf Ulrich, Paul M. Mantsch, B. Vargas Cárdenas, André Schulz, J. Debatin, M. Gómez Berisso, R. C. Shellard, L. Perrone, Jiri Chudoba, G. Rodriguez Fernandez, D. Torres Machado, V. Verzi, J. Pallotta, David Schmidt, M. L. Díaz Castro, G. Farrar, S. J. Sciutto, Katrin Link, Maria Rita Coluccia, Carola Dobrigkeit, Juan Carlos D'Olivo, M. Plum, Hernán Asorey, E. J. Quel, Bruno Daniel, Foteini Oikonomou, I. C. Mariş, Luis A. Nunez, R. Piegaia, Marcus Niechciol, Esteban Roulet, P. L. Ghia, Mario Buscemi, Francesca Zuccarello, Paula Gina Isar, J. J. Masías Meza, Jeffrey Brack, Olaf Scholten, Humberto Ibarguen Salazar, Thomas Harrison, Jesús Peña-Rodríguez, D. Nitz, A. Dorofeev, Alan Watson, Mihai Niculescu-Oglinzanu, F. Salesa Greus, G. Cataldi, Igor Katkov, J. Alvarez Castillo, P. Pieroni, Jan Pękala, Harald Schieler, F. Diogo, A. Taboada, A. E. Herve, A. Yushkov, Marco Torri, F. Arqueros, R. M. de Almeida, L. R. Wiencke, L. Villaseñor, Peter Hansen, Miguel Mostafa, Martina Bohacova, A. Śmiałkowski, D. Reinert, L. Tomankova, L. Ochilo, J. Sorokin, Z. Zong, Diego Harari, I. Valiño, P.F. Gómez Vitale, F. Guarino, Peter Buchholz, A. López Casado, Zbigniew Szadkowski, Brian Fick, Samo Stanič, Nicusor Arsene, A. Tapia, Rodrigo Pelayo, Stijn Buitink, E. Santos, I.M. Brancus, A. Bridgeman, B. Gookin, R. Ramos-Pollan, S. Messina, S. Querchfeld, S. J. Saffi, V. Novotny, Rossella Caruso, A. Lucero, S. Mathys, Marco Aglietta, J. Neuser, L. Niemietz, E. M. Santos, M. Erfani, R. A. Vázquez, Gaia Silli, F. Sarazin, Arnulfo Zepeda, Marc Weber, F. G. Schröder, B. Revenu, Markus Lauscher, Benedikt Zimmermann, Rúben Conceição, J. R. Vázquez, F. Pedreira, P. Sanchez-Lucas, P. Kasper, J. Phuntsok, Raul Sarmento, M. M. Freire, Bruce R. Dawson, Tim Huege, Alina Mihaela Badescu, M. Prouza, Tim Niggemann, Miroslav Pech, Nicolás González, A. C. Fauth, Corinne Berat, Q. Hasankiadeh, Pavel Horvath, Carla Bonifazi, A. Filipcic, Jose A. Bellido, S. Sonntag, B. Andrada, Sofia Andringa, R. Cester, C. A. Sarmiento, I.D. Vergara Quispe, M. Risse, Jonathan Blazek, G. Parente, Carlos Hojvat, R. Legumina, D. Rogozin, J. de Oliveira, Alejandro Almela, Julian Kemp, Michael Schimp, Colin Baus, Karl-Heinz Kampert, Antonella Castellina, Thomas Bretz, Corbin Covault, Geraldina Golup, Alexander Grillo, Lino Miramonti, B. García, Tobias Winchen, R. López, Karen S. Caballero-Mora, Roger W Clay, Stefano D'Amico, Johannes Schulz, M. Pimenta, Florian Lukas Briechle, Mariangela Settimo, Max Malacari, Lili Yang, Piotr Homola, J. Kleinfeller, Daniel Kuempel, Carlos Escobar, Ivone F. M. Albuquerque, Ke Fang, Jan Ebr, H.O. Klages, Gaetano Salina, A.M. van den Berg, Darko Veberič, Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes [2016-2019] (UGA [2016-2019]), Pierre Auger Collaboration, Research unit Astroparticle Physics, Aab, A., Abreu, P., Aglietta, M., Al Samarai, I., Albuquerque, I. . f. . m., Allekotte, I., Almela, A., Alvarez Castillo, J., Alvarez Muñiz, J., Ambrosio, M., Anastasi, G. . a., Anchordoqui, L., Andrada, B., Andringa, S., Aramo, C., Arqueros, F., Arsene, N., Asorey, H., Assis, P., Aublin, J., Avila, G., Badescu, A. . m., Balaceanu, A., Barreira Luz, R. . j., Baus, C., Beatty, J. . j., Becker, K. . h., Bellido, J. . a., Berat, C., Bertaina, M. . e., Bertou, X., Biermann, P. . l., Billoir, P., Biteau, J., Blaess, S. . g., Blanco, A., Blazek, J., Bleve, C., Boháčová, M., Boncioli, D., Bonifazi, C., Borodai, N., Botti, A. . m., Brack, J., Brancus, I., Bretz, T., Bridgeman, A., Briechle, F. . l., Buchholz, P., Bueno, A., Buitink, S., Buscemi, M., Caballero Mora, K. . s., Caccianiga, L., Cancio, A., Canfora, F., Caramete, L., Caruso, R., Castellina, A., Cataldi, G., Cazon, L., Cester, R., Chavez, A. . g., Chinellato, J. . a., Chudoba, J., Clay, R. . w., Colalillo, Roberta, Coleman, A., Collica, L., Coluccia, M. . r., Conceição, R., Contreras, F., Cooper, M. . j., Coutu, S., Covault, C. . e., Cronin, J., D’Amico, S., 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., Debatin, J., Deligny, O., Di Giulio, C., Di Matteo, A., Díaz Castro, M. . l., Diogo, F., Dobrigkeit, C., D’Olivo, J. . c., Dorofeev, A., dos Anjos, R. . c., Dova, M. . t., Dundovic, A., 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., Fick, B., Figueira, J. . m., Filipčič, A., Fratu, O., Freire, M. . m., Fujii, T., Fuster, A., Gaior, R., García, B., Garcia Pinto, D., Gaté, 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., Gorgi, A., Gorham, P., Gouffon, P., Grillo, A. . f., Grubb, T. . d., Guarino, Fausto, Guedes, G. . p., Hampel, M. . r., Hansen, P., Harari, D., Harrison, T. . a., Harton, J. . l., Hasankiadeh, Q., Haungs, A., Hebbeker, T., Heck, D., Heimann, P., Herve, A. . e., Hill, G. . c., Hojvat, C., Holt, E., Homola, P., Hörandel, J. . r., Horvath, P., Hrabovský, M., Huege, T., Hulsman, J., Insolia, A., Isar, P. . g., Jandt, I., Jansen, S., Johnsen, J. . a., Josebachuili, M., Kääpä, A., Kambeitz, O., Kampert, K. . h., Kasper, P., Katkov, I., Keilhauer, B., Kemp, E., Kemp, J., Kieckhafer, R. . m., Klages, H. . o., Kleifges, M., Kleinfeller, J., Krause, R., Krohm, N., Kuempel, D., Kukec Mezek, G., Kunka, N., Kuotb Awad, A., Lahurd, D., Lauscher, M., Lebrun, P., Legumina, R., Leigui de Oliveira, M. . a., Letessier Selvon, A., Lhenry Yvon, I., Link, K., Lopes, L., López, R., López Casado, A., Luce, Q., Lucero, A., Malacari, M., Mallamaci, M., Mandat, D., Mantsch, P., Mariazzi, A. . g., Mariş, I. . c., Marsella, G., Martello, D., Martinez, H., Martínez Bravo, O., Masías Meza, J. . j., Mathes, H. . j., Mathys, S., Matthews, J., Matthews, J. . a. . j., Matthiae, G., Mayotte, E., Mazur, P. . o., Medina, C., Medina Tanco, G., Melo, D., Menshikov, A., Messina, S., Micheletti, M. . i., Middendorf, L., Minaya, I. . a., Miramonti, L., Mitrica, B., Mockler, D., Molina Bueno, L., Mollerach, S., Montanet, F., Morello, C., Mostafá, M., Müller, G., Muller, M. . a., Müller, S., Naranjo, I., Nellen, L., Neuser, J., Nguyen, P. . h., Niculescu Oglinzanu, M., Niechciol, M., Niemietz, L., Niggemann, T., Nitz, D., Nosek, D., Novotny, V., Nožka, H., Núñez, L. . a., Ochilo, L., Oikonomou, F., Olinto, A., Pakk Selmi Dei, D., Palatka, M., Pallotta, J., Papenbreer, P., Parente, G., Parra, A., Paul, T., Pech, M., Pedreira, F., Pękala, J., Pelayo, R., Peña Rodriguez, J., Pereira, L. . a. . s., Perrone, L., Peters, C., Petrera, S., Phuntsok, J., Piegaia, R., Pierog, T., Pieroni, P., Pimenta, M., Pirronello, V., Platino, M., Plum, M., Porowski, C., Prado, R. . r., Privitera, P., Prouza, M., Quel, E. . j., Querchfeld, S., Quinn, S., Ramos Pollan, R., Rautenberg, J., Ravignani, D., Reinert, D., Revenu, B., Ridky, J., Risse, M., Ristori, P., Rizi, V., Rodrigues de Carvalho, W., Rodriguez Fernandez, G., Rodriguez Rojo, J., Rogozin, D., Roth, M., Roulet, E., Rovero, A. . c., Saffi, S. . j., Saftoiu, A., Salazar, H., Saleh, A., Salesa Greus, F., Salina, G., Sanabria Gomez, J. . d., Sánchez, F., Sanchez Lucas, P., Santos, E. . m., Santos, E., Sarazin, F., Sarkar, B., Sarmento, R., Sarmiento, C. . a., Sato, R., Schauer, M., Scherini, V., Schieler, H., Schimp, M., Schmidt, D., Scholten, O., Schovánek, P., Schröder, F. . g., Schulz, A., Schulz, J., Schumacher, J., Sciutto, S. . j., Segreto, A., Settimo, M., Shadkam, A., Shellard, R. . c., Sigl, G., Silli, G., Sima, O., Śmiałkowski, A., Šmída, R., Snow, G. . r., Sommers, P., Sonntag, S., Sorokin, J., Squartini, R., Stanca, D., Stanič, S., Stasielak, J., Stassi, P., Strafella, F., Suarez, F., Suarez Durán, M., Sudholz, T., Suomijärvi, T., Supanitsky, A. . d., Swain, J., Szadkowski, Z., Taboada, A., Taborda, O. . a., Tapia, A., Theodoro, V. . m., Timmermans, C., Todero Peixoto, C. . j., Tomankova, L., Tomé, B., Torralba Elipe, G., Torres Machado, D., Torri, M., Travnicek, P., Trini, M., 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 Vliet, A., Varela, E., Vargas Cárdenas, B., Varner, G., Vázquez, J. . r., Vázquez, R. . a., Veberič, D., Vergara Quispe, I. . d., Verzi, V., Vicha, J., Villaseñor, L., Vorobiov, S., Wahlberg, H., Wainberg, O., Walz, D., Watson, A. . a., Weber, M., Weindl, A., Wiencke, L., Wilczyński, H., Winchen, T., Wittkowski, D., Wundheiler, B., Wykes, S., Yang, L., Yelos, D., Yushkov, A., Zas, E., Zavrtanik, D., Zavrtanik, M., Zepeda, A., Zimmermann, B., Ziolkowski, M., Zong, Z., Zuccarello, F., Bleve, Carla, Colalillo, R., Coluccia, MARIA RITA, D'Amico, Stefano, DE MITRI, Ivan, Guarino, F., Marsella, Giovanni, Martello, Daniele, Perrone, Lorenzo, Strafella, Francesco, Valore, L., Elementary Particle Physics, and Physics
Subjects: [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, magnetic fields, 7. Clean energy, 01 natural sciences, Ultrahigh-energy neutrino, gravitational waves, ultra-high energy cosmic rays, Observatory, 0103 physical sciences, GW151226, binary systems, High Energy Physics, 010303 astronomy & astrophysics, GeneralLiterature_REFERENCE(e.g.,dictionaries,encyclopedias,glossaries), gravitational wave, Ciencias Exactas, Pierre Auger Observatory, Physics, High Energy Astrophysical Phenomena (astro-ph.HE), GAMMA-RAY BURSTS, 010308 nuclear & particles physics, Gravitational wave, Física, neutrinos, ASTROFÍSICA, black holes, LIGO, Black hole, 13. Climate action, Experimental High Energy Physics, Física nuclear, High Energy Physics::Experiment, Neutrino, Gamma-ray burst, Astrophysics - High Energy Astrophysical Phenomena
Abstract: On September 14, 2015 the Advanced LIGO detectors observed their first gravitational wave (GW) transient GW150914. This was followed by a second GW event observed on December 26, 2015. Both events were inferred to have arisen from the merger of black holes in binary systems. Such a system may emit neutrinos if there are magnetic fields and disk debris remaining from the formation of the two black holes. With the surface detector array of the Pierre Auger Observatory we can search for neutrinos with energy Eν above 100 PeV from pointlike sources across the sky with equatorial declination from about -65° to +60°, and, in particular, from a fraction of the 90% confidence-level inferred positions in the sky of GW150914 and GW151226. A targeted search for highly inclined extensive air showers, produced either by interactions of downward-going neutrinos of all flavors in the atmosphere or by the decays of tau leptons originating from tau-neutrino interactions in the Earth's crust (Earth-skimming neutrinos), yielded no candidates in the Auger data collected within ±500 s around or 1 day after the coordinated universal time (UTC) of GW150914 and GW151226, as well as in the same search periods relative to the UTC time of the GW candidate event LVT151012. From the nonobservation we constrain the amount of energy radiated in ultrahigh-energy neutrinos from such remarkable events., La lista completa de autores que integran el documento puede consultarse en el archivo., Facultad de Ciencias Exactas, Instituto de Física La Plata
Published: 2016

29. Measurement of the radiation energy in the radio signal of extensive air showers as a universal estimator of cosmic-ray energy

Author: Alaa Kuotb Awad, Benoît Revenu, James Matthews, Alexandra Saftoiu, Alberto Filevich, Peter Hansen, Ivan De Mitri, I. Lhenry-Yvon, John Matthews, Peter Buchholz, Philipp Papenbreer, Petr Travnicek, H. Wahlberg, A. Nelles, R. Piegaia, I.M. Brancus, Alan Coleman, T. Hebbeker, Trent D. Grubb, D. Huber, Marco Aglietta, Eun-Joo Ahn, S. Vorobiov, K. Weidenhaupt, E.M. Holt, B. Wundheiler, A. Saleh, A. Parra, R. J. Lauer, Juan Manuel Figueira, S. Jansen, Bruno Daniel, Maria-Teresa Dova, Foteini Oikonomou, M. R. Hampel, Peter Mazur, J. Sorokin, Marcelo Augusto Leigui de Oliveira, Sarka Wykes, R. Meissner, Octavian Fratu, G. Parente, M. Trini, Roberta Colalillo, O. Wainberg, C. Bleve, P. Pieroni, S. Müller, Vincenzo Rizi, Nicusor Arsene, Julian Rautenberg, V. B. B. Mello, K. H. Becker, A. G. Mariazzi, Eric Mayotte, Jeffrey A. Johnsen, Sven Querchfeld, L. Perrone, R. C. Shellard, W. Docters, Carlos Hojvat, Ernesto Kemp, Xavier Bertou, Luis del Peral, Ugo Giaccari, Henryk Wilczyński, J. J. Beatty, Norbert Kunka, D. Nitz, Silvia Mollerach, D. Lebrun, S. Quinn, Sjoert van Velzen, Primo F. Gómez Vitale, R. Sato, S. Coutu, Norberto Fazzini, Antonio Bueno, Antonio Insolia, M. Josebachuili, Gualberto Avila, Ingomar Allekotte, G. Matthiae, Angela V. Olinto, O. Kambeitz, M. Ambrosio, Eva Santos, R. Krause, Jose Sanabria Gomez, M. Zavrtanik, Fred Sarazin, Lukas Nellen, B. Caccianiga, Julien Aublin, A. Shadkam, Amin Aminaei, Rafael Alves Batista, Jakub Vicha, Pedro Assis, Radomir Smida, Diego Harari, B. Gookin, P. H. Nguyen, Alberto Etchegoyen, Darius Reinert, Lorenzo Caccianiga, V. M. Theodoro, Tobias Winchen, D. Martello, Karen S. Caballero-Mora, Michael Unger, D. Melo, Luca Latronico, Guenter Sigl, D. Garcia-Pinto, Alessio Gorgi, Paul Sommers, A. Blanco, M. J. Cooper, S. Stanič, Carlos Medina, Tanguy Pierog, Mariano Gómez Berisso, D. Rogozin, Alejandro Almela, E. M. Santos, P. Heimann, Florian Gaté, J. R. Vázquez, Carla Bonifazi, Bernardo Vargas Cárdenas, A. C. Rovero, B. Tome, Marco Giammarchi, D. Garcia-Gamez, J. W. H. Gordon, Jose A. Bellido, L. Niemietz, S. Hartmann, Martin Erdmann, Jan Pękala, Hans Klages, A. Chiavassa, P. Sanchez-Lucas, Vitor de Souza, Bruce R. Dawson, Tim Huege, Carola Dobrigkeit, M. Plum, P. Abreu, Miguel Mostafá, C. Porowski, S. Sonntag, Markus Risse, Christian Sarmiento-Cano, B. Vlcek, Dariusz Glas, Diego Ravignani, O. A. Taborda, M. Settimo, M. Blanco, Mário Pimenta, Gregory R Snow, Pablo Ristori, P. H. Kasper, Gaetano Salina, Maria Rita Coluccia, Yogendra N. Srivastava, Alan Watson, Glennys R. Farrar, C. Jarne, A. Śmiałkowski, Andreas Weindl, Jaime Rosado, R. Cester, Alina Mihaela Badescu, F. Sánchez, N. Awal, Beatriz García, Jeffrey Brack, Olaf Scholten, Humberto Ibarguen Salazar, J. W. Cronin, Harald Schieler, Antoine Letessier-Selvon, C. Aramo, B. Mitrica, Heino Falcke, Nicolás González, Mihai Niculescu-Oglinzanu, Jonny Kleinfeller, K. Louedec, Arnulfo Zepeda, Armando di Matteo, G. Cocciolo, Roger W Clay, R. López, M. Mallamaci, F. G. Schröder, Mary Lucia Díaz Castro, Denise Boncioli, Jiri Chudoba, P. Lebrun, Alex Kääpä, Alberto Segreto, G. Toma, Benedikt Zimmermann, Rúben Conceição, R. Vasquez, Dusan Mandat, Colin Baus, Darko Veberič, D. Martraire, Oscar Martínez Bravo, Miroslav Hrabovský, T. Yapici, Alexey Yushkov, G. A. Anastasi, Pascal Lautridou, W. R. Carvalho, Dieter Heck, Martin Urban, G. S. Varner, Nataliia Borodai, Toshihiro Fujii, A. Menshikov, C. Morello, Jaroslaw Stasielak, Luis A. Anchordoqui, Markus Roth, N. Griffith, S. G. Blaess, Niraj Dhital, Jörg R. Hörandel, Thomas Harrison, Jaime de Oliveira, I. Valiño, H. Blümer, Max Malacari, Lili Yang, Laura Valore, L. Lopes, Lukas Middendorf, Corinne Berat, Piotr Homola, Lawrence Wiencke, Fausto Guarino, A. Filipčič, A. Aab, Johannes Schumacher, J. Neuser, Alex Tapia, Christine Peters, Ad M. van den Berg, Juan Pallotta, S. Le Coz, Jaime Alvarez-Muñiz, Alexandru Gherghel-Lascu, Mauricio Suaréz Durán, Petr Schovanek, L. Caramete, Rita dos Anjos, João de Mello Neto, H. Gemmeke, Peter L. Biermann, Sergio Sciutto, L. Ochilo, T. Suomijärvi, Karl-Heinz Kampert, Antonella Castellina, M. I. Micheletti, Federico Suarez, A. Schulz, J. Stapleton, L. Molina-Bueno, Q. Hasankiadeh, L. Tomankova, F. Arqueros, P. Necesal, Daniel Pakk Selmi-Dei, Imen Al Samarai, Martina Bohacova, David Walz, Johannes Schulz, Ruben Squartini, Paolo Privitera, F. Diogo, Juan Carlos D'Olivo, Patrick van Bodegom, Esteban Roulet, Patrick Allison, I. A. Minaya, Hernán Asorey, John Swain, Thomas Bretz, R.R. Prado, Harm Schoorlemmer, John L. Harton, T. Paul, A. Lucero, Jan Ridky, Marc Weber, F. Werner, Katrin Link, Denis Stanca, Guus van Aar, D. Maurizio, A. P. Ferguson, Corbin Covault, Y. Petrov, Geraldina Golup, Alexander Grillo, Zbigniew Szadkowski, Alessio Porcelli, J. C. Diaz, Rodrigo Pelayo, Stijn Buitink, N. Hollon, Olivier Ravel, C. A. Moura, Jose F. Valdés Galicia, Brian Fick, Lino Miramonti, Luis A. Nunez, M. Buscemi, C. Scarso, C. Welling, Marcus Niechciol, V. Novotny, Arjen van Vliet, A. Stutz, E. Varela, Rossella Caruso, S. Mathys, M. Erfani, Eduardo Quel, Henry Glass, Michael Sutherland, Francisco Salesa Greus, Guillermo Torralba Elipe, Piera Luisa Ghia, I. Jandt, Octavian Sima, Manuel Platino, M. D. Rodríguez-Frías, M. Schauer, N. Pacheco, Tim Niggemann, D. Nosek, Jan Ebr, V. Scherini, Jimmy Masías Meza, M. Candusso, Peter Gorham, Valerio Pirronello, Charles Timmermans, L. Collica, Sergio Petrera, Paul M. Mantsch, Miroslav Palatka, Jesus Alvarez Castillo, J. Blazek, Gustavo Medina-Tanco, Anderson Fauth, Vincent Marin, Rogerio M. de Almeida, M. E. Bertaina, B. Sarkar, Christian Glaser, S. Messina, Claudio Di Giulio, L. Nožka, J. Espadanal, Diego Torres Machado, Paula Gina Isar, Pedro Brogueira, G. Cataldi, Sergio Dasso, Martín Miguel Freire, P. Billoir, Aida López Casado, Carlos J. Todero Peixoto, G. Marsella, Daniel Kuempel, Carlos Escobar, R.M. Kieckhafer, Iuri Muniz Pepe, Maria Giller, Hermann-Josef Mathes, A. Cordier, Ivone F. M. Albuquerque, Ke Fang, Gašper Kukec Mezek, I. Katkov, Richard Dallier, Francesca Zuccarello, Kai Daumiller, Maurice Stephan, M. Ziolkowski, A. Tonachini, A.E. Herve, F. Montanet, J. Maller, V. Verzi, David Schmidt, S. Sánchez Navas, Jose Chinellato, Lorenzo Cazon, Ioana Codrina Maris, Ricardo Vázquez, Giuseppe De Mauro, G. C. Hill, Ralph Engel, Andreas Haungs, M. Videla, A. Daniel Supanitsky, Matthias Kleifges, H. Martinez, David Wittkowski, Germano Guedes, Danielle LaHurd, Olivier Deligny, Marcio Aparecido Muller, A. Dorofeev, L. Villaseñor, Marco Cilmo, Jorge Rubén Rodriguez Rojo, A. Bridgeman, E. Petermann, S. J. Saffi, Markus Lauscher, J. Phuntsok, Raul Sarmento, M. Prouza, Bianca Keilhauer, A. G. Chavez, Enrique Zas, Sijbrand J. de Jong, Fernando Contreras, N. Krohm, Miroslav Pech, R. Ulrich, Pavel Horvath, P. Gouffon, Allan Widom, Danilo Zavrtanik, Gero Müller, Sofia Andringa, A. Tepe, Research unit Nuclear & Hadron Physics, Research unit Astroparticle Physics, Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes [2016-2019] (UGA [2016-2019]), 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), 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), Pierre Auger Collaboration, 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), 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., Anastasi, G. A., Anchordoqui, L., Andringa, S., Aramo, C., Arqueros, F., Arsene, N., Asorey, H., Assis, P., Aublin, J., Avila, G., Awal, N., Badescu, A. M., 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., Blazek, J., Bleve, C., Blümer, H., Boháčová, M., Boncioli, D., Bonifazi, C., Borodai, N., Brack, J., Brancus, I., Bretz, T., Bridgeman, A., Brogueira, P., 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., 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., 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., Dos Anjos, R. C., 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., Fick, B., Figueira, J. M., Filevich, A., Filipčič, A., Fratu, O., Freire, M. M., Fujii, T., García, B., Garcia Gamez, D., 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., Guarino, Fausto, 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., Keilhauer, B., Kemp, E., Kieckhafer, R. M., Klages, H. O., Kleifges, M., Kleinfeller, J., Krause, R., Krohm, N., Kuempel, D., Kukec Mezek, G., Kunka, N., Kuotb Awad, A. W., 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., Lucero, A., Malacari, M., Mallamaci, M., Maller, J., Mandat, D., Mantsch, P., Mariazzi, A. G., Marin, V., Mariş, I. C., Marsella, G., Martello, D., Martinez, H., Martínez Bravo, O., Martraire, D., Masías Meza, J. J., Mathes, H. J., Mathys, S., Matthews, J., Matthews, J. A. J., Matthiae, G., Maurizio, D., Mayotte, E., Mazur, P. O., Medina, C., Medina Tanco, G., Meissner, R., Mello, V. B. B., Melo, D., Menshikov, A., Messina, S., 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., 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., Núñez, L. A., 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., 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., Quel, E. J., Querchfeld, S., Quinn, S., Rautenberg, J., Ravel, O., Ravignani, D., Reinert, D., Revenu, B., Ridky, J., Risse, M., Ristori, P., Rizi, V., Rodrigues De Carvalho, W., Rodriguez Rojo, J., Rodríguez Frías, M. D., Rogozin, D., Rosado, J., Roth, M., Roulet, E., Rovero, A. C., Saffi, S. J., Saftoiu, A., Salazar, H., Saleh, A., Salesa Greus, F., Salina, G., Sanabria Gomez, J. D., Sánchez, F., Sanchez Lucas, P., Santos, E., Santos, E. M., Sarazin, F., Sarkar, B., Sarmento, R., Sarmiento Cano, C., Sato, R., Scarso, C., Schauer, M., Scherini, V., Schieler, H., 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., Sigl, G., Sima, O., Śmiałkowski, A., Šmída, R., Snow, G. R., Sommers, P., Sonntag, S., Sorokin, J., Squartini, R., Srivastava, Y. N., Stanca, D., Stanič, S., Stapleton, J., Stasielak, J., Stephan, M., Stutz, A., Suarez, F., Suarez Durán, M., Suomijärvi, T., Supanitsky, A. D., Sutherland, M. S., Swain, J., Szadkowski, Z., Taborda, O. A., Tapia, A., Tepe, A., Theodoro, V. M., Timmermans, C., Todero Peixoto, C. J., Toma, G., Tomankova, L., Tomé, B., Tonachini, A., Torralba Elipe, G., Torres Machado, D., Travnicek, P., Trini, M., 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., 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., Welling, C., 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., Zimmermann, B., Ziolkowski, M., Zuccarello, F., 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), 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), 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, Anastasi G A, Anchordoqui L, Andringa S, Aramo C, Arqueros F, Arsene N, Asorey H, Assis P, Aublin J, Avila G, Awal N, Badescu A M, 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, Blazek J, Bleve C, Blümer H, Boháčová M, Boncioli D, Bonifazi C, Borodai N, Brack J, Brancus I, Bretz T, Bridgeman A, Brogueira P, 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, 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, Dos Anjos R C, 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, Fick B, Figueira J M, Filevich A, Filipčič A, Fratu O, Freire M M, Fujii T, García B, Garcia-Gamez D, 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, 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, Keilhauer B, Kemp E, Kieckhafer R M, Klages H O, Kleifges M, Kleinfeller J, Krause R, Krohm N, Kuempel D, Kukec Mezek G, Kunka N, Kuotb Awad A W, 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, Lucero A, Malacari M, Mallamaci M, Maller J, Mandat D, Mantsch P, Mariazzi A G, Marin V, Mariş I C, Marsella G, Martello D, Martinez H, Martínez Bravo O, Martraire D, Masías Meza J J, Mathes H J, Mathys S, Matthews J, Matthews J A J, Matthiae G, Maurizio D, Mayotte E, Mazur P O, Medina C, Medina-Tanco G, Meissner R, Mello V B B, Melo D, Menshikov A, Messina S, 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, 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, Núñez L A, 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, Quel E J, Querchfeld S, Quinn S, Rautenberg J, Ravel O, Ravignani D, Reinert D, Revenu B, Ridky J, Risse M, Ristori P, Rizi V, Rodrigues de Carvalho W, Rodriguez Rojo J, Rodríguez-Frías M D, Rogozin D, Rosado J, Roth M, Roulet E, Rovero A C, Saffi S J, Saftoiu A, Salazar H, Saleh A, Salesa Greus F, Salina G, Sanabria Gomez J D, Sánchez F, Sanchez-Lucas P, Santos E, Santos E M, Sarazin F, Sarkar B, Sarmento R, Sarmiento-Cano C, Sato R, Scarso C, Schauer M, Scherini V, Schieler H, 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, Sigl G, Sima O, Śmiałkowski A, Šmída R, Snow G R, Sommers P, Sonntag S, Sorokin J, Squartini R, Srivastava Y N, Stanca D, Stanič S, Stapleton J, Stasielak J, Stephan M, Stutz A, Suarez F, Suarez Durán M, Suomijärvi T, Supanitsky A D, Sutherland M S, Swain J, Szadkowski Z, Taborda O A, Tapia A, Tepe A, Theodoro V M, Timmermans C, Todero Peixoto C J, Toma G, Tomankova L, Tomé B, Tonachini A, Torralba Elipe G, Torres Machado D, Travnicek P, Trini M, 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, Welling C, 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, 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, Anastasi, G. A, Anchordoqui, L, Andringa, S, Aramo, C, Arqueros, F, Arsene, N, Asorey, H, Assis, P, Aublin, J, Avila, G, Awal, N, Badescu, A. M, 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, Blazek, J, Bleve, Carla, Blümer, H, Boháčová, M, Boncioli, D, Bonifazi, C, Borodai, N, Brack, J, Brancus, I, Bretz, T, Bridgeman, A, Brogueira, P, 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, 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, Dos Anjos, R. C, 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, Fick, B, Figueira, J. M, Filevich, A, Filipčič, A, Fratu, O, Freire, M. M, Fujii, T, García, B, Garcia Gamez, D, 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, 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, Keilhauer, B, Kemp, E, Kieckhafer, R. M, Klages, H. O, Kleifges, M, Kleinfeller, J, Krause, R, Krohm, N, Kuempel, D, Kukec Mezek, G, Kunka, N, Kuotb Awad, A. W, 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, Lucero, A, Malacari, M, Mallamaci, M, Maller, J, Mandat, D, Mantsch, P, Mariazzi, A. G, Marin, V, Mariş, I. C, Marsella, Giovanni, Martello, Daniele, Martinez, H, Martínez Bravo, O, Martraire, D, Masías Meza, J. J, Mathes, H. J, Mathys, S, Matthews, J, Matthews, J. A. J, Matthiae, G, Maurizio, D, Mayotte, E, Mazur, P. O, Medina, C, Medina Tanco, G, Meissner, R, Mello, V. B. B, Melo, D, Menshikov, A, Messina, S, 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, 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, Núñez, L. A, 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, Quel, E. J, Querchfeld, S, Quinn, S, Rautenberg, J, Ravel, O, Ravignani, D, Reinert, D, Revenu, B, Ridky, J, Risse, M, Ristori, P, Rizi, V, Rodrigues de Carvalho, W, Rodriguez Rojo, J, Rodríguez Frías, M. D, Rogozin, D, Rosado, J, Roth, M, Roulet, E, Rovero, A. C, Saffi, S. J, Saftoiu, A, Salazar, H, Saleh, A, Salesa Greus, F, Salina, G, Sanabria Gomez, J. D, Sánchez, F, Sanchez Lucas, P, Santos, E, Santos, E. M, Sarazin, F, Sarkar, B, Sarmento, R, Sarmiento Cano, C, Sato, R, Scarso, C, Schauer, M, Scherini, V, Schieler, H, 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, Sigl, G, Sima, O, Śmiałkowski, A, Šmída, R, Snow, G. R, Sommers, P, Sonntag, S, Sorokin, J, Squartini, R, Srivastava, Y. N, Stanca, D, Stanič, S, Stapleton, J, Stasielak, J, Stephan, M, Stutz, A, Suarez, F, Suarez Durán, M, Suomijärvi, T, Supanitsky, A. D, Sutherland, M. S, Swain, J, Szadkowski, Z, Taborda, O. A, Tapia, A, Tepe, A, Theodoro, V. M, Timmermans, C, Todero Peixoto, C. J, Toma, G, Tomankova, L, Tomé, B, Tonachini, A, Torralba Elipe, G, Torres Machado, D, Travnicek, P, Trini, M, 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, Welling, C, 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, Zimmermann, B, Ziolkowski, M, Elementary Particle Physics, and Physics
Subjects: Ciencias Físicas, Astronomy, General Physics and Astronomy, ultra-high energy cosmic rays, Astrophysics, 01 natural sciences, High Energy Physics - Experiment, purl.org/becyt/ford/1 [https], High Energy Physics - Experiment (hep-ex), CODALEMA, Observatory, [PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex], GeneralLiterature_REFERENCE(e.g.,dictionaries,encyclopedias,glossaries), High Energy Astrophysical Phenomena (astro-ph.HE), Physics, Range (particle radiation), Radio detector, TUNKA-REX, Settore FIS/01 - Fisica Sperimentale, Detector, Astrophysics::Instrumentation and Methods for Astrophysics, Radio Technique, Física nuclear, Astrophysics - High Energy Astrophysical Phenomena, Astrophysics - Instrumentation and Methods for Astrophysics, radio emission, CIENCIAS NATURALES Y EXACTAS, Radio wave, [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], Astrophysics::High Energy Astrophysical Phenomena, FOS: Physical sciences, Cosmic ray, Astrophysics::Cosmology and Extragalactic Astrophysics, Physics and Astronomy (all), 0103 physical sciences, extensive air showers, High Energy Physics, ultra-high energy cosmic rays, extensive air showers, radio emission, 010306 general physics, Instrumentation and Methods for Astrophysics (astro-ph.IM), Cosmic rays, Pierre Auger Observatory, 010308 nuclear & particles physics, Radiant energy, Física, LOFAR, purl.org/becyt/ford/1.3 [https], ASTROFÍSICA, SIMULATIONS, Computational physics, Astronomía, COREAS, Experimental High Energy Physics, ARRAY, EMISSION, SIMULATIONS, LOFAR, EMISSION
Abstract: We measure the energy emitted by extensive air showers in the form of radio emission in the frequency range from 30 to 80 MHz. Exploiting the accurate energy scale of the Pierre Auger Observatory, we obtain a radiation energy of 15.8±0.7(stat)±6.7(syst) MeV for cosmic rays with an energy of 1 EeV arriving perpendicularly to a geomagnetic field of 0.24 G, scaling quadratically with the cosmic-ray energy. A comparison with predictions from state-of-the-art first-principles calculations shows agreement with our measurement. The radiation energy provides direct access to the calorimetric energy in the electromagnetic cascade of extensive air showers. Comparison with our result thus allows the direct calibration of any cosmic-ray radio detector against the well-established energy scale of the Pierre Auger Observatory., La lista completa de autores que integran el documento puede consultarse en el archivo, Instituto de Física La Plata
Published: 2016

30. Search for ultrarelativistic magnetic monopoles with the Pierre Auger Observatory

Author: Johannes Schulz, M. Pimenta, A. Aab, J. Biteau, E.M. Holt, A. Saleh, L. Caramete, Maria-Teresa Dova, M. R. Hampel, H. Gemmeke, Florian Lukas Briechle, M. I. Micheletti, Sarka Wykes, D. Torres Machado, Octavian Fratu, Paula Gina Isar, F. Salesa Greus, R.C. dos Anjos, Julian Rautenberg, J. Espadanal, M. Palatka, G. Cataldi, A. C. Fauth, Luis A. Nunez, Carla Bonifazi, Jose A. Bellido, Jaime Alvarez-Muñiz, G. Kukec Mezek, John N. Matthews, R. M. Kieckhafer, E. Varela, J.D. Sanabria Gomez, D. Yelos, M. E. Bertaina, I. Naranjo, A. Menshikov, R. Sarmento, S. Sonntag, Marcus Niechciol, Jesús Peña-Rodríguez, O. Wainberg, Alexandru Gherghel-Lascu, T. Suomijärvi, A. van Vliet, Andreas Haungs, B. García, Tobias Winchen, Antonio Bueno, M. Josebachuili, L. Lopes, Alberto Daniel Supanitsky, G. De Mauro, C. A. Sarmiento, I.D. Vergara Quispe, A. Dorofeev, Gualberto Avila, R. López, Ingomar Allekotte, Jörg R. Hörandel, Karen S. Caballero-Mora, F. Canfora, Z. Zong, Diego Harari, B. Gookin, S. Querchfeld, M. Zavrtanik, Paul Sommers, A. Blanco, L. Ochilo, Angela V. Olinto, C. Di Giulio, Markus Roth, J. F. Valdés Galicia, Miroslav Hrabovský, I. De Mitri, Dieter Heck, P. Gouffon, Igor Katkov, P. H. Nguyen, E. M. Santos, L. Niemietz, R.J. Barreira Luz, G. P. Guedes, Toshihiro Fujii, G. A. Anastasi, P. Abreu, Martin Urban, A. Kuotb Awad, J. L. Harton, S. G. Blaess, B. Vargas Cárdenas, Fausto Guarino, J. Pallotta, E. J. Quel, M. J. Cooper, F. Sánchez, Q. Luce, Carlos Medina, Martin Erdmann, D. Ravignani, I. A. Minaya, B. Keilhauer, André Schulz, L. Villaseñor, Luis A. Anchordoqui, J. Debatin, Peter Hansen, Tim Niggemann, Peter Buchholz, D. Nosek, Bruce R. Dawson, A. Fuster, Tim Huege, H. Glass, I. Valiño, S. J. Sciutto, Katrin Link, Valerio Pirronello, M. A. Leigui de Oliveira, I.M. Brancus, M. Platino, Danielle LaHurd, Olivier Deligny, J. Neuser, Johannes Schumacher, C. Aramo, Juan Carlos D'Olivo, Roger W Clay, B. Revenu, J. R. Vázquez, G. S. Varner, Marco Aglietta, V. Scherini, Esteban Roulet, M. Suarez Durán, Andreas Weindl, B. Mitrica, Heino Falcke, Francesco Strafella, I. C. Mariş, Hernan Wahlberg, C. J. Todero Peixoto, Stefano D'Amico, P. Sanchez-Lucas, P. Kasper, M. Gómez Berisso, M. Ambrosio, R. C. Shellard, F. Salamida, J. Stasielak, S. Coutu, J. Vicha, Norberto Fazzini, D. Garcia-Pinto, Miroslav Pech, R. R. Prado, Petr Schovanek, Antonio Insolia, Maria Rita Coluccia, Bruno Daniel, A. Parra, Foteini Oikonomou, J. J. Masías Meza, Jeffrey A. Johnsen, S. Quinn, Günter Sigl, D. Nitz, Andrej Dundovic, Lorenzo Caccianiga, V. M. Theodoro, Dusan Mandat, P. Ristori, M. Trini, Alexandra Saftoiu, Alina Mihaela Badescu, I. Lhenry-Yvon, A. Cancio, Pavel Horvath, N. Krohm, G. Rodriguez Fernandez, G. Torralba Elipe, R. Krause, P. Stassi, C. Porowski, M. Prouza, V. Verzi, Mariangela Settimo, J. Rodriguez Rojo, Nicolás González, Radomir Smida, S. Müller, Jan Pękala, A. E. Herve, L. R. Wiencke, B. Sarkar, H. Nožka, Jose Chinellato, Christian Glaser, A. Yushkov, B. Andrada, Marco Torri, J. D. Swain, David Schmidt, M. L. Díaz Castro, G. Farrar, Carola Dobrigkeit, M. Plum, A. G. Chavez, A. Gorgi, Denis Stanca, Sofia Andringa, R. Cester, Nicusor Arsene, A. Tapia, Florian Gaté, M. Kleifges, D. Zavrtanik, B. Tome, Peter Mazur, G. Müller, V. de Souza, Max Malacari, Lili Yang, Enrique Zas, Alan Watson, A. Di Matteo, Francesca Zuccarello, A. Letessier-Selvon, Denise Boncioli, B. Wundheiler, H. Wilczyński, P. Billoir, Dariusz Glas, Fernando Contreras, O. Kambeitz, Corinne Berat, E. Mayotte, K. H. Becker, M. Unger, Gregory R Snow, A. Segreto, Philipp Papenbreer, Lorenzo Cazon, Q. Hasankiadeh, Mihai Niculescu-Oglinzanu, J. Alvarez Castillo, L. Molina-Bueno, D. Melo, I. Al Samarai, Piotr Homola, David Walz, Ana Martina Botti, I. Jandt, F. Diogo, R. M. de Almeida, G. Marsella, Marco Giammarchi, R. Squartini, T. Paul, L. A. S. Pereira, Maria Giller, A. Taboada, D. Pakk Selmi-Dei, R. Sato, L. Nellen, Ralf Ulrich, C. Morello, P.F. Gómez Vitale, G. C. Hill, R. A. Vázquez, Gaia Silli, Ralph Engel, A. Filipčič, Paul M. Mantsch, F. Sarazin, A. Bridgeman, G. Medina-Tanco, J. Ridky, G. van Aar, D. Reinert, Marc Weber, M. Mallamaci, Tanguy Pierog, S. J. Saffi, F. G. Schröder, Benedikt Zimmermann, Rúben Conceição, Zbigniew Szadkowski, Peter L. Biermann, Rodrigo Pelayo, Stijn Buitink, E. Santos, R. Piegaia, Markus Lauscher, F. Pedreira, A. Śmiałkowski, J. Phuntsok, M. M. Freire, R. Ramos-Pollan, Paolo Privitera, J. Hulsman, W. Rodrigues de Carvalho, J. W. Cronin, P. van Bodegom, P. Lebrun, Nataliia Borodai, Lukas Middendorf, Christine Peters, Hernán Asorey, Martina Bohacova, J. Sorokin, S. J. De Jong, V. Novotny, L. Valore, Rossella Caruso, A. Lucero, S. Mathys, M. Erfani, Octavian Sima, Ugo Giaccari, F. Montanet, Petr Travnicek, M. Schauer, Alan Coleman, Trent D. Grubb, Juan Manuel Figueira, Roberta Colalillo, A. G. Mariazzi, J. R. T. de Mello Neto, Peter Gorham, P. L. Ghia, Charles Timmermans, L. Collica, Marcio Aparecido Muller, L. Perrone, Jiri Chudoba, Thomas Harrison, P. Pieroni, F. Arqueros, N. Kunka, R. Gaior, F. Suarez, Thomas Hebbeker, Sergio Dasso, Tristan Sudholz, Hermann-Josef Mathes, Kai Daumiller, J. A.J. Matthews, Xavier Bertou, Jeffrey Brack, Olaf Scholten, A. Zepeda, Humberto Ibarguen Salazar, Pedro Assis, Harald Schieler, A. Etchegoyen, P. Heimann, E. Kemp, Serguei Vorobiov, D. Mockler, O. A. Taborda, H. Martinez, Miguel Mostafa, L. Tomankova, A. López Casado, Brian Fick, Samo Stanič, J. J. Beatty, Silvia Mollerach, G. Matthiae, Julien Aublin, A. Shadkam, D. Martello, S. Jansen, David Wittkowski, A. C. Rovero, C. Bleve, Alexandru Balaceanu, Vincenzo Rizi, M. Ziolkowski, O. Martínez Bravo, Thomas Bretz, Corbin Covault, Geraldina Golup, Alexander Grillo, Lino Miramonti, M. Risse, Jonathan Blazek, G. Parente, Carlos Hojvat, R. Legumina, M. Buscemi, Jan Ebr, Sergio Petrera, D. Rogozin, J. de Oliveira, H.O. Klages, Alejandro Almela, S. Messina, Julian Kemp, Gaetano Salina, Michael Schimp, A.M. van den Berg, Darko Veberič, Alex Kääpä, Colin Baus, J. Kleinfeller, Daniel Kuempel, Carlos Escobar, Ivone F. M. Albuquerque, Ke Fang, Karl-Heinz Kampert, Antonella Castellina, Research unit Astroparticle Physics, Research unit Nuclear & Hadron Physics, 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 Physique Subatomique et de Cosmologie (LPSC), Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes [2016-2019] (UGA [2016-2019]), 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 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), Pierre Auger, Aab A., Abreu P., Aglietta M., Al Samarai I., Albuquerque I.F.M., Allekotte I., Almela A., Alvarez Castillo J., Alvarez-Muñiz J., Ambrosio M., Anastasi G.A., Anchordoqui L., Andrada B., Andringa S., Aramo C., Arqueros F., Arsene N., Asorey H., Assis P., Aublin J., Avila G., Badescu A.M., Balaceanu A., Barreira Luz R.J., Baus C., Beatty J.J., Becker K.H., Bellido J.A., Berat C., Bertaina M.E., Bertou X., Biermann P.L., Billoir P., Biteau J., Blaess S.G., Blanco A., Blazek J., Bleve C., Boháčová M., Boncioli D., Bonifazi C., Borodai N., Botti A.M., Brack J., Brancus I., Bretz T., Bridgeman A., Briechle F.L., Buchholz P., Bueno A., Buitink S., Buscemi M., Caballero-Mora K.S., Caccianiga L., Cancio A., Canfora F., Caramete L., Caruso R., Castellina A., Cataldi G., Cazon L., Cester R., Chavez A.G., Chinellato J.A., Chudoba J., Clay R.W., Colalillo R., Coleman A., Collica L., Coluccia M.R., Conceição R., Contreras F., Cooper M.J., Coutu S., Covault C.E., Cronin J., D'Amico S., 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., Debatin J., Deligny O., Di Giulio C., Di Matteo A., Díaz Castro M.L., Diogo F., Dobrigkeit C., D'Olivo J.C., Dorofeev A., dos Anjos R.C., Dova M.T., Dundovic A., 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., Fick B., Figueira J.M., Filipčič A., Fratu O., Freire M.M., Fujii T., Fuster A., Gaior R., García B., Garcia-Pinto D., Gaté 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., Gorgi A., Gorham P., Gouffon P., Grillo A.F., Grubb T.D., Guarino F., Guedes G.P., Hampel M.R., Hansen P., Harari D., Harrison T.A., Harton J.L., Hasankiadeh Q., Haungs A., Hebbeker T., Heck D., Heimann P., Herve A.E., Hill G.C., Hojvat C., Holt E., Homola P., Hörandel J.R., Horvath P., Hrabovský M., Huege T., Hulsman J., Insolia A., Isar P.G., Jandt I., Jansen S., Johnsen J.A., Josebachuili M., Kääpä A., Kambeitz O., Kampert K.H., Kasper P., Katkov I., Keilhauer B., Kemp E., Kemp J., Kieckhafer R.M., Klages H.O., Kleifges M., Kleinfeller J., Krause R., Krohm N., Kuempel D., Kukec Mezek G., Kunka N., Kuotb Awad A., Lahurd D., Lauscher M., Lebrun P., Legumina R., Leigui de Oliveira M.A., Letessier-Selvon A., Lhenry-Yvon I., Link K., Lopes L., López R., López Casado A., Luce Q., Lucero A., Malacari M., Mallamaci M., Mandat D., Mantsch P., Mariazzi A.G., Mariş I.C., Marsella G., Martello D., Martinez H., Martínez Bravo O., Masías Meza J.J., Mathes H.J., Mathys S., Matthews J., Matthews J.A.J., Matthiae G., Mayotte E., Mazur P.O., Medina C., Medina-Tanco G., Melo D., Menshikov A., Messina S., Micheletti M.I., Middendorf L., Minaya I.A., Miramonti L., Mitrica B., Mockler D., Molina-Bueno L., Mollerach S., Montanet F., Morello C., Mostafá M., Müller G., Muller M.A., Müller S., Naranjo I., Nellen L., Neuser J., Nguyen P.H., Niculescu-Oglinzanu M., Niechciol M., Niemietz L., Niggemann T., Nitz D., Nosek D., Novotny V., Nožka H., Núñez L.A., Ochilo L., Oikonomou F., Olinto A., Pakk Selmi-Dei D., Palatka M., Pallotta J., Papenbreer P., Parente G., Parra A., Paul T., Pech M., Pedreira F., Pękala J., Pelayo R., Peña-Rodriguez J., Pereira L. A. S., Perrone L., Peters C., Petrera S., Phuntsok J., Piegaia R., Pierog T., Pieroni P., Pimenta M., Pirronello V., Platino M., Plum M., Porowski C., Prado R.R., Privitera P., Prouza M., Quel E.J., Querchfeld S., Quinn S., Ramos-Pollan R., Rautenberg J., Ravignani D., Reinert D., Revenu B., Ridky J., Risse M., Ristori P., Rizi V., Rodrigues de Carvalho W., Rodriguez Fernandez G., Rodriguez Rojo J., Rogozin D., Roth M., Roulet E., Rovero A.C., Saffi S.J., Saftoiu A., Salamida F., Salazar H., Saleh A., Salesa Greus F., Salina G., Sanabria Gomez J.D., Sánchez F., Sanchez-Lucas P., Santos E.M., Santos E., Sarazin F., Sarkar B., Sarmento R., Sarmiento C.A., Sato R., Schauer M., Scherini V., Schieler H., Schimp M., Schmidt D., Scholten O., Schovánek P., Schröder F.G., Schulz A., Schulz J., Schumacher J., Sciutto S.J., Segreto A., Settimo M., Shadkam A., Shellard R.C., Sigl G., Silli G., Sima O., Śmiałkowski A., Šmída R., Snow G.R., Sommers P., Sonntag S., Sorokin J., Squartini R., Stanca D., Stanič S., Stasielak J., Stassi P., Strafella F., Suarez F., Suarez Durán M., Sudholz T., Suomijärvi T., Supanitsky A.D., Swain J., Szadkowski Z., Taboada A., Taborda O.A., Tapia A., Theodoro V.M., Timmermans C., Todero Peixoto C.J., Tomankova L., Tomé B., Torralba Elipe G., Torres Machado D., Torri M., Travnicek P., Trini M., 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 Vliet A., Varela E., Vargas Cárdenas B., Varner G., Vázquez J.R., Vázquez R.A., Veberič D., Vergara Quispe I.D., Verzi V., Vicha J., Villaseñor L., Vorobiov S., Wahlberg H., Wainberg O., Walz D., Watson A.A., Weber M., Weindl A., Wiencke L., Wilczyński H., Winchen T., Wittkowski D., Wundheiler B., Wykes S., Yang L., Yelos D., Yushkov A., Zas E., Zavrtanik D., Zavrtanik M., Zepeda A., Zimmermann B., Ziolkowski M., Zong Z., Zuccarello F., 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), 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), Aab, A., Abreu, P., Aglietta, M., Al Samarai, I., Albuquerque, I. 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R., Hansen, P., Harari, D., Harrison, T. A., Harton, J. L., Hasankiadeh, Q., Haungs, A., Hebbeker, T., Heck, D., Heimann, P., Herve, A. E., Hill, G. C., Hojvat, C., Holt, E., Homola, P., Hörandel, J. R., Horvath, P., Hrabovský, M., Huege, T., Hulsman, J., Insolia, A., Isar, P. G., Jandt, I., Jansen, S., Johnsen, J. A., Josebachuili, M., Kääpä, A., Kambeitz, O., Kampert, K. H., Kasper, P., Katkov, I., Keilhauer, B., Kemp, E., Kemp, J., Kieckhafer, R. M., Klages, H. O., Kleifges, M., Kleinfeller, J., Krause, R., Krohm, N., Kuempel, D., Kukec Mezek, G., Kunka, N., Kuotb Awad, A., Lahurd, D., Lauscher, M., Lebrun, P., Legumina, R., Leigui de Oliveira, M. A., Letessier Selvon, A., Lhenry Yvon, I., Link, K., Lopes, L., López, R., López Casado, A., Luce, Q., Lucero, A., Malacari, M., Mallamaci, M., Mandat, D., Mantsch, P., Mariazzi, A. G., Mariş, I. C., Marsella, Giovanni, Martello, Daniele, Martinez, H., Martínez Bravo, O., Masías Meza, J. J., Mathes, H. J., Mathys, S., Matthews, J., Matthews, J. A. J., Matthiae, G., Mayotte, E., Mazur, P. O., Medina, C., Medina Tanco, G., Melo, D., Menshikov, A., Messina, S., Micheletti, M. I., Middendorf, L., Minaya, I. A., Miramonti, L., Mitrica, B., Mockler, D., Molina Bueno, L., Mollerach, S., Montanet, F., Morello, C., Mostafá, M., Müller, G., Muller, M. A., Müller, S., Naranjo, I., Nellen, L., Neuser, J., Nguyen, P. H., Niculescu Oglinzanu, M., Niechciol, M., Niemietz, L., Niggemann, T., Nitz, D., Nosek, D., Novotny, V., Nožka, H., Núñez, L. A., Ochilo, L., Oikonomou, F., Olinto, A., Pakk Selmi Dei, D., Palatka, M., Pallotta, J., Papenbreer, P., Parente, G., Parra, A., Paul, T., Pech, M., Pedreira, F., Pękala, J., Pelayo, R., Peña Rodriguez, J., Pereira, L. A. S., Perrone, Lorenzo, Peters, C., Petrera, S., Phuntsok, J., Piegaia, R., Pierog, T., Pieroni, P., Pimenta, M., Pirronello, V., Platino, M., Plum, M., Porowski, C., Prado, R. R., Privitera, P., Prouza, M., Quel, E. J., Querchfeld, S., Quinn, S., Ramos Pollan, R., Rautenberg, J., Ravignani, D., Reinert, D., Revenu, B., Ridky, J., Risse, M., Ristori, P., Rizi, V., Rodrigues de Carvalho, W., Rodriguez Fernandez, G., Rodriguez Rojo, J., Rogozin, D., Roth, M., Roulet, E., Rovero, A. C., Saffi, S. J., Saftoiu, A., Salamida, F., Salazar, H., Saleh, A., Salesa Greus, F., Salina, G., Sanabria Gomez, J. D., Sánchez, F., Sanchez Lucas, P., Santos, E. M., Santos, E., Sarazin, F., Sarkar, B., Sarmento, R., Sarmiento, C. A., Sato, R., Schauer, M., Scherini, V., Schieler, H., Schimp, M., Schmidt, D., Scholten, O., Schovánek, P., Schröder, F. G., Schulz, A., Schulz, J., Schumacher, J., Sciutto, S. J., Segreto, A., Settimo, M., Shadkam, A., Shellard, R. C., Sigl, G., Silli, G., Sima, O., Śmiałkowski, A., Šmída, R., Snow, G. R., Sommers, P., Sonntag, S., Sorokin, J., Squartini, R., Stanca, D., Stanič, S., Stasielak, J., Stassi, P., Strafella, Francesco, Suarez, F., Suarez Durán, M., Sudholz, T., Suomijärvi, T., Supanitsky, A. D., Swain, J., Szadkowski, Z., Taboada, A., Taborda, O. A., Tapia, A., Theodoro, V. M., Timmermans, C., Todero Peixoto, C. J., Tomankova, L., Tomé, B., Torralba Elipe, G., Torres Machado, D., Torri, M., Travnicek, P., Trini, M., 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 Vliet, A., Varela, E., Vargas Cárdenas, B., Varner, G., Vázquez, J. R., Vázquez, R. A., Veberič, D., Vergara Quispe, I. D., Verzi, V., Vicha, J., Villaseñor, L., Vorobiov, S., Wahlberg, H., Wainberg, O., Walz, D., Watson, A. A., Weber, M., Weindl, A., Wiencke, L., Wilczyński, H., Winchen, T., Wittkowski, D., Wundheiler, B., Wykes, S., Yang, L., Yelos, D., Yushkov, A., Zas, E., Zavrtanik, D., Zavrtanik, M., Zepeda, A., Zimmermann, B., Ziolkowski, M., Zong, Z., Zuccarello, F., Bleve, C., Colalillo, Roberta, Coluccia, M. R., D'Amico, S., De Almeida, R. M., De Jong, S. J., De Mello Neto, J. R. T., De Mitri, I., De Oliveira, J., De Souza, V., Dos Anjos, R. C., Guarino, Fausto, Leigui De Oliveira, M. A., Marsella, G., Martello, D., Pkala, J., Perrone, L., Rodrigues De Carvalho, W., Strafella, F., Valore, Laura, Van Aar, G., Van Bodegom, P., Van Den Berg, A. M., and Van Vliet, A.
Subjects: FLUORESCENCE YIELD, Astronomy, magnetic monopole, magnetic field, Astrophysics, 7. Clean energy, 01 natural sciences, Observatory, UHE Cosmic Rays, air-shower, Monte Carlo, 010303 astronomy & astrophysics, Magnetic Monopoles, media_common, Physics, High Energy Astrophysical Phenomena (astro-ph.HE), Settore FIS/01 - Fisica Sperimentale, Astrophysics::Instrumentation and Methods for Astrophysics, critical phenomena, ENERGY LOSS, DETECTOR, Auger, Magnetic field, observatory, Lorentz factor, ComputingMethodologies_DOCUMENTANDTEXTPROCESSING, symbols, Física nuclear, fluorescence, Astrophysics - High Energy Astrophysical Phenomena, spatial distribution [showers], Lorentz, atmosphere [showers], energy, FLUX, Nuclear and High Energy Physics, [PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], air, media_common.quotation_subject, Astrophysics::High Energy Astrophysical Phenomena, UHE [cosmic radiation], Magnetic monopole, FOS: Physical sciences, Cosmic ray, Nuclear physics, symbols.namesake, cosmic rays, 0103 physical sciences, ddc:530, High Energy Physics, Ciencias Exactas, fluorescence [detector], Pierre Auger Observatory, background, 010308 nuclear & particles physics, Física, ASTROFÍSICA, Universe, flux, ultrarelativistic magnetic monopoles, Air shower, 13. Climate action, Experimental High Energy Physics, relativistic, galaxy, ENERGY-LOSS
Abstract: We present a search for ultra-relativistic magnetic monopoles with the Pierre Auger Observatory. Such particles, possibly a relic of phase transitions in the early universe, would deposit a large amount of energy along their path through the atmosphere, comparable to that of ultrahigh-energy cosmic rays (UHECRs). The air shower profile of a magnetic monopole can be effectively distinguished by the fluorescence detector from that of standard UHECRs. No candidate was found in the data collected between 2004 and 2012, with an expected background of less than 0.1 event from UHECRs. The corresponding 90% confidence level (C.L.) upper limits on the flux of ultra-relativistic magnetic monopoles range from 10⁻¹⁹ (cm² sr s)⁻¹ for a Lorentz factor γ = 10⁹ to 2.5 × 10⁻²¹ (cm² sr s)⁻¹ for γ = 10¹². These results -the first obtained with a UHECR detector- improve previously published limits by up to an order of magnitude., La lista completa de autores que integran el documento puede consultarse en el archivo., Facultad de Ciencias Exactas, Instituto de Física La Plata
Published: 2016
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31. KASCADE-Grande experiment measurements of the cosmic ray spectrum and large scale anisotropy

Author: A. Chiavassa, D. Kang, S. Schoo, H. Schieler, H.O. Klages, Ralph Engel, F. Cossavella, Jörg R. Hörandel, K. H. Kampert, H. J. Mathes, H. Bozdog, Andreas Haungs, P. Doll, S. Ostapchenko, F.G. Schröder, Alexandru Gherghel-Lascu, A. Weindl, D. Huber, B. Mitrica, Markus Roth, K. Bekk, V. de Souza, R. Glasstetter, H.J. Gils, J. Wochele, Octavian Sima, Claus Grupen, P. Łuczak, H.J. Mayer, N. Palmieri, D. Heck, G.C. Trinchero, F. Di Pierro, D. Fuhrmann, J. Oehlschläger, E. Cantoni, G. Toma, W. D. Apel, H. Ulrich, M. E. Bertaina, T. Pierog, J. Milke, J. Blümer, I.M. Brancus, K. Link, J. Zabierowski, H. Rebel, J.C. Arteaga-Velázquez, Kai Daumiller, T. Huege, and C. Morello
Subjects: Physics, Nuclear and High Energy Physics, Particle physics, Muon, Cosmic Rays, Extensive Air Showers, Knee, Spectra, 010308 nuclear & particles physics, Electromagnetic spectrum, Hadron, Cosmic ray, Astrophysics, 01 natural sciences, Charged particle, Spectral line, KASCADE, 0103 physical sciences, Anisotropy, 010303 astronomy & astrophysics
Abstract: The KASCADE-Grande experiment operated at KIT from January 2004 to November 2012, measuring Extensive Air Showers (EAS) generated by primary cosmic rays in the 10 16 – 10 18 e V energy range. The experiment measured, for each single event, with a high resolution, the total number of charged particles ( N c h ) and of muons ( N μ ). In this contribution we summarize the results obtained 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 c h ratio. This technique allowed us to unveil a steepening of the spectrum of heavy primaries at E ∼ 10 16.92 ± 0.04 e V and a hardening of the spectrum of light primaries at E ∼ 10 17.08 ± 0.08 e V . (ii) A search for large scale anisotropies.
Published: 2016

32. Radio Propagation Environment Analysis for Neutrino Radio Detection in Salt Mines

Author: Teodor Petrescu, Alina Mihaela Badescu, G. Toma, Alexandra Saftoiu, I. Lazanu, B. Mitrica, Octavian Fratu, I.M. Brancus, Octavian Sima, and Simona Halunga
Subjects: Physics, Electromagnetic shower, Salt (cryptography), Astrophysics::High Energy Astrophysical Phenomena, Environment analysis, Acoustics, Astronomy, Physics and Astronomy(all), Pulse (physics), Radio propagation, Observatory, salt, UHE cosmic neutrinos, Neutrino, Radio detection, Cherenkov radiation
Abstract: a We consider a neutrino large-scale radio Cherenkov observatory in a Romanian salt mine. We include propagation effects on the radio signal generated and make a threshold analysis, taking into account how the pulse couples to a realistic receiver and signal-to-noise ratio limiting situations.
Published: 2012
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33. 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

34. Restoring the azimuthal symmetry of lateral distributions of charged particles in the range of the KASCADE-Grande experiment

Author: H. Rebel, G. Toma, M. Finger, C. Manailescu, Ralph Engel, Karl-Heinz Kampert, J.C. Arteaga, P. Doll, D. Kang, K. Bekk, J. Blümer, H. Bozdog, M. Wommer, J. Oehlschläger, A. Chiavassa, H. J. Mathes, R. Glasstetter, Markus Roth, Andreas Haungs, V. de Souza, Claus Grupen, C. Morariu, M. E. Bertaina, F. Cosavella, I.M. Brancus, H.J. Mayer, J. Zabierowski, J. Wochele, Octavian Sima, D. Heck, and T. Huege
Subjects: Nuclear physics, Azimuth, Physics, Nuclear and High Energy Physics, Range (particle radiation), Air shower, Distribution function, KASCADE, Particle, Particle density, Instrumentation, Charged particle
Abstract: The reconstruction of Extensive Air Showers (EAS) observed by particle detectors at the ground is based on the characteristics of observables like the lateral particle density and the arrival times. The lateral densities, inferred for different EAS components from detector data, are usually parameterised by applying various lateral distribution functions (LDFs). The LDFs are used in turn for evaluating quantities like the total number of particles or the density at particular radial distances. Typical expressions for LDFs anticipate azimuthal symmetry of the density around the shower axis. The deviations of the lateral particle density from this assumption arising from various reasons are smoothed out in the case of compact arrays like KASCADE, but not in the case of arrays like Grande, which only sample a smaller part of the azimuthal variation. KASCADE-Grande, an extension of the former KASCADE experiment, is a multi-component Extensive Air Shower (EAS) experiment located at the Karlsruhe Institute of Technology (Campus North), Germany. The lateral distributions of charged particles are deduced from the basic information provided by the Grande scintillators – the energy deposits – first in the observation plane, then in the intrinsic shower plane. In all steps azimuthal dependences should be taken into account. As the energy deposit in the scintillators is dependent on the angles of incidence of the particles, azimuthal dependences are already involved in the first step: the conversion from the energy deposits to the charged particle density. This is done by using the Lateral Energy Correction Function (LECF) that evaluates the mean energy deposited by a charged particle taking into account the contribution of other particles (e.g. photons) to the energy deposit. By using a very fast procedure for the evaluation of the energy deposited by various particles we prepared realistic LECFs depending on the angle of incidence of the shower and on the radial and azimuthal coordinates of the location of the detector. Mapping the lateral density from the observation plane onto the intrinsic shower plane does not remove the azimuthal dependences arising from geometric and attenuation effects, in particular for inclined showers. Realistic procedures for applying correction factors are developed. Specific examples of the bias due to neglecting the azimuthal asymmetries in the conversion from the energy deposit in the Grande detectors to the lateral density of charged particles in the intrinsic shower plane are given.
Published: 2011

35. A mobile detector for measurements of the atmospheric muon flux

Author: H. Rebel, A. Saftoiu, B. Mitrica, G. Toma, Romul Margineanu, A. Apostu, A. Haungs, Marian Petre, M. Petcu, M. Dima, I.M. Brancus, and Octavian Sima
Subjects: Physics, Muon, Physics and Astronomy (miscellaneous), 010308 nuclear & particles physics, Detector, Astronomy and Astrophysics, Scintillator, 7. Clean energy, 01 natural sciences, Coincidence, Nuclear physics, Overburden, 0103 physical sciences, Muon flux, Neutrino, 010306 general physics, Meter water equivalent, Remote sensing
Abstract: Measurements of the underground atmospheric muon flux are important in order to determine accurately the overburden in mwe (meter water equivalent) of an un- derground laboratory for appreciating which kind of exper- iments are feasible for that location. Slanic- Prohava is one of the 7 possible locations for the European large un- derground experiment LAGUNA (Large Apparatus studying Grand Unification and Neutrino Astrophysics). A mobile de- vice consisting of 2 scintillator plates ( 0.9 m 2 , each) one above the other and measuring in coincidence, was set-up for determining the muon flux. The detector it is installed on a van which facilitates measurements on different positions at the surface or in the underground and it is in operation since autumn 2009. The measurements of muon fluxes pre- sented in this contribution have been performed in the under- ground salt mine Slanic-Prahova, Romania, where IFIN-HH has built a low radiation level laboratory, and at the surface on different sites of Romania, at different elevations from 0 m a.s.l up to 655 m a.s.l. Based on our measurements we can say that Slanic site is a feasible location for LAGUNA in Unirea salt mine at a water equivalent depth of 600 mwe. The results have been compared with Monte-Carlo simula- tions performed with the simulation codes CORSIKA and MUSIC.
Published: 2011

36. 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

37. 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

38. THE EXTENSIVE AIR SHOWER EXPERIMENT KASCADE-GRANDE

Author: R. Engel, H. J. Mathes, M. Finger, Wolfgang Walkowiak, H.J. Mayer, J. Blümer, Andrea Chiavassa, A. Haungs, T. Pierog, Y. Kolotaev, B. Mitrica, S. Over, C. Grupen, J. Zabierowski, Markus Roth, Piera Luisa Ghia, F. Di Pierro, S. Nehls, D. Fuhrmann, F. Cossavella, J. Engler, H. Ulrich, Frank G. Schröder, H. Bozdog, J.C. Arteaga, J. Wochele, C. Morello, P. Łuczak, J. van Buren, M. E. Bertaina, J. Oehlschläger, D. Heck, J. Milke, Paula Gina Isar, F. Badea, K. Bekk, G.C. Trinchero, H. Rebel, J.R. Hörandel, M. Wommer, H.J. Gils, G. Schatz, D. Kickelbick, R. Glasstetter, V. de Souza, Kai Daumiller, T. Huege, G. Navarra, Donghwa Kang, H.O. Klages, M. Petcu, Peter Buchholz, I.M. Brancus, M. Brüggemann, M. Stümpert, A. Weindl, E. Cantoni, G. Toma, S. Ostapchenko, W. D. Apel, K. H. Kampert, Octavian Sima, H. Schieler, and P. Doll
Subjects: Nuclear physics, Physics, Muon, Air shower, KASCADE, Calorimeter (particle physics), Scintillation counter, Detector, Cosmic ray, Scintillator
Abstract: The extensive air shower experiment KASCADE-Grande (KArlsruhe Shower Core and Array DEtector and Grande array) is located on site of the Forschungszentrum Karlsruhe in Germany. The original KASCADE experiment consisted of a densely packed scintillator array with unshielded and shielded detectors for the measurement of the electromagnetic and muonic shower component independently, as well as muon tracking devices and a hadron calorimeter. The Grande array as an extension of KASCADE consists of 37 scintillation detector stations covering an area of 700×700 m2. The main goal for the combined measurements of KASCADE and Grande is the investigation of the energy spectrum and composition of primary cosmic rays in the energy range of 1016 to 1018 eV. In this paper an overview of the KASCADE-Grande experiment and recent results will be presented.
Published: 2011

39. 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

40. Muon Production Height investigated by the Air-Shower Experiment KASCADE-Grande

Author: T. Pierog, Frank G. Schröder, J.C. Arteaga, M. E. Bertaina, H. Blümer, J. Wochele, J. Milke, F. Badea, G. Toma, Piera Luisa Ghia, E. Cantoni, Octavian Sima, H. Rebel, Markus Roth, S. Nehls, C. Grupen, J. Engler, D. Heck, K. Bekk, J. Oehlschläger, Peter Buchholz, Paula Gina Isar, M. Stümpert, H. Schieler, I.M. Brancus, Wolfgang Walkowiak, B. Mitrica, Kai Daumiller, P. Łuczak, P. Doll, H.J. Mayer, A. Weindl, Andrea Chiavassa, J.R. Hörandel, M. Wommer, W. D. Apel, T. Huege, R. Engel, Y. Kolotaev, S. Ostapchenko, A. Haungs, F. Di Pierro, C. Morello, D. Kickelbick, H. Bozdog, V. de Souza, J. Zabierowski, D. Kang, H. Ulrich, R. Glasstetter, H.O. Klages, G.C. Trinchero, G. Navarra, M. Finger, S. Over, M. Petcu, K. H. Kampert, D. Fuhrmann, J. van Buren, M. Brüggemann, F. Cossavella, H.J. Gils, and H. J. Mathes
Subjects: Physics, Nuclear and High Energy Physics, Muon, Physics::Instrumentation and Detectors, Astrophysics::High Energy Astrophysical Phenomena, Track (disk drive), Detector, Astrophysics::Instrumentation and Methods for Astrophysics, Cosmic ray, Tracking (particle physics), Atomic and Molecular Physics, and Optics, Nuclear physics, Air shower, KASCADE, Electromagnetic shielding, High Energy Physics::Experiment
Abstract: A large area (128m2) Muon Tracking Detector (MTD), located within the KASCADE experiment, has been built with the aim to identify muons ( E μ > 0.8 GeV ) and their directions in extensive air showers by track measurements under more than 18 r.l. shielding. The orientation of the muon track with respect to the shower axis is expressed in terms of the radial- and tangential angles. By means of triangulation the muon production height H μ is determined. By means of H μ , a transition from light to heavy cosmic ray primary particles with increasing shower energy E o from 1–10 PeV is observed.
Published: 2009

41. The Air-Shower Experiment KASCADE-Grande

Author: G. Toma, M. Finger, Kai Daumiller, Wolfgang Walkowiak, F. Badea, Jörg R. Hörandel, F. Cossavella, M. Petcu, D. Kickelbick, H.J. Mayer, F. Di Pierro, C. Morello, Andrea Chiavassa, V. de Souza, R. Engel, E. Cantoni, G.C. Trinchero, S. Ostapchenko, T. Huege, S. Over, Frank G. Schröder, M. E. Bertaina, D. Fuhrmann, J.C. Arteaga, H. Schieler, M. Stümpert, Karl-Heinz Kampert, D. Kang, A. Weindl, H. Bozdog, H.J. Gils, M. Brüggemann, J. Milke, Peter Buchholz, P. Łuczak, I.M. Brancus, P. Doll, H.O. Klages, J. Blümer, C. Grupen, W. D. Apel, G. Navarra, H. J. Mathes, K. Bekk, Andreas Haungs, T. Pierog, J. Zabierowski, Piera Luisa Ghia, S. Nehls, Paula Gina Isar, H. Rebel, R. Glasstetter, Markus Roth, J. Engler, M. Wommer, Y. Kolotaev, J. Oehlschläger, B. Mitrica, H. Ulrich, J. Wochele, Octavian Sima, and D. Heck
Subjects: Physics, Nuclear and High Energy Physics, Muon, Physics::Instrumentation and Detectors, Astrophysics::High Energy Astrophysical Phenomena, Detector, Astrophysics::Instrumentation and Methods for Astrophysics, Cosmic ray, Tracking (particle physics), Atomic and Molecular Physics, and Optics, law.invention, Nuclear physics, Air shower, KASCADE, law, Shielded cable, Energy spectrum
Abstract: KASCADE-Grande is an extensive air shower experiment at the 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. An overview on the performance of the apparatus and first results will be given.
Published: 2009

42. Test of the hadronic interaction model EPOS with KASCADE air shower data

Author: J.R. Hörandel, W.D. Apel, J.C. Arteaga, F. Badea, K. Bekk, M. Bertaina, J. Blümer, H. Bozdog, I.M. Brancus, M. Brüggemann, P. Buchholz, E. Cantoni, A. Chiavassa, F. Cossavella, K. Daumiller, V. de Souza, F. Di Pierro, P. Doll, R. Engel, J. Engler, M. Finger, D. Fuhrmann, P.L. Ghia, H.J. Gils, R. Glasstetter, C. Grupen, A. Haungs, D. Heck, T. Huege, P.G. Isar, K.-H. Kampert, D. Kang, D. Kickelbick, H.O. Klages, Y. Kolotaev, P. Łuczak, H.J. Mathes, H.J. Mayer, J. Milke, B. Mitrica, C. Morello, G. Navarra, S. Nehls, J. Oehlschläger, S. Ostapchenko, S. Over, M. Petcu, T. Pierog, H. Rebel, M. Roth, H. Schieler, F. Schröder, O. Sima, M. Stümpert, G. Toma, G. Trinchero, H. Ulrich, W. Walkowiak, A. Weindl, J. Wochele, M. Wommer, and J. Zabierowski
Subjects: Physics, Nuclear and High Energy Physics, Particle physics, Air shower, Hadron, Astrophysics::Instrumentation and Methods for Astrophysics, High Energy Physics::Experiment, Parameter space, Atomic and Molecular Physics, and Optics
Abstract: The description of high-energy hadronic interactions plays an important role in the (astrophysical) interpretation of air shower data. The parameter space important for the development of air showers (energy and kinematical range) extends well beyond todays accelerator capabilities. Therefore, accurate measurements of air showers are used to constrain modern models to describe high-energy hadronic interactions. The results obtained are complementary to information gained at accelerators and add to our understanding of high-energy hadronic interactions.
Published: 2009

43. 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

44. Investigation of cosmic ray muons with the WILLI detector compared with the predictions of theoretical models and with semi-analytical formulae

Author: Octavian Sima, M. Duma, I.M. Brancus, A. Haungs, H. Rebel, B. Mitrica, G. Toma, A. Saftoiu, and M. Petcu
Subjects: Physics, Nuclear and High Energy Physics, Muon, Physics::Instrumentation and Detectors, Cosmic ray muons, Detector, Theoretical models, Measure (physics), Charge (physics), Physics::History of Physics, Atomic and Molecular Physics, and Optics, Nuclear physics, Low energy, Muon flux, Physics::Accelerator Physics, High Energy Physics::Experiment
Abstract: The WILLI detector, built in IFIN-HH, Bucharest, is used to measure the muon flux and the muon charge ratio at low energy (
Published: 2009

45. WILLI - EAS - a detection system for investigating the muon charge ratio in Extensive Air Showers

Author: H. J. Mathes, A. Haungs, G. Toma, M. Duma, I.M. Brancus, M. Petcu, H. Rebel, B. Mitrica, Octavian Sima, and A. Saftoiu
Subjects: Nuclear physics, Physics, Nuclear and High Energy Physics, Wavelength, Photomultiplier, Muon, Detector, Charge (physics), Scintillator, Atomic and Molecular Physics, and Optics
Abstract: A concept of an experiment for investigating the muon charge ratio in EAS has been proposed based on the existing WILLI detector designed for measurements of the atmospheric muon charge ratio. A mini-array surrounding WILLI for measuring EAS is presently under construction. This array will serve as a core-finder system consisting of 12 stations of 1 m2, each unit containing 4 plastic scintillator sheets ( 50 × 50 × 3 ) cm 3 , seen by wave length shifters and 2 photomultipliers. Using CORSIKA and GEANT codes, simulation studies have been performed for H and Fe generated showers (1014–1015) eV to optimize the configuration of the WILLI-EAS arrangement. By this device, measurements of the charge ratio can be performed for both in parallel, inclusive muons and EAS muons.
Published: 2009

46. Analysis of inclined showers measured with LOPES

Author: A. Saftoiu, W.D. Apel, J.C. Arteaga, T. Asch, J. Auffenberg, 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, R. Engel, H. Falcke, M. Finger, D. Fuhrmann, H. Gemmeke, P.L. Ghia, R. Glasstetter, C. Grupen, A. Haungs, D. Heck, J.R. Hörandel, A. Horneffer, T. Huege, P.G. Isar, K.-H. Kampert, D. Kang, D. Kickelbick, Y. Kolotaev, O. Krömer, J. Kuijpers, S. Lafebre, P. Łuczak, H.J. Mathes, H.J. Mayer, J. Milke, B. Mitrica, C. Morello, G. Navarra, S. Nehls, A. Nigl, J. Oehlschläger, S. Over, M. Petcu, T. Pierog, J. Rautenberg, H. Rebel, M. Roth, H. Schieler, A. Schmidt, F. Schröder, O. Sima, K. Singh, M. Stümpert, G. Toma, G.C. Trinchero, H. Ulrich, W. Walkowiak, A. Weindl, J. Wochele, M. Wommer, J. Zabierowski, and J.A. Zensus
Subjects: Physics, Nuclear and High Energy Physics, LOPES, business.industry, Astronomy, Astrophysics::High Energy Astrophysical Phenomena, Detector, Astrophysics::Instrumentation and Methods for Astrophysics, Cosmic ray, Amplitude, Air shower, Optics, Earth's magnetic field, KASCADE, Antenna (radio), business, GeneralLiterature_REFERENCE(e.g.,dictionaries,encyclopedias,glossaries), Instrumentation
Abstract: In the present study, we analyze the radio signal from inclined air showers recorded by LOPES-30 in coincidence with KASCADE-Grande. LOPES-30 consists of 30 East–West oriented digital antennas, which are amplitude calibrated by an external source. Radio emission from air showers is considered a geomagnetic effect. Inclined events provide a larger range of values for geomagnetic angle (angle between shower axis and geomagnetic field direction) than vertical showers and thus more information on the emission processes can be gathered. In order to have the geometry of the air shower we use the reconstruction provided by the KASCADE-Grande particle detectors array. Analyzing events observed by both LOPES and the extended part of the KASCADE array, Grande, gives the possibility to test in particular the capability and efficiency of radio detection of more distant events. The results are compared with a previous analysis of inclined events recorded by the initial 10 antenna set-up, LOPES-10, in coincidence with the Grande array.
Published: 2009

47. 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

48. Air shower measurements with the LOPES radio antenna array

Author: A. Haungs, W.D. Apel, J.C. Arteaga, T. Asch, J. Auffenberg, 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, R. Engel, H. Falcke, M. Finger, D. Fuhrmann, H. Gemmeke, P.L. Ghia, R. Glasstetter, C. Grupen, D. Heck, J.R. Hörandel, A. Horneffer, T. Huege, P.G. Isar, K.-H. Kampert, D. Kang, D. Kickelbick, Y. Kolotaev, O. Krömer, J. Kuijpers, S. Lafebre, P. Łuczak, H.J. Mathes, H.J. Mayer, J. Milke, B. Mitrica, C. Morello, G. Navarra, S. Nehls, A. Nigl, J. Oehlschläger, S. Over, 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.C. Trinchero, H. Ulrich, W. Walkowiak, A. Weindl, J. Wochele, M. Wommer, J. Zabierowski, and J.A. Zensus
Subjects: Pierre Auger Observatory, Physics, Nuclear and High Energy Physics, LOPES, business.industry, Astrophysics::High Energy Astrophysical Phenomena, Astronomy, Astrophysics (astro-ph), Astrophysics::Instrumentation and Methods for Astrophysics, FOS: Physical sciences, Astrophysics, Digital radio, Antenna array, Interferometry, Air shower, Optics, Amplitude, ComputingMethodologies_DOCUMENTANDTEXTPROCESSING, business, Instrumentation, Radio wave
Abstract: LOPES is set up at the location of the KASCADE-Grande extensive air shower experiment in Karlsruhe, Germany and aims to measure and investigate radio pulses from Extensive Air Showers. Since radio waves suffer very little attenuation, radio measurements allow the detection of very distant or highly inclined showers. These waves can be recorded day and night, and provide a bolometric measure of the leptonic shower component. LOPES is designed as a digital radio interferometer using high bandwidths and fast data processing and profits from the reconstructed air shower observables of KASCADE-Grande. The LOPES antennas are absolutely amplitude calibrated allowing to reconstruct the electric field strength which can be compared with predictions from detailed Monte Carlo simulations. We report about the analysis of correlations present in the radio signals measured by the LOPES 30 antenna array. Additionally, LOPES operates antennas of a different type (LOPES-STAR) which are optimized for an application at the Pierre Auger Observatory. Status, recent results of the data analysis and further perspectives of LOPES and the possible large scale application of this new detection technique are discussed., Comment: 8 pages, 10 figures, Contribution to the Arena 2008 conference, Rome, June 2008
Published: 2009

49. KASCADE-Grande: An overview and first results

Author: H. J. Mathes, M. Petcu, D. Kickelbick, V. de Souza, H.O. Klages, H. Bozdog, A. Haungs, Peter Buchholz, I.M. Brancus, J. Zabierowski, Wolfgang Walkowiak, B. Mitrica, R. Engel, Markus Roth, J. Wochele, J. Engler, A. Chiavassa, H.J. Gils, S. Plewnia, Octavian Sima, F. Badea, D. Heck, Y. Kolotaev, P. Luczak, H.J. Mayer, M. E. Bertaina, J. Milke, K. H. Kampert, C. Meurer, S. Over, D. Fuhrmann, Tim Huege, G.C. Trinchero, M. Finger, K. Bekk, J.R. Hörandel, G. Toma, M. Stümpert, S. Ostapchenko, Paula Gina Isar, A. Morales, M. Brüggemann, F. Di Pierro, C. Morello, H. Schieler, A. Weindl, T. Pierog, J. Blümer, H. Ulrich, H. Rebel, P. Doll, Piera Luisa Ghia, F. Cossavella, S. Nehls, Claus Grupen, R. Glasstetter, J.C. Arteaga, G. Navarra, J. van Buren, Kai Daumiller, J. Oehlschläger, and W. D. Apel
Subjects: Nuclear physics, Physics, Nuclear and High Energy Physics, KASCADE, Astronomy, Detector, Cosmic ray, Astrophysics, Knee region, Scintillator, Instrumentation
Abstract: The KASCADE-Grande experiment, located at Forschungszentrum Karlsruhe (Germany), is a multi-component extensive air-shower experiment to study cosmic rays and their interactions at primary energies 10 14 –10 18 eV. After detailed investigations of the knee in the spectrum with KASCADE and EAS-TOP experiments, the main goal of KASCADE-Grande is to provide conclusive results on the knee region by detecting the expected iron knee in the spectrum at around 10 17 eV, and measuring the composition in the possible transition region between galactic and extragalactic components. Due to its multi-component characteristics, basically the former KASCADE experiment enriched by two new arrays of scintillator detectors (Grande and Piccolo), with the aim of providing a large acceptance area (0.5 km 2 ) and prompt trigger signal, KASCADE-Grande is a suitable array to provide refined measurements in the 10 16 –10 18 eV region. In the following, we briefly report on the characteristics of the detector, its performance, and first results based on 2 years of data taking. r 2008 Elsevier B.V. All rights reserved. PACS: 95.85.Ry
Published: 2008

50. WILLI – a scintillator detector setup for studies of the zenith and azimuth variation of charge ratio and flux of atmospheric muons

Author: B. Mitrica, Alexandru Bercuci, M. Petcu, I.M. Brancus, M. Duma, A. Saftoiu, A. Haungs, J. Wentz, C. Aiftimiei, Octavian Sima, G. Toma, and H. Rebel
Subjects: Physics, Nuclear and High Energy Physics, Muon, Physics::Instrumentation and Detectors, business.industry, Detector, Cosmic ray, Scintillator, Atomic and Molecular Physics, and Optics, Nuclear physics, Azimuth, Earth's magnetic field, Optics, Air shower, Physics::Accelerator Physics, High Energy Physics::Experiment, business, Zenith
Abstract: The primary and secondary components of the cosmic radiation are influenced by the geomagnetic field. This leads - in addition to the variation with the zenith angle - to an azimuth dependence, in particular of the ratio of positive and negative muons, pronounced as East-West effect of muon charge ratio for low energy muons. The compact scintillator detector arrangement, WILLI, able to register incident muons with different azimuth and zenith angles ( E 1 G e V ), has been used to study the azimuth dependence of the muon charge ratio. Positive and negative muons are discriminated by observing the different lifetimes when being stopped in matter, in the WILLI case by Al absorbers. We are considering the development of a mini array, installed close to the WILLI detector, for triggering the muon charge ratio measurements in extended air shower events.
Published: 2008

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