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<ri:Resource created="2015-01-13T12:07:53Z" 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>SDSS luminous red galaxies concentrations</title><shortName>J/ApJ/769/52</shortName><identifier>ivo://CDS.VizieR/J/ApJ/769/52</identifier><altIdentifier>doi:10.26093/cds/vizier.17690052</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Wong K.C.</name></creator><creator><name>Zabludoff A.I.</name></creator><creator><name>Ammons S.M.</name></creator><creator><name>Keeton C.R.</name></creator><creator><name>Hogg D.W.,Gonzalez A.H.</name></creator><date role="Updated">2017-10-13T15:42:02Z</date><date role="Created">2015-01-13T12:07:53Z</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>gravitational-lensing</subject><subject>galaxy-clusters</subject><subject>redshifted</subject><subject>galaxies</subject><subject>visible-astronomy</subject><description>The best gravitational lenses for detecting distant galaxies are those with the largest mass concentrations and the most advantageous configurations of that mass along the line of sight. Our new method for finding such gravitational telescopes uses optical data to identify projected concentrations of luminous red galaxies (LRGs). LRGs are biased tracers of the underlying mass distribution, so lines of sight with the highest total luminosity in LRGs are likely to contain the largest total mass. We apply this selection technique to the Sloan Digital Sky Survey and identify the 200 fields with the highest total LRG luminosities projected within a 3.5' radius over the redshift range 0.1&lt;=z&lt;=0.7. The redshift and angular distributions of LRGs in these fields trace the concentrations of non-LRG galaxies. These fields are diverse; 22.5% contain one known galaxy cluster and 56.0% contain multiple known clusters previously identified in the literature. Thus, our results confirm that these LRGs trace massive structures and that our selection technique identifies fields with large total masses. These fields contain two to three times higher total LRG luminosities than most known strong-lensing clusters and will be among the best gravitational lensing fields for the purpose of detecting the highest redshift galaxies.</description><source format="bibcode">2013ApJ...769...52W</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/769/52</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/V/139">V/139 : The SDSS Photometric Catalog, Release 9 (Adelman-McCarthy+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VII/110">VII/110 : Rich Clusters of Galaxies (Abell+ 1989)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VII/190">VII/190 : Zwicky Galaxy Catalog (Zwicky+ 1968)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/199/34">J/ApJS/199/34 : Clusters of galaxies in SDSS-III (Wen+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/757/22">J/ApJ/757/22 : Strong and weak lensing analysis of A2261 (Coe+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/199/25">J/ApJS/199/25 : CLASH sources for MACS1149.6+2223 (Postman+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/191/254">J/ApJS/191/254 : GMBCG galaxy cluster catalog from SDSS DR7 (Hao+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/183/197">J/ApJS/183/197 : Galaxy clusters identified from the SDSS-DR6 (Wen+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/137/4795">J/AJ/137/4795 : Dynamical state of brightest cluster galaxies (Coziol+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/675/234">J/ApJ/675/234 : Mass functions for galaxies 0&lt;z&lt;4 (Perez-Gonzalez+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/660/239">J/ApJ/660/239 : MaxBCG cat. of 13823 SDSS galaxy clusters (Koester+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/379/867">J/MNRAS/379/867 : BCG C4 cluster catalog (Von Der Linden+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/638/725">J/ApJ/638/725 : Fundamental manifold of spheroids (Zaritsky+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/633/174">J/ApJ/633/174 : Spheroidals and bulge dominated galaxies (Treu+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/128/1017">J/AJ/128/1017 : Northern Optical Cluster Survey. 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