I. F. M. Albuquerque
15 ta ish
University of São Paulo
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, P. Abreu, M. Aglietta +97
MaqolaOchiq kirish201412 iqtibosABICombined fit of spectrum and composition data as measured by the Pierre Auger Observatory
A. Aab, P. Abreu, M. Aglietta +97
MaqolaOchiq kirish20178 iqtibosABIDepth of maximum of air-shower profiles at the Pierre Auger Observatory. II. Composition implications
A. Aab, P. Abreu, M. Aglietta +97
MaqolaOchiq kirish20148 iqtibosABIObservation of a large-scale anisotropy in the arrival directions of cosmic rays above 8 × 10 <sup>18</sup> eV
A. Aab, P. Abreu, M. Aglietta +97
MaqolaOchiq kirish20176 iqtibosABIMuons in air showers at the Pierre Auger Observatory: Mean number in highly inclined events
A. Aab, P. Abreu, M. Aglietta +97
MaqolaOchiq kirish20156 iqtibosABITesting Hadronic Interactions at Ultrahigh Energies with Air Showers Measured by the Pierre Auger Observatory
A. Aab, P. Abreu, M. Aglietta +97
MaqolaOchiq kirish20166 iqtibosABIData-driven estimation of the invisible energy of cosmic ray showers with the Pierre Auger Observatory
A. Aab, P. Abreu, M. Aglietta +97
MaqolaOchiq kirish20195 iqtibosABIMuons in air showers at the Pierre Auger Observatory: Measurement of atmospheric production depth
A. Aab, P. Abreu, M. Aglietta +96
MaqolaOchiq kirish20144 iqtibosABIImpact of atmospheric effects on the energy reconstruction of air showers observed by the surface detectors of the Pierre Auger Observatory
A. Aab, P. Abreu, M. Aglietta +97
MaqolaOchiq kirish20173 iqtibosABIMeasurement of the Proton-Air Cross Section at<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:msqrt><mml:mi>s</mml:mi></mml:msqrt><mml:mo mathvariant="bold">=</mml:mo><mml:mn>57</mml:mn><mml:mtext> </mml:mtext><mml:mtext> </mml:mtext><mml:mi>TeV</mml:mi></mml:math>with the Pierre Auger Observatory
P. Abreu, M. Aglietta, E. J. Ahn +96
MaqolaOchiq kirish20123 iqtibosABI