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<ri:Resource created="2013-04-05T08:11:16Z" 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>Optical monitoring of extragalactic sources</title><shortName>J/A+A/552/A98</shortName><identifier>ivo://CDS.VizieR/J/A+A/552/A98</identifier><altIdentifier>doi:10.26093/cds/vizier.35520098</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Taris F.</name></creator><creator><name>Andrei A.</name></creator><creator><name>Klotz A.</name></creator><creator><name>Vachier F.</name></creator><creator><name>Cote R.</name></creator><creator><name>Bouquillon S.,Souchay J.</name></creator><creator><name>Lambert S.</name></creator><creator><name>Anton S.</name></creator><creator><name>Bourda G.</name></creator><creator><name>Coward D.</name></creator><date role="Updated">2017-11-29T11:49:04Z</date><date role="Created">2013-04-05T08:11:16Z</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>quasars</subject><subject>photometry</subject><description>The goal to this work is to observe a first set of 70 extragalactic sources at optical wavelengths that could achieve the link with the ICRF. Variations in the light curves of these targets are connected with astrophysical processes that could produce displacements of the optical photocenter. Such displacements, if they exist, are critical in the framework of the link of reference systems. Four telescope were used to observe the targets at optical wavelengths. Two of them are located in France, one in Chile, and the last in Australia. First observations were carried out during one year and a half in the R and V bands. 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