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<ri:Resource created="2017-09-01T10:36:54Z" 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>Bright white dwarfs IRAC photometry</title><shortName>J/MNRAS/459/1415</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/459/1415</identifier><altIdentifier>doi:10.26093/cds/vizier.74591415</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Barber S.D.</name></creator><creator><name>Belardi C.</name></creator><creator><name>Kilic M.</name></creator><creator><name>Gianninas A.</name></creator><date role="Updated">2024-08-16T20:16:44Z</date><date role="Created">2017-09-01T10:36:54Z</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>millimeter-astronomy</subject><subject>photometry</subject><subject>submillimeter-astronomy</subject><description>We cross-correlate several sources of archival photometry for 1265 bright (V~16mag) white dwarfs (WDs) with available high signal-to-noise spectroscopy. We find 381 WDs with archival Spitzer+IRAC data and investigate this subsample for infrared excesses due to circumstellar dust. This large data set reveals 15 dusty WDs, including three new debris discs and the hottest WD known to host dust (WD 0010+280). We study the frequency of debris discs at WDs as function of mass. The frequency peaks at 12.5 per cent for 0.7-0.75M_{sun}_ WDs (with 3M_{sun}_ main-sequence star progenitors) and falls off for stars more massive than this, which mirrors predicted planet occurrence rates for stars of different masses.</description><source format="bibcode">2016MNRAS.459.1415B</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/459/1415</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/J/ApJ/657/1013">J/ApJ/657/1013 : 2MASS/Spitzer white dwarfs IR photometry (Tremblay+, 2007)</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/ApJ/760/26">J/ApJ/760/26 : DA white dwarfs infrared photometry (Barber+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/146/34">J/AJ/146/34 : LAMOST DA white dwarfs infrared photometry (Zhang+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/743/138">J/ApJ/743/138 : Bright white dwarfs spectroscopic survey (Gianninas+, 2011)</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/MNRAS/459/1415</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/459/1415</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South 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