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View article: 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 Open
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 showers. These observations are compared to the data of the surface detector stations of the Observ…
View article: Measurement of the Radiation Energy in the Radio Signal of Extensive Air Showers as a Universal Estimator of Cosmic-Ray Energy
Measurement of the Radiation Energy in the Radio Signal of Extensive Air Showers as a Universal Estimator of Cosmic-Ray Energy Open
We measure the energy emitted by extensive air showers in the form of radio emission in the frequency range from 30 to 80 MHz. Exploiting the accurate energy scale of the Pierre Auger Observatory, we obtain a radiation energy of 15.8±0.7(s…
View article: The Pierre Auger Observatory: Contributions to the 34th International Cosmic Ray Conference (ICRC 2015)
The Pierre Auger Observatory: Contributions to the 34th International Cosmic Ray Conference (ICRC 2015) Open
One or more papers on each of the following topics are included in this volume: energy spectrum, arrival directions and anisotropies, composition, hadronic interactions, cosmology and geophysics, detectors, and outreach.
View article: Measurement of the cosmic ray spectrum above 4 × 10<sup>18</sup>eV using inclined events detected with the Pierre Auger Observatory
Measurement of the cosmic ray spectrum above 4 × 10<sup>18</sup>eV using inclined events detected with the Pierre Auger Observatory Open
A measurement of the cosmic-ray spectrum for energies exceeding\n$4{\\times}10^{18}$ eV is presented, which is based on the analysis of showers\nwith zenith angles greater than $60^{\\circ}$ detected with the Pierre Auger\nObservatory betw…
View article: Erratum: Muons in air showers at the Pierre Auger Observatory: Measurement of atmospheric production depth [Phys. Rev. D<b>90</b>, 012012 (2014)]
Erratum: Muons in air showers at the Pierre Auger Observatory: Measurement of atmospheric production depth [Phys. Rev. D<b>90</b>, 012012 (2014)] Open
\n Contains fulltext :\n 143727.pdf (Publisher’s version ) (Open Access)\n
View article: 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 Open
© Published by the American Physical Society 2015. Neutrinos in the cosmic ray flux with energies near 1 EeV and above are detectable with the Surface Detector array (SD) of the Pierre Auger Observatory. We report here on searches through …
View article: 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 Open
We analyze the distribution of arrival directions of ultra-high-energy cosmic rays recorded at the Pierre Auger Observatory in 10 years of operation. The data set, about three times larger than that used in earlier studies, includes arriva…
View article: LARGE SCALE DISTRIBUTION OF ULTRA HIGH ENERGY COSMIC RAYS DETECTED AT THE PIERRE AUGER OBSERVATORY WITH ZENITH ANGLES UP TO 80°
LARGE SCALE DISTRIBUTION OF ULTRA HIGH ENERGY COSMIC RAYS DETECTED AT THE PIERRE AUGER OBSERVATORY WITH ZENITH ANGLES UP TO 80° Open
We present the results of an analysis of the large angular scale distribution of the arrival directions of cosmic rays with energy above 4 EeV detected at the Pierre Auger Observatory including for the first time events with zenith angle b…
View article: Muons in air showers at the Pierre Auger Observatory: Mean number in highly inclined events
Muons in air showers at the Pierre Auger Observatory: Mean number in highly inclined events Open
We present the first hybrid measurement of the average muon number in air showers at ultrahigh energies, initiated by cosmic rays with zenith angles between 62° and 80°. The measurement is based on 174 hybrid events recorded simultaneously…
View article: ARCADE: Description of the project and setup of the Lidar/AMT system
ARCADE: Description of the project and setup of the Lidar/AMT system Open
\nThe ARCADE (Atmospheric Research for Climate and Astroparticle DEtection) project is a 3 years project funded by MIUR, that aims to study the aerosol attenuation of UV light in atmosphere using multiple instruments and techniques, as tho…