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<ri:Resource created="2012-05-13T14:43:37Z" 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>2007-2008 WIYN speckle observations of binaries</title><shortName>J/AJ/139/205</shortName><identifier>ivo://CDS.VizieR/J/AJ/139/205</identifier><altIdentifier>doi:10.26093/cds/vizier.51390205</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Horch E.P.</name></creator><creator><name>Falta D.</name></creator><creator><name>Anderson L.M.</name></creator><creator><name>Desousa M.D.</name></creator><creator><name>Miniter C.M.</name></creator><creator><name>Ahmed T.,Van Altena W.F.</name></creator><date role="Updated">2017-10-02T19:28:21Z</date><date role="Created">2012-05-13T14:43:37Z</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>photometry</subject><description>Results of 974 speckle observations of 546 binary stars are presented. Observations were obtained at the WIYN 3.5m Telescope at Kitt Peak National Observatory during the time interval from 2007 January to 2008 June. In all cases, the relative separation and position angle of the components are measured, and the magnitude difference is determined in 809 cases. The precision of the results as judged from repeat observations and objects with very well-determined orbits is similar to previous papers in this series, namely ~3mas in separation and &lt;1{deg} in position angle in most cases. Similarly, the photometric precision remains consistent with previous WIYN speckle data, on average ~0.1mag per observation. Six systems of special interest are discussed.</description><source format="bibcode">2010AJ....139..205H</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/139/205</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/J/AJ/117/548">J/AJ/117/548 : 1997 WIYN binary stars speckle observations (Horch+, 1999)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/127/1727">J/AJ/127/1727 : Differential magnitudes of binary stars (Horch+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/136/312">J/AJ/136/312 : 2001-2006 WIYN binary stars 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