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<ri:Resource created="2010-02-05T11:31:10Z" 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>X-ray-UV relations in SDSS DR5 QSOs</title><shortName>J/ApJ/685/773</shortName><identifier>ivo://CDS.VizieR/J/ApJ/685/773</identifier><altIdentifier>doi:10.26093/cds/vizier.16850773</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Gibson R.R.</name></creator><creator><name>Brandt W.N.</name></creator><creator><name>Schneider D.P.</name></creator><date role="Updated">2018-01-05T08:56:00Z</date><date role="Created">2010-02-05T11:31:10Z</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>quasars</subject><subject>x-ray-sources</subject><subject>ultraviolet-astronomy</subject><subject>redshifted</subject><description>We analyze archived Chandra and XMM-Newton X-ray observations of 536 Sloan Digital Sky Survey (SDSS) Data Release 5 (DR5) quasars (QSOs) at 1.7&lt;=z&lt;=2.7 in order to characterize the relative UV and X-ray spectral properties of QSOs that do not have broad UV absorption lines (BALs). We constrain the fraction of X-ray-weak, non-BAL QSOs and find that such objects are rare; for example, sources underluminous by a factor of 10 comprise &lt;~2% of optically selected SDSS QSOs. X-ray luminosities vary with respect to UV emission by a factor of &lt;~2 over several years for most sources. UV continuum reddening and the presence of narrow-line absorbing systems are not strongly associated with X-ray weakness in our sample. X-ray brightness is significantly correlated with UV emission-line properties, so that relatively X-ray-weak, non-BAL QSOs generally have weaker, blueshifted CIV {lambda}1549 emission and broader CIII] {lambda}1909 lines. The CIV emission-line strength depends on both UV and X-ray luminosity, suggesting that the physical mechanism driving the global Baldwin effect is also associated with X-ray emission.</description><source format="bibcode">2008ApJ...685..773G</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/685/773</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/252">VII/252 : SDSS-DR5 quasar catalog (Schneider+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/133/313">J/AJ/133/313 : AGN from RASS and SDSS DR5 (Anderson+, 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