| New mass bound on fermionic dark matter from a combined analysis of classical dSphs D Savchenko, A Rudakovskyi Monthly Notices of the Royal Astronomical Society 487 (4), 5711-5720, 2019 | 42 | 2019 |
| Constraints on warm dark matter from UV luminosity functions of high-z galaxies with Bayesian model comparison A Rudakovskyi, A Mesinger, D Savchenko, N Gillet Monthly Notices of the Royal Astronomical Society 507 (2), 3046-3056, 2021 | 31 | 2021 |
| 21-cm observations and warm dark matter models A Boyarsky, D Iakubovskyi, O Ruchayskiy, A Rudakovskyi, W Valkenburg Physical Review D 100 (12), 123005, 2019 | 30 | 2019 |
| Dark matter profiles of SPARC galaxies: a challenge to fuzzy dark matter M Khelashvili, A Rudakovskyi, S Hossenfelder Monthly Notices of the Royal Astronomical Society 523 (3), 3393-3405, 2023 | 14 | 2023 |
| Influence of∼ 7 keV sterile neutrino dark matter on the process of reionization A Rudakovskyi, D Iakubovskyi Journal of Cosmology and Astroparticle Physics 2016 (06), 017, 2016 | 12 | 2016 |
| Can EDGES observation favour any dark matter model? A Rudakovskyi, D Savchenko, M Tsizh Monthly Notices of the Royal Astronomical Society 497 (3), 3393-3399, 2020 | 8 | 2020 |
| Dark matter model favoured by reionization data: 7 keV sterile neutrino versus cold dark matter A Rudakovskyi, D Iakubovskyi Monthly Notices of the Royal Astronomical Society 483 (3), 4080-4084, 2019 | 4 | 2019 |
| New model of density distribution for fermionic dark matter halos A Rudakovskyi, D Savchenko arXiv preprint arXiv:1908.11196, 2019 | 2 | 2019 |
| SPARC galaxies prefer Dark Matter over MOND M Khelashvili, A Rudakovskyi, S Hossenfelder arXiv preprint arXiv:2401.10202, 2024 | | 2024 |
Denys SavchenkoBogolyubov Institute for Theoretical Physicsbitp.kiev.ua üzerinde doğrulanmış e-posta adresine sahip
