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<ri:Resource created="2024-06-05T06:26:17Z" status="active" updated="2026-07-02T11:44:45Z" 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>RATIR observations of 323 Near Earth Objects</title><shortName>J/AJ/167/163</shortName><identifier>ivo://CDS.VizieR/J/AJ/167/163</identifier><altIdentifier>doi:10.26093/cds/vizier.51670163</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Navarro-Meza S.</name></creator><creator><name>Trilling D.E.</name></creator><creator><name>Mommert M.</name></creator><creator><name>Butler N.</name></creator><creator><name>Reyes-Ruiz M.</name></creator><date role="Updated">2026-07-02T11:44:45Z</date><date role="Created">2024-06-05T06:26:17Z</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>visible-astronomy</subject><description>We present results from observations of 238 near-Earth objects (NEOs) obtained with the RATIR instrument on the 1.5m robotic telescope at San Pedro Martir's National Observatory in Mexico, in the frame of our multiobservatory, multifilter campaign. Our project is focused on rapid response photometric observations of NEOs with absolute magnitudes in the range 18.1-27.1 (diameter~600 and 10m, respectively). Data with coverage in the near-infrared and visible range were analyzed with a nonparametric classification algorithm, while visible-only data were independently analyzed via Monte Carlo simulations and a 1-Nearest Neighbor method. The rapid response and the use of spectrophotometry allows us to obtain taxonomic classifications of subkilometer objects with small telescopes, representing a convenient characterization strategy. We present taxonomic classifications of the 87 objects observed in the visible and near-infrared. We also present the taxonomic distribution of an additional 151 objects observed in the visible. Our most accurate method suggests a nonfeatured-to-featured ratio of ~0.75, which is consistent with the value found by the Mission Accessible Near-Earth Object Survey, which conducted a similar study using a spectral analysis. The results from the Monte Carlo method suggest a ratio of ~0.8, although this method has some limitations. The 1-Nearest Neighbor method showed to be not suitable for NEO classifications.</description><source format="bibcode">2024AJ....167..163N</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/167/163</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/AJ/154/162">J/AJ/154/162 : KMTNet-SAAO observation of nearEarth asteroids (Erasmus+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/158/196">J/AJ/158/196 : Near-Earth Object Survey (MANOS) spectroscopy (Devogele+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/247/13">J/ApJS/247/13 : ATLAS c-o colors &amp; classification of asteroids (Erasmus+, 2020)</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/167/163</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/AJ/167/163</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/AJ/167/163</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/AJ/167/163</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/AJ/167/163</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/AJ/167/163</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>Optical</waveband><waveband>Infrared</waveband></coverage><tableset><schema><name>default</name><table><name>J/AJ/167/163/table4</name><description>Observed targets analized with k-NN and a probability of belonging to a taxonomy larger than 50%</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>ID</name><description>Object identifier</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="10*">char</dataType></column><column><name>Date</name><description>Midtime of the observation; YYYY-MM-DD hh:mm</description><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType" arraysize="16*">char</dataType></column><column><name>Dur</name><description>Observation duration</description><unit>h</unit><ucd>time.duration;obs</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>VMAG</name><description>Absolute magnitude</description><unit>mag</unit><ucd>phys.magAbs</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>P(C+X)</name><description>? Probability belonging to non-featured C and X type</description><ucd>stat.fit.goodness</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>P(Q)</name><description>? Probability belonging to unweathered rocky Q type</description><ucd>stat.fit.goodness</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>P(S)</name><description>? Probability of belonging to rocky S type</description><ucd>stat.fit.goodness</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>P(D)</name><description>? Probability of belonging to D type</description><ucd>stat.fit.goodness</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>P(V)</name><description>? Probability of belonging to V type</description><ucd>stat.fit.goodness</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>Sets</name><description>[1/3] Set where this object belongs to</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column></table><table><name>J/AJ/167/163/table5</name><description>Equivalent to Table 4 for the objects which probability of belonging to a given taxonomy is less than 50%</description><column><name>ID</name><description>Object identifier</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. 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