Асосий контентга ўтиш
AkademIndex

Маҳсулотлар

Ишлаб чиқувчилар учун

AkademBaseЭкотизим учун очиқ API
← Ишга қайтиш

Ушбу иш иқтибос қилган ишлар

31 та иш

Иш: 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

    Мақола201610 иқтибос
    ABI

  2. The Pierre Auger Cosmic Ray Observatory

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

    Мақола201510 иқтибос
    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

    Мақола20148 иқтибос
    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

    Мақола20207 иқтибос
    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

    Мақола20236 иқтибос
    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

    Мақола20175 иқтибос
    ABI

  7. The offline software framework of the Pierre Auger Observatory

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

    Мақола20075 иқтибос
    ABI

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

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

    Мақола20205 иқтибос
    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

    Мақола20215 иқтибос
    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

    Мақола20235 иқтибос
    ABI

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

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

    Мақола20204 иқтибос
    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

    Мақола20084 иқтибос
    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

    Мақола20204 иқтибос
    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

    Мақола20173 иқтибос
    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

    Мақола20223 иқтибос
    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

    Мақола20193 иқтибос
    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

    Мақола20193 иқтибос
    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

    Мақола20233 иқтибос
    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

    Мақола20193 иқтибос
    ABI

  20. Сарлавҳасиз

    Бошқа3 иқтибос
    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

    Мақола20122 иқтибос
    ABI

  22. Fluctuation Effects on Directional Data

    J. Linsley

    Мақола19752 иқтибос
    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

    Мақола20152 иқтибос
    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

    МақолаLightning and Electromagnetic PhenomenaEarth and Space Science20201 иқтибос
    ABI

  25. Сарлавҳасиз

    Бошқа1 иқтибос
    ABI