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<ri:Resource created="2011-09-30T12:04:11Z" 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>AGNs in the Extended Groth Strip Survey</title><shortName>J/AJ/137/179</shortName><identifier>ivo://CDS.VizieR/J/AJ/137/179</identifier><altIdentifier>doi:10.26093/cds/vizier.51370179</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Ramos Almeida C.</name></creator><creator><name>Rodriguez Espinosa J.M.</name></creator><creator><name>Barro G.</name></creator><creator><name>Gallego J.,Perez-Gonzalez P.G.</name></creator><date role="Updated">2017-07-11T13:09:04Z</date><date role="Created">2011-09-30T12:04:11Z</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>active-galactic-nuclei</subject><subject>galaxies</subject><subject>infrared-sources</subject><subject>ultraviolet-astronomy</subject><subject>x-ray-sources</subject><description>We have employed a reliable technique of classification of active galactic nuclei (AGNs) based on the fit of well sampled spectral energy distributions (SEDs) with a complete set of AGN and starburst galaxy templates. We have compiled UV, optical, and IR data for a sample of 116 AGNs originally selected for their X-ray and mid-IR emissions (96 with single detections and 20 with double optical counterparts). This is the most complete compilation of multiwavelength data for such a large sample of AGN in the Extended Groth Strip. 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