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1. Status of the Yakutsk air shower array and future plans

2. A beam of ultrahigh energy particles of the same magnetic rigidity

3. Wide field-of-view Cherenkov telescope for the detection of cosmic rays in coincidence with the Yakutsk extensive air shower array

4. Cosmic ray spectrum in the energy range 1.0E15-1.0E18 eV and the second knee according to the small Cherenkov setup at the Yakutsk EAS array

5. Enhancement of the Yakutsk array by atmospheric Cherenkov telescopes to study cosmic rays above $10^{15}$ eV

6. Measuring extensive air showers with Cherenkov light detectors of the Yakutsk array: The energy spectrum of cosmic rays

7. Average mass composition of primary cosmic rays in the superhigh energy region by Yakutsk complex EAS array data

8. Behavior of some characteristics of EAS in the region of knee and ankle of spectrum

9. Recent results from Yakutsk experiment: development of EAS, energy spectrum and primary particle mass composition in the energy region of 10^15-10^19 eV

10. Fluctuations of Xmax and Primary Particle Mass Composition in the Range of Energy 5 10^{17} - 3 10^{19} ev by Yakutsk Data

11. Cosmic Rays with Energy Above 10^{17} ev

12. Muons with E_th >= 1 Gev and Mass Composition in the Energy Range 10^{18}-10^{20} ev Observed by Yakutsk Eas Array

13. Influence of Primary Cosmic Radiation Mass Composition on the Estimation of Eas Energy

14. Characteristics of EAS and Primary Particle Mass Composition in the Energy Region of $10^{17} - 3 \cdot 10^{19}$ eV by Yakutsk Data

15. Spectrum of cosmic rays with energy above $10^{17}$ eV

16. The spectrum features of UHECRs below and surrounding GZK

17. The energy spectrum of cosmic rays above 10^15 eV as derived from air Cherenkov light measurements in Yakutsk

18. Azimuthal modulation of the event rate of cosmic ray extensive air showers by the geomagnetic field

20. Status of the Yakutsk Air Shower Array and Future Plans

31. The composition of the primary particles at energies 3×1017-3×1019 eV observed at the Yakutsk array.

32. SPECTRUM OF COSMIC RAYS WITH ENERGY ABOVE 1017 EV.

33. FLUCTUATIONS OF Xmax AND PRIMARY PARTICLE MASS COMPOSITION IN THE RANGE OF ENERGY 5 × 1017 - 3 × 1019EV BY YAKUTSK DATA.

34. INFLUENCE OF PRIMARY COSMIC RADIATION MASS COMPOSITION ON THE ESTIMATION OF EAS ENERGY.

35. MUONS WITH Eth ≥ 1 GEV AND MASS COMPOSITION IN THE ENERGY RANGE 1018 - 1020EV OBSERVED BY YAKUTSK EAS ARRAY.

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

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