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<ri:Resource created="2026-01-22T08:13:24Z" status="active" updated="2026-03-02T06:25:50Z" 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>Asteroid masses obtained in INPOP25c</title><shortName>J/A+A/705/A189</shortName><identifier>ivo://CDS.VizieR/J/A+A/705/A189</identifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Mariani V.</name></creator><creator><name>Fienga A.</name></creator><creator><name>Murray Z.</name></creator><creator><name>Gastineau M.</name></creator><creator><name>Laskar J.</name></creator><date role="Updated">2026-03-02T06:25:50Z</date><date role="Created">2026-01-22T08:13:24Z</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>astronomical-models</subject><description>One of the main bottleneck in assessing the accuracy of Mars orbit is the unknown value of the asteroids in the Main Asteroid Belt. Nowadays a modeling with 343 asteroids as point masses is used, with the relative masses fitted to observational data. In the current work we propose an innovative methodology to reduce the number of asteroids implemented as point masses, thus reducing the number of parameters to be fitted, without a significant degradation of the postfit residuals. We use boosting decision trees to get a ranking by relative importance of the 343 asteroids of the current Main Belt modeling. We have been able to remove more than 100 of them without significantly degrading the postfit residuals and with a significant improvement of the uncertainties. Furthermore, we verified that the postfit masses found with the new modeling (INPOP25c) are consistent with respect to mass estimation found with an independent approach by means of albedo properties of the asteroids.</description><source format="bibcode">2026A&amp;A...705A.189M</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/705/A189</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></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/A+A/705/A189</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/705/A189</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/705/A189</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/705/A189</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/705/A189</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/705/A189</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/A+A/705/A189/tablea1</name><description>Postfit masses, sigmas, ranking position and Wasserstein barycenters for asteroids in INPOP25c</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>MPC</name><description>MPC number to identify the asteroid (MPC_num)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>massINPOP25c</name><description>Postfit mass INPOP25c (mass_INPOP25c)</description><unit>kg</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>sigmaINPOP25c</name><description>Postfit sigma INPOP25c (sigma_INPOP25c)</description><unit>kg</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>sigmratio</name><description>Sigma over mass ratio (postfit) INPOP25c (sig_m_ratio)</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>meanWass</name><description>Mean of the Wasserstein barycenter (mean_Wass)</description><unit>kg</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>sigmaWass</name><description>Sigma of the Wasserstein barycenter (sigma_Wass)</description><unit>kg</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Ranking</name><description>Position in the ranking (Ranking)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column></table><table><name>J/A+A/705/A189/tablea2</name><description>Ranking for the full list of 343 asteroids of INPOP21a</description><column><name>MPC</name><description>MPC number to identify the asteroid (MPC_num)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>recno</name><description>Record number assigned by the VizieR team. 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