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<ri:Resource created="2005-04-26T21:43:46Z" 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>XMM-Newton/2dF survey. II.</title><shortName>J/MNRAS/349/135</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/349/135</identifier><altIdentifier>doi:10.26093/cds/vizier.73490135</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Georgakakis A.</name></creator><creator><name>Georgantopoulos I.</name></creator><creator><name>Vallbe M.</name></creator><creator><name>Kolokotronis V.,Basilakos S.</name></creator><creator><name>Plionis M.</name></creator><creator><name>Stewart G.C.</name></creator><creator><name>Shanks T.</name></creator><creator><name>Boyle B.J.</name></creator><date role="Updated">2024-06-29T20:14:52Z</date><date role="Created">2005-04-26T21:43:46Z</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>surveys</subject><subject>x-ray-sources</subject><subject>astronomical-object-identification</subject><description>In this paper we investigate the properties of low X-ray-to-optical flux ratio sources detected in a wide-area (2.5{deg}^2^) shallow [fX(0.5-8keV)~10^-14^erg/s/cm^2^] XMM-Newton survey. We find a total of 26 sources (5 per cent of the total X-ray-selected population) with log(fX)/f(opt)&lt;-0.9 to the above flux limit. Optical spectroscopy is available for 20 of these low X-ray-to-optical flux ratio objects.</description><source format="bibcode">2004MNRAS.349..135G</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/349/135</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/VII/226">VII/226 : 2dF Galaxy Redshift Survey 100k Data Release (2dFGRS Team, 2001)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/B/xmm">B/xmm : XMM-Newton Observation Log (XMM-Newton SOC, 2002)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/IX/37">IX/37 : XMM-Newton Serendipitous Source Catalogue (1XMM) (XMM-SSC, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/352/91">J/MNRAS/352/91 : XMM-Newton/2dF survey. 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