CfA Redshift Survey

E550694

The CfA Redshift Survey is a pioneering large-scale galaxy redshift survey that mapped the three-dimensional distribution of galaxies in the nearby universe, revealing major structures such as superclusters and voids.

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Predicate Object
instanceOf astronomical survey
galaxy redshift survey
abbreviationOf Center for Astrophysics Redshift Survey NERFINISHED
aimedTo map the three-dimensional distribution of nearby galaxies
basedAt Harvard College Observatory NERFINISHED
Smithsonian Astrophysical Observatory NERFINISHED
conductedBy Harvard-Smithsonian Center for Astrophysics NERFINISHED
contributedTo constraints on cosmological models
discovery of the cosmic web
evidence for hierarchical structure formation
understanding of galaxy clustering
cosmologicalScale local universe
dataProduct redshift catalog of galaxies
dataType optical spectra of galaxies
field astronomy
cosmology
large-scale structure of the universe
helpedEstablish existence of large cosmic voids
non-uniform distribution of galaxies on large scales
inspired CfA2 Redshift Survey NERFINISHED
subsequent large-scale redshift surveys
locationOfObservation Northern Hemisphere sky
measured galaxy radial velocities
galaxy redshifts
method redshift-distance relation
notableFor detailed maps of galaxy superclusters
first clear evidence of cosmic voids
pioneering large-scale galaxy redshift mapping
observedObjectType galaxies
relatedTo 2dF Galaxy Redshift Survey NERFINISHED
Sloan Digital Sky Survey NERFINISHED
large-scale structure surveys
revealed filamentary large-scale structure
superclusters
voids
surveyType magnitude-limited galaxy survey
targeted nearby galaxies
timePeriod late 20th century
usedFor mapping three-dimensional galaxy distribution
studying supercluster-void network
usedInstrument 1.5-meter Tillinghast telescope NERFINISHED
Multiple Mirror Telescope NERFINISHED
usedTelescopeType optical telescope
uses galaxy redshift measurements

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Perseus–Pisces Supercluster studiedIn CfA Redshift Survey