Linked from

The 22 pages that link to Weak gravitational lensing, each with the reason it gives.

• Dark matter haloRelated: Statistical lensing measurements estimate halo masses without requiring visible tracers.

• Lambda-CDM modelRelated: It maps matter clustering and tests predictions for structure growth.

• Cosmic webRelated: It maps dark matter in filaments even where galaxies provide few visible tracers.

• Galaxy rotation curveRelated: It independently probes galaxy mass beyond what rotation curves measure.

• Large-scale structure of the universeRelated: Lensing maps the web's total mass, including invisible dark matter.

• Cosmic voidRelated: Lensing estimates the dark matter deficits inside and around voids.

• Circumgalactic mediumRelated: It maps the halo mass that confines circumgalactic gas, complementing gas observations.

• Euclid (space telescope)Related: Euclid maps these distortions to infer the distribution of matter across cosmic time.

• Galaxy filamentRelated: Lensing can help map filament mass, including dark matter that emits no light.

• Cosmological parametersRelated: The distortions probe matter clustering and combinations of cosmological parameters.

• Dark Energy SurveyRelated: DES used these distortions to map matter and test structure growth.

• Subaru TelescopeRelated: Subaru imaging measures these distortions to reconstruct cosmic mass distributions.

• Structure formationRelated: It maps mass growth even where dark matter emits no light.

• Galaxy groups and clustersRelated: Statistical lensing measurements estimate cluster masses without relying on visible matter.

• Giant VoidRelated: Lensing measurements estimate the otherwise faint matter inside and around voids.