[PDF] Top 20 Multi-resolution anisotropy studies of ultrahigh-energy cosmic rays detected at the Pierre Auger Observatory
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Multi-resolution anisotropy studies of ultrahigh-energy cosmic rays detected at the Pierre Auger Observatory
... Department of Energy, Contracts ...0450696; The Grainger Foundation; Marie Curie-IRSES/EPLANET; European Particle Physics Latin American Network; European Union 7th Framework Program, Grant ... See full document
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Searches for Large-Scale Anisotropy in the Arrival Directions of Cosmic Rays Detected above Energy of $10^{19}$ eV at the Pierre Auger Observatory and the Telescope Array
... evaluating the amplitude of the first harmonics for fictitious right ascension angles calculated by dilating the time of the events in a way that a solar day lasts about four ... See full document
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Large-scale distribution of arrival directions of cosmic rays detected above 1018 ev at the pierre auger observatory
... that the cosmic-ray composition includes a significant light component from various measurements of the depth of shower maximum X max (The Pierre Auger ... See full document
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Large Scale Distribution of Ultra High Energy Cosmic Rays Detected at the Pierre Auger Observatory With Zenith Angles up to 80°
... restrict the analysis to the first two harmonics k = 1, 2. The first harmonic coeffi- cients in right ascension and azimuth are enough to reconstruct the dipole in the hypothesis that ... 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
... by the Japan Society for the Promotion of Science through Grants-in-Aid for Scientific Research on Specially Promoted Research (21000002) “Extreme Phenomena in the Universe Explored by Highest ... See full document
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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 ... See full document
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Ultrahigh-Energy Neutrino Follow-Up of Gravitational Wave Events GW150914 and GW151226 with the Pierre Auger Observatory
... With the surface detector (SD) of the Pierre Auger Ob- servatory [20] we can identify neutrino-induced air show- ers in the energy range above 100 PeV ...neutrinos ... See full document
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Ultrahigh Energy Neutrinos at the Pierre Auger Observatory
... High energy neutrinos can be detected with a variety of techniques [13, ...arrays of detectors at ground level that are currently being used to measure extensive showers produced 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
... tion of arrival directions have been made with UHECR ...set the Pierre Auger Collaboration reported evidence of anisotropy with a confidence level of 99% in the ... 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
... use of mock data sets built from the large scale structure of the Universe provides a useful tool to study the sensitivity of the three ...methods. The toy model we ... See full document
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Origin of atmospheric aerosols at the Pierre Auger Observatory using studies of air mass trajectories in South America
... direction of air masses for clear, average and hazy aerosol conditions are presented in Figure 9 (bottom) for two different start altitudes at the location of the obser- vatory: 500 m ... See full document
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Particle physics measurements at the highest energies with the Pierre Auger Observatory
... in the interaction of hadronic primaries with the CMB. The corresponding fluxes at Earth are expected to be small, but the sen- sitivity of Auger will soon reach ... See full document
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Measurement of the Cosmic Ray Spectrum above 4 $\times$ 10$^{18}$ eV Using Inclined Events Detected with the Pierre Auger Observatory
... choice of deep-water Cherenkov detectors for the Pierre Auger Observatory was made to give substantial solid angle coverage for zenith angles exceeding 60 ◦ thus enabling detection ... See full document
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Spectral Calibration of the Fluorescence Telescopes of the Pierre Auger Observatory
... The energy of the primary cosmic ray is a key measurable for the science of the observatory, and the FD measurement of the ... See full document
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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 ...Center of Excellence, Italy; Consejo Nacional de Ciencia y Tecnolog´ıa (CONACYT), Mexico; ... See full document
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Hadronic physics with the Pierre Auger Observatory
... how the Pierre Auger Observatory is able to measure the proton-air cross section for particle produc- tion at a center-of-mass energy per nucleon of 39 TeV ... See full document
8
Large-scale cosmic-ray anisotropies above 4 EeV measured by the Pierre Auger Observatory
... ( The Pierre Auger Collaboration 2017b ), since, otherwise, systematic modulations of the rates as a function of the hour of the day or of the ... See full document
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Measurement of the average electromagnetic longitudinal shower profile at the Pierre Auger Observatory
... The Pierre Auger Observatory is a hybrid detector, consisting of a 3000 km 2 Surface Detector array (SD) overlooked by the Fluorescence Detector ...(FD). The FD consists ... See full document
8
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
Prototype muon detectors for the AMIGA component of the Pierre Auger Observatory
... Center of Excellence, Ministero degli Affari Esteri (MAE), Italy; Consejo Nacional de Ciencia y Tecnología (CONACYT), Mexico; Ministerie van Onderwijs, Cul- tuur en Wetenschap, Nederlandse Organisatie voor ... See full document
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