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Pierre Auger Observatory

Recent Ultra High Energy neutrino bounds and multimessenger observations with the Pierre Auger Observatory

Recent Ultra High Energy neutrino bounds and multimessenger observations with the Pierre Auger Observatory

... the Pierre Auger ...The Observatory is competitive in the search for neutrinos of all flavors above about 100 PeV by looking for very inclined showers produced deep in the atmosphere by neutri- nos ...

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Large scale anisotropy studies with the Pierre Auger Observatory

Large scale anisotropy studies with the Pierre Auger Observatory

... The Pierre Auger Observatory in Argentina mea- sures air showers initiated by cosmic rays at EeV energy scales (1 EeV = 10 18 ...the Pierre Auger Observatory since 1 January ...

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Studies of Cosmic Rays at the Highest Energies with the Pierre Auger Observatory

Studies of Cosmic Rays at the Highest Energies with the Pierre Auger Observatory

... Figure 5. Left: The black dots are 69 arrival directions of CRs with energy E ≥ 55 EeV detected by the Pierre Auger Observatory up to 31 December 2009 plotted in an Aitoff–Hammer projection of the sky ...

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Measurement of the muon content in air showers at the Pierre Auger Observatory

Measurement of the muon content in air showers at the Pierre Auger Observatory

... the Pierre Auger Observatory would not have been possible without the strong commitment and effort of all members of the Collaboration, and especially the technical and administrative staff in ...

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Results from the Pierre Auger Observatory

Results from the Pierre Auger Observatory

... The Pierre Auger Observatory was built to understand the nature and origin of the highest energy cosmic rays, ...existing observatory, covering an area of 3000 km 2 near the town of Malargüe ...

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Warped extra dimension and inclined events at Pierre Auger Observatory

Warped extra dimension and inclined events at Pierre Auger Observatory

... Recently, three neutrinos of energy 1-2 PeV, as well as tens of neutrinos above 10 TeV were de- tected with the IceCube experiment [1]. The cosmic neutrinos with energies near 1 EeV are detectable with the Surface ...

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Preliminary results of the AMIGA engineering array at the Pierre Auger Observatory

Preliminary results of the AMIGA engineering array at the Pierre Auger Observatory

... ing deployed (SD-433). Still, AMIGA’s main and novel contribution to the Pierre Auger Observatory is to provide direct muon measurements with dedicated underground muon detectors (UMD) made of ...

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Direct Measurement of the Muon Density in Air Showers with the Pierre Auger Observatory

Direct Measurement of the Muon Density in Air Showers with the Pierre Auger Observatory

... the Pierre Auger Observatory have led to major advances in our understanding of ultra-high en- ergy cosmic ...the Pierre Auger Observatory is currently being ...the Auger- ...

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Atmospheric monitoring and model applications at the Pierre Auger Observatory

Atmospheric monitoring and model applications at the Pierre Auger Observatory

... In the top left panel Fig. 3, a comparison in temperature versus height for a single profile is shown. Around 2 km above sea level, a temperature inversion is observed. This inversion is very well described by the GDAS ...

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The Pierre Auger Observatory status and the AugerPrime upgrade program

The Pierre Auger Observatory status and the AugerPrime upgrade program

... The Pierre Auger Observatory with its huge exposure provides us with a large set of high quality ...the Observatory has started a major upgrade, with an emphasis on improved mass composition ...

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The Pierre Auger Observatory: Review of Latest Results and Perspectives

The Pierre Auger Observatory: Review of Latest Results and Perspectives

... the Pierre Auger Observatory for a diffuse flux of neutrinos in the period 1 Jan 2004 - 31 March ...in Auger using hybrid events, the blue dashed boxes mark the systematic uncertainties of ...

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General overview of recent results from the Pierre Auger Observatory

General overview of recent results from the Pierre Auger Observatory

... The Pierre Auger Observatory was completed in 2008 and it is currently taking data. It is the first experiment in high energy cosmic ray physics using the powerful hybrid technique: joined use of ...

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The Pierre Auger Observatory: latest results and future perspectives

The Pierre Auger Observatory: latest results and future perspectives

... sources or during propagation through the Universe. Since neutrinos are chargeless particles they are not deflected by galactic and extra-galactic magnetic fields and then they are the best probe to point an UHECRs ...

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Measurements and tests of hadronic interactions at ultra-high energies with the Pierre Auger Observatory

Measurements and tests of hadronic interactions at ultra-high energies with the Pierre Auger Observatory

... the Pierre Auger Observatory show a composition which steadily becomes heavier with energy when interpreted with the latest available models ...

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Correlation between the UHECRs measured by the Pierre Auger Observatory and Telescope Array and neutrino candidate events from IceCube

Correlation between the UHECRs measured by the Pierre Auger Observatory and Telescope Array and neutrino candidate events from IceCube

... Figure 1. Map in Galactic coordinates showing the arrival directions of the IceCube cascades (black dots) and tracks (diamonds), as well as those of the UHECRs detected by the Pierre Auger ...

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A measurement of the muon number in showers using inclined events detected at the Pierre Auger Observatory

A measurement of the muon number in showers using inclined events detected at the Pierre Auger Observatory

... The Pierre Auger Observatory [1] is a hybrid cosmic ray air shower experiment that uses different techniques to detect extensive ...the Pierre Auger Observatory we have recorded ...

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Atmospheric aerosol attenuation effect on FD data analysis at the Pierre Auger Observatory

Atmospheric aerosol attenuation effect on FD data analysis at the Pierre Auger Observatory

... The Pierre Auger Observatory [1] is the largest hybrid detector for the study of UHECR: located in Argentina, it has operated since 2004 with 1660 water Cherenkov detectors (Surface Detector, SD) ...

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Search for a correlation between the UHECRs measured by the Pierre Auger Observatory and the Telescope Array and the neutrino candidate events from IceCube and ANTARES

Search for a correlation between the UHECRs measured by the Pierre Auger Observatory and the Telescope Array and the neutrino candidate events from IceCube and ANTARES

... Abstract. High-energy neutrinos are expected to be produced by the interaction of accelerated particles near the acceleration sites. For this reason, it is intresting to search for correlation in the arrival directions ...

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Average shape of longitudinal shower profiles measured at the Pierre Auger Observatory

Average shape of longitudinal shower profiles measured at the Pierre Auger Observatory

... The atmospheric e ff ects play an important role in the profile reconstruction and the Pierre Auger Observatory also has a large set of instruments dedicated to monitoring the atmospheric conditions ...

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Exploring cosmic rays at the highest-energy frontier with the Pierre Auger Observatory

Exploring cosmic rays at the highest-energy frontier with the Pierre Auger Observatory

... The latest spectrum reported by the Pierre Auger Observatory includes four data sets collected until the end of 2012 [9]. These data sets are combined to compose the spectrum shown in figure 1: hybrid ...

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