[PDF] Top 20 Large-scale distribution of arrival directions of cosmic rays detected above 1018 ev at the pierre auger observatory
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Large-scale distribution of arrival directions of cosmic rays detected above 1018 ev at the pierre auger observatory
... to the following agencies and or- ganizations for financial support: Comisi´on Nacional de Energ´ıa At´omica, Fundaci´on Antorchas, Gobierno De La Provincia de Mendoza, Municipalidad de Malarg¨ue, NDM ... 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
... for large scale anisotropies in the distribution of arrival directions of cosmic rays detected above 10 18 eV at ... See full document
16
Multi-resolution anisotropy studies of ultrahigh-energy cosmic rays detected at the Pierre Auger Observatory
... scenarios of UHECR origin ...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 ... See full document
27
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 ... See full document
16
Search for patterns by combining cosmic-ray energy and arrival directions at the Pierre Auger Observatory
... energies above 60 EeV (1 EeV = 10 18 eV) with the distribu- tion of nearby extragalactic matter [8, ...update of the analysis yielded a correlation strength which is reduced com- ... See full document
16
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
... fraction of the extragalactic neutrinos, those from sources relatively nearby, may have the same sources as the observed ...that the neutrino sources extend to at least z=1, ... 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
... The arrival direction (θ, φ) of the shower is obtained by fitting the start times of the signals recorded at the triggered stations to a plane front ... See full document
25
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 an- ode and from ... See full document
16
Results of a Self-Triggered Prototype System for Radio-Detection of Extensive Air Showers at the Pierre Auger Observatory
... The distribution of the arrival directions of cosmic rays, recorded by a radio-detection setup, can be described fairly well using a simple geomagnetic ... See full document
28
Depth of maximum of air-shower profiles at the Pierre Auger Observatory. I. Measurements at energies above $10^{17.8}$ eV
... telescopes. The inference of X max from only the rising or falling edge of the profile would introduce a large depen- dency of the results on the functional ... See full document
25
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. ... See full document
22
Large Scale Distribution of Ultra High Energy Cosmic Rays Detected at the Pierre Auger Observatory With Zenith Angles up to 80°
... regions of the sky, such as the vertical and inclined samples considered here, a small difference in the energy cross- calibration of the samples could give rise to a difference ... See full document
26
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 ... 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
33
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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Depth of maximum of air-shower profiles at the Pierre Auger Observatory. II. Composition implications
... Argentina; the Australian Research Council; 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 de ... See full document
13
Particle physics measurements at the highest energies with the Pierre Auger Observatory
... The Pierre Auger Observatory measures cosmic rays with energies between 10 ...17.5 eV and 10 20 eV, based on air shower sampling at ground, complemented with ... See full document
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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
27
Measurement of the Muon Content of EAS With the Pierre Auger Observatory
... From the 12, only the 3 simulated showers that best matched the real LP were considered for full simulation and posterior data ...On the bottom is the ground signal for the same ... See full document
6
Hadronic physics with the Pierre Auger Observatory
... depth at which the number of charged particles reaches its maximum in the air shower, X max , is sensi- tive to the mass composition of the primaries through the ... See full document
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