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<ri:Resource created="2018-03-21T08:27:17Z" 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/WFC3 obs. of z~2-8 galaxies in 4 HFF clusters</title><shortName>J/ApJ/843/41</shortName><identifier>ivo://CDS.VizieR/J/ApJ/843/41</identifier><altIdentifier>doi:10.26093/cds/vizier.18430041</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Bouwens R.J.</name></creator><creator><name>Illingworth G.D.</name></creator><creator><name>Oesch P.A.</name></creator><creator><name>Atek H.</name></creator><creator><name>Lam D.</name></creator><creator><name>Stefanon M.</name></creator><date role="Updated">2019-08-22T08:53:47Z</date><date role="Created">2018-03-21T08:27:17Z</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>hst-photometry</subject><subject>galaxies</subject><subject>infrared-sources</subject><subject>redshifted</subject><description>We provide the first observational constraints on the sizes of the faintest galaxies lensed by the Hubble Frontier Fields (HFF) clusters. Ionizing radiation from faint galaxies likely drives cosmic reionization, and the HFF initiative provides a key opportunity to find such galaxies. However, we cannot assess their ionizing emissivity without a robust measurement of their sizes, since this is key to quantifying both their prevalence and the faint- end slope to the UV luminosity function. Here we provide the first size constraints with two new techniques. The first utilizes the fact that the detectability of highly magnified galaxies as a function of shear is very dependent on a galaxy's size. Only the most compact galaxies remain detectable in high-shear regions (versus a larger detectable size range for low shear), a phenomenon we quantify using simulations. Remarkably, however, no correlation is found between the surface density of faint galaxies and the predicted shear, using 87 high-magnification ({mu}=10-100) z~2-8 galaxies seen behind the first four HFF clusters. This can only be the case if faint (~-15mag) galaxies have significantly smaller sizes than more luminous galaxies, i.e., &lt;~30mas or 160-240pc. As a second size probe, we rotate and stack 26 faint high-magnification sources along the major shear axis. Less elongation is found even for objects with an intrinsic half-light radius of 10mas. Together, these results indicate that extremely faint z~2-8 galaxies have near point-source profiles (half-light radii &lt;30mas and perhaps 5-10mas). These results suggest smaller completeness corrections and hence shallower faint-end slopes for the z~2-8 LFs than derived in some recent studies (by {Delta}{alpha}&gt;~0.1-0.3).</description><source format="bibcode">2017ApJ...843...41B</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/843/41</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/B/hst">B/hst : HST Archived Exposures Catalog (STScI, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/612/L93">J/ApJ/612/L93 : Candidates of z~5.5-7 galaxies in the HST-UDF (Yan+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/132/1729">J/AJ/132/1729 : HUDF BVI-dropout sources (Beckwith+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/754/83">J/ApJ/754/83 : UV continuum for z~4-7 star-forming gal. (Bouwens+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/756/164">J/ApJ/756/164 : UV galaxies in CANDELS from z=8 to z=4 (Finkelstein+, 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/762/L30">J/ApJ/762/L30 : MCS J0416.1-2403 strong lensing analysis (Zitrin+, 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/800/18">J/ApJ/800/18 : HST/WFC3 obs. of z~7-8 galaxies in A2744 (Atek+, 2015)</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/ApJS/219/15">J/ApJS/219/15 : Morphologies of z=0-10 galaxies with HST (Shibuya+, 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/A+A/590/A31">J/A+A/590/A31 : ASTRODEEP Frontier Fields Catalogues (Merlin+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/835/113">J/ApJ/835/113 : Gal. &gt;~6 from the Hubble Frontier Fields (Livermore+, 2017)</relatedResource></relationship></content><rights>https://cds.unistra.fr/vizier-org/licences_vizier.html</rights><capability><interface xsi:type="vr:WebBrowser"><accessURL use="full">https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJ/843/41</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/843/41</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/843/41</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/843/41</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/843/41</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South 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