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<ri:Resource created="2004-10-16T15:46:11Z" 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>Radio-loud QSOs at z~4</title><shortName>J/MNRAS/348/857</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/348/857</identifier><altIdentifier>doi:10.26093/cds/vizier.73480857</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Holt J.</name></creator><creator><name>Benn C.R.</name></creator><creator><name>Vigotti M.</name></creator><creator><name>Pedani M.</name></creator><creator><name>Carballo R.,Gonzalez-serrano J.I.</name></creator><creator><name>Mack K.-H.</name></creator><creator><name>Garcia B.</name></creator><date role="Updated">2024-06-29T20:14:45Z</date><date role="Created">2004-10-16T15:46:11Z</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>redshifted</subject><subject>photometry</subject><subject>radio-astronomy</subject><subject>spectroscopy</subject><description>We obtained spectra of 60 red, star-like objects (m_E_&lt;18.8) identified with FIRST radio sources, S_1.4GHz_&gt;1mJy. Eight are quasi-stellar objects (QSOs) with redshift z&gt;3.6. Combined with our earlier pilot search, our sample of 121 candidates yields a total of 18 z&gt;3.6 QSOs (10 of these with z&gt;4.0). 8 per cent of candidates with S_1.4GHz_&lt;10mJy and 37 per cent of candidates with S_1.4GHz_&gt;10mJy are QSOs with z&gt;3.6. The surface density of m_E_&lt;18.8, S_1.4GHz_&gt;1mJy, z&gt;4 QSOs is 0.003deg^-2^. This is currently the only well-defined sample of radio-loud QSOs at z~4 selected independently of radio spectral index. The QSOs are highly luminous in the optical (eight have M_B_&lt;28, q_0_=0.5, H_0_=50km/s/Mpc). The SEDs are as varied as those seen in optical searches for high-redshift QSOs, but the fraction of objects with weak (strongly self-absorbed) Ly emission is marginally higher (3 out of 18) than for high-redshift QSOs from SDSS (5 out of 96).</description><source format="bibcode">2004MNRAS.348..857H</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/348/857</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/71">VIII/71 : The FIRST Survey Catalog, Version 03Apr11 (Becker+ 2003)</relatedResource><relatedResource 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