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<ri:Resource created="2012-03-21T12:33:22Z" 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>EROs in Groth Strip</title><shortName>J/MNRAS/414/2246</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/414/2246</identifier><altIdentifier>doi:10.26093/cds/vizier.74142246</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Hempel A.</name></creator><creator><name>Cristobal-Hornillos D.</name></creator><creator><name>Prieto M.</name></creator><creator><name>Trujillo I.</name></creator><creator><name>Balcells M.,Lopez-Sanjuan C.</name></creator><creator><name>Abreu D.</name></creator><creator><name>Eliche-Moral M.C.</name></creator><creator><name>Dominguez-Palmero L.</name></creator><date role="Updated">2024-07-14T20:14:58Z</date><date role="Created">2012-03-21T12:33:22Z</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>infrared-sources</subject><subject>galaxies</subject><subject>photometry</subject><subject>galaxy-classification-systems</subject><description>We present a new catalogue of EROs from the Groth Strip and study the relation between their morphology and mass. With a selection criterion F814W-Ks&gt;=4 and Ks&lt;=21.0 we find 102 EROs, over a survey area of 155 arcmin2, leading to a surface density of 0.66arcmin^-2^. The photometric data include U, B, F606W, F814W, J, Ks bands. Morphologies are based on a by eye classification and we distinguish between three basic classes: compact objects, targets with a disc and/or a bulge component and irregular or merger candidates. An additional group consists of the few objects which could not be classified.</description><source format="bibcode">2011MNRAS.414.2246H</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/414/2246</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/581/844">J/ApJ/581/844 : Radio and Infrared observations of EROs (Smail+, 2002)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/330/1">J/MNRAS/330/1 : HST observations of Extremely Red Objects (Smith+, 2002)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/PASJ/55/1079">J/PASJ/55/1079 : BVRi'z'JHKs photometry of ERO objects (Miyazaki+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/346/1125">J/MNRAS/346/1125 : Faint Extremely Red Objects IK photometry (Gilbank+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/432/69">J/A+A/432/69 : Extremely Red Objects XMM-Newton observations (Brusa+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/627/621">J/ApJ/627/621 : Catalog of Extremely Red Objects (Sawicki+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/361/525">J/MNRAS/361/525 : Las Campanas Infrared Survey. 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