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<ri:Resource created="2011-02-18T07:54:23Z" 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>Lensed-arc statistics of galaxy clusters</title><shortName>J/MNRAS/406/1318</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/406/1318</identifier><altIdentifier>doi:10.26093/cds/vizier.74061318</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Horesh A.</name></creator><creator><name>Maoz D.</name></creator><creator><name>Ebeling H.</name></creator><creator><name>Seidel G.</name></creator><creator><name>Bartelmann M.</name></creator><date role="Updated">2024-07-11T20:16:59Z</date><date role="Created">2011-02-18T07:54:23Z</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>x-ray-sources</subject><subject>redshifted</subject><subject>hst-photometry</subject><description>The statistics of strongly lensed arcs in samples of galaxy clusters provide information on cluster structure that is complementary to that from individual clusters. However, samples of clusters that have been analysed to date have been either small, heterogeneous or observed with limited angular resolution. We measure the lensed-arc statistics of 97 clusters imaged at high angular resolution with the Hubble Space Telescope, identifying lensed arcs using two automated arc-detection algorithms. The sample includes similar numbers of X-ray-selected [MAssive Cluster Survey (MACS)] and optically selected [Red-Sequence Cluster Survey (RCS)] clusters, and spans cluster redshifts in the range 0.2&lt;z&lt;1. We compile a catalogue of 42 arcs in the X-ray-selected subsample and seven arcs in the optical subsample. All but five of these arcs are reported here for the first time.</description><source format="bibcode">2010MNRAS.406.1318H</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/406/1318</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/J/MNRAS/339/913">J/MNRAS/339/913 : Two distant massive clusters of galaxies (Edge+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/157/1">J/ApJS/157/1 : Red-Sequence Cluster Survey (Gladders+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/158/161">J/ApJS/158/161 : 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Mass enclosed within r200 (2)</description><unit>1e+15solMass</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Simbad</name><description>Simbad column added by the CDS</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column><column><name>NED</name><description>NED column added by the CDS</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column></table><table><name>J/MNRAS/406/1318/rcs</name><description>RCS (Red-Sequence Cluster Survey) low (0.3&lt;=z&lt;0.5), medium (0.5&lt;=z&lt;0.7) and high (0.7&lt;=z&lt;=1) redshift samples (tables 3, 4 and 5 of paper)</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. 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