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<ri:Resource created="2016-06-22T09:41:54Z" status="active" updated="2025-06-13T15:25:00Z" 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>SDSS-DR7 QSOs with X-ray and UV luminosities</title><shortName>J/ApJ/819/154</shortName><identifier>ivo://CDS.VizieR/J/ApJ/819/154</identifier><altIdentifier>doi:10.26093/cds/vizier.18190154</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Lusso E.</name></creator><creator><name>Risaliti G.</name></creator><date role="Updated">2018-01-05T08:57:04Z</date><date role="Created">2016-06-22T09:41:54Z</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>redshifted</subject><subject>x-ray-sources</subject><subject>ultraviolet-astronomy</subject><subject>surveys</subject><description>The observed relation between the soft X-ray and the optical-ultraviolet emission in active galactic nuclei (AGNs) is nonlinear and it is usually parametrized as a dependence between the logarithm of the monochromatic luminosity at 2500{AA} and at 2keV. Previous investigations have found that the dispersion of this relation is rather high (~0.35-0.4 in log units), which may be caused by measurement uncertainties, variability, and intrinsic dispersion due to differences in the AGN physical properties (e.g., different accretion modes). We show that, once optically selected quasars with homogeneous SED and X-ray detection are selected, and dust reddened and/or gas obscured objects are not included, the measured dispersion drops to significantly lower values (i.e., ~0.21-0.24dex). We show that the residual dispersion is due to some extent to variability, and to remaining measurement uncertainties. Therefore, the real physical intrinsic dispersion should be &lt;0.21dex. Such a tight relation, valid over four decades in luminosity, must be the manifestation of an intrinsic (and universal) physical relation between the disk, emitting the primary radiation, and the hot electron corona emitting X-rays.</description><source format="bibcode">2016ApJ...819..154L</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/819/154</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/IX/46">IX/46 : XMM-Newton Serendipitous Source Catalogue 3XMM-DR5 (XMM-SSC, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VII/270">VII/270 : SDSS quasar catalog: tenth data release (Paris+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VII/260">VII/260 : The SDSS-DR7 quasar catalog (Schneider+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/PAZh/42/313">J/PAZh/42/313 : 3XMM-DR4 QSO candidates at 3&lt;z&lt;5.5 (Khorunzhev+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/815/33">J/ApJ/815/33 : A Hubble diagram for quasars (Risaliti+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/201/10">J/ApJS/201/10 : SDSS quasar catalog with Swift observations (Wu+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/746/54">J/ApJ/746/54 : Chandra X-ray observations of SDSS-DR5 QSOs (Gibson+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/726/20">J/ApJ/726/20 : X-ray emission from quasars (Miller+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/194/45">J/ApJS/194/45 : QSO properties from SDSS-DR7 (Shen+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/519/A17">J/A+A/519/A17 : X-ray/UV ratio of 2XMM AGN (Vagnetti+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/405/2302">J/MNRAS/405/2302 : Improved redshifts for SDSS quasar spectra (Hewett+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/512/A34">J/A+A/512/A34 : XMM-COSMOS Type 1 AGNs (Lusso+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/183/17">J/ApJS/183/17 : The SDSS DR5/XMM-Newton quasar survey (Young+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/692/758">J/ApJ/692/758 : BAL QSOs in SDSS-DR5 (Gibson+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/493/339">J/A+A/493/339 : XMM-Newton serendipitous Survey. 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