L. Calcagni

6 ta ish

National Scientific and Technical Research Council

1. Measurement of the cosmic-ray energy spectrum above<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mn>2.5</mml:mn><mml:mo>×</mml:mo><mml:msup><mml:mn>10</mml:mn><mml:mn>18</mml:mn></mml:msup><mml:mtext> </mml:mtext><mml:mtext> </mml:mtext><mml:mi>eV</mml:mi></mml:math>using the Pierre Auger Observatory

   A. Aab, P. Abreu, M. Aglietta +97

   MaqolaOAOchiq kirish202010 iqtibos

   ABIABI:AkademIndex/2026.other.098936

2. Features of the Energy Spectrum of Cosmic Rays above <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mn>2.5</mml:mn><mml:mo>×</mml:mo><mml:msup><mml:mn>10</mml:mn><mml:mn>18</mml:mn></mml:msup><mml:mtext> </mml:mtext><mml:mtext> </mml:mtext><mml:mi>eV</mml:mi></mml:math> Using the Pierre Auger Observatory

   A. Aab, P. Abreu, M. Aglietta +97

   MaqolaOAOchiq kirish20205 iqtibos

   ABIABI:AkademIndex/2026.other.111776

3. Data-driven estimation of the invisible energy of cosmic ray showers with the Pierre Auger Observatory

   A. Aab, P. Abreu, M. Aglietta +97

   MaqolaOAOchiq kirish20195 iqtibos

   ABIABI:AkademIndex/2026.other.402620

4. Direct measurement of the muonic content of extensive air showers between $$\mathbf { 2\times 10^{17}}$$ and $$\mathbf {2\times 10^{18}}~$$eV at the Pierre Auger Observatory

   A. Aab, P. Abreu, M. Aglietta +97

   MaqolaOAOchiq kirish20204 iqtibos

   ABIABI:AkademIndex/2026.other.098937

5. Reconstruction of Events Recorded with the Surface Detector of the Pierre Auger Observatory

   A. Aab, P. Abreu, M. Aglietta +97

   MaqolaOAOchiq kirish20204 iqtibos

   ABIABI:AkademIndex/2026.other.098939

6. A 3‐Year Sample of Almost 1,600 Elves Recorded Above South America by the Pierre Auger Cosmic‐Ray Observatory

   A. Aab, P. Abreu, M. Aglietta +96

   MaqolaOAOchiq kirishLightning and Electromagnetic PhenomenaEarth and Space Science20202 iqtibos

   ABIABI:AkademIndex/2020.article.000190