Correlation of the Highest-Energy Cosmic Rays with Nearby Extragalactic ObjectsJ. Abraham, H. Blümer, P. Abreu et al.|Science|2007Cited by 794
Observation of the Suppression of the Flux of Cosmic Rays above<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mn>4</mml:mn><mml:mo>×</mml:mo><mml:msup><mml:mn>10</mml:mn><mml:mn>19</mml:mn></mml:msup><mml:mtext> </mml:mtext><mml:mtext> </mml:mtext><mml:mi>eV</mml:mi></mml:math>J. Abraham, H. Blümer, P. Abreu et al.|Physical Review Letters|2008Cited by 635
Measurement of the Depth of Maximum of Extensive Air Showers above<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><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>J. Abraham, R. Bonino, J. Aublin et al.|Physical Review Letters|2010Cited by 515
Measurement of the energy spectrum of cosmic rays above 1018 eV using the Pierre Auger ObservatoryJ. Abraham, Nataliia Borodai, P. Abreu et al.|Physics Letters B|2010Cited by 484
Depth of maximum of air-shower profiles at the Pierre Auger Observatory. I. Measurements at energies above<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mn>1</mml:mn><mml:msup><mml:mrow><mml:mn>0</mml:mn></mml:mrow><mml:mrow><mml:mn>17.8</mml:mn></mml:mrow></mml:msup><mml:mtext> </mml:mtext><mml:mi>eV</mml:mi></mml:mrow></mml:math>A. Aab, I. M. Brancus, P. Abreu et al.|Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields|2014Cited by 390