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Ish: Energy Spectrum of Ultrahigh-Energy Cosmic Rays across Declinations <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"> <mml:mo>−</mml:mo> <mml:mn>9</mml:mn> <mml:mn>0</mml:mn> <mml:mi>°</mml:mi> </mml:math> to <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"> <mml:mo>+</mml:mo> <mml:mn>44.8</mml:mn> <mml:mi>°</mml:mi> </mml:math> as Measured at the Pierre Auger Observatory

  1. The Pierre Auger Cosmic Ray Observatory

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

    MaqolaOchiq kirish201517 iqtibos
    ABI

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

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

    MaqolaOchiq kirish201514 iqtibos
    ABI

  3. 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

    MaqolaOchiq kirish201412 iqtibos
    ABI

  4. 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 iqtibos
    ABI

  5. 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

    MaqolaOchiq kirish20217 iqtibos
    ABI

  6. 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

    MaqolaOchiq kirish20237 iqtibos
    ABI

  7. Observation 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 iqtibos
    ABI

  8. A Heitler model of extensive air showers

    J. Matthews

    Maqola20045 iqtibos
    ABI

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

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

    Maqola20205 iqtibos
    ABI

  10. 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

    MaqolaOchiq kirish20205 iqtibos
    ABI

  11. The exposure of the hybrid detector of the Pierre Auger Observatory

    P. Abreu, M. Aglietta, E. J. Ahn +96

    Maqola20105 iqtibos
    ABI

  12. Data-driven estimation of the invisible energy of cosmic ray showers with the Pierre Auger Observatory

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

    MaqolaOchiq kirish20195 iqtibos
    ABI

  13. Diffuse Flux of Ultra-high-energy Photons from Cosmic-Ray Interactions in the Disk of the Galaxy and Implications for the Search for Decaying Super-heavy Dark Matter

    Corinne Bérat, C. Bleve, O. Deligny +3

    Maqola20224 iqtibos
    ABI

  14. 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

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

    MaqolaOchiq kirishAstrophysics and Cosmic PhenomenaPhysical Review Letters20253 iqtibos
    ABI

  15. Trigger and aperture of the surface detector array of the Pierre Auger Observatory

    J. Abraham, P. Abreu, M. Aglietta +96

    MaqolaOchiq kirish20103 iqtibos
    ABI

  16. Measurement of the depth of maximum of air-shower profiles with energies between <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> and <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:msup><mml:mn>10</mml:mn><mml:mn>20</mml:mn></mml:msup><mml:mtext> </mml:mtext><mml:mtext> </mml:mtext><mml:mi>eV</mml:mi></mml:math> using the surface detector of the Pierre Auger Observatory and deep learning

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

    MaqolaOchiq kirishAstrophysics and Cosmic PhenomenaPhysical review. D/Physical review. D.20253 iqtibos
    ABI

  17. Arrival Directions of Cosmic Rays above 32 EeV from Phase One of the Pierre Auger Observatory

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

    MaqolaOchiq kirish20223 iqtibos
    ABI

  18. The Fitting Procedure for Longitudinal Shower Profiles Observed with the Fluorescence Detector of the Pierre Auger Observatory

    Jose A. Bellido, Adila Abdul Halim, P. Abreu +96

    MaqolaOchiq kirish20233 iqtibos
    ABI

  19. A new cross-check and review of aerosol attenuation measurements at the Pierre Auger Observatory

    J.R. Hansen, Adila Abdul Halim, P. Abreu +97

    MaqolaOchiq kirish20233 iqtibos
    ABI

  20. Reconstruction of inclined air showers detected with the Pierre Auger Observatory

    The Pierre Auger collaboration

    Maqola20143 iqtibos
    ABI

  21. Sarlavhasiz

    Boshqa3 iqtibos
    ABI

  22. Sarlavhasiz

    Boshqa3 iqtibos
    ABI

  23. Measurement of the cosmic ray spectrum above 4 × 10<sup>18</sup>eV using inclined events detected with the Pierre Auger Observatory

    The Pierre Augur collaboration

    Maqola20152 iqtibos
    ABI

  24. Sarlavhasiz

    Boshqa2 iqtibos
    ABI

  25. Sarlavhasiz

    Boshqa2 iqtibos
    ABI