about
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 eVSearch for slowly moving magnetic monopoles with the MACRO detectorCorrelation of the highest-energy cosmic rays with nearby extragalactic objects.Search for patterns by combining cosmic-ray energy and arrival directions at the Pierre Auger Observatory.Testing Hadronic Interactions at Ultrahigh Energies with Air Showers Measured by the Pierre Auger Observatory.Measurement of the Radiation Energy in the Radio Signal of Extensive Air Showers as a Universal Estimator of Cosmic-Ray Energy.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 ObservatoryAn evaluation of the exposure in nadir observation of the JEM-EUSO missionProperties and performance of the prototype instrument for the Pierre Auger ObservatoryAn upper limit to the photon fraction in cosmic rays above 1019eV from the Pierre Auger ObservatoryAnisotropy studies around the galactic centre at EeV energies with the Auger ObservatoryA search for point sources of EeV neutronsMeasurement 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 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 ObservatoryThe Atmospheric Monitoring System of the JEM-EUSO space missionErratum 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]Publisher’s Note: Search for ultrahigh energy neutrinos in highly inclined events at the Pierre Auger Observatory [Phys. Rev. D84, 122005 (2011)]GREX/COVER_PLASTEX: an experiment to analyze the space-time structure of extensive air showers produced by primary cosmic rays of 1015 eVMuons in air showers at the Pierre Auger Observatory: Mean number in highly inclined eventsAzimuthal asymmetry in the risetime of the surface detector signals of the Pierre Auger ObservatoryImproved limit to the diffuse flux of ultrahigh energy neutrinos from the Pierre Auger ObservatoryThe cosmic ray primary composition between 1015 and 1016 eV from Extensive Air Showers electromagnetic and TeV muon dataThe cosmic ray proton, helium and CNO fluxes in the 100 TeV energy region from TeV muons and EAS atmospheric Cherenkov light observations of MACRO and EAS-TOPStudy of the primary cosmic ray composition around the knee of the energy spectrum
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P50
description
researcher, ORCID id # 0000-0003-1427-9885
@en
wetenschapper
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name
Fausto Guarino
@ast
Fausto Guarino
@en
Fausto Guarino
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Fausto Guarino
@nl
type
label
Fausto Guarino
@ast
Fausto Guarino
@en
Fausto Guarino
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Fausto Guarino
@nl
altLabel
F. Guarino
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prefLabel
Fausto Guarino
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Fausto Guarino
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Fausto Guarino
@es
Fausto Guarino
@nl
P1053
I-3166-2012
P106
P1153
56351995500
P21
P31
P3829
P496
0000-0003-1427-9885