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Xizmatlar

Fabio Convenga

50 ta ish

Gran Sasso Science Institute

AkademScholarda batafsil koʻrsatkichlar

  1. 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

  2. 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

  3. 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

  4. 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

  5. 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

  6. 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

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

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

    MaqolaOchiq kirish20204 iqtibos
    ABI

  8. 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

  9. 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

  10. 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

  11. 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

  12. Extraction of the muon signals recorded with the surface detector of the Pierre Auger Observatory using recurrent neural networks

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

    MaqolaOchiq kirish20213 iqtibos
    ABI

  13. Deep-learning based reconstruction of the shower maximum X$_{max}$ using the water-Cherenkov detectors of the Pierre Auger Observatory

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

    Maqola20213 iqtibos
    ABI

  14. 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

    MaqolaOchiq kirishAstrophysics and Cosmic PhenomenaPhysical review. D/Physical review. D.20253 iqtibos
    ABI

  15. Arrival 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 iqtibos
    ABI

  16. 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

    MaqolaOchiq kirish20233 iqtibos
    ABI

  17. A new cross-check and review of aerosol attenuation measurements at the Pierre Auger Observatory

    J.R. Hansen, Adila Abdul Halim, P. Abreu +97

    MaqolaOchiq kirish20233 iqtibos
    ABI

  18. Search for photons above 10<sup>19</sup> eV with the surface detector of the Pierre Auger Observatory

    P. Abreu, M. Aglietta, I. Allekotte +97

    Maqola20233 iqtibos
    ABI

  19. 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

    Adila Abdul Halim, P. Abreu, M. Aglietta +96

    MaqolaOchiq kirishAstrophysics and Cosmic PhenomenaPhysical Review Letters20252 iqtibos
    ABI

  20. Event-by-event reconstruction of the shower maximum $X_{\mathrm{max}}$ with the Surface Detector of the Pierre Auger Observatory using deep learning

    Jonas Glombitza, P. Abreu, M. Aglietta +97

    MaqolaOchiq kirish20212 iqtibos
    ABI

  21. Mass Composition from 3 EeV to 100 EeV using the Depth of the Maximum of Air-Shower Profiles Estimated with Deep Learning using Surface Detector Data of the Pierre Auger Observatory

    Jonas Glombitza, Adila Abdul Halim, P. Abreu +97

    MaqolaOchiq kirish20232 iqtibos
    ABI

  22. The Time Evolution of the Surface Detector of the Pierre Auger Observatory

    Orazio Zapparrata, Adila Abdul Halim, P. Abreu +97

    MaqolaOchiq kirish20232 iqtibos
    ABI

  23. Depth of Maximum of Air-Shower Profiles above $10^{17.8}$eV Measured with the Fluorescence Detector of the Pierre Auger Observatory and Mass Composition Implications

    Thomas Fitoussi, Adila Abdul Halim, P. Abreu +97

    MaqolaOchiq kirish20232 iqtibos
    ABI

  24. Limits to Gauge Coupling in the Dark Sector Set by the Nonobservation of Instanton-Induced Decay of Super-Heavy Dark Matter in the Pierre Auger Observatory Data

    P. Abreu, M. Aglietta, Justin M. Albury +97

    Maqola20232 iqtibos
    ABI

  25. A 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 iqtibos
    ABI