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31 ta ish

Ish: The Pierre Auger Observatory open data

  1. The FAIR Guiding Principles for scientific data management and stewardship

    Mark D. Wilkinson, Michel Dumontier, IJsbrand Jan Aalbersberg +50

    Maqola201610 iqtibos
    ABI

  2. The Pierre Auger Cosmic Ray Observatory

    Aab, A., Abreu, P., Aglietta, M. +30

    Maqola201510 iqtibos
    ABI

  3. 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

    Maqola20148 iqtibos
    ABI

  4. 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

    Maqola20207 iqtibos
    ABI

  5. 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

    Maqola20236 iqtibos
    ABI

  6. 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

    Maqola20175 iqtibos
    ABI

  7. The offline software framework of the Pierre Auger Observatory

    S. Argirò, S. L. C. Barroso, J. G. González +7

    Maqola20075 iqtibos
    ABI

  8. Reconstruction of events recorded with the surface detector of the Pierre Auger Observatory

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

    Maqola20205 iqtibos
    ABI

  9. 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

    Maqola20215 iqtibos
    ABI

  10. 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

    Pierre Auger Collaboration

    Maqola20235 iqtibos
    ABI

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

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

    Maqola20204 iqtibos
    ABI

  12. 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

    Maqola20084 iqtibos
    ABI

  13. 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

    Maqola20204 iqtibos
    ABI

  14. 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

    Maqola20173 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

    Maqola20223 iqtibos
    ABI

  16. Measurement of the average shape of longitudinal profiles of cosmic-ray air showers at the Pierre Auger Observatory

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

    Maqola20193 iqtibos
    ABI

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

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

    Maqola20193 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. Probing the origin of ultra-high-energy cosmic rays with neutrinos in the EeV energy range using the Pierre Auger Observatory

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

    Maqola20193 iqtibos
    ABI

  20. Sarlavhasiz

    Boshqa3 iqtibos
    ABI

  21. Measurement of the Proton-Air Cross Section at<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:msqrt><mml:mi>s</mml:mi></mml:msqrt><mml:mo mathvariant="bold">=</mml:mo><mml:mn>57</mml:mn><mml:mtext> </mml:mtext><mml:mtext> </mml:mtext><mml:mi>TeV</mml:mi></mml:math>with the Pierre Auger Observatory

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

    Maqola20122 iqtibos
    ABI

  22. Fluctuation Effects on Directional Data

    J. Linsley

    Maqola19752 iqtibos
    ABI

  23. 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

    Maqola20152 iqtibos
    ABI

  24. A 3‐Year Sample of Almost 1,600 Elves Recorded Above South America by the Pierre Auger Cosmic‐Ray Observatory

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

    MaqolaLightning and Electromagnetic PhenomenaEarth and Space Science20201 iqtibos
    ABI

  25. Sarlavhasiz

    Boshqa1 iqtibos
    ABI