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<ri:Resource created="2022-09-14T09:37:01Z" 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 1.266GHz MeerKAT DEEP2 component catalog</title><shortName>J/ApJ/909/193</shortName><identifier>ivo://CDS.VizieR/J/ApJ/909/193</identifier><altIdentifier>doi:10.26093/cds/vizier.19090193</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Matthews A.M.</name></creator><creator><name>Condon J.J.</name></creator><creator><name>Cotton W.D.</name></creator><creator><name>Mauch T.</name></creator><date role="Updated">2022-10-14T13:47:24Z</date><date role="Created">2022-09-14T09:37:01Z</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>radio-galaxies</subject><subject>radio-sources</subject><description>Brightness-weighted differential source counts S2n(S) spanning the eight decades of flux density between 0.25{mu}Jy and 25Jy at 1.4GHz were measured from (1) the confusion brightness distribution in the MeerKAT DEEP2 image below 10{mu}Jy, (2) counts of DEEP2 sources between 10{mu}Jy and 2.5mJy, and (3) counts of NVSS sources stronger than 2.5mJy. We present our DEEP2 catalog of 1.7x10^4^ discrete sources complete above S=10{mu}Jy over {Omega}=1.04deg^2^. The brightness-weighted counts converge as S^2^n(S){propto}S^1/2^ below S=10{mu}Jy, so &gt;99% of the {Delta}T_b_~0.06K sky brightness produced by active galactic nuclei and ~96% of the {Delta}T_b_~0.04K added by star-forming galaxies has been resolved into sources with S&gt;=0.25{mu}Jy. The {Delta}T_b_~0.4K excess brightness measured by ARCADE 2 cannot be produced by faint sources smaller than ~50kpc if they cluster like galaxies.</description><source format="bibcode">2021ApJ...909..193M</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/909/193</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/VIII/65">VIII/65 : 1.4GHz NRAO VLA Sky Survey (NVSS) (Condon+ 1998)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/77/405">J/AJ/77/405 : Intense radio sources at 1400MHz (BDFL set) (Bridle+, 1972)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/125/465">J/AJ/125/465 : Phoenix Deep Survey 1.4-GHz microJy Catalog (Hopkins+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/132/1729">J/AJ/132/1729 : HUDF BVI-dropout sources (Beckwith+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/136/1889">J/AJ/136/1889 : 20cm observations of deep Swire Field (Owen+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/188/178">J/ApJS/188/178 : VLA 1.4GHz obs. of GOODS-North field (Morrison+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/602/A1">J/A+A/602/A1 : VLA-COSMOS 3 GHz Large Project (Smolcic+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/856/67">J/ApJ/856/67 : VLA 3GHz radio sources in the Lockman Hole (Cotton+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/235/34">J/ApJS/235/34 : Deep JVLA imaging of GOODS-N at 20cm (Owen, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/481/4548">J/MNRAS/481/4548 : Constraints on the 1.4GHz source counts (Prandoni+, 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/ApJ/909/193</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/909/193</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/909/193</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/909/193</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/909/193</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South 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