[PDF] Top 20 Large-scale cosmic-ray anisotropies above 4 EeV measured by the Pierre Auger Observatory
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Large-scale cosmic-ray anisotropies above 4 EeV measured by the Pierre Auger Observatory
... – the Australian Research Council; Brazil – Conselho Nacional de Desenvolvimento Cient´ıfico e Tecnol´ ogico (CNPq); Financiadora de Estudos e Projetos (FINEP); Funda¸c˜ ao de Amparo `a Pesquisa do Estado de Rio ... 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
... section 4. In addition, although the techniques for assigning energies to events are nearly the same, there are differences as to how the primary energies are derived at the Telescope ... 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 flux of UHECRs at energies above 40 EeV has been established experimentally beyond any doubt (Abbasi et ...2013). The energy at which the spectrum steepens is in accordance with ... See full document
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Search for patterns by combining cosmic-ray energy and arrival directions at the Pierre Auger Observatory
... estimate the uncertainty on the measurement, we repeatedly vary the energy and arrival directions of all events detected with the Pierre Auger Observatory above E = ... 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
... 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 ... See full document
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Observation of inclined EeV air showers with the radio detector of the Pierre Auger Observatory
... For the subset of 50 events with a surface-detector reconstruction of the cosmic-ray energy, we have made a direct comparison with the associated ...compare the sim- ulated pulse ... 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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Multi-resolution anisotropy studies of ultrahigh-energy cosmic rays detected at the Pierre Auger Observatory
... type anisotropies are also expected in the case of an excess along a plane such as the Galactic or super-galactic planes, which are plausible source regions at high ...Although the actual ... 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
... from the large scale structure of the Universe provides a useful tool to study the sensitivity of the three ...methods. The toy model we choose here allows us to probe ... 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
... on the rigidity E/Z of the cosmic rays, with Z the electric charge of the ...illustrate the upper limits, we consider two extreme single primaries: protons and iron ...In ... 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
... for the Pierre Auger Observatory was made to give substantial solid angle coverage for zenith angles exceeding 60 ◦ thus enabling detection of showers over a much broader angular and ... See full document
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Questions and Answers in Extreme Energy Cosmic Rays – a guide to explore the data set of the Pierre Auger Observatory
... Cosmic ray showering, the way these particle cas- cades develop by interaction in the Earth’s atmosphere, is then briefly ...it, the basics of particle physics (presently not ... See full document
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Identifying Clouds over the Pierre Auger Observatory using Infrared Satellite Data
... test the efficacy of the algorithms for cloud identification by checking the cloudy/clear state of the pixel encompassing the CLF (CLF ...while the FD operates, the ... See full document
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Reconstruction of inclined air showers detected with the Pierre Auger Observatory
... Argentina; the Australian Research Council; Conselho Nacional de Desenvolvimento Cient´ıfico e Tecnol´ ogico (CNPq), Finan- ciadora de Estudos e Projetos (FINEP), Funda¸c˜ ao de Amparo ` a Pesquisa do Estado de Rio ... 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
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Measurement of the Muon Content of EAS With the Pierre Auger Observatory
... component: the signal amplitude and the time-of- arrival distribution. The energy deposition in WCD for muons (≈ 240 MeV) is much higher than for electrons and photons (≈ 10 ...MeV). The ... See full document
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Azimuthal Asymmetry in the Risetime of the Surface Detector Signals of the Pierre Auger Observatory
... conclude by making a comparison in ...from the measurements of (sec θ) max for the two distance ranges to previous mass estimates from the Pierre Auger Observatory [5, ... See full document
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Spectral Calibration of the Fluorescence Telescopes of the Pierre Auger Observatory
... Regarding the spectral calibration, what has to be evaluated is the change in the spectral response of a given FD telescope, ...i.e. the shape of the response curve vs ...at the ... See full document
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Search for photons with energies above 10$^{18}$ eV using the hybrid detector of the Pierre Auger Observatory
... and the possible misalignment of the telescopes which can affect the geometry ...reconstruction. The latter is periodically tested using lasers and time periods having misaligned mirrors are ... See full document
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Prototype muon detectors for the AMIGA component of the Pierre Auger Observatory
... PN-II-RU-PD-2011-3-0062, the Minister of National Education, Programme Space Technology and Advanced Research (STAR), Grant ...0450696, The Grainger Foundation, USA; NAFOSTED, Vietnam; Marie ... See full document
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