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<ri:Resource created="2013-05-23T13:47:13Z" 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>Bright northern radio sources with VLA/JVLA</title><shortName>J/A+A/549/A133</shortName><identifier>ivo://CDS.VizieR/J/A+A/549/A133</identifier><altIdentifier>doi:10.26093/cds/vizier.35490133</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Kurinsky N.</name></creator><creator><name>Sajina A.</name></creator><creator><name>Partridge B.</name></creator><creator><name>Myers S.</name></creator><creator><name>Chen X.</name></creator><creator><name>Lopez-caniego M.</name></creator><date role="Updated">2017-12-15T10:54:42Z</date><date role="Created">2013-05-23T13:47:13Z</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>radio-continuum-emission</subject><subject>radio-galaxies</subject><description>We report multiple epoch VLA/JVLA observations of 89 northern hemisphere sources, most with 37GHz flux density &gt;1Jy, observed at 4.8, 8.5, 33.5, and 43.3GHz. The high frequency selection leads to a predominantly flat spectrum sample, with 85% of our sources being in the Planck Early Release Compact Source Catalog (ERCSC, Cat. VIII/88). These observations allow us to: 1) validate Planck's 30 and 44GHz flux density scale; 2) extend the radio spectral energy distributions of Planck sources to lower frequencies allowing for the full 5-857GHz regime to be studied; and 3) characterize the variability of these sources. At 30GHz and 44GHz, the JVLA and Planck flux densities agree to within ~3%. On timescales of less than two months the median variability of our sources is 2%. On timescales of about a year the median variability increases to 14%. 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