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<ri:Resource created="2011-04-11T19:26:34Z" 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>A Bayesian search for binaries in Hipparcos</title><shortName>J/ApJS/192/2</shortName><identifier>ivo://CDS.VizieR/J/ApJS/192/2</identifier><altIdentifier>doi:10.26093/cds/vizier.21920002</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Shaya E.J.</name></creator><creator><name>Olling R.P.</name></creator><date role="Updated">2023-07-21T13:40:57Z</date><date role="Created">2011-04-11T19:26:34Z</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>proper-motions</subject><subject>radial-velocity</subject><description>We develop Bayesian statistical methods for discovering and assigning probabilities to non-random (e.g., physical) stellar companions. These companions are either presently bound or were previously bound. The probabilities depend on similarities in corrected proper motion parallel and perpendicular to the brighter component's motion, parallax, and the local phase-space density of field stars. Control experiments are conducted to understand the behavior of false positives. The technique is applied to the Hipparcos Catalogue (Cat. I/239) within 100pc. This is the first all-sky survey to locate escaped companions still drifting along with each other. In the &lt;100pc distance range, ~220 high probability companions with separations between 0.01 and 1pc are found. The first evidence for a population (~300) of companions separated by 1-8pc is found.</description><source format="bibcode">2011ApJS..192....2S</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJS/192/2</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/I/239">I/239 : The Hipparcos and Tycho Catalogues (ESA 1997)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/311">I/311 : Hipparcos, the New Reduction (van Leeuwen, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/259">I/259 : The Tycho-2 Catalogue (Hog+ 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25pc (table3; Seq 1-111) between 25 and 50pc (table4; Seq 112-376) or between 50 and 100pc (table5 of the paper; Seq 377-840)</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>[1/840] System index number</description><ucd>spect.index</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>HIP</name><description>HIP (Cat. I/239) number of star</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Simbad</name><description>Simbad column added by the CDS</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column><column><name>HIP1</name><description>? HIP number of primary (if HIP is not primary)</description><ucd>meta.id.assoc</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>GLon</name><description>HIP catalog Galactic longitude</description><unit>deg</unit><ucd>pos.galactic.lon</ucd></column><column><name>GLat</name><description>HIP catalog Galactic latitude</description><unit>deg</unit><ucd>pos.galactic.lat</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Vmag</name><description>HIP visual magnitude</description><unit>mag</unit><ucd>phot.mag;em.opt.V</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>n_Vmag</name><description>? Vmag brightness ranking within the table</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>pmLon</name><description>Proper motion along GLon (2)</description><unit>mas/yr</unit><ucd>pos.pm</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>pmLat</name><description>Proper motion along GLat (2)</description><unit>mas/yr</unit><ucd>pos.pm</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>dpmLon</name><description>? Proper motion difference along GLon (3)</description><unit>mas/yr</unit><ucd>pos.pm;arith.diff</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_dpmLon</name><description>? Uncertainty in dpmGLon</description><unit>mas/yr</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>dpmLat</name><description>? Proper motion difference along GLat (3)</description><unit>mas/yr</unit><ucd>pos.pm;arith.diff</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_dpmLat</name><description>? Uncertainty in dpmGLat</description><unit>mas/yr</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Dist</name><description>HIP2 (Cat. I/311) distance (obtained from the inverse of parallax)</description><unit>pc</unit><ucd>pos.distance;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Dist</name><description>Uncertainty in Dist</description><unit>pc</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>RV</name><description>? 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Projected radial separation (blank for primary)</description><unit>pc</unit><ucd>pos.distance</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Prob</name><description>[0/1]? Probability candidate is true companion</description><ucd>stat.probability</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>_RA</name><description>Position of the primary (from HIP2, Cat. I/311) (right ascension part)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>_DE</name><description>Position of the primary (from HIP2, Cat. I/311) (declination part)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column><column><name>Com</name><description>Additional comment(s) (7)</description><ucd>meta.note</ucd></column><column><name>SpT</name><description>Simbad MK spectral type</description><ucd>src.spType</ucd><dataType xsi:type="vs:VOTableType" arraysize="6*">char</dataType></column><column><name>OType</name><description>Simbad other object type (1)</description><ucd>src.class</ucd><dataType xsi:type="vs:VOTableType" arraysize="3*">char</dataType></column></table></schema></tableset></ri:Resource>