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<ri:Resource created="2017-09-18T12:50:10Z" 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>Robo-AO observed cool subdwarf companions</title><shortName>J/ApJ/804/30</shortName><identifier>ivo://CDS.VizieR/J/ApJ/804/30</identifier><altIdentifier>doi:10.26093/cds/vizier.18040030</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Ziegler C.</name></creator><creator><name>Law N.M.</name></creator><creator><name>Baranec C.</name></creator><creator><name>Riddle R.L.</name></creator><creator><name>Fuchs J.T.</name></creator><date role="Updated">2017-10-26T12:46:48Z</date><date role="Created">2017-09-18T12:50:10Z</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>subdwarf-stars</subject><subject>multiple-stars</subject><subject>late-type-stars</subject><subject>apparent-magnitude</subject><description>Cool subdwarfs are the oldest members of the low-mass stellar population. Mostly present in the galactic halo, subdwarfs are characterized by their low-metallicity. Measuring their binary fraction and comparing it to solar-metallicity stars could give key insights into the star formation process early in the Milky Way's history. However, because of their low luminosity and relative rarity in the solar neighborhood, binarity surveys of cool subdwarfs have suffered from small sample sizes and incompleteness. Previous surveys have suggested that the binary fraction of red subdwarfs is much lower than for their main-sequence cousins. Using the highly efficient Robo-AO system, we present the largest high-resolution survey of subdwarfs, sensitive to angular separations ({rho}&gt;=0.15") and contrast ratios ({Delta}_mi_&lt;=6) invisible in past surveys. Of 344 target cool subdwarfs, 43 are in multiple systems, 19 of which are newly discovered, for a binary fraction of 12.5+/-1.9%. We also discovered seven triple star systems for a triplet fraction of 2.0+/-0.8%. Comparisons to similar surveys of solar-metallicity dwarf stars gives a ~3{sigma} disparity in luminosity between companion stars, with subdwarfs displaying a shortage of low-contrast companions. We also observe a lack of close subdwarf companions in comparison to similar-mass dwarf multiple systems.</description><source format="bibcode">2015ApJ...804...30Z</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/804/30</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/98">I/98 : NLTT Catalogue (Luyten, 1979)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/582/1011">J/ApJ/582/1011 : Revised NLTT Catalog (Salim+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/PASP/115/22">J/PASP/115/22 : Stellar parameters for 134 cool subdwarfs (Yong+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/134/778">J/AJ/134/778 : BVRI photometry of candidate subdwarfs (Marshall, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/799/4">J/ApJ/799/4 : Robo-AO observations of binary stars (Riddle+, 2015)</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/ApJ/804/30</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/804/30</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/804/30</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL 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