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57 works

Work: Inference of the Mass Composition of Cosmic Rays with Energies from <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:msup><mml:mn>10</mml:mn><mml:mn>18.5</mml:mn></mml:msup></mml:math> to <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:msup><mml:mrow><mml:mn>10</mml:mn></mml:mrow><mml:mrow><mml:mn>20</mml:mn></mml:mrow></mml:msup><mml:mtext> </mml:mtext><mml:mtext> </mml:mtext><mml:mi>eV</mml:mi></mml:mrow></mml:math> Using the Pierre Auger Observatory and Deep Learning

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  3. End to the Cosmic-Ray Spectrum?

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  4. The Pierre Auger Cosmic Ray Observatory

    Aab, A., Abreu, P., Aglietta, M. +30

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  5. EPOS LHC: Test of collective hadronization with data measured at the CERN Large Hadron Collider

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  6. Depth of maximum of air-shower profiles at the Pierre Auger Observatory. I. Measurements at energies above<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mn>1</mml:mn><mml:msup><mml:mrow><mml:mn>0</mml:mn></mml:mrow><mml:mrow><mml:mn>17.8</mml:mn></mml:mrow></mml:msup><mml:mtext>  </mml:mtext><mml:mi>eV</mml:mi></mml:mrow></mml:math>

    A. Aab, P. Abreu, M. Aglietta +97

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  7. Constraining the sources of ultra-high-energy cosmic rays across and above the ankle with the spectrum and composition data measured at the Pierre Auger Observatory

    A. Abdul Halim, P. Abreu, M. Aglietta +97

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  8. Mass Composition of Cosmic Rays with Energies above 10$^{17.2}$ eV from the Hybrid Data of the Pierre Auger Observatory

    Alexey Yushkov

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  9. Hadronic interaction model sibyll 2.3d and extensive air showers

    Felix Riehn, R. Engel, Anatoli Fedynitch +2

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  10. Reconstruction of events recorded with the surface detector of the Pierre Auger Observatory

    A. Aab, P. Abreu, M. Aglietta +97

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  11. The energy spectrum of cosmic rays beyond the turn-down around $$\varvec{10^{17}}$$ eV as measured with the surface detector of the Pierre Auger Observatory

    P. Abreu, M. Aglietta, Justin M. Albury +97

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  12. Constraining the sources of ultra-high-energy cosmic rays across and above the ankle with the spectrum and composition data measured at the Pierre Auger Observatory

    Pierre Auger Collaboration

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  13. Combined fit of spectrum and composition data as measured by the Pierre Auger Observatory

    A. Aab, P. Abreu, M. Aglietta +97

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  14. Depth of maximum of air-shower profiles at the Pierre Auger Observatory. II. Composition implications

    A. Aab, P. Abreu, M. Aglietta +97

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  15. Testing Hadronic Interactions at Ultrahigh Energies with Air Showers Measured by the Pierre Auger Observatory

    A. Aab, P. Abreu, M. Aglietta +97

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  16. A generalized description of the time dependent signals in extensive air shower detectors and its applications

    M. Ave, M. Roth, A. Schulz

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  17. AugerPrime: the Pierre Auger Observatory Upgrade

    Antonella Castellina

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  18. Reconstruction of Events Recorded with the Surface Detector of the Pierre Auger Observatory

    A. Aab, P. Abreu, M. Aglietta +97

    Article20204 citations
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  19. Measurement of the Fluctuations in the Number of Muons in Extensive Air Showers with the Pierre Auger Observatory

    A. Aab, P. Abreu, M. Aglietta +97

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  20. Observation of the Suppression of the Flux of Cosmic Rays above<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mn>4</mml:mn><mml:mo>×</mml:mo><mml:msup><mml:mn>10</mml:mn><mml:mn>19</mml:mn></mml:msup><mml:mtext> </mml:mtext><mml:mtext> </mml:mtext><mml:mi>eV</mml:mi></mml:math>

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  21. Features 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

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  22. Interpretation of the depths of maximum of extensive air showers measured by the Pierre Auger Observatory

    P. Abreu

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  23. Reinterpreting the development of extensive air showers initiated by nuclei and photons

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  24. Muons in air showers at the Pierre Auger Observatory: Measurement of atmospheric production depth

    A. Aab, P. Abreu, M. Aglietta +96

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  25. Untitled

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