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<ri:Resource created="2009-09-27T21:22:31Z" 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>Rotation measures of extragalactic sources in SGPS</title><shortName>J/ApJ/663/258</shortName><identifier>ivo://CDS.VizieR/J/ApJ/663/258</identifier><altIdentifier>doi:10.26093/cds/vizier.16630258</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Brown J.C.</name></creator><creator><name>Haverkorn M.</name></creator><creator><name>Gaensler B.M.</name></creator><creator><name>Taylor A.R.</name></creator><creator><name>Bizunok N.S.,McClure-Griffiths N.M.</name></creator><creator><name>Dickey J.M.</name></creator><creator><name>Green A.J.</name></creator><date role="Updated">2009-09-27T21:29:59Z</date><date role="Created">2009-09-27T21:22:31Z</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>polarimetry</subject><description>We present new Faraday rotation measures (RMs) for 148 extragalactic radio sources behind the southern Galactic plane (253{deg}&lt;=l&lt;=356{deg}, |b|&lt;=1.5{deg}), and use these data in combination with published data to probe the large-scale structure of the Milky Way's magnetic field. We show that the magnitudes of these RMs oscillate with longitude in a manner that correlates with the locations of the Galactic spiral arms. The observed pattern in RMs requires the presence of at least one large-scale magnetic reversal in the fourth Galactic quadrant, located between the Sagittarius-Carina and Scutum-Crux spiral arms. To quantitatively compare our measurements to other recent studies, we consider all available extragalactic and pulsar RMs in the region we have surveyed, and jointly fit these data to simple models in which the large-scale field follows the spiral arms.</description><source format="bibcode">2007ApJ...663..258B</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/663/258</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/VII/6">VII/6 : Polarization of extragalactic radio sources (Eichendorf+ 1980)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/45/97">J/ApJS/45/97 : Extragal. radio sources Faraday rot. 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