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<ri:Resource created="2014-06-03T07:30:09Z" status="active" updated="2025-05-19T09:50:00Z" version="1.2" 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/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>Jet models for the quasar NRAO150</title><shortName>J/A+A/566/A26</shortName><identifier>ivo://CDS.VizieR/J/A+A/566/A26</identifier><altIdentifier>doi:10.26093/cds/vizier.35660026</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Molina S.N.</name></creator><creator><name>Agudo I.</name></creator><creator><name>Gomez J.L.</name></creator><creator><name>Krichbaum T.P.</name></creator><creator><name>Marta-Vidal I.</name></creator><creator><name>Roy A.L.</name></creator><date role="Updated">2014-11-29T17:45:22Z</date><date role="Created">2014-06-03T07:30:09Z</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>quasars</subject><subject>polarimetry</subject><description>We present the results of the study of the relativistic jet of the quasar NRAO150. Our study confirm that the jet is seen at an extremely small angle to the line of sight and there is not a clear region to be identify as the core of the jet. The innermost regions of the jet show a counter-clockwise jet position angle swing at a high angular rate. We have studied the kinematic of the emission features into the innermost regions by fitting a model which explain the jet position angle swing as a rotation of the jet material following the toroidal magnetic field. This could be the first direct evidences about the helical structure of the magnetic field into the innermost regions of relativistic jets.</description><source format="bibcode">2014A&amp;A...566A..26M</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/566/A26</referenceURL><type>Catalog</type><contentLevel>Research</contentLevel><relationship><relationshipType>IsServedBy</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/TAP">TAP VizieR generic service</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/A+A/566/A26</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/566/A26</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/566/A26</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/566/A26</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/566/A26</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/566/A26</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface></capability><capability standardID="ivo://ivoa.net/std/TAP#aux"><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://tapvizier.cds.unistra.fr/TAPVizieR/tap</accessURL></interface></capability><coverage><footprint ivo-id="ivo://ivoa.net/std/moc"/><waveband>Optical</waveband></coverage><tableset><schema><name>default</name><table><name>J/A+A/566/A26/modelfit</name><description>List of model-fits parameters of NRAO150 (tables 3-7)</description><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Freq</name><description>[8/86] Total intensity VLBI image frequency</description><unit>GHz</unit><ucd>em.freq</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Date</name><description>Observing epoch (between 2006 and 2010)</description><ucd>time.epoch</ucd><flag>nullable</flag></column><column><name>Comp</name><description>Name of emission component (Q0, Q1, Q2, Q3, Q5 or Qn)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="2*">char</dataType></column><column><name>Flux</name><description>Flux density</description><unit>Jy</unit><ucd>phot.flux</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Flux</name><description>rms uncertainty on Flux density</description><unit>Jy</unit><ucd>stat.error;phot.flux</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>oRA</name><description>Relative right ascension</description><unit>mas</unit><ucd>pos.eq.ra;arith.diff</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_oRA</name><description>rms uncertainty on oRA</description><unit>mas</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>oDE</name><description>Relative declination</description><unit>mas</unit><ucd>pos.eq.dec;arith.diff</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_oDE</name><description>rms uncertainty on oDE</description><unit>mas</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>l_Size</name><description>[&lt;= ] Limit flag on Size</description><ucd>meta.code.error;phys.angSize</ucd><dataType xsi:type="vs:VOTableType" arraysize="2*">char</dataType></column><column><name>Size</name><description>[0.02/2.5] Angular size of emission feature</description><unit>mas</unit><ucd>phys.angSize</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Size</name><description>? rms uncertainty on Size</description><unit>mas</unit><ucd>stat.error;phys.angSize</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Pol</name><description>[0.2/16]? Degree of polarization</description><unit>%</unit><ucd>phys.polarization</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_Pol</name><description>? rms uncertainty on Pol</description><unit>%</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>PolPA</name><description>[-180/180[? Electric vector position angle</description><unit>deg</unit><ucd>pos.posAng;phys.polarization</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_PolPA</name><description>? rms uncertainty on EVPA</description><unit>deg</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column></table></schema></tableset></ri:Resource>