[PDF] Top 20 Data-driven estimation of the invisible energy of cosmic ray showers with the Pierre Auger Observatory
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Data-driven estimation of the invisible energy of cosmic ray showers with the Pierre Auger Observatory
... within the Investissements d’Avenir Programme Grant ...Center of Excellence; Ministero degli Affari Esteri (MAE); M´exico – Consejo Nacional de Ciencia y Tecnología (CONACYT) ...DGAPA-UNAM; The ... 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
... four of the closest stations to the one with the highest signal are operational at the time of the ...that the reconstructed shower core be contained within ... 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
... The Pierre Auger Observatory is the largest extensive air shower detector, covering 3000 km 2 in ...Argentina. The Observatory makes available, for educational and ... See full document
5
Interpretation of the Depths of Maximum of Extensive Air Showers Measured by the Pierre Auger Observatory
... discuss the different roles of the two observables, hX max i and σ(X max ), with respect to mass ...In the interpretation of data they are often used as different, and ... See full document
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Impact of Atmospheric Effects on the Energy Reconstruction of Air Showers Observed by the Surface Detectors of the Pierre Auger Observatory
... Variation of the atmospheric conditions affect the signals from the extended air shower (EAS) which can be detected at ground level with arrays of surface detectors, such as ... 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 from sources ... See full document
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Large-scale cosmic-ray anisotropies above 4 EeV measured by the Pierre Auger observatory
... in the distribution of CR observed in the studies performed above 4 EeV is the large- scale dipolar modulation of the flux at energies above ...8EeV. The maximum ... See full document
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Constraints and measurements of hadronic interactions in extensive air showers with the Pierre Auger Observatory
... center of mass energy above those attained at the LHC are continuously happening in the upper layers of the Earth’s ...high energy cosmic rays (UHECR) collide ... See full document
9
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 ... 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 Pierre Auger Observatory is to date the largest detector of air showers induced by the ultra-high energy cosmic rays ...array of surface ... See full document
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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, while present ... See full document
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Search for patterns by combining cosmic-ray energy and arrival directions at the Pierre Auger Observatory
... Abstract Energy-dependent patterns in the arrival direc- tions of cosmic rays are searched for using data of the Pierre Auger ...around 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
... Observations of cosmic ray arrival directions made with the Pierre Auger Obser- vatory have previously provided evidence of anisotropy at the 99% CL using ... See full document
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Muons in air showers at the Pierre Auger Observatory: Measurement of atmospheric production depth
... However, the bulk of events collected by the obser- vatory have information only from the surface array, making SD observables, such as the one described in this work, very valuable for ... See full document
15
Multi-messenger physics with the Pierre Auger Observatory
... parameters, with standard software such as AIRES Sciutto (1999) and CORSIKA Heck et ...including the SD response of the individual detector stations using specific software ( Argiro et ...for ... See full document
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Measurement of the Radiation Energy in the Radio Signal of Extensive Air Showers as a Universal Estimator of Cosmic-Ray Energy
... quantified the difference be- tween radio amplitudes at the characteristic lateral dis- tance measured for the same showers at sea level (altitude of LOFAR [ 19 ]) and at 1560 m above ... See full document
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Limit on the diffuse flux of ultrahigh energy tau neutrinos with the surface detector of the Pierre Auger Observatory
... identification of showers induced by Earth- skimming neutrinos implies searching for very inclined (quasihorizontal) showers in an early stage of develop- ...as the electromagnetic ... See full document
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Results of a Self-Triggered Prototype System for Radio-Detection of Extensive Air Showers at the Pierre Auger Observatory
... origin of cosmic rays at ultra high energies (E > ...question of astroparticle physics. The induced shower of secondary particles in the atmosphere of the Earth ... See full document
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Search For Ultrarelativistic Magnetic Monopoles With The Pierre Auger Observatory
... below the Parker bound [15] of ∼10 −15 ðcm 2 sr sÞ −1 , which represents the largest possible magnetic-monopole flux consistent with survival of the galactic magnetic ...However, ... See full document
13
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 ... See full document
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