The MAGPI Survey: co-evolution of baryons and dark matter in star-forming disk-like galaxies at 0.1 z 0.85
The MAGPI survey analyzed dark matter content in star-forming disk galaxies at intermediate redshifts (0.1 to 0.85) using kinematic data to study baryon and dark matter co-evolution. Findings show low-mass galaxies are strongly DM dominated, while high-mass systems have lower DM fractions in their centers, suggesting mass-dependent structural differences driven by internal processes.