Effects of a central dark matter core on time-delay cosmography with galaxy clusters
astro-ph.CO
Submitted: 2026-09-30
Updated: 2026-09-30
Terminology
Sources
- Lower central dark matter densities in nearby galaxies than predicted by simulations
- Massive Galaxy Halos Contain Less Inner Dark Matter Than Predicted
- Planck 2018 results. VI. Cosmological parameters
- A Comprehensive Measurement of the Local Value of the Hubble Constant with 1 km/s/Mpc Uncertainty from the Hubble Space Telescope and the SH0ES Team
- Time-Delay Cosmography: Measuring the Hubble Constant and other cosmological parameters with strong gravitational lensing
- TDCOSMO 2025: Cosmological constraints from strong lensing time delays
- Hubble constant from the cluster-lensed quasar system SDSS J1004+4112: investigation of the lens model dependence
- Hubble Constant Measurement from Three Large-Separation Quasars Strongly Lensed by Galaxy Clusters
- The Frontier Fields Lens Modeling Comparison Project
- Multiple Images of a Highly Magnified Supernova Formed by an Early-Type Cluster Galaxy Lens
- Deja Vu All Over Again: The Reappearance of Supernova Refsdal
- Constraints on the Hubble constant from Supernova Refsdal's reappearance
- Cosmography with Supernova Refsdal through time-delay cluster lensing: independent measurements of the Hubble constant and geometry of the Universe
- Assessing the effect of mass-model assumptions on measuring the Hubble constant from the cluster-lensed supernova Refsdal
- The Hubble constant from the improved lens modeling of cluster-lensed supernova Refsdal with new spectroscopic redshifts and the Jackknife method
- The stellar and dark matter distributions in early-type galaxies measured by stacked weak gravitational lensing
- The Density Profiles of Massive, Relaxed Galaxy Clusters. I. The Total Density Over Three Decades in Radius
- The Density Profiles of Massive, Relaxed Galaxy Clusters. II. Separating Luminous and Dark Matter in Cluster Cores
- Detecting Dark Matter Cores in Galaxy Clusters with Strong Lensing
- A Stringent Upper Limit on Dark Matter Self-Interaction Cross Section from Cluster Strong Lensing
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