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<ri:Resource created="2012-11-04T19:17:16Z" 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>A catalogue of cross-matched radio/infrared/X-ray sources</title><shortName>V/138</shortName><identifier>ivo://CDS.VizieR/V/138</identifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Combi J.A.</name></creator><creator><name>Albacete-Colombo J.F.</name></creator><creator><name>Pellizza L.</name></creator><creator><name>Lopez-Santiago J.,Romero G.E.</name></creator><creator><name>Marti J.</name></creator><creator><name>Munoz-Arjonilla A.J.</name></creator><creator><name>Sanchez-Ayaso E.,Luque-Escamilla P.L.</name></creator><creator><name>Sanchez-Sutil J.R.</name></creator><date role="Updated">2018-01-04T08:22:38Z</date><date role="Created">2012-11-04T19:17:16Z</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><subject>radio-sources</subject><subject>infrared-sources</subject><subject>astronomical-object-identification</subject><description>We present a catalog of cross-correlated radio, infrared and X-ray sources using a very restrictive selection criteria with an IDL-based code developed by us. The significance of the observed coincidences was evaluated through Monte Carlo simulations of synthetic sources following a well-tested protocol. We found 3320 coincident radio/X-ray sources with a high statistical significance characterized by the sum of error-weighted coordinate differences. For 997 of them, 2MASS counterparts were found. The percentage of chance coincidences is less than 1%. X-ray hardness ratios of well-known populations of objects were used to provide a crude representation of their X-ray spectrum and to make a preliminary diagnosis of the possible nature of unidentified X-ray sources. The results support the fact that the X-ray sky is largely dominated by Active Galactic Nuclei at high galactic latitudes (|b|&gt;=10deg). At low galactic latitudes (|b|&lt;=10deg) most of unidentified X-ray sources (~94%) lie at |b|&gt;=2deg. This result suggests that most of the unidentified sources found toward the Milky Way plane are galactic objects. Well-known and unidentified sources were classified in different tables with their corresponding radio/infrared and X-ray properties. 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xsi:type="vs:VOTableType" arraysize="13*">char</dataType></column><column><name>recno</name><description>Record number assigned by the VizieR team. 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