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Иш: Data-driven estimation of the invisible energy of cosmic ray showers with the Pierre Auger Observatory

1. 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

   ABIABI:AkademIndex/openalex/2024.article.001562

2. The Pierre Auger Observatory open data

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

   МақолаAstrophysics and Cosmic PhenomenaThe European Physical Journal C20250 иқтибос

   ABIABI:AkademIndex/openalex/2025.article.001608

3. 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

   ABIABI:AkademIndex/openalex/2025.article.001865