Oleg Y. Gnedin
Physics and Astronomy · University of Michigan
Publications
220
Citations
9,150
Est. group size
~7
Recurring co-author estimate
Active years
35
Publishing since 1992
Typically publishes in teams of ~4 · 44% small-team papers (≤3 authors) · across 12 venues
- A Chemodynamical Census of the Milky Way's Ultra-Faint Compact Satellites. I. A First Population-Level Look at the Internal Kinematics and Metallicities of 19 Extremely-Low-Mass Halo Stellar Systems
Open MIND · 2026
- A Chemodynamical Census of the Milky Way's Ultra-Faint Compact Satellites. I. A First Population-Level Look at the Internal Kinematics and Metallicities of 19 Extremely-Low-Mass Halo Stellar Systems
arXiv (Cornell University) · 2026
- To What Extent Are Star Cluster Ages Encoded in Their Environments? Exploring the Spatial Distribution of Age-Related Information with PHANGS-HST Imaging and Convolutional Neural Networks
Open MIND · 2026
- To What Extent Are Star Cluster Ages Encoded in Their Environments? Exploring the Spatial Distribution of Age-Related Information with PHANGS-HST Imaging and Convolutional Neural Networks
arXiv (Cornell University) · 2026
- Characterizing the GD-1 Stream with DESI DR2 Data: Thin Stream and Hot Cocoon
HAL (Le Centre pour la Communication Scientifique Directe) · 2026
- Characterizing the GD-1 Stream with DESI DR2 Data: Thin Stream and Hot Cocoon
arXiv (Cornell University) · 2026
- To What Extent Are Star Cluster Ages Encoded in Their Environments? Exploring the Spatial Distribution of Age-related Information with PHANGS-HST Imaging and Convolutional Neural Networks
The Astrophysical Journal · 2026
- Disentangling the Distant Stellar Halo Using K-Giants in the DESI Year 3 Data
HAL (Le Centre pour la Communication Scientifique Directe) · 2026
- Disentangling the Distant Stellar Halo Using K-Giants in the DESI Year 3 Data
arXiv (Cornell University) · 2026
- Dynamical resonances in PHANGS galaxies
Astronomy and Astrophysics · 2024
- The Star Clusters as Links between Galaxy Evolution and Star Formation Project. I. Numerical Method
The Astrophysical Journal · 2024
- Dynamical resonances in PHANGS galaxies
arXiv (Cornell University) · 2024
- The mass-loss rates of star clusters with stellar-mass black holes: implications for the globular cluster mass function
Monthly Notices of the Royal Astronomical Society · 2023
- The evolution of the globular cluster mass function: The role of stellar-mass black holes
arXiv (Cornell University) · 2023
- Tidal disruption of star clusters in galaxy formation simulations
Monthly Notices of the Royal Astronomical Society · 2022
- arXiv (Cornell University)×32
- Monthly Notices of the Royal Astronomical Society×21
- The Astrophysical Journal×19
- The Astrophysical Journal Letters×5
- HAL (Le Centre pour la Communication Scientifique Directe)×4
- Mario Mateo
Physics and Astronomy · University of Michigan
- Mario Mateo
Physics and Astronomy · University of Michigan
- D. M. Terndrup
Physics and Astronomy · The Ohio State University
- Enrico Vesperini
Physics and Astronomy · Indiana University
- Liam O. Dubay
Physics and Astronomy · The Ohio State University
This profile was generated automatically from public scholarly data (OpenAlex). Group size and activity levels are estimates derived from co-authorship patterns.
Last updated Jul 25, 2026.
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