Asosiy kontentga oʻtish
AkademIndex

Xizmatlar

B. R. Dawson

67 ta ish

The University of Adelaide

AkademScholarda batafsil koʻrsatkichlar

  1. 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 iqtibos
    ABI

  2. 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

    MaqolaOchiq kirish202010 iqtibos
    ABI

  3. Combined fit of spectrum and composition data as measured by the Pierre Auger Observatory

    A. Aab, P. Abreu, M. Aglietta +97

    MaqolaOchiq kirish20178 iqtibos
    ABI

  4. An Indication of Anisotropy in Arrival Directions of Ultra-high-energy Cosmic Rays through Comparison to the Flux Pattern of Extragalactic Gamma-Ray Sources<sup>*</sup>

    A. Aab, P. Abreu, M. Aglietta +97

    MaqolaOchiq kirish20188 iqtibos
    ABI

  5. Depth of maximum of air-shower profiles at the Pierre Auger Observatory. II. Composition implications

    A. Aab, P. Abreu, M. Aglietta +97

    MaqolaOchiq kirish20148 iqtibos
    ABI

  6. 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

    MaqolaOchiq kirish20217 iqtibos
    ABI

  7. 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

    MaqolaOchiq kirish20176 iqtibos
    ABI

  8. Muons in air showers at the Pierre Auger Observatory: Mean number in highly inclined events

    A. Aab, P. Abreu, M. Aglietta +97

    MaqolaOchiq kirish20156 iqtibos
    ABI

  9. Testing Hadronic Interactions at Ultrahigh Energies with Air Showers Measured by the Pierre Auger Observatory

    A. Aab, P. Abreu, M. Aglietta +97

    MaqolaOchiq kirish20166 iqtibos
    ABI

  10. 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 iqtibos
    ABI

  11. 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, P. Abreu, M. Aglietta +97

    MaqolaOchiq kirish20086 iqtibos
    ABI

  12. 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

    MaqolaOchiq kirish20205 iqtibos
    ABI

  13. The exposure of the hybrid detector of the Pierre Auger Observatory

    P. Abreu, M. Aglietta, E. J. Ahn +96

    Maqola20105 iqtibos
    ABI

  14. Data-driven estimation of the invisible energy of cosmic ray showers with the Pierre Auger Observatory

    A. Aab, P. Abreu, M. Aglietta +97

    MaqolaOchiq kirish20195 iqtibos
    ABI

  15. Muons in air showers at the Pierre Auger Observatory: Measurement of atmospheric production depth

    A. Aab, P. Abreu, M. Aglietta +96

    MaqolaOchiq kirish20144 iqtibos
    ABI

  16. Direct measurement of the muonic content of extensive air showers between $$\mathbf { 2\times 10^{17}}$$ and $$\mathbf {2\times 10^{18}}~$$eV at the Pierre Auger Observatory

    A. Aab, P. Abreu, M. Aglietta +97

    MaqolaOchiq kirish20204 iqtibos
    ABI

  17. Reconstruction of Events Recorded with the Surface Detector of the Pierre Auger Observatory

    A. Aab, P. Abreu, M. Aglietta +97

    MaqolaOchiq kirish20204 iqtibos
    ABI

  18. 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, P. Abreu, M. Aglietta +96

    MaqolaOchiq kirish20104 iqtibos
    ABI

  19. Inferences on mass composition and tests of hadronic interactions from 0.3 to 100 EeV using the water-Cherenkov detectors of the Pierre Auger Observatory

    A. Aab, P. Abreu, M. Aglietta +97

    MaqolaOchiq kirish20174 iqtibos
    ABI

  20. The Energy Scale of the Pierre Auger Observatory

    B. R. Dawson

    Maqola20194 iqtibos
    ABI

  21. A search for ultra-high-energy photons at the Pierre Auger Observatory exploiting air-shower universality

    Pierpaolo Savina, P. Abreu, M. Aglietta +97

    Maqola20214 iqtibos
    ABI

  22. Testing 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 iqtibos
    ABI

  23. 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

    MaqolaOchiq kirishAstrophysics and Cosmic PhenomenaPhysical Review Letters20253 iqtibos
    ABI

  24. Impact 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 iqtibos
    ABI

  25. Monte Carlo simulations for the Pierre Auger Observatory using the VO auger grid resources

    Eva Santos, P. Abreu, M. Aglietta +97

    MaqolaOchiq kirish20213 iqtibos
    ABI