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<ri:Resource created="2022-03-03T09:39:42Z" status="active" updated="2025-06-13T15:25:00Z" 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>Spectroscopy of quiescent gal. in 9 lensing clusters</title><shortName>J/ApJ/902/17</shortName><identifier>ivo://CDS.VizieR/J/ApJ/902/17</identifier><altIdentifier>doi:10.26093/cds/vizier.19020017</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Sohn J.</name></creator><creator><name>Fabricant D.G.</name></creator><creator><name>Geller M.J.</name></creator><creator><name>Hwang Ho S.</name></creator><creator><name>Diaferio A.</name></creator><date role="Updated">2023-08-16T15:21:42Z</date><date role="Created">2022-03-03T09:39:42Z</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>redshifted</subject><subject>galaxies</subject><subject>spectroscopy</subject><subject>visible-astronomy</subject><subject>galaxy-kinematics</subject><subject>absolute-magnitude</subject><subject>sloan-photometry</subject><description>We measure the central stellar velocity dispersion function for quiescent galaxies in a set of nine northern clusters in the redshift range 0.18&lt;z&lt;0.29 and with strong lensing arcs in Hubble Space Telescope images. The velocity dispersion function links galaxies directly to their dark matter halos. From dense SDSS and MMT/Hectospec spectroscopy, we identify 222-463 spectroscopic members in each cluster. We derive physical properties of cluster members including redshift, D_n_4000, and central stellar velocity dispersion and we include a table of these measurements for 3419 cluster members. We construct the velocity dispersion functions for quiescent galaxies with D_n_4000&gt;1.5 and within R200. The cluster velocity dispersion functions all show excesses at {sigma}&gt;~250km/s compared to the field velocity dispersion function. The velocity dispersion function slope at large velocity dispersion ({sigma}&gt;160km/s) is steeper for more massive clusters, consistent with the trend observed for cluster luminosity functions. The spatial distribution of galaxies with large velocity dispersion at radii larger than R200 further underscores the probable major role of dry mergers in the growth of massive cluster galaxies during cluster assembly.</description><source format="bibcode">2020ApJ...902...17S</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/902/17</referenceURL><type>Catalog</type><contentLevel>Research</contentLevel><relationship><relationshipType>IsServedBy</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/TAP">TAP VizieR generic service</relatedResource></relationship><relationship><relationshipType>IsServedBy</relationshipType><relatedResource>Conesearch service</relatedResource></relationship><relationship><relationshipType>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/B/hst">B/hst : HST Archived Exposures Catalog (STScI, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/V/154">V/154 : Sloan Digital Sky Surveys (SDSS), Release 16 (DR16) (Ahumada+, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/496/39">J/ApJ/496/39 : Properties of poor groups of galaxies. 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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>RAJ2000</name><description>[9.26/328.4] Right ascension (J2000)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>z</name><description>[0.184/0.288] Redshift</description><ucd>src.redshift</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>DEJ2000</name><description>[-3.53/51.83] Declination (J2000)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column><column><name>Nm</name><description>[222/463] Number of spectroscopically identified members</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>N200</name><description>[117/266] Number of spectroscopic members within R200</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>N200Q</name><description>[92/217] Number of quiescent members (D_n_4000&gt;1.5) within R200</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>N200Qs</name><description>[89/207] Number of quiescent members with a central stellar velocity dispersion measurement</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>R200</name><description>[1.65/2.34] Radius that contains a mean density 200 times larger than the critical density of the universe</description><unit>Mpc</unit><ucd>phys.density;stat.mean</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_R200</name><description>[0.01/0.21] R200 uncertainty</description><unit>Mpc</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>M200</name><description>[6.15/18.42] Mass enclosed within R200</description><unit>1e+14solMass</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_M200</name><description>[0.16/4.2] M200 uncertainty</description><unit>1e+14solMass</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>NED</name><description>NED column added by the CDS</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column></table><table><name>J/ApJ/902/17/table2</name><description>Spectroscopic members</description><column><name>SimbadName</name><description>Simbad column added by the CDS</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="24*">char</dataType><flag>nullable</flag></column><column><name>e_Dn4000</name><description>[0.01/0.9]? Uncertainty in Dn4000</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>sigma</name><description>[31/806]? Velocity Dispersion (2)</description><unit>km/s</unit><ucd>phys.veloc.dispersion</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>e_sigma</name><description>[6/582]? Uncertainty in sigma</description><unit>km/s</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>Cluster</name><description>Name of the cluster</description><ucd>meta.id.parent</ucd><dataType xsi:type="vs:VOTableType" arraysize="7*">char</dataType></column><column><name>objID</name><description>SDSS DR14 object ID of the galaxy member</description><ucd>meta.id;meta.main</ucd></column><column><name>recno</name><description>Record number assigned by the VizieR team. 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