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<ri:Resource created="2020-04-14T12:11:40Z" 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>The invisible AGN catalogue</title><shortName>J/MNRAS/468/196</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/468/196</identifier><altIdentifier>doi:10.26093/cds/vizier.74680196</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Truebenbach A.E.</name></creator><creator><name>Darling J.</name></creator><date role="Updated">2024-08-17T20:18:32Z</date><date role="Created">2020-04-14T12:11:40Z</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>radio-sources</subject><subject>infrared-sources</subject><subject>millimeter-astronomy</subject><subject>photometry</subject><subject>submillimeter-astronomy</subject><description>A large fraction of active galactic nuclei (AGN) are 'invisible' in extant optical surveys due to either distance or dust-obscuration. The existence of this large population of dust-obscured, infrared (IR)-bright AGN is predicted by models of galaxy-supermassive black hole coevolution and is required to explain the observed X-ray and IR backgrounds. Recently, IR colour cuts with Wide-field Infrared Survey Explorer have identified a portion of this missing population. However, as the host galaxy brightness relative to that of the AGN increases, it becomes increasingly difficult to differentiate between IR emission originating from the AGN and from its host galaxy. As a solution, we have developed a new method to select obscured AGN using their 20-cm continuum emission to identify the objects as AGN. We created the resulting invisible AGN catalogue by selecting objects that are detected in AllWISE (mid-IR) and FIRST (20 cm), but are not detected in SDSS (optical) or 2MASS (near-IR), producing a final catalogue of 46 258 objects. 30 per cent of the objects are selected by existing selection methods, while the remaining 70 per cent represent a potential previously unidentified population of candidate AGN that are missed by mid-IR colour cuts. Additionally, by relying on a radio continuum detection, this technique is efficient at detecting radio-loud AGN at z&gt;=0.29, regardless of their level of dust obscuration or their host galaxy's relative brightness.</description><source format="bibcode">2017MNRAS.468..196T</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/468/196</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/328">II/328 : AllWISE Data Release (Cutri+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VIII/92">VIII/92 : The FIRST Survey Catalog, Version 2014Dec17 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Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>FIRST</name><description>ID as it appears in FIRST Catalogue</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="16*">char</dataType></column><column><name>RAJ2000</name><description>Right ascension from FIRST Catalogue (J2000)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd><flag>indexed</flag></column><column><name>e_RAJ2000</name><description>Uncertainty (90% confidence) of FIRST right ascension (1)</description><unit>arcsec</unit><ucd>stat.error;pos.eq.ra</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>DEJ2000</name><description>Declination from FIRST Catalogue (J2000)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd><flag>indexed</flag></column><column><name>e_DEJ2000</name><description>Uncertainty (90% confidence) of FIRST declination (1)</description><unit>arcsec</unit><ucd>stat.error;pos.eq.dec</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F1.4GHz</name><description>1.4GHz integrated flux density from FIRST</description><unit>mJy</unit><ucd>phot.flux.density;em.radio.750-1500MHz</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_F1.4GHz</name><description>Local noise estimate at the source position</description><unit>mJy</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>AllWISE</name><description>AllWISE ID as it appears in AllWISE Catalogue</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="19*">char</dataType></column><column><name>Note</name><description>[*] Note (2)</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>RAAdeg</name><description>Right ascension from AllWISE Catalogue</description><unit>deg</unit><ucd>pos.eq.ra</ucd></column><column><name>e_RAAdeg</name><description>1-sigma uncertainty of WISE right ascension (3)</description><unit>arcsec</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>DEAdeg</name><description>Declination from AllWISE Catalogue</description><unit>deg</unit><ucd>pos.eq.dec</ucd></column><column><name>e_DEAdeg</name><description>1-sigma uncertainty of WISE declination (3)</description><unit>arcsec</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>l_[3.4]</name><description>Upper limit flag on [3.4]</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>[3.4]</name><description>3.4 micron magnitude from AllWISE Catalogue</description><unit>mag</unit><ucd>phot.mag;em.IR.3-4um</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_[3.4]</name><description>? 1-sigma uncertainty on 3.4 micron magnitude from the AllWISE Catalogue</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>SNR3.4</name><description>? 3.4 micron magnitude measurement signal-to-noise ratio.</description><ucd>stat.snr</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>l_[4.6]</name><description>Upper limit flag on [4.6]</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>[4.6]</name><description>4.6 micron magnitude from AllWISE Catalogue</description><unit>mag</unit><ucd>phot.mag;em.IR.4-8um</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_[4.6]</name><description>? 1-sigma uncertainty on 4.6 micron magnitude from the AllWISE Catalogue</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>SNR4.6</name><description>4.6 micron magnitude measurement signal-to-noise ratio</description><ucd>stat.snr</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>l_[12]</name><description>Upper limit flag on [12]</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>[12]</name><description>? 12 micron magnitude from AllWISE Catalogue</description><unit>mag</unit><ucd>phot.flux.density;em.IR.8-15um</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_[12]</name><description>? 1-sigma uncertainty on 12 micron magnitude from the AllWISE Catalogue</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>SNR12</name><description>? 12 micron magnitude measurement signal-to-noise ratio.</description><ucd>stat.snr</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>l_[22]</name><description>Upper limit flag on [22]</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>[22]</name><description>? 22 micron magnitude from AllWISE Catalogue</description><unit>mag</unit><ucd>phot.flux.density;em.IR.15-30um</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_[22]</name><description>? 1-sigma uncertainty on 22 micron magnitude from the AllWISE Catalogue</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>SNR22</name><description>? 22 micron magnitude measurement signal-to-noise ratio.</description><ucd>stat.snr</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>theta</name><description>Angular separation between the FIRST source and the AllWISE source</description><unit>arcsec</unit><ucd>pos.angDistance</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_theta</name><description>1-sigma uncertainty in the angular separation calculated based on FIRST and WISE position uncertainties</description><unit>arcsec</unit><ucd>stat.error;pos.posAng</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Simbad</name><description>Simbad column added by the CDS</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column></table></schema></tableset></ri:Resource>