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<ri:Resource created="2016-08-03T08:28:28Z" 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>New companions to nearby low-mass stars</title><shortName>J/MNRAS/429/859</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/429/859</identifier><altIdentifier>doi:10.26093/cds/vizier.74290859</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Jodar E.</name></creator><creator><name>Perez-Garrido A.</name></creator><creator><name>Diaz-Sanchez A.</name></creator><creator><name>Villo I.</name></creator><creator><name>Rebolo R.,Perez-Prieto J.A.</name></creator><date role="Updated">2024-07-20T20:14:03Z</date><date role="Created">2016-08-03T08:28:28Z</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>photometry</subject><description>We present high-angular-resolution optical I-band imaging of 451 late K to mid-M nearby stars. These observations have been performed with Astralux and FastCam using the lucky imaging technique. We found 70 companions with separations between 0.1 and 3.5-arcsec, out of which 28 are new discoveries. We derive a total binary fraction of 20.3^+6.9^_-5.2_ per cent. Follow-up observations have been carried out for 16 of these new binaries and all of them were confirmed as physically associated systems. Parallaxes are available for 70 per cent of the binary sample, providing reliable estimates of physical separations. 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Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Name</name><description>Gliese name</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="9*">char</dataType></column><column><name>Comp</name><description>[ABC ] Component</description><ucd>meta.code.multip</ucd><dataType xsi:type="vs:VOTableType" arraysize="2*">char</dataType></column><column><name>n_Name</name><description>[*] *: objects that have companions and described in more detail in Table 2</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>SimbadName</name><description>Simbad column added by the CDS</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="10*">char</dataType></column><column><name>_RA</name><description>Right Ascension (J2000) from SIMBAD (not part of the original data)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>_DE</name><description>Declination (J2000) from SIMBAD (not part of the original data)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column></table><table><name>J/MNRAS/429/859/table2</name><description>Binary systems found with component separations lower than 3500mas</description><column><name>Notes</name><description>Notes (3)</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="92*">char</dataType></column><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>Name</name><description>Gliese name</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="9*">char</dataType></column><column><name>Comp</name><description>[ABC ] Component</description><ucd>meta.code.multip</ucd><dataType xsi:type="vs:VOTableType" arraysize="2*">char</dataType></column><column><name>SpType</name><description>SIMBAD, CDS spectral classification</description><ucd>src.spType</ucd><dataType xsi:type="vs:VOTableType" arraysize="5*">char</dataType></column><column><name>Obs.date</name><description>Observation date (1)</description><ucd>time.epoch;obs</ucd><flag>nullable</flag></column><column><name>rho</name><description>Aangular separation of components (2)</description><unit>mas</unit><ucd>pos.angDistance</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>theta</name><description>Position angle</description><unit>deg</unit><ucd>pos.posAng</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_theta</name><description>rms uncertainty on theta</description><unit>deg</unit><ucd>stat.error;pos.posAng</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Sep</name><description>? Projected separation</description><unit>AU</unit><ucd>pos.angDistance</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_Sep</name><description>? rms uncertainty on Sep</description><unit>AU</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>DImag</name><description>? Estimated magnitude difference in the SDSS i band (CAHA observations) or Johnson-Cousin I (OT observations)</description><unit>mag</unit><ucd>phot.mag;arith.diff</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column></table><table><name>J/MNRAS/429/859/table3</name><description>*Ultracool dwarf candidates</description><column><name>recno</name><description>Record number assigned by the VizieR team. 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