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ivo-id="ivo://CDS">CDS</publisher><creator><name>Brusa M.</name></creator><creator><name>Comastri A.</name></creator><creator><name>Daddi E.</name></creator><creator><name>Pozzetti L.</name></creator><creator><name>Zamorani G.</name></creator><creator><name>Vignali C.,Cimatti A.</name></creator><creator><name>Fiore F.</name></creator><creator><name>Mignoli M.</name></creator><creator><name>Ciliegi P.</name></creator><creator><name>Rottgering H.J.A.</name></creator><date role="Updated">2005-04-02T21:41:29Z</date><date role="Created">2005-04-02T21:41:14Z</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>infrared-sources</subject><subject>photometry</subject><description>We present the results of a deep (about 80ks) XMM-Newton survey of the largest sample of near-infrared selected 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