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<ri:Resource created="2006-06-02T09:29:40Z" 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. IV.</title><shortName>J/MNRAS/352/91</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/352/91</identifier><altIdentifier>doi:10.26093/cds/vizier.73520091</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Georgantopoulos I.</name></creator><creator><name>Georgakakis A.</name></creator><creator><name>Akylas A.</name></creator><creator><name>Stewart G.C.</name></creator><creator><name>Giannakis O.,Shanks T.</name></creator><creator><name>Kitsionas S.</name></creator><date role="Updated">2024-06-29T20:15:15Z</date><date role="Created">2006-06-02T09:29:40Z</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>radio-sources</subject><subject>quasars</subject><subject>active-galactic-nuclei</subject><description>We present an analysis of the X-ray spectral properties of 61 hard X-ray (2-8keV) selected sources from the bright XMM-Newton/2dF (f(2-8keV)&gt;10^-14^erg/cm^2^/s) survey. This comprises nine XMMNewton pointings in the North Galactic Pole region (~1.6deg^2^) and overlaps with the SDSS, 2QZ and 2dFGRS surveys. Our sources contribute about 50 per cent of the 2-10keV X-ray background down to the flux limit of 10^-14^erg/cm^2^/s. The hardness ratio distribution of the sample suggests a deficit of heavily absorbed sources. Spectroscopic identifications exist for 34 sources.</description><source format="bibcode">2004MNRAS.352...91G</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/352/91</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 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/VII/226">VII/226 : The 2dF Galaxy Redshift Survey 100k Data Release (2dFGRS, 2001)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/349/135">J/MNRAS/349/135 : XMM-Newton/2dF survey. 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Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>RAJ2000</name><description>X-ray right ascension (J2000)</description><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>X-ray declination (J2000)</description><ucd>pos.eq.dec;meta.main</ucd></column><column><name>CR</name><description>Counte rate at 2-8keV</description><unit>ct/s</unit><ucd>phot.count;em.X-ray</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>n_CR</name><description>[d] if count rate and flux from MOS; otherwise from PN instrument.</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>e_CR</name><description>rms uncertainty on CR</description><unit>ct/s</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Flux</name><description>Flux at 2-8keV (10^-14^erg/cm^2^/s)</description><unit>1e-17W.m**-2</unit><ucd>phot.flux;em.X-ray</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Flux</name><description>rms uncertainty on Flux</description><unit>1e-17W.m**-2</unit><ucd>stat.error;phot.flux</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>ExpTime</name><description>? 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