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4 ta ish

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

  1. Testing hadronic-model predictions of depth of maximum of air-shower profiles and ground-particle signals using hybrid data of the Pierre Auger Observatory

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

    MaqolaAstrophysics and Cosmic PhenomenaPhysical review. D/Physical review. D.20242 iqtibos
    ABI

  2. 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

  3. 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

  4. Cosmic ray interactions in the atmosphere: QGSJET-III and other models

    S. Ostapchenko

    MaqolaAstrophysics and Cosmic PhenomenaSciPost Physics Proceedings20230 iqtibos
    ABI