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<ri:Resource created="2017-04-07T15:50:30Z" 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>NIR albedos of main-belt asteroids</title><shortName>J/ApJ/791/121</shortName><identifier>ivo://CDS.VizieR/J/ApJ/791/121</identifier><altIdentifier>doi:10.26093/cds/vizier.17910121</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Masiero J.R.</name></creator><creator><name>Grav T.</name></creator><creator><name>Mainzer A.K.</name></creator><creator><name>Nugent C.R.</name></creator><creator><name>Bauer J.M.</name></creator><creator><name>Stevenson R.,Sonnett S.</name></creator><date role="Updated">2018-01-02T13:43:07Z</date><date role="Created">2017-04-07T15:50:30Z</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>asteroids</subject><description>We present revised near-infrared albedo fits of 2835 main-belt asteroids observed by WISE/NEOWISE over the course of its fully cryogenic survey in 2010. These fits are derived from reflected-light near-infrared images taken simultaneously with thermal emission measurements, allowing for more accurate measurements of the near-infrared albedos than is possible for visible albedo measurements. Because our sample requires reflected light measurements, it undersamples small, low-albedo asteroids, as well as those with blue spectral slopes across the wavelengths investigated. We find that the main belt separates into three distinct groups of 6%, 16%, and 40% reflectance at 3.4 {mu}m. Conversely, the 4.6 {mu}m albedo distribution spans the full range of possible values with no clear grouping. Asteroid families show a narrow distribution of 3.4 {mu}m albedos within each family that map to one of the three observed groupings, with the (221) Eos family being the sole family associated with the 16% reflectance 3.4 {mu}m albedo group. We show that near-infrared albedos derived from simultaneous thermal emission and reflected light measurements are important indicators of asteroid taxonomy and can identify interesting targets for spectroscopic follow-up.</description><source format="bibcode">2014ApJ...791..121M</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/791/121</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/J/ApJ/741/68">J/ApJ/741/68 : Main Belt asteroids with WISE/NEOWISE. I. (Masiero+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/770/7">J/ApJ/770/7 : WISE/NEOWISE Main Belt asteroids: family members</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/578/A42">J/A+A/578/A42 : Main Belt asteroids observed by Spitzer (Ryan+, 2015)</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/ApJ/791/121</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/791/121</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/791/121</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/791/121</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/791/121</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/791/121</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><coverage><footprint ivo-id="ivo://ivoa.net/std/moc"/></coverage><tableset><schema><name>default</name><table><name>J/ApJ/791/121/table1</name><description>Revised thermal fits of Main Belt asteroids</description><column><name>OName</name><description>Simbad column added by the CDS</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="7*">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>Asteroid number, MPC-packed format</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="5*">char</dataType></column><column><name>Dia</name><description>Diameter</description><unit>km</unit><ucd>phys.size.diameter</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Dia</name><description>Uncertainty in Dia</description><unit>km</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>eta</name><description>Beaming parameter</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_eta</name><description>Uncertainty in eta</description><ucd>stat.error;phys.electron.degen</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>pV</name><description>Visible albedo</description><ucd>phys.albedo</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_pV</name><description>Uncertainty in pV</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>pW1</name><description>WISE 3.4 micron band albedo</description><ucd>phys.albedo</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_pW1</name><description>Uncertainty in pW1</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>pW2</name><description>? 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