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<ri:Resource created="2024-05-06T13:25:06Z" status="active" updated="2026-02-10T20:05:23Z" 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>MMT/Hectospec spectra of ACO 1489</title><shortName>J/ApJ/930/156</shortName><identifier>ivo://CDS.VizieR/J/ApJ/930/156</identifier><altIdentifier>doi:10.26093/cds/vizier.19300156</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Rines K.J.</name></creator><creator><name>Sohn J.</name></creator><creator><name>Geller M.J.</name></creator><creator><name>Diaferio A.</name></creator><date role="Updated">2026-02-10T20:05:23Z</date><date role="Created">2024-05-06T13:25:06Z</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>visible-astronomy</subject><subject>spectroscopy</subject><subject>redshifted</subject><subject>surveys</subject><subject>galaxy-kinematics</subject><subject>photometry</subject><subject>two-color-diagrams</subject><description>We discuss a spectroscopic survey of the strong lensing cluster A1489 that includes redshifts for 195 cluster members along with central velocity dispersions for 188 cluster members. The caustic technique applied to the redshift survey gives the dynamical parameters M_200_=(1.25+/-0.09)x10^15^M_{sun}_, R_200_=1.97+/-0.05Mpc, and a cluster line-of-sight velocity dispersion of 1150+/-72km/s within R_200_. These parameters are very similar to those of other strong lensing systems with comparably large Einstein radii. We use the spectroscopy and deep photometry to demonstrate that A1489 is probably dynamically active; its four brightest cluster galaxies have remarkably different rest-frame radial velocities. Like other massive strong lensing clusters, the velocity dispersion function for members of A1489 shows an excess for dispersions &gt;~250km/s. The central dispersions also provide enhanced constraints on future lensing models.</description><source format="bibcode">2022ApJ...930..156R</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/930/156</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/VII/4">VII/4 : Abell and Zwicky Clusters of Galaxies (Abell+ 1974)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/282">II/282 : The SDSS Photometric Catalog, Release 6 (Adelman-McCarthy+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VIII/91">VIII/91 : Planck Catalog of Compact Sources Release 1 (Planck, 2013)</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/VII/292">VII/292 : DESI Legacy Imaging Surveys DR8 photometric redshifts (Duncan, 2022)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/132/1275">J/AJ/132/1275 : CIRS (Cluster Infall Regions in the SDSS). 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