[PDF] Top 20 The Pierre Auger Cosmic Ray Observatory
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The Pierre Auger Cosmic Ray Observatory
... RU-PD-2011-3-0062, the Minister of National Education, Programme for research - Space Technology and Advanced Research - STAR, project number 83/2013, Roma- nia; Slovenian Research Agency, Slovenia; Comunidad de ... See full document
97
Muon counting using silicon photomultipliers in the AMIGA detector of the Pierre Auger observatory
... shield the electromagnetic component of cosmic ray showers and it is composed of three scintillation ...bar. The light produced in the bars is absorbed by the WLS ...fiber. ... See full document
23
Techniques for Measuring Aerosol Attenuation using the Central Laser Facility at the Pierre Auger Observatory
... : The Pierre Auger Observatory in Malargüe, Argentina, is designed to study the prop- erties of ultra-high energy cosmic rays with energies above 10 18 ...from the FD, ... See full document
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Search for ultrahigh energy neutrinos in highly inclined events at the Pierre Auger Observatory
... GAAV KJB100100904, MSMT-CR LA08016, LC527, 1M06002, and MSM0021620859, Czech Republic; Centre de Calcul IN2P3/CNRS, Centre National de la Recherche Scientifique (CNRS), Conseil Re´gional Ile-de- France, De´partement ... See full document
16
Combined fit of spectrum and composition data as measured by the Pierre Auger Observatory
... to the increased level of interactions that produce abundant secondary protons, whereas with m < 0 the goodness of fit is not affected much and a higher injection spectral index is ...Limiting the ... See full document
40
Azimuthal Asymmetry in the Risetime of the Surface Detector Signals of the Pierre Auger Observatory
... from the measurements of (sec θ) max for the two distance ranges to previous mass estimates from the Pierre Auger Observatory [5, ...13]. The three mass measurements have ... See full document
16
A targeted search for point sources of EeV photons with the Pierre Auger Observatory
... 0450696; The Grainger Founda- tion; Marie Curie-IRSES/EPLANET; European Parti- cle Physics Latin American Network; European Union 7th Framework Program, Grant ... See full document
9
Measurement of the Muon Content of EAS With the Pierre Auger Observatory
... present the results of three different classes of methods: 1) separating the muonic and electromagnetic signals based on their different time structures, 2) using inclined showers, for which the ... See full document
6
Particle physics measurements at the highest energies with the Pierre Auger Observatory
... The Pierre Auger Observatory measures cosmic rays with energies between 10 ...duty-cycle. The cross-section for the primary interaction of 10 18 eV protons with air has ... See full document
7
Measurement of the average electromagnetic longitudinal shower profile at the Pierre Auger Observatory
... in the propagation of the light, so several sys- tematic uncertainties related to it were studied: cloud effects, uncertainties of the overall aerosol content as well as its height dependence, ... See full document
8
Large Scale Distribution of Ultra High Energy Cosmic Rays Detected at the Pierre Auger Observatory With Zenith Angles up to 80°
... As the amplitudes of the large scale modulations to be measured are rather small, at the few percent level, it is very important to carefully account for spurious effects that can modulate the ... See full document
26
Constraints on the origin of cosmic rays above $10^{18}$ eV from large scale anisotropy searches in data of the Pierre Auger Observatory
... While the turbulent component dominates in strength by a factor of a few, the regular component imprints dominant drift motions as soon as the Larmor radius of cosmic rays is larger than ... See full document
16
Measurement of the Proton-Air Cross Section at s√=57 TeV with the Pierre Auger Observatory
... range. The corresponding average center-of-mass energy of a proton interacting with a nucleon is 57 TeV, significantly above the reach of the Large Hadron ...to the cross section. Second, we ... See full document
9
Interpretation of the Depths of Maximum of Extensive Air Showers Measured by the Pierre Auger Observatory
... that the method provides an effective key to the interpretation of ...data. The energy dependences of hX max i and σ(X max ) are sometimes considered as different expressions of the same ... See full document
22
Upper limit on the diffuse flux of ultrahigh energy tau neutrinos from the pierre auger observatory
... of the Czech Republic; Centre de Calcul IN2P3/CNRS, Centre National de la Recherche Scientifique (CNRS), Conseil Re´gional Ile-de-France, De´partement Physique Nucle´aire et Corpusculaire (PNC-IN2P3/CNRS), ... See full document
7
Muons in air showers at the Pierre Auger Observatory: Mean number in highly inclined events
... and the Czech Science Founda- tion grant 14-17501S, Czech Republic; Centre de Cal- cul IN2P3/CNRS, Centre National de la Recherche Scientifique (CNRS), Conseil R´egional Ile-de-France, D´epartement Physique ... See full document
12
Testing Hadronic Interactions at Ultrahigh Energies with Air Showers Measured by the Pierre Auger Observatory
... PN-II-RU-PD-2011-3-0062, the Minister of National Education, Programme Space Tech- nology and Advanced Research (STAR), Grant ...and The Grainger Foun- dation, USA; NAFOSTED, Vietnam; Marie Curie- ... See full document
9
Improved limit to the diffuse flux of ultrahigh energy neutrinos from the Pierre Auger Observatory
... energy cosmic rays (UHECRs) above ∼ 5 × 10 19 eV is known to be suppressed with respect to that extrapolated from lower ...in the UHECR spectrum [1, 2], with the position of the break being ... See full document
14
Observation of inclined EeV air showers with the radio detector of the Pierre Auger Observatory
... – the Australian Research Council; Brazil – Conselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq); Finan- ciadora de Estudos e Projetos (FINEP); Fundação de Amparo à Pesquisa do Estado de Rio de ... See full document
20
Muons in air showers at the Pierre Auger Observatory: Measurement of atmospheric production depth
... within the Investissements d’Avenir Programme ANR- 11-IDEX-0004-02, French National Research Agency under grant ...2011-3-0062, the Minister of National Education, Programme for research - Space Technology ... See full document
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