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<ri:Resource created="2018-08-02T12:54:22Z" 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>NEOWISE: thermal model fits for NEOs and MBAs</title><shortName>J/AJ/154/168</shortName><identifier>ivo://CDS.VizieR/J/AJ/154/168</identifier><altIdentifier>doi:10.26093/cds/vizier.51540168</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Masiero J.R.</name></creator><creator><name>Nugent C.</name></creator><creator><name>Mainzer A.K.</name></creator><creator><name>Wright E.L.</name></creator><creator><name>Bauer J.M.</name></creator><creator><name>Cutri R.M.,Grav T.</name></creator><creator><name>Kramer E.</name></creator><creator><name>Sonnett S.</name></creator><date role="Updated">2018-08-27T07:51:00Z</date><date role="Created">2018-08-02T12:54:22Z</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>solar-system</subject><subject>asteroids</subject><subject>infrared-photometry</subject><subject>galaxy-classification-systems</subject><subject>surveys</subject><description>The Near-Earth ObjectWide-field Infrared Survey Explorer (NEOWISE) reactivation mission has completed its third year of surveying the sky in the thermal infrared for near-Earth asteroids and comets. NEOWISE collects simultaneous observations at 3.4 and 4.6 {mu}m of solar system objects passing through its field of regard. These data allow for the determination of total thermal emission from bodies in the inner solar system, and thus the sizes of these objects. In this paper, we present thermal model fits of asteroid diameters for 170 NEOs and 6110 Main Belt asteroids (MBAs) detected during the third year of the survey, as well as the associated optical geometric albedos. We compare our results with previous thermal model results from NEOWISE for overlapping sample sets, as well as diameters determined through other independent methods, and find that our diameter measurements for NEOs agree to within 26% (1{sigma}) of previously measured values. Diameters for the MBAs are within 17% (1{sigma}). This brings the total number of unique near-Earth objects characterized by the NEOWISE survey to 541, surpassing the number observed during the fully cryogenic mission in 2010.</description><source format="bibcode">2017AJ....154..168M</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/154/168</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/742/40">J/ApJ/742/40 : Jovian Trojans asteroids with WISE/NEOWISE (Grav+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/743/156">J/ApJ/743/156 : NEOWISE observations of NEOs: preliminary results</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/744/197">J/ApJ/744/197 : WISE/NEOWISE observations of Hilda asteroids (Grav+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/759/L8">J/ApJ/759/L8 : WISE/NEOWISE observations of main belt asteroids</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/760/L12">J/ApJ/760/L12 : WISE/NEOWISE NEOs preliminary thermal fits (Mainzer+, 2012)</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/ApJ/791/121">J/ApJ/791/121 : NIR albedos of main-belt asteroids (Masiero+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/792/30">J/ApJ/792/30 : NEOWISE magnitudes for near-Earth objects (Mainzer+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/814/117">J/ApJ/814/117 : NEOWISE Reactivation mission: 1st yr data (Nugent+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/152/63">J/AJ/152/63 : NEOWISE reactivation mission: 2nd yr data (Nugent+, 2016)</relatedResource><relatedResource>http://minorplanetcenter.net/ : IAU Minor Planet Center home page</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/154/168</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/AJ/154/168</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/AJ/154/168</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/AJ/154/168</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/AJ/154/168</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/AJ/154/168</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"/><waveband>Infrared</waveband><waveband>Optical</waveband></coverage><tableset><schema><name>default</name><table><name>J/AJ/154/168/table1</name><description>Thermal model fits for NEOs in the third year of the NEOWISE survey</description><column><name>NW1</name><description>[0/92] Number of unsaturated W1 band observations (3)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>NW2</name><description>[4/104] Number of unsaturated W2 band observations (3)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</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>Object identifier (1)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="7*">char</dataType></column><column><name>HMag</name><description>[6.74/25.2] Absolute visual magnitude (2)</description><unit>mag</unit><ucd>phys.magAbs;em.IR.H</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>G</name><description>[-0.27/0.82] Photometric slope parameter</description><ucd>arith.grad;stat.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Diam</name><description>[0.086/216.061] Diameter</description><unit>km</unit><ucd>phys.size.diameter</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Diam</name><description>[0.002/72.296] Uncertainty in Diam</description><unit>km</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>logpV</name><description>[-1.964/-0.112] Log of the visible albedo</description><ucd>phys.albedo</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_logpV</name><description>[0.023/0.603] Uncertainty in logpV</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>eta</name><description>[0.3/2.724] Beaming parameter {eta}</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_eta</name><description>[0/0.605] Uncertainty in eta</description><ucd>stat.error;phys.electron.degen</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Phase</name><description>[16.32/84.34] Phase angle</description><unit>deg</unit><ucd>pos.phaseAng</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Fitted</name><description>[0/1] Fitted beaming? 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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>Name</name><description>Object identifier (1)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="7*">char</dataType></column><column><name>HMag</name><description>[6.74/25.2] Absolute visual magnitude (2)</description><unit>mag</unit><ucd>phys.magAbs;em.IR.H</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>G</name><description>[-0.27/0.82] Photometric slope parameter</description><ucd>arith.grad;stat.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Diam</name><description>[0.086/216.061] Diameter</description><unit>km</unit><ucd>phys.size.diameter</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Diam</name><description>[0.002/72.296] Uncertainty in Diam</description><unit>km</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>logpV</name><description>[-1.964/-0.112] Log of the visible albedo</description><ucd>phys.albedo</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_logpV</name><description>[0.023/0.603] Uncertainty in logpV</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>eta</name><description>[0.3/2.724] Beaming parameter {eta}</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_eta</name><description>[0/0.605] Uncertainty in eta</description><ucd>stat.error;phys.electron.degen</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>NW1</name><description>[0/92] Number of unsaturated W1 band observations (3)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>NW2</name><description>[4/104] Number of unsaturated W2 band observations (3)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Phase</name><description>[16.32/84.34] Phase angle</description><unit>deg</unit><ucd>pos.phaseAng</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Fitted</name><description>[0/1] Fitted beaming? 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