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1. Implementing a Low-Threshold Analysis with the Askaryan Radio Array (ARA)

Author: Patrick Allison, K. D. de Vries, C.Y. Kuo, C. Xie, Alexander Novikov, Michael DuVernois, Eric Oberla, R. Gaior, K. Hughes, A. Karle, A. Nozdrina, M.-C. Kim, J. Davies, I. Kravchenko, J. Touart, Brian Clark, U. Latif, J. Flaherty, Thomas Meures, M.-Y. Lu, N. Harty, W. Clay, J. L. Kelley, M.-H. A. Huang, H. Landsman, A. Shultz, S. Archambault, M. Beydler, J. Roth, Stephanie Wissel, A. O'Murchadha, B. Hendricks, R. J. Nichol, N. Punsuebsay, Simona Toscano, S. Y. Hsu, K. Mase, E. Hong, Chun Hsiung Chen, S. De Kockere, Abigail G. Vieregg, Po-Hsun Chen, L. Cremonesi, A. Ishihara, J. J. Huang, Benjamin Hokanson-Fasig, G. Nir, M. Beheler-Amass, D. Z. Besson, K. Kurusu, P. Dasgupta, D. Seckel, Cosmin Deaconu, M. Z. Wang, R. Krebs, Y.H. Wang, J. C. Hanson, James C. Osborn, B. Madison, Y. Pan, Jiwoo Nam, Jorge Torres, P. Sandstrom, Yi Chen, A. Laundrie, E. Friedman, J. J. Beatty, K. D. Hoffman, Kael Hanson, N. van Eijndhoven, S. Yoshida, S. H. Wang, K.-C. Kim, Y. S. Shiao, Y. Ku, David J. Smith, Tsung-Che Liu, Amy Connolly, Carl Pfendner, R. D. Young, G. S. Varner, and R. Khandelwal
Subjects: Physics, Early results, Phased array, Astrophysics::High Energy Astrophysical Phenomena, Acoustics, Detector, Astrophysics::Instrumentation and Methods for Astrophysics, Neutrino, Energy (signal processing), Noise (radio)
Abstract: The Askaryan Radio Array (ARA) is a ground-based radio detector at the South Pole designed to capture Askaryan emission from ultra-high energy neutrinos interacting within the Antarctic ice. The newest ARA station has been equipped with a phased array trigger, in which radio signals in multiple antennas are summed in predetermined directions prior to the trigger. In this way, impulsive signals add coherently, while noise likely does not, allowing the trigger threshold to be lower than a traditional ARA station. Early results on just a fraction of available data from this new system prove the feasibility of a low-threshold analysis.
Published: 2021

2. The Calibration of the Geometry and Antenna Delay in Askaryan Radio Array Station 4 and 5

Author: A. O'Murchadha, S. Yoshida, P. Dasgupta, K. Hughes, P. Sandstrom, I. Kravchenko, U. Latif, M. Beheler-Amass, J. Touart, Y.H. Wang, J. Flaherty, M.-H. A. Huang, C. Xie, Kael Hanson, David J. Smith, M. A. Huang, Y. S. Shiao, G. S. Varner, R. D. Young, Y. Pan, Tsung-Che Liu, W. Clay, J. Roth, R. Krebs, A. Ishihara, Eric Oberla, S. De Kockere, A. Karle, S. Y. Hsu, D. Z. Besson, N. Punsuebsay, K. D. de Vries, R. J. Nichol, H. Landsman, Patrick Allison, James C. Osborn, N. van Eijndhoven, M. Z. Wang, Po-Hsun Chen, Brian Clark, B. Madison, Michael DuVernois, G. Nir, Paramita Dasgupta, C.Y. Kuo, S. Archambault, Jorge Torres, A. Nozdrina, Cosmin Deaconu, Chun Hsiung Chen, Abigail G. Vieregg, K. Mase, E. Hong, R. Gaior, Y. Ku, Jiwoo Nam, A. Shultz, Thomas Meures, R. Khandelwal, D. Seckel, Stephanie Wissel, Yi Chen, K. Kurusu, M Beheler Amass, J. J. Beatty, N. Harty, J. L. Kelley, Simona Toscano, Amy Connolly, Carl Pfendner, S. H. Wang, K.-C. Kim, J. C. Hanson, B. Hendricks, K. D. Hoffman, A. Laundrie, E. Friedman, J. J. Huang, L. Cremonesi, M. Beydler, Benjamin Hokanson-Fasig, M.-Y. Lu, Alexander Novikov, M.-C. Kim, and J. Davies
Subjects: Physics, Calibration (statistics), Acoustics, Antenna (radio)
Published: 2021

3. Application of parabolic equation methods to in-ice radiowave propagation for ultra high energy neutrino detection experiments

Author: J. J. Beatty, Patrick Allison, Nick van Eijndhoven, Rose S Stanley, Dieder Van den Broeck, Krijn D. de Vries, A. Nozdrina, S. Prohira, Chung-Yun Kuo, K. Mulrey, Vesna Lukic, Cosmin Deaconu, John Ralston, Jiwoo Nam, Thomas Meures, Enrique Huesca Santiago, Jorge Torres, Amy Connolly, D. Z. Besson, Paramita Dasgupta, U. Latif, Simona Toscano, Dylan Frikken, Cade Sbrocco, Stephanie Wissel, Simon De Kockere, C. Hast, and Eric Oberla
Subjects: Physics, High energy, Neutrino detector, Radiowave propagation, Computational physics
Published: 2021

4. A Template-based UHE Neutrino Search Strategy for the Askaryan Radio Array (ARA)

Author: A. Ishihara, Y. Pan, Y. S. Shiao, Chun Hsiung Chen, J. Roth, C. Xie, P. Dasgupta, Yi Chen, M.-Y. Lu, M. Z. Wang, S. Y. Hsu, R. J. Nichol, N. van Eijndhoven, Myoungchul Kim, Eric Oberla, R. Gaior, R. D. Young, N. Harty, A. Karle, A. Nozdrina, Cosmin Deaconu, Amy Connolly, L. Cremonesi, Jorge Torres, Patrick Allison, Benjamin Hokanson-Fasig, K. Hughes, Abigail G. Vieregg, James C. Osborn, C.Y. Kuo, Jiwoo Nam, D. Seckel, B. Madison, A. Shultz, B. Hendricks, S. Yoshida, J. C. Hanson, S. H. Wang, A. Laundrie, Stephanie Wissel, K.-C. Kim, Thomas Meures, E. Friedman, M. Beydler, J. J. Huang, I. Kravchenko, N. Punsuebsay, Alexander Novikov, Y.H. Wang, Carl Pfendner, J. Touart, Kael Hanson, K. D. Hoffman, J. J. Beatty, Brian Clark, M. Beheler-Amass, J. L. Kelley, J. Davies, P. Sandstrom, D. Z. Besson, K. Mase, S. De Kockere, Simona Toscano, S. Archambault, E. Hong, U. Latif, K. Kurusu, Po-Hsun Chen, G. Nir, R. Krebs, H. Landsman, A. O'Murchadha, K. D. de Vries, J. Flaherty, W. Clay, David J. Smith, Tsung-Che Liu, G. S. Varner, Y. Ku, R. Khandelwal, Michael DuVernois, and M.-H. A. Huang
Subjects: Physics, Astronomy, Template based, Neutrino
Published: 2021

5. A neural network based UHE neutrino reconstruction method for the Askaryan Radio Array (ARA)

Author: Thomas Meures, P. Dasgupta, R. Krebs, R. D. Young, J. Flaherty, Y. S. Shiao, A. Ishihara, K. Mase, M. Beydler, Jiwoo Nam, J. Roth, W. Clay, I. Kravchenko, M.-H. A. Huang, S. Y. Hsu, M.-Y. Lu, J. L. Kelley, E. Hong, K. Kurusu, U. Latif, J. Touart, Simona Toscano, Patrick Allison, K. D. de Vries, R. Khandelwal, R. J. Nichol, A. Laundrie, E. Friedman, R. Gaior, C.Y. Kuo, L. Cremonesi, P. Sandstrom, Po-Hsun Chen, Benjamin Hokanson-Fasig, Cosmin Deaconu, G. Nir, Y.H. Wang, D. Z. Besson, N. Harty, Amy Connolly, Chun Hsiung Chen, Alexander Novikov, N. Punsuebsay, Brian Clark, A. O'Murchadha, M.-C. Kim, J. Davies, Carl Pfendner, G. S. Varner, Y. Ku, S. H. Wang, B. Hendricks, K.-C. Kim, Yue Pan, H. Landsman, M. Z. Wang, C. Xie, J. J. Huang, Michael DuVernois, David J. Smith, A. Shultz, Tsung-Che Liu, K. Hughes, James C. Osborn, M. Beheler-Amass, Stephanie Wissel, Jorge Torres, B. Madison, Eric Oberla, A. Karle, Abigail G. Vieregg, D. Seckel, S. Archambault, A. Nozdrina, S. De Kockere, Y. Pan, K. D. Hoffman, Kael Hanson, Yi Chen, S. Yoshida, N. van Eijndhoven, J. C. Hanson, and J. J. Beatty
Subjects: Physics, Vertex (graph theory), Interferometry, Particle physics, Amplitude, Astrophysics::High Energy Astrophysical Phenomena, Detector, Filter (signal processing), Neutrino, Event (particle physics), Energy (signal processing)
Abstract: The Askaryan Radio Array (ARA) is an ultra-high energy (UHE) neutrino ($E_{\nu}$ > $10^{17}$ eV) detector at South Pole. ARA aims to utilize radio signals detected from UHE neutrino interactions in the glacial ice to infer properties about the interaction vertex as well as the incident neutrino. To retrieve these properties from experiment data, the first step is to extract timing, amplitude and frequency information from waveforms of different antennas buried in the deep ice. These features can then be utilized in a neural network to reconstruct the neutrino interaction vertex position, incoming neutrino direction and shower energy. So far, vertex can be reconstructed through interferometry while neutrino reconstruction is still under investigation. Here I will present a solution based on multi-task deep neural networks which can perform reconstruction of both vertex and incoming neutrinos with a reasonable precision. After training, this solution is capable of rapid reconstructions (e.g. 0.1 ms/event compared to 10000 ms/event in a conventional routine) useful for trigger and filter decisions, and can be easily generalized to different station configurations for both design and analysis purposes.
Published: 2021

6. Measurement of the real dielectric permittivity ϵ of glacial ice

Author: M. Beydler, D. Z. Besson, M. Relich, C. C. Chen, R. Gaior, Brian Clark, Patrick Allison, J. Roth, Eric Oberla, Y. S. Shiao, R. Young, Po-Hsun Chen, A. Karle, G. Nir, Alexander Novikov, J. C. Hanson, G. S. Varner, A. Ishihara, R. J. Nichol, T. Kuwabara, S. Archambault, S. Y. Hsu, J. L. Kelley, Y. Pan, M.-C. Kim, P. Sandstrom, Cosmin Deaconu, A. Shultz, Stephanie Wissel, E. Hong, Thomas Meures, M.-Y. Lu, A. Christenson, J. Auffenberg, M. Beheler-Amass, M. Z. Wang, J. J. Beatty, I. Kravchenko, Abigail G. Vieregg, J. Touart, R. Bard, L. Cremonesi, D. Seckel, A. Laundrie, U. Latif, J. J. Huang, Kara Hoffman, L. Hu, Amy Connolly, A. O’ Murchadha, R. Khandelwal, C.-J. Li, M. Song, S. H. Wang, Carl Pfendner, J. Kruse, Chun Hsiung Chen, J. Nam, Kenneth L. Ratzlaff, K. Mase, K. Kurusu, S. Yoshida, M.-H. A. Huang, Tsung-Che Liu, L. Friedman, J. Haugen, Kael Hanson, H. Landsman, and Michael DuVernois
Subjects: Physics, geography, geography.geographical_feature_category, 010308 nuclear & particles physics, Astrophysics::High Energy Astrophysical Phenomena, media_common.quotation_subject, Astronomy and Astrophysics, Glacier, Radiation, 01 natural sciences, Asymmetry, Computational physics, Glaciology, Radio propagation, 0103 physical sciences, Polar, Radio frequency, Neutrino, 010303 astronomy & astrophysics, Physics::Atmospheric and Oceanic Physics, media_common
Abstract: Owing to their small interaction cross-section, neutrinos are unparalleled astronomical tracers. Ultra-high energy (UHE; E > 10 PeV) neutrinos probe the most distant, most explosive sources in the Universe, often obscured to optical telescopes. Radio-frequency (RF) detection of Askaryan radiation in cold polar ice is currently regarded as the best experimental measurement technique for UHE neutrinos, provided the RF properties of the ice target can be well-understood. To that end, the Askaryan Radio Array (ARA) experiment at the South Pole has used long-baseline RF propagation to extract information on the index-of-refraction ( n = ϵ r ) in South Polar ice. Owing to the increasing ice density over the upper 150–200 m, rays are measured along two, nearly parallel paths, one of which refracts through an inflection point, with differences in both arrival time and arrival angle that can be used to constrain the neutrino properties. We also observe (first) indications for RF ice birefringence for signals propagating along predominantly horizontal trajectories, corresponding to an asymmetry of order 0.1% between the ordinary and extra-ordinary birefringent axes, numerically compatible with previous measurements of birefringent asymmetries for vertically-propagating radio-frequency signals at South Pole. Qualitatively, these effects offer the possibility of redundantly measuring the range from receiver to a neutrino interaction in Antarctic ice, if receiver antennas are deployed at shallow (z ∼ −25 m) depths. Such range information is essential in determining both the neutrino energy, as well as the incident neutrino direction.
Published: 2019

7. HiCal 2: An instrument designed for calibration of the ANITA experiment and for Antarctic surface reflectivity measurements

Author: A. Novikov, M. Mottram, D. Z. Besson, O. Banerjee, Eric Oberla, G. S. Varner, Abigail G. Vieregg, D. Seckel, F. Wu, J. W. Russell, Jiwoo Nam, Tsung-Che Liu, J. Stockham, John G. Learned, Chun Hsiung Chen, David Saltzberg, B. Dailey, Konstantin Belov, Cosmin Deaconu, J. J. Beatty, W. R. Binns, L. Batten, Kenneth L. Ratzlaff, Harm Schoorlemmer, Andrew Ludwig, P. F. Dowkontt, B. Rotter, J. M. Clem, S. Stafford, R. Young, Po-Hsun Chen, C. Hast, R. Hupe, Joshua A. Gordon, Stephanie Wissel, B. Strutt, V. Bugaev, B. Hill, M. H. Israel, K. Mulrey, B. D. Fox, L. Cremonesi, P. Cao, J. Roberts, K. Tatem, C. Miki, Brian Rauch, Joe Lam, Peter Gorham, S. Prohira, Kurt Liewer, R. J. Nichol, J. Kowalski, Patrick Allison, Amy Connolly, S. Matsuno, M. Stockham, and Andrew Romero-Wolf
Subjects: Physics, Surface (mathematics), Nuclear and High Energy Physics, Physics - Instrumentation and Detectors, 010504 meteorology & atmospheric sciences, 010308 nuclear & particles physics, business.industry, FOS: Physical sciences, High voltage, Instrumentation and Detectors (physics.ins-det), 01 natural sciences, Reflectivity, Pulse (physics), Optics, 0103 physical sciences, Calibration, business, Instrumentation, 0105 earth and related environmental sciences
Abstract: The NASA supported High-Altitude Calibration (HiCal)-2 instrument flew as a companion balloon to the ANITA-4 experiment in December 2016. Based on a HV discharge pulser producing radio-frequency (RF) calibration pulses, HiCal-2 comprised two payloads, which flew for a combined 18 days, covering 1.5 revolutions of the Antarctic continent. ANITA-4 captured over 10,000 pulses from HiCal, both direct and reflected from the surface, at distances varying from 100-800 km, providing a large dataset for surface reflectivity measurements. Herein we present details on the design, construction and performance of HiCal-2., Comment: Published in NIM-A, final version
Published: 2019

8. Modeling in-ice radio propagation with parabolic equation methods

Author: J. J. Beatty, Patrick Allison, Rose S Stanley, Thomas Meures, Jiwoo Nam, D. Van den Broeck, Cade Sbrocco, D. Z. Besson, C. Hast, Paramita Dasgupta, Radar Echo Telescope, Simona Toscano, Katie Mulrey, U. Latif, S. Prohira, Vesna Lukic, S. De Kockere, Chung-Yun Kuo, Amy Connolly, John Ralston, A. Nozdrina, Jorge Torres, Dylan Frikken, N. van Eijndhoven, Stephanie Wissel, Cosmin Deaconu, K. D. de Vries, E. Huesca Santiago, Faculty of Sciences and Bioengineering Sciences, Physics, and Elementary Particle Physics
Subjects: Physics, Current (mathematics), 010308 nuclear & particles physics, Detector, Finite-difference time-domain method, FOS: Physical sciences, Généralités, Computational Physics (physics.comp-ph), 01 natural sciences, law.invention, Computational physics, Telescope, Radio propagation, Neutrino detector, law, physics.comp-ph, 0103 physical sciences, Sensitivity (control systems), Radar, 010306 general physics, Astrophysics - Instrumentation and Methods for Astrophysics, Instrumentation and Methods for Astrophysics (astro-ph.IM), Physics - Computational Physics, Physics::Atmospheric and Oceanic Physics, astro-ph.IM
Abstract: We investigate the use of parabolic equation (PE) methods for solving radio-wave propagation in polar ice. PE methods provide an approximate solution to Maxwell's equations, in contrast to full-field solutions such as finite-difference-time-domain (FDTD) methods, yet provide a more complete model of propagation than simple geometric ray-tracing (RT) methods that are the current state of the art for simulating in-ice radio detection of neutrino-induced cascades. PEs are more computationally efficient than FDTD methods, and more flexible than RT methods, allowing for the inclusion of diffractive effects and modeling of propagation in regions that cannot be modeled with geometric methods. We present a new PE approximation suited to the in-ice case. We conclude that current ray-tracing methods may be too simplistic in their treatment of ice properties, and their continued use could overestimate experimental sensitivity for in-ice neutrino detection experiments. We discuss the implications for current in-ice Askaryan-type detectors and for the upcoming Radar Echo Telescope, two families of experiments for which these results are most relevant. We suggest that PE methods be investigated further for in-ice radio applications., SCOPUS: ar.j, info:eu-repo/semantics/published
Published: 2021

9. Calibration of the Surface Array of the Pierre Auger Observatory

Author: J. J. Beatty, E. Moreno, Humberto Ibarguen Salazar, T. Suomijärvi, C. Grunfeld, M. C. Medina, A. Filevitch, S. Ranchon, A. K. Tripathi, N.G. Busca, P. Bauleo, Marco Aglietta, D. Barnhill, Piera Luisa Ghia, I. Lhenry-Yvon, A. Creusot, Xavier Bertou, A. Etchegoyen, D. Supanitsky, D. Nitz, M. Urban, T. Ohnuki, C. Bonifazi, L. Villaseñor, Patrick Allison, F. Arneodo, D. Dornic, Institut de Physique Nucléaire d'Orsay (IPNO), Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de l'Accélérateur Linéaire (LAL), and PIERRE AUGER
Subjects: Nuclear and High Energy Physics, Photomultiplier, Physics::Instrumentation and Detectors, Astrophysics::High Energy Astrophysical Phenomena, Water Cherenkov detectors, Atmospheric muons, FOS: Physical sciences, Cosmic ray, 01 natural sciences, 7. Clean energy, Particle detector, [PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], Nuclear physics, Optics, Observatory, 0103 physical sciences, Calibration, [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], 010306 general physics, Instrumentation, Instrumentation and Methods for Astrophysics (astro-ph.IM), Cherenkov radiation, Physics, Pierre Auger Observatory, High Energy Astrophysical Phenomena (astro-ph.HE), [SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph], 010308 nuclear & particles physics, business.industry, Detector, Astrophysics::Instrumentation and Methods for Astrophysics, Física, 96.50.S, 96.50.sd, 29.40.Ka, business, Astrophysics - High Energy Astrophysical Phenomena, Astrophysics - Instrumentation and Methods for Astrophysics, Ultra high-energy cosmic rays
Abstract: The Pierre Auger Observatory is designed to study cosmic rays of the highest energies ($>10^{19}$ eV). The ground array of the Observatory will consist of 1600 water Cherenkov detectors deployed over 3000 km^2. The remoteness and large number of detectors require a robust, automatic self-calibration procedure. It relies on the measurement of the average charge collected by a photomultiplier tube from the Cherenkov light produced by a vertical and central through-going muon determined to 5 - 10% at the detector via a novel rate-based technique and to 3% precision through analysis of histograms of the charge distribution. The parameters needed for the calibration are measured every minute, allowing for an accurate determination of the signals recorded from extensive air showers produced by primary cosmic rays. The method also enables stable and uniform triggering conditions to be achieved., 8 pages, 6 figures
Published: 2021

10. The Radar Echo Telescope for Neutrinos (RET-N)

Author: Vesna Lukic, Cade Sbrocco, Enrique Huesca Santiago, Dieder Van den Broeck, John Ralston, Eric Oberla, Thomas Meures, S. Prohira, Jorge Torres, U. Latif, Paramita Dasgupta, C. Hast, A. Nozdrina, K. Mulrey, Simon De Kockere, Nick van Eijndhoven, Cosmin Deaconu, Krijn D. de Vries, Dylan Frikken, J. J. Beatty, Patrick Allison, D. Z. Besson, Chung-Yun Kuo, Stephanie Wissel, Rose S Stanley, Jiwoo Nam, Simona Toscano, and Amy Connolly
Subjects: Physics, Telescope, law, Echo (computing), Astronomy, Neutrino, Radar, law.invention
Published: 2021
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11. Toward High Energy Neutrino Detection with the Radar Echo Telescope for Cosmic Rays (RET-CR)

Author: K. Mulrey, Vesna Lukic, Dieder Van den Broeck, John Ralston, Chung-Yun Kuo, Jorge Torres, Krijn D. de Vries, S. Prohira, Nick van Eijndhoven, Thomas Meures, Enrique Huesca Santiago, Eric Oberla, Paramita Dasgupta, U. Latif, Simon De Kockere, Simona Toscano, J. J. Beatty, Rose S Stanley, Cosmin Deaconu, Jiwoo Nam, Cade Sbrocco, A. Nozdrina, Dylan Frikken, D. Z. Besson, Stephanie Wissel, C. Hast, Patrick Allison, and Amy Connolly
Subjects: Physics, business.industry, Astrophysics::High Energy Astrophysical Phenomena, Cosmic ray, 7. Clean energy, law.invention, Telescope, Air shower, Optics, Neutrino detector, law, Cascade, Ultra-high-energy cosmic ray, Radar, Neutrino, business, Physics::Atmospheric and Oceanic Physics
Abstract: The Radar Echo Telescope for Cosmic Rays (RET-CR) is a pathfinder experiment for the Radar Echo Telescope for Neutrinos (RET-N), a next-generation in-ice detection experiment for ultra high energy neutrinos. RET-CR will serve as the testbed for the radar echo method to probe high-energy particle cascades in nature, whereby a transmitted radio signal is reflected from the ionization left in its wake. This method, recently validated at SLAC experiment T576, shows promising preliminary sensitivity to neutrino-induced cascades above the energy range of optical detectors like IceCube. RET-CR intends to use an in-nature test beam: the dense, in-ice cascade produced when the air shower of an ultra high energy cosmic ray impacts a high-elevation ice sheet. This in-ice cascade, orders of magnitude more dense than the in-air shower that preceded it, is similar in profile and density to the expected cascade from a neutrino-induced cascade deep in the ice. RET-CR will be triggered using surface scintillator technology and will be used to develop, test, and deploy the hardware, firmware, and software needed for the eventual RET-N. We present the strategy, status, and design sensitivity of RET-CR, and discuss its application to eventual neutrino detection.
Published: 2021
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12. Simulation and Optimisation for the Radar Echo Telescope for Cosmic Rays

Author: A. Nozdrina, Nick van Eijndhoven, Vesna Lukic, Dieder Van den Broeck, K. Mulrey, C. Hast, Simon De Kockere, Cosmin Deaconu, Eric Oberla, Cade Sbrocco, Thomas Meures, S. Prohira, D. Z. Besson, Jiwoo Nam, Krijn D. de Vries, U. Latif, Paramita Dasgupta, Simona Toscano, J. J. Beatty, Dylan Frikken, Rose S Stanley, John Ralston, Stephanie Wissel, Enrique Huesca Santiago, Chung-Yun Kuo, Jorge Torres, Amy Connolly, Patrick Allison, Faculty of Sciences and Bioengineering Sciences, and Physics
Subjects: Physics, business.industry, Astrophysics::High Energy Astrophysical Phenomena, Detector, Transmitter, Astrophysics::Instrumentation and Methods for Astrophysics, Cosmic ray, law.invention, Telescope, Optics, law, Radar, Neutrino, business, Event (particle physics), Physics::Atmospheric and Oceanic Physics, Radio wave
Abstract: The SLAC T-576 beam test experiment showed the feasibility of the radar detection technique to probe high-energy particle cascades in dense media. Corresponding particle-level simulations indicate that the radar method has very promising sensitivity to probe the $>$PeV cosmic neutrino flux. As such, it is crucial to demonstrate the in-situ feasibility of the radar echo method, which is the main goal of the current RET-CR experiment. Although the final goal of the Radar Echo Telescope is to detect cosmic neutrinos, we seek a proof of principle using cosmic-ray air showers penetrating the (high-altitude) Antarctic ice sheet. When an UHECR particle cascade propagates into a high-elevation ice sheet, it produces a dense in-ice cascade of charged particles which can reflect incoming radio waves. Using a surface cosmic-ray detector, the energy and direction of the UHECR can be reconstructed, and as such this constitutes a nearly ideal in-situ test beam to provide the proof of principle for the radar echo technique. RET-CR will consist of a transmitter array, receiver antennas and a surface scintillator plate array. Here we present the simulation efforts for RET-CR performed to optimise the surface array layout and triggering system, which affords an estimate of the expected event rate.
Published: 2021
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13. The Radar Echo Telescope for Cosmic Rays: Pathfinder experiment for a next-generation neutrino observatory

Author: U. Latif, K. D. de Vries, Patrick Allison, John Ralston, A. Nozdrina, C. Hast, Jorge Torres, S. Prohira, Amy Connolly, E. Huesca Santiago, Vesna Lukic, S. De Kockere, N. van Eijndhoven, Cosmin Deaconu, Jiwoo Nam, Chung-Yun Kuo, D. Van den Broeck, Dylan Frikken, Cade Sbrocco, J. J. Beatty, Stephanie Wissel, Katie Mulrey, Rose S Stanley, Thomas Meures, Paramita Dasgupta, Eric Oberla, Simona Toscano, D. Z. Besson, Faculty of Sciences and Bioengineering Sciences, Physics, and Elementary Particle Physics
Subjects: Astronomy, FOS: Physical sciences, Cosmic ray, 01 natural sciences, 7. Clean energy, law.invention, High Energy Physics - Experiment, Telescope, High Energy Physics - Experiment (hep-ex), Observatory, law, 0103 physical sciences, Radar, 010306 general physics, Instrumentation and Methods for Astrophysics (astro-ph.IM), Physics, High Energy Astrophysical Phenomena (astro-ph.HE), astro-ph.HE, 010308 nuclear & particles physics, hep-ex, Echo (computing), Pathfinder, 13. Climate action, Neutrino, Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - High Energy Astrophysical Phenomena, astro-ph.IM
Abstract: The Radar Echo Telescope for Cosmic Rays (RET-CR) is a recently initiated experiment designed to detect the englacial cascade of a cosmic-ray initiated air shower via in-ice radar, toward the goal of a full-scale, next-generation experiment to detect ultra high energy neutrinos in polar ice. For cosmic rays with a primary energy greater than 10 PeV, roughly 10% of an air-shower's energy reaches the surface of a high elevation ice-sheet ($\gtrsim$2 km) concentrated into a radius of roughly 10 cm. This penetrating shower core creates an in-ice cascade many orders of magnitude more dense than the preceding in-air cascade. This dense cascade can be detected via the radar echo technique, where transmitted radio is reflected from the ionization deposit left in the wake of the cascade. RET-CR will test the radar echo method in nature, with the in-ice cascade of a cosmic-ray initiated air-shower serving as a test beam. We present the projected event rate and sensitivity based upon a three part simulation using CORSIKA, GEANT4, and RadioScatter. RET-CR expects $\sim$1 radar echo event per day.
Published: 2021

14. Constraints on the Diffuse Flux of Ultra-High Energy Neutrinos from Four Years of Askaryan Radio Array Data in Two Stations

Author: H. Landsman, R. Gaior, Michael DuVernois, K. D. de Vries, I. Kravchenko, A. Laundrie, E. Hong, E. Friedman, J. Touart, K. Mase, Brian Clark, P. Sandstrom, U. Latif, L. Hu, K. Kurusu, A. Shultz, Amy Connolly, C. C. Chen, A. Nozdrina, R. Young, Po-Hsun Chen, Thomas Meures, R. Khandelwal, D. Z. Besson, S. Archambault, G. Nir, David J. Smith, J. C. Hanson, Tsung-Che Liu, C.-J. Li, Stephanie Wissel, S. Yoshida, J. J. Huang, M.-H. A. Huang, S. H. Wang, G. S. Varner, J. Roth, K.-C. Kim, James C. Osborn, B. Madison, A. Ishihara, W. Clay, J. Nam, Y. S. Shiao, S. Y. Hsu, Kael Hanson, Kara Hoffman, S. De Kockere, N. van Eijndhoven, Patrick Allison, Chun Hsiung Chen, Aongus O'Murchadha, Abigail G. Vieregg, R. J. Nichol, D. Seckel, J. L. Kelley, M. Beheler-Amass, Y. Pan, Cosmin Deaconu, J. J. Beatty, Eric Oberla, A. Karle, K. Hughes, M.-Y. Lu, M. Beydler, L. Cremonesi, Benjamin Hokanson-Fasig, C. Pfendner, Alexander Novikov, M.-C. Kim, J. Davies, M. Z. Wang, Jorge Torres, Faculty of Sciences and Bioengineering Sciences, Physics, and Elementary Particle Physics
Subjects: Physics, High Energy Astrophysical Phenomena (astro-ph.HE), astro-ph.HE, 010308 nuclear & particles physics, Astrophysics::High Energy Astrophysical Phenomena, Flux, FOS: Physical sciences, 7. Clean energy, 01 natural sciences, Nuclear physics, Neutrino detector, 0103 physical sciences, Diffuse flux, High Energy Physics::Experiment, Ultrahigh energy, Neutrino, 010306 general physics, Astrophysics - High Energy Astrophysical Phenomena, Astrophysics - Instrumentation and Methods for Astrophysics, Instrumentation and Methods for Astrophysics (astro-ph.IM), Radio wave, astro-ph.IM
Abstract: The Askaryan Radio Array (ARA) is an ultra-high energy (UHE, $>10^{17}$ eV) neutrino detector designed to observe neutrinos by searching for the radio waves emitted by the relativistic products of neutrino-nucleon interactions in Antarctic ice. In this paper, we present constraints on the diffuse flux of ultra-high energy neutrinos between $10^{16}-10^{21}$ eV resulting from a search for neutrinos in two complementary analyses, both analyzing four years of data (2013-2016) from the two deep stations (A2, A3) operating at that time. We place a 90 % CL upper limit on the diffuse all flavor neutrino flux at $10^{18}$ eV of $EF(E)=5.6\times10^{-16}$ $\textrm{cm}^{-2}$$\textrm{s}^{-1}$$\textrm{sr}^{-1}$. This analysis includes four times the exposure of the previous ARA result, and represents approximately 1/5 the exposure expected from operating ARA until the end of 2022., 12 pages, 7 figures; Accepted to PRD
Published: 2020

15. IceCube-Gen2: The Window to the Extreme Universe

Author: J. Kim, A. Gartner, A. Obertacke Pollmann, B. Hoffmann, J. L. Kelley, Markus Ahlers, Jenni Adams, Akimichi Taketa, D. van Eijk, Daniel Bindig, G. H. Collin, T. C. Arlen, Robert Lahmann, J. J. Beatty, Tianlu Yuan, U. Nauman, Azadeh Keivani, Y. L. Li, Karl J. Clark, T. Kintscher, M. Song, T. L. Carver, Paras Koundal, Michael Kovacevich, Christian Glaser, Frederik Hermann Lauber, T. Huege, Erik Ganster, Benedikt Riedel, D. Seckel, Anna Nelles, R. G. Stokstad, F. McNally, R. Maunu, M. Prado Rodriguez, Kayla Leonard, N. Kurahashi, James E. Braun, Amy Connolly, Samvel Ter-Antonyan, A. Terliuk, Justin Lanfranchi, Pranav Dave, Jannis Necker, C. Wendt, S. Wren, A. Sharma, Sukeerthi Dharani, David Vannerom, M. H. Shaevitz, Alexander Trettin, Reina H. Maruyama, Francis Halzen, J. Merz, K. Krings, Rasha Abbasi, Ben Smithers, Qinrui Liu, M. J. Larson, T. Anderson, Summer Blot, G. de Wasseige, I. Ansseau, D. Hebecker, Jorge Torres, Killian Holzapfel, Martina Karl, C. J. Lozano Mariscal, John Hardin, Jean Pierre Twagirayezu, Daniel García-Fernández, T. Stezelberger, S. Mandalia, E. O'Sullivan, R. Hoffmann, M. Plum, Juliana Stachurska, H. Dembinski, C. Pérez de los Heros, S. Márka, G. WSullivan, A. Haungs, Paul Coppin, Z. Griffith, J. C. Gallagher, Saskia Philippen, Federica Bradascio, Jochen M. Schneider, Srubabati Goswami, Andrea Turcati, Wing Yan Ma, Nahee Park, Y. Makino, Sarah Mancina, C. Walck, M. Kauer, Suyong Choi, Anna Franckowiak, Tobias Hoinka, Chad Finley, David Kappesser, T. Gregoire, Ella Roberts, J. van Santen, S. De Ridder, Jan Weldert, Chunfai Tung, F. Jonske, Ken'ichi Kin, L. Halve, Philipp Eller, K. Hultqvist, N. L. Strotjohann, H. Dujmovic, Vedant Basu, M. A. Unland Elorrieta, Alex Pizzuto, K. D. de Vries, I. CMariş, Gerrit Wrede, R. Gernhaeuser, Thomas Huber, Matti Jansson, Thomas K. Gaisser, M. Richman, Christoph Tönnis, James DeLaunay, Gary Binder, K.-H. Becker, Ek Narayan Paudel, Allan Hallgren, U. Latif, Hiroyuki Tanaka, I. Safa, Steve Sclafani, J. Kiryluk, K. Andeen, P. B. Price, H. Schieler, Kirill Filimonov, Segev BenZvi, Alexander Fritz, D. Z. Besson, Darren Grant, Marjon Moulai, Yiqian Xu, Felix Henningsen, S. Robertson, Aswathi Balagopal, Francesco Lucarelli, Pisin Chen, Matt Dunkman, Merlin Schaufel, Patrick Allison, Spencer Klein, Cosmin Deaconu, Tim Ruhe, A. Ludwig, George Japaridze, Javier Gonzalez, C. B. Krauss, Roxanne Turcotte, T. O. B. Schmidt, Simona Toscano, Roger Moore, P. Heix, R. S. Busse, Chujie Chen, Pablo Correa, L. Gerhard, S. De Kockere, J. Felde, Surujhdeo Seunarine, R. Snihur, J. Buscher, D. Rysewyk Cantu, A. Weindl, R. Hellauer, Giorgio Maggi, H. Niederhausen, Mauricio Bustamante, D. Southall, Julia Böttcher, J. Bourbeau, Lenka Tomankova, Maryon Ahrens, A. Burgman, Christopher Wiebusch, Darko Veberič, Juanan Aguilar, T. R. Wood, Christian Spiering, Frederik Tenholt, R. Nagai, L. Schumacher, C. De Clercq, Benjamin Hokanson-Fasig, L. V. Nguyen, C. Lagunas Gualda, K. Hughes, Kara Hoffman, C. Alispach, J. M. LoSecco, Joshua Hignight, K. Helbing, Timo Sturwald, Xinyue Kang, Richard Naab, Kunal Deoskar, Janet Conrad, Zackary Meyers, K. Meagher, Mehmet Gunduz, Agnieszka Leszczyńska, R. C. Bay, David A. Williams, Kurt Woschnagg, M. Zöcklein, M. Silva, Claudio Kopper, Eric Oberla, Ramesh Koirala, E. Cheung, Thomas Stuttard, Martin Rongen, Najia Moureen Binte Amin, R. Cross, Paul Evenson, A. Karle, Sebastian Böser, Seongjin In, Johannes Werthebach, J. P. Lazar, Markus Ackermann, Austin Schneider, Yang Lyu, Justin Vandenbroucke, Juan Carlos Diaz-Velez, Beverley A. Clark, Timo Karg, Sarah Pieper, Hershal Pandya, Wolfgang Rhode, Zhedong Zhang, P. Schlunder, A. Ishihara, Elisa Resconi, Subir Sarkar, William Luszczak, Clara E. Hill, Ava Ghadimi, Alessio Porcelli, Alan Coleman, J. Auffenberg, Grant Parker, Robert Stein, Dirk Ryckbosch, Benjamin Bastian, Anastasia Maria Barbano, Abhishek Desai, T. Kittler, J. Nam, P. Mallik, E. Blaufuss, S. Zierke, T. Stanev, M. Bohmer, Stephan Meighen-Berger, Simone Garrappa, P. Muth, Dmitry Chirkin, M. E. Huber, Marcos Santander, Christoph Raab, Nadège Iovine, J. Becker Tjus, L. Classen, Colin Turley, S. C. Nowicki, K. Farrag, M. Kleifges, O. Kalekin, A. Olivas, Alexander Kappes, D. Berley, G. C. Hill, Abigail G. Vieregg, Frank G. Schröder, D. Heinen, Erin Carnie-Bronca, N. Kulacz, D. Tosi, J. C. Hanson, Bunheng Ty, Ralph Engel, Moritz Kellermann, Gisela Anton, Elisa Lohfink, Elisa Bernardini, Damian Pieloth, Ali Kheirandish, Jan Soedingrekso, Giovanni Renzi, Michael DuVernois, Jannes Brostean-Kaiser, K. Wiebe, S. Fahey, A. R. Fazely, Tyce DeYoung, J. Lünemann, Thomas Ehrhardt, Nathan Whitehorn, Immacolata Carmen Rea, M. U. Nisa, Aaron Fienberg, Gerald Przybylski, G. Krückl, L. Papp, Amirreza Raissi, L. Köpke, Chris Weaver, R. Halliday, Alejandro Diaz, Stephanie Bron, S. Söldner-Rembold, James Pinfold, Ryan Burley, M. Riegel, H. Bagherpour, Stephanie Wissel, Olga Botner, Y. Pan, A. Steuer, S. Tilav, D. Kang, M. deWith, V. Baum, J. P. Yanez, I. Taboada, Stephen L. Hauser, Raamis Hussain, Michael O. Wolf, M. Stamatikos, John Evans, Shefali Shefali, Christoph Welling, Abdul Rehman, Carsten Rott, K. Tollefson, A. Goldschmidt, Y. Popovych, Troels Petersen, S. E. Sanchez Herrera, Simeon Reusch, S. Hickford, Xianwu Xu, J. Sandroos, C. Bohm, R. Joppe, Spencer Axani, Sebastian Baur, Carlos Arguelles, Jessie Micallef, Teppei Katori, K. Rawlins, James Madsen, Lu Lu, M. G. Aartsen, T. Glüsenkamp, M. Meier, Michael Campana, P. Sandstrom, Kendall Mahn, B. J. P. Jones, K. Hoshina, Glenn Spiczak, Andres Medina, G. Momenté, D. Mockler, M. Rameez, D. F. Cowen, Daria Pankova, E. Friedman, R. Morse, T. Montaruli, E. Unger, Maximilian Karl Scharf, P. Peiffer, J. Stettner, Gerrit Roellinghoff, Mirco Hunnefeld, Marie Oehler, Max Renschler, D. J. Koskinen, E. Bourbeau, Spencer Griswold, Maria Tselengidou, D. Soldin, Z. Márka, Minjin Jeong, L. Rauch, S. Yoshida, N. van Eijndhoven, C. Haack, Emily Dvorak, D. R. Nygren, Marek Kowalski, Kael Hanson, Paolo Desiati, J. Haugen, Lars Steffen Weinstock, Johan Wulff, Won Nam Kang, Timothyblake Watson, X. Bai, G. Neer, Konstancja Satalecka, Theo Glauch, U. Katz, Alexander Sandrock, Ilse Plaisier, K. Mase, D. B. Fox, Hermann Kolanoski, M. J. Weiss, Stef Verpoest, Imre Bartos, David J. Smith, S. Kopper, René Reimann, Leander Fischer, F. Huang, Matthias Vraeghe, Physics, Faculty of Sciences and Bioengineering Sciences, Vriendenkring VUB, and Elementary Particle Physics
Subjects: Physics, High Energy Astrophysical Phenomena (astro-ph.HE), astro-ph.HE, Nuclear and High Energy Physics, Active galactic nucleus, 010308 nuclear & particles physics, High-energy astronomy, Gravitational wave, media_common.quotation_subject, Astrophysics::High Energy Astrophysical Phenomena, Astrophysics::Instrumentation and Methods for Astrophysics, Astronomy, FOS: Physical sciences, Cosmic ray, 01 natural sciences, Universe, Neutron star, 0103 physical sciences, Neutrino, Neutrino astronomy, Astrophysics - High Energy Astrophysical Phenomena, 010303 astronomy & astrophysics, media_common
Abstract: The observation of electromagnetic radiation from radio to $\gamma$-ray wavelengths has provided a wealth of information about the universe. However, at PeV (10$^{15}$ eV) energies and above, most of the universe is impenetrable to photons. New messengers, namely cosmic neutrinos, are needed to explore the most extreme environments of the universe where black holes, neutron stars, and stellar explosions transform gravitational energy into non-thermal cosmic rays. The discovery of cosmic neutrinos with IceCube has opened this new window on the universe. In this white paper, we present an overview of a next-generation instrument, IceCube-Gen2, which will sharpen our understanding of the processes and environments that govern the universe at the highest energies. IceCube-Gen2 is designed to: 1) Resolve the high-energy neutrino sky from TeV to EeV energies; 2) Investigate cosmic particle acceleration through multi-messenger observations; 3) Reveal the sources and propagation of the highest energy particles in the universe; 4) Probe fundamental physics with high-energy neutrinos. IceCube-Gen2 will increase the annual rate of observed cosmic neutrinos by a factor of ten compared to IceCube, and will be able to detect sources five times fainter than its predecessor. Furthermore, through the addition of a radio array, IceCube-Gen2 will extend the energy range by several orders of magnitude compared to IceCube. Construction will take 8 years and cost about \$350M. The goal is to have IceCube-Gen2 fully operational by 2033. IceCube-Gen2 will play an essential role in shaping the new era of multi-messenger astronomy, fundamentally advancing our knowledge of the high-energy universe. This challenging mission can be fully addressed only in concert with the new survey instruments across the electromagnetic spectrum and gravitational wave detectors which will be available in the coming years., Comment: 56 pages, 29 figures
Published: 2020

16. The Payload for Ultrahigh Energy Observations (PUEO): a white paper

Author: Jiwoo Nam, J. M. Clem, Stephanie Wissel, Yixuan Ku, D. Seckel, Andrew Zeolla, C. Xie, D. Z. Besson, Amy Connolly, J. J. Beatty, Z. Martin, C. Hornhuber, K. Hughes, A. Nozdrina, D. Southall, Chung-Yun Kuo, A. Hynous, Alexander Novikov, Y. H. Wang, Jaime Alvarez-Muñiz, J. Shiao, R. Young, S. H. Wang, K. Nishimura, Remy Prechelt, Y. Chen, Pisin Chen, Peter Gorham, Brian Rauch, Patrick Allison, S. Prohira, Abigail G. Vieregg, L. Cremonesi, J. W. Russell, Jarred Matthew Roberts, J. Ammerman Yebra, Andrew Romero-Wolf, Enrique Zas, C. Hast, D. Frikken, G. S. Varner, Eric Oberla, Quincy Abarr, C. Miki, J. Flaherty, J. J. Huang, R. J. Nichol, Cosmin Deaconu, David J. Smith, and Tsung-Che Liu
Subjects: High Energy Astrophysical Phenomena (astro-ph.HE), Physics, Physics - Instrumentation and Detectors, biology, business.industry, Payload, Astrophysics::High Energy Astrophysical Phenomena, Astrophysics::Instrumentation and Methods for Astrophysics, FOS: Physical sciences, Instrumentation and Detectors (physics.ins-det), biology.organism_classification, High Energy Physics - Experiment, High Energy Physics - Experiment (hep-ex), Optics, Neutrino detector, Ultrahigh energy, Pueo, Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - High Energy Astrophysical Phenomena, business, Instrumentation and Methods for Astrophysics (astro-ph.IM), Instrumentation, Mathematical Physics
Abstract: The Payload for Ultrahigh Energy Observations (PUEO) long-duration balloon experiment is designed to have world-leading sensitivity to ultrahigh-energy neutrinos at energies above 1 EeV. Probing this energy region is essential for understanding the extreme-energy universe at all distance scales. PUEO leverages experience from and supersedes the successful Antarctic Impulsive Transient Antenna (ANITA) program, with an improved design that drastically improves sensitivity by more than an order of magnitude at energies below 30 EeV. PUEO will either make the first significant detection of or set the best limits on ultrahigh-energy neutrino fluxes., Comment: 40 pages, 17 figures. Version accepted to JINST
Published: 2021

17. Constraints on the ultra-high-energy neutrino flux from Gamma-Ray bursts from a prototype station of the Askaryan radio array

Author: H. Landsman, B. Hill, D. Z. Besson, Mauricio Bustamante, Mark Sullivan, Kael Hanson, R. Maunu, Jiwoo Nam, Pisin Chen, Patrick Allison, L. Hu, Amy Connolly, M.-Y. Lu, D. Seckel, A. O Murchadha, G. S. Varner, Tsung-Che Liu, Michael DuVernois, K. Mase, R. Young, G. Nir, P. Sandstrom, J. L. Kelley, S. Yoshida, Thomas Meures, B. D. Fox, A. Shultz, J. Auffenberg, A. Laundrie, Albrecht Karle, Kenneth L. Ratzlaff, H.-Y. Tu, M. Song, C.-J. Li, J. J. Beatty, B. Rotter, R. J. Nichol, Peter Gorham, J. P. Davies, Dafne Guetta, C. C. Chen, Carl Pfendner, A. Ishihara, Ilya Kravchenko, J. Touart, J. Stockham, M. Stockham, E. Hong, Kara Hoffman, C. Bora, C. Miki, and R. Bard
Subjects: High Energy Astrophysical Phenomena (astro-ph.HE), Physics, High energy, Astrophysics::High Energy Astrophysical Phenomena, Astrophysics::Instrumentation and Methods for Astrophysics, FOS: Physical sciences, Flux, Astronomy, Astronomy and Astrophysics, Cosmic ray, Astrophysics, Light curve, 01 natural sciences, law.invention, Telescope, law, 0103 physical sciences, High Energy Physics::Experiment, Neutrino, Astrophysics - High Energy Astrophysical Phenomena, 010306 general physics, Gamma-ray burst, 010303 astronomy & astrophysics
Abstract: We report on a search for ultra-high-energy (UHE) neutrinos from gamma-ray bursts (GRBs) in the data set collected by the Testbed station of the Askaryan Radio Array (ARA) in 2011 and 2012. From 57 selected GRBs, we observed no events that survive our cuts, which is consistent with 0.12 expected background events. Using NeuCosmA as a numerical GRB reference emission model, we estimate upper limits on the prompt UHE GRB neutrino fluence and quasi-diffuse flux from $10^{7}$ to $10^{10}$ GeV. This is the first limit on the prompt UHE GRB neutrino quasi-diffuse flux above $10^{7}$ GeV., Comment: 14 pages, 8 figures, Published in Astroparticle Physics Journal
Published: 2017

18. Cosmic-ray Isotope Measurements with HELIX

Author: Emma Ellingwood, Dietrich Müller, Makoto Tabata, M. Gebhard, Yu Chen, Thomas Rosin, David Hanna, J. A. Musser, Gerard Visser, S. P. Wakely, S. Coutu, S. L. Nutter, Stephane O’Brien, Patrick Allison, Ethan Schreyer, Monong Yu, Nahee Park, I. G. Wisher, Noah Green, Gergory Tarle, Issac Mognet, A. D. Tomasch, Brandon Kunkler, Tyler Werner, K. McBride, J. J. Beatty, Lucas Beaufore, Kelli Michaels, and Rostom Mbarek
Subjects: Physics, High energy, Light isotope, Isotope, Cherenkov detector, Astrophysics::High Energy Astrophysical Phenomena, Detector, Astrophysics::Instrumentation and Methods for Astrophysics, Cosmic ray, Superconducting magnet, law.invention, Nuclear physics, law, Helix
Abstract: HELIX (High Energy Light Isotope eXperiment) is a balloon-borne experiment designed to measure the chemical and isotopic abundances of light cosmic ray nuclei. Detailed measurements by HELIX, especially of $^{10}$Be from 0.2 GeV/n to beyond 3 GeV/n, will provide an essential set of data for the study of propagation processes of the cosmic rays. HELIX consists of a 1 Tesla superconducting magnet with a high-resolution gas tracking system, time-of-flight detector, and a ring-imaging Cherenkov detector. The instrument is scheduled to have a long-duration balloon flight out of McMurdo Station during NASA's 2020/21 Antarctic balloon campaign. Here, we discuss the scientific goals and the design of the experiment, and report on its current status.
Published: 2019

19. Calibration of the Aerogel Tiles for the HELIX RICH

Author: J. J. Beatty, Gerard Visser, Makoto Tabata, S. P. Wakely, S. L. Nutter, Rostom Mbarek, Ethan Schreyer, A. D. Tomasch, Tyler Werner, Stephan O'Brien, S. Coutu, Noah Green, Emma Ellingwood, Thomas Rosin, Gregory Tarle, Yu Chen, J. A. Musser, Mark Gebharb, S. I. Mognet, Monong Yu, I. G. Wisher, Nahee Park, Kelli Michaels, Brandon Kunkler, K. McBride, Patrick Allison, Dietrich Müller, David Hanna, and Lucas Beaufore
Subjects: Physics, Isotope, Physics::Instrumentation and Detectors, Cherenkov detector, Detector, Cosmic ray, Aerogel, Superconducting magnet, law.invention, Silicon photomultiplier, law, Physics::Atomic Physics, Atomic physics, Refractive index
Abstract: HELIX (High Energy Light Isotope eXperiment) is a balloon-borne experiment designed to measure the chemical and isotopic abundances of light cosmic ray nuclei, especially the $^{\textrm{10}}\textrm{Be}/^{\textrm{9}}\textrm{Be}$ ratio over the energy range from 0.2 GeV/n to beyond 3 GeV/n. This is a key measurement for constraining cosmic-ray propagation models. The detector is a mass spectrometer, which is built around a 1 Tesla superconducting magnet and a high-resolution tracking system to determine particle rigidity. Time-of-flight counters and a ring-imaging Cherenkov detector (RICH) are used to measure velocities. The proximity-focused RICH consists of a radiator made of aerogel tiles (refractive index approximately 1.15) and a detector plane of silicon photomultipliers. For discrimination of the $^{\textrm{9}}\textrm{Be}$ and $^{\textrm{10}}\textrm{Be}$ isotopes at high energy, the refractive index of the aerogel must be known to a precision of 0.07%. Given the manufacturing tolerances in the production process, the index must be mapped over the lateral extent of aerogel tiles on a fine grid. In this contribution, we describe and show initial results from procedures developed for this task. These include laser-deflection and electron-beam measurements.
Published: 2019

20. Comprehensive analysis of anomalous ANITA events disfavors a diffuse tau-neutrino flux origin

Author: J. J. Beatty, Berkeley Hill, K. Mulrey, L. Batten, R. J. Nichol, L. Cremonesi, Jarred Matthew Roberts, Cosmin Deaconu, S. Matsuno, J. Stockham, G. S. Varner, Peter Gorham, S. H. Wang, Jaime Alvarez-Muñiz, Patrick Allison, S. Stafford, O. Banerjee, B. D. Fox, R. Hupe, Washington Rodrigues de Carvalho, Keith Bechtol, Enrique Zas, Abigail G. Vieregg, S. Prohira, Jiwoo Nam, M. Stockham, Harm Schoorlemmer, C. Miki, Andres Romero-Wolf, Charles J. Naudet, J. J. Huang, M. S. Sutherland, K. Hughes, D. Seckel, B. Dailey, Brian Rauch, C. C. Chen, V. Bugaev, B. Rotter, Paul Dowkontt, M. H. Israel, J. Shiao, J. W. H. Gordon, J. W. Russell, S. Y. Hsu, Chun Hsiung Chen, Andrew Ludwig, P. Cao, Konstantin Belov, Tsung-Che Liu, W. R. Binns, Eric Oberla, David Saltzberg, C. Hast, A. Novikov, D. Z. Besson, B. Strutt, Pisin Chen, Kurt Liewer, Stephanie Wissel, Amy Connolly, Luca Macchiarulo, and J. M. Clem
Subjects: High Energy Astrophysical Phenomena (astro-ph.HE), Pierre Auger Observatory, Physics, 010308 nuclear & particles physics, Astrophysics::High Energy Astrophysical Phenomena, High Energy Physics::Phenomenology, Astrophysics::Instrumentation and Methods for Astrophysics, FOS: Physical sciences, Flux, Astrophysics, 7. Clean energy, 01 natural sciences, Standard Model, Air shower, 13. Climate action, Observatory, Tau neutrino, 0103 physical sciences, High Energy Physics::Experiment, Neutrino, Astrophysics - High Energy Astrophysical Phenomena, 010306 general physics, Lepton
Abstract: Recently, the ANITA collaboration reported on two upward-going extensive air shower events consistent with a primary particle that emerges from the surface of the ice. These events may be of $\nu_\tau$ origin, in which the neutrino interacts within the Earth to produce a $\tau$ lepton that emerges from the Earth, decays in the atmosphere, and initiates an extensive air shower. In this paper we estimate an upper bound on the ANITA acceptance to a diffuse $\nu_\tau$ flux detected via $\tau$-lepton-induced air showers within the bounds of Standard Model (SM) uncertainties. By comparing this estimate with the acceptance of Pierre Auger Observatory and IceCube and assuming SM interactions, we conclude that a $\nu_\tau$ origin of these events would imply a neutrino flux at least two orders of magnitude above current bounds., Comment: 12 pages, 7 figures
Published: 2019

21. Constraints on the ultra-high energy cosmic neutrino flux from the fourth flight of ANITA

Author: J. J. Beatty, A. Romero-Wolf, Berkeley Hill, J. M. Clem, R. Hupe, P. Cao, J. W. H. Gordon, J. W. Russell, K. M. Liewer, C. Hast, Jiwoo Nam, J. J. Huang, B. Dailey, K. Hughes, W. R. Binns, S. Y. Hsu, Eric Oberla, S. Prohira, G. S. Varner, N. Wang, S. Matsuno, D. Z. Besson, Andrew Ludwig, J. Roberts, O. Banerjee, J. Stockham, Harm Schoorlemmer, Abigail G. Vieregg, R. J. Nichol, Tsung-Che Liu, D. Seckel, B. Rotter, Chun Hsiung Chen, Charles J. Naudet, David Saltzberg, Cosmin Deaconu, L. Batten, M. S. Sutherland, Luca Macchiarulo, P. F. Dowkontt, C. Miki, J. Shiao, Brian Rauch, S. H. Wang, Amy Connolly, Pisin Chen, Stephanie Wissel, Patrick Allison, B. D. Fox, M. Stockham, Jakub Ripa, K. McBride, Peter Gorham, Yang-Fang Chen, Konstantin Belov, Katharine Mulrey, V. Bugaev, Alexander Novikov, S. Stafford, M. H. Israel, L. Cremonesi, and B. Strutt
Subjects: Physics, High Energy Astrophysical Phenomena (astro-ph.HE), COSMIC cancer database, 010308 nuclear & particles physics, Flux, FOS: Physical sciences, Astrophysics, 01 natural sciences, 13. Climate action, 0103 physical sciences, Polar, Ultrahigh energy, Neutrino, Antenna (radio), 010306 general physics, Astrophysics - High Energy Astrophysical Phenomena, Astrophysics - Instrumentation and Methods for Astrophysics, Event (particle physics), Instrumentation and Methods for Astrophysics (astro-ph.IM), Radio wave
Abstract: The ANtarctic Impulsive Transient Antenna (ANITA) NASA long-duration balloon payload completed its fourth flight in December 2016, after 28 days of flight time. ANITA is sensitive to impulsive broadband radio emission from interactions of ultra-high-energy neutrinos in polar ice (Askaryan emission). We present the results of two separate blind analyses searching for signals from Askaryan emission in the data from the fourth flight of ANITA. The more sensitive analysis, with a better expected limit, has a background estimate of $0.64^{+0.69}_{-0.45}$ and an analysis efficiency of $82\pm2\%$. The second analysis has a background estimate of $0.34^{+0.66}_{-0.16}$ and an analysis efficiency of $71\pm6\%$. Each analysis found one event in the signal region, consistent with the background estimate for each analysis. The resulting limit further tightens the constraints on the diffuse flux of ultra-high-energy neutrinos at energies above $10^{19.5}$ eV., 11 pages, 7 figures
Published: 2019

22. Developing a silica aerogel radiator for the HELIX ring-imaging Cherenkov system

Author: David Hanna, Dietrich Müller, K. McBride, J. J. Beatty, S. L. Nutter, Makoto Tabata, Michael Lang, A. D. Tomasch, S. Coutu, Patrick Allison, Gregory Tarle, Noah Green, Gerard Visser, J. A. Musser, Nahee Park, I. G. Wisher, S. P. Wakely, Michael Schubnell, Brandon Kunkler, S. I. Mognet, and M. Gebhard
Subjects: Nuclear and High Energy Physics, Fabrication, Physics - Instrumentation and Detectors, Cherenkov detector, Physics::Instrumentation and Detectors, FOS: Physical sciences, Ring-imaging Cherenkov detector, law.invention, High Energy Physics - Experiment, High Energy Physics - Experiment (hep-ex), Optics, law, Nuclear Experiment (nucl-ex), Instrumentation, Instrumentation and Methods for Astrophysics (astro-ph.IM), Nuclear Experiment, Cherenkov radiation, Physics, Condensed Matter - Materials Science, Spectrometer, business.industry, Materials Science (cond-mat.mtrl-sci), Aerogel, Instrumentation and Detectors (physics.ins-det), visual_art, Radiator (engine cooling), visual_art.visual_art_medium, Tile, business, Astrophysics - Instrumentation and Methods for Astrophysics
Abstract: This paper reports the successful fabrication of silica aerogel Cherenkov radiators produced in the first batches from a 96-tile mass production performed using pin-drying technique in our laboratory. The aerogels are to be used in a ring-imaging Cherenkov detector in the spectrometer of a planned balloon-borne cosmic-ray observation program, HELIX (High Energy Light Isotope eXperiment). A total of 36 transparent, hydrophobic aerogel tiles with a high refractive index of 1.16 and dimensions of 10 cm $\times $ 10 cm $\times $ 1 cm will be chosen as the flight radiators. Thus far, 40 out of the 48 tiles fabricated were confirmed as having no tile cracking. In the first screening, 8 out of the first 16 tiles were accepted as flight-qualified candidates, based on basic optical measurement results. To fit the aerogel tiles into a radiator support structure, the trimming of previously manufactured prototype tiles using a water-jet cutting device was successful., Submitted to Nucl. Instrum. Methods Phys. Res. A (NIMA Proc. Special Issue: RICH 2018), 5 pages, 6 figures
Published: 2019

23. Observation of Radar Echoes From High-Energy Particle Cascades

Author: C. Hast, Stephanie Wissel, Jiwoo Nam, Thomas Meures, N. van Eijndhoven, U. Latif, D. Z. Besson, K. D. de Vries, Zoe Riesen, Jorge Torres, John P. Ralston, Cade Sbrocco, S. Prohira, A. Nozdrina, J. J. Beatty, Amy Connolly, Chung-Yun Kuo, Patrick Allison, Physics, and Elementary Particle Physics
Subjects: High energy particle, Astrophysics::High Energy Astrophysical Phenomena, General Physics and Astronomy, FOS: Physical sciences, 01 natural sciences, 7. Clean energy, law.invention, High Energy Physics - Experiment, Nuclear physics, High Energy Physics - Experiment (hep-ex), law, Ionization, 0103 physical sciences, Radar, 010306 general physics, Instrumentation and Methods for Astrophysics (astro-ph.IM), astro-ph.HE, Physics, High Energy Astrophysical Phenomena (astro-ph.HE), hep-ex, Neutrino detector, Cathode ray, Particle, Neutrino, Astrophysics - High Energy Astrophysical Phenomena, Astrophysics - Instrumentation and Methods for Astrophysics, astro-ph.IM, Radio wave
Abstract: We report the observation of radar echoes from the ionization trails of high-energy particle cascades. These data were taken at the SLAC National Accelerator Laboratory, where the full electron beam ($\sim$10$^9$ e$^-$ at $\sim$10 GeV/e$^-$) was directed into a plastic target to simulate an ultra high-energy neutrino interaction. This target was interrogated with radio waves, and coherent radio reflections from the cascades were detected, with properties consistent with theoretical expectations. This is the first definitive observation of radar echoes from high-energy particle cascades, which may lead to a viable neutrino detection technology for energies $\gtrsim 10^{16}$ eV., Comment: 6 pages, 4 figures
Published: 2019
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24. The Simulation of the Sensitivity of the Antarctic Impulsive Transient Antenna (ANITA) to Askaryan Radiation from Cosmogenic Neutrinos Interacting in the Antarctic Ice

Author: Tsung-Che Liu, David Saltzberg, O. Banerjee, A. Romero-Wolf, S. H. Wang, M. S. Sutherland, Keith Bechtol, Abigail G. Vieregg, L. Batten, R. J. Nichol, Brian Rauch, Po-Hsun Chen, D. Seckel, Luca Macchiarulo, P. F. Dowkontt, R. Hupe, B. Strutt, C. C. Chen, Cosmin Deaconu, Chun Hsiung Chen, S. Y. Lin, J. J. Beatty, Eric Oberla, K. M. Liewer, D. Z. Besson, J. Stockham, G. S. Varner, P. Cao, B. Rotter, S. Matsuno, Harm Schoorlemmer, Amy Connolly, Stephanie Wissel, Berkeley Hill, Jiwoo Nam, C. Miki, K. Hughes, Katharine Mulrey, V. Bugaev, Andrew Ludwig, Alexander Novikov, M. H. Israel, J. W. H. Gordon, J. W. Russell, L. Cremonesi, J. Shiao, W. R. Binns, J. J. Huang, B. Dailey, J. M. Robert, Konstantin Belov, S. Stafford, Patrick Allison, B. D. Fox, M. Stockham, J. Stuhr, K. McBride, Peter Gorham, J. M. Clem, and S. Prohira
Subjects: Physics, 010308 nuclear & particles physics, Astrophysics::High Energy Astrophysical Phenomena, Monte Carlo method, Astrophysics::Instrumentation and Methods for Astrophysics, FOS: Physical sciences, Geophysics, Radiation, 01 natural sciences, 7. Clean energy, 030218 nuclear medicine & medical imaging, 03 medical and health sciences, 0302 clinical medicine, 0103 physical sciences, Parametrization (atmospheric modeling), Sensitivity (control systems), Transient (oscillation), Antenna (radio), Neutrino, Astrophysics - Instrumentation and Methods for Astrophysics, Instrumentation, Instrumentation and Methods for Astrophysics (astro-ph.IM), Mathematical Physics, Radio detection, Physics::Atmospheric and Oceanic Physics
Abstract: A Monte Carlo simulation program for the radio detection of Ultra High Energy (UHE) neutrino interactions in the Antarctic ice as viewed by the Antarctic Impulsive Transient Antenna (ANITA) is described in this article. The program, icemc, provides an input spectrum of UHE neutrinos, the parametrization of the Askaryan radiation generated by their interaction in the ice, and the propagation of the radiation through ice and air to a simulated model of the third and fourth ANITA flights. This paper provides an overview of the icemc simulation, descriptions of the physics models used and of the ANITA electronics processing chain, data/simulation comparisons to validate the predicted performance, and a summary of the impact of published results.
Published: 2019
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25. Long-baseline horizontal radio-frequency transmission through polar ice

Author: Abigail G. Vieregg, W. Clay, J. Nam, David J. Smith, D. Seckel, Michael DuVernois, J. Hanson, Tsung-Che Liu, L. Friedman, A. Nozdrina, J. Kruse, Eric Oberla, K. Mase, A. Karle, A. Ishihara, K. Kurusu, J. J. Beatty, J. L. Kelley, Y. Pan, M. Z. Wang, C. Hornhuber, Jorge Torres, Kara Hoffman, R. Young, Thomas Meures, M. Relich, M.-H. A. Huang, J. Haugen, Carl Pfendner, R. Khandelwal, P. Sandstrom, A. Christenson, C.-J. Li, M. Song, Stephanie Wissel, T. Kuwabara, S. H. Wang, Cosmin Deaconu, G. S. Varner, B. Madison, Pisin Chen, Chun Hsiung Chen, I. Kravchenko, J. Touart, Y. S. Shiao, E. Hong, A. Laundrie, S. Archambault, L. Hu, Amy Connolly, Alexander Novikov, M.-C. Kim, L. Cremonesi, R. J. Nichols, M.-Y. Lu, C. C. Chen, Patrick Allison, J. J. Huang, U. Latif, Brian Clark, Thomas M. Jordan, K. Hughes, A. Shultz, D. Z. Besson, S. Yoshida, Kael Hanson, S. Y. Hsu, and R. Gaior
Subjects: Physics, 010308 nuclear & particles physics, business.industry, FOS: Physical sciences, Astronomy and Astrophysics, 01 natural sciences, Optics, Transmission (telecommunications), 0103 physical sciences, Polar, Radio frequency, Electric potential, Astrophysics - Instrumentation and Methods for Astrophysics, 010306 general physics, Baseline (configuration management), business, Instrumentation and Methods for Astrophysics (astro-ph.IM)
Abstract: We report on analysis of englacial radio-frequency (RF) pulser data received over horizontal baselines of 1--5 km, based on broadcasts from two sets of transmitters deployed to depths of up to 1500 meters at the South Pole. First, we analyze data collected usingtwo RF bicone transmitters 1400 meters below the ice surface, and frozen into boreholes drilled for the IceCube experiment in 2011. Additionally, in Dec., 2018, a fat-dipole antenna, fed by one of three high-voltage (~1 kV), fast (~(1-5 ns)) signal generators was lowered into the 1700-m deep icehole drilled for the South Pole Ice Core Experiment (SPICE), approximately 3 km from the geographic South Pole. Signals from transmitters were recorded on the five englacial multi-receiver ARA stations, with receiver depths between 60--200 m. We confirm the long, >1 km RF electric field attenuation length, test our observed signal arrival timing distributions against models, and measure birefringent asymmetries at the 0.15% level.
Published: 2020

26. Observation of an Unusual Upward-Going Cosmic-Ray-like Event in the Third Flight of ANITA

Author: Charles J. Naudet, L. Batten, Tsung-Che Liu, S. Y. Lin, B. Strutt, David Saltzberg, R. J. Nichol, Eric Oberla, Peter Gorham, Paul Dowkontt, J. Roberts, S. H. Wang, Pisin Chen, P. Cao, Cosmin Deaconu, A. Javaid, Konstantin Belov, S. Matsuno, J. J. Beatty, L. Cremonesi, S. Prohira, J. W. H. Gordon, J. W. Russell, J. J. Huang, A. Novikov, Keith Bechtol, B. Dailey, Abigail G. Vieregg, Andrew Ludwig, Harm Schoorlemmer, J. M. Clem, R. Prechelt, S. Stafford, D. Seckel, Luca Macchiarulo, Stephanie Wissel, Andres Romero-Wolf, J. Stockham, Jiwoo Nam, K. Hughes, W. R. Binns, O. Banerjee, B. Rotter, C. Hast, C. Miki, Berkeley Hill, Patrick Allison, B. D. Fox, C. C. Chen, Chun Hsiung Chen, D. Z. Besson, K. Mulrey, V. Bugaev, M. Olmedo, G. S. Varner, M. Stockham, Brian Rauch, J. Shiao, M. H. Israel, Joe Lam, R. Hupe, Kurt Liewer, and Amy Connolly
Subjects: High Energy Astrophysical Phenomena (astro-ph.HE), Physics, 010308 nuclear & particles physics, Astrophysics::High Energy Astrophysical Phenomena, Astrophysics::Instrumentation and Methods for Astrophysics, FOS: Physical sciences, General Physics and Astronomy, Flux, Cosmic ray, Astrophysics, 01 natural sciences, Standard Model, Air shower, 0103 physical sciences, High Energy Physics::Experiment, Neutrino, Astrophysics - High Energy Astrophysical Phenomena, 010306 general physics, Event (particle physics), Charged current, Lepton
Abstract: We report on an upward traveling, radio-detected cosmic-ray-like impulsive event with characteristics closely matching an extensive air shower. This event, observed in the third flight of the Antarctic Impulsive Transient Antenna (ANITA), a NASA-sponsored long-duration balloon payload, is consistent with a similar event reported in a previous flight. These events may be produced by the atmospheric decay of an upward-propagating $\tau$-lepton produced by a $\nu_{\tau}$ interaction, although their relatively steep arrival angles create tension with the standard model (SM) neutrino cross section. Each of the two events have $a~posteriori$ background estimates of $\lesssim 10^{-2}$ events. If these are generated by $\tau$-lepton decay, then either the charged-current $\nu_{\tau}$ cross section is suppressed at EeV energies, or the events arise at moments when the peak flux of a transient neutrino source was much larger than the typical expected cosmogenic background neutrinos., Comment: 5 pages, 4 figures. Supplemental material available from corresponding author by request
Published: 2018

27. LAB4D: A Low Power, Multi-GSa/s, Transient Digitizer with Sampling Timebase Trimming Capabilities

Author: Jarred Matthew Roberts, B. Rotter, Patrick Allison, B. D. Fox, Stefan Spack, Eric Oberla, and G. S. Varner
Subjects: Physics, Nuclear and High Energy Physics, Physics - Instrumentation and Detectors, 010308 nuclear & particles physics, business.industry, FOS: Physical sciences, Integrated circuit, Instrumentation and Detectors (physics.ins-det), Converters, 01 natural sciences, law.invention, Sampling (signal processing), Application-specific integrated circuit, law, 0103 physical sciences, Bandwidth (computing), Trimming, Radio frequency, Wideband, business, Astrophysics - Instrumentation and Methods for Astrophysics, 010303 astronomy & astrophysics, Instrumentation, Instrumentation and Methods for Astrophysics (astro-ph.IM), Computer hardware
Abstract: The LAB4D is a new application-specific integrated circuit (ASIC) of the Large Analog Bandwidth Recorder and Digitizer with Ordered Readout (LABRADOR) family, for use in direct wideband radio frequency digitization such as is used in ultrahigh energy neutrino and cosmic ray astrophysics . The LAB4D is a single channel switched-capacitor array (SCA) 12-bit sampler with integrated analog-to-digital converters (ADC), developed in the TSMC 0.25 µm process. The LAB4D, operating at 3 . 2 GSa ∕ s , contains 4096 total samples arranged in 32 windows, for a total record length of 1280 ns. The 3 dB bandwidth is approximately 1.3 GHz, with a directly-coupled 50 Ω input. This represents a factor of 16 increase in the sample depth and an increase in analog bandwidth in comparison to the previous generation (LAB3) digitizer. Individually addressable windows allow for sampling and digitization to occur simultaneously, leading to nearly dead time-free kHz readout rates. All biases and current references are generated via internal digital-to-analog converters (DACs), resulting in a digitizer that requires minimal support circuitry. In addition, the LAB4D contains sample cell timebase trimming capabilities, reducing the intrinsic sample-to-sample time variance to less than 5 ps, an improvement of about 80%. This feature allows the LAB4D to be used in precision timing applications and reduces post-hoc calibration requirements.
Published: 2018
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28. Constraints on the diffuse high-energy neutrino flux from the third flight of ANITA

Author: Charles J. Naudet, M. S. Sutherland, Brian Rauch, J. J. Huang, B. Dailey, S. Y. Hsu, Andrew Ludwig, Eric Oberla, Katharine Mulrey, J. M. Clem, R. J. Nichol, B. Rotter, V. Bugaev, Berkeley Hill, W. R. Binns, Alexander Novikov, G. S. Varner, Konstantin Belov, J. Shiao, Harm Schoorlemmer, Cosmin Deaconu, Keith Bechtol, S. Prohira, J. W. H. Gordon, J. W. Russell, D. Z. Besson, Abigail G. Vieregg, A. Romero-Wolf, S. Stafford, Jiwoo Nam, D. Seckel, M. H. Israel, O. Banerjee, J. Stockham, Stephanie Wissel, L. Cremonesi, B. Strutt, S. Matsuno, J. J. Beatty, C. C. Chen, Peter Gorham, K. Hughes, Luca Macchiarulo, Chun Hsiung Chen, P. F. Dowkontt, Patrick Allison, C. Hast, L. Batten, Po-Hsun Chen, C. Miki, B. D. Fox, R. Hupe, P. Cao, K. M. Liewer, J. Roberts, M. Stockham, Tsung-Che Liu, David Saltzberg, S. H. Wang, and Amy Connolly
Subjects: Physics, High Energy Astrophysical Phenomena (astro-ph.HE), High energy, 010308 nuclear & particles physics, Payload, Signal region, Flux, FOS: Physical sciences, Astrophysics, 01 natural sciences, High Energy Physics - Experiment, High Energy Physics - Experiment (hep-ex), 13. Climate action, 0103 physical sciences, Antenna (radio), Neutrino, Astrophysics - High Energy Astrophysical Phenomena, Astrophysics - Instrumentation and Methods for Astrophysics, 010306 general physics, Event (particle physics), Instrumentation and Methods for Astrophysics (astro-ph.IM), Radio wave
Abstract: The Antarctic Impulsive Transient Antenna (ANITA), a NASA long-duration balloon payload, searches for radio emission from interactions of ultra-high-energy neutrinos in polar ice. The third flight of ANITA (ANITA-III) was launched in December 2014 and completed a 22-day flight. We present the results of three analyses searching for Askaryan radio emission of neutrino origin. In the most sensitive of the analyses, we find one event in the signal region on an expected a priori background of $0.7^{+0.5}_{-0.3}$. Though consistent with the background estimate, the candidate event remains compatible with a neutrino hypothesis even after additional post-unblinding scrutiny., Comment: 15 pages, 15 figures, Accepted to PRD
Published: 2018
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29. Antarctic Surface Reflectivity Calculations and Measurements from the ANITA-4 and HiCal-2 Experiments

Author: J. M. Clem, Peter Gorham, P. Cao, Amy Connolly, Patrick Allison, Harm Schoorlemmer, B. Rotter, B. D. Fox, Konstantin Belov, B. Dailey, Kenneth L. Ratzlaff, O. Banerjee, R. J. Nichol, M. Stockham, C. Hast, Katharine Mulrey, V. Bugaev, Abigail G. Vieregg, Stephanie Wissel, Alexander Novikov, S. Nande, D. Z. Besson, F. Wu, M. H. Israel, Cosmin Deaconu, S. Matsuno, Tsung-Che Liu, G. S. Varner, D. Seckel, J. J. Beatty, P. Jain, M. Mottram, L. Cremonesi, R. Hupe, Paramita Dasgupta, S. Stafford, A. Romero-Wolf, Joshua A. Gordon, David Saltzberg, K. Tatem, L. Batten, W. R. Binns, Joe Lam, S. Prohira, Jiwoo Nam, R. Young, Po-Hsun Chen, Andrew Ludwig, P. F. Dowkontt, B. Strutt, J. W. Russell, Chun Hsiung Chen, Eric Oberla, J. Stockham, Berkeley Hill, Brian Rauch, and C. Miki
Subjects: Physics, 010308 nuclear & particles physics, business.industry, FOS: Physical sciences, Curvature, 01 natural sciences, Wavelength, Optics, Amplitude, Orders of magnitude (time), 0103 physical sciences, Reflection (physics), Surface roughness, Astrophysics - Instrumentation and Methods for Astrophysics, 010306 general physics, business, Instrumentation and Methods for Astrophysics (astro-ph.IM), Zenith, Radio wave
Abstract: The balloon-borne HiCal radio-frequency (RF) transmitter, in concert with the ANITA radio-frequency receiver array, is designed to measure the Antarctic surface reflectivity in the RF wavelength regime. The amplitude of surface-reflected transmissions from HiCal, registered as triggered events by ANITA, can be compared with the direct transmissions preceding them by O(10) microseconds, to infer the surface power reflection coefficient $\cal{R}$. The first HiCal mission (HiCal-1, Jan. 2015) yielded a sample of 100 such pairs, resulting in estimates of $\cal{R}$ at highly-glancing angles (i.e., zenith angles approaching $90^\circ$), with measured reflectivity for those events which exceeded extant calculations. The HiCal-2 experiment, flying from Dec., 2016-Jan., 2017, provided an improvement by nearly two orders of magnitude in our event statistics, allowing a considerably more precise mapping of the reflectivity over a wider range of incidence angles. We find general agreement between the HiCal-2 reflectivity results and those obtained with the earlier HiCal-1 mission, as well as estimates from Solar reflections in the radio-frequency regime. In parallel, our calculations of expected reflectivity have matured; herein, we use a plane-wave expansion to estimate the reflectivity R from both a flat, smooth surface (and, in so doing, recover the Fresnel reflectivity equations) and also a curved surface. Multiplying our flat-smooth reflectivity by improved Earth curvature and surface roughness corrections now provides significantly better agreement between theory and the HiCal 2a/2b measurements., Comment: submitted to Astropart. Phys
Published: 2018
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30. Design and Performance of an Interferometric Trigger Array for Radio Detection of High-Energy Neutrinos

Author: S. H. Wang, M. H. Huang, C. Pfendner, R. J. Nichol, Michael DuVernois, M.-Y. Lu, J. J. Beatty, Thomas Meures, M. Z. Wang, J. Kruse, Albrecht Karle, Eric Oberla, L. Cremonesi, M. Beydler, Benjamin Hokanson-Fasig, U. Latif, Kenneth L. Ratzlaff, Y. S. Shiao, A. Ishihara, M. Sullivan, D. Z. Besson, Brian Clark, Kara Hoffman, A. Clough, Aongus O'Murchadha, E. Hong, R. Khandelwal, Pisin Chen, Abigail G. Vieregg, S. Archambault, M. Bogdan, A. Laundrie, E. Friedman, C. C. Chen, H. Landsman, Patrick Allison, P. Sandstrom, D. Seckel, M.-C. Kim, K. Wei, J. Davies, A. Shultz, Cosmin Deaconu, Stephanie Wissel, J. L. Kelley, Y. Pan, Kael Hanson, Jiwoo Nam, I. Kravchenko, J. Touart, M. Ransom, K. Hughes, R. Bard, Chun Hsiung Chen, R. Young, David J. Smith, G. Nir, C.-J. Li, J. Hanson, Tsung-Che Liu, M. Song, J. Roth, S. Yoshida, Andrew Ludwig, M. Beheler-Amass, K. Mase, K. Kurusu, J. Haugen, J. J. Huang, S. Y. Hsu, L. Hu, Amy Connolly, and Physics
Subjects: Beamforming, Nuclear and High Energy Physics, Physics - Instrumentation and Detectors, Phased array, Astrophysics::High Energy Astrophysical Phenomena, FOS: Physical sciences, Near and far field, 7. Clean energy, 01 natural sciences, Optics, 0103 physical sciences, 010306 general physics, Instrumentation, Instrumentation and Methods for Astrophysics (astro-ph.IM), Physics, 010308 nuclear & particles physics, business.industry, Detector, Astrophysics::Instrumentation and Methods for Astrophysics, Instrumentation and Detectors (physics.ins-det), Interferometry, 13. Climate action, High Energy Physics::Experiment, Neutrino, Astrophysics - Instrumentation and Methods for Astrophysics, business, Noise (radio), Radio wave
Abstract: Ultra-high energy neutrinos are detectable through impulsive radio signals generated through interactions in dense media, such as ice. Subsurface in-ice radio arrays are a promising way to advance the observation and measurement of astrophysical high-energy neutrinos with energies above those discovered by the IceCube detector ($\geq$1 PeV) as well as cosmogenic neutrinos created in the GZK process ($\geq$100 PeV). Here we describe the $\textit{NuPhase}$ detector, which is a compact receiving array of low-gain antennas deployed 185 m deep in glacial ice near the South Pole. Signals from the antennas are digitized and coherently summed into multiple beams to form a low-threshold interferometric phased array trigger for radio impulses. The NuPhase detector was installed at an Askaryan Radio Array (ARA) station during the 2017/18 Austral summer season. $\textit{In situ}$ measurements with an impulsive, point-source calibration instrument show a 50% trigger efficiency on impulses with voltage signal-to-noise ratios (SNR) of $\le$2.0, a factor of $\sim$1.8 improvement in SNR over the standard ARA combinatoric trigger. Hardware-level simulations, validated with $\textit{in situ}$ measurements, predict a trigger threshold of an SNR as low as 1.6 for neutrino interactions that are in the far field of the array. With the already-achieved NuPhase trigger performance included in ARASim, a detector simulation for the ARA experiment, we find the trigger-level effective detector volume is increased by a factor of 1.8 at neutrino energies between 10 and 100 PeV compared to the currently used ARA combinatoric trigger. We also discuss an achievable near term path toward lowering the trigger threshold further to an SNR of 1.0, which would increase the effective single-station volume by more than a factor of 3 in the same range of neutrino energies., Comment: 19 pages, 19 figures, submitted to Nuclear Instruments and Methods in Physics Research A
Published: 2018
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31. Antarctic radio frequency albedo and implications for cosmic ray reconstruction

Author: M. Mottram, C. J. Naudet, K. M. Liewer, A. Javaid, M. H. Israel, D. Z. Besson, G. S. Varner, A. Romero-Wolf, Yuh-Lin Wang, Amy Connolly, Abigail G. Vieregg, J. M. Clem, Konstantin Belov, C. Miki, D. Seckel, L. L. Ruckman, W. R. Binns, R. Y. Shang, Peter Gorham, Pisin Chen, M. Stockham, J. J. Beatty, J. Stockham, S. Hoover, Patrick Allison, Chun Hsiung Chen, Paul Dowkontt, J. W. Nam, M. Sullivan, R. J. Nichol, S. Matsuno, and David Saltzberg
Subjects: Atmosphere, Physics, Surface roughness, General Earth and Planetary Sciences, Astronomy, Cosmic ray, Radius, Radio frequency, Electrical and Electronic Engineering, Neutrino, Albedo, Condensed Matter Physics, Snow
Abstract: We describe herein a measurement of the Antarctic surface “roughness” performed by the balloon-borne ANITA (Antarctic Impulsive Transient Antenna) experiment. Originally purposed for cosmic ray astrophysics, the radio frequency (RF) receiver ANITA gondola, from its 38 km altitude vantage point, can scan a disk of snow surface 600 km in radius. The primary purpose of ANITA is to detect RF emissions from cosmic rays incident on Antarctica, such as neutrinos which penetrate through the atmosphere and interact within the ice, resulting in signal directed upward which then refracts at the ice-air interface and up and out to ANITA, or high-energy nuclei (most likely irons or protons), which interact in the upper atmosphere (at altitudes below ANITA) and produce a spray of down-coming RF which reflects off the snow surface and back up to the gondola. The energy of such high-energy nuclei can be inferred from the observed reflected signal only if the surface reflectivity is known. We describe herein an attempt to quantify the Antarctic surface reflectivity, using the Sun as a constant, unpolarized RF source. We find that the reflectivity of the surface generally follows the expectations from the Fresnel equations, lending support to the use of those equations to give an overall correction factor to calculate cosmic ray energies for all locations in Antarctica. The analysis described below is based on ANITA-II data. After launching from McMurdo Station in December 2008, ANITA-II was aloft for a period of 31 days with a typical instantaneous duty cycle exceeding 95%.
Published: 2015

32. A Ground-Based Interferometric Phased Array Trigger for Ultra-high Energy Neutrinos

Author: Patrick Allison, Andres Romero-Wolf, Eric Oberla, Andrew Ludwig, Keith Bechtol, Abigail G. Vieregg, Mircea Bogdan, Michael DuVernois, Cosmin Deaconu, Kuang Wei, Stephanie Wissel, and MaCheaux Ransom
Subjects: Beamforming, Physics, Interferometry, Optics, Anechoic chamber, business.industry, Phased array, Astrophysics::High Energy Astrophysical Phenomena, Broadband, Monte Carlo method, business, Signal, Energy (signal processing)
Abstract: We are developing a ground-based radio interferometric phased array for radio detection of high energy neutrinos, in an effort to lower the energy threshold of radio detection experiments while increasing the effective volume at high energies. The radio detection technique looks for Askaryan emission from neutrinos interacting in large volumes of glacial ice. The principle behind the phased array technique is coherent summing of the broadband, impulsive Askaryan signal from multiple antenna channels, increasing the signal-to-noise ratio for triggering on weak signals. We first discuss simulations and validation measurements related to the phased array technique, including results from a preliminary Monte Carlo simulation, a demonstration of beamforming and measurements of thermal noise correlation in an anechoic chamber, and results from a trigger simulation. We then discuss the design and development of the first ground-based interferometric phased array trigger system, a 16-channel system that has been built and will be deployed as part of one Askaryan Radio Array (ARA) station in December 2017 at the South Pole.
Published: 2017

33. 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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34. Dynamic tunable notch filters for the Antarctic Impulsive Transient Antenna (ANITA)

Author: P. F. Dowkontt, A. Novikov, J. J. Beatty, B. Rotter, J. Stockham, J. J. Huang, B. Dailey, O. Banerjee, Stephanie Wissel, C. Miki, D. Z. Besson, Peter Gorham, Amy Connolly, Jiwoo Nam, K. Mulrey, J. Shiao, R. Young, J. Kowalski, Po-Hsun Chen, J. G. Learned, J. W. Russell, Patrick Allison, V. Bugaev, Yung-Yaw Chen, J. Ripa, R. J. Nichol, G. S. Varner, Kurt Liewer, Konstantin Belov, M. Stockham, S. Stafford, Andrew Romero-Wolf, Cosmin Deaconu, Andrew Ludwig, M. H. Israel, P. Cao, S.L. Wang, Brian Rauch, Shih-Chieh Hsu, F. Wu, W. R. Binns, L. Cremonesi, B. Strutt, M. Kovacevich, K. Tatem, R. Hupe, Chun Hsiung Chen, S. Matsuno, Joshua A. Gordon, Jay Roberts, S. Prohira, J. M. Clem, Tsung-Che Liu, David Saltzberg, L. Batten, Abigail G. Vieregg, D. Seckel, J. Lam, and Eric Oberla
Subjects: Physics, Nuclear and High Energy Physics, Signal processing, 010308 nuclear & particles physics, Acoustics, Amplifier, FOS: Physical sciences, Band-stop filter, 01 natural sciences, Askaryan effect, 13. Climate action, 0103 physical sciences, Radio frequency, Transient (oscillation), Antenna (radio), 010306 general physics, Astrophysics - Instrumentation and Methods for Astrophysics, Instrumentation, Instrumentation and Methods for Astrophysics (astro-ph.IM), Noise (radio)
Abstract: The Antarctic Impulsive Transient Antenna (ANITA) is a NASA long-duration balloon experiment with the primary goal of detecting ultra-high-energy ($>10^{18}\,\mbox{eV}$) neutrinos via the Askaryan Effect. The fourth ANITA mission, ANITA-IV, recently flew from Dec 2 to Dec 29, 2016. For the first time, the Tunable Universal Filter Frontend (TUFF) boards were deployed for mitigation of narrow-band, anthropogenic noise with tunable, switchable notch filters. The TUFF boards also performed second-stage amplification by approximately 45 dB to boost the $\sim\,��\mbox{V-level}$ radio frequency (RF) signals to $\sim$ mV-level for digitization, and supplied power via bias tees to the first-stage, antenna-mounted amplifiers. The other major change in signal processing in ANITA-IV is the resurrection of the $90^{\circ}$ hybrids deployed previously in ANITA-I, in the trigger system, although in this paper we focus on the TUFF boards. During the ANITA-IV mission, the TUFF boards were successfully operated throughout the flight. They contributed to a factor of 2.8 higher total instrument livetime on average in ANITA-IV compared to ANITA-III due to reduction of narrow-band, anthropogenic noise before a trigger decision is made., 27 pages, 19 figures
Published: 2017
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35. 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. 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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

36. New electronics for the surface detectors of the Pierre Auger Observatory

Author: Peter Buchholz, Marco Aglietta, R.E. Sobin, S. Gallian, Z. Szadkowski, A. Zampieri, T. Suomijärvi, M. Gajardo, M. Kleifges, J. J. Beatty, S. Maldera, E. Lagorio, Corinne Berat, D.A. Brandt, P. Creti, G. Marsella, Patrick Allison, Brian Fick, J. Bouvier, D. Nitz, J.P. Gongora, H. Lebbolo, C. Morello, R. Halliday, R. Assiro, R. Sato, Luca Latronico, Corbin Covault, Patrick Stassi, T. Nguyen Trung, K.-H. Becker, 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 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), 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), Pierre Auger, 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), and Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)
Subjects: Physics, Pierre Auger Observatory, Photomultiplier, Physics::Instrumentation and Detectors, business.industry, Astrophysics::High Energy Astrophysical Phenomena, Detector, Astrophysics::Instrumentation and Methods for Astrophysics, Cosmic ray, Scintillator, 7. Clean energy, 030218 nuclear medicine & medical imaging, Nuclear physics, 03 medical and health sciences, 0302 clinical medicine, Optics, Upgrade, 13. Climate action, Observatory, High Energy Physics::Experiment, Electronics, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], business
Abstract: The surface detector array of the Pierre Auger Observatory consists of 1660 water-Cherenkov detector stations (WCDs) that sample the charged particles and photons of air showers initiated by energetic cosmic rays. Each station continuously samples signals from photomultiplier tubes (PMTs) viewing the water volume, and records a approximately 20 micro-second trace whenever a local trigger condition is satisfied. Absolute timing is provided by a GPS receiver on each station, and power is provided by a solar power system. The Observatory is currently implementing an upgrade, "AugerPrime". AugerPrime includes the addition of a small PMT to increase dynamic range, a plastic scintillator above each WCD to enhance the separation of electromagnetic and muon shower components, a radio detector to measure the radio emission of inclined air showers, and an infill of buried muon counters to provide additional cross checks. Consequently, new electronics to support these additional detectors is also being implemented. In addition to more measurement channels, the new electronics includes improved GPS receivers, higher sampling frequency, increased dynamic range, increased processing capability, and improved calibration and monitoring systems. This paper presents the design of the new electronics and discusses performance characteristics observed in laboratory measurements and engineering array data.
Published: 2016

37. Ultra-high-energy cosmic ray flux and energy measurement with ANITA

Author: W. Robert Binns, Jiwoo Nam, Jay Roberts, Charles J. Naudet, J. J. Beatty, Enrique Zas, Michael DuVernois, John Clem, Tim Huege, David Zeke Besson, R. J. Nichol, P. Miocinovic, G. S. Varner, Paul Dowkontt, Abigail G. Vieregg, Harm Schoorlemmer, D. Seckel, Joe Lam, S. Hoover, Andres Romero-Wolf, B. Rotter, Jaime Alvarez-Muñiz, David Urdaneta, David Saltzberg, S. W. Barwick, Jason Link, Stephanie Wissel, K. J. Palladino, Konstantin Belov, Christian Miki, C. Hast, Peter Gorham, Brian Rauch, Patrick Allison, A. Javaid, W. R. Carvalho, Katharine Mulrey, M. H. Israel, and Amy Connolly
Subjects: Physics, Flux, Ultra-high-energy cosmic ray, Energy (signal processing), Computational physics
Published: 2016

38. Energy estimation of cosmic rays with the Engineering Radio Array of the Pierre Auger Observatory

Author: Pierre Auger Collaboration (Alexander Aab (Siegen, U. )., Pedro Abreu (LIP, Lisbon &amp, Lisbon, IST), Marco Aglietta (IFSI, Turin), Eun-Joo Ahn (Fermilab), Imen Al Samarai (Orsay, IPN), Ivone Albuquerque (Sao Paulo, U. )., Ingomar Allekotte (Centro Atomico Bariloche &amp, Balseiro, Inst., San Carlos de Bariloche), Patrick Allison (Ohio State, U. )., Alejandro Almela, (U. Tech. Natl., Argentina), Jesus Alvarez Castillo (Mexico, U. )., Jaime Alvarez-Muñiz (Santiago de Compostela, U. )., Rafael Alves Batista (Hamburg, U., II), Inst. Theor. Phys., amp, INFN, Michelangelo Ambrosio (Naples U., Naples), Amin Aminaei (Nijmegen, U., IMAPP), INFN, Gioacchino Alex Anastasi (Catania U., Catania), Luis Anchordoqui (Lehman, Coll. )., Sofia Andringa (LIP, INFN, Carla Aramo (Naples U., Fernando Arqueros (Madrid, U. )., Nicusor Arsene (Bucharest, U. )., Hernán Gonzalo Asorey (Centro Atomico Bariloche &amp, San Carlos de Bariloche &amp, Cantabria, U., Santander), Pedro Assis (LIP, Julien Aublin (Paris, U., VI-VII), Gualberto Avila (Pierre Auger, Observ. )., Nafiun Awal (New York, U. )., Alina Mihaela Badescu (Bucharest, Polytechnic, Inst. )., Colin Baus (KIT, Karlsruhe, EKP), Jim Beatty (Ohio State, U. )., Karl Heinz Becker (Wuppertal, U. )., Jose A Bellido (Adelaide, U. )., Corinne Berat (LPSC, Grenoble), Mario Edoardo Bertaina (IFSI, Xavier Bertou (Centro Atomico Bariloche &amp, Peter Biermann (Bonn, Max Planck, Inst., Radioastro, n. )., Pierre Billoir (Paris, U., Simon G Blaess (Adelaide, U. )., Alberto Blanco (LIP, Miguel Blanco (Paris, U., Jiri Blazek (Prague, Ins, t. Phys. )., INFN, Carla Bleve (Salento U., Lecce), Hans Blümer (KIT, Karlsruhe, IKP &amp, KIT, Karlsruhe, IKP), Martina Boháčová (Prague, Denise Boncioli (Gran Sasso), Carla Bonifazi (Rio de Janeiro Federal, U. )., Nataliia Borodai (Cracow, INP), Jeffrey Brack (Colorado State, U. )., Iliana Brancus (Bucharest, IFIN-HH), Thomas Bretz (Aachen, Tec, h. Hochsch. )., Ariel Bridgeman (KIT, Pedro Brogueira (LIP, Peter Buchholz (Siegen, U. )., CAFPE, Antonio Bueno (Granada U., Granada), Stijn Buitink (Nijmegen, U., INFN, Mario Buscemi (Naples U., Karen, S Caballero-Mora (Unlisted, FR), INFN, Barbara Caccianiga (Milan U., Milan), Lorenzo Caccianiga (Paris, U., Marina Candusso (Rome, U., Tor Vergata &amp, INFN, Rome2), Laurentiu Caramete (Bucharest, Space Sciences), Inst., Caruso, R, Antonella Castellina (IFSI, INFN, Gabriella Cataldi (Salento U., Lorenzo Cazon (LIP, INFN, Rosanna Cester (Turin U., Alan, G Chavez (IFM-UMSNH, Michoacan), Andrea Chiavassa (IFSI, Jose Augusto Chinellato (Campinas State, U. )., Jiri Chudoba (Prague, INFN, Marco Cilmo (Naples U., Roger W Clay (Adelaide, U. )., INFN, Giuseppe Cocciolo (Salento U., INFN, Roberta Colalillo (Naples U., Alan Coleman (Penn State, U. )., INFN, Laura Collica (Milan U., INFN, Maria Rita Coluccia (Salento U., Ruben Conceição (LIP, Fernando Contreras (Pierre Auger, Observ. )., Mathew J Cooper (Adelaide, U. )., Alain Cordier (Orsay, LAL), Stephane Coutu (Penn State, U. )., Corbin Covault (Case Western Reserve, U. )., James Cronin (Chicago, U., EFI), Richard Dallier (Station Radioastronomy, Nancay &amp, SUBATECH, Nantes), Bruno Daniel (Campinas State, U. )., Buenos Aires, Sergio Dasso (Buenos Aires U., IAFE), Kai Daumiller (KIT, Bruce R Dawson (Adelaide, U. )., Rogerio, M de Almeida (Niteroi, Fluminense, U. )., Sijbrand J de Jong (Nijmegen, U., IMAPP &amp, NIKHEF, Amsterdam), Giuseppe De Mauro (Nijmegen, U., Joao de Mello Neto (Rio de Janeiro Federal, U. )., INFN, Ivan De Mitri (Salento U., Jaime de Oliveira (Niteroi, Vitor de Souza (Sao Paulo, U., Sao, Carlos), Luis del Peral (Alcala de Henares, U. )., Olivier Deligny (Orsay, Niraj Dhital (Michigan, Tech. U. )., Claudio Di Giulio (Rome, U., INFN, Armando Di Matteo (L'Aquila U., Aquila), Johana Chirinos Diaz (Michigan, Tech. U. )., Mary Lucia Díaz Castro (Campinas State, U. )., Francisco Diogo (LIP, Carola Dobrigkeit (Campinas State, U. )., Wendy Docters (Groningen, KVI), Juan Carlos D'Olivo (Mexico, U. )., Alexei Dorofeev (Colorado State, U. )., Qader Dorosti Hasankiadeh (KIT, Rita dos Anjos (Sao Paulo, U., Maria Teresa Dova (La Plata, U. )., Jan Ebr (Prague, Ralph Engel (KIT, Martin Erdmann (Aachen, Mona Erfani (Siegen, U. )., Fermilab), Carlos O Escobar (Campinas State U., Joao Espadanal (LIP, Alberto Etchegoyen, (U. Tech. Natl., Heino Falcke (Nijmegen, U., Amsterdam &amp, ASTRON, Dwingeloo), Ke Fang (Chicago, U., Glennys Farrar (New York, U. )., Anderson Fauth (Campinas State, U. )., Norberto Fazzini (Fermilab), Andrew P Ferguson (Case Western Reserve, U. )., Brian Fick (Michigan, Tech. U. )., Juan Manuel Figueira, Alberto, Filevich, Andrej Filipčič (Stefan, Inst., Ljubljana &amp, Nova Gorica, U. )., Octavian Fratu (Bucharest, Martín Miguel Freire (IFIR, Rosario &amp, Rosario, U. )., Toshihiro Fujii (Chicago, U., Beatriz García, (Natl. Tech. U., San, Rafael), Diego Garcia-Gamez (Orsay, Diego Garcia-Pinto (Madrid, U. )., Florian Gate (SUBATECH, Hartmut Gemmeke (KIT, Karlsruhe, IPE), Alexandru Gherghel-Lascu (Bucharest, Piera Luisa Ghia (Paris, U., Ugo Giaccari (Rio de Janeiro Federal, U. )., INFN, Marco Giammarchi (Milan U., Maria, Giller, Dariusz Głas (Lodz, U. )., Christian Glaser (Aachen, Henry Glass (Fermilab), Geraldina, Golup, Mariano Gómez Berisso (Centro Atomico Bariloche &amp, Primo F Gómez Vitale (Pierre Auger, Observ. )., Nicolás, González, Ben Gookin (Colorado State, U. )., Jacob Gordon (Ohio State, U. )., Alessio Gorgi (IFSI, Peter Gorham (Hawaii, U. )., Philippe Gouffon (Sao Paulo, U. )., Nathan Griffith (Ohio State, U. )., Aurelio Grillo (Gran Sasso), Trent D Grubb (Adelaide, U. )., INFN, Fausto Guarino (Naples U., Germano Guedes (UEFS, Feira de Santana), Matías Rolf Hampel, Patricia Hansen (La Plata, U. )., Diego Harari (Centro Atomico Bariloche &amp, Thomas A Harrison (Adelaide, U. )., Sebastian Hartmann (Aachen, John Harton (Colorado State, U. )., Andreas Haungs (KIT, Thomas Hebbeker (Aachen, Dieter Heck (KIT, Philipp Heimann (Siegen, U. )., Alexander, E Herve (KIT, Gary C Hill (Adelaide, U. )., Carlos Hojvat (Fermilab), Nicholas Hollon (Chicago, U., Ewa Holt (KIT, Piotr Homola (Wuppertal, U. )., Jörg Hörandel (Nijmegen, U., Pavel Horvath (Palacky, U. )., Miroslav Hrabovský (Prague, Ins, t. Phys. &amp, Palacky U. )., Daniel Huber (KIT, Tim Huege (KIT, INFN, Antonio Insolia (Catania U., Paula Gina Isar (Bucharest, Ingolf Jandt (Wuppertal, U. )., Stefan Jansen (Nijmegen, U., Cecilia Jarne (La Plata, U. )., Jeffrey, A Johnsen (Colorado School of Mines), Mariela, Josebachuili, Alex Kääpä (Wuppertal, U. )., Olga Kambeitz (KIT, Karl Heinz Kampert (Wuppertal, U. )., Peter Kasper (Fermilab), Igor Katkov (KIT, Bianca Keilhauer (KIT, Ernesto Kemp (Campinas State, U. )., Roger Kieckhafer (Michigan, Tech. U. )., Hans Klages (KIT, Matthias Kleifges (KIT, Jonny Kleinfeller (Pierre Auger, Observ. )., Raphael Krause (Aachen, Nicole Krohm (Wuppertal, U. )., Daniel Kuempel (Aachen, Gasper Kukec Mezek (Nova Gorica, U. )., Norbert Kunka (KIT, Alaa Metwaly Kuotb Awad (KIT, Danielle LaHurd (Case Western Reserve, U. )., Luca Latronico (IFSI, Robert Lauer (New Mexico, U. )., Markus Lauscher (Aachen, Pascal Lautridou (SUBATECH, Sandra Le Coz, Didier Lebrun (LPSC, Paul Lebrun (Fermilab), Marcelo Augusto Leigui de Oliveira (ABC Federal, U. )., Antoine Letessier-Selvon (Paris, U., Isabelle Lhenry-Yvon (Orsay, Katrin Link (KIT, Luis Lopes (LIP, Rebeca López (Puebla, U., Ins, t. Fis. )., Aida López Casado (Santiago de Compostela, U. )., Karim Louedec (LPSC, Agustin, Lucero, Max Malacari (Adelaide, U. )., INFN, Manuela Mallamaci (Milan U., Jennifer Maller (SUBATECH, Dusan Mandat (Prague, Paul Mantsch (Fermilab), Analisa Mariazzi (La Plata, U. )., Vincent Marin (SUBATECH, CAFPE, Ioana Mariş (Granada U., Giovanni, Marsella, INFN, Daniele Martello (Salento U., Humberto Martinez (CINVESTAV, Oscar Martínez Bravo (Puebla, U., Diane Martraire (Orsay, Jimmy Masías Meza (Buenos Aires, U. )., Hermann-Josef Mathes (KIT, Sebastian Mathys (Wuppertal, U. )., James Matthews (Louisiana State, U. )., John Matthews (New Mexico, U. )., Giorgio Matthiae (Rome, U., Daniela Maurizio (Rio de Janeiro, CBPF), Eric Mayotte (Colorado School of Mines), Peter Mazur (Fermilab), Carlos Medina (Colorado School of Mines), Gustavo Medina-Tanco (Mexico, U. )., Rebecca Meissner (Aachen, Victor Mello (Rio de Janeiro Federal, U. )., Diego, Melo, Alexander Menshikov (KIT, Stefano Messina (Groningen, Maria Isabel Micheletti (IFIR, Lukas Middendorf (Aachen, Ignacio A Minaya (Madrid, U. )., INFN, Lino Miramonti (Milan U., Bogdan Mitrica (Bucharest, CAFPE, Laura Molina-Bueno (Granada U., Silvia Mollerach (Centro Atomico Bariloche &amp, François Montanet (LPSC, Carlo Morello (IFSI, Miguel Mostafá (Penn State, U. )., Celio A Moura (ABC Federal, U. )., Marcio Aparecido Muller (Campinas State, U. )., Gero Müller (Aachen, Sarah Müller (KIT, CAFPE, Sergio Navas (Granada U., Petr Necesal (Prague, Lukas Nellen (Mexico, U. )., Anna Nelles (Nijmegen, U., Jens Neuser (Wuppertal, U. )., Phong H Nguyen (Adelaide, U. )., Mihai Niculescu-Oglinzanu (Bucharest, Marcus Niechciol (Siegen, U. )., Lukas Niemietz (Wuppertal, U. )., Tim Niggemann (Aachen, Dave Nitz (Michigan, Tech. U. )., Dalibor, Nosek, Vladimir Novotny (Charles, U. )., Lyberis Nožka (Palacky, U. )., Luis Núñez (Cantabria, U., Livingstone Ochilo (Siegen, U. )., Foteini Oikonomou (Penn State, U. )., Angela Olinto (Chicago, U., Noelia Pacheco (Alcala de Henares, U. )., Daniel Pakk Selmi-Dei (Campinas State, U. )., Miroslav Palatka (Prague, Juan Pallotta (LIDAR CITEFA), Philipp Papenbreer (Wuppertal, U. )., Gonzalo Parente (Santiago de Compostela, U. )., Alejandra Parra (Puebla, U., Thomas Paul (Lehman, Coll. &amp, Northeastern U. )., Miroslav Pech (Prague, Jan Pękala (Cracow, Rodrigo Pelayo (Ulisted, MX), Iuri Pepe (Bahia, U. )., INFN, Lorenzo Perrone (Salento U., Emily Petermann (Nebraska, U. )., Christine Peters (Aachen, INFN, Sergio Petrera (L'Aquila U., Yevgeniy Petrov (Colorado State, U. )., Jamyang Phuntsok (Penn State, U. )., Ricardo Piegaia (Buenos Aires, U. )., Tanguy Pierog (KIT, Pablo Pieroni (Buenos Aires, U. )., Mário Pimenta (LIP, INFN, Valerio Pirronello (Catania U., Manuel, Platino, Matthias Plum (Aachen, Alessio Porcelli (KIT, Czeslaw Porowski (Cracow, Raul Ribeiro Prado (Sao Paulo, U., Paolo Privitera (Chicago, U., Michael Prouza (Prague, Eduardo, J Quel (LIDAR CITEFA), Sven Querchfeld (Wuppertal, U. )., Sean Quinn (Case Western Reserve, U. )., Julian Rautenberg (Wuppertal, U. )., Olivier Ravel (SUBATECH, Diego, Ravignani, Darius Reinert (Aachen, Benoît Revenu (SUBATECH, Jan Ridky (Prague, Markus Risse (Siegen, U. )., Pablo Ristori (LIDAR CITEFA), INFN, Vincenzo Rizi (L'Aquila U., Washington Rodrigues de Carvalho (Santiago de Compostela, U. )., Jorge Rubén Rodriguez Rojo (Pierre Auger, Observ. )., Maria Dolores Rodríguez-Frías (Alcala de Henares, U. )., Dmytro Rogozin (KIT, Jaime Rosado (Madrid, U. )., Markus Roth (KIT, Esteban Roulet (Centro Atomico Bariloche &amp, Adrian Rovero (Buenos Aires, Steven J Saffi (Adelaide, U. )., Alexandra Saftoiu (Bucharest, Humberto Salazar (Puebla, U., Ahmed Saleh (Nova Gorica, U. )., Francisco Salesa Greus (Penn State, U. )., Gaetano Salina (Rome, U., Jose Sanabria Gomez (Cantabria, U., Federico, Sánchez, CAFPE, Patricia Sanchez-Lucas (Granada U., Edivaldo Moura Santos (Sao Paulo, U. )., Eva Santos (Campinas State, U. )., Fred Sarazin (Colorado School of Mines), Biswaijt Sarkar (Wuppertal, U. )., Raul Sarmento (LIP, Christian Sarmiento-Cano (Cantabria, U., Ricardo, Sato, Carlos Scarso (Pierre Auger, Observ. )., Markus Schauer (Wuppertal, U. )., INFN, Viviana Scherini (Salento U., Harald, Schieler, David Schmidt (KIT, Olaf Scholten (Groningen, Harm Schoorlemmer (Hawaii, U. )., Petr Schovánek (Prague, Frank, G Schröder, Alexander Schulz (KIT, Johannes Schulz (Nijmegen, U., Johannes Schumacher (Aachen, Sergio Sciutto (La Plata, U. )., Alberto Segreto (IASF, Palermo), Mariangela Settimo (Paris, U., Amir Shadkam (Louisiana State, U. )., Ronald, C Shellard (Rio de Janeiro, Guenter Sigl (Hamburg, U., Octavian Sima (Bucharest, U. )., Andrzej Śmiałkowski (Lodz, U. )., Radomir Šmída (KIT, Gregory Snow (Nebraska, U. )., Paul Sommers (Penn State, U. )., Sebastian Sonntag (Siegen, U. )., J Sorokin (Adelaide, U. )., Ruben Squartini (Pierre Auger, Observ. )., Yogendra N Srivastava (Northeastern, U. )., Denis Stanca (Bucharest, Samo Stanič (Nova Gorica, U. )., James Stapleton (Ohio State, U. )., Jaroslaw Stasielak (Cracow, Maurice Stephan (Aachen, Anne Stutz (LPSC, Federico Suarez, (U. Tech. Natl., Mauricio Suarez Durán (Cantabria, U., Tiina Suomijärvi (Orsay, A Daniel Supanitsky (Buenos Aires, Michael Sutherland (Ohio State, U. )., John Swain (Northeastern, U. )., Zbigniew Szadkowski (Lodz, U. )., Oscar Alejandro Taborda (Centro Atomico Bariloche &amp, Alex, Tapia, Andreas Tepe (Siegen, U. )., Vanessa Menezes Theodoro (Campinas State, U. )., Omar Tibolla (Unlisted, Charles Timmermans (Nijmegen, U., Carlos, J Todero Peixoto, Gabriel Toma (Bucharest, Lenka Tomankova (KIT, Bernardo Tomé (LIP, INFN, Aurelio Tonachini (Turin U., Guillermo Torralba Elipe (Santiago de Compostela, U. )., Diego Torres Machado (Rio de Janeiro Federal, U. )., Petr Travnicek (Prague, Marta Trini (Nova Gorica, U. )., Ralf Ulrich (KIT, Michael Unger (KIT, New York, U. )., Martin Urban (Aachen, Jose F Valdés Galicia (Mexico, U. )., Ines Valiño (Santiago de Compostela, U. )., INFN, Laura Valore (Naples U., Guus van Aar (Nijmegen, U., Patrick van Bodegom (Adelaide, U. )., M van den Berg (Groningen, Ad, Sjoert van Velzen (Nijmegen, U., Arjen van Vliet (Hamburg, U., Enrique Varela (Puebla, U., Bernardo Vargas Cárdenas (Mexico, U. )., Gary Varner (Hawaii, U. )., Rafael Vasquez (Rio de Janeiro Federal, U. )., Jose R Vázquez (Madrid, U. )., Ricardo Vázquez (Santiago de Compostela, U. )., Darko Veberič (KIT, Valerio Verzi (Rome, U., Jakub Vicha (Prague, Mariela, Videla, Luis Villaseñor (IFM-UMSNH, Brian Vlcek (Alcala de Henares, U. )., Serguei Vorobiov (Nova Gorica, U. )., Hernan Wahlberg (La Plata, U. )., Oscar Wainberg, (U. Tech. Natl., David Walz (Aachen, Alan, Watson, Marc Weber (KIT, Klaus Weidenhaupt (Aachen, Andreas Weindl (KIT, Christoph Welling (Aachen, Felix Werner (KIT, Allan Widom (Northeastern, U. )., Lawrence Wiencke (Colorado School of Mines), Henryk Wilczyński (Cracow, Tobias, Winchen, David Wittkowski (Wuppertal, U. )., Brian, Wundheiler, Sarka Wykes (Nijmegen, U., Lili Yang (Nova Gorica, U. )., Tolga Yapici (Michigan, Tech. U. )., Alexey Yushkov (Siegen, U. )., Enrique Zas (Santiago de Compostela, U. )., Danilo, Zavrtanik, Marko Zavrtanik (Stefan, Inst., Arnulfo Zepeda (CINVESTAV, Benedikt Zimmermann (KIT, Michael Ziolkowski (Siegen, U. )., INFN, Francesca Zuccarello (Catania U., Catania), ), 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., Pokala, 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., 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 SUBATECH Nantes (SUBATECH), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université de Nantes (UN)-Mines Nantes (Mines Nantes), Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Université Grenoble Alpes [2016-2019] (UGA [2016-2019])-Centre National de la Recherche Scientifique (CNRS), Unité Scientifique de la Station de Nançay (USN), Centre National de la Recherche Scientifique (CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire des Sciences de l'Univers en région Centre (OSUC), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS)-Université d'Orléans (UO), Laboratoire de l'Accélérateur Linéaire (LAL), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), Institut de Physique Nucléaire d'Orsay (IPNO), Pierre AUGER, ANR-11-IDEX-0004,SUPER,Sorbonne Universités à Paris pour l'Enseignement et la Recherche(2011), ANR-10-LABX-0063,ILP,Institute Lagrange of Paris(2010), European Project: 328826,EC:FP7:PEOPLE,FP7-PEOPLE-2012-IEF,AUGER2FUTURE(2013), Elementary Particle Physics, Physics, 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), Mines Nantes (Mines Nantes)-Université de Nantes (UN)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Institut 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]), 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), 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), Ahn, E. . j., Albuquerque, I. . f. . m., Anastasi, G. . a., Badescu, A. . m., Beatty, J. . j., Becker, K. . h., Bellido, J. . a., Bertaina, M. . e., Biermann, P. . l., Blaess, S. . g., Bleve, Carla, Caballero Mora, K. . s., Chavez, A. . g., Chinellato, J. . a., Clay, R. . w., Colalillo, R., Coluccia, MARIA RITA, Cooper, M. . j., Covault, C. . e., Dawson, B. . r., de Almeida, R. . m., de Jong, S. . j., de Mello Neto, J. . r. . t., DE MITRI, Ivan, de Oliveira, J., de Souza, V., del Peral, L., Diaz, J. . c., Díaz Castro, M. . l., D’Olivo, J. . c., dos Anjos, R. . c., Dova, M. . t., Escobar, C. . o., Fauth, A. . c., Ferguson, A. . p., Figueira, J. . m., Freire, M. . m., Ghia, P. . l., Gómez Vitale, P. . f., Grillo, A. . f., Grubb, T. . d., Guarino, F., Guedes, G. . p., Hampel, M. . r., Harrison, T. . a., Harton, J. . l., Herve, A. . e., Hill, G. . c., Hörandel, J. . r., Isar, P. . g., Johnsen, J. . a., Kampert, K. . h., Kieckhafer, R. . m., Klages, H. . o., Kuotb Awad, A. . w., Leigui de Oliveira, M. . a., Mariazzi, A. . g., Mariş, I. . c., Marsella, Giovanni, Martello, Daniele, Masías Meza, J. . j., Mathes, H. . j., Matthews, J. . a. . j., Mazur, P. . o., Mello, V. . b. . b., Micheletti, M. . i., Minaya, I. . a., Moura, C. . a., Muller, M. . a., Nguyen, P. . h., Núñez, L. . a., Pȩkala, J., Pepe, I. . m., Perrone, Lorenzo, Prado, R. . r., Quel, E. . j., Rodrigues de Carvalho, W., Rodríguez Frías, M. . d., Rovero, A. . c., Saffi, S. . j., Sanabria Gomez, J. . d., Santos, E. . m., Schröder, F. . g., Sciutto, S. . j., Shellard, R. . c., Snow, G. . r., Srivastava, Y. . n., Supanitsky, A. . d., Sutherland, M. . s., Taborda, O. . a., Theodoro, V. . m., Todero Peixoto, C. . j., Valdés Galicia, J. . f., Valore, L., van Aar, G., van Bodegom, P., van den Berg, A. . m., van Velzen, S., van Vliet, A., Vázquez, J. . r., Vázquez, R. . a., Watson, A. . a., Research unit Astroparticle Physics, and Research unit Nuclear & Hadron Physics
Subjects: Cosmic ray showers, Astronomy, Ciencias Físicas, ULTRA HIGH ENERGY COSMIC RAYS, Astrophysics, 01 natural sciences, purl.org/becyt/ford/1 [https], ultra-high energy cosmic rays, extensive air showers, radio energy estimation, CODALEMA, Observatory, Radio detection, Physics, High Energy Astrophysical Phenomena (astro-ph.HE), Detector, Astrophysics::Instrumentation and Methods for Astrophysics, ComputingMethodologies_DOCUMENTANDTEXTPROCESSING, Física nuclear, Astrophysics - High Energy Astrophysical Phenomena, Astrophysics - Instrumentation and Methods for Astrophysics, CIENCIAS NATURALES Y EXACTAS, EXTENSIVE AIR-SHOWERS, MONTE-CARLO SIMULATIONS, EMISSION, [PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], Nuclear and High Energy Physics, EXTENSIVE AIR-SHOWERS, MONTE-CARLO SIMULATIONS, EMISSION, CODALEMA, COREAS, LOFAR, AIR SHOWERS, Astrophysics::High Energy Astrophysical Phenomena, FOS: Physical sciences, Cosmic ray, Astrophysics::Cosmology and Extragalactic Astrophysics, EXTENSIVE AIR-SHOWERS, RADIO EMISSION, 0103 physical sciences, High Energy Physics, 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, Computational physics, Astronomía, COREAS, Earth's magnetic field, Air shower, Experimental High Energy Physics, EMISSION, MONTE-CARLO SIMULATIONS
Abstract: The Auger Engineering Radio Array (AERA) is part of the Pierre Auger Observatory and is used to detect the radio emission of cosmic-ray air showers. These observations are compared to the data of the surface detector stations of the Observatory, which provide well-calibrated information on the cosmic-ray energies and arrival directions. The response of the radio stations in the 30-80 MHz regime has been thoroughly calibrated to enable the reconstruction of the incoming electric field. For the latter, the energy deposit per area is determined from the radio pulses at each observer position and is interpolated using a two-dimensional function that takes into account signal asymmetries due to interference between the geomagnetic and charge-excess emission components. The spatial integral over the signal distribution gives a direct measurement of the energy transferred from the primary cosmic ray into radio emission in the AERA frequency range. We measure 15.8 MeV of radiation energy for a 1 EeV air shower arriving perpendicularly to the geomagnetic field. This radiation energy - corrected for geometrical effects - is used as a cosmic-ray energy estimator. Performing an absolute energy calibration against the surface-detector information, we observe that this radio-energy estimator scales quadratically with the cosmic-ray energy as expected for coherent emission. We find an energy resolution of the radio reconstruction of 22% for the data set and 17% for a high-quality subset containing only events with at least five radio stations with signal., La lista completa de autores que integran el documento puede consultarse en el archivo, Instituto de Física La Plata
Published: 2016

39. 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

40. Design and initial performance of the Askaryan Radio Array prototype EeV neutrino detector at the South Pole

Author: M. A. Huang, Robert Bard, H. Landsman, Lisa Ritter, Sybille Böser, Andrew Wendorff, Patrick Allison, Carsten Rott, Berkeley Hill, E. Grashorn, Kenneth L. Ratzlaff, Thomas Meures, Daniel Kennedy, M.H.A. Huang, Min-Zu Wang, J. Davies, R. Nichol, Tsung-Che Liu, Chris Weaver, Kael Hanson, M. Richman, Sho Yoshida, J. J. Beatty, P. Sandstrom, M. Newcomb, R. Young, A. Ishihara, Robert Morse, Amy Connolly, Luca Macchiarulo, Christian Miki, D. Seckel, Peter Gorham, C. C. Chen, J. Auffenberg, Pisin Chen, G. S. Varner, R. Meyhandan, David Dzb Besson, K. Mase, J. Touart, B. D. Fox, Michael DuVernois, Kara Kdh Hoffman, E. Hong, Albrecht Karle, K. Helbing, B. Rotter, and James Haugen
Subjects: Planetary body, Physics, business.industry, Astrophysics::Instrumentation and Methods for Astrophysics, Astronomy, Astronomy and Astrophysics, law.invention, Askaryan effect, Jupiter, Orbiter, Neutrino detector, law, Astrophysics::Earth and Planetary Astrophysics, Aerospace engineering, Antenna (radio), Radar, Neutrino, business
Abstract: We describe a concept for an instrument to measure the thickness of the ice shell on a planetary body such as Jupiter’s moon Europa. Unlike a high powered and massive device such as an ice-penetrating radar, the instrument would be a passive receiver of a naturally occurring signal generated by interactions of deep penetrating cosmic ray neutrinos. We discuss the basic concept and consider the instrument design requirements from the perspective of a NASA Outer Planet Orbiter Mission. We show results of simulations, compare signal-to-noise estimates, and examine possible components and configurations for the antenna, receiver, and electronics. We note some options that can be used to reduce mass and power. Finally, we present a list of issues that would need further study to produce a more concrete design.
Published: 2012

41. Measurements of cosmic-ray secondary nuclei at high energies with the first flight of the CREAM balloon-borne experiment

Author: S. W. Nam, A. Malinin, K. C. Kim, Gabriele Bigongiari, Riccardo Zei, J. Yang, Jung-Suk Han, S. I. Mognet, S. Coutu, S. Y. Zinn, Moo Hyun Lee, L. Lutz, S. L. Nutter, P. J. Boyle, S. P. Wakely, J. K. Lee, J. A. Jeon, Eun-Suk Seo, Patrick Allison, S. Minnick, T. J. Brandt, R. Sina, Maria Grazia Bagliesi, Inkyu Park, Paolo Maestro, J. Wu, N. H. Park, Y. S. Yoon, O. Ganel, P. S. Marrocchesi, J. J. Beatty, N. B. Conklin, Michael DuVernois, J. T. Childers, H. J. Hyun, S. P. Swordy, and H. S. Ahn
Subjects: Cosmic-ray propagation, Physics, Cosmic rays, Astrophysics::High Energy Astrophysical Phenomena, Astrophysics (astro-ph), Astrophysics::Instrumentation and Methods for Astrophysics, FOS: Physical sciences, chemistry.chemical_element, Astronomy and Astrophysics, Cosmic ray, Astrophysics, Nitrogen, Oxygen, Semiconductor detector, Nuclear physics, Transition radiation detector, chemistry, astro-ph, Scintillation counter, Ultra-high-energy cosmic ray, Boron
Abstract: We present new measurements of heavy cosmic-ray nuclei at high energies per- formed during the first flight of the balloon-borne cosmic-ray experiment CREAM (Cosmic-Ray Energetics And Mass). This instrument uses multiple charge detectors and a transition radiation detector to provide the first high accuracy measurements of the relative abundances of elements from boron to oxygen up to energies around 1 TeV/n. The data agree with previous measurements at lower energies and show a relatively steep decline (~E$^-0.6$ to E$^-0.5$) at high energies. They further show the source abundance of nitrogen relative to oxygen is ~10% in the TeV/n region., Accepted for publication in Astroparticle Physics
Published: 2008

42. Preliminary results from the second flight of CREAM

Author: S. Coutu, S. Y. Zinn, T. J. Brandt, P. S. Marrocchesi, J. H. Han, Riccardo Zei, H. S. Ahn, Eun-Suk Seo, Patrick Allison, J. T. Childers, S. I. Mognet, L. M. Barbier, J. A. Jeon, Paolo Maestro, A. Malinine, J. J. Beatty, L. Lutz, Inkyu Park, N. H. Park, J. Yang, S. Minnick, N. B. Conklin, K. C. Kim, Gabriele Bigongiari, R. Sina, P. Walpole, Michael DuVernois, J. Wu, Y. S. Yoon, O. Ganel, S. W. Nam, Maria Grazia Bagliesi, M. H. Lee, and S. L. Nutter
Subjects: Balloon measurements, Physics, Atmospheric Science, Calorimeter (particle physics), Physics::Instrumentation and Detectors, business.industry, Astrophysics::High Energy Astrophysical Phenomena, Astrophysics::Instrumentation and Methods for Astrophysics, Aerospace Engineering, Astronomy and Astrophysics, Cosmic ray, Astrophysics, Scintillator, Pulse shaping, Geophysics, Optics, Space and Planetary Science, General Earth and Planetary Sciences, business
Abstract: Launched from McMurdo (Antarctica) in December 2005, the balloon experiment CREAM (cosmic ray energetics and mass) collected about 15 million triggers during its second flight of 28 days. Redundant charge identification, by two pixelated silicon arrays and a time resolved pulse shaping technique from a scintillator system, allowed a clear signature of the primary nuclei. The energy was measured with a tungsten/SciFi calorimeter preceded by a graphite target. Preliminary results from the analysis of the data of the second flight are presented.
Published: 2008

43. Performance of a Dual Layer Silicon Charge Detector During CREAM Balloon Flight

Author: Patrick Allison, R. Sina, T. J. Brandt, Eun-Suk Seo, J. T. Childers, K. C. Kim, Gabriele Bigongiari, S. Coutu, Maria Grazia Bagliesi, N. B. Conklin, J. J. Beatty, L. M. Barbier, H. S. Ahn, J. Wu, S. Y. Zinn, J. A. Jeon, Michael DuVernois, S. Minnick, Y. S. Yoon, O. Ganel, A. Malinine, Inkyu Park, S. W. Nam, M. H. Lee, N. H. Park, S. L. Nutter, P. S. Marrocchesi, J. H. Han, J. Yang, Paolo Maestro, P. Walpole, L. Lutz, Riccardo Zei, and S. I. Mognet
Subjects: Physics, Nuclear and High Energy Physics, Range (particle radiation), Silicon, business.industry, Payload, Detector, PIN diode, chemistry.chemical_element, Cosmic ray, Dissipation, COSMIC-RAY ENERGETICS, KNEE, law.invention, Optics, Nuclear Energy and Engineering, chemistry, law, Ultra-high-energy cosmic ray, Electrical and Electronic Engineering, business
Abstract: The balloon-borne cosmic-ray experiment CREAM (Cosmic Ray Energetics And Mass) has completed two flights in Antarctica, with a combined duration of 70 days. One of the detectors in the payload is the SCD (silicon charge detector) that measures the charge of high energy cosmic rays. The SCD was assembled with silicon sensors. A sensor is a 4 × 4 array of DC-coupled PIN diode pixels with the total active area of 21 × 16 mm2. The SCD used during the first flight (December 2004-January 2005) was a single layer device, then upgraded to a dual layer device for the second flight (December 2005-January 2006), covering the total sensitive area of 779 × 795 mm2. Flight data demonstrated that adding a second layer improved SCD performance, showing excellent particle charge resolution. With a total dissipation of 136 W for the dual layer system, special care was needed in designing thermal paths to keep the detector temperature within its operational range. As a consequence, flight temperatures of the SCD, even at diurnal maximum were kept below 38°C. The SCD mechanical structure was designed to minimize the possibility of damage to the sensors and electronics from the impacts of parachute deployment and landing. The detector was recovered successfully following the flight and is being refurbished for the next flight in 2007. Details of construction, operation, and performance are presented for the dual-layered SCD flown for the second CREAM flight.
Published: 2007

44. Large scale distribution of ultra high energy cosmic rays detected at the Pierre Auger Observatory with zenith angles up to 80°

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

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

Author: J. J. Masías Meza, S. Messina, D. Maurel, S. Müller, Nicusor Arsene, A. Tapia, H. Gemmeke, C. Aramo, J. Kleinfeller, Johannes Schulz, A. Gorgi, M. Pimenta, Kai Daumiller, A. ͆miałkowski, Q. Dorosti Hasankiadeh, Paul Sommers, A. Blanco, P. Gouffon, M. J. Cooper, F. Sánchez, Carlos Medina, Yogendra N. Srivastava, M. I. Micheletti, Daniel Kuempel, Carlos Escobar, B. Revenu, Benedikt Zimmermann, Rúben Conceição, R. Vasquez, Maria Rita Coluccia, K. Link, J. Stapleton, B. Mitrica, Heino Falcke, T. Huege, R. Mussa, J. J. Beatty, J. Vicha, A. Cordier, S. Maldera, D. Nitz, J. R. Vázquez, Jeffrey Brack, Olaf Scholten, Humberto Ibarguen Salazar, Yingchun Zhu, P. Sanchez-Lucas, H. Dembinski, N. Fazzini, Ivone F. M. Albuquerque, Ke Fang, Miroslav Hrabovský, L. Perrone, Jiri Chudoba, A. Haungs, J. L. Harton, S. G. Blaess, Azadeh Keivani, A. Aab, L. Caramete, Alex Kääpä, D. Torres Machado, W. Rodrigues de Carvalho, Richard Dallier, A. Nelles, D. Harari, F. Gate, Jaime Alvarez-Muñiz, Miguel Mostafa, Lorenzo Caccianiga, V. M. Theodoro, M. E. Bertaina, B. García, A. Menshikov, Colin Baus, Tobias Winchen, P. Lebrun, R. López, Karen S. Caballero-Mora, J. W. Cronin, Alexandru Gherghel-Lascu, Marcio Aparecido Muller, P. Mantsch, L. Tomankova, Thomas Harrison, M. Zavrtanik, G. Navarra, A. López Casado, Brian Fick, Samo Stanič, Z. Szadkowski, G. C. Hill, Ralph Engel, J. Ridky, G. S. Varner, H. Schieler, Julien Aublin, F. Werner, P. van Bodegom, M. Fernandes, G. Toma, Nataliia Borodai, Karl-Heinz Kampert, Y. Guardincerri, P. Pieroni, V. M. Aranda, Alina Mihaela Badescu, S. Hartmann, Martin Erdmann, Michael Unger, K. Weidenhaupt, A. Stutz, A. van Vliet, Lu Lu, Luca Latronico, Eric Mayotte, Paula Gina Isar, Antonella Castellina, Petr Schovanek, J. F. Valdés Galicia, Pedro Brogueira, F. Salesa Greus, I. De Mitri, I. A. Minaya, B. Keilhauer, G. Cataldi, Dieter Heck, G. Golup, P. Heimann, M. Gómez Berisso, F. Arqueros, N. Kunka, B. Tome, P. Necesal, A. Porcelli, G. Müller, S. J. De Jong, M. Prouza, André Schulz, R. C. Shellard, W. Docters, Martina Bohacova, P. E. Ghia, M. Ambrosio, M. Avenier, Patrick Allison, Roger W Clay, G. Matthiae, A. C. Fauth, P. Abreu, D. Ravignani, A.M. van den Berg, Peter Hansen, Darko Veberič, F. Guarino, John Matthews, E. Kemp, Serguei Vorobiov, G. Cocciolo, Corbin Covault, B. Vlcek, Dariusz Glas, Y. Petrov, Matías Rolf Hampel, Carola Dobrigkeit, Ugo Giaccari, M. Plum, J. Sorokin, Alexander Grillo, J. Stasielak, S. Coutu, Peter Schiffer, V. Scherini, Denis Stanca, K. Louedec, Mariangela Settimo, Jose Chinellato, Fred Sarazin, Alexey Yushkov, P. Lautridou, Peter Buchholz, Luis A. Anchordoqui, Lino Miramonti, A. Widom, J. A.J. Matthews, Xavier Bertou, J. R. T. de Mello Neto, A. Zepeda, F. Suarez, Thomas Hebbeker, Sergio Dasso, Alexandra Saftoiu, V. Purrello, H. Blümer, Antonio Bueno, Markus Risse, O. A. Taborda, B. D. Fox, Alan Watson, Mihai Niculescu-Oglinzanu, M. L. Díaz Castro, G. Farrar, I.M. Brancus, M. D. Rodríguez-Frías, Pedro Assis, Francesca Zuccarello, Martín Miguel Freire, L. Molina-Bueno, D. Melo, H. Glass, A. Etchegoyen, J. Alvarez Castillo, Jan Pękala, A. Chiavassa, H. Martinez, A. Letessier-Selvon, Max Malacari, Lili Yang, David Walz, Piotr Homola, A. E. Herve, K. B. Barber, M. Platino, Guenter Sigl, F. Diogo, Javier Tiffenberg, Marco Aglietta, Lukas Middendorf, Iuri Muniz Pepe, L. R. Wiencke, C. Porowski, I. Jandt, D. Pakk Selmi-Dei, J. D. Swain, A. Dorofeev, Lorenzo Cazon, R. M. de Almeida, M. Josebachuili, Dusan Mandat, Carla Bonifazi, Jose A. Bellido, C. Jarne, Christine Peters, A. Tepe, Corinne Berat, M. Giller, Ralf Ulrich, Maurice Stephan, M. Blanco, Gualberto Avila, S. Le Coz, R. Sato, Lourenco Lopes, Denise Boncioli, M. Kleifges, D. Zavrtanik, L. del Peral, M. Buscemi, Igor Katkov, Ingomar Allekotte, M. Mallamaci, O. Ravel, E. Petermann, O. Krömer, David Wittkowski, Balázs Kégl, G. Rodriguez Fernandez, Jaime Rosado, Miroslav Pech, S. Jansen, G. Salina, A. Tonachini, Danielle LaHurd, Olivier Deligny, Rodrigo Pelayo, Marcus Niechciol, G. Parente, Stijn Buitink, Hernán Asorey, N. Awal, Angela V. Olinto, C. Di Giulio, Alberto Daniel Supanitsky, D. Martraire, C. Hojvat, Jan Ebr, M. A. Leigui de Oliveira, S. Navas, R. Cester, L. Villaseñor, P.F. Gómez Vitale, D. Maurizio, J. L. Navarro, Joshua A. Gordon, R. A. Vázquez, C. Scarso, Pavel Horvath, Philipp Papenbreer, Iván Sidelnik, M. S. Sutherland, L. Martin, J. S. Díaz, Petr Travnicek, A. Filipčič, L. Nožka, E.M. Holt, M. Urban, D. Nosek, S. Querchfeld, R. Piegaia, A. C. Rovero, Alan Coleman, Marco Cilmo, R. Meyhandan, V. Novotny, J. Bäuml, Rossella Caruso, A. Lucero, C. Bleve, C. E. Moura, Trent D. Grubb, D. Huber, D. Rogozin, J. de Oliveira, A. Saleh, L. Niemietz, Alejandro Almela, J. Maller, S. Petrera, Marc Weber, Maria-Teresa Dova, H. J. Mathes, Juan Manuel Figueira, N. Pacheco, Valerio Pirronello, Roberta Colalillo, A. G. Mariazzi, B. Vargas Cárdenas, Sofia Andringa, Tim Niggemann, G. Marsella, Vincenzo Rizi, B. Gookin, T. Suomijärvi, J. Pallotta, P. H. Nguyen, A. Weindl, A. P. Ferguson, R. Alves Batista, S. Mathys, M. Erfani, D. Martello, Markus Roth, E. J. Quel, C. J. Todero Peixoto, E. M. Santos, M. Ziolkowski, Silvia Mollerach, N. Hollon, O. Martínez Bravo, Sarka Wykes, V. Verzi, O. Kambeitz, Bruce R. Dawson, Béatrice Fuchs, P.O. Mazur, Octavian Sima, David Schmidt, R. Meissner, S. Riggi, Niraj Dhital, I. Valiño, J. Rodriguez Rojo, D. Garcia-Pinto, N. Krohm, Octavian Fratu, A. Filevich, Eun-Joo Ahn, Johannes Schumacher, B. Sarkar, Christian Glaser, A. G. Chavez, D. Lebrun, M. Schauer, F.G. Schröder, Enrique Zas, J. Neuser, J. Espadanal, M. Palatka, V. B. B. Mello, H. Wilczyński, P. Billoir, François Montanet, Fernando Contreras, S. van Velzen, K. H. Becker, F. Salamida, R. Squartini, T. Paul, I. C. Mariş, Hernan Wahlberg, L. Nellen, M. Candusso, A. Bridgeman, G. Medina-Tanco, C. Morello, S. J. Saffi, Peter Gorham, G. van Aar, Charles Timmermans, R. R. Prado, L. Collica, A. Parra, H. E. Klages, A. Di Matteo, Markus Lauscher, Nicolas Martin Gonzalez, Peter L. Biermann, J. Phuntsok, Raul Sarmento, B. Wundheiler, Paolo Privitera, Gregory R Snow, R. J. Lauer, P. Ristori, P. H. Kasper, Harm Schoorlemmer, R. M. Kieckhafer, J. Rautenberg, O. Wainberg, W. C. Brown, B. Caccianiga, E. Varela, N. Griffith, Sergio Sciutto, L. Ochilo, G. De Mauro, Jörg R. Hörandel, M. Videla, I. Lhenry-Yvon, I. Al Samarai, Antonio Insolia, G. Torralba Elipe, Eva Santos, R. Krause, L. Valore, V. Marin, Amin Aminaei, G. P. Guedes, Toshihiro Fujii, Marco Giammarchi, A. Shadkam, Juan Carlos D'Olivo, T. Pierog, Esteban Roulet, Jeffrey A. Johnsen, S. Quinn, A. Segreto, Radomir Smida, M. Ave, V. de Souza, Bruno Daniel, T. Yapici, Foteini Oikonomou, Institut de Physique Nucléaire d'Orsay (IPNO), Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de 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), Department of Astrophysics [Nijmegen], Institute for Mathematics, Astrophysics and Particle Physics (IMAPP), Radboud University [Nijmegen]-Radboud University [Nijmegen], Joseph Louis LAGRANGE (LAGRANGE), Université Nice Sophia Antipolis (1965 - 2019) (UNS), COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de la Côte d'Azur, COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-Université Côte d'Azur (UCA)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de l'Accélérateur Linéaire (LAL), 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), Universidad de Buenos Aires [Buenos Aires] (UBA), Netherlands Institute for Radio Astronomy (ASTRON), Division Bajas Temperaturas (CAB-CNEA), Comisión Nacional de Energía Atómica [ARGENTINA] (CNEA), Lawrence Berkeley National Laboratory [Berkeley] (LBNL), Sydney Institute for Astronomy (SIfA), The University of Sydney, Karlsruher Institut für Technologie (KIT), Pennsylvania State University (Penn State), Penn State System, Istituto Nazionale di Fisica Nucleare, Sezione di Torino (INFN, Sezione di Torino), Istituto Nazionale di Fisica Nucleare (INFN), Istituto Nazionale di Fisica Nucleare, Sezione di Bologna (INFN, Sezione di Bologna), 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), National Institute of Physics and Nuclear Engineering, Dipartimento di Fı'sica Generale dell'Università, Laboratoire de Physique Théorique et Modèles Statistiques (LPTMS), Université Paris-Sud - Paris 11 (UP11)-Centre National de la Recherche Scientifique (CNRS), Division Applied Science, The Hebrew University of Jerusalem (HUJ), National Research Institute of Astronomy and Geophysics [Helwan] (NRIAG), Istituto di Astrofisica Spaziale e Fisica cosmica - Palermo (IASF-Pa), Istituto Nazionale di Astrofisica (INAF), Department of Physics, University of Bucharest (UniBuc), Vrije Universiteit Amsterdam [Amsterdam] (VU), University of Hawai‘i [Mānoa] (UHM), Laboratory for astroparticle physics (LAP-UNG), Laboratory for astroparticle physics, SLAC National Accelerator Laboratory (SLAC), Stanford University, Laboratoire Kastler Brossel (LKB (Jussieu)), Fédération de recherche du Département de physique de l'Ecole Normale Supérieure - ENS Paris (FRDPENS), École normale supérieure - Paris (ENS-PSL), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-École normale supérieure - Paris (ENS-PSL), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Centre National de la Recherche Scientifique (CNRS), Department of Materials Science and Engineering [Korea], Myongji University, Laboratoire d'études spatiales et d'instrumentation en astrophysique (LESIA), Université Pierre et Marie Curie - Paris 6 (UPMC)-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 Paris Diderot - Paris 7 (UPD7)-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., Anchordoqui, L., Andringa, S., Aramo, C., Aranda, V. M., Arqueros, F., Arsene, N., Asorey, H., Assis, P., Aublin, J., Ave, M., Avenier, M., Avila, G., Awal, N., Badescu, A. M., Barber, K. B., Bäuml, J., Baus, C., Beatty, J. J., Becker, K. H., Bellido, J. A., Berat, C., Bertaina, M. E., Bertou, X., Biermann, P. L., Billoir, P., Blaess, S. G., Blanco, A., Blanco, M., Bleve, C., Blümer, H., Boháčová, M., Boncioli, D., Bonifazi, C., Borodai, N., Brack, J., Brancus, I., Bridgeman, A., Brogueira, P., Brown, W. C., Buchholz, P., Bueno, A., Buitink, S., Buscemi, Mario, 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, Marco, 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., Dembinski, H., Dhital, N., Di Giulio, C., Di Matteo, A., Diaz, J. C., Díaz Castro, M. L., Diogo, F., Dobrigkeit, C., Docters, W., D'Olivo, J. C., Dorofeev, A., Dorosti Hasankiadeh, Q., Dova, M. T., Ebr, J., Engel, R., Erdmann, M., Erfani, M., Escobar, C. O., Espadanal, J., Etchegoyen, A., Falcke, H., Fang, K., Farrar, G., Fauth, A. C., Fazzini, N., Ferguson, A. P., Fernandes, M., Fick, B., Figueira, J. M., Filevich, A., Filipčič, A., Fox, B. D., Fratu, O., Freire, M. M., Fuchs, B., Fujii, T., García, B., Garcia Pinto, D., Gate, F., Gemmeke, H., Gherghel Lascu, A., Ghia, P. E., Giaccari, U., Giammarchi, M., Giller, M., Głas, D., Glaser, C., Glass, H., Golup, G., Gómez Berisso, M., Gómez Vitale, P. F., González, N., Gookin, B., Gordon, J., Gorgi, A., Gorham, P., Gouffon, P., Griffith, N., Grillo, A. F., Grubb, T. D., Guardincerri, Y., Guarino, 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., Kégl, B., Keilhauer, B., Keivani, A., Kemp, E., Kieckhafer, R. M., Klages, H. E., Kleifges, M., Kleinfeller, J., Krause, R., Krohm, N., Krömer, O., Kuempel, D., Kunka, N., Lahurd, D., Latronico, L., Lauer, R., Lauscher, M., Lautridou, P., Le Coz, S., Lebrun, D., Lebrun, P., Leigui De Oliveira, M. A., Letessier Selvon, A., Lhenry Yvon, I., Link, K., Lopes, L., López, R., López Casado, A., Louedec, K., Lu, L., Lucero, A., Malacari, M., Maldera, S., Mallamaci, M., Maller, J., Mandat, D., Mantsch, P., Mariazzi, A. G., Marin, V., Mariş, I. C., Marsella, G., Martello, D., Martin, L., Martinez, H., Martínez Bravo, O., Martraire, D., Masías Meza, J. J., Mathes, H. J., Mathys, S., Matthews, J., Matthews, J. A. J., Matthiae, G., Maurel, D., Maurizio, D., Mayotte, E., Mazur, P. O., Medina, C., Medina Tanco, G., Meissner, R., Mello, V. B. B., Melo, D., Menshikov, A., Messina, S., Meyhandan, R., Micheletti, M. I., Middendorf, L., Minaya, I. A., Miramonti, L., Mitrica, B., Molina Bueno, L., Mollerach, S., Montanet, F., Morello, C., Mostafá, M., Moura, C. E., Muller, M. A., Müller, G., Müller, S., Mussa, R., Navarra, G., Navarro, J. L., Navas, S., Necesal, P., Nellen, L., Nelles, A., Neuser, J., Nguyen, P. H., Niculescu Oglinzanu, M., Niechciol, M., Niemietz, L., Niggemann, T., Nitz, D., Nosek, D., Novotny, V., Nožka, L., Ochilo, L., Oikonomou, F., Olinto, A., Pacheco, N., Pakk Selmi Dei, D., Palatka, M., Pallotta, J., Papenbreer, P., Parente, G., Parra, A., Paul, T., Pech, M., Pekala, J., Pelayo, R., Pepe, I. M., Perrone, L., Petermann, E., Peters, C., Petrera, S., Petrov, Y., Phuntsok, J., Piegaia, R., Pierog, T., Pieroni, P., Pimenta, M., Pirronello, V., Platino, M., Plum, M., Porcelli, A., Porowski, C., Prado, R. R., Privitera, P., Prouza, M., Purrello, V., Quel, E. J., Querchfeld, S., Quinn, S., Rautenberg, J., Ravel, O., Ravignani, D., Revenu, B., Ridky, J., Riggi, S., Risse, M., Ristori, P., Rizi, V., Rodrigues De Carvalho, W., Rodriguez Fernandez, G., Rodriguez Rojo, J., Rodríguez Frías, M. D., Rogozin, D., Rosado, J., Roth, M., Roulet, E., Rovero, A. C., Saffi, S. J., Saftoiu, A., Salamida, F., Salazar, H., Saleh, A., Salesa Greus, F., Salina, G., Sánchez, F., Sanchez Lucas, P., Santos, E., Santos, E. M., Sarazin, F., Sarkar, B., Sarmento, R., Sato, R., Scarso, C., Schauer, M., Scherini, V., Schieler, H., Schiffer, P., Schmidt, D., Scholten, O., Schoorlemmer, H., Schovánek, P., Schröder, F. G., Schulz, A., Schulz, J., Schumacher, J., Sciutto, S. J., Segreto, A., Settimo, M., Shadkam, A., Shellard, R. C., Sidelnik, I., Sigl, G., Sima, O., ͆miałkowski, A., Šmída, R., Snow, G. R., Sommers, P., Sorokin, J., Squartini, R., Srivastava, Y. N., Stanca, D., Stanič, S., Stapleton, J., Stasielak, J., Stephan, M., Stutz, A., Suarez, F., Suomijärvi, T., Supanitsky, A. D., Sutherland, M. S., Swain, J., Szadkowski, Z., Taborda, O. A., Tapia, A., Tepe, A., Theodoro, V. M., Tiffenberg, J., Timmermans, C., Todero Peixoto, C. J., Toma, G., Tomankova, L., Tomé, B., Tonachini, A., Torralba Elipe, G., Torres Machado, D., Travnicek, P., Ulrich, R., Unger, M., Urban, M., Valdés Galicia, J. F., Valiño, I., Valore, 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., Werner, F., Widom, A., Wiencke, L., Wilczyński, H., Winchen, T., Wittkowski, D., Wundheiler, B., Wykes, S., Yang, L., Yapici, T., Yushkov, A., Zas, E., Zavrtanik, D., Zavrtanik, M., Zepeda, A., Zhu, Y., Zimmermann, B., Ziolkowski, M., Zuccarello, F., Physics, Elementary Particle Physics, UNIVERSIDADE DE ESTADUAL DE CAMPINAS, Research unit Astroparticle Physics, Ahn, E. . J., Albuquerque, I. . F. . M., Aranda, V. . M., Badescu, A. . M., Barber, K. . B., Beatty, J. . J., Becker, K. . H., Bellido, J. . A., Bertaina, M. . E., Biermann, P. . L., Blaess, S. . G., Bleve, Carla, Brown, W. . C., Buscemi, M., Caballero Mora, K. . S., Chavez, A. . G., Chinellato, J. . A., Cilmo, M., Clay, R. . W., Colalillo, R., Coluccia, MARIA RITA, Cooper, M. . J., Covault, C. . E., Dawson, B. . R., de Almeida, R. . M., de Jong, S. . J., de Mello Neto, J. . R. . T., DE MITRI, Ivan, de Oliveira, J., de Souza, V., del Peral, L., Diaz, J. . C., Díaz Castro, M. . L., D’Olivo, J. . C., Dova, M. . T., Escobar, C. . O., Fauth, A. . C., Ferguson, A. . P., Figueira, J. . M., Fox, B. . D., Freire, M. . M., Ghia, P. . L., Gómez Vitale, P. . F., Grillo, A. . F., Grubb, T. . D., Guarino, F., Guedes, G. . P., Hampel, M. . R., Harrison, T. . A., Harton, J. . L., Herve, A. . E., Hill, G. . C., Hörandel, J. . R., Isar, P. . G., Johnsen, J. . A., Kampert, K. . H., Kieckhafer, R. . M., Klages, H. . O., Leigui de Oliveira, M. . A., Mariazzi, A. . G., Mariş, I. . C., Marsella, Giovanni, Martello, Daniele, Masías Meza, J. . J., Mathes, H. . J., Matthews, J. . A. . J., Mazur, P. . O., Mello, V. . B. . B., Micheletti, M. . I., Minaya, I. . A., Moura, C. . A., Muller, M. . A., Navarro, J. . L., Nguyen, P. . H., Pȩkala, J., Pepe, I. . M., Perrone, Lorenzo, Prado, R. . R., Quel, E. . J., Rodrigues de Carvalho, W., Rodríguez Frías, M. . D., Rovero, A. . C., Saffi, S. . J., Santos, E. . M., Scherini, Viviana, Schröder, F. . G., Sciutto, S. . J., Shellard, R. . C., Śmiałkowski, A., Snow, G. . R., Srivastava, Y. . N., Supanitsky, A. . D., Sutherland, M. . S., Taborda, O. . A., Theodoro, V. . M., Todero Peixoto, C. . J., Valdés Galicia, J. . F., Valore, L., van Aar, G., van Bodegom, P., van den Berg, A. . M., van Velzen, S., van Vliet, A., Vázquez, J. . R., Vázquez, R. . A., Watson, A. . A., 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), Radboud university [Nijmegen]-Radboud university [Nijmegen], Université Côte d'Azur (UCA)-Université Nice Sophia Antipolis (... - 2019) (UNS), COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Observatoire de la Côte d'Azur, Université Côte d'Azur (UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Centre National de la Recherche Scientifique (CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire des Sciences de l'Univers en région Centre (OSUC), Université Paris sciences et lettres (PSL)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS)-Université d'Orléans (UO), Institut des Nanosciences de Paris (INSP), Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Laboratory for Integrated Micro Mechatronics Systems (LIMMS), Centre National de la Recherche Scientifique (CNRS)-The University of Tokyo (UTokyo), 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), Association des services de santé au travail de la Vienne (ASSTV), Immunologie et chimie thérapeutiques (ICT), Cancéropôle du Grand Est-Centre National de la Recherche Scientifique (CNRS), Centre National de la Recherche Scientifique (CNRS)-Université Paris-Sud - Paris 11 (UP11), Propriétés Optiques des Matériaux et Applications (POMA), Centre National de la Recherche Scientifique (CNRS)-Université d'Angers (UA), Colorado School of Mines, Radboud university [Nijmegen], Université Pierre et Marie Curie - Paris 6 (UPMC)-Fédération de recherche du Département de physique de l'Ecole Normale Supérieure - ENS Paris (FRDPENS), École normale supérieure - Paris (ENS Paris), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-École normale supérieure - Paris (ENS Paris), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Centre National de la Recherche Scientifique (CNRS), A. A. Noyes Laboratory of Chemical Physics, and California Institute of Technology (CALTECH)
Subjects: Physics::Instrumentation and Detectors, Astronomy, Solar neutrino, OBSERVATORY, Ciencias Físicas, 01 natural sciences, 7. Clean energy, Ultra-high-energy cosmic rays and neutrinos, high-energy showers, ground detector arrays, Pierre Auger Observatory, Settore FIS/04 - Fisica Nucleare e Subnucleare, purl.org/becyt/ford/1 [https], ENERGY, Neutrino, muon, pion, and other elementary particle detectors, cosmic ray detectors, HIGH, Cosmic-rays, DIFFUSE, ComputingMilieux_MISCELLANEOUS, High Energy Astrophysical Phenomena (astro-ph.HE), Physics, [PHYS]Physics [physics], Neutrino, muon, pion, and other elementary particles, cosmic rays, Settore FIS/01 - Fisica Sperimentale, IMPROVED, Physique atomique et nucléaire, Cosmic neutrino background, NEUTRINOS, ComputingMethodologies_DOCUMENTANDTEXTPROCESSING, Measurements of neutrino speed, Física nuclear, Neutrino, Astrophysics - High Energy Astrophysical Phenomena, physics, AUGER, CIENCIAS NATURALES Y EXACTAS, FLUX, Nuclear and High Energy Physics, Astrophysics::High Energy Astrophysical Phenomena, FOS: Physical sciences, Cosmic ray, Neutrino muon pion and other elementary particles, LIMIT, Nuclear physics, Settore FIS/05 - Astronomia e Astrofisica, Spectrum, 0103 physical sciences, ddc:530, 010306 general physics, ULTRA, Cosmic rays, Zenith, Pierre Auger Observatory, PIERRE, 010308 nuclear & particles physics, High Energy Physics::Phenomenology, Array, Física, Detector, purl.org/becyt/ford/1.3 [https], ASTROFÍSICA, Solar neutrino problem, Nuclei, Astronomía, Neutrino muon pion and other elementary particle detectors, Experimental High Energy Physics, High Energy Physics::Experiment, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
Abstract: Neutrinos in the cosmic ray flux with energies near 1 EeV and above are detectable with the Surface Detector array (SD) of the Pierre Auger Observatory. We report here on searches through Auger data from 1 January 2004 until 20 June 2013. No neutrino candidates were found, yielding a limit to the diffuse flux of ultrahigh energy neutrinos that challenges the Waxman-Bahcall bound predictions. Neutrino identification is attempted using the broad time structure of the signals expected in the SD stations, and is efficiently done for neutrinos of all flavors interacting in the atmosphere at large zenith angles, as well as for "Earth-skimming" neutrino interactions in the case of tau neutrinos. In this paper the searches for downward-going neutrinos in the zenith angle bins 60°-75°and 75°-90°as well as for upward-going neutrinos, are combined to give a single limit. The 90% C.L. single-flavor limit to the diffuse flux of ultrahigh energy neutrinos with an E⁻² spectrum in the energy range 1.0 × 10¹⁷ eV-2.5 × 10¹⁹ eV is E²νdNν/dEν < 6.4 × 10⁻⁹ GeVcm⁻² s⁻¹ sr⁻¹., La lista completa de autores que integran el documento puede consultarse en el archivo., Facultad de Ciencias Exactas, Instituto de Física La Plata
Published: 2015

46. The Pierre Auger cosmic ray observatory

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

47. Search for patterns by combining cosmic-ray energy and arrival directions at the Pierre Auger Observatory

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

48. Searches for anisotropies in the arrival directions of the highest energy cosmic rays detected by the Pierre Auger Observatory

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

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

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

50. Muons in air showers at the Pierre Auger Observatory: Measurement of atmospheric production depth

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

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