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<ri:Resource created="2017-01-16T13:41:59Z" 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>S-PASS &amp; NVSS bright extragalactic radio sources</title><shortName>J/ApJ/829/5</shortName><identifier>ivo://CDS.VizieR/J/ApJ/829/5</identifier><altIdentifier>doi:10.26093/cds/vizier.18290005</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Lamee M.</name></creator><creator><name>Rudnick L.</name></creator><creator><name>Farnes J.S.</name></creator><creator><name>Carretti E.</name></creator><creator><name>Gaensler B.M.,Haverkorn M.</name></creator><creator><name>Poppi S.</name></creator><date role="Updated">2018-01-02T13:42:47Z</date><date role="Created">2017-01-16T13:41:59Z</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>polarimetry</subject><subject>radio-sources</subject><subject>infrared-photometry</subject><description>We present a polarization catalog of 533 extragalactic radio sources that have a 2.3GHz total intensity above 420mJy from the S-band Polarization All Sky Survey, S-PASS, with corresponding 1.4GHz polarization information from the NRAO VLA Sky Survey, NVSS. We studied the selection effects and found that fractional polarization, {pi}, of radio objects at both wavelengths depends on the spectral index, the source magnetic field disorder, the source size, and depolarization. The relationship between depolarization, spectrum, and size shows that depolarization occurs primarily in the source vicinity. The median {pi}_2.3_ of resolved objects in NVSS is approximately two times larger than that of unresolved sources. Sources with little depolarization are ~2 times more polarized than both highly depolarized and re-polarized sources. This indicates that intrinsic magnetic field disorder is the dominant mechanism responsible for the observed low fractional polarization of radio sources at high frequencies. We predict that number counts from polarization surveys will be similar at 1.4GHz and at 2.3GHz, for fixed sensitivity, although ~10% of all sources may currently be missing because of strong depolarization. Objects with {pi}_1.4_~{pi}_2.3_&gt;=4% typically have simple Faraday structures, so they are most useful for background samples. Almost half of flat-spectrum ({alpha}&gt;=-0.5) and ~25% of steep-spectrum objects are re-polarized. Steep-spectrum, depolarized sources show a weak negative correlation of depolarization with redshift in the range 0&lt;z&lt;2.3. Previous non-detections of redshift evolution are likely due the inclusion of re-polarized sources as well.</description><source format="bibcode">2016ApJ...829....5L</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/829/5</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/311">II/311 : WISE All-Sky Data Release (Cutri+ 2012)</relatedResource><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/ApJS/212/15">J/ApJS/212/15 : Polarized NVSS sources SEDs (Farnes+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/771/105">J/ApJ/771/105 : MWA Stokes I 189MHz sources (Bernardi+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/436/2915">J/MNRAS/436/2915 : Polarization of bright AT20G sources (Massardi+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/755/21">J/ApJ/755/21 : Extragalactic radio source rotation measures (Mao+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/144/105">J/AJ/144/105 : MOJAVE. VIII. Faraday rotation in AGN jets. (Hovatta+, 2012)</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/MNRAS/402/2792">J/MNRAS/402/2792 : 1388MHz ATLBS Low-Brightness Survey (Subrahmanyan+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/702/1230">J/ApJ/702/1230 : Rotation measure image of the sky (Taylor+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/666/201">J/ApJ/666/201 : Radio polarimetry of the ELAIS N1 field (Taylor+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/371/898">J/MNRAS/371/898 : Extragalactic radio sources at 20GHz (Sadler+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/360/1305">J/MNRAS/360/1305 : Polarization of extragalactic sources (Roy+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/124/285">J/ApJS/124/285 : VLA Images of Extragalactic Objects (Reid+, 1999)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+AS/135/571">J/A+AS/135/571 : Extragalactic radio sources polarization (Zukowski+, 1999)</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/829/5</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/829/5</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/829/5</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/829/5</accessURL><mirrorURL title="VizieR at IUCAA: Pune, 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Uncertainty in NVPA (1)</description><unit>deg</unit><ucd>pos.posAng;phys.polarization</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>majaxis</name><description>[14/127] NVSS fitted deconvolved major axis (1)</description><unit>arcsec</unit><ucd>phys.angSize.smajAxis</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>f_majaxis</name><description>Upper limit flag on majaxis: limit=-1; resolved=1 (1)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>minaxis</name><description>[13/100] NVSS fitted deconvolved minor axis (1)</description><unit>arcsec</unit><ucd>phys.angSize.sminAxis</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>f_minaxis</name><description>Upper limit flag on minaxis: limit=-1; resolved=1 (1)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>ISP</name><description>[435/10096] S-PASS peak intensity</description><unit>mJy</unit><ucd>phot.flux.density;em.radio.1500-3000MHz</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_ISP</name><description>[7/18] Uncertainty in ISP</description><unit>mJy</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>PSP</name><description>[-1.7/427] S-PASS polarized intensity</description><unit>mJy</unit><ucd>phot.flux.density</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_PSP</name><description>[0.5/33] S-PASS Uncertainty in PSP</description><unit>mJy</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>PiSP</name><description>[0.005/0.3] S-PASS fractional polarization (3)</description><ucd>phot.flux.density</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_PiSP</name><description>[0.0002/0.04] Uncertainty in PiSP</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>f_PiSP</name><description>Upper limit flag on PiSP: limit=-1; detection=1</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>SPPA</name><description>? 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