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<ri:Resource created="2016-01-07T11:13:20Z" 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>Pulkovo visual double stars photographic obs.</title><shortName>J/PAZh/42/46</shortName><identifier>ivo://CDS.VizieR/J/PAZh/42/46</identifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Izmailov I.S.</name></creator><creator><name>Roshchina E.A.</name></creator><creator><name>Kiselev A.A.</name></creator><creator><name>Kiseleva T.P.,Kalinichenko O.A.</name></creator><creator><name>Bykov O.P.</name></creator><creator><name>Kiyaeva O.V.</name></creator><creator><name>Romanenko L.G.</name></creator><creator><name>Shakht N.A.,Maslennikov K.L.</name></creator><creator><name>Vasil'eva T.A.</name></creator><date role="Updated">2017-09-19T14:23:40Z</date><date role="Created">2016-01-07T11:13:20Z</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>multiple-stars</subject><subject>astrometry</subject><description>We present the results of determining the relative positions of the 359 pairs of stars. More then six thousands of plates had been obtained in 1960-2007 years using the 26-inch Zeiss refractor(D=650mm, F=10413mm, scale is 19.80-arcsec/mm) at Pulkovo (code is 084). The plate digitization was carried out using a digital camera Canon EOS 5D Mark II and the lens 21M Jupiter, the scale was 21um/pixel. The measurements were calibrated using a template which was digitized by means of the Belgian high-precision scanner ROB Digitizer. 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