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1. Proton-air interactions at ultra-high energies in muon-depleted air showers with different depths

2. $P_{tail}^{\alpha}$: a high resolution gamma/hadron and composition discriminant variable for Water-Cherenkov Detector cosmic-ray observatories

3. The Southern Wide-field Gamma-ray Observatory

4. Proton-proton interactions at the Highest Energies: the Grey-Disk and the Core-Corona models

5. Universality of the muon component of extensive air showers

6. Evaluation of the potential of a gamma-ray observatory to detect astrophysical neutrinos through inclined showers

7. On the muon scale of air showers and its application to the AGASA data

8. Self-consistent approach for measuring the energy spectra and composition of cosmic rays and determining the properties of hadronic interactions at high energy

9. Constraining the energy spectrum of neutral pions in ultra-high-energy proton-air interactions

10. Probing the high energy spectrum of neutral pions in ultra-high energy proton-Air interactions

11. Automatic Design of Artificial Neural Networks for Gamma-Ray Detection

12. The Properties of Neutrinos

13. The Higgs Mechanism and the Standard Model of Particle Physics

14. The Standard Model of Cosmology and the Dark Universe

15. Particle Detection

16. Interactions and Field Theories

17. Particles and Symmetries

18. Astrobiology and the Relation of Fundamental Physics to Life

19. Basics of Particle Physics

20. Cosmic Rays and the Development of Particle Physics

22. Messengers from the High-Energy Universe

23. Probing the $\pi^0$ spectrum at high-$x$ in proton-Air interactions at ultra-high energies

24. Probing the energy spectrum of hadrons in proton air interactions at ultrahigh energies through the fluctuations of the muon content of extensive air showers

25. Autonomous RPCs for a Cosmic Ray ground array

26. Interpretation of measurements of the number of muons in extensive air shower experiments

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

28. High-energy interactions at the Pierre Auger Observatory

29. Energy Estimation of Cosmic Rays with the Engineering Radio Array of the Pierre Auger Observatory

30. An improved limit to the diffuse flux of ultra-high energy neutrinos from the Pierre Auger Observatory

31. Measurement of the cosmic ray spectrum above $4{\times}10^{18}$ eV using inclined events detected with the Pierre Auger Observatory

32. The Pierre Auger Observatory: Contributions to the 33rd International Cosmic Ray Conference (ICRC 2013)

33. The Pierre Auger Observatory: results on the highest energy particles

34. The interplay between the electromagnetic and the muonic longitudinal profile at production

35. Sensitivity to primary composition and hadronic models from average shape of high energy cosmic ray shower profiles

40. Mando et Lego: as pontes nos testamentos eclesiásticos portugueses (1071 a 1325)

41. The upgrade of the Pierre Auger Observatory with the Scintillator Surface Detector

42. Indication of a mass-dependent anisotropy above 10 18.7 eV in the hybrid data of the Pierre Auger Observatory

43. A tau scenario application to a search for upward-going showers with the Fluorescence Detector of the Pierre Auger Observatory

44. Universality of the muon component of extensive air showers

45. UHECR arrival directions in the latest data from the original Auger and TA surface detectors and nearby galaxies

47. Gamma/hadron discrimination using a small-WCD with four PMTs

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