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<ri:Resource created="2010-02-10T17:39:44Z" 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>Multiply imaged gravitational lens systems</title><shortName>J/ApJ/668/643</shortName><identifier>ivo://CDS.VizieR/J/ApJ/668/643</identifier><altIdentifier>doi:10.26093/cds/vizier.16680643</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Limousin M.</name></creator><creator><name>Richard J.</name></creator><creator><name>Jullo E.</name></creator><creator><name>Kneib J.-P.</name></creator><creator><name>Fort B.</name></creator><creator><name>Soucail G.,Eliasdottir A.</name></creator><creator><name>Natarajan P.</name></creator><creator><name>Ellis R.S.</name></creator><creator><name>Smail I.</name></creator><creator><name>Czoske O.</name></creator><creator><name>Smith G.P.,Hudelot P.</name></creator><creator><name>Bardeau S.</name></creator><creator><name>Ebeling H.</name></creator><creator><name>Egami E.</name></creator><creator><name>Knudsen K.K.</name></creator><date role="Updated">2017-09-19T14:21:20Z</date><date role="Created">2010-02-10T17:39:44Z</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>galaxy-clusters</subject><subject>redshifted</subject><description>We present a reconstruction of the mass distribution of galaxy cluster Abell 1689 at z=0.18 using detected strong lensing features from deep ACS observations and extensive ground based spectroscopy. Earlier analyses have reported up to 32 multiply imaged systems in this cluster, of which only 3 were spectroscopically confirmed. In this work, we present a parametric strong lensing mass reconstruction using 34 multiply imaged systems of which 24 have newly determined spectroscopic redshifts, which is a major step forward in building a robust mass model. 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