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<ri:Resource created="2011-10-04T14:52:26Z" 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>Near-infrared imaging polarimetry in S106</title><shortName>J/AJ/137/3149</shortName><identifier>ivo://CDS.VizieR/J/AJ/137/3149</identifier><altIdentifier>doi:10.26093/cds/vizier.51373149</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Saito H.</name></creator><creator><name>Tamura M.</name></creator><creator><name>Kandori R.</name></creator><creator><name>Kusakabe N.</name></creator><creator><name>Hashimoto J.</name></creator><creator><name>Nakajima Y.,Sato Y.</name></creator><creator><name>Nagata T.</name></creator><creator><name>Nagayama T.</name></creator><creator><name>Kato D.</name></creator><date role="Updated">2017-12-12T14:44:37Z</date><date role="Created">2011-10-04T14:52:26Z</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>h-ii-regions</subject><subject>polarimetry</subject><subject>infrared-photometry</subject><description>We present the results of wide-field JHKS polarimetry toward the HII region S106 using the Infrared Survey Facility telescope. Our polarimetry data revealed an extended (up to ~5') polarized nebula over S106. We confirmed the position of the illuminating source of most of the nebula as consistent with S106 IRS 4 through an analysis of polarization vectors. 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