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<ri:Resource created="2016-04-20T15:06:52Z" 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>HST Frontier Fields clusters</title><shortName>J/MNRAS/444/268</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/444/268</identifier><altIdentifier>doi:10.26093/cds/vizier.74440268</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Richard J.</name></creator><creator><name>Jauzac M.</name></creator><creator><name>Limousin M.</name></creator><creator><name>Jullo E.</name></creator><creator><name>Clement B.</name></creator><creator><name>Ebeling H.,Kneib J.-P.</name></creator><creator><name>Atek H.</name></creator><creator><name>Natarajan P.</name></creator><creator><name>Egami E.</name></creator><creator><name>Livermore R.</name></creator><creator><name>Bower R.</name></creator><date role="Updated">2024-08-10T20:18:47Z</date><date role="Created">2016-04-20T15:06:52Z</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>gravitational-lensing</subject><subject>redshifted</subject><description>Extending over three Hubble Space Telescope (HST) cycles, the Hubble Frontier Fields (HFF) initiative constitutes the largest commitment ever of HST time to the exploration of the distant Universe via gravitational lensing by massive galaxy clusters. Here, we present models of the mass distribution in the six HFF cluster lenses, derived from a joint strong- and weak-lensing analysis anchored by a total of 88 multiple-image systems identified in existing HST data. The resulting maps of the projected mass distribution and of the gravitational magnification effectively calibrate the HFF clusters as gravitational telescopes. Allowing the computation of search areas in the source plane, these maps are provided to the community to facilitate the exploitation of forthcoming HFF data for quantitative studies of the gravitationally lensed population of background galaxies. Our models of the gravitational magnification afforded by the HFF clusters allow us to quantify the lensing-induced boost in sensitivity over blank-field observations and predict that galaxies at z&gt;10 and as faint as m(AB)=32 will be detectable, up to 2mag fainter than the limit of the Hubble Ultra Deep Field.</description><source format="bibcode">2014MNRAS.444..268R</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/444/268</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/ApJ/800/18">J/ApJ/800/18 : HST/WFC3 observations of z~7-8 galaxies in A2744 (Atek+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/811/29">J/ApJ/811/29 : GLASS. 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