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<ri:Resource created="2022-02-25T06:53:38Z" 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>COSMOS-XS. II. Ultra-faint radio population</title><shortName>J/ApJ/903/139</shortName><identifier>ivo://CDS.VizieR/J/ApJ/903/139</identifier><altIdentifier>doi:10.26093/cds/vizier.19030139</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Algera H.S.B.</name></creator><creator><name>van der Vlugt D.</name></creator><creator><name>Hodge J.A.</name></creator><creator><name>Smail I.R.</name></creator><creator><name>Novak M.,Radcliffe J.F.</name></creator><creator><name>Riechers D.A.</name></creator><creator><name>Rottgering H.</name></creator><creator><name>Smolcic V.</name></creator><creator><name>Walter F.</name></creator><date role="Updated">2023-09-05T07:21:44Z</date><date role="Created">2022-02-25T06:53:38Z</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>surveys</subject><subject>active-galactic-nuclei</subject><subject>radio-sources</subject><description>Ultra-deep radio surveys are an invaluable probe of dust-obscured star formation, but require a clear understanding of the relative contribution from radio active galactic nuclei (AGNs) to be used to their fullest potential. We study the composition of the {mu}Jy radio population detected in the Karl G. Jansky Very Large Array COSMOS-XS survey based on a sample of 1540 sources detected at 3GHz over an area of ~350arcmin^2^. This ultra-deep survey consists of a single pointing in the well-studied COSMOS field at both 3 and 10GHz and reaches rms sensitivities of 0.53 and 0.41{mu}Jy/beam, respectively. We find multiwavelength counterparts for 97% of radio sources, based on a combination of near-UV/optical to sub-millimeter data, and through a stacking analysis at optical/near-IR wavelengths we further show that the sources lacking such counterparts are likely to be high-redshift in nature (typical z~4-5). Utilizing the multiwavelength data over COSMOS, we identify AGNs through a variety of diagnostics and find these to make up 23.2~1.3% of our sample, with the remainder constituting uncontaminated star-forming galaxies. However, more than half of the AGNs exhibit radio emission consistent with originating from star formation, with only 8.8~0.8% of radio sources showing a clear excess in radio luminosity. At flux densities of ~30{mu}Jy at 3GHz, the fraction of star formation-powered sources reaches ~90%, and this fraction is consistent with unity at even lower flux densities. Overall, our findings imply that ultra-deep radio surveys such as COSMOS-XS constitute a highly effective means of obtaining clean samples of star formation-powered radio sources.</description><source format="bibcode">2020ApJ...903..139A</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/903/139</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/284">II/284 : COSMOS Multi-Wavelength Photometry Catalog (Capak+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VIII/103">VIII/103 : Herschel Multi-tiered Extragalactic Survey (Oliver+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VIII/95">VIII/95 : Herschel Multi-tiered Extragalactic Survey (Oliver+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/554/803">J/ApJ/554/803 : New VLA Sky Survey Cat of IRAS 2 Jy Galaxies (Yun+ 2001)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/586/794">J/ApJ/586/794 : Multiwavelength luminosities of galaxies (Bell, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/172/70">J/ApJS/172/70 : zCOSMOS-bright catalog (Lilly+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/172/46">J/ApJS/172/46 : VLA-COSMOS survey. 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