[PDF] Top 20 Multi-messenger physics with the Pierre Auger Observatory
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Multi-messenger physics with the Pierre Auger Observatory
... The Pierre Auger Observatory is the largest and most precise detector of ultra-high energy air showers, such as those regularly induced by cosmic ...correlation with light ... See full document
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Azimuthal Asymmetry in the Risetime of the Surface Detector Signals of the Pierre Auger Observatory
... of the properties and origin of cosmic rays with energies greater than 1 Joule ...for the origin of these particles must account for the observations of their energy spectrum, arrival direc- ... See full document
16
Ultrahigh Energy Neutrinos at the Pierre Auger Observatory
... astroparticle physics. UHEνs can be detected with a variety of ...in the atmosphere (downward-going ν) or in the Earth crust (Earth-skimming ν), producing air showers that can be observed ... See full document
36
Reconstruction of inclined air showers detected with the Pierre Auger Observatory
... Argentina; the Australian Research Council; Conselho Nacional de Desenvolvimento Cient´ıfico e Tecnol´ ogico (CNPq), Finan- ciadora de Estudos e Projetos (FINEP), Funda¸c˜ ao de Amparo ` a Pesquisa do Estado de Rio ... See full document
33
A targeted search for point sources of EeV photons with the Pierre Auger Observatory
... within the Investissements d’Avenir Programme Grant ...Astroparticle Physics (HAP); Helmholtz-Gemeinschaft Deutscher Forschungszentren (HGF); Ministerium f¨ ur Innovation, Wissenschaft und Forschung des ... See full document
9
The Pierre Auger Observatory: review of latest results and perspectives
... of the most important questions in astrophysics: what are the sources of high energy cosmic rays (CRs); where are they produced; what are the corresponding acceleration mechanisms; and what is their ... See full document
13
A Targeted Search For Point Sources Of Eeev Photons With The Pierre Auger Observatory
... of the Pierre Auger Observatory would not have been possible without the strong commitment and effort from the technical and administrative staff in ...to the following ... See full document
7
Multi-resolution anisotropy studies of ultrahigh-energy cosmic rays detected at the Pierre Auger Observatory
... – the Australian Research Council; Brazil – Conselho Nacional de Desenvolvimento Cient´ıfico e Tecnol´ ogico (CNPq); Financiadora de Estudos e Projetos (FINEP); Funda¸c˜ ao de Amparo ` a Pesquisa do Estado de Rio ... See full document
27
Muon counting using silicon photomultipliers in the AMIGA detector of the Pierre Auger observatory
... for the Ground Array) is an upgrade of the Pierre Auger Observatory designed to extend its energy range of detection and to directly measure the muon content of the cosmic ... See full document
23
Muon detection with AMIGA at the Pierre Auger Observatory : Detecção de múons com o AMIGA no Observatório Pierre Auger
... rays, the mass composition is very well ...to the very low uxes. The mass estimation, in this case, is based on predictions from Monte Carlo simulations, which depend on hadronic interaction ...even ... See full document
119
Search for photons with energies above 10$^{18}$ eV using the hybrid detector of the Pierre Auger Observatory
... 0450696; The Grainger Foundation; Marie Curie-IRSES/EPLANET; European Particle Physics Latin American Network; European Union 7th Framework Pro- gram, Grant ... See full document
23
Observation of inclined EeV air showers with the radio detector of the Pierre Auger Observatory
... DGAPA-UNAM; The Netherlands – Ministry of Education, Culture and Science; Netherlands Organisation for Scientific Research (NWO); Dutch national e-infrastructure with the support of SURF Cooperative; ... See full document
20
Energy Estimation of Cosmic Rays with the Engineering Radio Array of the Pierre Auger Observatory
... of the Pierre Auger Observatory would not have been possible without the strong commitment and effort from the technical and administrative staff in ...to the following ... See full document
14
Testing Hadronic Interactions At Ultrahigh Energies With Air Showers Measured By The Pierre Auger Observatory
... Argentina; the Australian Research Council; Conselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq), Financiadora de Estudos e Projetos (FINEP), Fundação de Amparo à Pesquisa do Estado de Rio de ... See full document
10
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 ...of the particles produced in high energy collisions are pions, of which approximately 1/3 are neutral ...feeding the ... See full document
9
Data-driven estimation of the invisible energy of cosmic ray showers with the Pierre Auger Observatory
... within the Investissements d’Avenir Programme Grant ...Astroparticle Physics (HAP); Helmholtz-Gemeinschaft Deutscher Forschungszentren (HGF); Ministerium für Innovation, Wissenschaft und Forschung des ... See full document
19
Testing Hadronic Interactions at Ultrahigh Energies with Air Showers Measured by the Pierre Auger Observatory
... Argentina; the Aus- tralian Research Council; Conselho Nacional de De- senvolvimento Cient´ıfico e Tecnol´ ogico (CNPq), Fi- nanciadora de Estudos e Projetos (FINEP), Funda¸ c˜ ao de Amparo ` a Pesquisa do Estado ... See full document
9
Azimuthal asymmetry in the risetime of the surface detector signals of the Pierre Auger Observatory
... of the properties and origin of cosmic rays with energies greater than 1 Joule ( ...for the origin of these particles must account for the observations of their energy spectrum, arrival ... See full document
17
Search For Ultrarelativistic Magnetic Monopoles With The Pierre Auger Observatory
... of the greatest achievements of 19th century ...On the other hand, there are essential theoretical motivations for magnetic ...explain the quantization of electric charge, as first noted by Dirac [1] ... See full document
13
The Pierre Auger Cosmic Ray Observatory
... on the locally measured atmospheric profiles, monthly models of atmo- spheric conditions at the Pampa Amarilla were derived in December 2008 [78, ...79]. The monthly models are also compiled for ... See full document
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