Annika H. G. Peter
Physics and Astronomy · The Ohio State University
Publications
220
Citations
6,993
Est. group size
~4
Recurring co-author estimate
Active years
22
Publishing since 2005
Annika H. G. Peter studies dark matter and small galaxies (dwarf galaxies and satellite galaxies of larger galaxies like the Milky Way) to understand what dark matter is made of and how it shapes the structure of the universe. Her work combines observations from telescopes like JWST and the Rubin Observatory with computer simulations of galaxy formation, often focusing on faint, low-mass galaxies and galaxy clusters as natural laboratories for testing dark matter theories.
Publication output has fluctuated over the past decade but shows a generally steady-to-growing pace, with higher annual counts in recent years (2022-2026) compared to a dip around 2020-2021.
Generated by claude-sonnet-5 from public bibliographic data · Jul 20, 2026
- Mapping dark matter in the Bullet Cluster using JWST imaging and spectroscopy
Open MIND · 2026
- Mapping dark matter in the Bullet Cluster using JWST imaging and spectroscopy
ArXiv.org · 2026
- The Merian Survey: A Statistical Census of Bright Satellites of Milky Way Analogs
The Astrophysical Journal · 2026
- $V/σ$ Trends with Mass for Dwarf Galaxies from the Marvelous Massive Dwarfs Suite
arXiv (Cornell University) · 2026
- $V/σ$ Trends with Mass for Dwarf Galaxies from the Marvelous Massive Dwarfs Suite
arXiv (Cornell University) · 2026
- Galaxy Size and Rotation Curve Diversity in ΛCDM with Baryons
The Astrophysical Journal · 2026
- Dwarf Galaxies in the TNG50 Field: connecting their Star-formation Rates with their Environments
The Open Journal of Astrophysics · 2025
- Predictions for the Detectability of Milky Way Satellite Galaxies and Outer-Halo Star Clusters with the Vera C. Rubin Observatory
The Open Journal of Astrophysics · 2025
- Predictions for detecting a turndown in the baryonic Tully–Fisher relation
Monthly Notices of the Royal Astronomical Society · 2025
- A Deep Dive down the Broad-line Region: Permitted O <scp>I</scp> , Ca <scp>II,</scp> and Fe <scp>II</scp> Emission in an Active Galactic Nucleus Little Red Dot at <i>z</i> = 5.3
The Astrophysical Journal Letters · 2025
- The Roman View of Strong Gravitational Lenses
The Astrophysical Journal · 2025
- First Data Release of the Merian Survey: A Wide-field Imaging Survey of Dwarf Galaxies at <i>z</i> ∼ 0.06–0.10
The Astrophysical Journal · 2025
- Star Formation under a Cosmic Microscope: Highly Magnified <i>z</i> = 11 Galaxy behind the Bullet Cluster
The Astrophysical Journal Letters · 2025
- Segue 2 Recently Collided with the Cetus-Palca Stream: New Opportunities to Constrain Dark Matter in an Ultra-faint Dwarf
The Astrophysical Journal · 2025
- Monolithic CFET Flow Improvements Integrating Cover Spacer and Dual-WF RMG
2025
- arXiv (Cornell University)×64
- Monthly Notices of the Royal Astronomical Society×21
- Physical review. D/Physical review. D.×18
- The Astrophysical Journal×17
- AAS×8
- Zhichao Carton Zeng
Physics and Astronomy · The Ohio State University
- Raymond T. Co
Physics and Astronomy · Indiana University
- J. Qin
Physics and Astronomy · Purdue University West Lafayette
- R. F. Lang
Physics and Astronomy · Purdue University West Lafayette
- A. Baxter
Physics and Astronomy · Purdue University West Lafayette
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 19, 2026.
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