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1. Direct measurement of the muonic content of extensive air showers between $$\mathbf { 2\times 10^{17}}$$ 2×1017 and $$\mathbf {2\times 10^{18}}~$$ 2×1018 eV at the Pierre Auger Observatory

2. A 3‐Year Sample of Almost 1,600 Elves Recorded Above South America by the Pierre Auger Cosmic‐Ray Observatory

3. Multi-Messenger Physics With the Pierre Auger Observatory

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

5. Extraction of the Muon Signals Recorded with the Surface Detector of the Pierre Auger Observatory Using Recurrent Neural Networks

6. The FRAM robotic telescope for atmospheric monitoring at the Pierre Auger Observatory

7. 3D Microstructural Characterization of Ni/YSZ Electrodes Exposed to 1 Year of Electrolysis Testing

8. Towards the Validation of a Phase Field Model for Ni Coarsening in Solid Oxide Cells

9. Measurement of the Fluctuations in the Number of Muons in Extensive Air Showers with the Pierre Auger Observatory

10. Design, upgrade and characterization of the silicon photomultiplier front-end for the AMIGA detector at the Pierre Auger Observatory

11. Deep-learning based reconstruction of the shower maximum X max using the water-Cherenkov detectors of the Pierre Auger Observatory

12. Neutrosophic Spherical Cubic Sets

13. Studies on the response of a water-Cherenkov detector of the Pierre Auger Observatory to atmospheric muons using an RPC hodoscope

14. A 3-Year Sample of Almost 1,600 Elves Recorded Above South America by the Pierre Auger Cosmic-Ray Observatory

15. Reconstruction of events recorded with the surface detector of the Pierre Auger Observatory

16. Comparison of microstructural evolution of fuel electrodes in solid oxide fuel cells and electrolysis cells

17. Direct measurement of the muonic content of extensive air showers between $\mathbf { 2\times 10^{17}}$ and $\mathbf {2\times 10^{18}}~$eV at the Pierre Auger Observatory

18. The energy spectrum of ultra-high energy cosmic rays measured at the Pierre Auger Observatory and at the Telescope Array

19. Multi-Messenger Physics With the Pierre Auger Observatory

20. Ultra-high energy neutrinos searches with the Pierre Auger Observatory

21. (Invited) Fuel Electrode Degradation for Solid Oxide Electrolysis Cells – How to Characterize It and What to Do about It

22. Astrophysical interpretation of Pierre Auger Observatory measurements of the UHECR energy spectrum and mass composition

23. Impact of atmospheric effects on the energy reconstruction of air showers observed by the surface detectors of the Pierre Auger Observatory

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

25. Ultrahigh-energy neutrino follow-up of gravitational wave events GW150914 and GW151226 with the Pierre Auger Observatory

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

27. Search for ultrarelativistic magnetic monopoles with the Pierre Auger Observatory

28. Bipolar neutrosophic soft generalized pre-closed sets and pre-open sets in topological space

29. Dysregulation of the miRNome unveils a crosstalk between obesity and prostate cancer: miR-107 asa personalized diagnostic and therapeutic tool

30. Bipolar neutrosophic graded soft sets and their topological spaces

31. Changes in severity, mortality, and virus genome among a Spanish cohort of patients hospitalized with SARS-CoV-2

32. How Donor and Surgical Factors Affect the Viability and Functionality of Human Hepatocytes Isolated From Liver Resections

33. Experimental and theoretical study of theH2(d⃗,γ)H4ereaction belowEc.m.=60keV

34. Some similarity and entropy measurements of bipolar neutrosophic soft sets

35. Can Acceptable Pulp be Obtained from Eucalyptus globulus Wood Chips after Hemicellulose Extraction?

36. Phase field modelling of microstructural changes in NI/YSZ solid oxide electrolysis cell electrodes

37. Microstructural Characterization of Ni/YSZ Electrodes in a Solid Oxide Electrolysis Stack Tested for 9000 Hours

38. Measurement of the Fluctuations in the Number of Muons in Extensive Air Showers with the Pierre Auger Observatory.

39. Features of the Energy Spectrum of Cosmic Rays above 2.5×10^{18}  eV Using the Pierre Auger Observatory.

40. Testing Hadronic Interactions at Ultrahigh Energies with Air Showers Measured by the Pierre Auger Observatory.

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

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