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<ri:Resource created="2024-02-09T06:24:58Z" 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>7 white dwarfs systems J-, H-, and K-band spectroscopy</title><shortName>J/AJ/166/5</shortName><identifier>ivo://CDS.VizieR/J/AJ/166/5</identifier><altIdentifier>doi:10.26093/cds/vizier.51660005</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Owens D.</name></creator><creator><name>Xu S.</name></creator><creator><name>Manjavacas E.</name></creator><creator><name>Leggett S.K.</name></creator><creator><name>Casewell S.L.</name></creator><creator><name>Dennihy E.,Dufour P.</name></creator><creator><name>Klein B.L.</name></creator><creator><name>Yeh S.</name></creator><creator><name>Zuckerman B.</name></creator><date role="Updated">2024-11-06T20:18:47Z</date><date role="Created">2024-02-09T06:24:58Z</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>white-dwarf-stars</subject><subject>infrared-astronomy</subject><subject>spectroscopy</subject><description>Excess infrared flux from white dwarf stars is likely to arise from a dusty debris disk or a cool companion. In this work, we present near-infrared spectroscopic observations with Keck/MOSFIRE, Gemini/GNIRS, and Gemini/Flamingos-2 of seven white dwarfs with infrared excesses identified in previous studies. We confirmed the presence of dust disks around four white dwarfs (GaiaJ0611-6931, GaiaJ0006+2858, GaiaJ2100+2122, and WD0145+234) as well as two new white dwarf-brown dwarf pairs (GaiaJ0052+4505 and GaiaJ0603+4518). In three of the dust disk systems, we detected for the first time near-infrared metal emissions (MgI, SiI, and possibly FeI) from a gaseous component of the disk. We developed a new Markov Chain Monte Carlo framework to constrain the geometric properties of each dust disk. In three systems, the dust disk and the gas disk appear to coincide spatially. For the two brown dwarf-white dwarf pairs, we identified broad molecular absorption features typically seen in L dwarfs. The origin of the infrared excess around GaiaJ0723+6301 remains a mystery. Our study underlines how near-infrared spectroscopy can be used to determine sources of infrared excess around white dwarfs, which has now been detected photometrically in hundreds of systems.</description><source format="bibcode">2023AJ....166....5O</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/166/5</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/354">I/354 : StarHorse2, Gaia EDR3 photo-astrometric distances (Anders+, 2022)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/131/2722">J/AJ/131/2722 : New L and T dwarfs from the SDSS (Chiu+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/663/1291">J/ApJ/663/1291 : DZ stars in SDSS DR4 (Dufour+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/197/38">J/ApJS/197/38 : The WIRED survey. 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(Debes+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/417/1210">J/MNRAS/417/1210 : DA-white dwarfs from SDSS and UKIDSS (Girven+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/449/574">J/MNRAS/449/574 : Circumstellar discs at white dwarfs (Rocchetto+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/898/84">J/ApJ/898/84 : Spectro follow-up of 100pc WDs in SDSS &amp; Gaia (Kilic+, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/902/127">J/ApJ/902/127 : Bright Gaia white dwarfs with unWISE photometry (Xu+, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/508/3877">J/MNRAS/508/3877 : Catalogue of white dwarfs in Gaia EDR3 (Gentile+, 2021)</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/AJ/166/5</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/AJ/166/5</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/AJ/166/5</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/AJ/166/5</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/AJ/166/5</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/AJ/166/5</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/AJ/166/5/table1 (White dwarf parameters)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/AJ/166/5/table1?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/AJ/166/5/table1?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/AJ/166/5/table1?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>1.644755</ra><dec>28.979655</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>6/2068 2682 6842 7727 13059 20328 37512</spatial><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/AJ/166/5?format=ascii</footprint><waveband>Infrared</waveband></coverage><tableset><schema><name>default</name><table><name>J/AJ/166/5/table1</name><description>White dwarf parameters</description><column><name>recno</name><description>Record number assigned by the VizieR team. 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