A. C. Cobos Cerutti
16 ta ish
National Scientific and Technical Research Council
Measurement 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 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 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 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 iqtibosABIMeasurement of the depth of maximum of air-shower profiles with energies between <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> and <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:msup><mml:mn>10</mml:mn><mml:mn>20</mml:mn></mml:msup><mml:mtext> </mml:mtext><mml:mtext> </mml:mtext><mml:mi>eV</mml:mi></mml:math> using the surface detector of the Pierre Auger Observatory and deep learning
Adila Abdul Halim, P. Abreu, M. Aglietta +97
MaqolaOchiq kirishAstrophysics and Cosmic PhenomenaPhysical review. D/Physical review. D.20253 iqtibosABIArrival Directions of Cosmic Rays above 32 EeV from Phase One of the Pierre Auger Observatory
P. Abreu, M. Aglietta, Justin M. Albury +97
MaqolaOchiq kirish20223 iqtibosABIEnergy 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
Adila Abdul Halim, P. Abreu, M. Aglietta +96
ABIA Search for Photons with Energies Above 2 × 1017 eV Using Hybrid Data from the Low-Energy Extensions of the Pierre Auger Observatory
P. Abreu, M. Aglietta, Justin M. Albury +97
MaqolaOchiq kirish20222 iqtibosABIDepth of maximum of air-shower profiles above <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"> <mml:msup> <mml:mn>10</mml:mn> <mml:mn>17.7</mml:mn> </mml:msup> <mml:mtext> </mml:mtext> <mml:mtext> </mml:mtext> <mml:mi>eV</mml:mi> </mml:math> measured with the fluorescence detector of the Pierre Auger Observatory
A. Abdul Halim, P. Abreu, M. Aglietta +97
Maqola20260 iqtibosABI