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6 ta ish

Ish: 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

  1. 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

    MaqolaAstrophysics and Cosmic PhenomenaPhysical Review Letters20252 iqtibos
    ABI

  2. 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

    MaqolaAstrophysics and Cosmic PhenomenaPhysical review. D/Physical review. D.20252 iqtibos
    ABI

  3. Large-scale Cosmic-ray Anisotropies with 19 yr of Data from the Pierre Auger Observatory

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

    MaqolaAstrophysics and Cosmic PhenomenaThe Astrophysical Journal20241 iqtibos
    ABI

  4. The Pierre Auger Observatory open data

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

    MaqolaAstrophysics and Cosmic PhenomenaThe European Physical Journal C20250 iqtibos
    ABI

  5. 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

    Adila Abdul Halim, P. Abreu, M. Aglietta +96

    MaqolaAstrophysics and Cosmic PhenomenaPhysical Review Letters20250 iqtibos
    ABI

  6. Constraints on the diffuse flux of multi-PeV astrophysical neutrinos obtained with the Baikal Gigaton Volume Detector

    V. A. Allakhverdyan, A. D. Avrorin, A. V. Avrorin +69

    MaqolaAstrophysics and Cosmic PhenomenaPhysical review. D/Physical review. D.20250 iqtibos
    ABI