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<ri:Resource created="2008-11-07T07:53:15Z" 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>u_j_br photometry and redshifts of QSOs</title><shortName>J/MNRAS/341/993</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/341/993</identifier><altIdentifier>doi:10.26093/cds/vizier.73410993</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><creator><name>Danese L.</name></creator><date role="Updated">2024-06-28T20:17:18Z</date><date role="Created">2008-11-07T07:53:15Z</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>We present a detailed analysis of a sample of radio-detected quasars, obtained by matching together objects from the FIRST (&lt;VIII/71&gt;) survey and the 2dF Quasar Redshift Survey (2dF, &lt;VII/223&gt;). The data set consists of 113 sources, spanning a redshift range 0.35&lt;~z&lt;~2.2, with optical magnitudes 18.25&lt;=bj&lt;=20.85 and radio fluxes S_1.4GHz_&gt;=1mJy. These objects exhibit properties such as redshift and colour distribution in full agreement with those derived for the whole quasar population, suggesting that the mechanism(s) controlling the birth and lifetime of quasars are independent of their level of radio emission. The long-debated question of the radio-loud/radio quiet (RL/RQ) dichotomy is then investigated for the combined FIRST-2dF and FIRST-LBQS (Large Bright Quasar Survey) samples, as they present similar selection criteria.</description><source format="bibcode">2003MNRAS.341..993C</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/341/993</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/357/1267">J/MNRAS/357/1267 : bJur photometry and redshifts of QSOs (Cirasuolo+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VII/223">VII/223 : The 2dF QSO Redshift Survey. 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