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<ri:Resource created="2014-08-22T13:31:29Z" 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>WISE/NEOWISE observations of main belt asteroids</title><shortName>J/ApJ/759/L8</shortName><identifier>ivo://CDS.VizieR/J/ApJ/759/L8</identifier><altIdentifier>doi:10.26093/cds/vizier.17599008</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Masiero J.R.</name></creator><creator><name>Mainzer A.K.</name></creator><creator><name>Grav T.</name></creator><creator><name>Bauer J.M.</name></creator><creator><name>Cutri R.M.</name></creator><creator><name>Nugent C.,Cabrera M.S.</name></creator><date role="Updated">2017-10-12T12:59:48Z</date><date role="Created">2014-08-22T13:31:29Z</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>asteroids</subject><subject>infrared-sources</subject><subject>surveys</subject><description>We present preliminary diameters and albedos for 13511 Main Belt asteroids (MBAs) that were observed during the 3-Band Cryo phase of the Wide-field Infrared Survey Explorer (WISE; after the outer cryogen tank was exhausted) and as part of the NEOWISE Post-Cryo Survey (after the inner cryogen tank was exhausted). With a reduced or complete loss of sensitivity in the two long wavelength channels of WISE, the uncertainty in our fitted diameters and albedos is increased to ~20% for diameter and ~40% for albedo. Diameter fits using only the 3.4 and 4.6 {mu}m channels are shown to be dependent on the literature optical H absolute magnitudes. These data allow us to increase the number of size estimates for large MBAs which have been identified as members of dynamical families. We present thermal fits for 14 asteroids previously identified as the parents of a dynamical family that were not observed during the fully cryogenic mission.</description><source format="bibcode">2012ApJ...759L...8M</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/759/L8</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/B/astorb">B/astorb : Orbits of Minor Planets (Bowell+ 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/190">II/190 : IRAS Minor Planet Survey (IMPS) (Tedesco 1992)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VII/91">VII/91 : IRAS Asteroid and Comet Survey (Veeder+ 1986)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/542/A11">J/A+A/542/A11 : Main-belt asteroids polarimetry. III (Canada-Assandri+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/545/A131">J/A+A/545/A131 : Photometry of 8 main belt asteroids (Marciniak+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/539/A115">J/A+A/539/A115 : Main-belt asteroids polarimetric survey II (Gil-Hutton+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/759/49">J/ApJ/759/49 : Jovian Trojan with WISE/NEOWISE: taxonomy (Grav+, 2012)</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/743/156">J/ApJ/743/156 : NEOWISE obs. of NEOs: preliminary results (Mainzer+, 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/741/68">J/ApJ/741/68 : Main Belt asteroids with WISE/NEOWISE. 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(Masiero+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/529/A86">J/A+A/529/A86 : Polarimetric survey of main-belt asteroids (Gil-Hutton+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/529/A107">J/A+A/529/A107 : Photometry of 4 main belt asteroids (Marciniak+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/498/313">J/A+A/498/313 : Photometry of 3 main belt asteroids (Marciniak+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/423/381">J/A+A/423/381 : Asteroidal I, J, K in the DENIS Survey (Baudrand+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/123/2070">J/AJ/123/2070 : ISO deep asteroid search (Tedesco+, 2002)</relatedResource><relatedResource>http://www.minorplanetcenter.net/ : Minor Planet Center home page</relatedResource><relatedResource>http://wise2.ipac.caltech.edu/docs/release/3band/ : WISE 3-Band Cryo release</relatedResource><relatedResource>http://wise2.ipac.caltech.edu/docs/release/postcryo_prelim/ : NEOWISE Post-Cryo</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/759/L8</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/759/L8</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/759/L8</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/759/L8</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/759/L8</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/759/L8</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></coverage><tableset><schema><name>default</name><table><name>J/ApJ/759/L8/table1</name><description>Thermal model fits for Main Belt Asteroids in the 3-Band Cryo and NEOWISE Post-Cryo Survey</description><column><name>Name</name><description>Simbad column added by the CDS</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="10*">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>MPC</name><description>Asteroid name, in MPC packed format</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="7*">char</dataType></column><column><name>HMag</name><description>[5.3/19.6]? Literature absolute H band magnitude</description><unit>mag</unit><ucd>phys.magAbs;em.IR.H</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>G</name><description>[0.01/0.5]? Magnitude slope parameter</description><ucd>arith.grad;stat.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Diam</name><description>[1/304] Asteroid diameter</description><unit>km</unit><ucd>phys.size.diameter</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Diam</name><description>The 1{sigma} uncertainty in Diam</description><unit>km</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>pV</name><description>[0.001/1]? Visible geometrical albedo</description><ucd>phys.albedo</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_pV</name><description>? The 1{sigma} uncertainty in pV</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>N1</name><description>[0/38] Number of WISE W1 (3.3um) band observations</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>N2</name><description>[0/66] Number of WISE W2 (4.6um) band observations</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>N3</name><description>[0/62] Number of WISE W3 (12um) band observations</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>M11</name><description>Display the data from Masiero+ 2011 (J/ApJ/741/68), if any</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column></table></schema></tableset></ri:Resource>