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<ri:Resource created="2020-06-01T08:33:33Z" 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>SED-selected AGN in the VIPERS field</title><shortName>J/MNRAS/495/1853</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/495/1853</identifier><altIdentifier>doi:10.26093/cds/vizier.74951853</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Pouliasis E.</name></creator><creator><name>Mountrichas G.</name></creator><creator><name>Georgantopoulos I.</name></creator><creator><name>Ruiz A.</name></creator><creator><name>Yang M.,Bonanos A.Z.</name></creator><date role="Updated">2024-08-21T20:14:30Z</date><date role="Created">2020-06-01T08:33:33Z</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>x-ray-sources</subject><subject>redshifted</subject><description>The detection of X-ray emission constitutes a reliable and efficient tool for the selection of active galactic nuclei (AGNs), although it may be biased against the most heavily absorbed AGNs. Simple mid-infrared (IR) broad-band selection criteria identify a large number of luminous and absorbed AGNs, yet again host contamination could lead to non-uniform and incomplete samples. Spectral energy distribution (SED) decomposition is able to decouple the emission from the AGN versus that from star-forming regions, revealing weaker AGN components. We aim to identify the obscured AGN population in the VIMOS Public Extragalactic Redshift Survey in the Canada-France-Hawaii Telescope Legacy Survey W1 field through SED modelling. We construct SEDs for 6860 sources and identify 160 AGNs at a high confidence level using a Bayesian approach. Using optical spectroscopy, we confirm the nature of ~85 per cent of the AGNs. Our AGN sample is highly complete (~92 per cent) compared to mid-IR colour-selected AGNs, including a significant number of galaxy-dominated systems with lower luminosities. In addition to the lack of X-ray emission (80 per cent), the SED fitting results suggest that the majority of the sources are obscured. We use a number of diagnostic criteria in the optical, IR, and X-ray regimes to verify these results. Interestingly, only 35 per cent of the most luminous mid-IR-selected AGNs have X-ray counterparts suggesting strong absorption. Our work emphasizes the importance of using SED decomposition techniques to select a population of type II AGNs, which may remain undetected by either X-ray or IR colour surveys.</description><source format="bibcode">2020MNRAS.495.1853P</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/495/1853</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/317">II/317 : The CFHTLS Survey (T0007 release) (Hudelot+ 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/352">II/352 : The VISTA Hemisphere Survey (VHS) catalog (McMahon+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/328">II/328 : AllWISE Data Release (Cutri+ 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/562/A23">J/A+A/562/A23 : VIMOS Public Extragalactic Survey (VIPERS) DR1 (Garilli+ 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/642/673">J/ApJ/642/673 : IR-selected obscured AGN candidates (Polletta+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/702/441">J/ApJ/702/441 : Obscured active galaxies (Greene+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/740/37">J/ApJ/740/37 : Obscured AGN at z~0.5-1 in the CDFS (Luo+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/556/A114">J/A+A/556/A114 : Obscured AGNs in XMM deep survey in CDF-S</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/814/11">J/ApJ/814/11 : Obscured AGNs from XMM-Newton and AKARI (Terashima+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/618/A66">J/A+A/618/A66 : Redshifts of obscured AGN (Simmonds+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/626/A9">J/A+A/626/A9 : Obscured AGN at 1.5&lt;z&lt;3.0 (Mignoli+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/636/A37">J/A+A/636/A37 : High-z AGN obscured by host galaxy ISM (D'Amato+, 2020)</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/MNRAS/495/1853</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/495/1853</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/495/1853</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL 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