معرفی
Sarah Pearson is an Assistant Professor at the Niels Bohr Institute (University of Copenhagen). Her research focuses on astrophysics, particularly dark matter, stellar streams, galaxy dynamics, and cosmology. She works within the DARK research group and contributes to observational and computational studies of galactic structures.
- Affiliation: Niels Bohr Institute, University of Copenhagen
- Contact: sarah.pearson@nbi.ku.dk | +4535323870
Research Interests
- Dark Matter Halo Structure
- Globular Cluster Dynamics
- Galactic Archaeology
- Extragalactic Stellar Streams
- Galaxy Formation and Evolution
- Observational Cosmology
Recent Publication Trends (2022-2025): Sarah's work emphasizes using stellar streams to probe dark matter distribution, with applications to upcoming telescopes like the Nancy Grace Roman Space Telescope. Her research spans simulations of galaxy mergers, observational studies of tidal features, and methodological advancements in stream detection.
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