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<ri:Resource created="1997-12-09T18:20:12Z" status="active" updated="2025-05-19T09:50:00Z" version="1.2" 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/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>Proper motions of stars in NGC 2286</title><shortName>J/A+AS/105/15</shortName><identifier>ivo://CDS.VizieR/J/A+AS/105/15</identifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Tian K.P.</name></creator><creator><name>Zhao J.L.</name></creator><creator><name>van Leeuwen F.</name></creator><date role="Updated">1997-12-09T17:20:17Z</date><date role="Created">1997-12-09T18:20:12Z</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>open-star-clusters</subject><subject>proper-motions</subject><description>Relative proper motions, their corresponding observed errors and membership probabilities of 2400 stars in the open cluster NGC 2286 region are determined from ASTROSCAN measurements of 8 plates made at Leiden Observatory. The plates have the maximum epoch difference of some 70 years and were taken with the double astrograph at Zo-Se station of Shanghai Observatory, which has an aperture of 40 cm, a focal length of 6.9 m and a scale of 30 arcsec/mm. The number of stars with membership probabilities higher than 0.7 and radial distances from the cluster centre less than 12' is 90. The average standard errors of proper motions vary from +/-0.0007"/yr for bright stars in the inner part of the field to some +/-0.0016"/yr for faint stars in the outer part of the field, and are statistically dependent on the number of measured plates per star. It is found from an analysis of the surface number density distribution of cluster members that the angular radius of NGC 2286 is some 12' and the corresponding linear radius 4.5 pc.</description><source format="bibcode">1994A&amp;AS..105...15T</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+AS/105/15</referenceURL><type>Catalog</type><contentLevel>Research</contentLevel><relationship><relationshipType>IsServedBy</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/TAP">TAP VizieR generic service</relatedResource></relationship></content><rights>https://cds.unistra.fr/vizier-org/licences_vizier.html</rights><capability><interface xsi:type="vr:WebBrowser"><accessURL use="full">https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+AS/105/15</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+AS/105/15</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+AS/105/15</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+AS/105/15</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/A+AS/105/15</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+AS/105/15</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface></capability><capability standardID="ivo://ivoa.net/std/TAP#aux"><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://tapvizier.cds.unistra.fr/TAPVizieR/tap</accessURL></interface></capability><coverage><footprint ivo-id="ivo://ivoa.net/std/moc"/><waveband>Optical</waveband></coverage><tableset><schema><name>default</name><table><name>J/A+AS/105/15/table7</name><description>Catalogue of proper motion and membership probabilities in the NGC2286</description><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Seq</name><description>Ordinal number of stars</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Li</name><description>Identification numbers in Li's catalogue (Ann. Shanghai Obs. Zo-Se 23, 19, 1954)</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="5*">char</dataType></column><column><name>Xpos</name><description>X coordinate</description><unit>cm</unit><ucd>pos.cartesian.x;instr.det</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Ypos</name><description>Y coordinate</description><unit>cm</unit><ucd>pos.cartesian.y;instr.det</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>n_Bmag</name><description>[* ] An * indicates that the photographic magnitude is taken from Chicarini</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="2*">char</dataType></column><column><name>Bmag</name><description>Photographic magnitude</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>BLi</name><description>Magnitudes of stars listed in Li's catalogue</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>pmX</name><description>X-proper motion (arcsec/century)</description><unit>10mas/yr</unit><ucd>pos.pm</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_pmX</name><description>Observed error of X-proper motion</description><unit>10mas/yr</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>pmY</name><description>Y-proper motion (arcsec/century)</description><unit>10mas/yr</unit><ucd>pos.pm</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_pmY</name><description>Observed error of Y-proper motion</description><unit>10mas/yr</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Pr</name><description>Proper motion membership probabilities</description><unit>%</unit><ucd>stat.fit.goodness</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Npl</name><description>Numbers of measured plates of stars</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column></table></schema></tableset></ri:Resource>