A. Blanco

16 ta ish

LIP - Laboratory of Instrumentation and Experimental Particle Physics

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

   MaqolaOAOchiq kirish202010 iqtibos

   ABIABI:AkademIndex/2026.other.098936

2. An Indication of Anisotropy in Arrival Directions of Ultra-high-energy Cosmic Rays through Comparison to the Flux Pattern of Extragalactic Gamma-Ray Sources^*

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

   MaqolaOAOchiq kirish20188 iqtibos

   ABIABI:AkademIndex/2026.other.029037

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

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

   MaqolaOAOchiq kirish20166 iqtibos

   ABIABI:AkademIndex/2026.other.098923

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

   MaqolaOAOchiq kirish20205 iqtibos

   ABIABI:AkademIndex/2026.other.111776

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

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

   MaqolaOAOchiq kirish20195 iqtibos

   ABIABI:AkademIndex/2026.other.402620

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

   MaqolaOAOchiq kirish20204 iqtibos

   ABIABI:AkademIndex/2026.other.098937

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

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

   MaqolaOAOchiq kirish20204 iqtibos

   ABIABI:AkademIndex/2026.other.098939

8. 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

   MaqolaOAOchiq kirish20174 iqtibos

   ABIABI:AkademIndex/2026.other.111762

9. 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

   MaqolaOAOchiq kirish20173 iqtibos

   ABIABI:AkademIndex/2026.other.098926

10. Two-pion production in the second resonance region in <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mrow><mml:msup><mml:mi>π</mml:mi><mml:mo>−</mml:mo></mml:msup><mml:mi>p</mml:mi></mml:mrow></mml:math> collisions with the High-Acceptance Di-Electron Spectrometer (HADES)

    J. Adamczewski-Musch, O. Arnold, E. T. Atomssa +97

    Maqola20203 iqtibos

    ABIABI:AkademIndex/2026.other.307642

11. Medium effects in proton-induced<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:msup><mml:mi>K</mml:mi><mml:mn>0</mml:mn></mml:msup></mml:math>production at 3.5 GeV

    G. Agakishiev, O. Arnold, D. Belver +94

    Maqola20143 iqtibos

    ABIABI:AkademIndex/2026.other.449244

12. 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

    MaqolaOAOchiq kirishLightning and Electromagnetic PhenomenaEarth and Space Science20202 iqtibos

    ABIABI:AkademIndex/2020.article.000190

13. First measurement of proton-induced low-momentum dielectron radiation off cold nuclear matter

    G. Agakishiev, A. Bałanda, D. Belver +95

    Maqola20122 iqtibos

    ABIABI:AkademIndex/2026.other.307615

14. Production of hydrogen isotopes and charged pions in <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mi>p</mml:mi></mml:math> (3.5 GeV) <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mo>+</mml:mo><mml:mo> </mml:mo><mml:mmultiscripts><mml:mi>Nb</mml:mi><mml:mprescripts/><mml:none/><mml:mn>93</mml:mn></mml:mmultiscripts></mml:math> reactions

    R. Abou Yassine, O. Arnold, M. Becker +85

    MaqolaOAOchiq kirishNuclear physics research studiesPhysical review. C20231 iqtibos

    ABIABI:AkademIndex/2023.article.001846

15. Investigation of the $$\mathbf {\Sigma ^{0}}$$ Production Mechanism in p(3.5 GeV)+p Collisions

    R. Abou Yassine, O. Arnold, M. Becker +88

    Maqola20241 iqtibos

    ABIABI:AkademIndex/2026.other.783549

16. Inclusive <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mrow> <mml:msup> <mml:mi>e</mml:mi> <mml:mo>+</mml:mo> </mml:msup> <mml:msup> <mml:mi>e</mml:mi> <mml:mo>−</mml:mo> </mml:msup> </mml:mrow> </mml:math> production in collisions of pions with protons and nuclei in the second resonance region of baryons

    R. Abou Yassine, J. Adamczewski-Musch, O. Arnold +97

    MaqolaOAOchiq kirishParticle physics theoretical and experimental studiesPhysical review. C20250 iqtibos

    ABIABI:AkademIndex/2025.article.000860