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<ri:Resource created="2008-07-25T12:10:05Z" status="active" updated="2025-09-09T14:13:07Z" 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>Metal-strong damped Ly{alpha} systems</title><shortName>J/PASP/118/1077</shortName><identifier>ivo://CDS.VizieR/J/PASP/118/1077</identifier><altIdentifier>doi:10.26093/cds/vizier.61181077</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Herbert-Fort S.</name></creator><creator><name>Prochaska J.X.</name></creator><creator><name>Dessauges-Zavadsky M.</name></creator><creator><name>Ellison S.L.,Howk J.C.</name></creator><creator><name>Wolfe A.M.</name></creator><creator><name>Prochter G.E.</name></creator><date role="Updated">2025-09-09T14:13:07Z</date><date role="Created">2008-07-25T12:10:05Z</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>spectroscopy</subject><description>We have identified a metal-strong [logN(Zn+)&gt;=13.15 or logN(Si^+^)&gt;=15.95] damped Ly{alpha} (MSDLA) population from an automated quasar (QSO) absorber search in the Sloan Digital Sky Survey (SDSS) Data Release 3 quasar sample and find that MSDLAs comprise &gt;&gt;5% of the entire DLA population with z_abs_&gt;=2.2 found in QSO sight lines with r&lt;19.5. We have also acquired 27 Keck ESI (Echellete Spectrograph and Imager) follow-up spectra of metal strong candidates in order to evaluate our automated technique and examine the MSDLA candidates at higher resolution.</description><source format="bibcode">2006PASP..118.1077H</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/PASP/118/1077</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/243">VII/243 : SDSS quasar catalog. III. 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