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<ri:Resource created="2002-07-20T18:18:11Z" 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>Asiago-ESO/RASS QSO survey. I.</title><shortName>J/AJ/119/2540</shortName><identifier>ivo://CDS.VizieR/J/AJ/119/2540</identifier><altIdentifier>doi:10.26093/cds/vizier.51192540</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Grazian A.</name></creator><creator><name>Cristiani S.</name></creator><creator><name>D'Odorico V.</name></creator><creator><name>Omizzolo A.</name></creator><creator><name>Pizzella A.</name></creator><date role="Updated">2023-04-06T16:50:37Z</date><date role="Created">2002-07-20T18:18:11Z</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>apparent-magnitude</subject><subject>redshifted</subject><description>This paper presents the first results of a survey for bright quasars (V&lt;14.5 and R&lt;15.4) covering the northern hemisphere at Galactic latitudes |b|&gt;30{deg}. The photometric database is derived from the Guide Star and USNO catalogs. Quasars are identified on the basis of their X-ray emission measured in the ROSAT All-Sky Survey. The surface density of quasars brighter than 15.5mag turns out to be (10+/-2)x10^-3^deg^-2^, about 3 times higher than that estimated by the Palomar-Green (PG) survey. The quasar optical luminosity function (LF) at 0.04&lt;z&lt;=0.3 is computed and shown to be consistent with a luminosity-dependent luminosity evolution of the type derived by La Franca &amp; Cristiani (1997AJ....113.1517L) in the range 0.3&lt;z&lt;=2.2. The predictions of semianalytical models of hierarchical structure formation agree remarkably well with the present observations.</description><source format="bibcode">2000AJ....119.2540G</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/119/2540</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/II/207">II/207 : Palomar-Green catalog UV-excess stellar objects (Green+ 1986)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/243">I/243 : The PMM USNO-A1.0 Catalogue (Monet 1997)</relatedResource><relatedResource 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