The Role of the Third Dredge-up and Mass Loss in Shaping the Initial–Final Mass Relation of White Dwarfs F Addari, P Marigo, A Bressan, G Costa, K Shepherd, G Volpato The Astrophysical Journal 964 (1), 51, 2024 | 7 | 2024 |
Grids of stellar models with rotation-VIII. Models from 1.7 to 500 M⊙ at metallicity Z= 10− 5 Y Sibony, KG Shepherd, N Yusof, R Hirschi, C Chambers, S Tsiatsiou, ... Astronomy & Astrophysics 690, A91, 2024 | 5 | 2024 |
The cosmic rate of pair-instability supernovae F Gabrielli, A Lapi, L Boco, C Ugolini, G Costa, C Sgalletta, K Shepherd, ... Monthly Notices of the Royal Astronomical Society 534 (1), 151-172, 2024 | 3 | 2024 |
Evolutionary tracks, ejecta, and ionizing photons from intermediate-mass to very massive stars with PARSEC G Costa, KG Shepherd, A Bressan, F Addari, Y Chen, X Fu, G Volpato, ... arXiv preprint arXiv:2501.12917, 2025 | | 2025 |
Evolution and final fates of low-and intermediate-mass stars A Bressan, KG Shepherd arXiv preprint arXiv:2412.13039, 2024 | | 2024 |
Grids of stellar models with rotation VIII: Models from 1.7 to 500 at metallicity Y Sibony, KG Shepherd, N Yusof, R Hirschi, C Chambers, S Tsiatsiou, ... arXiv preprint arXiv:2407.06739, 2024 | | 2024 |
The role of mixing, rotation and mass-loss in stellar evolution A Bressan, F Addari, G Costa, CT Nguyen, KG Shepherd, G Volpato, X Fu, ... EAS2024, 2572, 2024 | | 2024 |
Very massive stars chemical enrichment in extremely metal-poor galaxies A Bressan, G Costa, S Goswami, V Grisoni, KG Shepherd, L Silva, ... Memorie della Società Astronomica Italiana Journal of the Italian …, 2023 | | 2023 |
Discovery of a New Massive ZZ Ceti Star KG Shepherd, W Hall, BG Castanheira Research Notes of the AAS 6 (5), 107, 2022 | | 2022 |
White Dwarf Stars Observed with NASA's Kepler & K2 Space Telescope K Shepherd, W Hall, B Castanheira Endl PhD Bulletin of the American Physical Society, 2021 | | 2021 |
Grids of stellar models with rotation Y Sibony, KG Shepherd, N Yusof, R Hirschi, C Chambers, S Tsiatsiou, ... Astronomy & Astrophysics 690, 0 | | |