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<ri:Resource created="2006-06-04T23:10:19Z" 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>b_j_ur photometry and redshifts of QSOs</title><shortName>J/MNRAS/357/1267</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/357/1267</identifier><altIdentifier>doi:10.26093/cds/vizier.73571267</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Cirasuolo M.</name></creator><creator><name>Magliocchetti M.</name></creator><creator><name>Celotti A.</name></creator><date role="Updated">2024-06-30T20:17:06Z</date><date role="Created">2006-06-04T23:10:19Z</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>radio-sources</subject><subject>photometry</subject><subject>redshifted</subject><description>The quasar sample selected by cross-correlating the Faint Images of the Radio Sky at Twenty cm (FIRST, &lt;VIII/71&gt;) survey and the 2-degree Field Quasar Redshift Survey (2QZ, &lt;VII/223&gt;) allows us to explore, for the first time, the faint end of the radio and optical luminosity functions up to z=~2.2. We find indications (~3{sigma}) of a negative evolution for these faint sources at z&gt;~1.8, both in radio and optical bands. This corresponds to a decrement in the space density of faint quasars of approximately a factor 2 at z=2.2 and confirms the presence of a differential evolution for the population of radio-active quasars. The faint end of both luminosity functions flattens and the comparison with the (optical) number density of the whole quasar population supports a dependence of the fraction of radio-detected quasars on the optical luminosity. A progressive decrease in the fraction of quasars in the whole radio source population can be consistently accounted for within the receding torus scenario. The population of low-luminosity quasars, which the FIRST-2dF detects, appears to depart from the classical scheme for radio-loud quasars.</description><source format="bibcode">2005MNRAS.357.1267C</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/357/1267</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/J/MNRAS/341/993">J/MNRAS/341/993 : u_j_br photometry and redshifts of QSOs (Cirasuolo+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VII/223">VII/223 : The 2dF QSO Redshift Survey. V. The 10k cat. 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