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<ri:Resource created="2006-04-05T15:17:55Z" 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>The 2dF QSO Redshift Survey. VIII</title><shortName>J/MNRAS/328/805</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/328/805</identifier><altIdentifier>doi:10.26093/cds/vizier.73280805</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Outram P.J.</name></creator><creator><name>Smith R.J.</name></creator><creator><name>Shanks T.</name></creator><creator><name>Boyle B.J.</name></creator><creator><name>Croom S.M.</name></creator><creator><name>Loaring N.S.,Miller L.</name></creator><date role="Updated">2024-06-27T20:17:52Z</date><date role="Created">2006-04-05T15:17:55Z</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>surveys</subject><subject>spectroscopy</subject><description>We examine the highest signal-to-noise ratio spectra from the 2dF QSO Redshift Survey (2QZ) 10k release (Cat. &lt;VII/223&gt;) and identify over 100 new low-ionization heavy-element absorbers: damped Lyman-{alpha} (DLA) candidates suitable for higher-resolution follow-up observations. These absorption systems map the spatial distribution of high-z metals in exactly the same volumes as the foreground 2QZ QSOs themselves sample and hence the 2QZ gives us the unique opportunity to compare directly the two tracers of large-scale structure. We examine the cross-correlation of the two populations to see how they are relatively clustered, and, by considering the colour of the QSOs, detect a small amount of dust in these metal systems.</description><source format="bibcode">2001MNRAS.328..805O</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/328/805</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/223">VII/223 : The 2dF QSO Redshift Survey. V. 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