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Иш: Energy 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

The Pierre Auger Cosmic Ray Observatory
Aab, A., Abreu, P., Aglietta, M. +30
Мақола201510 иқтибос
ABI
EPOS LHC: Test of collective hadronization with data measured at the CERN Large Hadron Collider
T. Pierog, Iu. Karpenko, J. Katzy +2
Мақола20159 иқтибос
ABI
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
Мақола20148 иқтибос
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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
Мақола20207 иқтибос
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Constraining the sources of ultra-high-energy cosmic rays across and above the ankle with the spectrum and composition data measured at the Pierre Auger Observatory
A. Abdul Halim, P. Abreu, M. Aglietta +97
Мақола20236 иқтибос
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Observation 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
Мақола20175 иқтибос
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Reconstruction of events recorded with the surface detector of the Pierre Auger Observatory
A. Aab, P. Abreu, M. Aglietta +97
Мақола20205 иқтибос
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The energy spectrum of cosmic rays beyond the turn-down around $$\varvec{10^{17}}$$ eV as measured with the surface detector of the Pierre Auger Observatory
P. Abreu, M. Aglietta, Justin M. Albury +97
Мақола20215 иқтибос
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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
Мақола20204 иқтибос
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Arrival Directions of Cosmic Rays above 32 EeV from Phase One of the Pierre Auger Observatory
P. Abreu, M. Aglietta, Justin M. Albury +97
Мақола20223 иқтибос
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The exposure of the hybrid detector of the Pierre Auger Observatory
P. Abreu, M. Aglietta, E. J. Ahn +96
Мақола20103 иқтибос
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Data-driven estimation of the invisible energy of cosmic ray showers with the Pierre Auger Observatory
A. Aab, P. Abreu, M. Aglietta +97
Мақола20193 иқтибос
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Diffuse Flux of Ultra-high-energy Photons from Cosmic-Ray Interactions in the Disk of the Galaxy and Implications for the Search for Decaying Super-heavy Dark Matter
Corinne Bérat, C. Bleve, O. Deligny +3
Мақола20223 иқтибос
ABI
Inference 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
МақолаAstrophysics and Cosmic PhenomenaPhysical Review Letters20252 иқтибос
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A Heitler model of extensive air showers
J. Matthews
Мақола20042 иқтибос
ABI
Trigger and aperture of the surface detector array of the Pierre Auger Observatory
J. Abraham, P. Abreu, M. Aglietta +96
Мақола20102 иқтибос
ABI
Measurement 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
МақолаAstrophysics and Cosmic PhenomenaPhysical review. D/Physical review. D.20252 иқтибос
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The Fitting Procedure for Longitudinal Shower Profiles Observed with the Fluorescence Detector of the Pierre Auger Observatory
Jose A. Bellido, Adila Abdul Halim, P. Abreu +96
Мақола20232 иқтибос
ABI
A new cross-check and review of aerosol attenuation measurements at the Pierre Auger Observatory
J.R. Hansen, Adila Abdul Halim, P. Abreu +97
Мақола20232 иқтибос
ABI
Measurement of the cosmic ray spectrum above 4 × 10<sup>18</sup>eV using inclined events detected with the Pierre Auger Observatory
The Pierre Augur collaboration
Мақола20152 иқтибос
ABI
Reconstruction of inclined air showers detected with the Pierre Auger Observatory
The Pierre Auger collaboration
Мақола20142 иқтибос
ABI
Large-scale Cosmic-ray Anisotropies with 19 yr of Data from the Pierre Auger Observatory
Adila Abdul Halim, P. Abreu, M. Aglietta +97
МақолаAstrophysics and Cosmic PhenomenaThe Astrophysical Journal20241 иқтибос
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Сарлавҳасиз
Бошқа1 иқтибос
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Сарлавҳасиз
Бошқа1 иқтибос
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Сарлавҳасиз
Бошқа1 иқтибос
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