Testing subhalo abundance matching with galaxy kinematics

arXiv:2601.07799 · astro-ph.GA, astro-ph.CO · Submitted 2026-01-12 · Read on arXiv

astro-ph.GA, astro-ph.CO

Submitted: 2026-01-12

Updated: 2026-01-12

Terminology

• Clustering — 45× in this paper · explained in 2 episodes
• Abundance — 18× in this paper · explained in 1 episode
• Consistency — 9× in this paper · explained in 3 episodes
• Trace — 5× in this paper · explained in 2 episodes
• Core — 2× in this paper · explained in 2 episodes
• Accuracy — 1× in this paper · explained in 1 episode
• Alignment — 1× in this paper · explained in 1 episode
• Aperture — 1× in this paper · explained in 1 episode
• Aperture Photometry — 1× in this paper · explained in 1 episode
• Baryonic Feedback — 1× in this paper · explained in 3 episodes
• Bayesian Framework — 1× in this paper · explained in 3 episodes
• Metallicity — 1× in this paper · explained in 3 episodes
• NASA-Sloan Atlas2 — 1× in this paper
• Population Synthesis — 1× in this paper · explained in 2 episodes
• Post-Selection — 1× in this paper · explained in 2 episodes
• Simulation-based Inference — 1× in this paper · explained in 2 episodes
• Sloan Digital Sky Survey — 1× in this paper
• Velocity Dispersion — 1× in this paper · explained in 2 episodes
• Weak Lensing — 1× in this paper · explained in 2 episodes

Sources

• Exploring Neutral Hydrogen and Galaxy Evolution with the SKA
• Modified Newtonian Dynamics: Observational Successes and Failures
• Modified Newtonian Dynamics (MOND)
• Halo Contraction Effect in Hydrodynamic Simulations of Galaxy Formation
• Understanding Place Identity with Generative AI
• The MeerKAT International GHz Tiered Extragalactic Exploration (MIGHTEE) Survey
• The Milky Way satellite velocity function is a sharp probe of small-scale structure problems
• BASILISK III. Stress-testing the Conditional Luminosity Function model
• Differential Music: Automated Music Generation Using LSTM Networks with Representation Based on Melodic and Harmonic Intervals

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