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<ri:Resource created="2010-06-13T22:11:34Z" 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>Deep 15GHz survey (9C continued)</title><shortName>J/MNRAS/404/1005</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/404/1005</identifier><altIdentifier>doi:10.26093/cds/vizier.74041005</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Waldram E.M.</name></creator><creator><name>Pooley G.G.</name></creator><creator><name>Davies M.L.</name></creator><creator><name>Grainge K.J.B.</name></creator><creator><name>Scott P.F.</name></creator><date role="Updated">2024-07-11T20:16:22Z</date><date role="Created">2010-06-13T22:11:34Z</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-sources</subject><subject>surveys</subject><subject>radio-continuum-emission</subject><description>The 9C survey of radio sources with the Ryle Telescope at 15.2GHz was set up to survey the fields of the cosmic microwave background telescope, the Very Small Array. In our first paper we described three regions of the survey, constituting a total area of to a completeness limit of ~25mJy. Here we present results from series of deeper regions, amounting to an area of 115deg^2^ complete to ~10mJy and of 29deg^2^ complete to ~5.5mJy. 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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>Name</name><description>9C source designation J2000 (JHHMM+DDMMa)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="11*">char</dataType></column><column><name>Dflag</name><description>[D ] D if from one of deeper regions (1)</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>RAJ2000</name><description>Right Ascension J2000</description><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>Declination J2000</description><ucd>pos.eq.dec;meta.main</ucd></column><column><name>S</name><description>15.2GHz flux density from subsequent pointed observation</description><unit>Jy</unit><ucd>phot.flux.density;em.radio.12-30GHz</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Date</name><description>Date of observation yymmdd</description><ucd>time.epoch</ucd><flag>nullable</flag></column><column><name>Mflag</name><description>[be? ] binary/extended source morphology flag (2)</description><ucd>meta.code;src.morph</ucd><dataType xsi:type="vs:VOTableType" arraysize="2*">char</dataType></column><column><name>SED</name><description>Plot the spectrum with SPECFIND (Vollmer et al. 2009, Cat. 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