Benedikt Diemer

Physics and Astronomy · Physical Sciences

26h-index4.0kcitations97works2.42yr avg
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Research Topics

Galaxies: Formation, Evolution, Phenomena(67), Astronomy and Astrophysical Research(50), Stellar, planetary, and galactic studies(28), Astrophysics and Star Formation Studies(18), Gamma-ray bursts and supernovae(12)

Publications97 total

One Halo, Two Boundaries: Relating Accretion Shocks and Splashback Radii in Galaxy Clusters
arXiv (Cornell University)·2026Open Access
One Halo, Two Boundaries: Relating Accretion Shocks and Splashback Radii in Galaxy Clusters
ArXiv.org·2026Open Access
Distinguishing Orbiting and Infalling Dark Matter Particles with Machine Learning
The Astrophysical Journal·2025Open Access
Lost in the FoG: Pitfalls of Models for Large-scale Hydrogen Distributions
The Astrophysical Journal·2025Open Access
Reaching for the Edge II: Stellar Halos out to Large Radii as a Tracer of Dark Matter Halo Mass
arXiv (Cornell University)·2025Open Access
Relationship between 2D and 3D galaxy stellar mass and correlations with halo mass
Journal of Cosmology and Astroparticle Physics·2025Open Access
The Outskirt Stellar Mass of Low-redshift Massive Galaxies Is an Excellent Halo Mass Proxy in Illustris/IllustrisTNG Simulations
The Astrophysical Journal·2025· 2 citedOpen Access
Distinguishing Orbiting and Infalling Dark Matter Particles with Machine Learning
2025Open Access
ULULA: An ultra-lightweight 2D hydrodynamics code for teaching and experimentation
arXiv (Cornell University)·2025Open Access
A Multiwavelength Technique for Estimating Galaxy Cluster Mass Accretion Rates
The Astrophysical Journal·2025· 1 citedOpen Access
Lost in the FoG: Pitfalls of Models for Large-Scale Hydrogen Distributions
arXiv (Cornell University)·2025Open Access
The mass-dependent UVJ diagram at cosmic noon
Astronomy and Astrophysics·2025· 6 citedOpen Access
Dynamics-based halo model for large scale structure
Physical review. D/Physical review. D.·2025· 3 citedOpen Access
Relationship between 2D and 3D Galaxy Stellar Mass and Correlations with Halo Mass
arXiv (Cornell University)·2025Open Access
The mass-dependent UVJ diagram at cosmic noon: A challenge for galaxy evolution models and dust radiative transfer
arXiv (Cornell University)·2025Open Access
A dynamics-based density profile for dark haloes – III. Parameter space
Monthly Notices of the Royal Astronomical Society·2024· 3 citedOpen Access
A Multi-Wavelength Technique for Estimating Galaxy Cluster Mass Accretion Rates
arXiv (Cornell University)·2024Open Access
The Outskirt Stellar Mass of Low-Redshift Massive Galaxies is an Excellent Halo Mass Proxy in Illustris/IllustrisTNG Simulations
arXiv (Cornell University)·2024Open Access
A dynamics-based density profile for dark haloes -- III. Parameter space
arXiv (Cornell University)·2024Open Access
Haunted haloes: tracking the ghosts of subhaloes lost by halo finders
Monthly Notices of the Royal Astronomical Society·2024· 12 citedOpen Access
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Frequent Co-authors

Dylan Nelson(15), Annalisa Pillepich(14), Lars Hernquist(14), Mark Vogelsberger(12), Federico Marinacci(10), Adam R. H. Stevens(9), Claudia del P. Lagos(7), Paul Torrey(6), Alexie Leauthaud(6), Volker Springel(5), Vicente Rodríguez-Gómez(5), Rüdiger Pakmor(5), Rainer Weinberger(5), Andrey V. Kravtsov(5), Sandro Tacchella(5), Shy Genel(4), Surhud More(4), Toby Brown(4), Enia Xhakaj(4), Eduardo Rozo(3)