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<ri:Resource created="2016-03-14T14:49:55Z" status="active" updated="2025-05-19T09:50:00Z" version="1.2" xmlns:cs="http://www.ivoa.net/xml/ConeSearch/v1.0" 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/ConeSearch/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/ConeSearch.xsd 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>Autoclassification of the variable 3XMM sources</title><shortName>J/ApJ/813/28</shortName><identifier>ivo://CDS.VizieR/J/ApJ/813/28</identifier><altIdentifier>doi:10.26093/cds/vizier.18130028</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Farrell S.A.</name></creator><creator><name>Murphy T.</name></creator><creator><name>Lo K.K.</name></creator><date role="Updated">2017-01-23T22:00:00Z</date><date role="Created">2016-03-14T14:49:55Z</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>x-ray-sources</subject><description>In the current era of large surveys and massive data sets, autoclassification of astrophysical sources using intelligent algorithms is becoming increasingly important. In this paper we present the catalog of variable sources in the Third XMM-Newton Serendipitous Source catalog (3XMM) autoclassified using the Random Forest machine learning algorithm (RF). We used a sample of manually classified variable sources from the second data release of the XMM-Newton catalogs (2XMMi-DR2) to train the classifier, obtaining an accuracy of ~92%. We also evaluated the effectiveness of identifying spurious detections using a sample of spurious sources, achieving an accuracy of ~95%. Manual investigation of a random sample of classified sources confirmed these accuracy levels and showed that the Random Forest machine learning algorithm is highly effective at automatically classifying 3XMM sources. Here we present the catalog of classified 3XMM variable sources. We also present three previously unidentified unusual sources that were flagged as outlier sources by the algorithm: a new candidate supergiant fast X-ray transient, a 400s X-ray pulsar, and an eclipsing 5hr binary system coincident with a known Cepheid.</description><source format="bibcode">2015ApJ...813...28F</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/813/28</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>IsServedBy</relationshipType><relatedResource>Conesearch service</relatedResource></relationship><relationship><relationshipType>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/B/xmm">B/xmm : XMM-Newton Observation Log (XMM-Newton Science Operation Center, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/IX/46">IX/46 : XMM-Newton Serendipitous Source Catalogue 3XMM-DR5 (XMM-SSC, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/IX/44">IX/44 : XMM-Newton Serendipitous Source Catalogue 3XMM-DR4 (XMM-SSC, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/414/2602">J/MNRAS/414/2602 : Automated classification of HIP variables (Dubath+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/493/339">J/A+A/493/339 : XMM-Newton serendipitous Survey. 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