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1. Isotropy of cosmic rays beyond $10^{20}$ eV favors their heavy mass composition

2. Mass composition of ultra-high energy cosmic rays from distribution of their arrival directions with the Telescope Array

3. Observation of Declination Dependence in the Cosmic Ray Energy Spectrum

4. First High-speed Video Camera Observations of a Lightning Flash Associated with a Downward Terrestrial Gamma-ray Flash

5. Search for Spatial Correlations of Neutrinos with Ultra-High-Energy Cosmic Rays

6. Observation of Variations in Cosmic Ray Single Count Rates During Thunderstorms and Implications for Large-Scale Electric Field Changes

7. Indications of a Cosmic Ray Source in the Perseus-Pisces Supercluster

8. The energy spectrum of cosmic rays measured by the Telescope Array using 10 years of fluorescence detector data

9. Evidence for Declination Dependence of the Ultrahigh Energy Cosmic Ray Spectrum in the Northern Hemisphere

10. First High‐Speed Video Camera Observations of a Lightning Flash Associated With a Downward Terrestrial Gamma‐Ray Flash

11. Search for Spatial Correlations of Neutrinos with Ultra-high-energy Cosmic Rays

12. Observation of variations in cosmic ray single count rates during thunderstorms and implications for large-scale electric field changes

13. Joint analysis of the energy spectrum of ultra-high-energy cosmic rays measured at the Pierre Auger Observatory and the Telescope Array

14. The UHECR dipole and quadrupole in the latest data from the original Auger and TA surface detectors

16. Intermediate Fluence Downward Terrestrial Gamma Ray Flashes as Observed by the Telescope Array Surface Detector

17. First Time‐Resolved Leader Spectra Associated With a Downward Terrestrial Gamma‐Ray Flash Detected at the Telescope Array Surface Detector

19. Evidence for Declination Dependence of the Ultrahigh Energy Cosmic Ray Spectrum in the Northern Hemisphere

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

21. Update on the Combined Analysis of Muon Measurements from Nine Air Shower Experiments

23. Isotropy of Cosmic Rays beyond 10^{20}  eV Favors Their Heavy Mass Composition.

24. An extremely energetic cosmic ray observed by a surface detector array.

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