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<ri:Resource created="2012-10-16T15:43:53Z" 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>GALEX UV-bright high-redshift quasars</title><shortName>J/ApJ/728/23</shortName><identifier>ivo://CDS.VizieR/J/ApJ/728/23</identifier><altIdentifier>doi:10.26093/cds/vizier.17280023</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Worseck G.</name></creator><creator><name>Prochaska J.X.</name></creator><date role="Updated">2017-11-28T13:21:31Z</date><date role="Created">2012-10-16T15:43:53Z</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>ultraviolet-photometry</subject><subject>visible-astronomy</subject><subject>sloan-photometry</subject><subject>redshifted</subject><subject>quasars</subject><subject>surveys</subject><description>We study the small population of high-redshift (z_em_&gt;2.7) quasars detected by the Galaxy Evolution Explorer(GALEX), whose far-UV emission is not extinguished by intervening HI Lyman limit systems. We correlate almost all verified z_em_&gt;2.7 quasars to the GALEX GR4 source catalog covering ~25000deg^2^, yielding 304 sources detected at signal-to-noise ratio (S/N)&gt;3. However, ~50% of these are only detected in the GALEX NUV band, signaling the truncation of the FUV flux by low-redshift optically thick Lyman limit systems. We regard 52 quasars detected at S/N&gt;3 to be most promising for Hubble Space Telescope follow-up, with an additional 114 quasars if we consider S/N&gt;2 detections in the FUV. Combining the statistical properties of HI absorbers with the Sloan Digital Sky Survey (SDSS) quasar luminosity function, we predict a large all-sky population of ~200 quasars with z_em_&gt;2.7 and i&lt;~19 that should be detectable at the HeII edge at m_304_&lt;21. However, SDSS provides just half of the NUV-bright quasars that should have been detected by SDSS and GALEX. With mock quasar photometry we revise the SDSS quasar selection function, finding that SDSS systematically misses quasars with blue u-g&lt;~2 colors at 3&lt;~z_em_&lt;~3.5 due to overlap with the stellar locus in color space.</description><source format="bibcode">2011ApJ...728...23W</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/728/23</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/VII/260">VII/260 : The SDSS-DR7 quasar catalog (Schneider+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VII/258">VII/258 : Quasars and Active Galactic Nuclei (13th Ed.) (Veron+ 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/294">II/294 : The SDSS Photometric Catalog, Release 7 (Adelman-McCarthy+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/193/28">J/ApJS/193/28 : Galaxy survey around 20 UV-bright quasars (Prochaska+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/399/728">J/MNRAS/399/728 : UV-bright sources behind M31 halo (Fittingoff+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/137/3761">J/AJ/137/3761 : Ultraviolet quasi-stellar objects (Bianchi+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/185/20">J/ApJS/185/20 : Additional HeII quasar sightlines (Syphers+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/690/1181">J/ApJ/690/1181 : UV-bright quasars (Syphers+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/383/1513">J/MNRAS/383/1513 : 2MASS, SDSS and FIRST fluxes of QSOs (Labita+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/133/1780">J/AJ/133/1780 : GALEX/SDSS quasar catalog (Trammell+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/664/53">J/ApJ/664/53 : UV photometry of GALEX QSO candidates (Atlee+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/134/35">J/ApJS/134/35 : Large Bright Quasar Survey emission lines (Forster+, 2001)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+AS/111/169">J/A+AS/111/169 : UV-excess quasar candidates (Moreau+, 1995)</relatedResource><relatedResource>http://www.sdss.org/ : SDSS home page</relatedResource><relatedResource>http://galex.stsci.edu/GR4/ : GALEX GR4/GR5 at MAST</relatedResource></relationship></content><rights>https://cds.unistra.fr/vizier-org/licences_vizier.html</rights><capability><interface xsi:type="vr:WebBrowser"><accessURL 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