| 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 |
| Testing the origin of~ 3.55 keV line in individual galaxy clusters observed with XMM-Newton D Iakubovskyi, E Bulbul, AR Foster, D Savchenko, V Sadova arXiv preprint arXiv:1508.05186, 2015 | 39 | 2015 |
| UkrVO Astroinformatics Software and Web-services IB Vavilova, YS Yatskiv, LK Pakuliak, IL Andronov, VM Andruk, ... Proceedings of the International Astronomical Union 12 (S325), 361-366, 2016 | 37 | 2016 |
| 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 | 36 | 2021 |
| Hint for a TeV neutrino emission from the Galactic Ridge with ANTARES A Albert, S Alves, M André, M Ardid, S Ardid, JJ Aubert, J Aublin, B Baret, ... Physics Letters B, 137951, 2023 | 31 | 2023 |
| Technical comment on the paper of Dessert et al." The dark matter interpretation of the 3.5 keV line is inconsistent with blank-sky observations" A Boyarsky, D Malyshev, O Ruchayskiy, D Savchenko arXiv preprint arXiv:2004.06601, 2020 | 27 | 2020 |
| Hard-Core Radius of Nucleons within the Induced Surface Tension Approach KA Bugaev, AI Ivanytskyi, VV Sagun, BE Grinyuk, DO Savchenko, ... Universe 5 (2), 63, 2019 | 18 | 2019 |
| Surface brightness profile of the 3.5 keV line in the Milky Way halo A Boyarsky, D Iakubovskyi, O Ruchayskiy, D Savchenko arXiv preprint arXiv:1812.10488, 2018 | 15 | 2018 |
| Neutrino Signal from a Population of Seyfert Galaxies A Neronov, D Savchenko, DV Semikoz Physical Review Letters 132 (10), 101002, 2024 | 13 | 2024 |
| On separate chemical freeze-outs of hadrons and light (anti) nuclei in high energy nuclear collisions KA Bugaev, BE Grinyuk, AI Ivanytskyi, VV Sagun, DO Savchenko, ... Journal of Physics: Conference Series 1390 (1), 012038, 2019 | 11 | 2019 |
| 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 |
| Possible signals of two QCD phase transitions at NICA-FAIR energies KA Bugaev, AI Ivanytskyi, VV Sagun, BE Grinyuk, DO Savchenko, ... EPJ Web of Conferences 204, 03001, 2019 | 7 | 2019 |
| Energy-dependent periodicities of LS I+ 61° 303 in the GeV band M Chernyakova, D Malyshev, A Neronov, D Savchenko Monthly Notices of the Royal Astronomical Society 525 (2), 2202-2207, 2023 | 3 | 2023 |
| Identification of the~ 3.55 keV emission line candidate objects across the sky D Savchenko, D Iakubovskyi Advances in Astronomy and Space Physics 5 (2), 89-92, 2015 | 3 | 2015 |
| Creation of 2-5 keV and 5-10 keV sky maps using XMM-Newton data D Savchenko, D Iakubovskyi Advances in Astronomy and Space Physics 4 (1-2), 51-53, 2014 | 3 | 2014 |
| Neutrino signal from Cygnus region of the Milky Way A Neronov, D Semikoz, D Savchenko Physical Review D 110 (4), 043024, 2024 | 2 | 2024 |
| New Model of Density Distribution for Fermionic Dark Matter Halos AV Rudakovskyi, DO Savchenko Ukrainian Journal of Physics 63 (9), 769-776, 2018 | 2 | 2018 |
| The study of x-ray spectrum of the Coma cluster L Zadorozhna, A Tugay, O Prikhodko, D Malyshev, Y Sahai, D Savchenko, ... arXiv preprint arXiv:2311.08603, 2023 | 1 | 2023 |
| The Study of X-Ray Spectrum of Coma Galaxy Cluster L Zadorozhna, A Tugay, O Prikhodko, D Malyshev, Y Sahai, D Savchenko, ... Odessa Astronomical Publications 36, 37, 2023 | 1 | 2023 |
| Towards Robust Detection of a Faint Narrow Line in X-Rays – the Role of Continuum-Induced Systematics D Savchenko, D Iakubovskyi Ukr. J. Phys. 62 (7), 642-649, 2017 | 1 | 2017 |
Dmytro IakubovskyiBogolyubov Institute for Theoretical Physics, Kyiv, UkraineVerified email at bitp.kiev.ua
