K. Daumiller
66 ta ish
Karlsruhe Institute of Technology
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 iqtibosABIMeasurement 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
MaqolaOchiq kirish202010 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 iqtibosABIMeasurement of the Fluctuations in the Number of Muons in Extensive Air Showers with the Pierre Auger Observatory
A. Aab, P. Abreu, M. Aglietta +97
MaqolaOchiq kirish20216 iqtibosABIObservation 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, P. Abreu, M. Aglietta +97
MaqolaOchiq kirish20086 iqtibosABIFeatures 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
MaqolaOchiq kirish20205 iqtibosABIThe exposure of the hybrid detector of the Pierre Auger Observatory
P. Abreu, M. Aglietta, E. J. Ahn +96
Maqola20105 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 iqtibosABIReconstruction of Events Recorded with the Surface Detector of the Pierre Auger Observatory
A. Aab, P. Abreu, M. Aglietta +97
MaqolaOchiq kirish20204 iqtibosABIMeasurement 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, P. Abreu, M. Aglietta +96
MaqolaOchiq kirish20104 iqtibosABITesting hadronic-model predictions of depth of maximum of air-shower profiles and ground-particle signals using hybrid data of the Pierre Auger Observatory
Adila Abdul Halim, P. Abreu, M. Aglietta +96
MaqolaOchiq kirishAstrophysics and Cosmic PhenomenaPhysical review. D/Physical review. D.20243 iqtibosABIInference of the Mass Composition of Cosmic Rays with Energies from <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:msup><mml:mn>10</mml:mn><mml:mn>18.5</mml:mn></mml:msup></mml:math> to <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:msup><mml:mrow><mml:mn>10</mml:mn></mml:mrow><mml:mrow><mml:mn>20</mml:mn></mml:mrow></mml:msup><mml:mtext> </mml:mtext><mml:mtext> </mml:mtext><mml:mi>eV</mml:mi></mml:mrow></mml:math> Using the Pierre Auger Observatory and Deep Learning
Adila Abdul Halim, P. Abreu, M. Aglietta +97
ABIImpact 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 iqtibosABIMonte Carlo simulations for the Pierre Auger Observatory using the VO auger grid resources
Eva Santos, P. Abreu, M. Aglietta +97
MaqolaOchiq kirish20213 iqtibosABITrigger and aperture of the surface detector array of the Pierre Auger Observatory
J. Abraham, P. Abreu, M. Aglietta +96
MaqolaOchiq kirish20103 iqtibosABI