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

2. Multi-Messenger Physics With the Pierre Auger Observatory

3. Evidence for a mixed mass composition at the ‘ankle’ in the cosmic-ray spectrum

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

5. Multi-Messenger Physics With the Pierre Auger Observatory

6. Muons in air showers at the Pierre Auger Observatory: Measurement of atmospheric production depth

7. Astrophysical interpretation of Pierre Auger Observatory measurements of the UHECR energy spectrum and mass composition

8. Impact of atmospheric effects on the energy reconstruction of air showers observed by the surface detectors of the Pierre Auger Observatory

9. Evidence for a mixed mass composition at the 'ankle' in the cosmic-ray spectrum

10. A Targeted Search for Point Sources of EeV Neutrons

11. Ultrahigh-energy neutrino follow-up of gravitational wave events GW150914 and GW151226 with the Pierre Auger Observatory

12. Measurement of the radiation energy in the radio signal of extensive air showers as a universal estimator of cosmic-ray energy

13. Search for ultrarelativistic magnetic monopoles with the Pierre Auger Observatory

14. Large scale distribution of ultra high energy cosmic rays detected at the Pierre Auger Observatory with zenith angles up to 80°

15. Muons in air showers at the Pierre Auger Observatory

16. Improved limit to the diffuse flux of ultrahigh energy neutrinos from the Pierre Auger Observatory

17. The Pierre Auger cosmic ray observatory

18. Search for patterns by combining cosmic-ray energy and arrival directions at the Pierre Auger Observatory

19. Searches for anisotropies in the arrival directions of the highest energy cosmic rays detected by the Pierre Auger Observatory

20. Depth of maximum of air-shower profiles at the Pierre Auger Observatory. I. Measurements at energies above1017.8 eV

21. Searches for Large-Scale Anisotropy in the Arrival Directions of Cosmic Rays Detected above Energy of $10^{19}$ eV at the Pierre Auger Observatory and the Telescope Array

22. Depth of maximum of air-shower profiles at the Pierre Auger Observatory. II. Composition implications

23. Reconstruction of inclined air showers detected with the Pierre Auger Observatory

24. A search for point sources of EeV photons

25. Depth of maximum of air-shower profiles at the Pierre Auger Observatory. I. Measurements at energies above 1017.8eV

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

27. Measurement of the Radiation Energy in the Radio Signal of Extensive Air Showers as a Universal Estimator of Cosmic-Ray Energy.

28. Search for patterns by combining cosmic-ray energy and arrival directions at the Pierre Auger Observatory.

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