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<ri:Resource created="2003-03-27T06:04:40Z" 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>Parkes Quarter-Jansky Flat-Spectrum Sample. II.</title><shortName>J/A+A/399/469</shortName><identifier>ivo://CDS.VizieR/J/A+A/399/469</identifier><altIdentifier>doi:10.26093/cds/vizier.33990469</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Hook I.M.</name></creator><creator><name>Shaver P.A.</name></creator><creator><name>Jackson C.A.</name></creator><creator><name>Wall J.V.</name></creator><creator><name>Kellermann K.I.</name></creator><date role="Updated">2018-01-10T11:47:47Z</date><date role="Created">2003-03-27T06:04:40Z</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><description>We present optical spectra and redshift measurements for 178 flat-spectrum objects from the Parkes quarter-Jansky flat-spectrum sample. These spectra were obtained in order to compile a complete sample of quasars for use in a study of quasar evolution. We present a composite optical spectrum made from the subset of 109 quasars that have flux densities in the range 0.25Jy&lt;S(2.7GHz)&lt;0.5Jy, and make a comparison with a composite spectrum for radio-quiet QSOs from the Large Bright Quasar Survey. Our large sample of radio-loud quasars allows us to strengthen previous reports that the Ly and CIV emission lines have larger equivalent width in radio-loud quasars than radio-quiet QSOs to greater than the 3{sigma} level. However we see no significant difference in the equivalent widths of CIII] or MgII. We also show that the flux decrements across the Lyman-{alpha} line (DA) measured from these spectra show the same trend with redshift as for optically selected QSOs.</description><source format="bibcode">2003A&amp;A...399..469H</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/399/469</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/VIII/34">VIII/34 : Parkes Half-Jansky Flat-Spectrum Sample (Drinkwater + 1997)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/386/97">J/A+A/386/97 : Parkes Quarter-Jansky Flat-Spectrum Sample. I. 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