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<ri:Resource created="1997-12-09T20:46:44Z" status="active" updated="2025-05-19T09:50:00Z" version="1.2" xmlns:cs="http://www.ivoa.net/xml/ConeSearch/v1.0" xmlns:ri="http://www.ivoa.net/xml/RegistryInterface/v1.0" xmlns:vr="http://www.ivoa.net/xml/VOResource/v1.0" xmlns:vs="http://www.ivoa.net/xml/VODataService/v1.1" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.ivoa.net/xml/ConeSearch/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/ConeSearch.xsd http://www.ivoa.net/xml/VOResource/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/VOResource.xsd http://www.ivoa.net/xml/VODataService/v1.1 http://vo.ari.uni-heidelberg.de/docs/schemata/VODataService.xsd" xsi:type="vs:CatalogService"><title>Redshifts of a sample of distant Abell clusters</title><shortName>J/ApJ/365/66</shortName><identifier>ivo://CDS.VizieR/J/ApJ/365/66</identifier><altIdentifier>doi:10.26093/cds/vizier.13650066</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>HUCHRA J.P.</name></creator><creator><name>HENRY J.P.</name></creator><creator><name>POSTMAN M.</name></creator><creator><name>GELLER M.J.</name></creator><date role="Updated">2013-03-05T06:33:51Z</date><date role="Created">1997-12-09T20:46:44Z</date><contact><name>CDS support team</name><address>CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France</address><email>cds-question@unistra.fr</email></contact></curation><content><subject>surveys</subject><subject>galaxy-clusters</subject><subject>redshifted</subject><description>We have measured redshifts for a complete sample of 145 Abell clusters of galaxies. The sample covers a 561 square degree region at high Galactic latitude. The median redshift of the clusters in the sample is 0.16. For R &gt;= 1 clusters the correlation length is r_0_ = 21 h^-1^ Mpc. The amplitude of the correlation function is a factor of 1.4 less than that obtained by Bahcall and Soneira, but the difference is within the 1 {sigma} uncertainties. In this sample we cannot detect clustering on scales &gt;~ 70 h^-1^ Mpc. Although the maps of the cluster distribution in redshift space show a large void of diameter ~20,000 km s^-1^, frequent occurrence of such large empty regions is consistent with the smaller scale behaviour of the correlation function of the survey. Large-scale peculiar motions are &lt;~1000 km s^-1^. This limit is inconsistent with the claim of detection by Bahcall, Soneira, and Burgett of ~2000 km/s peculiar motions. We suggest that the earlier result is affected by the Corona Borealis supercluster, which contributes more than a third of the excess pairs in the shallower survey. Notes: Some errors have been corrected. 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Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>CluID</name><description>[A] A for "Abell" added at CDS for clarity</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>Anumb</name><description>[909,2013]+ number in the Abell catalogue</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>primary</flag><flag>indexed</flag></column><column><name>RAB1950</name><description>[0,24[ Right ascension (B1950) of the cluster centre</description><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEB1950</name><description>[0,90] declination of the cluster center (B1950)</description><ucd>pos.eq.dec;meta.main</ucd></column><column><name>R</name><description>[0,3] Abell's richness class</description><ucd>src.class.richness</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>D</name><description>[3,7] Abell's distance class</description><ucd>src.class.distance</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>m1</name><description>[13.6,18.3]? brightness of 1st-ranked galaxy from Leir &amp; vandenBergh 1977, ApJS 34, 381 (1),(2)</description><unit>mag</unit><ucd>phot.mag</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>m10</name><description>[15.3,18.4] brightness of 10th-ranked galaxy (1),(2)</description><unit>mag</unit><ucd>phot.mag</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Zest</name><description>[]? estimated redshift (2)</description><ucd>src.redshift</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Zobs</name><description>observed redshift</description><ucd>src.redshift</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Ngal</name><description>[1,16]? number of galaxies with measured z</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>Ref</name><description>reference code(s), see (3)</description><ucd>meta.bib</ucd><dataType xsi:type="vs:VOTableType" arraysize="10*">char</dataType></column><column><name>NOTE</name><description>notes (4)</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="20*">char</dataType></column><column><name>_RA.icrs</name><description>Right ascension (ICRS) (computed by VizieR, not part of the original data)</description><ucd>pos.eq.ra</ucd><flag>nullable</flag><flag>indexed</flag></column><column><name>_DE.icrs</name><description>Declination (ICRS) (computed by VizieR, not part of the original data)</description><ucd>pos.eq.dec</ucd><flag>nullable</flag><flag>indexed</flag></column></table><table><name>J/ApJ/365/66/table2</name><description>Redshifts of individual galaxies</description><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Name</name><description>name of object, either in format hhmm+ddmm appended by A or B for close pairs of galaxies, or N.... for an NGC number</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="10*">char</dataType></column><column><name>RAB1950</name><description>[0,24[? Right ascension (B1950) of galaxy</description><ucd>pos.eq.ra;meta.main</ucd><flag>nullable</flag></column><column><name>DEB1950</name><description>[0,90]? declination (B1950) of galaxy</description><ucd>pos.eq.dec;meta.main</ucd><flag>nullable</flag></column><column><name>Zobs</name><description>[]? observed redshift</description><ucd>src.redshift</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Vhel</name><description>[]? heliocentric radial velocity</description><unit>km/s</unit><ucd>spect.dopplerVeloc;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>Verr</name><description>[]? heliocentric radial velocity error</description><unit>km/s</unit><ucd>stat.error;spect.dopplerVeloc;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>Ref</name><description>reference code(s), see (3)</description><ucd>meta.bib</ucd><dataType xsi:type="vs:VOTableType" arraysize="3*">char</dataType></column><column><name>Abell</name><description>Abell name 'Annnn' or 'Annnn/m', the latter stands for 'Annnn or Annnm' (5) (6)</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="7*">char</dataType></column><column><name>NOTE</name><description>notes as published</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="15*">char</dataType></column><column><name>_RA.icrs</name><description>Right ascension (ICRS) (computed by VizieR, not part of the original data)</description><ucd>pos.eq.ra</ucd><flag>nullable</flag><flag>indexed</flag></column><column><name>_DE.icrs</name><description>Declination (ICRS) (computed by VizieR, not part of the original data)</description><ucd>pos.eq.dec</ucd><flag>nullable</flag><flag>indexed</flag></column></table></schema></tableset></ri:Resource>