An Optically Based Search for Distant Galaxy Clusters

dc.contributor.authorLidman, Christopher E.en
dc.contributor.authorPeterson, Bruce A.en
dc.date.accessioned2026-01-01T13:41:28Z
dc.date.available2026-01-01T13:41:28Z
dc.date.issued1996en
dc.description.abstractWe describe an automated, optically based search for distant galaxy clusters. The search covers 13 square degrees of deep I-band CCD data from which we present a catalogue of 105 candidates. Half of the candidates from this search are expected to be as rich as Abell richness class zero. These Abell-like clusters are expected to have a median redshift greater than z = 0.5. The other half are likely to be poorer clusters or chance overdensities.en
dc.description.statusPeer-revieweden
dc.identifier.otherBibtex:1996AJ....112.2454Len
dc.identifier.scopus0002043640en
dc.identifier.urihttps://hdl.handle.net/1885/733800696
dc.language.isoenen
dc.sourceajen
dc.subjectGALAXIES: CLUSTERINGen
dc.subjectCATALOGSen
dc.subjectEARLY UNIVERSEen
dc.titleAn Optically Based Search for Distant Galaxy Clustersen
dc.typeJournal articleen
dspace.entity.typePublicationen
local.bibliographicCitation.lastpage2470en
local.bibliographicCitation.startpage2454en
local.contributor.affiliationLidman, Christopher E.; RSAA Academic Program, Research School of Astronomy & Astrophysics, ANU College of Science and Medicine, The Australian National Universityen
local.contributor.affiliationPeterson, Bruce A.; RSAA Academic Program, Research School of Astronomy & Astrophysics, ANU College of Science and Medicine, The Australian National Universityen
local.identifier.citationvolume112en
local.identifier.doi10.1086/118195en
local.identifier.pure86c3d725-b86c-4122-a806-75796d782001en
local.identifier.urlhttps://www.scopus.com/pages/publications/0002043640en
local.type.statusPublisheden

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