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<ri:Resource created="2016-08-08T06:16:45Z" 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 observations of 105 near-Earth objects</title><shortName>J/ApJ/784/110</shortName><identifier>ivo://CDS.VizieR/J/ApJ/784/110</identifier><altIdentifier>doi:10.26093/cds/vizier.17840110</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Mainzer A.</name></creator><creator><name>Bauer J.</name></creator><creator><name>Grav T.</name></creator><creator><name>Masiero J.</name></creator><creator><name>Cutri R.M.</name></creator><creator><name>Wright E.,Nugent C.R.</name></creator><creator><name>Stevenson R.</name></creator><creator><name>Clyne E.</name></creator><creator><name>Cukrov G.</name></creator><creator><name>Masci F.</name></creator><date role="Updated">2018-01-05T08:56:57Z</date><date role="Created">2016-08-08T06:16:45Z</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>surveys</subject><subject>asteroids</subject><subject>infrared-photometry</subject><description>Only a very small fraction of the asteroid population at size scales comparable to the object that exploded over Chelyabinsk, Russia has been discovered to date, and physical properties are poorly characterized. We present previously unreported detections of 105 close approaching near-Earth objects (NEOs) by the Wide-field Infrared Survey Explorer (WISE) mission's NEOWISE project. These infrared observations constrain physical properties such as diameter and albedo for these objects, many of which are found to be smaller than 100m. Because these objects are intrinsically faint, they were detected by WISE during very close approaches to the Earth, often at large apparent on-sky velocities. We observe a trend of increasing albedo with decreasing size, but as this sample of NEOs was discovered by visible light surveys, it is likely that selection biases against finding small, dark NEOs influence this finding.</description><source format="bibcode">2014ApJ...784..110M</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/784/110</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+ 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/328">II/328 : AllWISE Data Release (Cutri+ 2013)</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/ApJ/770/7">J/ApJ/770/7 : WISE/NEOWISE Main Belt asteroids (Masiero+, 2013)</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/759/L8">J/ApJ/759/L8 : WISE/NEOWISE obs. of main belt asteroids (Masiero+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/759/49">J/ApJ/759/49 : Jovian Trojan asteroids with WISE/NEOWISE (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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Absolute H band magnitude (1)</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>[0.15] Phase curve slope parameter (1)</description><ucd>arith.grad;stat.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Diam</name><description>[0.008/1.9] Diameter (D) (1)</description><unit>km</unit><ucd>phys.size.diameter</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Diam</name><description>[0.001/0.41] 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>[0.01/0.61]? Visible albedo (p_V_) (1)</description><ucd>phys.albedo</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_pV</name><description>[0/0.33]? The 1{sigma} uncertainty in pV</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>eta</name><description>[0.75/3.2] Beaming parameter ({eta}) (1)</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_eta</name><description>[0.025/0.61] The 1{sigma} uncertainty in eta</description><ucd>stat.error;phys.electron.degen</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>pIR</name><description>[0.01/0.93] Infrared albedo (p_IR_) (1)</description><ucd>phys.albedo</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_pIR</name><description>[0/0.43] The 1{sigma} uncertainty in pIR</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table><table><name>J/ApJ/784/110/table1</name><description>Observed WISE magnitudes for each of the Near-Earth Objects (NEOs) presented here, including the Modified Julian Date (MJD)</description><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>Source name</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="7*">char</dataType><flag>primary</flag></column><column><name>f_Name</name><description>[*] Flag on Name (*=stacked object) (1)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>P</name><description>Simbad column added by the CDS</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>MJD</name><description>[55203.4/55571.4] Modified Julian Date of observation</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>l_W1mag</name><description>[&gt;] The 2{sigma} upper limit flag on W1mag (2)</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>W1mag</name><description>[10.8/17.3] WISE 3.4{mu}m band magnitude</description><unit>mag</unit><ucd>phot.mag;em.IR.3-4um</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_W1mag</name><description>[0.02/0.52]? 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