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<ri:Resource created="2005-04-22T15:44:47Z" 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>Redshifts for X-ray selected AGNs</title><shortName>J/A+A/434/475</shortName><identifier>ivo://CDS.VizieR/J/A+A/434/475</identifier><altIdentifier>doi:10.26093/cds/vizier.34340475</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Kitsionas S.</name></creator><creator><name>Hatziminaoglou E.</name></creator><creator><name>Georgakakis A.</name></creator><creator><name>Georgantopoulos I.</name></creator><date role="Updated">2017-11-10T11:15:54Z</date><date role="Created">2005-04-22T15:44:47Z</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>quasars</subject><subject>active-galactic-nuclei</subject><subject>redshifted</subject><subject>visible-astronomy</subject><subject>sloan-photometry</subject><description>We present photometric redshift estimates for X-ray selected sources detected in the XMM/2dF survey. 5-band photometry for 193 sources has been obtained from the SDSS. We exclude 10 sources associated with Galactic stars. The tabulated data include the optical coordinate of all sources in our sample, their photometric redshift estimate, their r-band magnitude and g-r colour as well as their morphological classification (these optical parameters have been used in the discussion of our results). Spectroscopic redshifts are available only for a sub-sample of our data and are included in Table 1 together with the survey from which they have been obtained.</description><source format="bibcode">2005A&amp;A...434..475K</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/434/475</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/J/MNRAS/349/135">J/MNRAS/349/135 : XMM-Newton/2dF survey. II. 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