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23 results on '"Platino, M"'

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1. A Catalog of the Highest-Energy Cosmic Rays Recorded During Phase I of Operation of the Pierre Auger Observatory

2. 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

3. QUBIC II: Spectral polarimetry with bolometric interferometry

4. Status of QUBIC, the Q&U Bolometer for Cosmology

5. QUBIC I: Overview and ScienceProgram

6. QUBIC VI: cryogenic half wave plate rotator, design and performances

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

8. QUBIC II: Spectro-Polarimetry with Bolometric Interferometry

9. QUBIC I: Overview and Science Program

10. QUBIC: using NbSi TESs with a bolometric interferometer to characterize the polarisation of the CMB

11. QUBIC III: Laboratory Characterization

12. Observation of inclined EeV air showers with the radio detector of the Pierre Auger Observatory

13. The Pierre Auger Observatory: Contributions to the 36th International Cosmic Ray Conference (ICRC 2019) The Pierre Auger Collaboration

14. The Pierre Auger Observatory status and latest results

15. The Pierre Auger Observatory III: Other Astrophysical Observations

16. Calibration and Monitoring of the Pierre Auger Observatory

17. The Cosmic Ray Energy Spectrum and Related Measurements with the Pierre Auger Observatory

18. Erratum to 'Correlation of the highest-energy cosmic rays with the positions of nearby active galactic nuclei' [Astroparticle Physics 29(3) (2008) 188-204]

19. Features of the Energy Spectrum of Cosmic Rays above 2.5×10$^{18}$ eV Using the Pierre Auger Observatory

20. TES Bolometer Arrays for the QUBIC B-Mode CMB Experiment

21. QUBIC: the Q \& U Bolometric Interferometer for Cosmology

22. The Lateral Trigger Probability function for the Ultra-High Energy Cosmic Ray Showers detected by the Pierre Auger Observatory

23. Measurement of the energy spectrum of cosmic rays above 10^18 eV using the Pierre Auger Observatory

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