[PDF] Top 20 The Pierre Auger Observatory: review of latest results and perspectives
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The Pierre Auger Observatory: review of latest results and perspectives
... on the ground by large arrays of surface detectors (SD), which sample their lateral distribution every certain distance ...for the Auger Observatory), and/or fluorescence ... See full document
13
Muon detection with AMIGA at the Pierre Auger Observatory : Detecção de múons com o AMIGA no Observatório Pierre Auger
... In the AMIGA proposal [75], the depth for the scintillator modules was estab- lished as ...months of data from the UC, it seems now that this value was overestimated and too much ... See full document
119
Search for ultrarelativistic magnetic monopoles with the Pierre Auger Observatory
... 6% of the UHECR proton showers of 10 ...cut, the fraction increasing to 32% for 10 ...on the penetration of the shower and its energy ...4(a) the correlation ... See full document
12
Search For Ultrarelativistic Magnetic Monopoles With The Pierre Auger Observatory
... ANALYSIS AND RESULTS The search for ultrarelativistic IMMs was performed following a blind ...procedure. The selection criteria described in ...simulations and a small fraction (10%) ... See full document
13
Results of a Self-Triggered Prototype System for Radio-Detection of Extensive Air Showers at the Pierre Auger Observatory
... to the following agencies and organizations for financial support: Comisi´ on Nacional de Energ´ıa At´ omica, Fundaci´ on Antorchas, Gobierno De La Provincia de Mendoza, Munici- palidad de Malarg¨ ue, NDM ... See full document
28
Combined fit of spectrum and composition data as measured by the Pierre Auger Observatory
... to the increased level of interactions that produce abundant secondary protons, whereas with m < 0 the goodness of fit is not affected much and a higher injection spectral index is ... See full document
40
A targeted search for point sources of EeV photons with the Pierre Auger Observatory
... discovery of photon fluxes from any target set or individual targets in this study would have proved that EeV protons are being accelerated at discrete sources within the Galaxy or its ...neighborhood. ... See full document
9
Azimuthal Asymmetry in the Risetime of the Surface Detector Signals of the Pierre Auger Observatory
... 11 of mass values (in terms of hln Ai) obtained from the measurements of (sec θ) max for the two distance ranges to previous mass estimates from the Pierre Auger ... See full document
16
Measurement of the average electromagnetic longitudinal shower profile at the Pierre Auger Observatory
... fit of data profiles to the Gaisser-Hillas function ( ...(right). The fitted function follows data points through the whole depth range used in this work, [−300, +200] g/cm 2 , with residuals ... See full document
8
Measurement of the Muon Content of EAS With the Pierre Auger Observatory
... present the results of three different classes of methods: 1) separating the muonic and electromagnetic signals based on their different time structures, 2) using inclined ... See full document
6
Constraints and measurements of hadronic interactions in extensive air showers with the Pierre Auger Observatory
... The Pierre Auger Observatory has unique capabilities to make measurements of the highest energy hadronic interactions and to constraint the models that attempt to ... See full document
9
Particle physics measurements at the highest energies with the Pierre Auger Observatory
... The Pierre Auger Observatory measures cosmic rays with energies between 10 ...eV and 10 20 eV, based on air shower sampling at ground, complemented with shower development measurements ... See full document
7
Muon counting using silicon photomultipliers in the AMIGA detector of the Pierre Auger observatory
... Muons and Infill for the Ground Array) is an upgrade of the Pierre Auger Observatory designed to extend its energy range of detection and to directly measure ... See full document
23
Depth of maximum of air-shower profiles at the Pierre Auger Observatory. II. Composition implications
... improves the fits for all hadronic interaction models. Results using EPOS-LHC in particular are satisfactory over most of the energy ...brings the models into remarkable agreement in ... See full document
13
Ultrahigh-Energy Neutrino Follow-Up of Gravitational Wave Events GW150914 and GW151226 with the Pierre Auger Observatory
... use the same identification criteria as in [21] to search for neutrinos in temporal and spa- tial coincidence with GW150914 and GW151226, as well as with the GW candidate event LVT151012 ... See full document
10
Search for patterns by combining cosmic-ray energy and arrival directions at the Pierre Auger Observatory
... with the energy, and an isotropic background fraction. The values of Ωi j can be positive or negative depending on the cosmic-ray pair having energies above or below the average ... See full document
16
Bounds on the density of sources of ultra-high energy cosmic rays from the Pierre Auger Observatory
... in the data can be used to establish a lower bound on the density of sources (the same happens also in the case of the 60 and 80 EeV energy ...estimator the ... See full document
25
Azimuthal asymmetry in the risetime of the surface detector signals of the Pierre Auger Observatory
... tainties and are sensitive to very different types of hadronic interactions since the importance of the muonic shower component is different within each of ...In the ... See full document
17
Highlights from the Pierre Auger Observatory
... At the low energy end (between 0.01 and 1 EeV) we have the HEAT and AMIGA ...modified the local trigger conditions of the surface array detectors to lower our full trigger ... See full document
9
Hadronic physics with the Pierre Auger Observatory
... how the Pierre Auger Observatory is able to measure the proton-air cross section for particle produc- tion at a center-of-mass energy per nucleon of 39 TeV and 56 ... See full document
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