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1. Software Suite for Modeling Cherenkov Images of Extensive Air Showers in the SPHERE-3 Detector

2. SPHERE-3: tackling the problem of primary cosmic ray mass composition with a new approach

3. Application of convolutional neural networks for extensive air shower separation in the SPHERE-3 experiment

5. Directional Sensitivity of the NEWSdm Experiment to Cosmic Ray Boosted Dark Matter

6. Updated constraints on sterile neutrino mixing in the OPERA experiment using a new $\nu_e$ identification method

7. Design of the Simulation Scheme for SPHERE-3 Telescope for the \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$${10^{15}{-}10^{18}}$$\end{document} eV Primary Cosmic Ray Studies Using Direct and Reflected Cherenkov Light from the Extensive Air Showers

9. Muography of the Cave Church of the Holy Dormition Pskovo-Pechersky Monastery

11. EAS observation conditions in the SPHERE-2 balloon experiment

12. Measurement of the muon flux at the SND@LHC experiment

13. Sensitivity of the SHiP experiment to dark photons decaying to a pair of charged particles

14. Investigation of energy spectrum and chemical composition of primary cosmic rays in 1-100 PeV energy range with a UAV-borne installation

15. SND@LHC

16. The SPHERE-2 detector for observation of extensive air showers in 1 PeV -- 1 EeV energy range

17. First observation of a tau neutrino charged current interaction with charm production in the Opera experiment

18. A Noninvasive Muonography-Based Method for Exploration of Cultural Heritage Objects

20. Final results on neutrino oscillation parameters from the OPERA experiment in the CNGS beam

21. Spatial and temporal structure of EAS reflected Cherenkov light signal

22. Latest results of the OPERA experiment on nu-tau appearance in the CNGS neutrino beam

23. Measurement of the cosmic ray muon flux seasonal variation with the OPERA detector

24. Final results of the OPERA experiment on $\nu_\tau$ appearance in the CNGS beam

25. Final results of the search for $\nu_{\mu} \to \nu_{e}$ oscillations with the OPERA detector in the CNGS beam

26. Muon Radiography of Large Natural and Industrial Objects—A New Stage in the Nuclear Emulsion Technique

27. Discovery potential for directional Dark Matter detection with nuclear emulsions

28. The active muon shield in the SHiP experiment

30. Search for Hidden Rooms in the Holy Trinity Danilov Monastery by the Muon Radiography Method

31. Muography of Large Natural and Industrial Objects

32. NEWS: Nuclear Emulsions for WIMP Search

33. Discovery of tau neutrino appearance in the CNGS neutrino beam with the OPERA experiment

34. Constraints on the energy spectra of charged particles predicted in some model interactions of hadrons with help of the atmospheric muon flux

35. Constrains of hadronic interaction models from the cosmic muon observations

36. A facility to Search for Hidden Particles (SHiP) at the CERN SPS

37. Search for Sterile Neutrinos in the Muon Neutrino Disappearance Mode at FNAL

38. Event-by-event study of CR composition with the SPHERE experiment using the 2013 data

39. Results and prospects on registration of reflected Cherenkov light of EAS from cosmic particles above 10^{15} eV

40. Limits on muon-neutrino to tau-neutrino oscillations induced by a sterile neutrino state obtained by OPERA at the CNGS beam

41. The SHiP experiment at the proposed CERN SPS Beam Dump Facility

42. The NESSiE way to searches for sterile neutrinos at FNAL

43. Observation of nu_tau appearance in the CNGS beam with the OPERA experiment

44. Determination of the muon charge sign with the dipolar spectrometers of the OPERA experiment

45. Procedure for short-lived particle detection in the OPERA experiment and its application to charm decays

46. Prospects for the measurement of muon-neutrino disappearance at the FNAL-Booster

47. Measurement of TeV atmospheric muon charge ratio with the full OPERA data

48. Evidence for $\nu_\mu \to \nu_\tau$ appearance in the CNGS neutrino beam with the OPERA experiment

49. The NESSiE Concept for Sterile Neutrinos

50. OPERA tau neutrino charged current interactions

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