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<ri:Resource created="2005-08-23T08:51:11Z" 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>High proper motion stars in USNO-B</title><shortName>J/AJ/126/472</shortName><identifier>ivo://CDS.VizieR/J/AJ/126/472</identifier><altIdentifier>doi:10.26093/cds/vizier.51260472</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Gould A.</name></creator><date role="Updated">2023-04-06T16:50:59Z</date><date role="Created">2005-08-23T08:51:11Z</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>proper-motions</subject><description>The completeness of USNO-B detections of high proper motion ({mu}&gt;180mas/yr) stars is tested, and the accuracy of its measurements is compared to the revised New Luyten Two-Tenths catalog of Salim &amp; Gould (2002ApJ...575L..83S). For 14.5&lt;V&lt;18.5, only 6% of such stars are missing from USNO-B (Cat. &lt;I/284&gt;), while another 3% have large errors, mostly too large to be useful. Including both classes, incompleteness is 9%. These fractions rise toward both brighter and fainter magnitudes. Incompleteness rises with proper motion to 30% at {mu}=1"/yr. It also rises to 35% at the Galactic plane, although this is only determined for relatively bright stars V&lt;~14. For binaries, incompleteness rises from 9% at separations of 30" to 47% at 10". The proper-motion errors reported internally by USNO-B are generally correct. However, there is a value of {sigma}{mu}~4mas/yr below which the reported errors should not be taken at face value. The small number of stars with relatively large reported errors ({sigma}{mu}&gt;~20mas/yr) may actually have still larger errors than tabulated.</description><source format="bibcode">2003AJ....126..472G</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/126/472</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/284">I/284 : The USNO-B1.0 Catalog (Monet+ 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/98">I/98 : NLTT Catalogue (Luyten, 1979)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/582/1011">J/ApJ/582/1011 : 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