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<ri:Resource created="2018-10-19T08:37:14Z" 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>Radio-loud NLSy1 galaxies optical polarisation</title><shortName>J/A+A/618/A92</shortName><identifier>ivo://CDS.VizieR/J/A+A/618/A92</identifier><altIdentifier>doi:10.26093/cds/vizier.36180092</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Angelakis E.</name></creator><creator><name>Kiehlmann S.</name></creator><creator><name>Myserlis I.</name></creator><creator><name>Blinov D.</name></creator><creator><name>Eggen J.</name></creator><creator><name>Itoh R.,Marchili N.</name></creator><creator><name>Zensus J.A.</name></creator><date role="Updated">2018-11-05T10:52:51Z</date><date role="Created">2018-10-19T08:37:14Z</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>galaxies</subject><subject>visible-astronomy</subject><subject>polarimetry</subject><description>We quantify the temporal behaviour of the optical polarisation fraction and angle for a selected sample of radio-loud NLSy1s. We also search for rotations of the polarisation plane similar to those commonly observed in blazars. The dataset was obtained with the RoboPol polarimeter of the Skinakas observatory as well as the KANATA, Perkins, and Steward observatories. We carried out numerical simulations to assess the probability that long rotations of the polarisation plane were caused by intrinsically evolving electric vector position angles (EVPAs) instead of observational noise. 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