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<ri:Resource created="2025-02-18T09:19:32Z" status="active" updated="2025-05-21T20:01:49Z" 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>Identifying CT-AGNs in the COSMOS. I.</title><shortName>J/A+A/694/A241</shortName><identifier>ivo://CDS.VizieR/J/A+A/694/A241</identifier><altIdentifier>doi:10.26093/cds/vizier.36940241</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Guo X.</name></creator><creator><name>Gu Q.</name></creator><creator><name>Fang G.</name></creator><creator><name>Chen Y.</name></creator><creator><name>Ding N.</name></creator><creator><name>Yu X.</name></creator><creator><name>Wang H.</name></creator><date role="Updated">2025-05-21T20:01:49Z</date><date role="Created">2025-02-18T09:19:32Z</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>x-ray-sources</subject><description>Compton-thick active galactic nuclei (CT-AGNs), characterized by a significant absorption with column densities of N_H_&gt;=1.5x10^24^cm^-2^, emit feeble X-ray radiation, even undetectable by X-ray instruments, making them difficult to identify. The X-ray radiations from AGNs are the predominant origin of the cosmic X-ray background (CXB). Based on the AGN synthesis models for the CXB, the fraction of CT-AGNs should constitute a substantial portion, approximately 30% or more. The fraction of CT-AGNs discovered in the Cosmological Evolution Survey (COSMOS) is significantly lower than this value. These mean that many CT-AGNs may be hidden in AGNs that exhibit low photon counts or that have not been detected by X-ray instruments. This work focuses on identifying CT-AGNs hidden in AGNs with low photon counts. Firstly, we selected 440 AGNs with abundant multiwavelength data as our sample. Secondly, we analyzed multiwavelength data, extracting crucial physical parameters required for the CT-AGN diagnosis. Finally, we used the multiwavelength approaches to identify CT-AGNs. We have successfully identified 18 CT-AGNs in our sample. Among the CT-AGNs, four AGNs showed discrepant results across different diagnostic methods. We discussed the potential reasons behind these diagnostic discrepancies. We explored the impact of estimating [OIII]{lambda}5007 luminosities based on [OII]{lambda}3727 luminosities for the CT-AGN diagnosis. We also found that the properties of host galaxies for CT-AGNs and non-CT-AGNs did not show significant discrepancies.</description><source format="bibcode">2025A&amp;A...694A.241G</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/694/A241</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/819/62">J/ApJ/819/62 : The COSMOS-Legacy Survey (CLS) catalog (Civano+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/817/34">J/ApJ/817/34 : C-COSMOS Legacy sources multiwavelength catalog (Marchesi+ 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/858/77">J/ApJ/858/77 : DEIMOS 10K spectroscopic survey in COSMOS field (Hasinger+ 2018)</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/A+A/694/A241</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/694/A241</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/694/A241</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/694/A241</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/694/A241</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/694/A241</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface></capability><capability standardID="ivo://ivoa.net/std/TAP#aux"><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://tapvizier.cds.unistra.fr/TAPVizieR/tap</accessURL></interface></capability><capability xsi:type="cs:ConeSearch" standardID="ivo://ivoa.net/std/ConeSearch"><description>Cone search capability for table J/A+A/694/A241/tablea1 (Physical properties of our AGN sample)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+A/694/A241/tablea1?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/694/A241/tablea1?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/694/A241/tablea1?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>149.6727</ra><dec>2.0058</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>5/6814 6/27245 27247 27344</spatial><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/A+A/694/A241?format=ascii</footprint><waveband>X-ray</waveband></coverage><tableset><schema><name>default</name><table><name>J/A+A/694/A241/tablea1</name><description>Physical properties of our AGN sample</description><column><name>recno</name><description>Record number assigned by the VizieR team. 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