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1. Analysis of a Tau Neutrino Origin for the Near-Horizon Air Shower Events Observed by the Fourth Flight of the Antarctic Impulsive Transient Antenna (ANITA)

2. Measurement of R=σL/σT and the separated longitudinal and transverse structure functions in the nucleon-resonance region

3. A search for ultrahigh-energy neutrinos associated with astrophysical sources using the third flight of ANITA

4. Unusual Near-horizon Cosmic-ray-like Events Observed by ANITA-IV

5. A novel approach to building micromegas detectors enabled by precision manufacturing

6. The Simulation of the Sensitivity of the Antarctic Impulsive Transient Antenna (ANITA) to Askaryan Radiation from Cosmogenic Neutrinos Interacting in the Antarctic Ice

7. Constraints on the ultra-high energy cosmic neutrino flux from the fourth flight of ANITA

9. A comprehensive analysis of anomalous ANITA events disfavors a diffuse tau-neutrino flux origin

10. Upward-Pointing Cosmic-Ray-like Events Observed with ANITA

11. Observation of Reconstructable Radio Emission Coincident with an X-Class Solar Flare in the Askaryan Radio Array Prototype Station

12. Observation of an Unusual Upward-going Cosmic-ray-like Event in the Third Flight of ANITA

13. Constraints on the diffuse high-energy neutrino flux from the third flight of ANITA

14. Antarctic Surface Reflectivity Calculations and Measurements from the ANITA-4 and HiCal-2 Experiments

17. HiCal 2: An instrument designed for calibration of the ANITA experiment and for Antarctic surface reflectivity measurements

18. Picosecond timing of Microwave Cherenkov Impulses from High-Energy Particle Showers Using Dielectric-loaded Waveguides

19. Antarctic Surface Reflectivity Measurements from the ANITA-3 and HiCal-1 Experiments

22. The Pierre Auger Observatory Upgrade - Preliminary Design Report

23. Characteristics of Four Upward-pointing Cosmic-ray-like Events Observed with ANITA

24. Performance of two Askaryan Radio Array stations and first results in the search for ultra-high energy neutrinos

25. Constraints on the Ultra-High Energy Neutrino Flux from Gamma-Ray Bursts from a Prototype Station of the Askaryan Radio Array

28. 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

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

30. A Targeted Search for Point Sources of EeV Neutrons

31. A search for point sources of EeV photons

32. First Constraints on the Ultra-High Energy Neutrino Flux from a Prototype Station of the Askaryan Radio Array

33. Transverse-energy distributions at midrapidity in $p$$+$$p$, $d$$+$Au, and Au$+$Au collisions at $\sqrt{s_{_{NN}}}=62.4$--200~GeV and implications for particle-production models

36. Highlights from the Pierre Auger Observatory

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

38. Planning, Scheduling, and Uncertainty in the Sequence of Future Events

40. Direct photon production in d+Au collisions at sqrt(s_NN)=200 GeV

41. Searching for soft relativistic jets in Core-collapse Supernovae with the IceCube Optical Follow-up Program

42. Observation of an Anisotropy in the Galactic Cosmic Ray arrival direction at 400 TeV with IceCube

43. The Microwave Air Yield Beam Experiment (MAYBE): measurement of GHz radiation for Ultra-High Energy Cosmic Rays detection

44. Searches for periodic neutrino emission from binary systems with 22 and 40 strings of IceCube

45. IceCube Sensitivity for Low-Energy Neutrinos from Nearby Supernovae

46. Neutrino analysis of the September 2010 Crab Nebula flare and time-integrated constraints on neutrino emission from the Crab using IceCube

47. Design and Initial Performance of the Askaryan Radio Array Prototype EeV Neutrino Detector at the South Pole

48. Observation of Anisotropy in the Arrival Directions of Galactic Cosmic Rays at Multiple Angular Scales with IceCube

49. A Search for a Diffuse Flux of Astrophysical Muon Neutrinos with the IceCube 40-String Detector

50. Time-Dependent Searches for Point Sources of Neutrinos with the 40-String and 22-String Configurations of IceCube

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