| Updated radio relation for Galactic supernova remnants MZ Pavlović, A Dobardžić, B Vukotić, D Urošević arXiv preprint arXiv:1411.2234, 2014 | 67 | 2014 |
| DeepMerge: Classifying high-redshift merging galaxies with deep neural networks A Ćiprijanović, GF Snyder, B Nord, JEG Peek Astronomy and Computing 32, 100390, 2020 | 62 | 2020 |
| DeepMerge–II. Building robust deep learning algorithms for merging galaxy identification across domains A Ćiprijanović, D Kafkes, K Downey, S Jenkins, GN Perdue, S Madireddy, ... Monthly Notices of the Royal Astronomical Society 506 (1), 677-691, 2021 | 51 | 2021 |
| DeepShadows: Separating low surface brightness galaxies from artifacts using deep learning D Tanoglidis, A Ćiprijanović, A Drlica-Wagner Astronomy and Computing 35, 100469, 2021 | 35 | 2021 |
| DeepAdversaries: examining the robustness of deep learning models for galaxy morphology classification. A Ciprijanovic, D Kafkes, GF Snyder, FJ Sánchez, GN Perdue, K Pedro, ... Mach. Learn. Sci. Technol. 3 (3), 35007, 2022 | 18 | 2022 |
| DeepAstroUDA: semi-supervised universal domain adaptation for cross-survey galaxy morphology classification and anomaly detection A Ćiprijanović, A Lewis, K Pedro, S Madireddy, B Nord, GN Perdue, ... Machine Learning: Science and Technology 4 (2), 025013, 2023 | 16 | 2023 |
| Updated radio relation for Galactic supernova remnants -- II B Vukotić, A Ćiprijanović, MM Vučetić, D Onić, D Urošević arXiv preprint arXiv:1912.06379, 2019 | 16 | 2019 |
| DeepGhostBusters: Using Mask R-CNN to detect and mask ghosting and scattered-light artifacts from optical survey images D Tanoglidis, A Ćiprijanović, A Drlica-Wagner, B Nord, MHLS Wang, ... Astronomy and Computing 39, 100580, 2022 | 14 | 2022 |
| DeepAdversaries: examining the robustness of deep learning models for galaxy morphology classification A Ćiprijanović, D Kafkes, G Snyder, FJ Sánchez, GN Perdue, K Pedro, ... Machine Learning: Science and Technology 3 (3), 035007, 2022 | 12 | 2022 |
| Machine learning and cosmology C Dvorkin, S Mishra-Sharma, B Nord, VA Villar, C Avestruz, K Bechtol, ... arXiv preprint arXiv:2203.08056, 2022 | 11 | 2022 |
| Galactic cosmic-ray induced production of lithium in the Small Magellanic Cloud A Ćiprijanović Astroparticle Physics 85, 24-28, 2016 | 10 | 2016 |
| Optical observations of the nearby galaxy IC342 with narrow band [SII] and H filters. I MM Vucetic, B Arbutina, D Urosevic, A Dobardzic, MZ Pavlovic, ... arXiv preprint arXiv:1312.1510, 2013 | 10 | 2013 |
| Diffuse pionic gamma-ray emission from large-scale structures in the Fermi era A Dobardžić, T Prodanović The Astrophysical Journal 782 (2), 109, 2014 | 9 | 2014 |
| Optical observations of the nearby galaxy IC342 with narrow band [SII] and H filters. II - Detection of 16 Optically-Identified Supernova Remnant Candidates MM Vucetic, A Ciprijanovic, MZ Pavlovic, TG Pannuti, N Petrov, UD Goker, ... arXiv preprint arXiv:1511.05307, 2015 | 8 | 2015 |
| Relativistic non-thermal bremsstrahlung radiation V Zeković, B Arbutina, A Dobardžić, MZ Pavlović International Journal of Modern Physics A 28 (29), 1350141, 2013 | 8 | 2013 |
| Optical observations of the nearby galaxy NGC 2366 through narrowband H and SII filters. Supernova remnants status MM Vučetić, D Onić, N Petrov, A Ćiprijanović, MZ Pavlović arXiv preprint arXiv:1902.08671, 2019 | 7 | 2019 |
| DIGS: deep inference of galaxy spectra with neural posterior estimation G Khullar, B Nord, A Ćiprijanović, J Poh, F Xu Machine Learning: Science and Technology 3 (4), 04LT04, 2022 | 6 | 2022 |
| Domain adaptation techniques for improved cross-domain study of galaxy mergers A Ćiprijanović, D Kafkes, S Jenkins, K Downey, GN Perdue, S Madireddy, ... arXiv preprint arXiv:2011.03591, 2020 | 6 | 2020 |
| Neutrino Constraints to the Diffuse Gamma-Ray Emission from Accretion Shocks A Dobardžić, T Prodanović The Astrophysical Journal 806 (2), 184, 2015 | 5 | 2015 |
| The LSST AGN Data Challenge: Selection Methods ĐV Savić, I Jankov, W Yu, V Petrecca, MJ Temple, Q Ni, R Shirley, ... The Astrophysical Journal 953 (2), 138, 2023 | 4 | 2023 |
