Linked from

The 18 pages that link to Galaxy redshift survey, each with the reason it gives.

• Cosmic webRelated: Redshift surveys reveal the web’s galaxy distribution across cosmic distances.

• Large-scale structure of the universeRelated: Redshift surveys expose the filaments, clusters, and voids across large volumes.

• Radial velocityRelated: Radial motions contribute to the redshifts used to map large-scale galaxy distributions.

• Comoving distanceRelated: Redshift maps become three-dimensional distributions when interpreted with comoving distances.

• Great AttractorRelated: Redshift surveys traced structures in the obscured region and refined the attractor's location.

• Galaxy filamentRelated: Survey maps reveal the elongated galaxy patterns used to identify filaments.

• Field galaxyRelated: Redshift surveys identify cluster membership and isolate galaxies in lower-density surroundings.

• Large quasar groupRelated: Survey design and sampling determine which apparent quasar concentrations can be detected.

• Local SheetRelated: Redshift surveys supply distances and motions used to map the Local Sheet.

• Tired lightRelated: Their patterns reveal time-dependent cosmic structure beyond a redshift–distance relation alone.

• 2MASSRelated: 2MASS galaxy positions and magnitudes helped define targets for infrared-selected redshift surveys.

• Local HoleRelated: Redshift surveys provide the three-dimensional galaxy counts used to identify nearby underdensities.

• Recessional velocityRelated: Survey redshifts map large-scale recession patterns and cosmic structure.

• Sandra FaberRelated: Redshift surveys let Faber and collaborators map galaxy distributions and large-scale flows.

• South Pole WallRelated: Survey data revealed the wall as a connected concentration rather than isolated galaxies.