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2. High-Energy and Ultra-High-Energy Neutrinos: A Snowmass White Paper

3. Through the looking-glass with ALICE into the quark-gluon plasma: A new test for hadronic interaction models used in air shower simulations

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

5. Air showers, hadronic models, and muon production

6. Energy estimation of cosmic rays with the Engineering Radio Array of the Pierre Auger Observatory

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

8. Muons in air showers at the Pierre Auger Observatory

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

10. Photoproduction models for total cross section and shower development

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

12. 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

13. Characterization of the atmospheric depth profile using the ground-level temperature: the case of Malargüe, Argentina

14. Enhancements to the Southern Pierre Auger Observatory

15. Comparative study of two algorithms for the calculation of the extreme eigenvalues of large matrices

16. POWEV: a subroutine package to evaluate eigenvalues and eigenvectors of large sparse matrices

17. SPARSEM: a subroutine package to operate with large sparse matrices

18. Trigger and aperture of the surface detector array of the Pierre Auger Observatory

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

21. Correlation of the highest-energy cosmic rays with the positions of nearby active galactic nuclei

22. Hunting long-lived gluinos at the Pierre Auger Observatory

23. Physics of astroparticles

24. The influence of the geomagnetic field and of the uncertainties in the primary spectrum on the development of the muon flux in the atmosphere

25. Properties and performance of the prototype instrument for the Pierre Auger Observatory

26. Flux of atmospheric muons: Comparison between AIRES simulations and CAPRICE98 data

27. Extensive air shower simulations at the highest energies

28. Polyfit — A package for polynomial fitting

29. Operations of the Pierre Auger Observatory

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