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<ri:Resource created="2026-05-28T08:38:48Z" status="active" updated="2026-06-15T00:00:00Z" 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>Multiple images of Abell 2744 from JWST</title><shortName>J/ApJ/961/186</shortName><identifier>ivo://CDS.VizieR/J/ApJ/961/186</identifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Cha S.</name></creator><creator><name>HyeongHan K.</name></creator><creator><name>Scofield Z.P.</name></creator><creator><name>Joo H.</name></creator><creator><name>Jee M.J.</name></creator><date role="Updated">2026-05-28T07:57:17Z</date><date role="Created">2026-05-28T08:38:48Z</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>infrared-sources</subject><subject>redshifted</subject><subject>galaxy-clusters</subject><description>We present a new high-resolution free-form mass model of A2744 that combines both weak-lensing (WL) and strong-lensing (SL) data sets from JWST. The SL data set comprises 286 multiple images, presenting the most extensive SL constraint to date for a single cluster. The WL data set, employing photo-z selection, yields a source density of ~350arcmin^-2^, marking the densest WL constraint ever. The combined mass reconstruction enables the highest-resolution mass map of A2744 within the ~1.8Mpcx1.8Mpc reconstruction region to date, revealing an isosceles triangular structure with two legs of ~1Mpc and a base of ~0.6Mpc. Although our algorithm, which is called MAximum-entropy ReconStruction (MARS), is entirely blind to the cluster galaxy distribution, the resulting mass reconstruction traces the brightest cluster galaxies remarkably well. The five strongest mass peaks coincide with the five most luminous cluster galaxies within &lt;~2". We do not detect any unusual mass peaks that are not traced by the cluster galaxies, unlike the findings in previous studies. Our mass model shows the smallest scatter of SL multiple images in both source (~0.05") and image (~0.1") planes, which is lower than in previous studies by a factor of ~4. Although MARS represents the mass field with an extremely large number of free parameters (~300000), it converges to a solution within a few hours because we use a deep-learning technique. We make our mass and magnification maps publicly available.</description><source format="bibcode">2024ApJ...961..186C</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/961/186</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/621/53">J/ApJ/621/53 : Multiple arc systems in A1689 (Broadhurst+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/551/A24">J/A+A/551/A24 : GMRT Radio Halo Cluster Survey sources (Venturi+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/564/A125">J/A+A/564/A125 : AGN Torus model comparison of AGN in CDFS (Buchner+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/444/268">J/MNRAS/444/268 : HST Frontier Fields clusters (Richard+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/452/1437">J/MNRAS/452/1437 : Abell 2744 strong-lensing analysis (Jauzac+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/811/29">J/ApJ/811/29 : GLASS. IV. Lensing cluster Abell 2744 (Wang+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/801/44">J/ApJ/801/44 : HST lensing analysis of the CLASH sample (Zitrin+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/819/114">J/ApJ/819/114 : Strong lensing mass modeling (Kawamata+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/473/663">J/MNRAS/473/663 : MUSE and HFFs Photometry of A2744 (Mahler+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/485/3738">J/MNRAS/485/3738 : 3D structure in the A370 MUSE Mosaic (Lagattuta+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/646/A57">J/A+A/646/A57 : VLT/MUSE MACS J0416.1-2403 redshift cat. 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