C. Di Giulio
8 ta ish
University of Rome Tor Vergata
Measurement of the cosmic-ray energy spectrum above<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mn>2.5</mml:mn><mml:mo>×</mml:mo><mml:msup><mml:mn>10</mml:mn><mml:mn>18</mml:mn></mml:msup><mml:mtext> </mml:mtext><mml:mtext> </mml:mtext><mml:mi>eV</mml:mi></mml:math>using the Pierre Auger Observatory
A. Aab, P. Abreu, M. Aglietta +97
MaqolaOchiq kirish202010 iqtibosABICombined fit of spectrum and composition data as measured by the Pierre Auger Observatory
A. Aab, P. Abreu, M. Aglietta +97
MaqolaOchiq kirish20178 iqtibosABIObservation of a large-scale anisotropy in the arrival directions of cosmic rays above 8 × 10 <sup>18</sup> eV
A. Aab, P. Abreu, M. Aglietta +97
MaqolaOchiq kirish20176 iqtibosABIMuons in air showers at the Pierre Auger Observatory: Mean number in highly inclined events
A. Aab, P. Abreu, M. Aglietta +97
MaqolaOchiq kirish20156 iqtibosABITesting Hadronic Interactions at Ultrahigh Energies with Air Showers Measured by the Pierre Auger Observatory
A. Aab, P. Abreu, M. Aglietta +97
MaqolaOchiq kirish20166 iqtibosABIFeatures of the Energy Spectrum of Cosmic Rays above <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mn>2.5</mml:mn><mml:mo>×</mml:mo><mml:msup><mml:mn>10</mml:mn><mml:mn>18</mml:mn></mml:msup><mml:mtext> </mml:mtext><mml:mtext> </mml:mtext><mml:mi>eV</mml:mi></mml:math> Using the Pierre Auger Observatory
A. Aab, P. Abreu, M. Aglietta +97
MaqolaOchiq kirish20205 iqtibosABIMuons in air showers at the Pierre Auger Observatory: Measurement of atmospheric production depth
A. Aab, P. Abreu, M. Aglietta +96
MaqolaOchiq kirish20144 iqtibosABIImpact of atmospheric effects on the energy reconstruction of air showers observed by the surface detectors of the Pierre Auger Observatory
A. Aab, P. Abreu, M. Aglietta +97
MaqolaOchiq kirish20173 iqtibosABI