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Description of atmospheric conditions at the Pierre Auger Observatory using the Global Data Assimilation System (GDAS)Search for signatures of magnetically-induced alignment in the arrival directions measured by the Pierre Auger ObservatoryThe Lateral Trigger Probability function for the Ultra-High Energy Cosmic Ray showers detected by the Pierre Auger ObservatoryUpper limit on the cosmic-ray photon fraction at EeV energies from the Pierre Auger ObservatoryThe fluorescence detector of the Pierre Auger ObservatoryObservation of the Suppression of the Flux of Cosmic Rays above 4 × 10 19 eVRelic neutrino decoupling including flavour oscillationsCorrelation of the highest-energy cosmic rays with nearby extragalactic objects.Relic density of neutrinos with primordial asymmetries.Correlation of the highest-energy cosmic rays with the positions of nearby active galactic nucleiMeasurement of the energy spectrum of cosmic rays above 1018 eV using the Pierre Auger ObservatoryA White Paper on keV sterile neutrino Dark MatterConstraining the window on sterile neutrinos as warm dark matterA targeted search for point sources of EeV neutronsA search for point sources of EeV photonsUltrahigh Energy Neutrinos at the Pierre Auger ObservatoryConstraints on the origin of cosmic rays above 10^18^ eV from large-scale anisotropy searches in data of the pierre auger observatoryA search for point sources of EeV neutronsAntennas for the detection of radio emission pulses from cosmic-ray induced air showers at the Pierre Auger ObservatoryMeasurement of the Proton-Air Cross Section ats=57 TeVwith the Pierre Auger ObservatoryA search for anisotropy in the arrival directions of ultra high energy cosmic rays recorded at the Pierre Auger ObservatoryLarge-scale distribution of arrival directions of cosmic rays detected above 10^18^ eV at the Pierre Auger observatorySearch for point-like sources of ultra-high energy neutrinos at the pierre auger observatory and improved limit on the diffuse flux of Tau neutrinosSearch for ultrahigh energy neutrinos in highly inclined events at the Pierre Auger ObservatoryThe exposure of the hybrid detector of the Pierre Auger ObservatorySearch for first harmonic modulation in the right ascension distribution of cosmic rays detected at the Pierre Auger ObservatoryAdvanced functionality for radio analysis in the Offline software framework of the Pierre Auger ObservatoryMeasurement of the Depth of Maximum of Extensive Air Showers above1018 eVTrigger and aperture of the surface detector array of the Pierre Auger ObservatoryAtmospheric effects on extensive air showers observed with the surface detector of the Pierre Auger observatoryLimit on the diffuse flux of ultrahigh energy tau neutrinos with the surface detector of the Pierre Auger ObservatoryUpper limit on the cosmic-ray photon flux above 1019eV using the surface detector of the Pierre Auger ObservatoryUpper Limit on the Diffuse Flux of Ultrahigh Energy Tau Neutrinos from the Pierre Auger ObservatoryDisentangling neutrino-nucleon cross section and high energy neutrino flux with akm3neutrino telescopeRole of dense matter in collective supernova neutrino transformationsUltrahigh energy neutrinos in the Mediterranean: detecting ντ and νμ with a km3 telescopeEffects of non-standard neutrino–electron interactions on relic neutrino decouplingErratum to “The Lateral Trigger Probability function for the Ultra-High Energy Cosmic Ray Showers detected by the Pierre Auger Observatory” [Astroparticle Physics 35 (2011) 266–276]Muons in air showers at the Pierre Auger Observatory: Measurement of atmospheric production depthOrigin of atmospheric aerosols at the Pierre Auger Observatory using studies of air mass trajectories in South America
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S. Pastor
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S. Pastor
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Sergio Pastor
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Sergio Pastor
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Sergio Pastor
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Sergio Pastor
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S. Pastor
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S. Pastor
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Sergio Pastor
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Sergio Pastor
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Sergio Pastor
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