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45 ta ish

Ish: 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

  1. The Pierre Auger Cosmic Ray Observatory

    Aab, A., Abreu, P., Aglietta, M. +30

    Maqola201510 iqtibos
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  2. The exposure of the hybrid detector of the Pierre Auger Observatory

    P. Abreu, M. Aglietta, E. J. Ahn +96

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  3. A Heitler model of extensive air showers

    J. Matthews

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  4. Sarlavhasiz

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  5. Sarlavhasiz

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