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

1. 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

   MaqolaOAOchiq kirishAstrophysics and Cosmic PhenomenaPhysical Review Letters20252 iqtibos

   ABIABI:AkademIndex/2025.article.001865