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1. Individual particle approach to the diffusive shock acceleration. Effect of the non-uniform flow velocity downstream of the shock

2. Dark Matter Line Searches with the Cherenkov Telescope Array

3. Prospects for $\gamma$-ray observations of the Perseus galaxy cluster with the Cherenkov Telescope Array

4. Sensitivity of the Cherenkov Telescope Array to spectral signatures of hadronic PeVatrons with application to Galactic Supernova Remnants

5. Polarized radio emission unveils the structure of the pre-supernova circumstellar magnetic field and the radio emission in SN1987A

6. Rectangular core-collapse supernova remnants: application to Puppis A

7. Magneto-hydrodynamic simulations of young supernova remnants and their energy-conversion phase

8. Modeling particle acceleration and non-thermal emission in supernova remnants

9. Sensitivity of the Cherenkov Telescope Array for probing cosmology and fundamental physics with gamma-ray propagation

10. Sensitivity of the Cherenkov Telescope Array to a dark matter signal from the Galactic centre

11. GeV light curves of young supernova remnants

12. Hydrodynamic simulations unravel the progenitor-supernova-remnant connection in SN 1987A

13. Sensitivity of the Cherenkov Telescope Array to spectral signatures of hadronic PeVatrons with application to Galactic Supernova Remnants

14. Monte Carlo studies for the optimisation of the Cherenkov Telescope Array layout

15. 3D MHD modeling of the expanding remnant of SN 1987A. Role of magnetic field and non-thermal radio emission

16. Post-adiabatic supernova remnants in an interstellar magnetic field: oblique shocks and non-uniform environment

17. Investigating the high-frequency spectral features of SNRs Tycho, W44 and IC443 with the Sardinia Radio Telescope

19. Science with the Cherenkov Telescope Array

20. Cherenkov Telescope Array Contributions to the 35th International Cosmic Ray Conference (ICRC2017)

21. Linking gamma-ray spectra of supernova remnants to the cosmic ray injection properties in the aftermath of supernovae

22. Radio polarization maps of shell-type SNRs II. Sedov models with evolution of turbulent magnetic field

23. Bridging the gap between supernovae and their remnants through multi-dimensional hydrodynamic modeling

24. Prospects for CTA observations of the young SNR RX J1713.7-3946

25. Contributions of the Cherenkov Telescope Array (CTA) to the 6th International Symposium on High-Energy Gamma-Ray Astronomy (Gamma 2016)

26. Post-adiabatic supernova remnants in the interstellar magnetic field. Parallel and perpendicular shocks

28. Role of ejecta clumping and back-reaction of accelerated cosmic rays in the evolution of Type Ia supernova remnants

29. Hadronic gamma-ray images of Sedov supernova remnants

30. The properties of gamma-ray images of supernova remnants due to proton-proton interactions

31. Constraints on magnetic field strength in the remnant SN1006 from its nonthermal images

32. Role of ejecta clumping and back-reaction of accelerated cosmic rays in the evolution of supernova remnants

33. Constraints on local interstellar magnetic field from non-thermal emission of SN1006

34. Observational constraints on the modeling of SN1006

35. Radio, X-ray and gamma-ray surface brightness profiles as powerful diagnostic tools for non-thermal SNR shells

36. Effects of non-uniform interstellar magnetic field on synchrotron X-ray and inverse-Compton gamma-ray morphology of SNRs

37. A statistical approach to radio emission from shell-type SNRs. I. Basic ideas, techniques, and first results

38. Predicted gamma-ray image of SN 1006 due to inverse Compton emission

39. Thermal emission, shock modification, and X-ray emitting ejecta in SN 1006

40. Some properties of synchrotron radio and inverse-Compton gamma-ray images of supernova remnants

41. Aspect angle for interstellar magnetic field in SN 1006

42. Approximation for radiation power of electrons due to inverse-Compton process in the black-body photon field

43. On the Origin of Asymmetries in Bilateral Supernova Remnants

44. Artificial broadening of the high-energy end of electron spectrum in supernova remnants

45. Influence of Thermalisation on Electron Injection in Supernova Remnant Shocks

46. On the transition of the adiabatic supernova remnant to the radiative stage in a nonuniform interstellar medium

47. Analytic Solutions for the Evolution of Radiative Supernova Remnants

48. Model for Synchrotron Emission from Shell Supernova Remnants in Nonuniform Interstellar Medium and Nonuniform Magnetic Field

49. Thermal X-ray emission of the remnants of ashperical Supernova explosions

50. A New Model for the Thermal X-ray Composites and the Neutral Pion Decay Gamma-Rays from Supernova Remnants

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