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<ri:Resource created="2026-09-03T16:08:12Z" status="active" updated="2026-09-03T15:15:44Z" 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>Physical properties of AGNs opt/IR/X selections</title><shortName>J/MNRAS/522/3506</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/522/3506</identifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Zhu S.</name></creator><creator><name>Brandt W.N.</name></creator><creator><name>Zou F.</name></creator><creator><name>Luo B.</name></creator><creator><name>Ni Q.</name></creator><creator><name>Xue Y.</name></creator><creator><name>Yan W.</name></creator><date role="Updated">2026-09-03T15:15:44Z</date><date role="Created">2026-09-03T16:08:12Z</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>redshifted</subject><subject>infrared-astronomy</subject><subject>radio-sources</subject><subject>stellar-masses</subject><subject>star-forming-regions</subject><description>The Australia Telescope Large Area Survey (ATLAS) and the VLA survey in the XMM-LSS/VIDEO deep field provide deep (~=15 {mu}m Jy/beam) and high-resolution (~=4.5-8 arcsec) radio coverage of the three XMM-SERVS fields (W-CDF-S, ELAIS-S1, and XMM-LSS). These data cover a total sky area of 11.3 deg^2^ and contain ~=11000 radio components. Furthermore, about 3 deg^2^ of the XMM-LSS field also has deeper MIGHTEE data that achieve a median RMS of 5.6 {mu}m Jy/beam and detect more than 20000 radio sources. We analyse all these radio data and find source counterparts at other wavebands utilizing deep optical and infrared (IR) surveys. The nature of these radio sources is studied using radio-band properties (spectral slope and morphology) and the IR-radio correlation. Radio AGNs are selected and compared with those selected using other methods (e.g. X-ray). We found 1656 new AGNs that were not selected using X-ray and/or MIR methods. We constrain the FIR-to-UV SEDs of radio AGNs using CIGALE and investigate the dependence of radio AGN fraction upon galaxy stellar mass and star formation rate.</description><source format="bibcode">2023MNRAS.522.3506Z</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/522/3506</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/MNRAS/509/2150">J/MNRAS/509/2150 : MIGHTEE catalogues of COSMOS/XMM-LSS fields (Heywood+, 2022)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/496/3469">J/MNRAS/496/3469 : VLA imaging of the XMM-LSS/VIDEO deep field (Heywood+, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/496/245">J/MNRAS/496/245 : L_x_-L_uv_-L_radio_ relation in radio-loud quasars</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/480/1022">J/MNRAS/480/1022 : Black-hole growth and cosmic environment (Yang+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/478/2132">J/MNRAS/478/2132 : XMM-LSS field. 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The flux density at 24 {mu}m (S24micron)</description><unit>mJy</unit><ucd>phot.flux.density;em.IR.15-30um</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_F24um</name><description>? Error of F24um (S24micron_err)</description><unit>mJy</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>M*gal</name><description>? The stellar mass of the cigale fits with a galaxy-only model (Mstar_gal)</description><unit>solMass</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>SFRgal</name><description>? The SFR of the cigale fits with a galaxy-only model (SFR_gal)</description><unit>solMass/yr</unit><ucd>phys.SFR</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>Chigal</name><description>? 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