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<ri:Resource created="2023-07-19T11:42:29Z" status="active" updated="2025-05-19T09:50:00Z" version="1.2" 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/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>Discovery of an L dwarf co-moving BD+60 1417</title><shortName>J/ApJ/923/48</shortName><identifier>ivo://CDS.VizieR/J/ApJ/923/48</identifier><altIdentifier>doi:10.26093/cds/vizier.19230048</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Faherty J.K.</name></creator><creator><name>Gagne J.</name></creator><creator><name>Popinchalk M.</name></creator><creator><name>Vos J.M.</name></creator><creator><name>Burgasser A.J.,Schumann J.</name></creator><creator><name>Schneider A.C.</name></creator><creator><name>Kirkpatrick J.D.</name></creator><creator><name>Meisner A.M.</name></creator><creator><name>Kuchner M.J.,Bardalez Gagliuffi D.C.</name></creator><creator><name>Marocco F.</name></creator><creator><name>Caselden D.</name></creator><creator><name>Gonzales E.C.,Rothermich A.</name></creator><creator><name>Casewell S.L.</name></creator><creator><name>Debes J.H.</name></creator><creator><name>Aganze C.</name></creator><creator><name>Ayala A.</name></creator><creator><name>Hsu C.-C.,Cooper W.J.</name></creator><creator><name>Smart R.L.</name></creator><creator><name>Gerasimov R.</name></creator><creator><name>Theissen C.A.,The Backyard Worlds: Planet 9 Collaboration</name></creator><date role="Updated">2023-11-03T12:19:07Z</date><date role="Created">2023-07-19T11:42:29Z</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>brown-dwarfs</subject><subject>l-dwarfs</subject><subject>multiple-stars</subject><subject>infrared-astronomy</subject><subject>spectroscopy</subject><subject>visible-astronomy</subject><subject>k-stars</subject><description>Through the Backyard Worlds: Planet 9 citizen science project we discovered a late-type L dwarf co-moving with the young K0 star BD+60 1417 at a projected separation of 37" or 1662au. The secondary-CWISER J124332.12+600126.2 (W1243)-is detected in both the CatWISE2020 and 2MASS reject tables. The photometric distance and CatWISE proper motion both match that of the primary within ~1{sigma} and our estimates for a chance alignment yield a zero probability. Follow-up near-infrared spectroscopy reveals W1243 to be a very red 2MASS (J-Ks=2.72), low surface gravity source that we classify as L6-L8{gamma}. Its spectral morphology strongly resembles that of confirmed late-type L dwarfs in 10-150Myr moving groups as well as that of planetary mass companions. The position on near- and mid-infrared color-magnitude diagrams indicates the source is redder and fainter than the field sequence, a telltale sign of an object with thick clouds and a complex atmosphere. For the primary we obtained new optical spectroscopy and analyzed all available literature information for youth indicators. We conclude that the LiI abundance, its loci on color-magnitude and color-color diagrams, and the rotation rate revealed in multiple TESS sectors are all consistent with an age of 50-150Myr. Using our re-evaluated age of the primary and the Gaia parallax, along with the photometry and spectrum for W1243, we find Teff=1303+/-31K, log g=4.3+/-0.17cm/s^2^, and a mass of 15+/-5MJup. We find a physical separation of ~1662au and a mass ratio of ~0.01 for this system. Placing it in the context of the diverse collection of binary stars, brown dwarfs, and planetary companions, the BD+60 1417 system falls in a sparsely sampled area where the formation pathway is difficult to assess.</description><source format="bibcode">2021ApJ...923...48F</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/923/48</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>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/I/259">I/259 : The Tycho-2 Catalogue (Hog+ 2000)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/246">II/246 : 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/365">II/365 : The CatWISE2020 catalog (updated version 28-Jan-2021) (Marocco+, 2021)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/IV/39">IV/39 : TESS Input Catalog version 8.2 (TIC v8.2) (Paegert+, 2021)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/other/ARA+A/43.195">J/other/ARA+A/43.195 : L and T dwarf stars (Kirkpatrick, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/670/1367">J/ApJ/670/1367 : Gemini Deep Planet Survey (Lafreniere+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/676/1281">J/ApJ/676/1281 : L and T dwarfs in 2MASS/SDSS (Metchev+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/181/62">J/ApJS/181/62 : Survey of young solar analogs (Metchev+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/517/A76">J/A+A/517/A76 : Near-IR spectrum of 2M1207b (Patience+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/190/1">J/ApJS/190/1 : A survey of stellar families (Raghavan+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/752/56">J/ApJ/752/56 : BDKP. 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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>lambda</name><description>Wavelength</description><unit>um</unit><ucd>em.wl</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Flux</name><description>Flux in erg/s/cm^2^/{AA}</description><unit>cW.m**-2.nm**-1</unit><ucd>phot.flux</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_Flux</name><description>Uncertainty in Flux</description><unit>cW.m**-2.nm**-1</unit><ucd>stat.error;phot.flux</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column></table><table><name>J/ApJ/923/48/fig6</name><description>The Kast optical spectrum of BD+60 1417</description><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>lambda</name><description>Wavelength; Angstroms</description><unit>0.1nm</unit><ucd>em.wl</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Flux</name><description>Flux in erg/s/cm^2^/{AA}</description><unit>cW.m**-2.nm**-1</unit><ucd>phot.flux</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_Flux</name><description>Uncertainty in Flux</description><unit>cW.m**-2.nm**-1</unit><ucd>stat.error;phot.flux</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column></table></schema></tableset></ri:Resource>