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<ri:Resource created="2013-10-11T09:40:59Z" 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>Massive galaxies in CANDELS-UDS field</title><shortName>J/MNRAS/427/1666</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/427/1666</identifier><altIdentifier>doi:10.26093/cds/vizier.74271666</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Bruce V.A.</name></creator><creator><name>Dunlop J.S.</name></creator><creator><name>Cirasuolo M.</name></creator><creator><name>McLure R.J.</name></creator><creator><name>Targett T.A.,Bell E.F.</name></creator><creator><name>Croton D.J.</name></creator><creator><name>Dekel A.</name></creator><creator><name>Faber S.M.</name></creator><creator><name>Ferguson H.C.</name></creator><creator><name>Grogin N.A.,Kocevski D.D.</name></creator><creator><name>Koekemoer A.M.</name></creator><creator><name>Koo D.C.</name></creator><creator><name>Lai K.</name></creator><creator><name>Lotz J.M.</name></creator><creator><name>McGrath E.J.,Newman J.A.</name></creator><creator><name>van der Wel A.</name></creator><date role="Updated">2024-07-19T20:17:03Z</date><date role="Created">2013-10-11T09:40:59Z</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>galaxies</subject><subject>catalogs</subject><subject>galaxy-classification-systems</subject><description>We have used high-resolution, Hubble Space Telescope, near-infrared imaging to conduct a detailed analysis of the morphological properties of the most massive galaxies at high redshift, modelling the WFC3/IR H_160_-band images of the =~200 galaxies in the CANDELS-UDS field with photometric redshifts 1&lt;z&lt;3, and stellar masses M_*_&gt;10^11^M_{sun}_. We have explored the results of fitting single-Sersic and bulge+disc models, and have investigated the additional errors and potential biases introduced by uncertainties in the background and the on-image point spread function.</description><source format="bibcode">2012MNRAS.427.1666B</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/427/1666</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/II/314">II/314 : UKIDSS-DR8 LAS, GCS and DXS Surveys (Lawrence+ 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/176/301">J/ApJS/176/301 : Subaru/XMM-Newton deep survey IV. 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