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3. 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

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

7. A Targeted Search for Point Sources of EeV Neutrons

8. A search for point sources of EeV photons

9. Highlights from the Pierre Auger Observatory

10. Pierre Auger Observatory and Telescope Array: Joint Contributions to the 33rd International Cosmic Ray Conference (ICRC 2013)

11. Antennas for the Detection of Radio Emission Pulses from Cosmic-Ray induced Air Showers at the Pierre Auger Observatory

12. The Rapid Atmospheric Monitoring System of the Pierre Auger Observatory

13. A search for ultra-high energy neutrinos in highly inclined events at the Pierre Auger Observatory

14. Description of Atmospheric Conditions at the Pierre Auger Observatory using the Global Data Assimilation System (GDAS)

15. The effect of the geomagnetic field on cosmic ray energy estimates and large scale anisotropy searches on data from the Pierre Auger Observatory

16. Trigger and Aperture of the Surface Detector Array of the Pierre Auger Observatory

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

18. Search for signatures of magnetically-induced alignment in the arrival directions measured by the Pierre Auger Observatory

19. The Pierre Auger Observatory I: The Cosmic Ray Energy Spectrum and Related Measurements

20. The Pierre Auger Observatory III: Other Astrophysical Observations

21. The Pierre Auger Observatory IV: Operation and Monitoring

22. The Pierre Auger Observatory II: Studies of Cosmic Ray Composition and Hadronic Interaction models

23. The Pierre Auger Observatory V: Enhancements

24. Anisotropy and chemical composition of ultra-high energy cosmic rays using arrival directions measured by the Pierre Auger Observatory

25. Search for First Harmonic Modulation in the Right Ascension Distribution of Cosmic Rays Detected at the Pierre Auger Observatory

26. Advanced functionality for radio analysis in the Offline software framework of the Pierre Auger Observatory

27. Update on the correlation of the highest energy cosmic rays with nearby extragalactic matter

28. The Fluorescence Detector of the Pierre Auger Observatory

29. Calibration and Monitoring of the Pierre Auger Observatory

30. Operations of and Future Plans for the Pierre Auger Observatory

31. Astrophysical Sources of Cosmic Rays and Related Measurements with the Pierre Auger Observatory

32. Studies of Cosmic Ray Composition and Air Shower Structure with the Pierre Auger Observatory

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

34. Upper limit on the cosmic-ray photon fraction at EeV energies from the Pierre Auger Observatory

35. Line‐field confocal optical coherence tomography: New insights for psoriasis treatment monitoring.

38. Identifying clouds over the Pierre Auger Observatory using infrared satellite data

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

40. Description of atmospheric conditions at the Pierre Auger Observatory using the Global Data Assimilation System (GDAS)

41. Search for signatures of magnetically-induced alignment in the arrival directions measured by the Pierre Auger Observatory

42. Characteristic of chronic plaque psoriasis patients treated with biologics in Italy during the COVID-19 pandemic. risk analysis from the PSO-BIO-COVID observational study

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

45. Search for first harmonic modulation in the right ascension distribution of cosmic rays detected at the Pierre Auger Observatory

46. The exposure of the hybrid detector of the Pierre Auger Observatory

47. Advanced functionality for radio analysis in the Offline software framework of the Pierre Auger Observatory

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