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B. Andrada

10 та иш

Instituto de Tecnologías en Detección y Astropartículas

  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

    МақолаAstrophysics and Cosmic PhenomenaPhysical review. D/Physical review. D.20242 иқтибос
    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

    МақолаAstrophysics and Cosmic PhenomenaPhysical Review Letters20252 иқтибос
    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

    МақолаAstrophysics and Cosmic PhenomenaPhysical review. D/Physical review. D.20252 иқтибос
    ABI

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

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

    МақолаAstrophysics and Cosmic PhenomenaThe Astrophysical Journal20241 иқтибос
    ABI

  5. Search for photons above <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>18</mml:mn></mml:mrow></mml:msup></mml:mrow><mml:mtext> </mml:mtext><mml:mtext> </mml:mtext><mml:mi>eV</mml:mi></mml:math> by simultaneously measuring the atmospheric depth and the muon content of air showers at the Pierre Auger Observatory

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

    МақолаAstrophysics and Cosmic PhenomenaPhysical review. D/Physical review. D.20240 иқтибос
    ABI

  6. Search for the Anomalous Events Detected by ANITA Using the Pierre Auger Observatory

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

    МақолаAstrophysics and Cosmic PhenomenaPhysical Review Letters20250 иқтибос
    ABI

  7. The Pierre Auger Observatory open data

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

    МақолаAstrophysics and Cosmic PhenomenaThe European Physical Journal C20250 иқтибос
    ABI

  8. 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

    МақолаAstrophysics and Cosmic PhenomenaPhysical Review Letters20250 иқтибос
    ABI

  9. Measuring the muon content of inclined air showers using AERA and the water-Cherenkov detectors of the Pierre Auger Observatory

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

    МақолаAstrophysics and Cosmic PhenomenaPhysical review. D/Physical review. D.20250 иқтибос
    ABI

  10. Search for Ultra-high-energy Neutrons from Galactic Sources with the Pierre Auger Observatory

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

    МақолаAstrophysics and Cosmic PhenomenaThe Astrophysical Journal20260 иқтибос
    ABI