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<ri:Resource created="2019-08-28T13:26:54Z" 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>High-z galaxy candidates in the HFF cluster fields</title><shortName>J/ApJ/862/156</shortName><identifier>ivo://CDS.VizieR/J/ApJ/862/156</identifier><altIdentifier>doi:10.26093/cds/vizier.18620156</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Leung E.</name></creator><creator><name>Broadhurst T.</name></creator><creator><name>Lim J.</name></creator><creator><name>Diego J.M.</name></creator><creator><name>Chiueh T.</name></creator><creator><name>Schive H.-Y.,Windhorst R.</name></creator><date role="Updated">2021-01-25T12:32:35Z</date><date role="Created">2019-08-28T13:26:54Z</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>galaxies</subject><subject>photometry</subject><subject>redshifted</subject><subject>hst-photometry</subject><subject>infrared-photometry</subject><subject>ultraviolet-astronomy</subject><description>Acting as powerful gravitational lenses, the strong lensing galaxy clusters of the deep Hubble Frontier Fields (HFF) program permit access to lower-luminosity galaxies lying at higher redshifts than hitherto possible. We analyzed the HFF to measure the volume density of Lyman-break galaxies at z&gt;4.75 by identifying a complete and reliable sample up to z~10. A marked deficit of such galaxies was uncovered in the highly magnified regions of the clusters relative to their outskirts, implying that the magnification of the sky area dominates over additional faint galaxies magnified above the flux limit. This negative magnification bias is consistent with a slow rollover at the faint end of the UV luminosity function and it indicates a preference for Bose-Einstein condensate dark matter with a light boson mass of m_B_~10^-22^eV over standard cold dark matter. We emphasize that measuring the magnification bias requires no correction for multiply-lensed images (with typically three or more images per source), whereas directly reconstructing the luminosity function will lead to an overestimate unless such images can be exhaustively matched up, especially at the faint end that is only accessible in the strongly lensed regions. In addition, we detected a distinctive downward transition in galaxy number density at z&gt;~8, which may be linked to the relatively late reionization reported by Planck. Our results suggests that JWST will likely peer into an "abyss" with essentially no galaxies detected in deep NIR imaging at z&gt;10.</description><source format="bibcode">2018ApJ...862..156L</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/862/156</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/VII/4">VII/4 : Abell and Zwicky Clusters of Galaxies (Abell+ 1974)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VII/110">VII/110 : Rich Clusters of Galaxies (Abell+ 1989)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/150/1">J/ApJS/150/1 : VV29 and NGC 4676 HST photometry (Benitez+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/132/926">J/AJ/132/926 : Galaxies in the Hubble Ultra Deep Field (Coe+, 2006)</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/MNRAS/432/2696">J/MNRAS/432/2696 : Galaxy luminosity function at z = 7-9 (McLure+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/793/115">J/ApJ/793/115 : UV-continuum slopes beta for z~4-8 galaxies (Bouwens+, 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/ApJ/803/34">J/ApJ/803/34 : z~4-10 galaxies from HST legacy fields (Bouwens+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/810/71">J/ApJ/810/71 : UV mag of cand. galaxies at 3~&lt;z~&lt;8.5 (Finkelstein+, 2015)</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/819/114">J/ApJ/819/114 : Strong lensing mass modeling of 4 HFF cl. 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