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<ri:Resource created="2025-06-17T08:40:50Z" status="active" updated="2026-02-27T20:00:51Z" 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>3C 273 multi-frequency polarimetric images</title><shortName>J/A+A/698/A210</shortName><identifier>ivo://CDS.VizieR/J/A+A/698/A210</identifier><altIdentifier>doi:10.26093/cds/vizier/bc-nt/lcba</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Toscano T.</name></creator><creator><name>Molina S.N.</name></creator><creator><name>Gomez J.L.</name></creator><creator><name>Zeng A.-L.</name></creator><creator><name>Dahale R.</name></creator><creator><name>Cho I.,Moriyama K.</name></creator><creator><name>Wielgus M.</name></creator><creator><name>Fuentes A.</name></creator><creator><name>Foschi M.</name></creator><creator><name>Roeder J.</name></creator><creator><name>Myserlis I.,Angelakis E.</name></creator><creator><name>Zensus A.</name></creator><date role="Updated">2026-02-27T20:00:51Z</date><date role="Created">2025-06-17T08:40:50Z</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>quasars</subject><subject>very-long-baseline-interferometry</subject><subject>polarimetry</subject><description>We present a study on rotation measure (RM) of the quasar 3C 273. This analysis aims to discern the magnetic field structure and its temporal evolution. The quasar 3C 273 is one of the most studied active galactic nuclei due to its high brightness, strong polarization, and proximity, which enables resolving the transverse structure of its jet in detail. We used polarized data from 2014, collected at six frequencies (5, 8, 15, 22, 43, 86 GHz) with the Very Long Baseline Array, to produce total and linear polarization intensity images, as well as RM maps. Our analysis reveals a well-defined transverse RM gradient across the jet, indicating a helical, ordered magnetic field that threads the jet and likely contributes to its collimation. Furthermore, we identified temporal variations in the RM magnitude when compared with prior observations. These temporal variations show that the environment around the jet is dynamic, with changes in the density and magnetic field strength of the sheath that are possibly caused by interactions with the surrounding medium.</description><source format="bibcode">2025A&amp;A...698A.210T</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/698/A210</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/J/MNRAS/392/1181">J/MNRAS/392/1181 : BV(RI)c photometry of 3C 273 (Dai+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/213/26">J/ApJS/213/26 : Optical light curves of PHL 1811 and 3C 273 (Fan+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/576/A122">J/A+A/576/A122 : 3C 273 high energy spectrum (Esposito+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/601/A35">J/A+A/601/A35 : High-fidelity VLA imaging of 3C 273 (Perley+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/604/A111">J/A+A/604/A111 : 22GHz image of 3C 273 (Bruni+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/229/21">J/ApJS/229/21 : VRI monitoring of the QSO 3C 273 in 2005-2016 (Xiong+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/876/49">J/ApJ/876/49 : 3C 273 10yr reverberation mapping campaign (Zhang+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/880/155">J/ApJ/880/155 : RI photometry of blazars S5 0716+714 and 3C 273 (Liu+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/636/A62">J/A+A/636/A62 : Light curves of 3C273 during 2015-2019 (Kim+, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/159/259">J/AJ/159/259 : Quasar 3C 273 opt-NIR light curve (Sobrino Figaredo+, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/897/18">J/ApJ/897/18 : Swift UVOT observation of radio quasar 3C 273 (Li+, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/658/A8">J/A+A/658/A8 : Resolved jet of 3C 273 at 150MHz (Harwood+, 2022)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/683/L5">J/A+A/683/L5 : FITS images of 3C 273 host galaxy (Ren+, 2024)</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/698/A210</accessURL><mirrorURL title="VizieR at IUCAA: Pune, 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