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<ri:Resource created="2020-02-14T10:47:54Z" status="active" updated="2025-08-11T20:18:50Z" 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>Optical polarization properties of AGNs</title><shortName>J/MNRAS/493/L54</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/493/L54</identifier><altIdentifier>doi:10.26093/cds/vizier.74939054</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Kovalev Y.Y.</name></creator><creator><name>Zobnina D.I.</name></creator><creator><name>Plavin A.V.</name></creator><creator><name>Blinov D.</name></creator><date role="Updated">2025-08-11T20:18:50Z</date><date role="Created">2020-02-14T10:47:54Z</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>active-galactic-nuclei</subject><subject>polarimetry</subject><description>Significant positional offsets of the value from 1 mas to more than 10mas were found previously between radio (VLBI) and optical (Gaia) positions of active galactic nuclei (AGNs). They happen preferentially parallel to the parsec-scale jet direction. AGNs with VLBI-to-Gaia offsets pointed downstream the jet are found to have favourably higher optical polarization, as expected if extended optical jets dominate in the emission and shift the Gaia centroid away from the physical nucleus of the source. Upstream offsets with the suggested domination of accretion discs manifest themselves through the observed low optical polarization. Direction of linear optical polarization is confirmed to preferentially align with parsec-scale jets in AGNs with dominant jets consistent with a toroidal magnetic field structure. Our findings support the disc-jet interpretation of the observed positional offsets. These results call on an intensification of AGN optical polarization monitoring programs in order to collect precious observational data. Taken together with the continued VLBI and Gaia observations, they will allow researchers to reconstruct detailed models of the disc-jet system in AGNs on parsec scales.</description><source format="bibcode">2020MNRAS.493L..54K</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/493/L54</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/I/345">I/345 : Gaia DR2 (Gaia Collaboration, 2018)</relatedResource></relationship></content><rights>https://cds.unistra.fr/vizier-org/licences_vizier.html</rights><capability><interface xsi:type="vr:WebBrowser"><accessURL 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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>GaiaDR2</name><description>ID in Gaia DR2</description><ucd>meta.id;meta.main</ucd></column><column><name>RAJ2000</name><description>Gaia DR2 right ascension (J2000)</description><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>Gaia DR2 declination (J2000)</description><ucd>pos.eq.dec;meta.main</ucd></column><column><name>RPmag</name><description>? RP-magnitude in Gaia DR2</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Gmag</name><description>G-magnitude in Gaia DR2</description><unit>mag</unit><ucd>phot.mag;em.opt</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>BPmag</name><description>? BP-magnitude in Gaia DR2</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>J2000</name><description>J2000 name from RFC</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="10*">char</dataType></column><column><name>PAj</name><description>VLBI jet position angle</description><unit>deg</unit><ucd>pos.posAng</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>offset</name><description>Offset between VLBI and Gaia positions</description><unit>mas</unit><ucd>pos;arith.diff</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>psi</name><description>VLBI-Gaia offset direction relative to jet</description><unit>deg</unit><ucd>pos;arith.diff</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>s_psi</name><description>Standard deviation of VLBI-Gaia offset direction</description><unit>deg</unit><ucd>stat.stdev;pos.angDistance;arith.diff</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Polfrac</name><description>? 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