[PDF] Top 20 Bounds on the density of sources of ultra-high energy cosmic rays from the Pierre Auger Observatory
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Bounds on the density of sources of ultra-high energy cosmic rays from the Pierre Auger Observatory
... that the propagation of particles was performed under the assump- tion that UHECRs are ...matter of fact, the propagation for iron nuclei and its secondaries, mainly determined by ... See full document
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Searches for Anisotropies in the Arrival Directions of the Highest Energy Cosmic Rays Detected by the Pierre Auger Observatory
... In the later sections we analyze the distribution of the arrival ...update the fraction of events correlating with AGNs in the VCV ...spite of the large data ... See full document
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Interpretation of the Depths of Maximum of Extensive Air Showers Measured by the Pierre Auger Observatory
... for the study of the composition of Ultra High Energy Cosmic Rays (UHECR) are the mean value of the depth of shower maximum, hX ... See full document
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Search for patterns by combining cosmic-ray energy and arrival directions at the Pierre Auger Observatory
... mic rays with energies above E = 5 × 10 18 eV arriving within an angular separation of approximately ...characterize the energy distributions inside these regions by two inde- pendent methods, ... See full document
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Upper limit on the diffuse flux of ultrahigh energy tau neutrinos from the pierre auger observatory
... detection of ultrahigh energy (UHE) cosmic neu- trinos at EeV (1 EeV 10 18 eV) energies and above is a long-standing experimental ...to the universe [ 4 ], and provide an unique opportunity ... See full document
7
High-energy interactions at the Pierre Auger Observatory
... interaction of Ultra High Energy Cosmic Rays (UHECRs) with the atoms of the atmosphere can occur at center-of-mass energies that surpass 100 TeV, ... See full document
7
An Indication of anisotropy in arrival directions of ultra-high-energy cosmic rays through comparison to the flux pattern of extragalactic gamma-ray sources
... analysis of the dataset from the Pierre Auger Observatory provides evidence for anisotropy in the arrival directions of ... See full document
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Highlights from the Pierre Auger Observatory
... information of our spectrum measurement, it is possible that the cut-off region represents more a consequence of the source maximal acceleration energy (of the order ... See full document
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Search for correlations between the arrival directions of IceCube neutrino events and ultrahigh-energy cosmic rays detected by the Pierre Auger Observatory and the Telescope Array
... calculate the pre-trial p-values. To evaluate the sensitivity and discovery potential of this method we perform the same simulation of cosmic-ray signal events as in Section ... See full document
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Large-scale cosmic-ray anisotropies above 4 EeV measured by the Pierre Auger Observatory
... examples of the large-scale anisotropies expected from a Galactic CR component, we show in ...5 the direction of the dipole that would result for cosmic rays coming ... See full document
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Search for point-like sources of ultra-high energy neutrinos at the Pierre Auger Observatory and improved limit on the diffuse flux of tau neutrinos
... Although the primary goal of the SD is to detect UHECRs, it can also identify ultra-high energy ...Neutrinos of all flavours can interact at any atmospheric depth through ... See full document
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Improved limit to the diffuse flux of ultrahigh energy neutrinos from the Pierre Auger Observatory
... flux of ultra-high 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 ... See full document
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Search for point-like sources of ultra-high energy neutrinos at the Pierre auger observatory and improved limit on the diffuse flux of tau neutrinos
... Although the primary goal of the SD is to detect UHECRs, it can also identify UHE ...Neutrinos of all flavors can interact at any atmospheric depth through charged or neutral currents and ... See full document
7
Constraints on the origin of cosmic rays above $10^{18}$ eV from large scale anisotropy searches in data of the Pierre Auger Observatory
... in the distribution of arrival directions of cosmic rays detected above 10 18 eV at the Pierre Auger Observatory is ...For the first time, these large ... See full document
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Search for High-energy Neutrinos from Binary Neutron Star Merger GW170817 with ANTARES, IceCube, and the Pierre Auger Observatory
... 2017, the Advanced LIGO ( Aasi et ...GW170817, from a bi- nary neutron star inspiral ( Abbott et ...GRB170817A, from a consistent location ( Gold- stein et ...Subsequently, ultra-violet, ... See full document
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The Pierre Auger Cosmic Ray Observatory
... High-energy cosmic ray air showers generate radio emission via two processes: one is a geomagnetic, current-induced emission mechanism [152]; the other is a charge- excess mechanism ...[153]. ... See full document
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A search for anisotropy in the arrival directions of ultra high energy cosmic rays recorded at the Pierre Auger Observatory
... Ministry of Science and Higher Education, Grant ...Innovaci´ on and Consolider-Ingenio 2010 (CPAN), Xunta de Galicia, Spain; Science and Technology Facilities Council, United Kingdom; Department of ... See full document
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Azimuthal Asymmetry in the Risetime of the Surface Detector Signals of the Pierre Auger Observatory
... components of extensive air showers with a duty cycle of nearly ...liters of ultra-pure water. The water volume is viewed by three 9” photomultiplier tubes ...(from the ... See full document
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Measurement of the Muon Content of EAS With the Pierre Auger Observatory
... The Pierre Auger Observatory is a hybrid detector with the aim of studying the characteristics of the longitudinal and lateral profiles of extensive ... See full document
6
Energy Estimation of Cosmic Rays with the Engineering Radio Array of the Pierre Auger Observatory
... 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 ...to ... See full document
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