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<ri:Resource created="2025-08-26T10:10:31Z" status="active" updated="2025-09-01T07:18:35Z" 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>89 new utlra cool dwarfs comoving companions</title><shortName>J/AJ/167/253</shortName><identifier>ivo://CDS.VizieR/J/AJ/167/253</identifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Rothermich A.</name></creator><creator><name>Faherty J.K.</name></creator><creator><name>Bardalez-Gagliuffi D.</name></creator><creator><name>Schneider A.C.,Kirkpatrick J.D.</name></creator><creator><name>Meisner A.M.</name></creator><creator><name>Burgasser A.J.</name></creator><creator><name>Kuchner M.</name></creator><creator><name>Allers K.,Gagne J.</name></creator><creator><name>Caselden D.</name></creator><creator><name>Calamari E.</name></creator><creator><name>Popinchalk M.</name></creator><creator><name>Suarez G.,Gerasimov R.</name></creator><creator><name>Aganze C.</name></creator><creator><name>Softich E.</name></creator><creator><name>Hsu C.-C.</name></creator><creator><name>Karpoor P.</name></creator><creator><name>Theissen C.A.,Rees J.</name></creator><creator><name>Cecilio-Flores-Elie R.</name></creator><creator><name>Cushing M.C.</name></creator><creator><name>Marocco F.</name></creator><creator><name>Casewell S.,Bickle T.P.</name></creator><creator><name>Hamlet L.</name></creator><creator><name>Allen M.B.</name></creator><creator><name>Beaulieu P.</name></creator><creator><name>Colin G.</name></creator><creator><name>Gantier J.M.,Gramaize L.</name></creator><creator><name>Jalowiczor P.</name></creator><creator><name>Kabatnik M.</name></creator><creator><name>Kiwy F.</name></creator><creator><name>Martin D.W.,Pendrill B.</name></creator><creator><name>Pumphrey B.</name></creator><creator><name>Sainio A.</name></creator><creator><name>Schumann J.</name></creator><creator><name>Stevnbak N.</name></creator><creator><name>Sun G.,Tanner C.</name></creator><creator><name>Thakur V.</name></creator><creator><name>Thevenot M.</name></creator><creator><name>Wedracki Z.</name></creator><date role="Updated">2025-09-01T07:18:35Z</date><date role="Created">2025-08-26T10:10:31Z</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>brown-dwarfs</subject><subject>t-dwarfs</subject><subject>astrometry</subject><subject>radial-velocity</subject><subject>infrared-photometry</subject><description>We report the identification of 89 new systems containing ultracool dwarf companions to main-sequence stars and white dwarfs, using the citizen science project Backyard Worlds: Planet 9 and cross-reference between Gaia and CatWISE2020. 32 of these companions and 33 host stars were followed up with spectroscopic observations, with companion spectral types ranging from M7-T9 and host spectral types ranging from G2-M9. These systems exhibit diverse characteristics, from young to old ages, blue to very red spectral morphologies, potential membership to known young moving groups, and evidence of spectral binarity in nine companions. 20 of the host stars in our sample show evidence for higher-order multiplicity, with an additional 11 host stars being resolved binaries themselves. We compare this sample's characteristics with those of the known stellar binary and exoplanet populations, and find our sample begins to fill in the gap between directly imaged exoplanets and stellar binaries on mass ratio-binding energy plots. With this study, we increase the population of ultracool dwarf companions to FGK stars by ~42%, and more than triple the known population of ultracool dwarf companions with separations larger than 1000AU, providing excellent targets for future atmospheric retrievals.</description><source format="bibcode">2024AJ....167..253R</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/167/253</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/B/pastel">B/pastel : The PASTEL catalogue (Soubiran+, 2016-)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/III/123">III/123 : Dwarf K and M stars of small proper motion (Stephenson 1986)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/146">I/146 : Positions and Proper Motions - North (Roeser+, 1988)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/196">I/196 : Hipparcos Input Catalogue, Version 2 (Turon+ 1993)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/179">II/179 : Southern Spectrophotometric Standards. 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References for plx measurement (2)</description><ucd>meta.ref;pos.parallax</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>SepA</name><description>[0.3/1124]? Angular separation from host star</description><unit>arcsec</unit><ucd>pos.angDistance</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>SepL</name><description>[5/4e4]? Linear separation from host star (3)</description><unit>AU</unit><ucd>pos.distance;phys.size</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>GaiaDR3Cat</name><description>Display data from Gaia DR3 (I/355) within 10" (added by CDS)</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>2MASSCat</name><description>Display data from 2MASS-PSC (II/246) within 5" (added by CDS)</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>CWISECat</name><description>Display data from CatWISE2020 (II/365) within 5" (added by CDS)</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></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><column><name>SimbadName</name><description>Simbad column added by the CDS</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="28*">char</dataType><flag>nullable</flag></column></table><table><name>J/AJ/167/253/table2</name><description>Photometry of high-probability comoving systems</description><column><name>Syst</name><description>[1/89] System number; column and numbers added by CDS</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>primary</flag></column><column><name>e_BPmag</name><description>[3e-3/0.31]? Uncertainty in BPmag</description><unit>mag</unit><ucd>stat.error;phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>RPmag</name><description>[6.3/20]? Gaia DR3 (I/357) RP (797nm) magnitude</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_RPmag</name><description>[4e-3/0.11]? Uncertainty in RPmag</description><unit>mag</unit><ucd>stat.error;phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Jmag</name><description>[6/21.4]? J-band (1.25um) magnitude (1)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_Jmag</name><description>[0/0.33]? Uncertainty in Jmag</description><unit>mag</unit><ucd>stat.error;phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>l_Hmag</name><description>Lower limit &gt;= on Hmag</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>Hmag</name><description>[5.8/19.7]? H-band (1.65um) magnitude</description><unit>mag</unit><ucd>phot.mag;em.IR.H</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_Hmag</name><description>[0.01/0.25]? Uncertainty in Hmag</description><unit>mag</unit><ucd>stat.error;phot.mag;em.IR.H</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Kmag</name><description>[5.7/18.3]? K- and Ks-bands (2.20-2.17um) magnitude (1)</description><unit>mag</unit><ucd>phot.mag;em.IR.K</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></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>ID</name><description>Object identifier</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="26*">char</dataType></column><column><name>m_ID</name><description>[A/B] Component of the object identifier</description><ucd>meta.code.multip</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>Coord</name><description>Truncated coordinates (HHMM+DDMM) or alternative ID</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="11*">char</dataType></column><column><name>Gmag</name><description>[6.7/21]? Gaia DR3 (I/357) G (673nm) magnitude</description><unit>mag</unit><ucd>phot.mag;em.opt.V</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_Gmag</name><description>[3e-3/0.02]? Uncertainty in Gmag</description><unit>mag</unit><ucd>stat.error;phot.mag;em.opt.V</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>BPmag</name><description>[6.9/22]? Gaia DR3 (I/357) BP (532nm) magnitude</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_Kmag</name><description>[0/0.31]? Uncertainty in Kmag</description><unit>mag</unit><ucd>stat.error;phot.mag;em.IR.K</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>RefNIR</name><description>Near infrared references (2)</description><ucd>meta.ref;phot.mag;em.IR.NIR</ucd><dataType xsi:type="vs:VOTableType" arraysize="5*">char</dataType></column><column><name>l_W1mag</name><description>Lower limit &gt;= on W1mag</description><ucd>meta.code;phot.mag;em.IR.3-4um</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>W1mag</name><description>[5.9/20]? CatWISE2020 (II/365) W1 (3.35um) magnitude</description><unit>mag</unit><ucd>phot.mag;em.IR.3-4um</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_W1mag</name><description>[0.01/0.33]? Uncertainty in W1mag</description><unit>mag</unit><ucd>stat.error;phot.mag;em.IR.3-4um</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>W2mag</name><description>[5.7/18.3]? CatWISE2020 (II/365) W2 (4.6um) magnitude</description><unit>mag</unit><ucd>phot.mag;em.IR.4-8um</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_W2mag</name><description>[0.01/0.54]? Uncertainty in W2mag</description><unit>mag</unit><ucd>stat.error;phot.mag;em.IR.4-8um</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column></table><table><name>J/AJ/167/253/table11</name><description>Binding energies and masses of high-probability comoving systems</description><column><name>Syst</name><description>[1/89] System number; column and numbers added by CDS</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>primary</flag></column><column><name>l_tau</name><description>Limit flag on tau</description><ucd>meta.code.error;time.lifetime</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">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>Host1</name><description>First host identifier</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="26*">char</dataType></column><column><name>m_Host1</name><description>[AB] Composant of first host identifier</description><ucd>meta.code.multip</ucd><dataType xsi:type="vs:VOTableType" arraysize="2*">char</dataType></column><column><name>Host2</name><description>Second host identifier</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="22*">char</dataType></column><column><name>Comp</name><description>Companion identifier</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="25*">char</dataType></column><column><name>Mhost</name><description>[0.05/1.53] Mass of the host M_Host_ (1)</description><unit>solMass</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Mcomp</name><description>[0.01/0.11] Mass of the companion M_Comp_</description><unit>solMass</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Mtot</name><description>[0.09/1.64] Total mass of the system</description><unit>solMass</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Mrat</name><description>[0.01/1] Mass ratio M_Comp_/M_Host_</description><unit>solMass</unit><ucd>phys.mass;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Ebind</name><description>[0.1/21]? Binding energy (in units of 10^41^ erg)</description><unit>2.4e30W.h</unit><ucd>phys.energy</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>tau</name><description>[2/14]? Estimated dissipation lifetime of the system {tau} (2)</description><unit>Gyr</unit><ucd>time.lifetime</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column></table></schema></tableset></ri:Resource>