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<ri:Resource created="2018-10-04T08:09:15Z" 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>Gaia DR1 Upper Scorpius new member candidates</title><shortName>J/A+A/618/A12</shortName><identifier>ivo://CDS.VizieR/J/A+A/618/A12</identifier><altIdentifier>doi:10.26093/cds/vizier.36180012</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Wilkinson S.</name></creator><creator><name>Merin B.</name></creator><creator><name>Riviere-Marichalar P.</name></creator><date role="Updated">2018-11-05T10:52:51Z</date><date role="Created">2018-10-04T08:09:15Z</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>standard-stars</subject><description>Selecting a cluster in proper motion space is an established method for identifying members of a star forming region. The first data release from Gaia (DR1) provides an extremely large and precise stellar catalogue, which when combined with the Tycho-2 catalogue gives the 2.5 million parallaxes and proper motions contained within the Tycho-Gaia Astrometric Solution (TGAS). We aim to identify new member candidates of the nearby Upper Scorpius subgroup of the Scorpius-Centaurus Complex within the TGAS catalogue. In doing so, we also aim to validate the use of the DBSCAN clustering algorithm on spatial and kinematic data as a robust member selection method. We constructed a method for member selection using a density-based clustering algorithm (DBSCAN) applied over proper motion and distance. We then applied this method to Upper Scorpius, and evaluated the results and performance of the method. We identified 167 member candidates of Upper Scorpius, of which 78 are new, distributed within a 10{deg} radius from its core. These member candidates have a mean distance of 145.6+/-7.5pc, and a mean proper motion of (-11.4, -23.5)+/-(0.7, 0.4)mas/yr. These values are consistent with measured distances and proper motions of previously identified bona-fide members of the Upper Scorpius association.</description><source format="bibcode">2018A&amp;A...618A..12W</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/618/A12</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/ApJ/746/154">J/ApJ/746/154 : Improved kinematic parallaxes for Sco-Cen members</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/758/31">J/ApJ/758/31 : IR photometry for members of Upper Sco (Luhman+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/756/133">J/ApJ/756/133 : ScoCen debris disks around B- and A-type stars (Chen+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/461/794">J/MNRAS/461/794 : Scorpius-Centaurus K-Type Stars (Pecaut+, 2016)</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+A/618/A12</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/618/A12</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/618/A12</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/618/A12</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/618/A12</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/618/A12</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><capability xsi:type="cs:ConeSearch" standardID="ivo://ivoa.net/std/ConeSearch"><description>Cone search capability for table J/A+A/618/A12/table1 (Member candidates of Upper Scorpius)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+A/618/A12/table1?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/618/A12/table1?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/618/A12/table1?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>241.76942810822803</ra><dec>-16.943350307223707</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>5/10744 11088-11090 11094 6/29320 29353 29358 30759 42749 42751 42811 42851 42854 42857 42861 42866 42873 42876 42886 42903 42908-42909 42911-42913 42917 42921 42925 42932 42939 42941 42943-42945 42949 42953 42955-42956 42958 42970 42972 42980-42982 42985-42987 42989-42991 42994-42995 43000 43002-43003 44289 44292-44293 44301-44303 44307-44308 44310 44312 44314 44317-44321 44324 44337 44341 44343 44346 44351 44365-44366 44368 44371 44385 44388-44389 44393 44397 44400 44403 44409 44435</spatial><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/A+A/618/A12?format=ascii</footprint></coverage><tableset><schema><name>default</name><table><name>J/A+A/618/A12/table1</name><description>Member candidates of Upper Scorpius</description><column><name>recno</name><description>Record number assigned by the VizieR team. 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