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Ish: 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

  1. Long Short-Term Memory

    Sepp Hochreiter, Jürgen Schmidhuber

    Maqola199741 iqtibos
    ABI

  2. Deep learning

    Yann LeCun, Yoshua Bengio, Geoffrey E. Hinton

    Sharh maqola201536 iqtibos
    ABI

  3. End to the Cosmic-Ray Spectrum?

    K. Greisen

    Maqola196613 iqtibos
    ABI

  4. The Pierre Auger Cosmic Ray Observatory

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

    Maqola201510 iqtibos
    ABI

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

    T. Pierog, Iu. Karpenko, J. Katzy +2

    Maqola20159 iqtibos
    ABI

  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

    Maqola20148 iqtibos
    ABI

  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

    Maqola20236 iqtibos
    ABI

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

    Alexey Yushkov

    Maqola20195 iqtibos
    ABI

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

    Felix Riehn, R. Engel, Anatoli Fedynitch +2

    Maqola20205 iqtibos
    ABI

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

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

    Maqola20205 iqtibos
    ABI

  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

    Maqola20215 iqtibos
    ABI

  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

    Maqola20235 iqtibos
    ABI

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

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

    Maqola20174 iqtibos
    ABI

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

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

    Maqola20144 iqtibos
    ABI

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

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

    Maqola20164 iqtibos
    ABI

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

    M. Ave, M. Roth, A. Schulz

    Maqola20174 iqtibos
    ABI

  17. AugerPrime: the Pierre Auger Observatory Upgrade

    Antonella Castellina

    Maqola20194 iqtibos
    ABI

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

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

    Maqola20204 iqtibos
    ABI

  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

    Maqola20214 iqtibos
    ABI

  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>

    J. Abraham, P. Abreu, M. Aglietta +97

    Maqola20084 iqtibos
    ABI

  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

    Maqola20204 iqtibos
    ABI

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

    P. Abreu

    Maqola20133 iqtibos
    ABI

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

    Manlio De Domenico, Mariangela Settimo, Simone Riggi +1

    Maqola20133 iqtibos
    ABI

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

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

    Maqola20143 iqtibos
    ABI

  25. Sarlavhasiz

    Boshqa3 iqtibos
    ABI