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<ri:Resource created="2022-07-07T14:43:53Z" 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>1959 massive galaxy clusters at high redshifts</title><shortName>J/MNRAS/481/4158</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/481/4158</identifier><altIdentifier>doi:10.26093/cds/vizier.74814158</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Wen Z.L.</name></creator><creator><name>Han J.L.</name></creator><date role="Updated">2024-08-19T20:14:20Z</date><date role="Created">2022-07-07T14:43:53Z</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>galaxy-clusters</subject><subject>galaxies</subject><subject>catalogs</subject><subject>redshifted</subject><subject>photometry</subject><description>We identify a sample of 1959 massive clusters of galaxies in the redshift range of 0.7&lt;z&lt;1.0 from the survey data of Sloan Digital Sky Survey (SDSS) and Wide-field Infrared Survey Explorer (WISE). These clusters are recognized as the overdensity regions of galaxies in the foreground-cleaned WISE data around the SDSS luminous red galaxies, having a richness greater than 15 or an equivalent mass M500&gt;=2.5x10^14^M_{sun}_. Among them, 1505 clusters are identified for the first time, which significantly enlarge the number of high-redshift clusters of z&gt;0.75. By comparing them with clusters at lower redshifts, we confirm that richer clusters host more luminous brightest cluster galaxies (BCGs) also at high redshifts, and that the fraction of blue galaxies is larger in clusters at higher redshifts. A small fraction of BCGs show ongoing star formation or active nuclei. 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36814 36834 36845-36846 36856 36863</spatial><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/MNRAS/481/4158?format=ascii</footprint></coverage><tableset><schema><name>default</name><table><name>J/MNRAS/481/4158/table1</name><description>The 1959 massive clusters of galaxies identified from the SDSS and WISE</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>f_Name</name><description>[WH ] Flag on name (1)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="2*">char</dataType></column><column><name>Name</name><description>Cluster name with J2000 coordinates of cluster</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="16*">char</dataType></column><column><name>RAJ2000</name><description>Right ascension (J2000) of cluster BCG</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>Declination (J2000) of cluster BCG</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column><column><name>z</name><description>Spectroscopic redshift of the cluster</description><ucd>src.redshift</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>imag</name><description>BCG magnitude in i</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>W1mag</name><description>BCG magnitude in W1</description><unit>mag</unit><ucd>phot.mag;em.IR.3-4um</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>SNR</name><description>Signal-to-noise ratio for cluster detection</description><ucd>stat.snr</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>R500</name><description>Cluster radius (2)</description><unit>Mpc</unit><ucd>phys.size.radius</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>L500</name><description>Total W1-band luminosity within R500 in units of L* (3)</description><ucd>phys.luminosity;em.IR</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Rich</name><description>Cluster richness (4)</description><ucd>src.class.richness</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>M500</name><description>Cluster mass within R500 (5)</description><unit>1e+14solMass</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Ngal</name><description>Number of member galaxy candidates within R500</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>OCat</name><description>Other catalogues (6)</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="10*">char</dataType></column></table><table><name>J/MNRAS/481/4158/tablea1</name><description>Parameters of 45 clusters with known mass (M500) from literature</description><column><name>z</name><description>Redshift</description><ucd>src.redshift</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><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>NSeq</name><description>Cluster number sequence</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>RAJ2000</name><description>Right ascension (J2000)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>Declination (J2000)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column><column><name>M500</name><description>Cluster mass</description><unit>1e+14solMass</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_M500</name><description>Error on M500</description><unit>1e+14solMass</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>R500</name><description>Cluster radius</description><unit>Mpc</unit><ucd>phys.size.radius</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_R500</name><description>Error on R500</description><unit>Mpc</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>r_M500</name><description>References for cluster mass (1)</description><ucd>meta.ref;pos.frame</ucd><dataType xsi:type="vs:VOTableType" arraysize="8*">char</dataType></column><column><name>L1Mpc</name><description>W1-band total luminosity within a radius of 1Mpc in units of L* (2)</description><ucd>phys.luminosity;em.IR</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>L500</name><description>Total W1-band luminosity within R500 in units of L* (2)</description><ucd>phys.luminosity;em.IR</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table></schema></tableset></ri:Resource>