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[PDF] Top 20 Measurement of the Muon Content of EAS With the Pierre Auger Observatory

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Measurement of the Muon Content of EAS With the Pierre Auger Observatory

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). ... See full document

6

Ultrahigh Energy Neutrinos at the Pierre Auger Observatory

Ultrahigh Energy Neutrinos at the Pierre Auger Observatory

... consists of water Cherenkov detectors in the form of cylinders of ...tonnes of purified water. Charged particles entering the station emit Cherenkov light which is reflected at ... See full document

36

Measurement of the Cosmic Ray Spectrum above 4 $\times$ 10$^{18}$ eV Using Inclined Events Detected with the Pierre Auger Observatory

Measurement of the Cosmic Ray Spectrum above 4 $\times$ 10$^{18}$ eV Using Inclined Events Detected with the Pierre Auger Observatory

... φ) of the shower is obtained by fitting the start times of the signals recorded at the triggered stations to a plane front corrected for small time delays associated with ... See full document

25

Azimuthal Asymmetry in the Risetime of the Surface Detector Signals of the Pierre Auger Observatory

Azimuthal Asymmetry in the Risetime of the Surface Detector Signals of the Pierre Auger Observatory

... appreciate the origin of the asymmetries, we have to un- derstand the behavior of the copious number of muons and electromagnetic particles that reach the ...shower ... See full document

16

Particle physics measurements at the highest energies with the Pierre Auger Observatory

Particle physics measurements at the highest energies with the Pierre Auger Observatory

... and the SD can be used to extend the available beam energies even further, giving also independent measurements in the overlap ...region. Of special importance are the measurements ... See full document

7

High-energy interactions at the Pierre Auger Observatory

High-energy interactions at the Pierre Auger Observatory

... underline the complementarity of the information provided by the longitudinal profiles of the electromagnetic particles and the ...muons. The EM profile in a shower ... See full document

7

Energy Estimation of Cosmic Rays with the Engineering Radio Array of the Pierre Auger Observatory

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 the ... See full document

14

Muons in air showers at the Pierre Auger Observatory: Measurement of atmospheric production depth

Muons in air showers at the Pierre Auger Observatory: Measurement of atmospheric production depth

... an EAS develops in the atmosphere, the trans- verse momentum of secondary particles makes them deviate from the shower axis on their way to the ...Unlike the ... See full document

15

Measurement of the proton-air cross-section at $\sqrt{s}=57$ TeV with the Pierre Auger Observatory

Measurement of the proton-air cross-section at $\sqrt{s}=57$ TeV with the Pierre Auger Observatory

... representation of cosmic-ray data in all respects, these have been found to give reasonably good descriptions of many of the main ...that the differences be- tween the models used ... See full document

9

Limit on the diffuse flux of ultrahigh energy tau neutrinos with the surface detector of the Pierre Auger Observatory

Limit on the diffuse flux of ultrahigh energy tau neutrinos with the surface detector of the Pierre Auger Observatory

... level of uncertainty in EAS simu- lation because accelerator data have to be extrapolated to the shower energies under ...on the final result since the electromagnetic component ... See full document

15

Searches for Anisotropies in the Arrival Directions of the Highest Energy Cosmic Rays Detected by the Pierre Auger Observatory

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 ... See full document

38

Calibration of the logarithmic-periodic dipole antenna (LPDA) radio stations at the Pierre Auger Observatory using an octocopter

Calibration of the logarithmic-periodic dipole antenna (LPDA) radio stations at the Pierre Auger Observatory using an octocopter

... by the company TESEQ [ 40 ], is used as the signal ...MHz with a spacing of 5 ...for the measurement using the LPDA. The output signal injected into the ... See full document

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Testing Hadronic Interactions at Ultrahigh Energies with Air Showers Measured by the Pierre Auger Observatory

Testing Hadronic Interactions at Ultrahigh Energies with Air Showers Measured by the Pierre Auger Observatory

... to the corresponding muon excess detected in highly inclined air showers [7], as is expected because at high zenith angle the nonharonic contribution to the sig- nal (shown with red ... See full document

9

Impact of Atmospheric Effects on the Energy Reconstruction of Air Showers Observed by the Surface Detectors of the Pierre Auger Observatory

Impact of Atmospheric Effects on the Energy Reconstruction of Air Showers Observed by the Surface Detectors of the Pierre Auger Observatory

... correct the effects due to changes in the atmospheric variables that have an impact on the development of ...here the data from the two arrays of WCDs of the ... See full document

29

Bounds on the density of sources of ultra-high energy cosmic rays from the Pierre Auger Observatory

Bounds on the density of sources of ultra-high energy cosmic rays from the Pierre Auger Observatory

... patible with a transition from a light composition at 1 EeV to a heavier composition at 35 EeV, the highest energy for which results using this tech- nique have been reported [9, ...from the surface ... See full document

25

Improved limit to the diffuse flux of ultrahigh energy neutrinos from the Pierre Auger Observatory

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 [1, 2], with the ... See full document

14

Search for photons with energies above 10$^{18}$ eV using the hybrid detector of the Pierre Auger Observatory

Search for photons with energies above 10$^{18}$ eV using the hybrid detector of the Pierre Auger Observatory

... photons with energies above 1 EeV is performed using nine years of data collected by the Pierre Auger Observatory in hybrid operation ...measurements of the ... See full document

23

Constraints and measurements of hadronic interactions in extensive air showers with the Pierre Auger Observatory

Constraints and measurements of hadronic interactions in extensive air showers with the Pierre Auger Observatory

... is the main engine that drives the development of nuclei-induced ...80% of the particles produced in high energy collisions are pions, of which approximately 1/3 are neutral ... See full document

9

Spectral Calibration of the Fluorescence Telescopes of the Pierre Auger Observatory

Spectral Calibration of the Fluorescence Telescopes of the Pierre Auger Observatory

... energy of the primary cosmic ray is a key measurable for the science of the observatory, and the FD measurement of the energy, with lower ... See full document

33

Muon counting using silicon photomultipliers in the AMIGA detector of the Pierre Auger observatory

Muon counting using silicon photomultipliers in the AMIGA detector of the Pierre Auger observatory

... The Pierre Auger Obsevatory [ 1 ] is located in the province of Mendoza, Argentina and has an area of 3000 km 2 ...showers with a hybrid detection ...grid, with a ... See full document

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